English

Basic Elements of Strong Gravitational Lensing

Cosmology and Nongalactic Astrophysics 2025-05-30 v1

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.

Keywords

Cite

@article{arxiv.2505.22738,
  title  = {Basic Elements of Strong Gravitational Lensing},
  author = {Paul L. Schechter and Jeremy D. Schnittman},
  journal= {arXiv preprint arXiv:2505.22738},
  year   = {2025}
}

Comments

Comments: 28 pages, 15 figures. Contribution to ISSI conference on"Strong Gravitational Lensing." Accepted 2 May 2025 Space Sci. Rev

R2 v1 2026-07-01T02:47:09.171Z