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Title: Crystalline chiral condensates as a component of compact stars

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; ; ;
Publication Date:
Sponsoring Org.:
USDOE
OSTI Identifier:
1225678
Grant/Contract Number:  
SC0002179
Resource Type:
Publisher's Accepted Manuscript
Journal Name:
Physical Review D
Additional Journal Information:
Journal Name: Physical Review D Journal Volume: 92 Journal Issue: 10; Journal ID: ISSN 1550-7998
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English

Citation Formats

Carignano, S., Ferrer, E. J., de la Incera, V., and Paulucci, L. Crystalline chiral condensates as a component of compact stars. United States: N. p., 2015. Web. doi:10.1103/PhysRevD.92.105018.
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Carignano, S., Ferrer, E. J., de la Incera, V., & Paulucci, L. Crystalline chiral condensates as a component of compact stars. United States. https://doi.org/10.1103/PhysRevD.92.105018
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Carignano, S., Ferrer, E. J., de la Incera, V., and Paulucci, L. Tue . "Crystalline chiral condensates as a component of compact stars". United States. https://doi.org/10.1103/PhysRevD.92.105018.
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@article{osti_1225678,
title = {Crystalline chiral condensates as a component of compact stars},
author = {Carignano, S. and Ferrer, E. J. and de la Incera, V. and Paulucci, L.},
abstractNote = {},
doi = {10.1103/PhysRevD.92.105018},
journal = {Physical Review D},
number = 10,
volume = 92,
place = {United States},
year = {2015},
month = {11}
}
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https://doi.org/10.1103/PhysRevD.92.105018
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The gap equation based on the Ginzburg-Landau expansion is precisely the mKdV or AKNS hierarchy of integrable nonlinear equations for the Gross-Neveu model with discrete or continuous chiral symmetry, respectively.</div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1063/1.3479358" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="21410772" data-product-type="Journal Article" data-product-subtype="" >https://doi.org/10.1063/1.3479358</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="1" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/biblio/21132429-self-consistent-crystalline-condensate-chiral-gross-neveu-bogoliubov-de-gennes-systems" itemprop="url">Self-Consistent Crystalline Condensate in Chiral Gross-Neveu and Bogoliubov-de Gennes Systems</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Basar, Goekce</span> ; <span class="author">Dunne, Gerald V</span> <span class="text-muted pubdata"> - Physical Review Letters</span> </span> </div> <div class="abstract">We derive a new exact self-consistent crystalline condensate in the (1+1)-dimensional chiral Gross-Neveu model. This also yields a new exact crystalline solution for the one dimensional Bogoliubov-de Gennes equations and the Eilenberger equation of semiclassical superconductivity. We show that the functional gap equation can be reduced to a solvable nonlinear equation and discuss implications for the temperature-chemical potential phase diagram.</div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/PHYSREVLETT.100.200404" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="21132429" data-product-type="Journal Article" data-product-subtype="" >https://doi.org/10.1103/PHYSREVLETT.100.200404</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="2" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/biblio/21054843-phase-diagram-non-local-chiral-quark-models-under-compact-star-conditions" itemprop="url">Phase diagram of non-local chiral quark models under compact star conditions</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Gomez Dumm, D</span> ; <span class="author">CONICET, Rivadavia 1917, 1033 Buenos Aires</span> ; <span class="author">Grunfeld, A G</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - AIP Conference Proceedings</span> </span> </div> <div class="abstract">We study the properties of isospin asymmetric quark matter under compact stars constraints using a relativistic quark model with non local interactions in the mean field approximation. We consider a Gaussian regulator, and medium coupling ratio. We present the corresponding phase diagrams and discuss, in particular, the competition between chiral symmetry restoration and the various forms of two flavor color superconductivity.</div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1063/1.2710607" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="21054843" data-product-type="Journal Article" data-product-subtype="" >https://doi.org/10.1063/1.2710607</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="3" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/biblio/20699017-kaon-condensation-quark-meson-coupling-model-compact-stars" itemprop="url">Kaon condensation in the quark-meson coupling model and compact stars</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Menezes, D P</span> ; <span class="author">School of Physics, University of Sydney, Sydney, New South Wales 2006</span> ; <span class="author">Panda, P K</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - Physical Review. C, Nuclear Physics</span> </span> </div> <div class="abstract">The properties of neutron stars, consisting of a crust of hadrons and an internal part of hadrons and kaon condensate, are calculated within the quark-meson-coupling model. We considered stars with nucleons only in the hadron phase and also stars with hyperons as well. The results are compared with the ones obtained from the nonlinear Walecka model for the hadronic phase.