Remarks on the beta stability in neutron stars

Details Remarks on the beta stability in neutron stars Remarks on the beta stability in neutron stars

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phlb..106..255b&link_type=abstract

Physics Letters B, Volume 106, Issue 4, p. 255-258.

Physics

66

Scientific paper

We show that in a relativistic theory of nuclear matter the usually suppressed beta decay of neutrons n --> p + e- + g¯ne is allowed. It can serve as a cooling mechanism. The theory also predicts the existence of real pions inside dense neutron stars. These conclusions rest primarily on the correct phenomenological description of symmetry energy in symmetric (N = Z) nuclear matter.

Affiliated with

Also associated with

No associations

Rating

Remarks on the beta stability 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 Remarks on the beta stability in neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Remarks on the beta stability in neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-744623