Stellar energy-loss rates due to S, P, or T neutral currents

Details Stellar energy-loss rates due to S, P, or T neutral currents Stellar energy-loss rates due to S, P, or T neutral currents

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phrvd..15..977d&link_type=abstract

Physical Review D (Particles and Fields), Volume 15, Issue 4, 15 February 1977, pp.977-982

Physics

6

Scientific paper

The energy-loss rate in stellar matter due to neutrino production is calculated assuming that the weak leptonic neutral current includes scalar, pseudoscalar, or tensor covariants. The processes e+ + e--->ν + ν¯, γ + e-->e + ν + ν¯, e + Z-->e + Z + ν + ν¯, and γ + γ-->ν + ν¯ are considered in the respective temperature and density regions of physical significance. Comparison with observed stellar lifetimes allows an upper limit to be placed on the new couplings.

Affiliated with

Also associated with

No associations

Rating

Stellar energy-loss rates due to S, P, or T neutral currents 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 Stellar energy-loss rates due to S, P, or T neutral currents, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar energy-loss rates due to S, P, or T neutral currents will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-800692