Isovector Channel Role of Relativistic Mean Field Models in the Neutrino Mean Free Path

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dc.creatorSulaksono, A.
dc.creatorHutauruk, P. T. P.
dc.creatorMart, T.
dc.date2005-12-27
dc.date.accessioned2026-07-07T10:46:50Z
dc.date.available2026-07-07T10:46:50Z
dc.descriptionAn improvement in the treatment of the isovector channel of relativistic mean field (RMF) models based on effective field theory (E-RMF) is suggested, by adding an isovector scalar (delta) meson and using a similar procedure to the one used by Horowitz and Piekarewicz to adjust the isovector-vector channel in order to achieve a softer density dependent symmetry energy of the nuclear matter at high density. Their effects on the equation of state (EOS) at high density and on the neutrino mean free path (NMFP) in neutron stars are discussed.
dc.description20 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0512093
dc.identifierhttp://arxiv.org/abs/nucl-th/0512093
dc.identifierPhys.Rev.C72:065801,2005
dc.identifierdoi:10.1103/PhysRevC.72.065801
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183369
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleIsovector Channel Role of Relativistic Mean Field Models in the Neutrino Mean Free Path
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