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class="title is-5 mathjax"> Mirror Symmetry Breaking Disclosed in the Decay of Three-Proton Emitter 20Al </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Xu%2C+X+-">X. -D. Xu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mukha%2C+I">I. Mukha</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Li%2C+J+G">J. G. Li</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wang%2C+S+M">S. M. Wang</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acosta%2C+L">L. Acosta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bajzek%2C+M">M. Bajzek</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Espino%2C+J+M">J. M. Espino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fomichev%2C+A">A. Fomichev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gomez-Camacho%2C+J">J. Gomez-Camacho</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grigorenko%2C+L+V">L. V. Grigorenko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kiselev%2C+O">O. Kiselev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Korsheninnikov%2C+A+A">A. A. Korsheninnikov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kostyleva%2C+D">D. Kostyleva</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kurz%2C+N">N. Kurz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Litvinov%2C+Y+A">Yu. A. Litvinov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martel%2C+I">I. Martel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nociforo%2C+C">C. Nociforo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pfutzner%2C+M">M. Pfutzner</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rodr%C4%B1guez-Tajes%2C+C">C. Rodr谋guez-Tajes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Scheidenberger%2C+C">C. Scheidenberger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Stanoiu%2C+M">M. Stanoiu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suemmerer%2C+K">K. Suemmerer</a> , et al. (3 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2412.08245v1-abstract-short" style="display: inline;"> The previously-unknown nucleus 20Al has been observed for the first time by detecting its in-flight decays. Tracking trajectories of all decay products with silicon micro-strip detectors allowed for a conclusion that 20Al is unbound with respect to three-proton (3p) emission. The 3p-decay energy of 20Al ground state has been determined to be 1.93(+0.11,-0.09) MeV through a detailed study of angula&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.08245v1-abstract-full').style.display = 'inline'; document.getElementById('2412.08245v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2412.08245v1-abstract-full" style="display: none;"> The previously-unknown nucleus 20Al has been observed for the first time by detecting its in-flight decays. Tracking trajectories of all decay products with silicon micro-strip detectors allowed for a conclusion that 20Al is unbound with respect to three-proton (3p) emission. The 3p-decay energy of 20Al ground state has been determined to be 1.93(+0.11,-0.09) MeV through a detailed study of angular correlations of its decay products, 17Ne+p+p+p. This value is much smaller in comparison with the predictions inferred from the isospin symmetry by using the known energy of its mirror nucleus 20N, which indicates a possible mirror symmetry violation in the structure of 3p emitters. Such an isospin symmetry breaking is supported by the calculations of the continuum embedded theoretical frameworks, describing the observed 20Al ground state as an 1p s-wave state with a spin-parity of 1-, which contradicts to the spin-parity (2-) of the 20N ground state. The 20Al ground state decays by sequential 1p-2p emission via intermediate ground state of 19Mg, which is the first observed case of daughter two-proton radioactivity following 1p decay of the parent state. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2412.08245v1-abstract-full').style.display = 'none'; document.getElementById('2412.08245v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">9 pages, 6 figures, to be submitted to APS</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2406.04771">arXiv:2406.04771</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2406.04771">pdf</a>, <a href="https://arxiv.org/format/2406.04771">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.110.L031301">10.1103/PhysRevC.110.L031301 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Observation and spectroscopy of proton-unbound nucleus $^{21}$Al </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Kostyleva%2C+D">D. Kostyleva</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Xu%2C+X+-">X. -D. Xu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mukha%2C+I">I. Mukha</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acosta%2C+L">L. Acosta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bajzek%2C+M">M. Bajzek</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ciemny%2C+A+A">A. A. Ciemny</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dominik%2C+W">W. Dominik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Due%C3%B1as%2C+J+A">J. A. Due帽as</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Espino%2C+J+M">J. M. Espino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Estrad%C3%A9%2C+A">A. Estrad茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Farinon%2C+F">F. Farinon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fomichev%2C+A">A. Fomichev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=G%C3%B3mez-Camacho%2C+J">J. G贸mez-Camacho</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorshkov%2C+A">A. Gorshkov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grigorenko%2C+L+V">L. V. Grigorenko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Janas%2C+Z">Z. Janas</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kami%C5%84ski%2C+G">G. Kami艅ski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kiselev%2C+O">O. Kiselev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kn%C3%B6bel%2C+R">R. Kn枚bel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Korsheninnikov%2C+A+A">A. A. Korsheninnikov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Krupko%2C+S">S. Krupko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kuich%2C+M">M. Kuich</a> , et al. (29 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2406.04771v1-abstract-short" style="display: inline;"> We report on the observation of previously-unknown isotope $^{21}$Al, the first unbound aluminum isotope located beyond the proton dripline. The $^{21}$Al nucleus decays by one-proton (1p) emission, and its in-flight decays were detected by tracking trajectories of all decay products with micro-strip silicon detectors. The 1p-emission processes were studied by analyses of the measured angular corr&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2406.04771v1-abstract-full').style.display = 'inline'; document.getElementById('2406.04771v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2406.04771v1-abstract-full" style="display: none;"> We report on the observation of previously-unknown isotope $^{21}$Al, the first unbound aluminum isotope located beyond the proton dripline. The $^{21}$Al nucleus decays by one-proton (1p) emission, and its in-flight decays were detected by tracking trajectories of all decay products with micro-strip silicon detectors. The 1p-emission processes were studied by analyses of the measured angular correlations of decay products $^{20}$Mg+p. The 1p-decay energies of ground and low-lying excited states of $^{21}$Al, its mass excess and proton separation energy value $S_p$=$-1.1(1)$ MeV were determined. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2406.04771v1-abstract-full').style.display = 'none'; document.getElementById('2406.04771v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 June, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 7 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physical Review C 110, L031301 (2024) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2310.00409">arXiv:2310.00409</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2310.00409">pdf</a>, <a href="https://arxiv.org/ps/2310.00409">ps</a>, <a href="https://arxiv.org/format/2310.00409">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Neutrons from projectile fragmentation at 600 MeV/nucleon </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Paw%C5%82owski%2C+P">P. Paw艂owski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Buyukcizmeci%2C+N">N. Buyukcizmeci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Johansson%2C+H+T">H. T. Johansson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Trautmann%2C+W">W. Trautmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wieloch%2C+A">A. Wieloch</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">K. Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botvina%2C+A+S">A. S. Botvina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heil%2C+M">M. Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%A8vre%2C+A+L">A. Le F猫vre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Leifels%2C+Y">Y. Leifels</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=L%C3%BChning%2C+J">J. L眉hning</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%C5%81ukasik%2C+J">J. 艁ukasik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lynen%2C+U">U. Lynen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Majka%2C+Z">Z. Majka</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mishustin%2C+I+N">I. N. Mishustin</a> , et al. (11 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2310.00409v1-abstract-short" style="display: inline;"> The neutron emission in projectile fragmentation at relativistic energies was studied with the Large-Area-Neutron-Detector LAND coupled to the ALADIN forward spectrometer at the GSI Schwerionen-Synchrotron (SIS). Stable 124Sn and radioactive 107Sn and 124La beams with an incident energy of 600 MeV/nucleon were used to explore the N/Z dependence of the identified neutron source. A cluster-recogniti&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2310.00409v1-abstract-full').style.display = 'inline'; document.getElementById('2310.00409v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2310.00409v1-abstract-full" style="display: none;"> The neutron emission in projectile fragmentation at relativistic energies was studied with the Large-Area-Neutron-Detector LAND coupled to the ALADIN forward spectrometer at the GSI Schwerionen-Synchrotron (SIS). Stable 124Sn and radioactive 107Sn and 124La beams with an incident energy of 600 MeV/nucleon were used to explore the N/Z dependence of the identified neutron source. A cluster-recognition algorithm is applied for identifying individual particles within the hit distributions registered with LAND. The obtained momentum distributions are extrapolated over the full phase space occupied by the neutrons from the projectile-spectator source. The mean multiplicities of spectator neutrons reach values of up to about 11 and depend strongly on the isotopic composition of the projectile. An effective source temperature of T \approx 2-5 MeV, monotonically increasing with decreasing impact parameter, is deduced from the transverse momentum distributions. For the interpretation of the data, calculations with the statistical multifragmentation model were performed. The variety of excited projectile spectators assumed to decay statistically is represented by an ensemble of excited sources with parameters determined previously from the fragment production observed in the same experiments. The obtained agreement is very satisfactory for more peripheral collisions where, according to the model, neutrons are mainly emitted during the secondary decays of excited fragments. The neutron multiplicity in more central collisions is underestimated, indicating that other sources besides the modeled statistical breakup contribute to the observed neutron yield. The choice made for the symmetry-term coefficient of the liquid-drop description of produced fragments has a weak effect on the predicted neutron multiplicities. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2310.00409v1-abstract-full').style.display = 'none'; document.getElementById('2310.00409v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 September, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2023. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">22 pages, 24 figures, to appear in Physical Review C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 108, 044610 (2023) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2101.11474">arXiv:2101.11474</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2101.11474">pdf</a>, <a href="https://arxiv.org/format/2101.11474">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.physletb.2022.136957">10.1016/j.physletb.2022.136957 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Unveiling the Two-Proton Halo Character of 17Ne: Exclusive Measurement of Quasi-free Proton-Knockout Reactions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Lehr%2C+C">C. Lehr</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Wamers%2C+F">F. Wamers</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aksouh%2C+F">F. Aksouh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aksyutina%2C+Y">Yu. Aksyutina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez-Pol%2C+H">H. Alvarez-Pol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Atar%2C+L">L. Atar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beceiro-Novo%2C+S">S. Beceiro-Novo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bertulani%2C+C+A">C. A. Bertulani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">K. Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borge%2C+M+J+G">M. J. G. Borge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caesar%2C+C">C. Caesar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chartier%2C+M">M. Chartier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatillon%2C+A">A. Chatillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chulkov%2C+L+V">L. V. Chulkov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fernandez%2C+P+D">P. Diaz Fernandez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ershova%2C+O">O. Ershova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fraile%2C+L+M">L. M. Fraile</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fynbo%2C+H+O+U">H. O. U. Fynbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galaviz%2C+D">D. Galaviz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heil%2C+M">M. Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heine%2C+M">M. Heine</a> , et al. (40 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2101.11474v1-abstract-short" style="display: inline;"> The proton drip-line nucleus 17Ne is investigated experimentally in order to determine its two-proton halo character. A fully exclusive measurement of the 17Ne(p,2p)16F-&gt;15O+p quasi-free one-proton knockout reaction has been performed at GSI at around 500 MeV/nucleon beam energy. All particles resulting from the scattering process have been detected. The relevant reconstructed quantities are the a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.11474v1-abstract-full').style.display = 'inline'; document.getElementById('2101.11474v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2101.11474v1-abstract-full" style="display: none;"> The proton drip-line nucleus 17Ne is investigated experimentally in order to determine its two-proton halo character. A fully exclusive measurement of the 17Ne(p,2p)16F-&gt;15O+p quasi-free one-proton knockout reaction has been performed at GSI at around 500 MeV/nucleon beam energy. All particles resulting from the scattering process have been detected. The relevant reconstructed quantities are the angles of the two protons scattered in quasi-elastic kinematics, the decay of 16F into 15O (including gamma decays from excited states) and a proton, as well as the 15O+p relative-energy spectrum and the 16F momentum distributions. The latter two quantities allow an independent and consistent determination of the ratio of l=0 and l=2 motion of the valence protons in 17Ne. With a resulting relatively small l=0 component of only around 35(3)%, it is concluded that 17Ne exhibits a rather modest halo character only. The quantitative agreement of the two values deduced from the energy spectrum and the momentum distributions supports the theoretical treatment of the calculation of momentum distributions after quasi-free knockout reactions at high energies by taking into account distortions based on the Glauber theory. Moreover, the experimental data allow the separation of valence-proton knockout and knockout from the 15O core. The latter process contributes with 11.8(3.1) mb around 40% to the total proton-knockout cross section of 30.3(2.3) mb, which explains previously reported contradicting conclusions derived from inclusive cross sections. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.11474v1-abstract-full').style.display = 'none'; document.getElementById('2101.11474v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 27 January, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 5 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2101.06422">arXiv:2101.06422</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2101.06422">pdf</a>, <a href="https://arxiv.org/ps/2101.06422">ps</a>, <a href="https://arxiv.org/format/2101.06422">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epja/s10050-020-00341-3">10.1140/epja/s10050-020-00341-3 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Detailed study of the decay of 32Ar </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Blank%2C+B">B. Blank</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adimi%2C+N">N. Adimi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alcorta%2C+M">M. Alcorta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bey%2C+A">A. Bey</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borge%2C+M+J+G">M. J. G Borge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brown%2C+B+A">B. A. Brown</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Santos%2C+F+d+O">F. de Oliveira Santos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dossat%2C+C">C. Dossat</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fynbo%2C+H+O+U">H. O. U. Fynbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giovinazzo%2C+J">J. Giovinazzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Knudsen%2C+H+H">H. H. Knudsen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Madurga%2C+M">M. Madurga</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Magilligan%2C+A">A. Magilligan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Matea%2C+I">I. Matea</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Perea%2C+A">A. Perea</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suemmerer%2C+K">K. Suemmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tengblad%2C+O">O. Tengblad</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Thomas%2C+J+C">J. C. Thomas</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2101.06422v1-abstract-short" style="display: inline;"> In an experiment performed at the SPIRAL1 facility of GANIL, the beta decay of 32Ar has been studied by means of the &#34;Silicon Cube&#34; device associated with germanium clover detectors from the EXOGAM array. Beta-delayed protons and gamma rays have been observed and allowed the determination of all relevant decay branches. The Gamow-Teller strength distribution is compared to shell-model calculations&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.06422v1-abstract-full').style.display = 'inline'; document.getElementById('2101.06422v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2101.06422v1-abstract-full" style="display: none;"> In an experiment performed at the SPIRAL1 facility of GANIL, the beta decay of 32Ar has been studied by means of the &#34;Silicon Cube&#34; device associated with germanium clover detectors from the EXOGAM array. Beta-delayed protons and gamma rays have been observed and allowed the determination of all relevant decay branches. The Gamow-Teller strength distribution is compared to shell-model calculations and excellent agreement is found. The Fermi strength is inline with expectations. A quasi-complete decay scheme of 32Ar is established. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.06422v1-abstract-full').style.display = 'none'; document.getElementById('2101.06422v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 January, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">accepted for publication in EPJA</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2006.05774">arXiv:2006.05774</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2006.05774">pdf</a>, <a href="https://arxiv.org/ps/2006.05774">ps</a>, <a href="https://arxiv.org/format/2006.05774">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.physletb.2020.135962">10.1016/j.physletb.2020.135962 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Systematic reduction of the proton-removal cross section in neutron-rich medium-mass nuclei </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=D%C3%ADaz-Cort%C3%A9s%2C+J">J. D铆az-Cort茅s</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rodr%C3%ADguez-S%C3%A1nchez%2C+J+L">J. L. Rodr铆guez-S谩nchez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%C3%81lvarez-Pol%2C+H">H. 脕lvarez-Pol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bertulani%2C+C+A">C. A. Bertulani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Blank%2C+B">B. Blank</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dragosavac%2C+D">D. Dragosavac</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%B6hr%2C+V">V. F枚hr</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gargano%2C+A">A. Gargano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gasc%C3%B3n%2C+M">M. Gasc贸n</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gawlikowicz%2C+W">W. Gawlikowicz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heinz%2C+A">A. Heinz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Helariutta%2C+K">K. Helariutta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keli%C4%87-Heil%2C+A">A. Keli膰-Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Luki%C4%87%2C+S">S. Luki膰</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Montes%2C+F">F. Montes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=P%C3%A9rez-Loureiro%2C+D">D. P茅rez-Loureiro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pie%C5%84kowski%2C+L">L. Pie艅kowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schmidt%2C+K">K-H. Schmidt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Staniou%2C+M">M. Staniou</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suboti%C4%87%2C+K">K. Suboti膰</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=S%C3%BCmmerer%2C+K">K. S眉mmerer</a> , et al. (2 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2006.05774v1-abstract-short" style="display: inline;"> Single neutron- and proton-removal cross sections have been systematically measured for 72 medium-mass neutron-rich nuclei around Z=50 and energies around 900A MeV using the FRagment Separator (FRS) at GSI. Neutron-removal cross sections are described by considering the knock-out process together with initial- and final-state interactions. Proton-removal cross sections are, however, significantly&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.05774v1-abstract-full').style.display = 'inline'; document.getElementById('2006.05774v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2006.05774v1-abstract-full" style="display: none;"> Single neutron- and proton-removal cross sections have been systematically measured for 72 medium-mass neutron-rich nuclei around Z=50 and energies around 900A MeV using the FRagment Separator (FRS) at GSI. Neutron-removal cross sections are described by considering the knock-out process together with initial- and final-state interactions. Proton-removal cross sections are, however, significantly smaller than predicted by the same calculations. The observed difference can be explained as due to the knockout of short-correlated protons in neutron-proton dominating pairs. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2006.05774v1-abstract-full').style.display = 'none'; document.getElementById('2006.05774v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 June, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2020. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1507.04916">arXiv:1507.04916</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1507.04916">pdf</a>, <a href="https://arxiv.org/ps/1507.04916">ps</a>, <a href="https://arxiv.org/format/1507.04916">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.92.035803">10.1103/PhysRevC.92.035803 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First Measurement of the $^{96}$Ru(p,$纬$)$^{97}$Rh Cross Section for the p-Process with a Storage Ring </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Mei%2C+B">Bo Mei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">Thomas Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bishop%2C+S">Shawn Bishop</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Blaum%2C+K">Klaus Blaum</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">Konstanze Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bosch%2C+F">Fritz Bosch</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brandau%2C+C">Carsten Brandau</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Br%C3%A4uning%2C+H">Harald Br盲uning</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Davinson%2C+T">Thomas Davinson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dillmann%2C+I">Iris Dillmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dimopoulou%2C+C">Christina Dimopoulou</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ershova%2C+O">Olga Ershova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%BCl%C3%B6p%2C+Z">Zsolt F眉l枚p</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">Hans Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Glorius%2C+J">Jan Glorius</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gy%C3%BCrky%2C+G">Gy枚rgy Gy眉rky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heil%2C+M">Michael Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=K%C3%A4ppeler%2C+F">Franz K盲ppeler</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kelic-Heil%2C+A">Aleksandra Kelic-Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kozhuharov%2C+C">Christophor Kozhuharov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Langer%2C+C">Christoph Langer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bleis%2C+T+L">Tudi Le Bleis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Litvinov%2C+Y">Yuri Litvinov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lotay%2C+G">Gavin Lotay</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marganiec%2C+J">Justyna Marganiec</a> , et al. (22 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1507.04916v1-abstract-short" style="display: inline;"> This work presents a direct measurement of the $^{96}$Ru($p, 纬$)$^{97}$Rh cross section via a novel technique using a storage ring, which opens opportunities for reaction measurements on unstable nuclei. A proof-of-principle experiment was performed at the storage ring ESR at GSI in Darmstadt, where circulating $^{96}$Ru ions interacted repeatedly with a hydrogen target. The $^{96}$Ru($p, 纬$)&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1507.04916v1-abstract-full').style.display = 'inline'; document.getElementById('1507.04916v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1507.04916v1-abstract-full" style="display: none;"> This work presents a direct measurement of the $^{96}$Ru($p, 纬$)$^{97}$Rh cross section via a novel technique using a storage ring, which opens opportunities for reaction measurements on unstable nuclei. A proof-of-principle experiment was performed at the storage ring ESR at GSI in Darmstadt, where circulating $^{96}$Ru ions interacted repeatedly with a hydrogen target. The $^{96}$Ru($p, 纬$)$^{97}$Rh cross section between 9 and 11 MeV has been determined using two independent normalization methods. As key ingredients in Hauser-Feshbach calculations, the $纬$-ray strength function as well as the level density model can be pinned down with the measured ($p, 纬$) cross section. Furthermore, the proton optical potential can be optimized after the uncertainties from the $纬$-ray strength function and the level density have been removed. As a result, a constrained $^{96}$Ru($p, 纬$)$^{97}$Rh reaction rate over a wide temperature range is recommended for $p$-process network calculations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1507.04916v1-abstract-full').style.display = 'none'; document.getElementById('1507.04916v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 July, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">10 pages, 7 figs, Accepted for publication at PRC</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 92, 035803 (2015) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1310.2165">arXiv:1310.2165</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1310.2165">pdf</a>, <a href="https://arxiv.org/format/1310.2165">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> </div> <p class="title is-5 mathjax"> Measurement of the 92,93,94,100Mo(g,n) reactions by Coulomb Dissociation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=G%C3%B6bel%2C+K">K. G枚bel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Altstadt%2C+S">S. Altstadt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez-Pol%2C+H">H. Alvarez-Pol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aksouh%2C+F">F. Aksouh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Babilon%2C+M">M. Babilon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Behr%2C+K">K-H. Behr</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%2C+T">T. Berg</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=B%C3%B6hmer%2C+M">M. B枚hmer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">K. Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Br%C3%BCnle%2C+A">A. Br眉nle</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beyer%2C+R">R. Beyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chartier%2C+M">M. Chartier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatillon%2C+A">A. Chatillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pramanik%2C+U+D">U. Datta. Pramanik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Deveaux%2C+L">L. Deveaux</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Elvers%2C+M">M. Elvers</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Elze%2C+T+W">T. W. Elze</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Erhard%2C+M">M. Erhard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ershova%2C+O">O. Ershova</a> , et al. (48 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1310.2165v1-abstract-short" style="display: inline;"> The Coulomb Dissociation (CD) cross sections of the stable isotopes 92,94,100Mo and of the unstable isotope 93Mo were measured at the LAND/R3B setup at GSI Helmholtzzentrum f眉r Schwerionenforschung in Darmstadt, Germany. Experimental data on these isotopes may help to explain the problem of the underproduction of 92,94Mo and 96,98Ru in the models of p-process nucleosynthesis. The CD cross sections&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.2165v1-abstract-full').style.display = 'inline'; document.getElementById('1310.2165v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1310.2165v1-abstract-full" style="display: none;"> The Coulomb Dissociation (CD) cross sections of the stable isotopes 92,94,100Mo and of the unstable isotope 93Mo were measured at the LAND/R3B setup at GSI Helmholtzzentrum f眉r Schwerionenforschung in Darmstadt, Germany. Experimental data on these isotopes may help to explain the problem of the underproduction of 92,94Mo and 96,98Ru in the models of p-process nucleosynthesis. The CD cross sections obtained for the stable Mo isotopes are in good agreement with experiments performed with real photons, thus validating the method of Coulomb Dissociation. The result for the reaction 93Mo(g,n) is especially important since the corresponding cross section has not been measured before. A preliminary integral Coulomb Dissociation cross section of the 94Mo(g,n) reaction is presented. Further analysis will complete the experimental database for the (g,n) production chain of the p-isotopes of molybdenum. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.2165v1-abstract-full').style.display = 'none'; document.getElementById('1310.2165v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 8 October, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Talk given at the Conference Nuclear Physice in Astrophysics VI (NPA6), Lisbon, Portugal, May 19-24 2013. To appear in the NPA6 Proceedings in Journal of Physics: Conference Series (JPCS). 6 pages, 6 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1310.1632">arXiv:1310.1632</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1310.1632">pdf</a>, <a href="https://arxiv.org/format/1310.1632">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1742-6596/665/1/012044">10.1088/1742-6596/665/1/012044 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Nuclear astrophysics with radioactive ions at FAIR </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Reifarth%2C+R">R. Reifarth</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Altstadt%2C+S">S. Altstadt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=G%C3%B6bel%2C+K">K. G枚bel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heftrich%2C+T">T. Heftrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heil%2C+M">M. Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Koloczek%2C+A">A. Koloczek</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Langer%2C+C">C. Langer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Plag%2C+R">R. Plag</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pohl%2C+M">M. Pohl</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Sonnabend%2C+K">K. Sonnabend</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Weigand%2C+M">M. Weigand</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adachi%2C+T">T. Adachi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aksouh%2C+F">F. Aksouh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Khalili%2C+J">J. Al-Khalili</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=AlGarawi%2C+M">M. AlGarawi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=AlGhamdi%2C+S">S. AlGhamdi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alkhazov%2C+G">G. Alkhazov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alkhomashi%2C+N">N. Alkhomashi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez-Pol%2C+H">H. Alvarez-Pol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez-Rodriguez%2C+R">R. Alvarez-Rodriguez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andreev%2C+V">V. Andreev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andrei%2C+B">B. Andrei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Atar%2C+L">L. Atar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avdeichikov%2C+V">V. Avdeichikov</a> , et al. (295 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1310.1632v1-abstract-short" style="display: inline;"> The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those processes, because they are shielded from the s-process flow and r-process beta-decay chains. These nuclei are attributed to the p and rp process. For all those processes, current research in nuclear astrophysics addresses t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.1632v1-abstract-full').style.display = 'inline'; document.getElementById('1310.1632v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1310.1632v1-abstract-full" style="display: none;"> The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those processes, because they are shielded from the s-process flow and r-process beta-decay chains. These nuclei are attributed to the p and rp process. For all those processes, current research in nuclear astrophysics addresses the need for more precise reaction data involving radioactive isotopes. Depending on the particular reaction, direct or inverse kinematics, forward or time-reversed direction are investigated to determine or at least to constrain the desired reaction cross sections. The Facility for Antiproton and Ion Research (FAIR) will offer unique, unprecedented opportunities to investigate many of the important reactions. The high yield of radioactive isotopes, even far away from the valley of stability, allows the investigation of isotopes involved in processes as exotic as the r or rp processes. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.1632v1-abstract-full').style.display = 'none'; document.getElementById('1310.1632v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 October, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Invited Talk given at the Conference Nuclear Physice in Astrophysics VI (NPA6), Lisbon, Portugal, May 19-24 2013. To appear in the NPA6 Proceedings in Journal of Physics: Conference Series (JPCS)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Journal of Physics: Conference Series 665 (2016) 012044 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1209.1024">arXiv:1209.1024</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1209.1024">pdf</a>, <a href="https://arxiv.org/ps/1209.1024">ps</a>, <a href="https://arxiv.org/format/1209.1024">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1742-6596/420/1/012072">10.1088/1742-6596/420/1/012072 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Coulomb excitation of exotic nuclei at the R3B-LAND setup </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Rossi%2C+D+M">D. M. Rossi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aksouh%2C+F">F. Aksouh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez-Pol%2C+H">H. Alvarez-Pol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=B%C3%B6hmer%2C+M">M. B枚hmer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">K. Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chartier%2C+M">M. Chartier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatillon%2C+A">A. Chatillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pramanik%2C+U+D">U. Datta Pramanik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ershova%2C+O">O. Ershova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fernandez-Dominguez%2C+B">B. Fernandez-Dominguez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorska%2C+M">M. Gorska</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heil%2C+M">M. Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Johansson%2C+H">H. Johansson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Junghans%2C+A">A. Junghans</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kiselev%2C+O">O. Kiselev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Klimkiewicz%2C+A">A. Klimkiewicz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kratz%2C+J+V">J. V. Kratz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kurz%2C+N">N. Kurz</a> , et al. (19 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1209.1024v1-abstract-short" style="display: inline;"> Exotic Ni isotopes have been measured at the R3B-LAND setup at GSI in Darmstadt, using Coulomb excitation in inverse kinematics at beam energies around 500 MeV/u. As the experimental setup allows kinematically complete measurements, the excitation energy was reconstructed using the invariant mass method. The GDR and additional low-lying strength have been observed in 68Ni, the latter exhausting 4.&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.1024v1-abstract-full').style.display = 'inline'; document.getElementById('1209.1024v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1209.1024v1-abstract-full" style="display: none;"> Exotic Ni isotopes have been measured at the R3B-LAND setup at GSI in Darmstadt, using Coulomb excitation in inverse kinematics at beam energies around 500 MeV/u. As the experimental setup allows kinematically complete measurements, the excitation energy was reconstructed using the invariant mass method. The GDR and additional low-lying strength have been observed in 68Ni, the latter exhausting 4.1(1.9)% of the E1 energy-weighted sum rule. Also, the branching ratio for the non-statistical decay of the excited 68Ni nuclei was measured and amounts to 24(4)%. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.1024v1-abstract-full').style.display = 'none'; document.getElementById('1209.1024v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 September, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">11 pages, 7 figures. Invited Talk given at the 11th International Conference on Nucleus-Nucleus Collisions (NN2012), San Antonio, Texas, USA, May 27-June 1, 2012. To appear in the NN2012 Proceedings in Journal of Physics: Conference Series (JPCS)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1205.5436">arXiv:1205.5436</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1205.5436">pdf</a>, <a href="https://arxiv.org/ps/1205.5436">ps</a>, <a href="https://arxiv.org/format/1205.5436">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.86.014601">10.1103/PhysRevC.86.014601 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Improved Empirical Parametrization of Fragmentation Cross Sections </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=S%C3%BCmmerer%2C+K">Klaus S眉mmerer</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1205.5436v2-abstract-short" style="display: inline;"> A new version is proposed for the universal empirical formula, EPAX, which describes fragmentation cross sections in high-energy heavy-ion reactions. The new version, EPAX 3, can be shown to yield cross sections that are in better agreement with experimental data for the most neutron-rich fragments than the previous version. At the same time, the very good agreement of EPAX 2 with data on the neut&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1205.5436v2-abstract-full').style.display = 'inline'; document.getElementById('1205.5436v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1205.5436v2-abstract-full" style="display: none;"> A new version is proposed for the universal empirical formula, EPAX, which describes fragmentation cross sections in high-energy heavy-ion reactions. The new version, EPAX 3, can be shown to yield cross sections that are in better agreement with experimental data for the most neutron-rich fragments than the previous version. At the same time, the very good agreement of EPAX 2 with data on the neutron-deficient side has been largely maintained. Comparison with measured cross sections show that the bulk of the data is reproduced within a factor of about 2, for cross sections down to the pico-barn range. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1205.5436v2-abstract-full').style.display = 'none'; document.getElementById('1205.5436v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 June, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 May, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">9 pages, 9 figures, accepted for publication in Phys. Rev. C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 86, 014601 (2012) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1203.5608">arXiv:1203.5608</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1203.5608">pdf</a>, <a href="https://arxiv.org/ps/1203.5608">ps</a>, <a href="https://arxiv.org/format/1203.5608">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2012.07.019">10.1016/j.nima.2012.07.019 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Neutron recognition in the LAND detector for large neutron multiplicity </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Paw%C5%82owski%2C+P">P. Paw艂owski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Leifels%2C+Y">Y. Leifels</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Trautmann%2C+W">W. Trautmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+O">C. O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bassini%2C+R">R. Bassini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boiano%2C+C">C. Boiano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">K. Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Napoli%2C+M">M. De Napoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorbinet%2C+T">T. Gorbinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstr%C3%B6m%2C+M">M. Hellstr枚m</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henzlova%2C+D">D. Henzlova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hlavac%2C+S">S. Hlavac</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imm%C3%A8%2C+J">J. Imm猫</a> , et al. (39 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1203.5608v3-abstract-short" style="display: inline;"> The performance of the LAND neutron detector is studied. Using an event-mixing technique based on one-neutron data obtained in the S107 experiment at the GSI laboratory, we test the efficiency of various analytic tools used to determine the multiplicity and kinematic properties of detected neutrons. A new algorithm developed recently for recognizing neutron showers from spectator decays in the ALA&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.5608v3-abstract-full').style.display = 'inline'; document.getElementById('1203.5608v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1203.5608v3-abstract-full" style="display: none;"> The performance of the LAND neutron detector is studied. Using an event-mixing technique based on one-neutron data obtained in the S107 experiment at the GSI laboratory, we test the efficiency of various analytic tools used to determine the multiplicity and kinematic properties of detected neutrons. A new algorithm developed recently for recognizing neutron showers from spectator decays in the ALADIN experiment S254 is described in detail. Its performance is assessed in comparison with other methods. The properties of the observed neutron events are used to estimate the detection efficiency of LAND in this experiment. