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name="order"><option selected value="-announced_date_first">Announcement date (newest first)</option><option value="announced_date_first">Announcement date (oldest first)</option><option value="-submitted_date">Submission date (newest first)</option><option value="submitted_date">Submission date (oldest first)</option><option value="">Relevance</option></select> </span> </div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2105.09233">arXiv:2105.09233</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2105.09233">pdf</a>, <a href="https://arxiv.org/format/2105.09233">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"> Symmetry energy at high densities from neutron/proton flow excitation functions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</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=%C5%81ukasik%2C+J">J. 艁ukasik</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=Cozma%2C+M+D">M. D. Cozma</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ga%C5%A1pari%C4%87%2C+I">I. Ga拧pari膰</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=Lihtar%2C+I">I. Lihtar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Trautmann%2C+W">W. Trautmann</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="2105.09233v1-abstract-short" style="display: inline;"> Determination of the high density behavior of the symmetry energy through the simultaneous measurement of elliptic flow excitation functions of neutrons, protons and light clusters is proposed. The elliptic flow developed in relativistic heavy ion collisions has been proven theoretically and experimentally to have a unique sensitivity and robustness in probing the symmetry energy up to around&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.09233v1-abstract-full').style.display = 'inline'; document.getElementById('2105.09233v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2105.09233v1-abstract-full" style="display: none;"> Determination of the high density behavior of the symmetry energy through the simultaneous measurement of elliptic flow excitation functions of neutrons, protons and light clusters is proposed. The elliptic flow developed in relativistic heavy ion collisions has been proven theoretically and experimentally to have a unique sensitivity and robustness in probing the symmetry energy up to around $2 蟻_{o}$. The knowledge of the density dependence of the symmetry energy in a broad range of densities will provide a missing link for astrophysical predictions of the neutron star mass--radius relation. In particular, the data colud provide tighter constraints on the slope parameter L and entirely new limits on $K_{sym}$, the currently poorly constrained symmetry energy curvature parameter. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.09233v1-abstract-full').style.display = 'none'; document.getElementById('2105.09233v1-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> 19 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2021. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1907.05471">arXiv:1907.05471</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1907.05471">pdf</a>, <a href="https://arxiv.org/format/1907.05471">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.100.034320">10.1103/PhysRevC.100.034320 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Experimental investigation of $伪$-condensation in light nuclei </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Bishop%2C+J">Jack Bishop</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kokalova%2C+T">Tzany Kokalova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Freer%2C+M">Martin Freer</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=Assie%2C+M">M Assie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bailey%2C+S">S Bailey</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Curtis%2C+N">N Curtis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Aquila%2C+D">D Dell&#39;Aquila</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Luca%2C+S">S De Luca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Francalanza%2C+L">L Francalanza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gnoffo%2C+B">B Gnoffo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martorana%2C+N+S">N. S. Martorana</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Norella%2C+S">S Norella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+E+V">E. V. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P Russotto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Quattrocchi%2C+L">L Quattrocchi</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="1907.05471v2-abstract-short" style="display: inline;"> Method: To examine signatures of this alpha-condensation, a compound nucleus reaction using 160, 280, and 400 MeV 16O beams impinging on a carbon target was used to investigate the 12C(16O,7a) reaction. This permits a search for near-threshold states in the alpha-conjugate nuclei up to 24Mg. Results: Events up to an alpha-particle multiplicity of 7 were measured and the results were compared to bo&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1907.05471v2-abstract-full').style.display = 'inline'; document.getElementById('1907.05471v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1907.05471v2-abstract-full" style="display: none;"> Method: To examine signatures of this alpha-condensation, a compound nucleus reaction using 160, 280, and 400 MeV 16O beams impinging on a carbon target was used to investigate the 12C(16O,7a) reaction. This permits a search for near-threshold states in the alpha-conjugate nuclei up to 24Mg. Results: Events up to an alpha-particle multiplicity of 7 were measured and the results were compared to both an Extended Hauser-Feshbach calculation and the Fermi break-up model. The measured multiplicity distribution exceeded that predicted from a sequential decay mechanism and had a better agreement with the multi-particle Fermi break-up model. Examination of how these 7 alpha final states could be reconstructed to form 8Be and 12C(0_2+) showed a quantitative difference in which decay modes were dominant compared to the Fermi break-up model. No new states were observed in 16O, 20Ne, and 24Mg due to the effect of the N-alpha penetrability suppressing the total alpha-particle dissociation decay mode. Conclusion: The reaction mechanism for a high energy compound nucleus reaction can only be described by a hybrid of sequential decay and multi-particle breakup. Highly alpha-clustered states were seen which did not originate from simple binary reaction processes. Direct investigations of near-threshold states in N-alpha systems are inherently impeded by the Coulomb barrier prohibiting the observation of states in the N-alpha decay channel. No evidence of a highly clustered 15.1 MeV state in 16O was observed from (28Si*,12C(0_2+))16O(0_6+) when reconstructing the Hoyle state from 3 alpha-particles. Therefore, no experimental signatures for alpha-condensation were observed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1907.05471v2-abstract-full').style.display = 'none'; document.getElementById('1907.05471v2-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> 19 August, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 July, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. C 100, 034320 (2019) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1902.05262">arXiv:1902.05262</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1902.05262">pdf</a>, <a href="https://arxiv.org/format/1902.05262">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="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/10.1393/ncr/i2019-10157-1">10.1393/ncr/i2019-10157-1 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Experimental nuclear astrophysics in Italy </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Broggini%2C+C">C. Broggini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Straniero%2C+O">O. Straniero</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Taiuti%2C+M+G+F">M. G. F. Taiuti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+Angelis%2C+G">G. de Angelis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benzoni%2C+G">G. Benzoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bruno%2C+G+E">G. E. Bruno</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bufalino%2C+S">S. Bufalino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colonna%2C+N">N. Colonna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Contalbrigo%2C+M">M. Contalbrigo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cosentino%2C+G">G. Cosentino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cristallo%2C+S">S. Cristallo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Curceanu%2C+C">C. Curceanu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Depalo%2C+R">R. Depalo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Leva%2C+A">A. Di Leva</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Feliciello%2C+A">A. Feliciello</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gammino%2C+S">S. Gammino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galat%C3%A0%2C+A">A. Galat脿</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Cognata%2C+M">M. La Cognata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lea%2C+R">R. Lea</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Leoni%2C+S">S. Leoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manzari%2C+V">V. Manzari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mascali%2C+D">D. Mascali</a> , et al. (14 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="1902.05262v3-abstract-short" style="display: inline;"> Nuclear astrophysics, the union of nuclear physics and astronomy, went through an impressive expansion during the last twenty years. This could be achieved thanks to milestone