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• W2015172574 abstract "In 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 ${mathrm{AV}}_{18}$, Reid93, ${mathrm{UV}}_{14}$, and ${mathrm{AV}}_{14}$ 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." @default.
• W2015172574 created "2016-06-24" @default.
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• W2015172574 date "2008-01-16" @default.
• W2015172574 modified "2023-10-17" @default.
• W2015172574 title "Spin polarized asymmetric nuclear matter and neutron star matter within the lowest order constrained variational method" @default.
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• W2015172574 doi "https://doi.org/10.1103/physrevc.77.015805" @default.
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