Rapid cooling of magnetized neutron stars

Details Rapid cooling of magnetized neutron stars Rapid cooling of magnetized neutron stars

1998-04-15

arxiv.org/abs/astro-ph/9804145v1

Astronomy and Astrophysics

Astrophysics

9 pages; Revtex; figure included

Scientific paper

10.1103/PhysRevD.58.121301

The neutrino emissivities resulting from direct URCA processes in neutron stars are calculated in a relativistic Dirac-Hartree approach in presence of a magnetic field. In a quark or a hyperon matter environment, the emissivity due to nucleon direct URCA processes is suppressed relative to that from pure nuclear matter. In all the cases studied, the magnetic field enhances emissivity compared to the field-free cases.

Affiliated with

Also associated with

No associations

Rating

Rapid cooling of magnetized 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 Rapid cooling of magnetized neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapid cooling of magnetized neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-465813