improvements in astronomical observations, cross section measurements, powerful computer simulations and much refined stellar models. Italian groups are giving quite important contributions to every domain of nuclear astroph&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1902.05262v3-abstract-full').style.display = 'inline'; document.getElementById('1902.05262v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1902.05262v3-abstract-full" style="display: none;"> Nuclear astrophysics, the union of nuclear physics and astronomy, went through an impressive expansion during the last twenty years. This could be achieved thanks to milestone improvements in astronomical observations, cross section measurements, powerful computer simulations and much refined stellar models. Italian groups are giving quite important contributions to every domain of nuclear astrophysics, sometimes being the leaders of worldwide unique experiments. In this paper we will discuss the astrophysical scenarios where nuclear astrophysics plays a key role and we will provide detailed descriptions of the present and future of the experiments on nuclear astrophysics which belong to the scientific programme of INFN (the National Institute for Nuclear Physics in Italy). <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1902.05262v3-abstract-full').style.display = 'none'; document.getElementById('1902.05262v3-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> 9 April, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 14 February, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2019. </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">Added paragraphs 5.6 and 7.2. Paragraph 7.3 (former 7.2) revised. Accepted for publication in La Rivista del Nuovo Cimento</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Rivista del Nuovo Cimento 42, 3 (2019) pp. 103-152 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1803.03046">arXiv:1803.03046</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1803.03046">pdf</a>, <a href="https://arxiv.org/ps/1803.03046">ps</a>, <a href="https://arxiv.org/format/1803.03046">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"> Isospin influence on dynamical production of Intermediate Mass Fragments at Fermi Energies </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+E+V">E. V. Pagano</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=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cap%2C+T">T. Cap</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Luca%2C+S">S. De Luca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gnoffo%2C+B">B. Gnoffo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martorana%2C+N+S">N. S. Martorana</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Minniti%2C+T">T. Minniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Norella%2C+S">S. Norella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piasecki%2C+E">E. Piasecki</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Quattrocchi%2C+L">L. Quattrocchi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Siwek-Wilczy%C5%84ska%2C+K">K. Siwek-Wilczy艅ska</a> , et al. (4 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="1803.03046v1-abstract-short" style="display: inline;"> The Intermediate Mass Fragments emission probability from Projectile-Like Fragment break-up in semi-peripheral reactions has been measured in collisions of $^{124}$Xe projectiles with two different targets of $^{64}$Ni and $^{64}$Zn at the laboratory energy of 35 \amev. The two colliding systems differ only for the target atomic number Z and, consequently, for the Isospin $N/Z$ ratio. An enhanceme&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1803.03046v1-abstract-full').style.display = 'inline'; document.getElementById('1803.03046v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1803.03046v1-abstract-full" style="display: none;"> The Intermediate Mass Fragments emission probability from Projectile-Like Fragment break-up in semi-peripheral reactions has been measured in collisions of $^{124}$Xe projectiles with two different targets of $^{64}$Ni and $^{64}$Zn at the laboratory energy of 35 \amev. The two colliding systems differ only for the target atomic number Z and, consequently, for the Isospin $N/Z$ ratio. An enhancement of Intermediate Mass Fragments production for the neutron rich $^{64}$Ni target, with respect to the $^{64}$Zn, is found. In the case of one Intermediate Mass Fragment emission, the contributions of the dynamical and statistical emissions have been evaluated, showing that the increase of the effect above is due to an enhancement of the dynamical emission probability, especially for heavy IMFs (Z$\gtrsim$ 7). This proves an influence of the target Isospin on inducing the dynamical fragment production from Projectile-Like Fragment break-up. In addition, a comparison of the Xe+Ni,Zn results with the previously studied $^{112,124}Sn+^{58,64}Ni$ systems is discussed in order to investigate the influence of the projectile Isospin alone and to disentangle between Isospin effects against system-size effects on the emission probability. These comparisons suggest that the prompt-dynamical emission is mainly ruled by the $N/Z$ content of, both, projectile and target; for the cases here investigated, the influence of the system size on the dynamical emission probability can be excluded. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1803.03046v1-abstract-full').style.display = 'none'; document.getElementById('1803.03046v1-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 March, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2018. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1608.04332">arXiv:1608.04332</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1608.04332">pdf</a>, <a href="https://arxiv.org/ps/1608.04332">ps</a>, <a href="https://arxiv.org/format/1608.04332">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.94.034608">10.1103/PhysRevC.94.034608 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gannon%2C+S">S. Gannon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kupny%2C+S">S. Kupny</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lasko%2C+P">P. Lasko</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=Adamczyk%2C+M">M. Adamczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Ajlan%2C+A">A. Al-Ajlan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Garawi%2C+M">M. Al-Garawi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Homaidhi%2C+S">S. Al-Homaidhi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</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=Ayyad%2C+Y">Y. Ayyad</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Basrak%2C+Z">Z. Basrak</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=Boisjoli%2C+M">M. Boisjoli</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=Brzychczyk%2C+J">J. Brzychczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Budzanowski%2C+A">A. Budzanowski</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=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cammarata%2C+P">P. Cammarata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chajecki%2C+Z">Z. Chajecki</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=Chbihi%2C+A">A. Chbihi</a> , et al. (67 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="1608.04332v2-abstract-short" style="display: inline;"> Directed and elliptic flows of neutrons and light charged particles were measured for the reaction 197Au+197Au at 400 MeV/nucleon incident energy within the ASY-EOS experimental campaign at the GSI laboratory. The detection system consisted of the Large Area Neutron Detector LAND, combined with parts of the CHIMERA multidetector, of the ALADIN Time-of-flight Wall, and of the Washington-University&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1608.04332v2-abstract-full').style.display = 'inline'; document.getElementById('1608.04332v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1608.04332v2-abstract-full" style="display: none;"> Directed and elliptic flows of neutrons and light charged particles were measured for the reaction 197Au+197Au at 400 MeV/nucleon incident energy within the ASY-EOS experimental campaign at the GSI laboratory. The detection system consisted of the Large Area Neutron Detector LAND, combined with parts of the CHIMERA multidetector, of the ALADIN Time-of-flight Wall, and of the Washington-University Microball detector. The latter three arrays were used for the event characterization and reaction-plane reconstruction. In addition, an array of triple telescopes, KRATTA, was used for complementary measurements of the isotopic composition and flows of light charged particles. From the comparison of the elliptic flow ratio of neutrons with respect to charged particles with UrQMD predictions, a value 纬= 0.72 \pm 0.19 is obtained for the power-law coefficient describing the density dependence of the potential part in the parametrization of the symmetry energy. It represents a new and more stringent constraint for the regime of supra-saturation density and confirms, with a considerably smaller uncertainty, the moderately soft to linear density dependence deduced from the earlier FOPI-LAND data. The densities probed are shown to reach beyond twice saturation. