Stellar energy loss rates due to SPT neutral currents

Details Stellar energy loss rates due to SPT neutral currents Stellar energy loss rates due to SPT neutral currents

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976selr.book.....d&link_type=abstract

Unknown

Physics

Energy Dissipation, Neutrinos, Stars, Density, Electrons, Particle Production, Positrons, Stellar Evolution, Stellar Temperature

Scientific paper

The energy loss rate in stellar matter due to neutrino production was calculated assuming the weak leptonic neutral current includes scalar, pseudoscalar, or tensor covariants. Different processes were considered in the respective temperature and density regions of physical significance. Comparison with observed stellar lifetimes allow an upper limit to be placed on the new couplings.

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