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• W2022175196 abstract "The equation of state (EOS) of dense matter and neutrino mean free path (NMFP) in a neutron star have been studied by using relativistic mean field models motivated by effective field theory. It is found that the models predict too large proton fractions, although one of the models (G2) predicts an acceptable EOS. This is caused by the isovector terms. Except G2, the other two models predict anomalous NMFP's. In order to minimize the anomaly, besides an acceptable EOS, a large ${M}^{*}$ is favorable. A model with large ${M}^{*}$ retains the regularity in the NMFP even for a small neutron fraction." @default.
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• W2022175196 date "2004-12-01" @default.
• W2022175196 modified "2023-09-26" @default.
• W2022175196 title "Neutron fraction and neutrino mean free path predictions in relativistic mean field models" @default.
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• W2022175196 doi "https://doi.org/10.1103/physrevc.70.068801" @default.
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