Stellar energy loss through scalar-neutrino production

Details Stellar energy loss through scalar-neutrino production Stellar energy loss through scalar-neutrino production

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..32.3081h&link_type=abstract

Physical Review D (Particles and Fields), Volume 32, Issue 12, 15 December 1985, pp.3081-3083

Physics

1

Radiation Mechanisms, Polarization, Supersymmetry

Scientific paper

We consider the role of massless scalar neutrinos in processes relevant to stellar evolution. Special attention is given to eē-->ν~ ν¯~ and the more exotic process γγ-->ν~ ν¯~. We conclude that ultralight scalar neutrinos, if they exist, will be produced most copiously through neutral-current interactions and will enhance the energy-loss rate by 5%.

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