Sun and Stars as Cosmological Tools:. Probing Supersymmetric Dark Matter

Details Sun and Stars as Cosmological Tools:. Probing Supersymmetric Dark Matter Sun and Stars as Cosmological Tools:. Probing Supersymmetric Dark Matter

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006nwap.conf..312l&link_type=abstract

NEW WORLDS IN ASTROPARTICLE PHYSICS. Proceedings of the Fifth International Workshop. Held 8-10 January 2005 in Faro, Portugal.

Physics

Scientific paper

Observational cosmology has shown that a quarter of the matter of the universe is composed by nonbaryonic dark matter. This dark matter may well constitute halos of massive and annihilating particles, weakly interacting and if so, these particles would be trapped in the interior of stars like our Sun. Whence solar evolution, in combination with helioseismic data, can provide clues as to the existence of nonbaryonic dark matter and some of their intrinsic properties. The current status of the solar standard model opens the way for using the current solar observations, namely, the neutrino flux detections and the solar acoustic data to test and probe the new physics behind the standard model of particle physics and cosmology. In this article we make a brief presentation of the physics behind the presence of dark matter inside stars.

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