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.5608v3-abstract-full').style.display = 'none'; document.getElementById('1203.5608v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 July, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 26 March, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">16 pages, 8 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nuclear Inst. and Methods in Physics Research, A 694, 47-54(2012) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1105.0487">arXiv:1105.0487</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1105.0487">pdf</a>, <a href="https://arxiv.org/ps/1105.0487">ps</a>, <a href="https://arxiv.org/format/1105.0487">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.physletb.2011.08.037">10.1016/j.physletb.2011.08.037 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Production of neutron-rich nuclei in fragmentation reactions of 132Sn projectiles at relativistic energies </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=P%C3%A9rez-Loureiro%2C+D">D. P茅rez-Loureiro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%C3%81lvarez-Pol%2C+H">H. 脕lvarez-Pol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Blank%2C+B">B. Blank</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dragosavac%2C+D">D. Dragosavac</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%B6hr%2C+V">V. F枚hr</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gasc%C3%B3n%2C+M">M. Gasc贸n</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gawlikowicz%2C+W">W. Gawlikowicz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heinz%2C+A">A. Heinz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Helariutta%2C+K">K. Helariutta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keli%C4%87%2C+A">A. Keli膰</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Luki%C4%87%2C+S">S. Luki膰</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Montes%2C+F">F. Montes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pie%C5%84kowski%2C+L">L. Pie艅kowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schmidt%2C+K">K-H. Schmidt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Staniou%2C+M">M. Staniou</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suboti%C4%87%2C+K">K. Suboti膰</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=S%C3%BCmmerer%2C+K">K. S眉mmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Taieb%2C+J">J. Taieb</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Trzci%C5%84ska%2C+A">A. Trzci艅ska</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1105.0487v1-abstract-short" style="display: inline;"> The fragmentation of neutron-rich 132Sn nuclei produced in the fission of 238U projectiles at 950 MeV/u has been investigated at the FRagment Separator (FRS) at GSI. This work represents the first investigation of fragmentation of medium-mass radioactive projectiles with a large neutron excess. The measured production cross sections of the residual nuclei are relevant for the possible use of a two&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1105.0487v1-abstract-full').style.display = 'inline'; document.getElementById('1105.0487v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1105.0487v1-abstract-full" style="display: none;"> The fragmentation of neutron-rich 132Sn nuclei produced in the fission of 238U projectiles at 950 MeV/u has been investigated at the FRagment Separator (FRS) at GSI. This work represents the first investigation of fragmentation of medium-mass radioactive projectiles with a large neutron excess. The measured production cross sections of the residual nuclei are relevant for the possible use of a two-stage reaction scheme (fission+fragmentation) for the production of extremely neutron-rich medium-mass nuclei in future rare-ion-beam facilities. Moreover, the new data will provide a better understanding of the &#34;memory&#34; effect in fragmentation reactions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1105.0487v1-abstract-full').style.display = 'none'; document.getElementById('1105.0487v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 May, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2011. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">5 pages, 3 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Physics Letters B, 703, 552 (2001) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1011.6179">arXiv:1011.6179</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1011.6179">pdf</a>, <a href="https://arxiv.org/ps/1011.6179">ps</a>, <a href="https://arxiv.org/format/1011.6179">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.82.065803">10.1103/PhysRevC.82.065803 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> High-energy break-up of 6Li as a tool to study the Big-Bang nucleosynthesis reaction 2H(alpha,gamma)6Li </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Hammache%2C+F">F. Hammache</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heil%2C+M">M. Heil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Typel%2C+S">S. Typel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galaviz%2C+D">D. Galaviz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=S%C3%BCmmerer%2C+K">K. S眉mmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Coc%2C+A">A. Coc</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Uhlig%2C+F">F. Uhlig</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Attallah%2C+F">F. Attallah</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caamano%2C+M">M. Caamano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina%2C+D">D. Cortina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstr%C3%B6m%2C+M">M. Hellstr枚m</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iwasa%2C+N">N. Iwasa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kiener%2C+J">J. Kiener</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Koczon%2C+P">P. Koczon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohlmeyer%2C+B">B. Kohlmeyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mohr%2C+P">P. Mohr</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schwab%2C+E">E. Schwab</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schwarz%2C+K">K. Schwarz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Sch%C3%BCmann%2C+F">F. Sch眉mann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Senger%2C+P">P. Senger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Sorlin%2C+O">O. Sorlin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tatischeff%2C+V">V. Tatischeff</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Thibaud%2C+J+P">J. P. Thibaud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vangioni%2C+E">E. Vangioni</a> , et al. (2 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1011.6179v1-abstract-short" style="display: inline;"> The recently claimed observations of non-negligible amounts of 6Li in old halo stars have renewed interest in the Big-Bang Nucleosynthesis (BBN) of 6Li. One important ingredient in the predicted BBN abundance of 6Li is the low-energy 2H(alpha,gamma)6Li cross section. Up to now, the only available experimental result for this cross section showed an almost constant astrophysical S-factor below 400&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1011.6179v1-abstract-full').style.display = 'inline'; document.getElementById('1011.6179v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1011.6179v1-abstract-full" style="display: none;"> The recently claimed observations of non-negligible amounts of 6Li in old halo stars have renewed interest in the Big-Bang Nucleosynthesis (BBN) of 6Li. One important ingredient in the predicted BBN abundance of 6Li is the low-energy 2H(alpha,gamma)6Li cross section. Up to now, the only available experimental result for this cross section showed an almost constant astrophysical S-factor below 400 keV, contrary to theoretical expectations. We report on a new measurement of the 2H(alpha,gamma)6Li reaction using the break-up of 6Li at 150 A MeV. Even though we cannot separate experimentally the Coulomb contribution from the nuclear one, we find clear evidence for Coulomb-nuclear interference by analyzing the scattering-angular distributions. This is in-line with our theoretical description which indicates a drop of the S_24-factor at low energies as predicted also by most other models. Consequently, we find even lower upper limits for the calculated primordial 6Li abundance than before. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1011.6179v1-abstract-full').style.display = 'none'; document.getElementById('1011.6179v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 November, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">12 pages, 11 figures, LaTeX, submitted to Phy. Rev. C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C82:065803,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1006.3723">arXiv:1006.3723</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1006.3723">pdf</a>, <a href="https://arxiv.org/ps/1006.3723">ps</a>, <a href="https://arxiv.org/format/1006.3723">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.83.024608">10.1103/PhysRevC.83.024608 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isospin dependent multifragmentation of relativistic projectiles </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Ogul%2C+R">R. Ogul</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botvina%2C+A+S">A. S. Botvina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Atav%2C+U">U. Atav</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Buyukcizmeci%2C+N">N. Buyukcizmeci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mishustin%2C+I+N">I. N. Mishustin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+O">C. O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bassini%2C+R">R. Bassini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boiano%2C+C">C. Boiano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Napoli%2C+M">M. De Napoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstrom%2C+M">M. Hellstrom</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henzlova%2C+D">D. Henzlova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imme%2C+G">G. Imme</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iori%2C+I">I. Iori</a> , et al. (35 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1006.3723v2-abstract-short" style="display: inline;"> The N/Z dependence of projectile fragmentation at relativistic energies has been studied with the ALADIN forward spectrometer at the GSI Schwerionen Synchrotron (SIS). Stable and radioactive Sn and La beams with an incident energy of 600 MeV per nucleon have been used in order to explore a wide range of isotopic compositions. For the interpretation of the data, calculations with the statistical mu&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1006.3723v2-abstract-full').style.display = 'inline'; document.getElementById('1006.3723v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1006.3723v2-abstract-full" style="display: none;"> The N/Z dependence of projectile fragmentation at relativistic energies has been studied with the ALADIN forward spectrometer at the GSI Schwerionen Synchrotron (SIS). Stable and radioactive Sn and La beams with an incident energy of 600 MeV per nucleon have been used in order to explore a wide range of isotopic compositions. For the interpretation of the data, calculations with the statistical multifragmentation model for a properly chosen ensemble of excited sources were performed. The parameters of the ensemble, representing the variety of excited spectator nuclei expected in a participant-spectator scenario, are determined empirically by searching for an optimum reproduction of the measured fragment-charge distributions and correlations. An overall very good agreement is obtained. The possible modification of the liquid-drop parameters of the fragment description in the hot freeze-out environment is studied, and a significant reduction of the symmetry-term coefficient is found necessary to reproduce the mean neutron-to-proton ratios &lt;N&gt;/Z and the isoscaling parameters of Z&lt;=10 fragments. The calculations are, furthermore, used to address open questions regarding the modification of the surface-term coefficient at freeze-out, the N/Z dependence of the nuclear caloric curve, and the isotopic evolution of the spectator system between its formation during the initial cascade stage of the reaction and its subsequent breakup. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1006.3723v2-abstract-full').style.display = 'none'; document.getElementById('1006.3723v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 25 February, 2011; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 18 June, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">23 pages, 29 figures, published in Physical Review C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C83:024608,2011 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1004.2318">arXiv:1004.2318</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1004.2318">pdf</a>, <a href="https://arxiv.org/format/1004.2318">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Solar and Stellar Astrophysics">astro-ph.SR</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/RevModPhys.83.195">10.1103/RevModPhys.83.195 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Solar fusion cross sections II: the pp chain and CNO cycles </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Adelberger%2C+E+G">E. G. Adelberger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Balantekin%2C+A+B">A. B. Balantekin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bemmerer%2C+D">D. Bemmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bertulani%2C+C+A">C. A. Bertulani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chen%2C+J+-">J. -W. Chen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Costantini%2C+H">H. Costantini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Couder%2C+M">M. Couder</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cyburt%2C+R">R. Cyburt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Davids%2C+B">B. Davids</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Freedman%2C+S+J">S. J. Freedman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gai%2C+M">M. Gai</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Garcia%2C+A">A. Garcia</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gazit%2C+D">D. Gazit</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gialanella%2C+L">L. Gialanella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Greife%2C+U">U. Greife</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hass%2C+M">M. Hass</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Heeger%2C+K">K. Heeger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Haxton%2C+W+C">W. C. Haxton</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imbriani%2C+G">G. Imbriani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Itahashi%2C+T">T. Itahashi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Junghans%2C+A">A. Junghans</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kubodera%2C+K">K. Kubodera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Langanke%2C+K">K. Langanke</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Leitner%2C+D">D. Leitner</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Leitner%2C+M">M. Leitner</a> , et al. (23 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1004.2318v3-abstract-short" style="display: inline;"> We summarize and critically evaluate the available data on nuclear fusion cross sections important to energy generation in the Sun and other hydrogen-burning stars and to solar neutrino production. Recommended values and uncertainties are provided for key cross sections, and a recommended spectrum is given for 8B solar neutrinos. We also discuss opportunities for further increasing the precision o&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.2318v3-abstract-full').style.display = 'inline'; document.getElementById('1004.2318v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1004.2318v3-abstract-full" style="display: none;"> We summarize and critically evaluate the available data on nuclear fusion cross sections important to energy generation in the Sun and other hydrogen-burning stars and to solar neutrino production. Recommended values and uncertainties are provided for key cross sections, and a recommended spectrum is given for 8B solar neutrinos. We also discuss opportunities for further increasing the precision of key rates, including new facilities, new experimental techniques, and improvements in theory. This review, which summarizes the conclusions of a workshop held at the Institute for Nuclear Theory, Seattle, in January 2009, is intended as a 10-year update and supplement to Reviews of Modern Physics 70 (1998) 1265. