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- W3100836780 abstract "The property difference between the neutron star PSR J0348[Formula: see text]0432 and its proto neutron star is studied in the framework of the relativistic mean field theory considering neutrino trapping. We see that the central baryon number density of the proto neutron star PSR J0348+0432 is in the range [Formula: see text][Formula: see text]fm[Formula: see text], which is smaller than that of the neutron star PSR J0348[Formula: see text]0432 [Formula: see text][Formula: see text]fm[Formula: see text]. Inside the neutron star PSR J0348[Formula: see text]0432, only the neutrons, protons, [Formula: see text] and [Formula: see text] produce, whereas the hyperons [Formula: see text] and [Formula: see text] all do not appear. But in the proto neutron star PSR J0348[Formula: see text]0432, hyperons [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text] all will produce, though their relative particle number density is still very small, no more than 2%. This shows that higher temperature will be advantageous to the hyperon production." @default.
- W3100836780 created "2020-11-23" @default.
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- W3100836780 date "2017-09-19" @default.
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- W3100836780 title "Property difference between the neutron star PSR J0348+0432 and its proto neutron star" @default.
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- W3100836780 doi "https://doi.org/10.1142/s0218271817501334" @default.
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