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arxiv: 1404.6768 · v1 · pith:ZG4ZKM3Xnew · submitted 2014-04-27 · 🌌 astro-ph.SR · astro-ph.HE· gr-qc

Composition temperature-dependent g-modes in superfluid neutron stars

classification 🌌 astro-ph.SR astro-ph.HEgr-qc
keywords neutronddotmodesstarssuperfluidcompositiontemperature-dependentapproximation
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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.

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