Nuclear pasta structure in hot neutron stars

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dc.creatorWatanabe, Gentaro
dc.creatorSato, Katsuhiko
dc.creatorYasuoka, Kenji
dc.creatorEbisuzaki, Toshikazu
dc.date2003-10-10
dc.date.accessioned2026-07-07T02:10:18Z
dc.date.available2026-07-07T02:10:18Z
dc.descriptionStructure of cold and hot dense matter at subnuclear densities is investigated by quantum molecular dynamics (QMD) simulations. Obtained phase diagrams show that the density of the phase boundaries between the different nuclear structures decreases with increasing temperature due to the thermal expansion of nuclear matter region.
dc.description2 pages, 1figure, To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0310290
dc.identifierhttp://arxiv.org/abs/astro-ph/0310290
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6698
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleNuclear pasta structure in hot neutron stars
dc.typetext

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