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- W2015996716 abstract "Recently ∼2M⊙ neutron stars PSR J1614-2230 and PSR J0348+0432 have been observed in neutron star-white dwarf binaries. These observations ruled out many neutron star equations of states with which the maximum neutron star mass becomes less than 2M⊙. On the other hand, all well-measured neutron star masses in double neutron star binaries are still less than 1.5M⊙. In this article we suggest that 2M⊙ neutron stars in neutron star-white dwarf binaries are the result of the supercritical accretion onto the first-born neutron star during the evolution of the binary progenitors." @default.
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- W2015996716 date "2014-08-01" @default.
- W2015996716 modified "2023-09-27" @default.
- W2015996716 title "Supercritical accretion in the evolution of neutron star binaries and its implications" @default.
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- W2015996716 doi "https://doi.org/10.1016/j.nuclphysa.2014.04.019" @default.
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