Neutral currents and stellar cooling

Details Neutral currents and stellar cooling Neutral currents and stellar cooling

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974phlb...52..275b&link_type=abstract

Physics Letters B, Volume 52, Issue 3, p. 275-278.

Physics

10

Scientific paper

If weak neutral currents couple with the strengths suggested by recent experiments, then stellar cooling via neutrino pair emission from thermally excited nuclear states may be significant in white dwarfs with central temperature <~108° K. At higher temperatures, other neutrino cooling processes are more important. In the sun, the decay of thermally excited 57Fe nuclei may produce a moderately large, but probably unobservable, low-energy flux of νμ, g¯nμ, νe, and g¯ne neutrinos.
Alfred P. Sloan Foundation Fellow.

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