WIMP direct detection: astrophysical input

Details WIMP direct detection: astrophysical input WIMP direct detection: astrophysical input

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005newar..49..181g&link_type=abstract

New Astronomy Reviews, v. 49, iss. 2-6 [SPECIAL ISSUE], p. 181-184.

Astronomy and Astrophysics

Astronomy

Scientific paper

The WIMP direct detection event rate (and in particular its annual modulation) depends on the local dark matter distribution and also the Earth’s velocity with respect to the Galactic rest frame. I discuss the effect of these astrophysical inputs on the expected WIMP signals, focussing on exclusions limits and the size and phase of the annual modulation signal.

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