Neutrino Helioseismology

Details Neutrino Helioseismology Neutrino Helioseismology

1992-08-11

arxiv.org/abs/hep-ph/9208223v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, HUTP-92/A038

Scientific paper

The observed deficit of $\rm ^8B$ solar neutrinos may call for an improved standard model of the sun or an expanded standard model of particle physics ({\it e.g.,} with neutrino masses and mixing). In the former case, contemporary fluid motions and thermal fluctuations in the sun's core may modify nuclear reaction rates and restore agreement. To test this notion, we propose a search for short--term variations of the solar neutrino flux.

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