Abstract
We discuss gravitational lensing by elliptical galaxies with some particular mass distributions. Using simple techniques from the theory of quadrature domains and the Schwarz function (cf. [18]) we show that when the mass density is constant on confocal ellipses, the total number of lensed images of a point source cannot exceed 5 (4 bright images and 1 dim image). Also, using the Dive-Nikliborc converse of the celebrated Newton’s theorem concerning the potentials of ellipsoids, we show that “Einstein rings” must always be either circles (in the absence of a tidal shear), or ellipses.
The third author gratefully acknowledges partial support from the National Science Foundation under the grant DMS-0701873. The first and third authors are also grateful to Kavli Institute of Theoretical Physics for the partial support of their visit there in 10/2006 under the NSF grant PHY05-51164.
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Fassnacht, C., Keeton, C., Khavinson, D. (2009). Gravitational Lensing by Elliptical Galaxies, and the Schwarz Function. In: Gustafsson, B., Vasil’ev, A. (eds) Analysis and Mathematical Physics. Trends in Mathematics. Birkhäuser Basel. https://doi.org/10.1007/978-3-7643-9906-1_6
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