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| Paper IPM / P / 7232 |
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| Abstract: | |
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Since one decade, the theory of gravitational microlensing entered
into the reality and some experimental groups like EROS and MACHOS
started to observe dozen of microlensing candidates towards Large
Magellanic Cloud (LMC). The interpretation of these events in the
framework of galactic models is the matter of debate. In this
article we summarize the results of experiments and the
statistical analysis and show that the known galactic models are
not able to fit with the microlensing data. The conclusion could
be either correction on the galactic models or the microlensing
events might be due to the background. Using the parallax and
finite size effects for breaking degeneracy between the lens
parameters in the Next Generation Microlensing Experiments will
certainly resolve this problem.
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