Microlensing by the non-compact invisible bodies

Details Microlensing by the non-compact invisible bodies Microlensing by the non-compact invisible bodies

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phla..219..199s&link_type=abstract

Physics Letters A, v. 219, p. 199-204.

Physics

19

Scientific paper

The observation of microlensing events toward the Large Magellanic Cloud has led to the discovery of a new population of our Galaxy which consists of dark bodies with a mass of the order of 0.1 Msolar. The nature of these objects is still unknown, though the most reliable hypothesis is that they are brown dwarfs. Other hypotheses include mirror stars, black holes, and exotic stars which consist of cold dark matter particles. The last hypothesis is attractive from the point of view of modern particle physics. It says that at least part of the dark body population can consist of these objects. Here we discuss the possibility of explaining the current observational data in the framework of this hypothesis. Our conclusion is that the current observational data indicate that at least two events from the seven events of OGLE data can be explained in the framework of this hypothesis.

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