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- W202110910 abstract "We analyze the restriction on the equation of state for neutron stars given by the more or less known masses (1.445 ± 0.007M ⊙ and 1.85 ± 0.30M ⊙) of neutron stars and the also more or less known frequencies of fast rotating pulsars like PSR1957+20 (Ω = 4033 Hz) and perhaps by a newborne pulsar in the supernova SN1987A (Ω = 12369 Hz), where the latter one is seen only by one group for 8 hours and then never again. Softer equations of state generally yield stable rotating pulsars of lower mass, while stiffer ones are leading to heavier neutron stars." @default.
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- W202110910 date "1989-01-01" @default.
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- W202110910 title "Constraints on the equation of state for neutron stars from fast rotating pulsars" @default.
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