From multifragmentation to supernovae and neutron stars

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dc.creatorGulminelli, F.
dc.creatorChomaz, P.
dc.creatorDucoin, C.
dc.creatorNapolitani, P.
dc.creatorHasnaoui, K.
dc.date2006-05-18
dc.date.accessioned2026-07-07T10:42:43Z
dc.date.available2026-07-07T10:42:43Z
dc.descriptionThe thermodynamics properties of globally neutral dense stellar matter are analyzed both in terms of mean field instabilities and structures beyond the mean field. The mean field response to finite wavelenght fluctuations is calculated with the realistic Sly230a effective interaction. A Monte Carlo simulation of a schematic lattice Hamiltonian shows the importance of calculations beyond the mean field to calculate the phase diagram of stellar matter. The analogies and differences respect to the thermodynamics of nuclear matter and finite nuclei are stressed.
dc.descriptionTo be published in Acta Phys. Hung. A
dc.identifierhttps://arxiv.org/abs/nucl-th/0605042
dc.identifierhttp://arxiv.org/abs/nucl-th/0605042
dc.identifierAIPConf.Proc.884:318-326,2007
dc.identifierdoi:10.1063/1.2710599
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/182043
dc.subjectNuclear Theory
dc.titleFrom multifragmentation to supernovae and neutron stars
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