Temperature Effects on Core g-Modes of Neutron Stars

Neutron stars provide a unique physical laboratory to study the properties of matter at high density. We diagnostic composition high-density matter, namely, g-mode oscillations, which are driven by buoyancy forces. These oscillations can be excited tidal forces and couple gravitational waves. extend prior results for spectrum cold neutron star temperatures that expected achieved in mergers using parameterization finite-temperature effects recently proposed Raithel, \"Ozel Psaltis. find g-modes canonical mass ($\approx$1.4$M_{\odot}$) suppressed temperature, core $g$-modes supported only most massive ($\geq $2$M_{\odot}$) hot stars.