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- W1580157819 abstract "We shall show this report that the theoretical evolution of a particular class of systems containing a neutron star, the so-called black widow binaries, suggest masses above the $sim 2 M_{odot}$, a fact that would bring serious concerns about the right description of the equation of state above the saturation density. Moreover, so far the actual determinations of masses for these systems consistently give values above $2 M_{odot}$, reinforcing the quandary. In this sense, and given that the confirmation of these ideas would create problems for the microphysical description, we argue that a crisis could be in the works neutron star physics." @default.
- W1580157819 created "2016-06-24" @default.
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- W1580157819 date "2012-01-01" @default.
- W1580157819 modified "2023-09-27" @default.
- W1580157819 title "Is There a Crisis in Neutron Star Physics" @default.
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