Dark matter

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Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nyasa.571..298s&link_type=abstract

(NASA, NSF, Texas Academy of Science, et al., Texas Symposium on Relativistic Astrophysics, 14th, Dallas, TX, Dec. 11-16, 1988)

Astronomy and Astrophysics

Astrophysics

1

Baryons, Dark Matter, Elementary Particle Interactions, Missing Mass (Astrophysics), Neutrinos, Halos, Intergalactic Media

Scientific paper

The evidence for the existence of dark matter in the universe is reviewed; the different classes of particles proposed to account for the 'missing mass' are briefly characterized; and the current status of efforts to detect these particles is surveyed. The emphasis is on the problem of Galactic dark matter and its detection. Consideration is given to baryons, black holes, neutrinos, axions, and the weakly interacting massive particles predicted by supersymmetry models (photinos, higgsinos, zinos, and solar cosmions).

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