The Galactic Dark Matter: Predictions and Obsevations

Details The Galactic Dark Matter: Predictions and Obsevations The Galactic Dark Matter: Predictions and Obsevations

1997-04-13

arxiv.org/abs/astro-ph/9704115v1

Astrophys.Space Sci. 257 (1998) 271

Astronomy and Astrophysics

Astrophysics

14 pages 1 figure

Scientific paper

10.1023/A:1001108212691

After two decades of efforts to identify the enigmatic dark matter that comprises the dominant form of matter in our galaxy, the mass range for viable candidates appears to have been reduced by more than 50 orders of magnitude. Positive results have thus far been confined to the range: 10-7 Mo to 1.0 Mo, with apparent clustering within the ranges 10-5 Mo to 10-3 Mo and 0.08 Mo to 0.5 Mo. Positive and negative results are compared with specific predictions of cosmological models.

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