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and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-ph</span> </div> </div> <p class="title is-5 mathjax"> First application of superconducting transition-edge-sensor microcalorimeters to hadronic-atom x-ray spectroscopy </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Okada%2C+S">S. Okada</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+D+A">D. A. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Curceanu%2C+C">C. Curceanu</a>, <a href="/search/physics?searchtype=author&amp;query=Doriese%2C+W+B">W. B. Doriese</a>, <a href="/search/physics?searchtype=author&amp;query=Fowler%2C+J+W">J. W. Fowler</a>, <a href="/search/physics?searchtype=author&amp;query=Gard%2C+J">J. Gard</a>, <a href="/search/physics?searchtype=author&amp;query=Gustafsson%2C+F+P">F. P. Gustafsson</a>, <a href="/search/physics?searchtype=author&amp;query=Hashimoto%2C+T">T. Hashimoto</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">R. S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hirenzaki%2C+S">S. Hirenzaki</a>, <a href="/search/physics?searchtype=author&amp;query=Hays-Wehle%2C+J+P">J. P. Hays-Wehle</a>, <a href="/search/physics?searchtype=author&amp;query=Hilton%2C+G+C">G. C. Hilton</a>, <a href="/search/physics?searchtype=author&amp;query=Ikeno%2C+N">N. Ikeno</a>, <a href="/search/physics?searchtype=author&amp;query=Iliescu%2C+M">M. Iliescu</a>, <a href="/search/physics?searchtype=author&amp;query=Ishimoto%2C+S">S. Ishimoto</a>, <a href="/search/physics?searchtype=author&amp;query=Itahashi%2C+K">K. Itahashi</a>, <a href="/search/physics?searchtype=author&amp;query=Iwasaki%2C+M">M. Iwasaki</a>, <a href="/search/physics?searchtype=author&amp;query=Koike%2C+T">T. Koike</a>, <a href="/search/physics?searchtype=author&amp;query=Kuwabara%2C+K">K. Kuwabara</a>, <a href="/search/physics?searchtype=author&amp;query=Ma%2C+Y">Y. Ma</a>, <a href="/search/physics?searchtype=author&amp;query=Marton%2C+J">J. Marton</a>, <a href="/search/physics?searchtype=author&amp;query=Noda%2C+H">H. Noda</a>, <a href="/search/physics?searchtype=author&amp;query=O%27Neil%2C+G+C">G. C. O&#39;Neil</a>, <a href="/search/physics?searchtype=author&amp;query=Outa%2C+H">H. Outa</a>, <a href="/search/physics?searchtype=author&amp;query=Reintsema%2C+C+D">C. D. Reintsema</a> , et al. (13 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1608.05436v1-abstract-short" style="display: inline;"> High-resolution pionic-atom x-ray spectroscopy was performed with an x-ray spectrometer based on a 240-pixel array of superconducting transition-edge-sensor (TES) microcalorimeters at the piM1 beam line of the Paul Scherrer Institute. X-rays emitted by pionic carbon via the 4f-&gt;3d transition and the parallel 4d-&gt;3p transition were observed with a full-width-at-half-maximum energy resolution of 6.8&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1608.05436v1-abstract-full').style.display = 'inline'; document.getElementById('1608.05436v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1608.05436v1-abstract-full" style="display: none;"> High-resolution pionic-atom x-ray spectroscopy was performed with an x-ray spectrometer based on a 240-pixel array of superconducting transition-edge-sensor (TES) microcalorimeters at the piM1 beam line of the Paul Scherrer Institute. X-rays emitted by pionic carbon via the 4f-&gt;3d transition and the parallel 4d-&gt;3p transition were observed with a full-width-at-half-maximum energy resolution of 6.8 eV at 6.4 keV. Measured x-ray energies are consistent with calculated electromagnetic values which considered the strong-interaction effect assessed via the Seki-Masutani potential for the 3p energy level, and favor the electronic population of two filled 1s electrons in the K-shell. Absolute energy calibration with an uncertainty of 0.1 eV was demonstrated under a high-rate hadron beam condition of 1.45 MHz. This is the first application of a TES spectrometer to hadronic-atom x-ray spectroscopy and is an important milestone towards next-generation high-resolution kaonic-atom x-ray spectroscopy. