Dynamical Coupling of the Core-Superfluid in Neutron Stars

Details Dynamical Coupling of the Core-Superfluid in Neutron Stars Dynamical Coupling of the Core-Superfluid in Neutron Stars

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...501l.185j&link_type=abstract

Astrophysical Journal Letters v.501, p.L185

Astronomy and Astrophysics

Astronomy

7

Hydrodynamics, Stars: Neutron, Stars: Pulsars: Individual Name: Vela Pulsar

Scientific paper

Coupling of the neutron superfluid in the core of a neutron star to the rest of the star is discussed, assuming no pinning for the superfluid vortices. The earlier calculation of the relevant dynamical coupling timescale is shown to be incomplete. The corrected timescale is shorter by an order of magnitude; hence the observationally inferred upper limit on the core-coupling time remains much larger than, and in agreement with, the new predicted value.

Affiliated with

Also associated with

No associations

Rating

Dynamical Coupling of the Core-Superfluid in Neutron Stars 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 Dynamical Coupling of the Core-Superfluid in Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical Coupling of the Core-Superfluid in Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1343433