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1608.04332v2-abstract-full').style.display = 'none'; document.getElementById('1608.04332v2-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 September, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 15 August, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2016. </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">25 pages, 22 figures, accepted for publication 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 94, 034608 (2016) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1603.01114">arXiv:1603.01114</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1603.01114">pdf</a>, <a href="https://arxiv.org/format/1603.01114">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"> Probing clustering in excited alpha-conjugate buclei </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Raduta%2C+A+R">Ad. R. Raduta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alba%2C+R">R. Alba</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjee%2C+M">M. Chatterjee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzano%2C+G">G. Lanzano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</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="1603.01114v1-abstract-short" style="display: inline;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}$Ca+$^{12}$C at 25 MeV per nucleon bombarding energy was used to produce $伪$-emission sources. From a careful selection of these sources provided by a complete detection and from comparisons with models of sequential and simultaneous decays, evidence in favor of $伪$-particle clustering from excited $^{16}O$, $^{20}Ne$ and&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1603.01114v1-abstract-full').style.display = 'inline'; document.getElementById('1603.01114v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1603.01114v1-abstract-full" style="display: none;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}$Ca+$^{12}$C at 25 MeV per nucleon bombarding energy was used to produce $伪$-emission sources. From a careful selection of these sources provided by a complete detection and from comparisons with models of sequential and simultaneous decays, evidence in favor of $伪$-particle clustering from excited $^{16}O$, $^{20}Ne$ and $^{24}Mg$ is reported. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1603.01114v1-abstract-full').style.display = 'none'; document.getElementById('1603.01114v1-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 March, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2016. </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">15 pages, 6 figures, accepted in Physics Letters B</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1602.05827">arXiv:1602.05827</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1602.05827">pdf</a>, <a href="https://arxiv.org/ps/1602.05827">ps</a>, <a href="https://arxiv.org/format/1602.05827">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/10.1051/epjconf/201611707014">10.1051/epjconf/201611707014 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Alpha-particle clustering in excited expanding self-conjugate nuclei </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Raduta%2C+A+R">Ad. R. Raduta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</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="1602.05827v1-abstract-short" style="display: inline;"> The fragmentation of quasi-projectiles from the nuclear reaction 40Ca + 12C at 25 MeV/nucleon was used to produce alpha-emission sources. From a careful selection of these sources provided by a complete detection and from comparisons with models of sequential and simultaneous decays, strong indications in favour of $伪$-particle clustering in excited 16O, 20Ne and 24}Mg are reported. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1602.05827v1-abstract-full" style="display: none;"> The fragmentation of quasi-projectiles from the nuclear reaction 40Ca + 12C at 25 MeV/nucleon was used to produce alpha-emission sources. From a careful selection of these sources provided by a complete detection and from comparisons with models of sequential and simultaneous decays, strong indications in favour of $伪$-particle clustering in excited 16O, 20Ne and 24}Mg are reported. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1602.05827v1-abstract-full').style.display = 'none'; document.getElementById('1602.05827v1-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> 18 February, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2016. </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">8 pages, 4 figures, 12th International Conference on Nucleus-Nucleus collisions (NN2015), 21-26 June 2015, Catania, Italy</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1507.03139">arXiv:1507.03139</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1507.03139">pdf</a>, <a href="https://arxiv.org/ps/1507.03139">ps</a>, <a href="https://arxiv.org/format/1507.03139">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.92.064614">10.1103/PhysRevC.92.064614 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Freeze-out configuration properties in the 197Au + 197Au reaction at 23 AMeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Najman%2C+R">R. Najman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Planeta%2C+R">R. Planeta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Sochocka%2C+A">A. Sochocka</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cap%2C+T">T. Cap</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grzeszczuk%2C+A">A. Grzeszczuk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kowalski%2C+S">S. Kowalski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kozik%2C+T">T. Kozik</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</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=Nicolis%2C+N+G">N. G. Nicolis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piasecki%2C+E">E. Piasecki</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Siwek-Wilczynska%2C+K">K. Siwek-Wilczynska</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Skwira-Chalot%2C+I">I. Skwira-Chalot</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Trifiro%2C+A">A. Trifiro</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="1507.03139v1-abstract-short" style="display: inline;"> Data from the experiment on the 197Au + 197Au reaction at 23 AMeV are analyzed with an aim to find signatures of exotic nuclear configurations such as toroid-shaped objects. The experimental data are compared with predictions of the ETNA code dedicated to look for such configurations and with the QMD model. A novel criterion of selecting events possibly resulting from the formation of exotic freez&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1507.03139v1-abstract-full').style.display = 'inline'; document.getElementById('1507.03139v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1507.03139v1-abstract-full" style="display: none;"> Data from the experiment on the 197Au + 197Au reaction at 23 AMeV are analyzed with an aim to find signatures of exotic nuclear configurations such as toroid-shaped objects. The experimental data are compared with predictions of the ETNA code dedicated to look for such configurations and with the QMD model. A novel criterion of selecting events possibly resulting from the formation of exotic freeze-out configurations, &#34;the efficiency factor&#34;, is tested. Comparison between experimental data and model predictions may indicate for the formation of flat/toroidal nuclear systems. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1507.03139v1-abstract-full').style.display = 'none'; document.getElementById('1507.03139v1-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 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">Journal ref:</span> Phys. Rev. C 92, 064614 (2015) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1501.00801">arXiv:1501.00801</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1501.00801">pdf</a>, <a href="https://arxiv.org/ps/1501.00801">ps</a>, <a href="https://arxiv.org/format/1501.00801">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.91.041601">10.1103/PhysRevC.91.041601 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Dipolar degrees of freedom and Isospin equilibration processes in Heavy Ion collisions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berceanu%2C+I">I. Berceanu</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=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Agodi%2C+C">C. Agodi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cavallaro%2C+S">S. Cavallaro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjee%2C+M+B">M. B. Chatterjee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Francalanza%2C+L">L. Francalanza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grassi%2C+L">L. Grassi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gnoffo%2C+B">B. Gnoffo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Han%2C+J">J. Han</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+C+M+T+M+A">C. Maiolino T. Minniti A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+E+V">E. V. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Quattrocchi%2C+L">L. Quattrocchi</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="1501.00801v1-abstract-short" style="display: inline;"> Background: In heavy ion collision at the Fermi energies Isospin equilibration processes occur- ring when nuclei with different charge/mass asymmetries interacts have been investigated to get information on the nucleon-nucleon Iso-vectorial effective interaction. Purpose: In this paper, for the system 48Ca +27 Al at 40 MeV/nucleon, we investigate on this process by means of an observable tightly l&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.00801v1-abstract-full').style.display = 'inline'; document.getElementById('1501.00801v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1501.00801v1-abstract-full" style="display: none;"> Background: In heavy ion collision at the Fermi energies Isospin equilibration processes occur- ring when nuclei with different charge/mass asymmetries interacts have been investigated to get information on the nucleon-nucleon Iso-vectorial effective interaction. Purpose: In this paper, for the system 48Ca +27 Al at 40 MeV/nucleon, we investigate on this process by means of an observable tightly linked to isospin equilibration processes and sensitive in exclusive way to the dynamical stage of the collision. From the comparison with dynamical model calculations we want also to obtain information on the Iso-vectorial effective microscopic interaction. Method: The average time derivative of the total dipole associated to the relative motion of all emitted charged particles and fragments has been determined from the measured charges and velocities by using the 4? multi-detector CHIMERA. The average has been determined for semi- peripheral collisions and for different charges Zb of the biggest produced fragment. Experimental evidences collected for the systems 27Al+48Ca and 27Al+40Ca at 40 MeV/nucleon used to support this novel method of investigation are also discussed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.00801v1-abstract-full').style.display = 'none'; document.getElementById('1501.00801v1-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 January, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">Submitted for publication on Phys. Rev. C. 0n 24-oct-2014</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1404.3758">arXiv:1404.3758</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1404.3758">pdf</a>, <a href="https://arxiv.org/ps/1404.3758">ps</a>, <a href="https://arxiv.org/format/1404.3758">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"> Evidence for a Novel Reaction Mechanism of a Prompt Shock-Induced Fission Following the Fusion of 78Kr and 40Ca Nuclei at E/A =10 MeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Henry%2C+E">E. Henry</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Toke%2C+J">J. Toke</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nyibule%2C+S">S. Nyibule</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Quinlan%2C+M">M. Quinlan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Schroder%2C+W+U">W. U. Schroder</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ademard%2C+G">G. Ademard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beck%2C+C">C. Beck</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berceanu%2C+I">I. Berceanu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bonnet%2C+E">E. Bonnet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</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=Colonna%2C+M">M. Colonna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=DOnofrio%2C+A">A. DOnofrio</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=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Commara%2C+M">M. La Commara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lebhertz%2C+D">D. Lebhertz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a> , et al. (18 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="1404.3758v1-abstract-short" style="display: inline;"> An analysis of experimental data from the inverse-kinematics ISODEC experiment on 78Kr+40Ca reaction at a bombarding energy of 10 AMeV has revealed signatures of a hitherto unknown reaction mechanism, intermediate between the classical damped binary collisions and fusion-fission, but also substantially different from what is being termed in the literature as fast fission or quasi fission. These si&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1404.3758v1-abstract-full').style.display = 'inline'; document.getElementById('1404.3758v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1404.3758v1-abstract-full" style="display: none;"> An analysis of experimental data from the inverse-kinematics ISODEC experiment on 78Kr+40Ca reaction at a bombarding energy of 10 AMeV has revealed signatures of a hitherto unknown reaction mechanism, intermediate between the classical damped binary collisions and fusion-fission, but also substantially different from what is being termed in the literature as fast fission or quasi fission. These signatures point to a scenario where the system fuses transiently while virtually equilibrating mass asymmetry and energy and, yet, keeping part of the energy stored in a collective shock-imparted and, possibly, angular momentum bearing form of excitation. Subsequently the system fissions dynamically along the collision or shock axis with the emerging fragments featuring a broad mass spectrum centered around symmetric fission, relative velocities somewhat higher along the fission axis than in transverse direction, and virtually no intrinsic spin. The class of massasymmetric fission events shows a distinct preference for the more massive fragments to proceed along the beam direction, a characteristic reminiscent of that reported earlier for dynamic fragmentation of projectile-like fragments alone and pointing to the memory of the initial mass and velocity distribution. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1404.3758v1-abstract-full').style.display = 'none'; document.getElementById('1404.3758v1-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 April, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2014. </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">Report number:</span> UR-NCUR 14-032 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1212.4593">arXiv:1212.4593</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1212.4593">pdf</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.2013.03.028">10.1016/j.nima.2013.03.028 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Kinematical coincidence method in transfer reactions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Acosta%2C+L">L. Acosta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berceanu%2C+I">I. Berceanu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjiee%2C+M+B">M. B. Chatterjiee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=FrancalanzA%2C+L">L. FrancalanzA</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gian%C3%AC%2C+R">R. Gian矛</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grassi%2C+L">L. Grassi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grzeszczuk%2C+A">A. Grzeszczuk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Loria%2C+D">D. Loria</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Minniti%2C+T">T. Minniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+E+V">E. V. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pop%2C+A">A. Pop</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rosato%2C+E">E. Rosato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a> , et al. (5 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="1212.4593v2-abstract-short" style="display: inline;"> A new method to extract high resolution angular distributions from kinematical coincidence measurements in binary reactions is presented. Kinematic is used to extract the center of mass angular distribution from the measured energy spectrum of light particles. Results obtained in the case of 10Be+p--&gt;9Be+d reaction measured with the CHIMERA detector are shown. An angular resolution of few degrees&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1212.4593v2-abstract-full').style.display = 'inline'; document.getElementById('1212.4593v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1212.4593v2-abstract-full" style="display: none;"> A new method to extract high resolution angular distributions from kinematical coincidence measurements in binary reactions is presented. Kinematic is used to extract the center of mass angular distribution from the measured energy spectrum of light particles. Results obtained in the case of 10Be+p--&gt;9Be+d reaction measured with the CHIMERA detector are shown. An angular resolution of few degrees in the center of mass is obtained. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1212.4593v2-abstract-full').style.display = 'none'; document.getElementById('1212.4593v2-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 December, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 19 December, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 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">6 Page 10 Figures submitted to Nuclear Instruments and Methods 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/1209.6461">arXiv:1209.6461</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1209.6461">pdf</a>, <a href="https://arxiv.org/ps/1209.6461">ps</a>, <a href="https://arxiv.org/format/1209.6461">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/10.1088/1742-6596/420/1/012105">10.1088/1742-6596/420/1/012105 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Correlations between isospin dynamics and Intermediate Mass Fragments emission time scales: a probe for the symmetry energy in asymmetric nuclear matter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baran%2C+V">V. Baran</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berceanu%2C+I">I. Berceanu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colonna%2C+M">M. Colonna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gian%C3%AC%2C+S">S. Gian矛</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grassi%2C+L">L. Grassi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grzeszczuk%2C+A">A. Grzeszczuk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guazzoni%2C+P">P. Guazzoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Han%2C+J">J. Han</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Minniti%2C+T">T. Minniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piasecki%2C+E">E. Piasecki</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pop%2C+A">A. Pop</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a> , et al. (9 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="1209.6461v1-abstract-short" style="display: inline;"> We show new data from the $^{64}$Ni+$^{124}$Sn and $^{58}$Ni+$^{112}$Sn reactions studied in direct kinematics with the CHIMERA detector at INFN-LNS and compared with the reverse kinematics reactions at the same incident beam energy (35 A MeV). Analyzing the data with the method of relative velocity correlations, fragments coming from statistical decay of an excited projectile-like (PLF) or target&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.6461v1-abstract-full').style.display = 'inline'; document.getElementById('1209.6461v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1209.6461v1-abstract-full" style="display: none;"> We show new data from the $^{64}$Ni+$^{124}$Sn and $^{58}$Ni+$^{112}$Sn reactions studied in direct kinematics with the CHIMERA detector at INFN-LNS and compared with the reverse kinematics reactions at the same incident beam energy (35 A MeV). Analyzing the data with the method of relative velocity correlations, fragments coming from statistical decay of an excited projectile-like (PLF) or target-like (TLF) fragments are discriminated from the ones coming from dynamical emission in the early stages of the reaction. By comparing data of the reverse kinematics experiment with a stochastic mean field (SMF) + GEMINI calculations our results show that observables from neck fragmentation mechanism add valuable constraints on the density dependence of symmetry energy. An indication is found for a moderately stiff symmetry energy potential term of EOS. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.6461v1-abstract-full').style.display = 'none'; document.getElementById('1209.6461v1-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 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">Talk given by E. De Filippo 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/1209.5961">arXiv:1209.5961</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1209.5961">pdf</a>, <a href="https://arxiv.org/ps/1209.5961">ps</a>, <a href="https://arxiv.org/format/1209.5961">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/10.1088/1742-6596/420/1/012092">10.1088/1742-6596/420/1/012092 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The ASY-EOS experiment at GSI: investigating the symmetry energy at supra-saturation densities </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</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=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=F%C3%A9vre%2C+A+L">A. Le F茅vre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gannon%2C+S">S. Gannon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ga%C5%A1pari%C4%87%2C+I">I. Ga拧pari膰</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ki%C5%A1%2C+M">M. Ki拧</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kupny%2C+S">S. Kupny</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=Lemmon%2C+R+C">R. C. Lemmon</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=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <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=Santoro%2C+S">S. Santoro</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=Veselsky%2C+M">M. Veselsky</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=Adamczyk%2C+M">M. Adamczyk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Ajlan%2C+A">A. Al-Ajlan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Garawi%2C+M">M. Al-Garawi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Al-Homaidhi%2C+S">S. Al-Homaidhi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aumann%2C+T">T. Aumann</a> , et al. (67 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="1209.5961v1-abstract-short" style="display: inline;"> The elliptic-flow ratio of neutrons with respect to protons in reactions of neutron rich heavy-ions systems at intermediate energies has been proposed as an observable sensitive to the strength of the symmetry term in the nuclear Equation Of State (EOS) at supra-saturation densities. The recent results obtained from the existing FOPI/LAND data for $^{197}$Au+$^{197}$Au collisions at 400 MeV/nucleo&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.5961v1-abstract-full').style.display = 'inline'; document.getElementById('1209.5961v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1209.5961v1-abstract-full" style="display: none;"> The elliptic-flow ratio of neutrons with respect to protons in reactions of neutron rich heavy-ions systems at intermediate energies has been proposed as an observable sensitive to the strength of the symmetry term in the nuclear Equation Of State (EOS) at supra-saturation densities. The recent results obtained from the existing FOPI/LAND data for $^{197}$Au+$^{197}$Au collisions at 400 MeV/nucleon in comparison with the UrQMD model allowed a first estimate of the symmetry term of the EOS but suffer from a considerable statistical uncertainty. In order to obtain an improved data set for Au+Au collisions and to extend the study to other systems, a new experiment was carried out at the GSI laboratory by the ASY-EOS collaboration in May 2011. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1209.5961v1-abstract-full').style.display = 'none'; document.getElementById('1209.5961v1-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> 26 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">Talk given by P. Russotto 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/1206.0697">arXiv:1206.0697</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1206.0697">pdf</a>, <a href="https://arxiv.org/ps/1206.0697">ps</a>, <a href="https://arxiv.org/format/1206.0697">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.86.014610">10.1103/PhysRevC.86.014610 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Correlations between emission timescale of fragments and isospin dynamics in $^{124}$Sn+$^{64}$Ni and $^{112}$Sn+$^{58}$Ni reactions at 35 AMeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baran%2C+V">V. Baran</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berceanu%2C+I">I. Berceanu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bougault%2C+R">R. Bougault</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bruno%2C+M">M. Bruno</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cap%2C+T">T. Cap</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cavallaro%2C+S">S. Cavallaro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjee%2C+M+B">M. B. Chatterjee</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=Colonna%2C+M">M. Colonna</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Agostino%2C+M">M. D&#39;Agostino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dayras%2C+R">R. Dayras</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Toro%2C+M">M. Di Toro</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=Galichet%2C+E">E. Galichet</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=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grzeszczuk%2C+A">A. Grzeszczuk</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="1206.0697v1-abstract-short" style="display: inline;"> We present a new experimental method to correlate the isotopic composition of intermediate mass fragments (IMF) emitted at mid-rapidity in semi-peripheral collisions with the emission timescale: IMFs emitted in the early stage of the reaction show larger values of $&lt;$N/Z$&gt;$ isospin asymmetry, stronger angular anisotropies and reduced odd-even staggering effects in neutron to proton ratio $&lt;$N/Z&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0697v1-abstract-full').style.display = 'inline'; document.getElementById('1206.0697v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1206.0697v1-abstract-full" style="display: none;"> We present a new experimental method to correlate the isotopic composition of intermediate mass fragments (IMF) emitted at mid-rapidity in semi-peripheral collisions with the emission timescale: IMFs emitted in the early stage of the reaction show larger values of $&lt;$N/Z$&gt;$ isospin asymmetry, stronger angular anisotropies and reduced odd-even staggering effects in neutron to proton ratio $&lt;$N/Z$&gt;$ distributions than those produced in sequential statistical emission. All these effects support the concept of isospin &#34;migration&#34;, that is sensitive to the density gradient between participant and quasi-spectator nuclear matter, in the so called neck fragmentation mechanism. By comparing the data to a Stochastic Mean Field (SMF) simulation we show that this method gives valuable constraints on the symmetry energy term of nuclear equation of state at subsaturation densities. An indication emerges for a linear density dependence of the symmetry energy. