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Excitation of the Solar Oscillations by Objects Consisting of y-Matter*

Published online by Cambridge University Press:  12 April 2016

S. I. Blinnikov
Affiliation:
Institute of Theoretical and Experimental Physics, Moscow, U.S.S.R.
M. Yu. Khlopov
Affiliation:
Institute of Applied Mathematics, Academy of Sciences, Moscow, U.S.S.R.

Abstract

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Modern development of particle physics makes it probable that new, still undiscovered, particles exist interacting with the ordinary matter by means of gravitation only. Okun suggested to call such particles the y-particles and to call the matter consisting of them the y-matter. We show that planet-like object orbiting inside the Sun and consisting of y-matter may explain 160 min nonradial solar oscillations.

Type
Research Article
Copyright
Copyright © Reidel 1983

Footnotes

*

Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.

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