Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-09-30
Astronomy and Astrophysics
Astrophysics
6 pages; to appear in the Proceedings of the XXth Moriond Astrophysics Meeting "Cosmological Physics with Gravitational Lensin
Scientific paper
10.1071/AS01016
There are two possible causes of variability in gravitationally lensed quasars: intrinsic fluctuations of the quasar and ``microlensing'' by compact objects along the line of sight. If disentangled from each other, microlens-induced variability can be used to study two cosmological issues of great interest: the size and brightness profile of quasars on one hand, and the distribution of compact (dark) matter along the line of sight on the other. Here we present a summary of recent observational evidence for quasar microlensing as well as of theoretical progress in the field. Particular emphasis is given to the questions which microlensing can address regarding the search for dark matter, both in the halos of lensing galaxies and in a cosmologically distributed form. A discussion of desired observations and required theoretical studies is presented as a conclusion/outlook.
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