The Contribution of the Cosmological Constant to the Relativistic Bending of Light Revisited
arXiv:0709.2948 · doi:10.1103/PhysRevD.76.043006
Abstract
We study the effect of the cosmological constant 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, does indeed contribute to the bending.
5 pages, 2 figures
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