Solar models with rotating cores

Details Solar models with rotating cores Solar models with rotating cores

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974natur.252..366r&link_type=abstract

Nature, vol. 252, Nov. 29, 1974, p. 366-368. NSF-supported research.

Astronomy and Astrophysics

Astronomy

9

Angular Momentum, Astronomical Models, Momentum Transfer, Solar Oblateness, Solar Rotation, Neutrinos, Particle Flux Density, Radiative Transfer, Stellar Evolution

Scientific paper

The results obtained by Sakurai (1972) regarding the transfer of angular momentum occurring in connection with Eddington-Sweet circulation are considered along with an investigation by Demarque et al. (1973), giving attention to the oblateness in solar models. Possibilities for inducing a transient phase with a core that is spinning up are discussed and the solar neutrino problem is taken into account.

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