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0697v1-abstract-full').style.display = 'none'; document.getElementById('1206.0697v1-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, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 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">17 pages, 7 figures; submitted to Physical Rev. C</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1202.0192">arXiv:1202.0192</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1202.0192">pdf</a>, <a href="https://arxiv.org/ps/1202.0192">ps</a>, <a href="https://arxiv.org/format/1202.0192">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.86.011602">10.1103/PhysRevC.86.011602 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Persistence of odd-even staggering in charged fragment yields from the 112Sn+58Ni collision at 35 MeV/nucleon </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Casini%2C+G">G. Casini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piantelli%2C+S">S. Piantelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maurenzig%2C+P+R">P. R. Maurenzig</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Olmi%2C+A">A. Olmi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bardelli%2C+L">L. Bardelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barlini%2C+S">S. Barlini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benelli%2C+M">M. Benelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bini%2C+M">M. Bini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Calviani%2C+M">M. Calviani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Marini%2C+P">P. Marini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mangiarotti%2C+A">A. Mangiarotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pasquali%2C+G">G. Pasquali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Poggi%2C+G">G. Poggi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Stefanini%2C+A+A">A. A. Stefanini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bruno%2C+M">M. Bruno</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Morelli%2C+L">L. Morelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kravchuk%2C+V+L">V. L. Kravchuk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzano%27%2C+G">G. Lanzano&#39;</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="1202.0192v2-abstract-short" style="display: inline;"> Odd-even staggering effects on charge distributions are investigated for fragments produced in semiperipheral and central collisions of 112Sn+58Ni at 35 MeV/nucleon. For fragments with Z&lt;16 one observes a clear overproduction of even charges, which decreases for heavier fragments. In peripheral collisions staggering effects persist up to Z about 40. For light fragments, staggering appears to be su&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1202.0192v2-abstract-full').style.display = 'inline'; document.getElementById('1202.0192v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1202.0192v2-abstract-full" style="display: none;"> Odd-even staggering effects on charge distributions are investigated for fragments produced in semiperipheral and central collisions of 112Sn+58Ni at 35 MeV/nucleon. For fragments with Z&lt;16 one observes a clear overproduction of even charges, which decreases for heavier fragments. In peripheral collisions staggering effects persist up to Z about 40. For light fragments, staggering appears to be substantially independent of the centrality of the collisions, suggesting that it is mainly related to the last few steps in the decay of hot nuclei. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1202.0192v2-abstract-full').style.display = 'none'; document.getElementById('1202.0192v2-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> 9 July, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 1 February, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 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">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. C 86, 011602 (2012) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1110.1617">arXiv:1110.1617</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1110.1617">pdf</a>, <a href="https://arxiv.org/ps/1110.1617">ps</a>, <a href="https://arxiv.org/format/1110.1617">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.2011.10.008">10.1016/j.physletb.2011.10.008 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Evidence for $伪$-particle condensation in nuclei from the Hoyle state deexcitation </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Raduta%2C+A+R">Ad. R. Raduta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</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=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alba%2C+R">R. Alba</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjee%2C+M">M. Chatterjee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzano%2C+G">G. Lanzano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a> , et al. (1 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="1110.1617v1-abstract-short" style="display: inline;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}$Ca+$^{12}$C at 25 MeV/nucleon was used to produce excited states candidates to $伪$-particle condensation. Complete kinematic characterization of individual decay events, made possible by a high-granularity 4$蟺$ charged particle multi-detector, reveals that 7.5$\pm$4.0% of the particle decays of the Hoyle state correspond to di&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1110.1617v1-abstract-full').style.display = 'inline'; document.getElementById('1110.1617v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1110.1617v1-abstract-full" style="display: none;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}$Ca+$^{12}$C at 25 MeV/nucleon was used to produce excited states candidates to $伪$-particle condensation. Complete kinematic characterization of individual decay events, made possible by a high-granularity 4$蟺$ charged particle multi-detector, reveals that 7.5$\pm$4.0% of the particle decays of the Hoyle state correspond to direct decays in three equal-energy $伪$-particles. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1110.1617v1-abstract-full').style.display = 'none'; document.getElementById('1110.1617v1-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 October, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">Phys. Lett. B, in press</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Lett. B705, 65-70 (2011) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1009.1669">arXiv:1009.1669</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1009.1669">pdf</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.82.051603">10.1103/PhysRevC.82.051603 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isospin Diffusion and Equilibration for Sn+Sn collisions at E/A=35 MeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Sun%2C+Z+Y">Z. Y. Sun</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tsang%2C+M+B">M. B. Tsang</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lynch%2C+W+G">W. G. Lynch</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Verde%2C+G">G. Verde</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andronenko%2C+L">L. Andronenko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andronenko%2C+M">M. Andronenko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterje%2C+M">M. Chatterje</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danielewicz%2C+P">P. Danielewicz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dinh%2C+P">P. Dinh</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galichet%2C+E">E. Galichet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hua%2C+H">H. Hua</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Liu%2C+H">H. Liu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lu%2C+F">F. Lu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lukyanov%2C+S">S. Lukyanov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Piantelli%2C+S">S. Piantelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</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="1009.1669v3-abstract-short" style="display: inline;"> Equilibration and equilibration rates have been measured by colliding Sn nuclei with different isospin asymmetries at beam energies of E/A=35 MeV. Using the yields of mirror nuclei of 7Li and 7Be, we have studied the diffusion of isospin asymmetry by combining data from asymmetric 112Sn+124Sn and 124Sn+112Sn collisions with that from symmetric 112Sn+112Sn and 124Sn+124Sn collisions. We use these m&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1009.1669v3-abstract-full').style.display = 'inline'; document.getElementById('1009.1669v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1009.1669v3-abstract-full" style="display: none;"> Equilibration and equilibration rates have been measured by colliding Sn nuclei with different isospin asymmetries at beam energies of E/A=35 MeV. Using the yields of mirror nuclei of 7Li and 7Be, we have studied the diffusion of isospin asymmetry by combining data from asymmetric 112Sn+124Sn and 124Sn+112Sn collisions with that from symmetric 112Sn+112Sn and 124Sn+124Sn collisions. We use these measurements to probe isospin equilibration in central collisions where nucleon-nucleon collisions are strongly blocked by the Pauli exclusion principal. The results are consistent with transport theoretical calculations that predict a degree of transparency in these collisions, but inconsistent with the emission of intermediate mass fragments by a single chemically equilibrated source. Comparisons with ImQMD calculations are consistent with results obtained at higher incident energies that provide constraints on the density dependence of the symmetry energy. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1009.1669v3-abstract-full').style.display = 'none'; document.getElementById('1009.1669v3-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> 12 October, 2010; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 8 September, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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">13 pages, 3 figures, submitted to PRC Rapid Communications</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.C82:051603,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1009.1267">arXiv:1009.1267</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1009.1267">pdf</a>, <a href="https://arxiv.org/ps/1009.1267">ps</a>, <a href="https://arxiv.org/format/1009.1267">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/10.1142/S0218301311018939">10.1142/S0218301311018939 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Production of $伪$-particle condensate states in heavy-ion collisions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Raduta%2C+A+R">Ad. R. Raduta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</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=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alba%2C+R">R. Alba</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjee%2C+M">M. Chatterjee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzano%2C+G">G. Lanzano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a> , et al. (1 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="1009.1267v1-abstract-short" style="display: inline;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}Ca$ + $^{12}C$ at 25 MeV/nucleon was used to produce excited states candidates to $伪$-particle condensation. The experiment was performed at LNS-Catania using the CHIMERA multidetector. Accepting the emission simultaneity and equality among the $伪$-particle kinetic energies as experimental criteria for deciding in favor of the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1009.1267v1-abstract-full').style.display = 'inline'; document.getElementById('1009.1267v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1009.1267v1-abstract-full" style="display: none;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}Ca$ + $^{12}C$ at 25 MeV/nucleon was used to produce excited states candidates to $伪$-particle condensation. The experiment was performed at LNS-Catania using the CHIMERA multidetector. Accepting the emission simultaneity and equality among the $伪$-particle kinetic energies as experimental criteria for deciding in favor of the condensate nature of an excited state, we analyze the $0_2^+$ and $2_2^+$ states of $^{12}$C and the $0_6^+$ state of $^{16}$O. A sub-class of events corresponding to the direct 3-$伪$ decay of the Hoyle state is isolated. