Ising analogue to compact-star matter

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dc.creatorNapolitani, P.
dc.creatorChomaz, Ph.
dc.creatorGulminelli, F.
dc.creatorHasnaoui, K. H. O.
dc.date2006-09-22
dc.date2007-06-12
dc.date.accessioned2026-07-07T10:26:30Z
dc.date.available2026-07-07T10:26:30Z
dc.descriptionBy constructing an Ising analogue of compact-star matter at sub-saturation density we explored the effect of Coulomb frustration on the nuclear liquid-gas phase transition. Our conclusions is twofold. First, the range of temperatures where inhomogeneous phases form expands with increasing Coulomb-field strength. Second, within the approximation of uniform electron distribution, the limiting point upon which the phase-coexistence region ends does not exhibit any critical behaviour. Possible astrophysics consequences and thermodynamical connections are discussed.
dc.description4 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0609063
dc.identifierhttp://arxiv.org/abs/nucl-th/0609063
dc.identifierPhys.Rev.Lett.98:131102,2007
dc.identifierdoi:10.1103/PhysRevLett.98.131102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176901
dc.subjectNuclear Theory
dc.subjectStatistical Mechanics
dc.titleIsing analogue to compact-star matter
dc.typetext

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