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Basic Elements of Strong Gravitational Lensing

Author(s)
Schechter, Paul L.; Schnittman, Jeremy D.
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Abstract
Even when used to describe the same phenomenon, equations, graphics and words each give different perspectives and lead to complementary insights. The basic elements of strong gravitational lensing are introduced here favoring words and graphics over equations whenever possible. Fermat’s principle is the fundamental driver of strong lensing. Three “D’s” encapsulate the essential effects of lensing: Delay, Deflection and Distortion. Gravity and geometry both contribute to the delay of photons from a lensed source. Their interplay determines how the images of a source are deflected and how they are stretched or compressed. Caustics and critical curves are explained. Images of doubly, triply, quadruply and quintuply lensed sources are displayed. A table of symbols, their definitions and distinctions provides a summary of the basic elements of strong lensing.
Date issued
2025-05-30
URI
https://hdl.handle.net/1721.1/163660
Department
Massachusetts Institute of Technology. Department of Physics; MIT Kavli Institute for Astrophysics and Space Research
Journal
Space Science Reviews
Publisher
Springer Netherlands
Citation
Schechter, P.L., Schnittman, J.D. Basic Elements of Strong Gravitational Lensing. Space Sci Rev 221, 49 (2025).
Version: Final published version

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