</div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/PhysRevC.72.035802" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="20699017" data-product-type="Journal Article" data-product-subtype="" >https://doi.org/10.1103/PhysRevC.72.035802</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="4" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/biblio/21537037-class-compact-entities-three-component-bose-einstein-condensates" itemprop="url">Class of compact entities in three-component Bose-Einstein condensates</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Szankowski, Piotr</span> ; <span class="author">Trippenbach, Marek</span> ; <span class="author">Infeld, Eryk</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - Physical Review. A</span> </span> </div> <div class="abstract">We introduce a class of solitonlike entities in spinor three-component Bose-Einstein condensates. These entities generalize well-known solitons. For special values of coupling constants, the system considered is completely integrable and supports N soliton solutions. The one-soliton solutions can be generalized to systems with different values of coupling constants. However, they no longer interact elastically. When two so-generalized solitons collide, a spin component oscillation is observed in both emerging entities. We propose to call these newfound entities oscillatons. They propagate without dispersion and retain their character after collisions. We derive an exact mathematical model for oscillatons and show that the well-known<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> one-soliton solutions are a particular case.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/PHYSREVA.83.013626" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="21537037" data-product-type="Journal Article" data-product-subtype="" >https://doi.org/10.1103/PHYSREVA.83.013626</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> </ul> </aside> </div> </section> </div> <div class="col-sm-3 order-sm-3"> <ul class="nav nav-stacked"> <li class="active"><a class="tab-nav disabled" data-tab="related" style="color: #636c72 !important; opacity: 1;"><span class="fa fa-angle-right"></span> Similar Records</a></li> </ul> </div> </div> </section> </div></div> </div> </div> </section> <footer class="" style="background-color:#f9f9f9; /* padding-top: 0.5rem; */"> <div class="footer-minor"> <div class="container"> <hr class="footer-separator" /> <div class="text-center" style="margin-top:1.25rem;"> <div class="pure-menu pure-menu-horizontal"> <ul class="pure-menu-list" id="footer-org-menu"> <li class="pure-menu-item"> <a href="https://energy.gov" target="_blank" rel="noopener noreferrer"> <img src="data:image/gif;base64,R0lGODlhAQABAIAAAP///wAAACH5BAEAAAAALAAAAAABAAEAAAICRAEAOw==" class="sprite sprite-footer-us-doe-min" alt="U.S. Department of Energy" /> </a> </li> <li class="pure-menu-item"> <a href="https://www.energy.gov/science/office-science" target="_blank" rel="noopener noreferrer"> <img src="data:image/gif;base64,R0lGODlhAQABAIAAAP///wAAACH5BAEAAAAALAAAAAABAAEAAAICRAEAOw==" class="sprite sprite-footer-office-of-science-min" alt="Office of Science" /> </a> </li> <li class="pure-menu-item"> <a href="/"> <img src="data:image/gif;base64,R0lGODlhAQABAIAAAP///wAAACH5BAEAAAAALAAAAAABAAEAAAICRAEAOw==" class="sprite sprite-footer-osti-min" alt="Office of Scientific and Technical Information" /> </a> </li> </ul> </div> </div> <div class="text-center small" style="margin-top:0.5em;margin-bottom:2.0rem;"> <div class="pure-menu pure-menu-horizontal"> <ul class="pure-menu-list"> <li class="pure-menu-item"><a href="/disclaim" class="pure-menu-link"><span class="fa fa-institution"></span> Website Policies <span class="hidden-xs">/ Important Links</span></a></li> <li class="pure-menu-item"><a href="/pages/contact" class="pure-menu-link"><span class="fa fa-comments-o"></span> Contact Us</a></li> <li class="d-block d-md-none"></li> <li class="pure-menu-item"><a href="https://www.facebook.com/ostigov" target="_blank" rel="noopener noreferrer" class="pure-menu-link social"><span class="sr-only">Facebook</span><em class="fa fa-facebook" style=""></em></a></li> <li class="pure-menu-item"><a href="https://twitter.com/OSTIgov" target="_blank" rel="noopener noreferrer" class="pure-menu-link social"><span class="sr-only">Twitter</span><em class="fa fa-twitter" style=""></em></a></li> <li class="pure-menu-item"><a href="https://www.youtube.com/user/ostigov" target="_blank" rel="noopener noreferrer" class="pure-menu-link social"><span class="sr-only">YouTube</span><em class="fa fa-youtube-play" style=""></em></a></li> </ul> </div> </div> </div> </div> </footer> <link href="/pages/css/pages.fonts.220701.1625.css" rel="stylesheet"> <script src="/pages/js/pages.220701.1625.js"></script><noscript></noscript> <script defer src="/pages/js/pages.biblio.220701.1625.js"></script><noscript></noscript> <script defer src="/pages/js/lity.js"></script><noscript></noscript> <script async�type="text/javascript" src="/pages/js/Universal-Federated-Analytics-Min.js?agency=DOE" id="_fed_an_ua_tag"></script><noscript></noscript> </body> <!-- DOE PAGES v.220701.1625 --> </html>