WIMPs and solar evolution code

Details WIMPs and solar evolution code WIMPs and solar evolution code

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..128...21g&link_type=abstract

(IAU, The Inside the Sun Colloquium, 121st, Versailles, France, May 22-26, 1989) Solar Physics (ISSN 0038-0938), vol. 128, July

Astronomy and Astrophysics

Astrophysics

9

Dark Matter, Nuclear Astrophysics, Solar Neutrinos, Stellar Evolution, Weak Interactions (Field Theory), Chlorine, Radiation Detectors, Stellar Models

Scientific paper

The Saclay solar evolution code is used to check the effect of WIMPs on
solar evolution. This paper examines the effects of various types of
Cosmion-matter interactions, gives constraints on the cross-sections
compatible with the measured neutrino rate of 2 SNU on chlorine, and
relates these constraints to ongoing dark matter detection experiments.

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