Relativistic two-constituent superfluid neutron stars at finite temperature
Abstract
We apply the relativistic two-constituent superfluid hydrodynamics to consider a general relativistic non-rotating star at finite temperature. The normal contribution is determined by phonon excitations. As a probe of the equations derived we calculate a thermal contribution to the mass of the star.
- Publication:
-
Physics Letters A
- Pub Date:
- February 1997
- DOI:
- 10.1016/S0375-9601(96)00884-5
- Bibcode:
- 1997PhLA..226..332V