The optical geometry definition of the total deflection angle of a light ray in curved spacetime

DOI10.1088/1475-7516/2021/08/028zbMath1492.83024arXiv2006.13435OpenAlexW3125990092MaRDI QIDQ5070233

Hideyoshi Arakida

Publication date: 11 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2006.13435

zbMATH Keywords

gravitydark energy theory

Mathematics Subject Classification ID

Black holes (83C57) Diffraction, scattering (78A45) Electromagnetic fields in general relativity and gravitational theory (83C50) Lasers, masers, optical bistability, nonlinear optics (78A60) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Dark matter and dark energy (83C56)

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Cites Work

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• Classical tests of general relativity in the Newtonian limit of the Schwarzschild-de Sitter spacetime
• The cosmological constant and the gravitational light bending
• Light deflection and Gauss-Bonnet theorem: definition of total deflection angle and its applications
• Optical reference geometry for stationary and static dynamics
• Bergman-Vekua theory in differential form
• The relevance of the cosmological constant for lensing
• An online interactive geometric database including exact solutions of Einstein's field equations
• A NOTE ON THE EFFECT OF THE COSMOLOGICAL CONSTANT ON THE BENDING OF LIGHT
• Applications of the Gauss–Bonnet theorem to gravitational lensing
• DOES THE COSMOLOGICAL TERM INFLUENCE GRAVITATIONAL LENSING?
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae