Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures

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dc.creatorHuber, H.
dc.creatorWeber, F.
dc.creatorWeigel, M. K.
dc.date1998-03-09
dc.date.accessioned2026-07-07T11:11:36Z
dc.date.available2026-07-07T11:11:36Z
dc.descriptionThe properties of hot matter are studied in the frame of the relativistic Brueckner-Hartree-Fock theory. The equations are solved self-consistently in the full Dirac space. For the interaction we used the potentials given by Brockmann and Machleidt. The obtained critical temperatures are smaller than in most of the nonrelativistic investigations. We also calculated the thermodynamic properties of hot matter in the relativistic Hartree--Fock approximation, where the force parameters were adjusted to the outcome of the relativistic Brueckner--Hartree--Fock calculations at zero temperature. Here, one obtains higher critical temperatures, which are comparable with other relativistic calculations in the Hartree scheme.
dc.description8 pages, 9 figures, submitted in a shorter version to Phys. Rev. C
dc.identifierhttps://arxiv.org/abs/nucl-th/9803026
dc.identifierhttp://arxiv.org/abs/nucl-th/9803026
dc.identifierPhys.Rev.C57:3484-3487,1998
dc.identifierdoi:10.1103/PhysRevC.57.3484
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191150
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleSymmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures
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