Stellar Energy-Loss Rates in a Convergent Theory of Weak and Electromagnetic Interactions

Details Stellar Energy-Loss Rates in a Convergent Theory of Weak and Electromagnetic Interactions Stellar Energy-Loss Rates in a Convergent Theory of Weak and Electromagnetic Interactions

Aug 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phrvd...6..941d&link_type=abstract

Physical Review D, vol. 6, Issue 4, pp. 941-949

Physics

160

Scientific paper

The stellar energy-loss rates due to the production of neutrino pairs are calculated in Weinberg's theory of electromagnetic and weak interactions. The ratio of the total rate calculated here to the rate calculated in the ordinary theory of weak interactions is 100+0.93-0.30, where the uncertainty comes entirely from the lack of knowledge of the W-meson mass. The ratio of the experimental rate to the rate calculated in the ordinary theory is 100+/-2. Thus Weinberg's theory gives numbers well within the experimental limits for all values of the W mass.

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