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.2318v3-abstract-full').style.display = 'none'; document.getElementById('1004.2318v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 October, 2010; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 14 April, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">54 pages, 20 figures, version to be published in Reviews of Modern Physics; various typos corrected and several updates made</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> INT-PUB-10-016,UCB-NPAT-10-001 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1003.2800">arXiv:1003.2800</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1003.2800">pdf</a>, <a href="https://arxiv.org/ps/1003.2800">ps</a>, <a href="https://arxiv.org/format/1003.2800">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> </div> <p class="title is-5 mathjax"> Tracing a phase transition with fluctuations of the largest fragment size: Statistical multifragmentation models and the ALADIN S254 data </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Pietrzak%2C+T">T. Pietrzak</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+O">C. O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bassini%2C+R">R. Bassini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boiano%2C+C">C. Boiano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botvina%2C+A+S">A. S. Botvina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Napoli%2C+M">M. De Napoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstrom%2C+M">M. Hellstrom</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henzlova%2C+D">D. Henzlova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imme%2C+G">G. Imme</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iori%2C+I">I. Iori</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Johansson%2C+H">H. Johansson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kezzar%2C+K">K. Kezzar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lafriakh%2C+A">A. Lafriakh</a> , et al. (32 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1003.2800v1-abstract-short" style="display: inline;"> A phase transition signature associated with cumulants of the largest fragment size distribution has been identified in statistical multifragmentation models and examined in analysis of the ALADIN S254 data on fragmentation of neutron-poor and neutron-rich projectiles. Characteristics of the transition point indicated by this signature are weakly dependent on the A/Z ratio of the fragmenting spect&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1003.2800v1-abstract-full').style.display = 'inline'; document.getElementById('1003.2800v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1003.2800v1-abstract-full" style="display: none;"> A phase transition signature associated with cumulants of the largest fragment size distribution has been identified in statistical multifragmentation models and examined in analysis of the ALADIN S254 data on fragmentation of neutron-poor and neutron-rich projectiles. Characteristics of the transition point indicated by this signature are weakly dependent on the A/Z ratio of the fragmenting spectator source. In particular, chemical freeze-out temperatures are estimated within the range 5.9 to 6.5 MeV. The experimental results are well reproduced by the SMM model. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1003.2800v1-abstract-full').style.display = 'none'; document.getElementById('1003.2800v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 March, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 3 figures, Proceedings of the International Workshop on Multifragmentation and Related Topics (IWM2009), Catania, Italy, November 2009.</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1001.2641">arXiv:1001.2641</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1001.2641">pdf</a>, <a href="https://arxiv.org/ps/1001.2641">ps</a>, <a href="https://arxiv.org/format/1001.2641">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.81.024311">10.1103/PhysRevC.81.024311 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Detailed beta-decay study of 33Ar </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Adimi%2C+N">N. Adimi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dominguez-Reyes%2C+R">R. Dominguez-Reyes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alcorta%2C+M">M. Alcorta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bey%2C+A">A. Bey</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Blank%2C+B">B. Blank</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borge%2C+M+J+G">M. J. G. Borge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Santos%2C+F+d+O">F. de Oliveira Santos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dossat%2C+C">C. Dossat</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fynbo%2C+H+O+U">H. O. U. Fynbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giovinazzo%2C+J">J. Giovinazzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Knudsen%2C+H+H">H. H. Knudsen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Madurga%2C+M">M. Madurga</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Matea%2C+I">I. Matea</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Perea%2C+A">A. Perea</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Summerer%2C+K">K. Summerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tengblad%2C+O">O. Tengblad</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Thomas%2C+J+C">J. C. Thomas</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1001.2641v1-abstract-short" style="display: inline;"> The proton-rich nucleus 33Ar has been studied by detailed proton and gamma-ray spectroscopy at the low-energy facility of SPIRAL at GANIL. Proton and gamma-ray singles and coincidence measurements allowed to establish a quasi complete decay scheme of this nucleus. By comparing the proton intensity to different daughter states, tentative spin assignments have been made for some of the states of 3&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1001.2641v1-abstract-full').style.display = 'inline'; document.getElementById('1001.2641v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1001.2641v1-abstract-full" style="display: none;"> The proton-rich nucleus 33Ar has been studied by detailed proton and gamma-ray spectroscopy at the low-energy facility of SPIRAL at GANIL. Proton and gamma-ray singles and coincidence measurements allowed to establish a quasi complete decay scheme of this nucleus. By comparing the proton intensity to different daughter states, tentative spin assignments have been made for some of the states of 33Cl. The Gamow-Teller strength distribution is deduced and compared to shell-model calculations and a quenching factor is determined. States close to the isobaric analogue state are searched for with respect to isospin mixing. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1001.2641v1-abstract-full').style.display = 'none'; document.getElementById('1001.2641v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 January, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">14 pages, 9 figures, accepted for publication in PRC</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0907.1196">arXiv:0907.1196</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0907.1196">pdf</a>, <a href="https://arxiv.org/ps/0907.1196">ps</a>, <a href="https://arxiv.org/format/0907.1196">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.ppnp.2008.12.006">10.1016/j.ppnp.2008.12.006 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isotopic Dependence of the Caloric Curve </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=The+ALADIN2000+Collaboration"> The ALADIN2000 Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Trautmann%2C+W">W. Trautmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+O">C. O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bassini%2C+R">R. Bassini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boiano%2C+C">C. Boiano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botvina%2C+A+S">A. S. Botvina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Napoli%2C+M">M. De Napoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstroem%2C+M">M. Hellstroem</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henzlova%2C+D">D. Henzlova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imme%2C+G">G. Imme</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iori%2C+I">I. Iori</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Johansson%2C+H">H. Johansson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kezzar%2C+K">K. Kezzar</a> , et al. (32 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0907.1196v1-abstract-short" style="display: inline;"> Isotopic effects in projectile fragmentation at relativistic energies have been studied with the ALADIN forward spectrometer at SIS. Stable and radioactive Sn and La beams with an incident energy of 600 MeV per nucleon have been used in order to explore a wide range of isotopic compositions. Chemical freeze-out temperatures are found to be nearly invariant with respect to the A/Z ratio of the pr&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0907.1196v1-abstract-full').style.display = 'inline'; document.getElementById('0907.1196v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0907.1196v1-abstract-full" style="display: none;"> Isotopic effects in projectile fragmentation at relativistic energies have been studied with the ALADIN forward spectrometer at SIS. Stable and radioactive Sn and La beams with an incident energy of 600 MeV per nucleon have been used in order to explore a wide range of isotopic compositions. Chemical freeze-out temperatures are found to be nearly invariant with respect to the A/Z ratio of the produced spectator sources, consistent with predictions for expanded systems. Consequences for the proposed interpretation of chemical breakup temperatures as representing the limiting temperatures predicted by microscopic models are discussed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0907.1196v1-abstract-full').style.display = 'none'; document.getElementById('0907.1196v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 July, 2009; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2009. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 4 figures, contribution to proceedings of International School of Nuclear Physics, 30th Course, Heavy-Ion Collisions from the Coulomb Barrier to the Quark-Gluon Plasma, Erice-Sicily: 16 - 24 September 2008</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Prog.Part.Nucl.Phys.62:407-412,2009 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0903.1772">arXiv:0903.1772</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0903.1772">pdf</a>, <a href="https://arxiv.org/ps/0903.1772">ps</a>, <a href="https://arxiv.org/format/0903.1772">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.102.152701">10.1103/PhysRevLett.102.152701 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isotopic Dependence of the Nuclear Caloric Curve </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=The+ALADIN2000+Collaboration"> The ALADIN2000 Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Sfienti%2C+C">C. Sfienti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+O">C. O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bassini%2C+R">R. Bassini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boiano%2C+C">C. Boiano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botvina%2C+A+S">A. S. Botvina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Napoli%2C+M">M. De Napoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstroem%2C+M">M. Hellstroem</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henzlova%2C+D">D. Henzlova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imme%2C+G">G. Imme</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iori%2C+I">I. Iori</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Johansson%2C+H">H. Johansson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kezzar%2C+K">K. Kezzar</a> , et al. (32 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0903.1772v1-abstract-short" style="display: inline;"> The A/Z dependence of projectile fragmentation at relativistic energies has been studied with the ALADIN forward spectrometer at SIS. A stable beam of 124Sn and radioactive beams of 124La and 107Sn at 600 MeV per nucleon have been used in order to explore a wide range of isotopic compositions. Chemical freeze-out temperatures are found to be nearly invariant with respect to the A/Z of the produc&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0903.1772v1-abstract-full').style.display = 'inline'; document.getElementById('0903.1772v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0903.1772v1-abstract-full" style="display: none;"> The A/Z dependence of projectile fragmentation at relativistic energies has been studied with the ALADIN forward spectrometer at SIS. A stable beam of 124Sn and radioactive beams of 124La and 107Sn at 600 MeV per nucleon have been used in order to explore a wide range of isotopic compositions. Chemical freeze-out temperatures are found to be nearly invariant with respect to the A/Z of the produced spectator sources, consistent with predictions for expanded systems. Small Coulomb effects (螖T \approx 0.6 MeV) appear for residue production near the onset of multifragmentation. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0903.1772v1-abstract-full').style.display = 'none'; document.getElementById('0903.1772v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 March, 2009; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2009. