Contribution of the cosmological constant to the relativistic bending of light revisited
By W. Rindler, M. Ishak. 2007
177 citations recorded by the source corpus.
We study the effect of the cosmological constant $\ensuremath{\Lambda}$ on the bending of light by a concentrated spherically symmetric mass. Contrarily to previous claims, we show that, when the Schwarzschild-de Sitter geometry is taken into account, $\ensuremath{\Lambda}$ does indeed contribute to the bending.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/02aef741e9be327e04238aa25966c7bc28c6dc5b
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In Astronomy and Astrophysics
- O. Tsupko
- G. Bisnovatyi-Kogan
- V. Perlick
- M. Bartelmann
- Sushant G. Ghosh
- Rahul Kumar
- M. Werner
- A. Rogers
In Nuclear and High Energy Physics
Citations in the corpus
- Gravitational lensing (2010, background): “Loosely related in this context, arguments that the cosmological constant might measurably affect gravitational lensing by isolated objects [407] were refuted in [455].”
- Black holes with scalar hair in light of the Event Horizon Telescope (2020, unknown): “The angle ψ is given by [179]:”
- Calculating black hole shadows: Review of analytical studies (2021, background): “A 97 (1983) 239 [206] W. Rindler, M. Ishak, Contribution of the cosmological constant to the relativistic bending of light revisited, Phys.”
- Black hole shadow in an expanding universe with a cosmological constant (2018, background): “However, it was realized by Rindler and Ishak [13] that this is not true: Although the coordinate representation of the lightlike geodesics is unaffected by Λ, the cosmological constant does influence the lensing features because it changes the angle measurements.”