New Signatures in Direct Dark Matter Searches

Details New Signatures in Direct Dark Matter Searches New Signatures in Direct Dark Matter Searches

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007idm..conf...71v&link_type=abstract

THE IDENTIFICATION OF DARK MATTER. Proceedings of the Sixth International Workshop. Held 11-16 September 2006 in Rhodes, Greece.

Mathematics

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Scientific paper

The event rates for direct cold dark matter detection, both directional and non directional, are presented using a velocity distribution function obtained by considering a coupling between dark matter and dark energy. The magnitude of the effect depends on the strength κ of this new interaction relative to gravity. The resulting isothermal velocity distribution for dark matter in galaxy halos is still Maxwell-Boltzmann (M-B), but the characteristic velocity and the escape velocity are increased by √ {1 + κ 2}. We adopt a phenomenological approach and consider values of κ near unity. The phenomenological implications of such a coupling are discussed.

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