Particle dark matter and its indirect detection

Details Particle dark matter and its indirect detection Particle dark matter and its indirect detection

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998newar..42..245b&link_type=abstract

New Astronomy Reviews, Volume 42, Issue 3-4, p. 245-257.

Astronomy and Astrophysics

Astronomy

7

Scientific paper

The need for dark matter is briefly reviewed. A wealth of observational information points to the existence of a non-baryonic component. To the theoretically favoured candidates today belong axions, supersymmetric particles, and to some extent massive neutrinos. The theoretical foundation and experimental situation for each of these are examined. In particular, indirect detection methods of supersymmetric dark matter are described. Present experiments are just reaching the required sensitivity to discover or rule out some of these candidates, and major improvements are planned over the next few years.

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