Neutrino Energy Loss in Neutron Star Matter

Details Neutrino Energy Loss in Neutron Star Matter Neutrino Energy Loss in Neutron Star Matter

Dec 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972pthph..48.1849i&link_type=abstract

Progress of Theoretical Physics, Vol. 48, No. 6, pp. 1849-1859

Physics

18

Scientific paper

The theory of the energy loss due to neutrino processes in neutron stars is formulated in such a form that one can include the effect of strong interaction systematically. As an application the rates of energy loss are calculated for the following cases of interest in the study of neutron stars; i) the neutron and the proton liquid are both normal, ii) the proton or iii) the neutron liquid is in the superfluid state. Our results largely confirm the earlier calculations by Bahcall and Wolf and by Wolf. The rate of energy loss in the state of nuclei coexisting with free neutrons is also discussed.

Affiliated with

Also associated with

No associations

Rating

Neutrino Energy Loss in Neutron Star Matter 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 Neutrino Energy Loss in Neutron Star Matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino Energy Loss in Neutron Star Matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1641085