Low-energy solar anti-neutrinos

Details Low-energy solar anti-neutrinos Low-energy solar anti-neutrinos

1998-08-13

arxiv.org/abs/hep-ph/9808314v1

Nucl.Phys.Proc.Suppl.70:348-350,1999

Physics

High Energy Physics

High Energy Physics - Phenomenology

Talk given at TAUP 97, Gran Sasso, Italy, Sep. 1997; LaTeX, 3 pages, 1 postscript figure, uses espcrc2.sty

Scientific paper

10.1016/S0920-5632(98)00448-4

If neutrino conversions within the Sun result in partial polarization of initial solar neutrino fluxes, then a new opportunity arises to observe the anti-\nu_e's in future neutrino experiments in the low energy region (such as BOREXINO or HELLAZ) and thus to probe the Majorana nature of the neutrinos. The \nu_e -> anti-\nu_e conversions may take place for low energy solar neutrinos while being unobservable at the Kamiokande and Super-Kamiokande experiments.

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