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">11 pages, 3 figures, accepted for publ. in Phys. Rev. Lett</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.102:152701,2009 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0810.3157">arXiv:0810.3157</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0810.3157">pdf</a>, <a href="https://arxiv.org/ps/0810.3157">ps</a>, <a href="https://arxiv.org/format/0810.3157">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.physletb.2009.03.049">10.1016/j.physletb.2009.03.049 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Structure of 55Ti from relativistic one-neutron knockout </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Maierbeck%2C+P">P. Maierbeck</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gernh%C3%A4user%2C+R">R. Gernh盲user</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kr%C3%BCcken%2C+R">R. Kr眉cken</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kr%C3%B6ll%2C+T">T. Kr枚ll</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez-Pol%2C+H">H. Alvarez-Pol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aksouh%2C+F">F. Aksouh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Behr%2C+K">K. Behr</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benjamim%2C+E+A">E. A. Benjamim</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bildstein%2C+V">V. Bildstein</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=B%C3%B6hmer%2C+M">M. B枚hmer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boretzky%2C+K">K. Boretzky</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borge%2C+M+J+G">M. J. G. Borge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Br%C3%BCnle%2C+A">A. Br眉nle</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=B%C3%BCrger%2C+A">A. B眉rger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caama%C3%B1o%2C+M">M. Caama帽o</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatillon%2C+A">A. Chatillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chulkov%2C+L+V">L. V. Chulkov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Enders%2C+J">J. Enders</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Eppinger%2C+K">K. Eppinger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Faestermann%2C+T">T. Faestermann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Friese%2C+J">J. Friese</a> , et al. (40 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0810.3157v2-abstract-short" style="display: inline;"> Results are presented from a one-neutron knockout reaction at relativistic energies on 56Ti using the GSI FRS as a two-stage magnetic spectrometer and the Miniball array for gamma-ray detection. Inclusive and exclusive longitudinal momentum distributions and cross-sections were measured enabling the determination of the orbital angular momentum of the populated states. First-time observation of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0810.3157v2-abstract-full').style.display = 'inline'; document.getElementById('0810.3157v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0810.3157v2-abstract-full" style="display: none;"> Results are presented from a one-neutron knockout reaction at relativistic energies on 56Ti using the GSI FRS as a two-stage magnetic spectrometer and the Miniball array for gamma-ray detection. Inclusive and exclusive longitudinal momentum distributions and cross-sections were measured enabling the determination of the orbital angular momentum of the populated states. First-time observation of the 955(6) keV nu p3/2-hole state in 55Ti is reported. The measured data for the first time proves that the ground state of 55Ti is a 1/2- state, in agreement with shell-model calculations using the GXPF1A interaction that predict a sizable N=34 gap in 54Ca. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0810.3157v2-abstract-full').style.display = 'none'; document.getElementById('0810.3157v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 February, 2009; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 October, 2008; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2008. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">12 pages, 3 figures, submitted to Physics Letters B 13 pages, 4 figures, resubmitted to Physics Letters B (major revision to meet the suggestions of the reviewers)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Lett.B675:22-27,2009 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0802.4263">arXiv:0802.4263</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0802.4263">pdf</a>, <a href="https://arxiv.org/ps/0802.4263">ps</a>, <a href="https://arxiv.org/format/0802.4263">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.77.061303">10.1103/PhysRevC.77.061303 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Proton-proton correlations observed in two-proton decay of $^{19}$Mg and $^{16}$Ne </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Mukha%2C+I">I. Mukha</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grigorenko%2C+L">L. Grigorenko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Summerer%2C+K">K. Summerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acosta%2C+L">L. Acosta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez%2C+M+A+G">M. A. G. Alvarez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatillon%2C+A">A. Chatillon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Espino%2C+J">J. Espino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fomichev%2C+A">A. Fomichev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Garcia-Ramos%2C+J+E">J. E. Garcia-Ramos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gomez-Camacho%2C+J">J. Gomez-Camacho</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hofmann%2C+J">J. Hofmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kiselev%2C+O">O. Kiselev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Korsheninnikov%2C+A">A. Korsheninnikov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kurz%2C+N">N. Kurz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Litvinov%2C+Y">Yu. Litvinov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martel%2C+I">I. Martel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nociforo%2C+C">C. Nociforo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ott%2C+W">W. Ott</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pfutzner%2C+M">M. Pfutzner</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rodriguez-Tajes%2C+C">C. Rodriguez-Tajes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roeckl%2C+E">E. Roeckl</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Stanoiu%2C+M">M. Stanoiu</a> , et al. (2 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0802.4263v1-abstract-short" style="display: inline;"> Proton-proton correlations were observed for the two-proton decays of the ground states of $^{19}$Mg and $^{16}$Ne. The trajectories of the respective decay products, $^{17}$Ne+p+p and $^{14}$O+p+p, were measured by using a tracking technique with microstrip detectors. These data were used to reconstruct the angular correlations of fragments projected on planes transverse to the precursor moment&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0802.4263v1-abstract-full').style.display = 'inline'; document.getElementById('0802.4263v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0802.4263v1-abstract-full" style="display: none;"> Proton-proton correlations were observed for the two-proton decays of the ground states of $^{19}$Mg and $^{16}$Ne. The trajectories of the respective decay products, $^{17}$Ne+p+p and $^{14}$O+p+p, were measured by using a tracking technique with microstrip detectors. These data were used to reconstruct the angular correlations of fragments projected on planes transverse to the precursor momenta. The measured three-particle correlations reflect a genuine three-body decay mechanism and allowed us to obtain spectroscopic information on the precursors with valence protons in the $sd$ shell. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0802.4263v1-abstract-full').style.display = 'none'; document.getElementById('0802.4263v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 February, 2008; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2008. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">5 pages 6 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C77:061303,2008 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0711.4462">arXiv:0711.4462</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0711.4462">pdf</a>, <a href="https://arxiv.org/ps/0711.4462">ps</a>, <a href="https://arxiv.org/format/0711.4462">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1142/S0218301308010829">10.1142/S0218301308010829 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> N/Z Dependence of Projectile Fragmentation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Trautmann%2C+W">W. Trautmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+O">C. O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bassini%2C+R">R. Bassini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boiano%2C+C">C. Boiano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botvina%2C+A+S">A. S. Botvina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Napoli%2C+M">M. De Napoli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J+D">J. D. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstroem%2C+M">M. Hellstroem</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henzlova%2C+D">D. Henzlova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imme%2C+G">G. Imme</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iori%2C+I">I. Iori</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Johansson%2C+H">H. Johansson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kezzar%2C+K">K. Kezzar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lafriakh%2C+A">A. Lafriakh</a> , et al. (31 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0711.4462v1-abstract-short" style="display: inline;"> The N/Z dependence of projectile fragmentation at relativistic energies has been studied in a recent experiment at the GSI laboratory with the ALADiN forward spectrometer coupled to the LAND neutron detector. Besides a primary beam of 124Sn, also secondary beams of 124La and 107Sn delivered by the FRS fragment separator have been used in order to extend the range of isotopic compositions of the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0711.4462v1-abstract-full').style.display = 'inline'; document.getElementById('0711.4462v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0711.4462v1-abstract-full" style="display: none;"> The N/Z dependence of projectile fragmentation at relativistic energies has been studied in a recent experiment at the GSI laboratory with the ALADiN forward spectrometer coupled to the LAND neutron detector. Besides a primary beam of 124Sn, also secondary beams of 124La and 107Sn delivered by the FRS fragment separator have been used in order to extend the range of isotopic compositions of the produced spectator sources. With the achieved mass resolution of 螖A/A \approx 1.5%, lighter isotopes with atomic numbers Z \le 10 are individually resolved. The presently ongoing analyses of the measured isotope yields focus on isoscaling and its relation to the properties of hot fragments at freeze-out and on the derivation of chemical freeze-out temperatures which are found to be independent of the isotopic composition of the studied systems. The latter result is at variance with the predictions for limiting temperatures as obtained with finite-temperature Hartree-Fock calculations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0711.4462v1-abstract-full').style.display = 'none'; document.getElementById('0711.4462v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 November, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2007. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">11 pages, 5 figures, Proceedings of International Workshop on Nuclear Dynamics in Heavy-Ion Reactions and Neutron Stars, Beijing, July 10-14, 2007, to appear in International Journal of Modern Physics E</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Int.J.Mod.Phys.E17:1838-1849,2008 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0707.0598">arXiv:0707.0598</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0707.0598">pdf</a>, <a href="https://arxiv.org/ps/0707.0598">ps</a>, <a href="https://arxiv.org/format/0707.0598">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2008.01.071">10.1016/j.nima.2008.01.071 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Discriminant Analysis and Secondary-Beam Charge Recognition </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Lukasik%2C+J">J. Lukasik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adrich%2C+P">P. Adrich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+O">C. O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barczyk%2C+T">T. Barczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bassini%2C+R">R. Bassini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bianchin%2C+S">S. Bianchin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boiano%2C+C">C. Boiano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Botvina%2C+A+S">A. S. Botvina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chbihi%2C+A">A. Chbihi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cibor%2C+J">J. Cibor</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czech%2C+B">B. Czech</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Emling%2C+H">H. Emling</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Frankland%2C+J">J. Frankland</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstroem%2C+M">M. Hellstroem</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Henzlova%2C+D">D. Henzlova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Imme%2C+G">G. Imme</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iori%2C+I">I. Iori</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Johansson%2C+H">H. Johansson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kezzar%2C+K">K. Kezzar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lafriakh%2C+A">A. Lafriakh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fevre%2C+A+L">A. Le Fevre</a> , et al. (31 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0707.0598v1-abstract-short" style="display: inline;"> The discriminant-analysis method has been applied to optimize the exotic-beam charge recognition in a projectile fragmentation experiment. The experiment was carried out at the GSI using the fragment separator (FRS) to produce and select the relativistic secondary beams, and the ALADIN setup to measure their fragmentation products following collisions with Sn target nuclei. The beams of neutron&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0707.0598v1-abstract-full').style.display = 'inline'; document.getElementById('0707.0598v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0707.0598v1-abstract-full" style="display: none;"> The discriminant-analysis method has been applied to optimize the exotic-beam charge recognition in a projectile fragmentation experiment. The experiment was carried out at the GSI using the fragment separator (FRS) to produce and select the relativistic secondary beams, and the ALADIN setup to measure their fragmentation products following collisions with Sn target nuclei. The beams of neutron poor isotopes around 124La and 107Sn were selected to study the isospin dependence of the limiting temperature of heavy nuclei by comparing with results for stable 124Sn projectiles. A dedicated detector to measure the projectile charge upstream of the reaction target was not used, and alternative methods had to be developed. The presented method, based on the multivariate discriminant analysis, allowed to increase the efficacy of charge recognition up to about 90%, which was about 20% more than achieved with the simple scalar methods. