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Updated: Feb 17, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Weak Gravitational Lensing of Finite Beams
Pierre Fleury1, Julien Larena2, Jean-Philippe Uzan3
1Départment de Physique Théorique, Université de Genève, 24 quai Ernest-Ansermet, 1211 Genève 4, Switzerland.
This study introduces a new formalism for weak gravitational lensing, moving beyond the infinitesimal light beam approximation. It resolves the Ricci-Weyl problem, showing convergence depends on enclosed matter and enhancing shear for finite beams, impacting lensing survey interpretations.
Area of Science:
- Astrophysics
- Cosmology
- Gravitational Lensing
Background:
- Standard weak gravitational lensing theory uses the infinitesimal light beam approximation.
- This approximation leads to the unphysical Ricci-Weyl problem, where lensing sources depend on matter distribution resolution.
Purpose of the Study:
- To develop a strong-lensing-inspired formalism for finite light beams.
- To address and resolve the Ricci-Weyl problem within gravitational lensing theory.
Main Methods:
- Proposed a new theoretical framework for analyzing gravitational lensing of finite beams.
- Applied this formalism to investigate the relationship between matter distribution and lensing effects.
Main Results:
- Demonstrated that convergence is determined by the matter enclosed within the beam, independent of its distribution.
- Showed that shear is systematically enhanced for finite beams.
- Established that the Kaiser-Squires relation between shear and convergence is violated.
Conclusions:
- The findings challenge the standard weak lensing approximation.
- The violation of the Kaiser-Squires relation has significant implications for interpreting weak-lensing survey data.
- A revised understanding of gravitational lensing is needed for finite beams.
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