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Abstract
1Introduction
2Lensing in Arbitrary Spacetimes
2.1Light cone and exact lens map
2.2Wave fronts
2.3Optical scalars and Sachs equations
2.4Distance measures
2.5Image distortion
2.6Brightness of images
2.7Conjugate points and cut points
2.8Criteria for multiple imaging
2.9Fermat’s principle for light rays
3Lensing in Globally Hyperbolic Spacetimes
3.1Criteria for multiple imaging in globally hyperbolic spacetimes
3.2Wave fronts in globally hyperbolic spacetimes
3.3Fermat’s principle and Morse theory in globally hyperbolic spacetimes
3.4Lensing in asymptotically simple and empty spacetimes
4Lensing in Spacetimes with Symmetry
4.1Lensing in conformally flat spacetimes
4.2Lensing in conformally stationary spacetimes
4.3Lensing in spherically symmetric and static spacetimes
4.4Lensing in axisymmetric stationary spacetimes
5Examples
5.1Schwarzschild spacetime
5.2Kottler spacetime
5.3Reissner-Nordström spacetime
5.4Morris-Thorne wormholes
5.5Barriola-Vilenkin monopole
5.6Janis-Newman-Winicour spacetime
5.7Boson and fermion stars
5.8Kerr spacetime
5.9Rotating disk of dust
5.10Straight spinning string
5.11Plane gravitational waves
6Acknowledgements
open ReferencesReferences
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