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1009.1267v1-abstract-full').style.display = 'none'; document.getElementById('1009.1267v1-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 September, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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">contribution to the 2nd Workshop on &#34;State of the Art in Nuclear Cluster Physics&#34; (SOTANCP2), Universite Libre de Bruxelles (Belgium), May 25-28, 2010, to be published in the 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.E20:902-905,2011 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1004.3234">arXiv:1004.3234</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1004.3234">pdf</a>, <a href="https://arxiv.org/ps/1004.3234">ps</a>, <a href="https://arxiv.org/format/1004.3234">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"> Alpha-particle condensation in excited 12C </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Raduta%2C+A+R">Ad. R. Raduta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borderie%2C+B">B. Borderie</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</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=Rivet%2C+M+F">M. F. Rivet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alba%2C+R">R. Alba</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjee%2C+M">M. Chatterjee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Guinet%2C+D">D. Guinet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lautesse%2C+P">P. Lautesse</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzano%2C+G">G. Lanzano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez%2C+O">O. Lopez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Porto%2C+F">F. Porto</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rizzo%2C+F">F. Rizzo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Russotto%2C+P">P. Russotto</a> , et al. (1 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="1004.3234v2-abstract-short" style="display: inline;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}Ca$+$^{12}C$ at 25 MeV/nucleon was used to produce excited states candidates to $伪$-particle condensation. The methodology relies on high granularity 4$蟺$ detection coupled to correlation function techniques. Under the assumption that the equality among the kinetic energies of the emitted $伪$-particles and the emission simultan&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.3234v2-abstract-full').style.display = 'inline'; document.getElementById('1004.3234v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1004.3234v2-abstract-full" style="display: none;"> The fragmentation of quasi-projectiles from the nuclear reaction $^{40}Ca$+$^{12}C$ at 25 MeV/nucleon was used to produce excited states candidates to $伪$-particle condensation. The methodology relies on high granularity 4$蟺$ detection coupled to correlation function techniques. Under the assumption that the equality among the kinetic energies of the emitted $伪$-particles and the emission simultaneity constitutes a reliable fingerprint of $伪$ condensation, we identify several tens of events corresponding to the deexcitation of the Hoyle state of $^{12}$C which fulfill the condition. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.3234v2-abstract-full').style.display = 'none'; document.getElementById('1004.3234v2-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> 22 July, 2010; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 19 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">5 pages, 3 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/0809.1196">arXiv:0809.1196</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/0809.1196">pdf</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.102.112701">10.1103/PhysRevLett.102.112701 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Isospin Dependence of Incomplete Fusion Reactions at 25 Mev/a </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Amorini%2C+F">F. Amorini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardella%2C+G">G. Cardella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+G">G. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Papa%2C+M">M. Papa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Agodi%2C+C">C. Agodi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alba%2C+R">R. Alba</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berceanu%2C+I">I. Berceanu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cavallaro%2C+S">S. Cavallaro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chatterjee%2C+M+B">M. B. Chatterjee</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Coniglione%2C+R">R. Coniglione</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Pietro%2C+A">A. Di Pietro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+E">E. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grassi%2C+L">L. Grassi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grzeszczuk%2C+A">A. Grzeszczuk</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Figuera%2C+P">P. Figuera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=La+Guidara%2C+E">E. La Guidara</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzalone%2C+G">G. Lanzalone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Neindre%2C+N+L">N. Le Neindre</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lombardo%2C+I">I. Lombardo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Maiolino%2C+C">C. Maiolino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirrone%2C+S">S. Pirrone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</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="0809.1196v1-abstract-short" style="display: inline;"> 40Ca+40,48Ca,46Ti reactions at 25 MeV/A have been studied using the 4p CHIMERA detector. An isospin effect on the competition between incomplete fusion and dissipative binary reaction mechanisms has been observed. The probability of producing a compound system is observed to be lower in the case of N=Z colliding systems as compared to the case of reactions induced on the more neutron rich 48Ca t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0809.1196v1-abstract-full').style.display = 'inline'; document.getElementById('0809.1196v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0809.1196v1-abstract-full" style="display: none;"> 40Ca+40,48Ca,46Ti reactions at 25 MeV/A have been studied using the 4p CHIMERA detector. An isospin effect on the competition between incomplete fusion and dissipative binary reaction mechanisms has been observed. The probability of producing a compound system is observed to be lower in the case of N=Z colliding systems as compared to the case of reactions induced on the more neutron rich 48Ca target. Predictions based on CoMD-II calculations show that the competition between fusion-like and dissipative reactions, for the selected centrality, can strongly constraint the parameterization of symmetry energy and its density dependence in the nuclear equation of state. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0809.1196v1-abstract-full').style.display = 'none'; document.getElementById('0809.1196v1-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> 8 September, 2008; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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">4 pages 3 figures submitted to phys.rew.