Spin Polarized Asymmetric Nuclear Matter and Neutron Star Matter Within the Lowest Order Constrained Variational Method

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dc.creatorBordbar, G. H.
dc.creatorBigdeli, M.
dc.date2008-09-20
dc.date2008-11-20
dc.date.accessioned2026-07-07T11:45:51Z
dc.date.available2026-07-07T11:45:51Z
dc.descriptionIn this paper, we calculate properties of the spin polarized asymmetrical nuclear matter and neutron star matter, using the lowest order constrained variational (LOCV) method with the $AV_{18}$, $Reid93$, $UV_{14}$ and $AV_{14}$ potentials. According to our results, the spontaneous phase transition to a ferromagnetic state in the asymmetrical nuclear matter as well as neutron star matter do not occur.
dc.description21 pages, 11 figures
dc.identifierhttps://arxiv.org/abs/0809.3498
dc.identifierhttp://arxiv.org/abs/0809.3498
dc.identifierPhys.Rev.C77:015805,2008
dc.identifierdoi:10.1103/PhysRevC.77.015805
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202020
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleSpin Polarized Asymmetric Nuclear Matter and Neutron Star Matter Within the Lowest Order Constrained Variational Method
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