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0707.0598v1-abstract-full').style.display = 'none'; document.getElementById('0707.0598v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 July, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2007. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 7 eps figures, elsart, submitted to Nucl. Instr. and Meth. A</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/0612001">arXiv:nucl-ex/0612001</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/0612001">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/0612001">ps</a>, <a href="https://arxiv.org/format/nucl-ex/0612001">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.75.044603">10.1103/PhysRevC.75.044603 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Spallation Residues in the Reaction 56Fe + p at 0.3, 0.5, 0.75, 1.0 and 1.5 A GeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Villagrasa-Canton%2C+C">C. Villagrasa-Canton</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boudard%2C+A">A. Boudard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ducret%2C+J+-">J. -E. Ducret</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fernandez%2C+B">B. Fernandez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Leray%2C+S">S. Leray</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Volant%2C+C">C. Volant</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armbruster%2C+P">P. Armbruster</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Enqvist%2C+T">T. Enqvist</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hammache%2C+F">F. Hammache</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Helariutta%2C+K">K. Helariutta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jurado%2C+B">B. Jurado</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ricciardi%2C+M+-">M. -V. Ricciardi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schmidt%2C+K+-">K. -H. Schmidt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Summerer%2C+K">K. Summerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vives%2C+F">F. Vives</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Yordanov%2C+O">O. Yordanov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Audouin%2C+L">L. Audouin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bacri%2C+C+-">C. -O. Bacri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferrant%2C+L">L. Ferrant</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Napolitani%2C+P">P. Napolitani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rejmund%2C+F">F. Rejmund</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Stephan%2C+C">C. Stephan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tassan-Got%2C+L">L. Tassan-Got</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a> , et al. (13 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="nucl-ex/0612001v1-abstract-short" style="display: inline;"> The spallation residues produced in the bombardment of 56}Fe at 1.5, 1.0, 0.75, 0.5 and 0.3 A GeV on a liquid-hydrogen target have been measured using the reverse kinematics technique and the Fragment Separator at GSI (Darmstadt). This technique has permitted the full identification in charge and mass of all isotopes produced with cross-sections larger than 10^{-2} mb down to Z=8. Their individu&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0612001v1-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/0612001v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/0612001v1-abstract-full" style="display: none;"> The spallation residues produced in the bombardment of 56}Fe at 1.5, 1.0, 0.75, 0.5 and 0.3 A GeV on a liquid-hydrogen target have been measured using the reverse kinematics technique and the Fragment Separator at GSI (Darmstadt). This technique has permitted the full identification in charge and mass of all isotopes produced with cross-sections larger than 10^{-2} mb down to Z=8. Their individual production cross-sections and recoil velocities at the five energies are presented. Production cross-sections are compared to previously existing data and to empirical parametric formulas, often used in cosmic-ray astrophysics. The experimental data are also extensively compared to different combinations of intra-nuclear cascade and de-excitation models. It is shown that the yields of the lightest isotopes cannot be accounted for by standard evaporation models. The GEMINI model, which includes an asymmetric fission decay mode, gives an overall good agreement with the data. These experimental data can be directly used for the estimation of composition modifications and damages in materials containing iron in spallation sources. They are also useful for improving high precision cosmic-ray measurements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0612001v1-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/0612001v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 1 December, 2006; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2006. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Submited to Phys. Rev. C (10/2006)</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C75:044603,2007 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/0508014">arXiv:nucl-ex/0508014</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/0508014">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/0508014">ps</a>, <a href="https://arxiv.org/format/nucl-ex/0508014">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.73.015806">10.1103/PhysRevC.73.015806 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Low-energy cross section of the 7Be(p,g)8B solar fusion reaction from Coulomb dissociation of 8B </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Schuemann%2C+F">F. Schuemann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Typel%2C+S">S. Typel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hammache%2C+F">F. Hammache</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Uhlig%2C+F">F. Uhlig</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suemmerer%2C+K">K. Suemmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boettcher%2C+I">I. Boettcher</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina%2C+D">D. Cortina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Foerster%2C+A">A. Foerster</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gai%2C+M">M. Gai</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Greife%2C+U">U. Greife</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grosse%2C+E">E. Grosse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iwasa%2C+N">N. Iwasa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Koczon%2C+P">P. Koczon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohlmeyer%2C+B">B. Kohlmeyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kulessa%2C+R">R. Kulessa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kumagai%2C+H">H. Kumagai</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kurz%2C+N">N. Kurz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Menzel%2C+M">M. Menzel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Motobayashi%2C+T">T. Motobayashi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Oeschler%2C+H">H. Oeschler</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ozawa%2C+A">A. Ozawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ploskon%2C+M">M. Ploskon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Prokopowicz%2C+W">W. Prokopowicz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schwab%2C+E">E. Schwab</a> , et al. (7 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="nucl-ex/0508014v2-abstract-short" style="display: inline;"> Final results from an exclusive measurement of the Coulomb breakup of 8B into 7Be+p at 254 A MeV are reported. Energy-differential Coulomb-breakup cross sections are analyzed using a potential model of 8B and first-order perturbation theory. The deduced astrophysical S_17 factors are in good agreement with the most recent direct 7Be(p,gamma)8B measurements and follow closely the energy dependenc&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0508014v2-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/0508014v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/0508014v2-abstract-full" style="display: none;"> Final results from an exclusive measurement of the Coulomb breakup of 8B into 7Be+p at 254 A MeV are reported. Energy-differential Coulomb-breakup cross sections are analyzed using a potential model of 8B and first-order perturbation theory. The deduced astrophysical S_17 factors are in good agreement with the most recent direct 7Be(p,gamma)8B measurements and follow closely the energy dependence predicted by the cluster-model description of 8B by Descouvemont. We extract a zero-energy S_17 factor of 20.6 +- 0.8 (stat) +- 1.2 (syst) eV b. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0508014v2-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/0508014v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 November, 2005; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 August, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2005. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">14 pages including 16 figures, LaTeX, accepted for publication in Physical Review C. Minor changes in text and layout</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C73:015806,2006 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/0310033">arXiv:nucl-ex/0310033</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/0310033">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/0310033">ps</a>, <a href="https://arxiv.org/format/nucl-ex/0310033">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nuclphysa.2004.01.070">10.1016/j.nuclphysa.2004.01.070 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Production cross-sections and momentum distributions of fragments from neutron-deficient 36Ar at 1.05 A.GeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Caamano%2C+M">M. Caamano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suemmerer%2C+K">K. Suemmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benlliure%2C+J">J. Benlliure</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casarejos%2C+E">E. Casarejos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Muenzenberg%2C+G">G. Muenzenberg</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pereira%2C+J">J. Pereira</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="nucl-ex/0310033v1-abstract-short" style="display: inline;"> We have measured production cross sections and longitudinal momentum distributions of fragments from neutron-deficient 36Ar at 1.05 A.GeV. The production cross-sections show excellent agreement with the predictions of the semiempirical formula EPAX. We have compared these results, involving extremly neutron deficient nuclei, with model calculations to extract informa tion about the response of t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0310033v1-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/0310033v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/0310033v1-abstract-full" style="display: none;"> We have measured production cross sections and longitudinal momentum distributions of fragments from neutron-deficient 36Ar at 1.05 A.GeV. The production cross-sections show excellent agreement with the predictions of the semiempirical formula EPAX. We have compared these results, involving extremly neutron deficient nuclei, with model calculations to extract informa tion about the response of these models close to the driplines. The longitudinal momentum distributions have also been extracted and are compared with the Goldhaber and Morrissey systematics. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0310033v1-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/0310033v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 October, 2003; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2003. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">16 pages, 6 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl.Phys. A733 (2004) 187-199 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/0304011">arXiv:nucl-ex/0304011</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/0304011">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/0304011">ps</a>, <a href="https://arxiv.org/format/nucl-ex/0304011">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.90.232501">10.1103/PhysRevLett.90.232501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Coulomb dissociation of 8B and the low-energy cross section of the 7Be(p,gamma)8B solar fusion reaction </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Schuemann%2C+F">F. Schuemann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hammache%2C+F">F. Hammache</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Typel%2C+S">S. Typel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Uhlig%2C+F">F. Uhlig</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suemmerer%2C+K">K. Suemmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boettcher%2C+I">I. Boettcher</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina%2C+D">D. Cortina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Foerster%2C+A">A. Foerster</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gai%2C+M">M. Gai</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Greife%2C+U">U. Greife</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iwasa%2C+N">N. Iwasa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Koczon%2C+P">P. Koczon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohlmeyer%2C+B">B. Kohlmeyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kulessa%2C+R">R. Kulessa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kumagai%2C+H">H. Kumagai</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kurz%2C+N">N. Kurz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Menzel%2C+M">M. Menzel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Motobayashi%2C+T">T. Motobayashi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Oeschler%2C+H">H. Oeschler</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ozawa%2C+A">A. Ozawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ploskon%2C+M">M. Ploskon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Prokopowicz%2C+W">W. Prokopowicz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schwab%2C+E">E. Schwab</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Senger%2C+P">P. Senger</a> , et al. (6 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="nucl-ex/0304011v2-abstract-short" style="display: inline;"> An exclusive measurement of the Coulomb breakup of 8B into 7Be+p at 254 A MeV allowed to study the angular correlations of the breakup particles. These correlations demonstrate clearly that E1 multipolarity dominates and that E2 multipolarity can be neglected. By using a simple single-particle model for 8B and treating the breakup in first-order perturbation theory, we extract a zero-energy S fa&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0304011v2-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/0304011v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/0304011v2-abstract-full" style="display: none;"> An exclusive measurement of the Coulomb breakup of 8B into 7Be+p at 254 A MeV allowed to study the angular correlations of the breakup particles. These correlations demonstrate clearly that E1 multipolarity dominates and that E2 multipolarity can be neglected. By using a simple single-particle model for 8B and treating the breakup in first-order perturbation theory, we extract a zero-energy S factor of S-(17)(0) = 18.6 +- 1.2 +- 1.0 eV b. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0304011v2-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/0304011v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 June, 2003; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 10 April, 2003; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2003. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">4 pages including 4 figures, LaTeX</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.90:232501,2003 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/9911006">arXiv:nucl-ex/9911006</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/9911006">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/9911006">ps</a>, <a href="https://arxiv.org/format/nucl-ex/9911006">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.61.034607">10.1103/PhysRevC.61.034607 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Modified Empirical Parametrization of Fragmentation Cross Sections </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=S%C3%BCmmerer%2C+K">K. S眉mmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Blank%2C+B">B. Blank</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="nucl-ex/9911006v1-abstract-short" style="display: inline;"> New experimental data obtained mainly at the GSI/FRS facility allow to modify the empirical parametrization of fragmentation cross sections, EPAX. It will be shown that minor modifications of the parameters lead to a much better reproduction of measured cross sections. The most significant changes refer to the description of fragmentation yields close to the projectile and of the memory effect o&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/9911006v1-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/9911006v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/9911006v1-abstract-full" style="display: none;"> New experimental data obtained mainly at the GSI/FRS facility allow to modify the empirical parametrization of fragmentation cross sections, EPAX. It will be shown that minor modifications of the parameters lead to a much better reproduction of measured cross sections. The most significant changes refer to the description of fragmentation yields close to the projectile and of the memory effect of neutron-deficient projectiles. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/9911006v1-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/9911006v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 November, 1999; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 1999. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">10 pages, latex file, 11 postscript figures, submitted to Phys. Rev. C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C61:034607,2000 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/astro-ph/9909317">arXiv:astro-ph/9909317</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/astro-ph/9909317">pdf</a>, <a href="https://arxiv.org/ps/astro-ph/9909317">ps</a>, <a href="https://arxiv.org/format/astro-ph/9909317">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics">astro-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.83.2910">10.1103/PhysRevLett.83.2910 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A Measurement of the Coulomb Dissociation of 8B at 254 MeV/nucleon and the 8B Solar Neutrino Flux </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Iwasa%2C+N">N. Iwasa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boue%2C+F">F. Boue</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Surowka%2C+G">G. Surowka</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suemmerer%2C+K">K. Suemmerer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baumann%2C+T">T. Baumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Blank%2C+B">B. Blank</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Czajkowski%2C+S">S. Czajkowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Forster%2C+A">A. Forster</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gai%2C+M">M. Gai</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grosse%2C+E">E. Grosse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstrom%2C+M">M. Hellstrom</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Koczon%2C+P">P. Koczon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kohlmeyer%2C+B">B. Kohlmeyer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kulessa%2C+R">R. Kulessa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Laue%2C+F">F. Laue</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marchand%2C+C">C. Marchand</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Motobayashi%2C+T">T. Motobayashi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Oeschler%2C+H">H. Oeschler</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ozawa%2C+A">A. Ozawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pravikoff%2C+M+S">M. S. Pravikoff</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schwab%2C+E">E. Schwab</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schwab%2C+W">W. Schwab</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Senger%2C+P">P. Senger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Speer%2C+J">J. Speer</a> , et al. (7 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="astro-ph/9909317v3-abstract-short" style="display: inline;"> We have measured the Coulomb dissociation of 8B into 7Be and proton at 254 MeV/nucleon using a large-acceptance focusing spectrometer. The astrophysical S17 factor for the 7Be(p,gamma)8B reaction at E{c.m.} = 0.25-2.78 MeV is deduced yielding S17(0)=20.6 \pm 1.2 (exp.) \pm 1.0 (theo.) eV-b. This result agrees with the presently adopted zero-energy S17 factor obtained in direct-reaction measure&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/9909317v3-abstract-full').style.display = 'inline'; document.getElementById('astro-ph/9909317v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="astro-ph/9909317v3-abstract-full" style="display: none;"> We have measured the Coulomb dissociation of 8B into 7Be and proton at 254 MeV/nucleon using a large-acceptance focusing spectrometer. The astrophysical S17 factor for the 7Be(p,gamma)8B reaction at E{c.m.} = 0.25-2.78 MeV is deduced yielding S17(0)=20.6 \pm 1.2 (exp.) \pm 1.0 (theo.) eV-b. This result agrees with the presently adopted zero-energy S17 factor obtained in direct-reaction measurements and with the results of other Coulomb-dissociation studies performed at 46.5 and 51.2 MeV/nucleon. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/9909317v3-abstract-full').style.display = 'none'; document.getElementById('astro-ph/9909317v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 October, 1999; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 September, 1999; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 1999. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">paper to be published in Phys. Rev. Lett. 3 figures. New Version fixes formatting problems with the figures only. There are no other changes</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.83:2910-2913,1999 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/9810011">arXiv:nucl-ex/9810011</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/9810011">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/9810011">ps</a>, <a href="https://arxiv.org/format/nucl-ex/9810011">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/S0370-2693(98)01097-1">10.1016/S0370-2693(98)01097-1 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Longitudinal momentum distributions of {16,18}C fragments after one-neutron removal from {17,19}C </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Baumann%2C+T">T. Baumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lenske%2C+H">H. Lenske</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Markenroth%2C+K">K. Markenroth</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schwab%2C+W">W. Schwab</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Smedberg%2C+M+H">M. H. Smedberg</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Axelsson%2C+L">L. Axelsson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bergmann%2C+U">U. Bergmann</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borge%2C+M+J+G">M. J. G. Borge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cortina-Gil%2C+D">D. Cortina-Gil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fraile%2C+L">L. Fraile</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hellstroem%2C+M">M. Hellstroem</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ivanov%2C+M">M. Ivanov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Iwasa%2C+N">N. Iwasa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Janik%2C+R">R. Janik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Jonson%2C+B">B. Jonson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Muenzenberg%2C+G">G. Muenzenberg</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nickel%2C+F">F. Nickel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nilsson%2C+T">T. Nilsson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ozawa%2C+A">A. Ozawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Richter%2C+A">A. Richter</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Riisager%2C+K">K. Riisager</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Scheidenberger%2C+C">C. Scheidenberger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schrieder%2C+G">G. Schrieder</a> , et al. (8 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="nucl-ex/9810011v2-abstract-short" style="display: inline;"> The fragment separator FRS at GSI was used as an energy-loss spectrometer to measure the longitudinal momentum distributions of {16,18}C fragments after one-neutron removal reactions in {17,19}C impinging on a carbon target at about 910 MeV/u. The distributions in the projectile frames are characterized by a FWHM of 141+-6 MeV/c for {16}C and 69+-3 MeV/c for {18}C. The results are compared with&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/9810011v2-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/9810011v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/9810011v2-abstract-full" style="display: none;"> The fragment separator FRS at GSI was used as an energy-loss spectrometer to measure the longitudinal momentum distributions of {16,18}C fragments after one-neutron removal reactions in {17,19}C impinging on a carbon target at about 910 MeV/u. The distributions in the projectile frames are characterized by a FWHM of 141+-6 MeV/c for {16}C and 69+-3 MeV/c for {18}C. The results are compared with experimental data obtained at lower energies and discussed within existing theoretical models. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/9810011v2-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/9810011v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 October, 1998; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 16 October, 1998; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 1998. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">10 pages, 5 figures; uses elsart style; corrected list of authors; will be published in Phys. Lett. B</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> GSI-Preprint-98-51 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Lett. B439 (1998) 256-261 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/nucl-ex/9803014">arXiv:nucl-ex/9803014</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/9803014">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/9803014">ps</a>, <a href="https://arxiv.org/format/nucl-ex/9803014">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevC.58.247">10.1103/PhysRevC.58.247 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Projectile fragmentation of 129Xe at Elab=790 AMeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Reinhold%2C+J">J. Reinhold</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Friese%2C+J">J. Friese</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Koerner%2C+H+-">H. -J. Koerner</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schneider%2C+R">R. Schneider</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Zeitelhack%2C+K">K. Zeitelhack</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geissel%2C+H">H. Geissel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Magel%2C+A">A. Magel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Muenzenberg%2C+G">G. Muenzenberg</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suemmerer%2C+K">K. Suemmerer</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="nucl-ex/9803014v1-abstract-short" style="display: inline;"> We have measured production yields and longitudinal momentum distributions of projectile-like fragments in the reaction 129Xe + 27Al at an energy of Elab=790 AMeV. Production cross sections higher than expected from systematics were observed for nuclei in the neutron-deficient tails of the isotopic distributions. A comparison with previously measured data from the fragmentation of 136Xe ions sho&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/9803014v1-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/9803014v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/9803014v1-abstract-full" style="display: none;"> We have measured production yields and longitudinal momentum distributions of projectile-like fragments in the reaction 129Xe + 27Al at an energy of Elab=790 AMeV. Production cross sections higher than expected from systematics were observed for nuclei in the neutron-deficient tails of the isotopic distributions. A comparison with previously measured data from the fragmentation of 136Xe ions shows that the production yields strongly depend on the neutron excess of the projectile with respect to the line of beta-stability. The momentum distributions exhibit a dependence on the fragment neutron-to-proton ratio in isobaric chains, which was not expected from systematics so far. This can be interpreted by a higher excitation of the projectile during the formation of neutron-deficient fragments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/9803014v1-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/9803014v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 March, 1998; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 1998. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">21 pages, 8 figures, 1 table</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> GSI-Preprint 98-13, March 1998 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C58:247-255,1998 </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>&nbsp;&nbsp;</span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- MetaColumn 1 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 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