Detecting dark matter via microlensing

Details Detecting dark matter via microlensing Detecting dark matter via microlensing

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..243.1080g&link_type=abstract

Intersections between particle and nuclear physics. AIP Conference Proceedings, Volume 243, pp. 1080-1085 (1992).

Physics

Nuclear Physics

Scientific paper

Gravitational microlensing of stars in the nearby LMC galaxy is
discussed as a method of detecting baryonic dark matter in the halo of
our Galaxy, if it consists of objects in the 10-6 to 100Msolar mass
range. The progress of the MACHO collaboration observing program is
described.

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