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1608.05436v1-abstract-full').style.display = 'none'; document.getElementById('1608.05436v1-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 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">11 pages, 3 figures, submitted to PTEP</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1601.03293">arXiv:1601.03293</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1601.03293">pdf</a>, <a href="https://arxiv.org/ps/1601.03293">ps</a>, <a href="https://arxiv.org/format/1601.03293">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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/10.1007/s10909-016-1491-2">10.1007/s10909-016-1491-2 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Absolute Energy Calibration of X-ray TESs with 0.04 eV Uncertainty at 6.4 keV in a Hadron-Beam Environment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Tatsuno%2C+H">H. Tatsuno</a>, <a href="/search/physics?searchtype=author&amp;query=Doriese%2C+W+B">W. B. Doriese</a>, <a href="/search/physics?searchtype=author&amp;query=Bennett%2C+D+A">D. A. Bennett</a>, <a href="/search/physics?searchtype=author&amp;query=Curceanu%2C+C">C. Curceanu</a>, <a href="/search/physics?searchtype=author&amp;query=Fowler%2C+J+W">J. W. Fowler</a>, <a href="/search/physics?searchtype=author&amp;query=Gard%2C+J">J. Gard</a>, <a href="/search/physics?searchtype=author&amp;query=Gustafsson%2C+F+P">F. P. Gustafsson</a>, <a href="/search/physics?searchtype=author&amp;query=Hashimoto%2C+T">T. Hashimoto</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">R. S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hays-Wehle%2C+J+P">J. P. Hays-Wehle</a>, <a href="/search/physics?searchtype=author&amp;query=Hilton%2C+G+C">G. C. Hilton</a>, <a href="/search/physics?searchtype=author&amp;query=Iliescu%2C+M">M. Iliescu</a>, <a href="/search/physics?searchtype=author&amp;query=Ishimoto%2C+S">S. Ishimoto</a>, <a href="/search/physics?searchtype=author&amp;query=Itahashi%2C+K">K. Itahashi</a>, <a href="/search/physics?searchtype=author&amp;query=Iwasaki%2C+M">M. Iwasaki</a>, <a href="/search/physics?searchtype=author&amp;query=Kuwabara%2C+K">K. Kuwabara</a>, <a href="/search/physics?searchtype=author&amp;query=Ma%2C+Y">Y. Ma</a>, <a href="/search/physics?searchtype=author&amp;query=Marton%2C+J">J. Marton</a>, <a href="/search/physics?searchtype=author&amp;query=Noda%2C+H">H. Noda</a>, <a href="/search/physics?searchtype=author&amp;query=O%27Neil%2C+G+C">G. C. O&#39;Neil</a>, <a href="/search/physics?searchtype=author&amp;query=Okada%2C+S">S. Okada</a>, <a href="/search/physics?searchtype=author&amp;query=Outa%2C+H">H. Outa</a>, <a href="/search/physics?searchtype=author&amp;query=Reintsema%2C+C+D">C. D. Reintsema</a>, <a href="/search/physics?searchtype=author&amp;query=Sato%2C+M">M. Sato</a>, <a href="/search/physics?searchtype=author&amp;query=Schmidt%2C+D+R">D. R. Schmidt</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="1601.03293v1-abstract-short" style="display: inline;"> A performance evaluation of superconducting transition-edge sensors (TESs) in the environment of a pion beam line at a particle accelerator is presented. Averaged across the 209 functioning sensors in the array, the achieved energy resolution is 5.2 eV FWHM at Co $K_伪$ (6.9 keV) when the pion beam is off and 7.3 eV at a beam rate of 1.45 MHz. Absolute energy uncertainty of $\pm$0.04 eV is demonstr&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.03293v1-abstract-full').style.display = 'inline'; document.getElementById('1601.03293v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1601.03293v1-abstract-full" style="display: none;"> A performance evaluation of superconducting transition-edge sensors (TESs) in the environment of a pion beam line at a particle accelerator is presented. Averaged across the 209 functioning sensors in the array, the achieved energy resolution is 5.2 eV FWHM at Co $K_伪$ (6.9 keV) when the pion beam is off and 7.3 eV at a beam rate of 1.45 MHz. Absolute energy uncertainty of $\pm$0.04 eV is demonstrated for Fe $K_伪$ (6.4 keV) with in-situ energy calibration obtained from other nearby known x-ray lines. To achieve this small uncertainty, it is essential to consider the non-Gaussian energy response of the TESs and thermal cross-talk pile-up effects due to charged-particle hits in the silicon substrate of the TES array. