Relativistic effects in the hydrodynamics of the superfluid component of a neutron star

Details Relativistic effects in the hydrodynamics of the superfluid component of a neutron star Relativistic effects in the hydrodynamics of the superfluid component of a neutron star

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....98...36r&link_type=abstract

Astronomy and Astrophysics, vol. 98, no. 1, May 1981, p. 36-38.

Astronomy and Astrophysics

Astrophysics

5

Hydrodynamics, Neutron Stars, Relativistic Effects, Superfluidity, Vortices, Differential Equations, Gravitational Effects, Stellar Rotation

Scientific paper

The effect of high gravitational fields on the geometry of the array of vortices of a uniformly superfluid neutron star is considered. In the case of the simplest possible superfluid model of a rotating star, a very simple relation is obtained between the shape of the vortex lines and the general relativistic functions describing a uniform rotating sphere. The deviation of the shape of the vortices from a straight line is shown to be unimportant for masses not reaching the upper limit.

Affiliated with

Also associated with

No associations

Rating

Relativistic effects in the hydrodynamics of the superfluid component of a neutron star does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Relativistic effects in the hydrodynamics of the superfluid component of a neutron star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relativistic effects in the hydrodynamics of the superfluid component of a neutron star will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1440608