Finite temperature effects on g-modes of inviscid neutron stars
David Morales-Zapien · Prashanth Jaikumar · Thomas Klähn
We study the effect of temperature on secular, compositional -modes in the core of inviscid neutron stars. Using a chiral sigma model, we construct isentropic temperature profiles for hot and dense matter and find that the frequency of the global core -mode's dependence on temperature is governed by the nuclear symmetry energy slope parameter . As a result, the -mode frequency of a warm neutron star can be either higher or lower than that of its cold counterpart, depending on . Our results highlight the interplay of thermal effects and composition gradients, and demonstrate the potential of neutron star -mode observations to constrain the density dependence of the symmetry energy.