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.03293v1-abstract-full').style.display = 'none'; document.getElementById('1601.03293v1-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> 13 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">Accepted for publication in J. Low Temperature Physics, special issue for the proceedings of the Low Temperature Detectors 16 conference</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1501.05548">arXiv:1501.05548</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1501.05548">pdf</a>, <a href="https://arxiv.org/format/1501.05548">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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/10.5506/APhysPolB.46.101">10.5506/APhysPolB.46.101 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of the strong interaction induced shift and width of the 1s state of kaonic deuterium at J-PARC </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Zmeskal%2C+J">J. Zmeskal</a>, <a href="/search/physics?searchtype=author&amp;query=Sato%2C+M">M. Sato</a>, <a href="/search/physics?searchtype=author&amp;query=Ajimura%2C+S">S. Ajimura</a>, <a href="/search/physics?searchtype=author&amp;query=Bazzi%2C+M">M. Bazzi</a>, <a href="/search/physics?searchtype=author&amp;query=Beer%2C+G">G. Beer</a>, <a href="/search/physics?searchtype=author&amp;query=Berucci%2C+C">C. Berucci</a>, <a href="/search/physics?searchtype=author&amp;query=Bhang%2C+H">H. Bhang</a>, <a href="/search/physics?searchtype=author&amp;query=Bosnar%2C+D">D. Bosnar</a>, <a href="/search/physics?searchtype=author&amp;query=Bragadireanu%2C+M">M. Bragadireanu</a>, <a href="/search/physics?searchtype=author&amp;query=Buehler%2C+P">P. Buehler</a>, <a href="/search/physics?searchtype=author&amp;query=Busso%2C+L">L. Busso</a>, <a href="/search/physics?searchtype=author&amp;query=Cargnelli%2C+M">M. Cargnelli</a>, <a href="/search/physics?searchtype=author&amp;query=Choi%2C+S">S. Choi</a>, <a href="/search/physics?searchtype=author&amp;query=Clozza%2C+A">A. Clozza</a>, <a href="/search/physics?searchtype=author&amp;query=Curceanu%2C+C">C. Curceanu</a>, <a href="/search/physics?searchtype=author&amp;query=D%27uffizi%2C+A">A. D&#39;uffizi</a>, <a href="/search/physics?searchtype=author&amp;query=Enomoto%2C+S">S. Enomoto</a>, <a href="/search/physics?searchtype=author&amp;query=Fabbietti%2C+L">L. Fabbietti</a>, <a href="/search/physics?searchtype=author&amp;query=Faso%2C+D">D. Faso</a>, <a href="/search/physics?searchtype=author&amp;query=Fiorini%2C+C">C. Fiorini</a>, <a href="/search/physics?searchtype=author&amp;query=Fujioka%2C+H">H. Fujioka</a>, <a href="/search/physics?searchtype=author&amp;query=Ghio%2C+F">F. Ghio</a>, <a href="/search/physics?searchtype=author&amp;query=Golser%2C+R">R. Golser</a>, <a href="/search/physics?searchtype=author&amp;query=Guaraldo%2C+C">C. Guaraldo</a>, <a href="/search/physics?searchtype=author&amp;query=Hashimoto%2C+T">T. Hashimoto</a> , et al. (52 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="1501.05548v1-abstract-short" style="display: inline;"> The antikaon-nucleon interaction close to threshold provides crucial information on the interplay between spontaneous and explicit chiral symmetry breaking in low-energy QCD. In this context the importance of kaonic deuterium X-ray spectroscopy has been well recognized, but no experimental results have yet been obtained due to the difficulty of the measurement. We propose to measure the shift and&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.05548v1-abstract-full').style.display = 'inline'; document.getElementById('1501.05548v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1501.05548v1-abstract-full" style="display: none;"> The antikaon-nucleon interaction close to threshold provides crucial information on the interplay between spontaneous and explicit chiral symmetry breaking in low-energy QCD. In this context the importance of kaonic deuterium X-ray spectroscopy has been well recognized, but no experimental results have yet been obtained due to the difficulty of the measurement. We propose to measure the shift and width of the kaonic deuterium 1s state with an accuracy of 60 eV and 140 eV respectively at J-PARC. These results together with the kaonic hydrogen data (KpX at KEK, DEAR and SIDDHARTA at DAFNE) will then permit the determination of values of both the isospin I=0 and I=1 antikaon-nucleon scattering lengths and will provide the most stringent constraints on the antikaon-nucleon interaction, promising a breakthrough. Refined Monte Carlo studies were performed, including the investigation of background suppression factors for the described setup. These studies have demonstrated the feasibility of determining the shift and width of the kaonic deuterium atom 1s state with the desired accuracy of 60 eV and 140 eV. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.05548v1-abstract-full').style.display = 'none'; document.getElementById('1501.05548v1-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 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">12 pages, 9 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/1206.0077">arXiv:1206.0077</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1206.0077">pdf</a>, <a href="https://arxiv.org/ps/1206.0077">ps</a>, <a href="https://arxiv.org/format/1206.0077">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1093/ptep/pts039">10.1093/ptep/pts039 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The K1.8BR spectrometer system at J-PARC </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Agari%2C+K">Keizo Agari</a>, <a href="/search/physics?searchtype=author&amp;query=Ajimura%2C+S">Shuhei Ajimura</a>, <a href="/search/physics?searchtype=author&amp;query=Beer%2C+G">George Beer</a>, <a href="/search/physics?searchtype=author&amp;query=Bhang%2C+H">Hyoungchan Bhang</a>, <a href="/search/physics?searchtype=author&amp;query=Bragadireanu%2C+M">Mario Bragadireanu</a>, <a href="/search/physics?searchtype=author&amp;query=Buehler%2C+P">Paul Buehler</a>, <a href="/search/physics?searchtype=author&amp;query=Busso%2C+L">Luigi Busso</a>, <a href="/search/physics?searchtype=author&amp;query=Cargnelli%2C+M">Michael Cargnelli</a>, <a href="/search/physics?searchtype=author&amp;query=Choi%2C+S">Seonho Choi</a>, <a href="/search/physics?searchtype=author&amp;query=Curceanu%2C+C">Catalina Curceanu</a>, <a href="/search/physics?searchtype=author&amp;query=Enomoto%2C+S">Shun Enomoto</a>, <a href="/search/physics?searchtype=author&amp;query=Faso%2C+D">Diego Faso</a>, <a href="/search/physics?searchtype=author&amp;query=Fujioka%2C+H">Hiroyuki Fujioka</a>, <a href="/search/physics?searchtype=author&amp;query=Fujiwara%2C+Y">Yuya Fujiwara</a>, <a href="/search/physics?searchtype=author&amp;query=Fukuda%2C+T">Tomokazu Fukuda</a>, <a href="/search/physics?searchtype=author&amp;query=Guaraldo%2C+C">Carlo Guaraldo</a>, <a href="/search/physics?searchtype=author&amp;query=Hashimoto%2C+T">Tadashi Hashimoto</a>, <a href="/search/physics?searchtype=author&amp;query=Hayano%2C+R+S">Ryugo S. Hayano</a>, <a href="/search/physics?searchtype=author&amp;query=Hiraiwa%2C+T">Toshihiko Hiraiwa</a>, <a href="/search/physics?searchtype=author&amp;query=Hirose%2C+E">Erina Hirose</a>, <a href="/search/physics?searchtype=author&amp;query=Ieiri%2C+M">Masaharu Ieiri</a>, <a href="/search/physics?searchtype=author&amp;query=Iio%2C+M">Masami Iio</a>, <a href="/search/physics?searchtype=author&amp;query=Iliescu%2C+M">Mihai Iliescu</a>, <a href="/search/physics?searchtype=author&amp;query=Inoue%2C+K">Kentaro Inoue</a>, <a href="/search/physics?searchtype=author&amp;query=Ishiguro%2C+Y">Yosuke Ishiguro</a> , et al. (60 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="1206.0077v2-abstract-short" style="display: inline;"> A new spectrometer system was designed and constructed at the secondary beam line K1.8BR in the hadron hall of J-PARC to investigate $\bar K N$ interactions and $\bar K$-nuclear bound systems. The spectrometer consists of a high precision beam line spectrometer, a liquid $^3$He/$^4$He/D$_2$ target system, a Cylindrical Detector System that surrounds the target to detect the decay particles from th&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0077v2-abstract-full').style.display = 'inline'; document.getElementById('1206.0077v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1206.0077v2-abstract-full" style="display: none;"> A new spectrometer system was designed and constructed at the secondary beam line K1.8BR in the hadron hall of J-PARC to investigate $\bar K N$ interactions and $\bar K$-nuclear bound systems. The spectrometer consists of a high precision beam line spectrometer, a liquid $^3$He/$^4$He/D$_2$ target system, a Cylindrical Detector System that surrounds the target to detect the decay particles from the target region, and a neutron time-of-flight counter array located $\sim$15 m downstream from the target position. Details of the design, construction, and performance of the detector components are described. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0077v2-abstract-full').style.display = 'none'; document.getElementById('1206.0077v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 November, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 1 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">33 pages, 25 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Prog. Theor. Exp. Phys. (2012) 02B011 </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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