Relativistic two-constituent superfluid neutron stars at finite temperature

Details Relativistic two-constituent superfluid neutron stars at finite temperature Relativistic two-constituent superfluid neutron stars at finite temperature

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phla..226..332v&link_type=abstract

Physics Letters A, v. 226, p. 332-335.

Physics

Scientific paper

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.

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