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A. O. Petters, B. Rider, and A. M. Teguia
From first principles, we initiate the development of a mathematical theory of stochastic microlensing—a central tool in probing dark matter on galactic scales. The results of this paper are relevant to the theory of random fields and provide a platform for further generalizations as well as analytical limits for checking astrophysical studies of stochastic microlensing.
J. Math. Phys. 50, 072503 (2009) |
