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Do Solar Models with Weakly Interacting Massive Particles Reproduce the Stanford Seismic Data?

  • A. N. Ellis
  • D. O. Gough
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 123)

Abstract

The discrepancy between theoretical eigenfrequencies of standard solar models and the frequencies of solar modes of degree between 2 and 5 measured at Stanford is degree-independent for cyclic frequencies above about 2 mHz. Below that frequency the discrepancy for dotriacontapole modes diverges from that of the modes of lower degree. The differences between eigenfrequencies of a simple solar model containing a cloud of weakly interacting particles in its core and of one without do not reproduce this behaviour.

Keywords

Massive Particle Convection Zone Cyclic Frequency Solar Mode Solar Model 
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

  • A. N. Ellis
    • 1
  • D. O. Gough
    • 1
  1. 1.Department of Applied Mathematics and Theoretical Physics, and Institute of AstronomyUniversity of CambridgeUK

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