Do gravitational lenses always magnify?

Talk for the general ASTRON/JIVE colloquium, 28 June 2007

O. Wucknitz [1]

  1. Joint Institute for VLBI in Europe, Postbus 2, 7990 AA Dwingeloo, Netherlands

Abstract

[ paper abstract ]
We discuss the classic theorem according to which a gravitational lens always produces at least one image with a magnification greater than unity. This theorem seems to contradict the conservation of total flux from a lensed source. The standard solution to this paradox is based on the exact definition of the reference 'unlensed' situation, in which the lens mass can either be removed or smoothly redistributed.

We calculate magnifications and amplifications (in photon number and energy flux density) for general lensing scenarios not limited to regions close to the optical axis. In this way the formalism is naturally extended from tangential planes for the source and lensed images to complete spheres. We derive the lensing potential theory on the sphere and find that the Poisson equation is modified by an additional source term that is related to the mean density and to the Newtonian potential at the positions of observer and source. This new term generally reduces the magnification and violates the theorem far from the optical axis, ensuring conservation of the total photon number received on a sphere around the source.

By exchanging source and observer, we confirm that magnification and amplification differ according to Etherington's reciprocity law, so that surface brightness is no longer strictly conserved. At this level we also have to distinguish between different surface brightness definitions that are based on photon number, photon flux, and energy flux.

Key words: Gravitational lensing -- Cosmology: miscellaneous

This is the abstract for my paper about the subject. For more details, click here.




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