[Submitted on 10 Apr 2026] (cross-list from astro-ph.HE)
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.
- Comments:
- 14 pages, 12 figures
- Subjects:
- High Energy Astrophysical Phenomena (astro-ph.HE); Solar and Stellar Astrophysics (astro-ph.SR); Nuclear Theory (nucl-th)
- arXiv:
- 2604.11815 [pdf]