Composition temperature-dependent g-modes in superfluid neutron stars

Understand

We demonstrate a possibility of existence of a peculiar temperature-dependent composition $g$-modes in superfluid neutron stars.

• We calculate the Brunt-V$\ddot{\rm a}$is$\ddot{\rm a}$l$\ddot{\rm a}$ frequency for these modes, as well as their eigenfrequencies.
• The latter turn out to be rather large, up to $\sim 500$ Hz for a chosen model of a neutron star.
• This result indicates, in particular, that use of the barotropic equation of state may be not a good approximation for calculation of inertial modes even in most rapidly rotating superfluid neutron stars.