A New Study of the Transition to Uniform Nuclear Matter in Neutron Stars and Supernovae

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dc.creatorNewton, W. G.
dc.date2007-08-23
dc.date.accessioned2026-07-07T12:13:41Z
dc.date.available2026-07-07T12:13:41Z
dc.descriptionA comprehensive microscopic study of the properties of bulk matter at densities just below nuclear saturation $ρ_s = 2.5 \sim 10^{14}$ g cm$^{-3}$, zero and finite temperature and high neutron fraction, is outlined, and preliminary results presented. Such matter is expected to exist in the inner crust of neutron stars and during the core collapse of massive stars with $M \gtrsim 8M_{\odot}
dc.description4 pages, 2 figures. Participant Contribution at the ``Dense Matter in Heavy Ion Collisions and Astrophysics" Summer School, JINR, Dubna, Aug. 21 - Sept. 1, 2006. To be published in PEPAN letters
dc.identifierhttps://arxiv.org/abs/0708.3212
dc.identifierhttp://arxiv.org/abs/0708.3212
dc.identifierPhys.Part.Nucl.39:1173-1175,2008
dc.identifierdoi:10.1134/S1063779608070356
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/210934
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleA New Study of the Transition to Uniform Nuclear Matter in Neutron Stars and Supernovae
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