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.102:112701,2009 </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/0412038">arXiv:nucl-ex/0412038</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/0412038">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/0412038">ps</a>, <a href="https://arxiv.org/format/nucl-ex/0412038">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.2005.11.019">10.1016/j.nuclphysa.2005.11.019 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Correlation functions and emission time sequence of light charged particles from projectile-like fragment source in E/A = 44 and 77 MeV 40Ar + 27Al collisions </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Ghetti%2C+R">R. Ghetti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Helgesson%2C+J">J. Helgesson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lanzano%27%2C+G">G. Lanzano&#39;</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Filippo%2C+E">E. De Filippo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Geraci%2C+M">M. Geraci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aiello%2C+S">S. Aiello</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cavallaro%2C+S">S. Cavallaro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagano%2C+A">A. Pagano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Politi%2C+G">G. Politi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Charvet%2C+J+L">J. L. Charvet</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dayras%2C+R">R. Dayras</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pollacco%2C+E">E. Pollacco</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=Beck%2C+C">C. Beck</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Mahboub%2C+D">D. Mahboub</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nouicer%2C+R">R. Nouicer</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/0412038v1-abstract-short" style="display: inline;"> Two-particle correlation functions, involving protons, deuterons, tritons, and alpha-particles, have been measured at very forward angles (0.7 deg &lt; theta_lab &lt; 7 deg), in order to study projectile-like fragment (PLF) emission in E/A = 44 and 77 MeV 40Ar + 27Al collisions. Peaks, originating from resonance decays, are larger at E/A = 44 than at 77 MeV. This reflects the larger relative importanc&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0412038v1-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/0412038v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/0412038v1-abstract-full" style="display: none;"> Two-particle correlation functions, involving protons, deuterons, tritons, and alpha-particles, have been measured at very forward angles (0.7 deg &lt; theta_lab &lt; 7 deg), in order to study projectile-like fragment (PLF) emission in E/A = 44 and 77 MeV 40Ar + 27Al collisions. Peaks, originating from resonance decays, are larger at E/A = 44 than at 77 MeV. This reflects the larger relative importance of independently emitted light particles, as compared to two-particle decay from unstable fragments, at the higher beam energy. The time sequence of the light charged particles, emitted from the PLF, has been deduced from particle-velocity-gated correlation functions (discarding the contribution from resonance decays). Alpha-particles are found to have an average emission time shorter than protons but longer than tritons and deuterons. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0412038v1-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/0412038v1-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 December, 2004; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2004. </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">18 pages, 5 figures, submitted to Nuclear Physics 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/0307021">arXiv:nucl-ex/0307021</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/nucl-ex/0307021">pdf</a>, <a href="https://arxiv.org/ps/nucl-ex/0307021">ps</a>, <a href="https://arxiv.org/format/nucl-ex/0307021">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.2003.09.047">10.1016/j.nima.2003.09.047 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Elements Discrimination in the Study of Super-Heavy Elements using an Ionization Chamber </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=FULIS+Collaboration"> FULIS Collaboration</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=Sosin%2C+Z">Z. Sosin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Peter%2C+J">J. Peter</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lojek%2C+K">K. Lojek</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alamanos%2C+N">N. Alamanos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amar%2C+N">N. Amar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Anne%2C+R">R. Anne</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Angelique%2C+J+C">J. C. Angelique</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Auger%2C+G">G. Auger</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dayras%2C+R">R. Dayras</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Drouart%2C+A">A. Drouart</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fontbonne%2C+J+M">J. M. Fontbonne</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gillibert%2C+A">A. Gillibert</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Grevy%2C+S">S. Grevy</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hanappe%2C+F">F. Hanappe</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hannachi%2C+F">F. Hannachi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Hue%2C+R">R. Hue</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Khouaja%2C+A">A. Khouaja</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Legou%2C+T">T. Legou</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lopez-Martens%2C+A">A. Lopez-Martens</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Lienard%2C+E">E. Lienard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Manduci%2C+L">L. Manduci</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=Politi%2C+G">G. Politi</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/0307021v1-abstract-short" style="display: inline;"> Dedicated ionization chamber was built and installed to measure the energy loss of very heavy nuclei at 2.7 MeV/u produced in fusion reactions in inverse kinematics (beam of 208Pb). After going through the ionization chamber, products of reactions on 12C, 18O targets are implanted in a Si detector. Their identification through their alpha decay chain is ambiguous when their half-life is short. A&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0307021v1-abstract-full').style.display = 'inline'; document.getElementById('nucl-ex/0307021v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="nucl-ex/0307021v1-abstract-full" style="display: none;"> Dedicated ionization chamber was built and installed to measure the energy loss of very heavy nuclei at 2.7 MeV/u produced in fusion reactions in inverse kinematics (beam of 208Pb). After going through the ionization chamber, products of reactions on 12C, 18O targets are implanted in a Si detector. Their identification through their alpha decay chain is ambiguous when their half-life is short. After calibration with Pb and Th nuclei, the ionization chamber signal allowed us to resolve these ambiguities. In the search for rare super-heavy nuclei produced in fusion reactions in inverse or symmetric kinematics, such a chamber will provide direct information on the nuclear charge of each implanted nucleus. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('nucl-ex/0307021v1-abstract-full').style.display = 'none'; document.getElementById('nucl-ex/0307021v1-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 July, 2003; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">submitted to NIMA, 10 pages+4 figures, Latex, uses elsart.cls and grahpicx</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl.Instrum.Meth. A517 (2004) 364-371 </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 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg> <a href="https://info.arxiv.org/help/contact.html"> Contact</a> </li> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>subscribe to arXiv mailings</title><desc>Click here to subscribe</desc><path d="M476 3.2L12.5 270.6c-18.1 10.4-15.8 35.6 2.2 43.2L121 358.4l287.3-253.2c5.5-4.9 13.3 2.6 8.6 8.3L176 407v80.5c0 23.6 28.5 32.9 42.5 15.8L282 426l124.6 52.2c14.2 6 30.4-2.9 33-18.2l72-432C515 7.8 493.3-6.8 476 3.2z"/></svg> <a href="https://info.arxiv.org/help/subscribe"> Subscribe</a> </li> </ul> </div> </div> </div> <!-- end MetaColumn 1 --> <!-- MetaColumn 2 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/license/index.html">Copyright</a></li> <li><a href="https://info.arxiv.org/help/policies/privacy_policy.html">Privacy Policy</a></li> </ul> </div> <div class="column sorry-app-links"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/web_accessibility.html">Web Accessibility Assistance</a></li> <li> <p class="help"> <a class="a11y-main-link" href="https://status.arxiv.org" target="_blank">arXiv Operational Status <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 256 512" class="icon filter-dark_grey" role="presentation"><path d="M224.3 273l-136 136c-9.4 9.4-24.6 9.4-33.9 0l-22.6-22.6c-9.4-9.4-9.4-24.6 0-33.9l96.4-96.4-96.4-96.4c-9.4-9.4-9.4-24.6 0-33.9L54.3 103c9.4-9.4 24.6-9.4 33.9 0l136 136c9.5 9.4 9.5 24.6.1 34z"/></svg></a><br> Get status notifications via <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/email/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><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 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg>email</a> or <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/slack/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 448 512" class="icon filter-black" role="presentation"><path d="M94.12 315.1c0 25.9-21.16 47.06-47.06 47.06S0 341 0 315.1c0-25.9 21.16-47.06 47.06-47.06h47.06v47.06zm23.72 0c0-25.9 21.16-47.06 47.06-47.06s47.06 21.16 47.06 47.06v117.84c0 25.9-21.16 47.06-47.06 47.06s-47.06-21.16-47.06-47.06V315.1zm47.06-188.98c-25.9 0-47.06-21.16-47.06-47.06S139 32 164.9 32s47.06 21.16 47.06 47.06v47.06H164.9zm0 23.72c25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06H47.06C21.16 243.96 0 222.8 0 196.9s21.16-47.06 47.06-47.06H164.9zm188.98 47.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06h-47.06V196.9zm-23.72 0c0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06V79.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06V196.9zM283.1 385.88c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06v-47.06h47.06zm0-23.72c-25.9 0-47.06-21.16-47.06-47.06 0-25.9 21.16-47.06 47.06-47.06h117.84c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06H283.1z"/></svg>slack</a> </p> </li> </ul> </div> </div> </div> <!-- end MetaColumn 2 --> </div> </footer> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/member_acknowledgement.js"></script> </body> </html>

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