Computes quasiradial frequencies of rotating neutron and hybrid stars in slow-rotation limit and identifies distinct spin-down behavior between the two classes using BHF, RMF, and Dyson-Schwinger EOS models.
Rutherfordet al., Constraining the dense matter equation of state with new NICER mass–radius measurements and new chiral effective field theory inputs, Astrophys
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Quasiradial oscillations of rotating hybrid neutron stars
Computes quasiradial frequencies of rotating neutron and hybrid stars in slow-rotation limit and identifies distinct spin-down behavior between the two classes using BHF, RMF, and Dyson-Schwinger EOS models.