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Constraints on central solar conditions from helioseismology and neutrino counts
Published online by Cambridge University Press: 03 August 2017
Abstract
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Interesting joint constraints are placed on central solar conditions by the solar neutrino detection rate and the frequency separations of high-order, low-degree p-modes of pulsation. A new form of diagnostic diagram is introduced that illustrates the difficulty in standard theories of simultaneously satisfying these joint constraints. A model employing WIMPs (= weakly interacting massive particles) appears to be the only model extant capable of fitting both kinds of data. Unambiguous identification and fitting of g-modes can provide a further test of the WIMP model provided a certain caution is exercised.
- Type
- Chapter 2: Theory of Solar Oscillations
- Information
- Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 105 - 109
- Copyright
- Copyright © Reidel 1988
References
Cleveland, B.T., Davis, R. and Rowley, J.K.
1984, in Resonance Ionization Spectroscopy 1984 (eds. Hurst, G.S. and Payne, M.G.; Institute of Physics Conf. Ser. 71, Bristol), p. 241.Google Scholar
Schatzman, E., Maeder, A., Angrand, F. and Glowinski, R.
1981, Astron. Astrophys.
96, 1.Google Scholar
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