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- W2112967511 abstract "We investigate the structure of protoneutron stars (PNS) formed by hadronic and quark matter in {beta}-equilibrium described by appropriate equations of state (EOS). For the hadronic matter, we use a finite temperature EOS based on the Brueckner-Bethe-Goldstone many-body theory, with realistic two- and three-body forces. For the quark sector, we employ the Nambu-Jona-Lasinio model. We find that the allowed maximum masses are comprised in a narrow range around 1.8 solar masses, with a slight dependence on the temperature. Metastable hybrid protoneutron stars are not found." @default.
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- W2112967511 date "2008-04-25" @default.
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- W2112967511 title "Structure of hybrid protoneutron stars within the Nambu–Jona-Lasinio model" @default.
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- W2112967511 doi "https://doi.org/10.1103/physrevd.77.085022" @default.
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