Lower bound on neutrino pair emission

Details Lower bound on neutrino pair emission Lower bound on neutrino pair emission

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phlb...57..181m&link_type=abstract

Physics Letters B, Volume 57, Issue 2, p. 181-182.

Physics

2

Scientific paper

Weak neutral currents affect the rates with which stars lose energy by emitting neutrino pairs. These rates can be calculated once the parameters of the underlying theory are fixed. Here we show that any new gauge theory will have a minimum rate, equal to half the old rate. The proof rests on the (assumed) μ-e universality of neutral currents. We also speculate on the possible existence of new types of neutrinos which may considerably enhance stellar cooling. The minimum becomes ((n+1)/(n+2)) times the old rate, where n=number of new neutrinos.

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