The frequency of global core g-modes in warm neutron stars can be higher or lower than in cold stars depending on the nuclear symmetry energy slope L.
Lai, Resonant oscillations and tidal heating in coa- lescing binary neutron stars, The Astrophysical Journal 437, 742 (1994)
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Finite temperature effects on g-modes of inviscid neutron stars
The frequency of global core g-modes in warm neutron stars can be higher or lower than in cold stars depending on the nuclear symmetry energy slope L.