Solar Rotation and Neutrino Flux

Details Solar Rotation and Neutrino Flux Solar Rotation and Neutrino Flux

Dec 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968phrvl..21.1602s&link_type=abstract

Physical Review Letters, vol. 21, Issue 23, pp. 1602-1605

Physics

20

Scientific paper

If the sun possesses a fast-rotating core, mixing in its interior may be a possibility. We calculate the solar neutrino flux as a function of fractional mass qm in the mixed zone for "slow," "fast," and "very fast" mixing. Only for "slow" mixing and large qm could the neutrino flux be decreased appreciably, but such large values of qm are unlikely.

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