Energy loss from stellar bodies through neutrino production by a second-class weak neutral current

Details Energy loss from stellar bodies through neutrino production by a second-class weak neutral current Energy loss from stellar bodies through neutrino production by a second-class weak neutral current

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979phrvd..19..721b&link_type=abstract

Physical Review D (Particles and Fields), Volume 19, Issue 2, 15 January 1979, pp.721-723

Physics

1

Scientific paper

Using a second-class V, A weak neutral current, we have calculated the
rate of energy loss in stellar bodies through the photoneutrino
processes on protons. We find that at temperatures of the order of
1011K, the energy-loss rate compares with the rate calculated
in the unified SU(2) × U(1) theory of Salam and Weinberg.

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