The nuclear symmetry energy and stability of matter in neutron star

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dc.creatorKubis, Sebastian
dc.date2006-11-23
dc.date.accessioned2026-07-07T10:36:38Z
dc.date.available2026-07-07T10:36:38Z
dc.descriptionIt is shown that behavior of the nuclear symmetry energy is the key quantity in the stability consideration in neutron star matter. The symmetry energy controls the position of crust-core transition and also may lead to new effects in the inner core of neutron star.
dc.description5 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0611740
dc.identifierhttp://arxiv.org/abs/astro-ph/0611740
dc.identifierPhys.Rev.C76:025801,2007
dc.identifierdoi:10.1103/PhysRevC.76.025801
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180118
dc.subjectAstrophysics
dc.titleThe nuclear symmetry energy and stability of matter in neutron star
dc.typetext

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