Microlensing by non-compact halo objects

Details Microlensing by non-compact halo objects Microlensing by non-compact halo objects

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phla..214..232g&link_type=abstract

Physics Letters A, v. 214, p. 232-238.

Physics

36

Scientific paper

A detailed theory is developed for microlensing by non-compact dark matter objects - the neutralino stars - predicted by Gurevich and Zybin [Phys. Lett. A 208 (1995) 276]. It is shown that microlensing observations are in agreement with the theory. A method allowing one to test the presence of non-compact objects is pointed out. Among the available observational data, one case is presented where the difference between the microlensing by non-compact and compact objects is clearly seen. The size of the object determined from these observations is Rx ~= 1014 cm.

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