Computer Science – Sound
Scientific paper
Jul 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207..601n&link_type=abstract
Astrophysical Journal, vol. 207, July 15, 1976, pt. 1, p. 601-604.
Computer Science
Sound
6
Acoustic Excitation, Energy Transfer, Neutrinos, Solar Physics, Stellar Models, Astronomical Models, Radiative Transfer, Solar Temperature, Sound Waves, Stellar Structure
Scientific paper
A sequence of solar models is presented in which decreasing fractions of the energy flux are carried by radiation. It is found that counting rates below 1 SNU can be obtained for Cl-37 observations if more than half of the solar energy is transported to the convective layers by nonradiative means. It is shown that the low-SNU models have very low central temperatures, require extremely helium-poor compositions, and are unable to penetrate below Ulrich's (1974) theoretical limit of 0.5 SNU, a characteristic shared by all models in which nuclear reactions provide all the power. Energy transport by acoustic waves is mentioned as a possible, if somewhat unpromising, candidate for a nonradiative mechanism.
Fowler William A.
Newman Michael J.
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