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Role ofΛin the Cosmological Lens Equation

2008/07/31 by M. Sereno · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Physics #Solar and Space Plasma Dynamics #astro-ph #gr-qc

paper · pdf · doi:10.1103/physrevlett.102.021301

published as Phys.Rev.Lett.102:021301,2009 · 4 pages. (Univ. Zuerich); v2: presentation improved, discussion extended, references to papers posted after the v1-version added. In press on Phys. Rev. Lett

arxiv created 2008/10/30 · openalex publication_date 2009/01/14 · arxiv updated 2009/12/01 · openalex created_date 2016/08/23 · openalex updated_date 2026/08/05

Abstract

The cosmological constant \ensuremathΛ affects cosmological gravitational lensing. Effects due to \ensuremathΛ can be studied in the framework of the Schwarzschild--de Sitter spacetime. Two novel contributions, which cannot be accounted for by a proper use of angular diameter distances, are derived. First, a term \ensuremathδ\stackrel^\ensuremathα_\ensuremathΛ=2mb\ensuremathΛ/3 has to be added to the bending angle, where m is the lens mass and b the impact parameter. Second, \ensuremathΛ brings about a difference in the redshifts of multiple images. Both effects are quite small for real astrophysical systems, \ensuremathδ\stackrel^\ensuremathα_\ensuremathΛ\ensuremath\lesssim1\ensuremathμarcsec and \ensuremathΔzs\ensuremath\lesssim10^\ensuremath-7.

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