Evidence from solar seismology against non-standard solar-core models

Details Evidence from solar seismology against non-standard solar-core models Evidence from solar seismology against non-standard solar-core models

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990natur.347..536e&link_type=abstract

Nature (ISSN 0028-0836), vol. 347, Oct. 11, 1990, p. 536-539. Research supported by SERC and CAICYT.

Computer Science

Sound

54

Helioseismology, Solar Interior, Solar Oscillations, Stellar Models, Acoustic Sounding, Fine Structure, Quadrupoles, Solar Neutrinos, Stellar Cores

Scientific paper

Precision measurements of the fine structure of the solar acoustic spectrum and its variation with frequency are presented. The results agree with standard solar models and seem to remove the need for significant mixing or weakly interacting massive particles (WIMPs) in the solar core, both of which have been advanced to explain the low measured flux of solar neutrinos. This suggests that the solar neutrino problem must be resolved within neutrino physics, not solar physics.

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