Light bending by the cosmological constant

DOI10.1088/1475-7516/2022/02/009zbMath1487.83063arXiv2109.09785OpenAlexW4210710898MaRDI QIDQ5063477

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Publication date: 21 March 2022

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

Full work available at URL: https://arxiv.org/abs/2109.09785

zbMATH Keywords

gravitygravitational lensingweak gravitational lensingdark energy experiments

Mathematics Subject Classification ID

Diffraction, scattering (78A45) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Electromagnetic fields in general relativity and gravitational theory (83C50) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Geodesics in global differential geometry (53C22) Dark matter and dark energy (83C56)

Related Items (1)

Total light bending in non-asymptotically flat black hole spacetimes

Uses Software

• SciPy

Cites Work

• Cosmological constant and lensing
• Strong lensing in the Einstein-Straus solution
• A family of embedded Runge-Kutta formulae
• The relevance of the cosmological constant for lensing
• Effect of accelerated global expansion on the bending of light
• DOES THE COSMOLOGICAL TERM INFLUENCE GRAVITATIONAL LENSING?
• Light bending in Schwarzschild–de Sitter: projective geometry of the optical metric

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