Stellar energy loss and supersymmetry

Details Stellar energy loss and supersymmetry Stellar energy loss and supersymmetry

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phrvd..29.1270a&link_type=abstract

Physical Review D (Particles and Fields), Volume 29, Issue 6, 15 March 1984, pp.1270-1272

Physics

3

Scientific paper

We calculate the rate of energy loss from stellar bodies through production of γ~ and G~, the supersymmetric partners of the conventional photon and graviton, in γ+γ-->γ~+γ~―,γ~+G~―,γ~―+G~. For the light masses of γ~ and G~, we find that the γ~ luminosity is dominant over the standard neutrino luminosity in γ-γ reactions at all temperatures. Furthermore, the ν luminosity due to supersymmetric contributions from scalar electrons and W~'s is insignificant if the present constraints on the masses of W~'s and scalar electrons are taken seriously.

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