Abstract
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.
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© 1988 International Astronomical Union
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Faulkner, J. (1988). Constraints on Central Solar Conditions from Helioseismology and Neutrino Counts. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_22
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DOI: https://doi.org/10.1007/978-94-009-4009-3_22
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-2615-5
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