Astronomical limits on the nature of the dark matter

Details Astronomical limits on the nature of the dark matter Astronomical limits on the nature of the dark matter

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..222..481s&link_type=abstract

In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 19

Astronomy and Astrophysics

Astronomy

1

Baryons, Black Holes (Astronomy), Dark Matter, Dwarf Galaxies, Gravitational Lenses, Neutrinos, Anisotropy, Particle Mass, Weak Interactions (Field Theory)

Scientific paper

Astronomical observations can constrain, and potentially detect, the nature of the dark matter. Baryonic dark matter or black holes can be detected through their microlensing of stars in nearby galaxies. Dwarf galaxies serve as a laboratory for searches for dark matter. WIMPS can be potentially detected through annihilation in stars. The current limits on axions from supernovae and cosmology may rule out these particles as dark matter candidates.

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