Solar neutrino spectroscopy.

Details Solar neutrino spectroscopy. Solar neutrino spectroscopy.

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..70..292v&link_type=abstract

Nuclear Physics B, Proc. Suppl., Vol. 70, p. 292 - 300

Physics

Nuclear Physics

Solar Neutrinos, Neutrinos

Scientific paper

All solar neutrino experiments find a considerably lower flux than expected by standard solar models. This finding is generally called the solar neutrino problem. Many attempts have been made to explain this result by altering the solar models, or assuming different nuclear cross sections for fusion processes assumed to be the energy sources in the sun. There have been performed numerous experiments recently to investigate the different possibilities to explain the solar neutrino problem. Up to now no convincing explanation based on "standard" physics was suggested. However, assuming non-standard neutrino properties, i.e. neutrino masses and mixing as expected in most extensions of the standard theory of elementary particle physics, natural solutions for the solar neutrino problem can be found. In this contribution an attempt is made to review the situation of the neutrino astronomy for solar neutrino spectroscopy and discuss the future prospects in this field.

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