Kerr Black Hole Gravitational Lensing in the Strong Deflection Limit:. AN Analytical Approach

Details Kerr Black Hole Gravitational Lensing in the Strong Deflection Limit:. AN Analytical Approach Kerr Black Hole Gravitational Lensing in the Strong Deflection Limit:. AN Analytical Approach

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1713d&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Statistics

Applications

Gravitational Lensing

Scientific paper

The caustics, critical curves and Kerr black hole shadow structure are derived from the lens equations solved by means of a perturbative approach and assuming large deflections. Starting from the Schwarzschild lens we will add terms up to the second order in the lens spin. We will focus on the degeneracy, which arises at this order of approximation, between the lens angular momentum and the height of the observer on the equatorial plane that cannot be disentangled, no matter which observable is measured. Some applications of the results will be described.

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