Classification of image distortions in terms of Petrov types

Abstract

An observer surrounded by sufficiently small spherical light sources at a fixed distance will see a pattern of elliptical images distributed over the sky, owing to the distortion effect (shearing effect) of the spacetime geometry upon light bundles. In lowest non-trivial order with respect to the distance, this pattern is completely determined by the conformal curvature tensor (Weyl tensor) at the observation event. In this paper we derive formulas that allow to calculate these distortion patterns in terms of the Newman-Penrose formalism. Then we represent the distortion patterns graphically for all Petrov types, and we discuss their dependence on the velocity of the observer.

22 pages, 8 eps-figures; revised version, parts of Introduction and Conclusions rewritten

References in corpus (5)

• Weak Gravitational Lensing
• Detection of weak gravitational lensing distortions of distant galaxies by cosmic dark matter at large scales
• Detection of Weak Gravitational Lensing by Large-scale Structure
• Image distortion from optical scalars in non perturbative gravitational lensing
• Image distortion in non perturbative gravitational lensing

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