Fully relativistic KEH calculations with five Skyrme EoSs show rotation shifts neutron star mass-radius curves and suggest the empirical 716 Hz limit may exclude some low-mass configurations that are actually stable.
This pulsar is also known to be rotating at a spin frequency of 346 Hz
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Fully general relativistic description of rapidly-rotating axially-symmetric neutron stars for constraining nuclear matter equations of state
Fully relativistic KEH calculations with five Skyrme EoSs show rotation shifts neutron star mass-radius curves and suggest the empirical 716 Hz limit may exclude some low-mass configurations that are actually stable.