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Constraints on Central Solar Conditions from Helioseismology and Neutrino Counts

  • John Faulkner
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 123)

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.

Keywords

Sound Speed Solar Neutrino Frequency Separation Solar Model Joint Constraint 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© International Astronomical Union 1988

Authors and Affiliations

  • John Faulkner
    • 1
  1. 1.Lick ObservatoryUniversity of CaliforniaSanta CruzUSA

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