Stellar energy loss from the reaction γγ-->e+e-νν¯

Details Stellar energy loss from the reaction γγ-->e+e-νν¯ Stellar energy loss from the reaction γγ-->e+e-νν¯

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976phrvd..14..335s&link_type=abstract

Physical Review D (Particles and Fields), Volume 14, Issue 2, 15 July 1976, pp.335-339

Physics

1

Scientific paper

We discuss here a new mechanism for energy loss by stars via a γγ collision which for temperatures >~me is several orders of magnitude more efficient than the direct reaction γγ-->νν¯. For most (but perhaps not all) stellar densities and temperatures the energy loss rate is, however, still small compared with that due to γ e-->eνν¯ and e+e--->νν¯.

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