On solar neutrinos and the method of spherically averaged rotation

Details On solar neutrinos and the method of spherically averaged rotation On solar neutrinos and the method of spherically averaged rotation

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.170p..67p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 170, Mar. 1975, p. 67P-70P.

Astronomy and Astrophysics

Astronomy

2

Astronomical Models, Error Analysis, Neutrinos, Solar Rotation, Integral Equations, Particle Flux Density, Solar Flux, Stellar Rotation, Stellar Structure

Scientific paper

It is shown that the use of a spherically averaged rotation force results in a small underestimation of the neutrino flux in rotating stars, and an overestimation in solar models with a rapidly rotating core. The method of spherical averages is analyzed for uniformly rotating models and for rapidly rotating core models. Calculations for the first case result in a maximum 10% underestimation when only the surface of a single sphere is considered, and a 1% underestimation when the whole star is considered. Calculations for the second case indicate an overestimation of the neutrino flux when a spherically averaged rotation force is derived.

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