2011
DOI: 10.1007/s10714-011-1186-6
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The cosmological constant and the gravitational light bending

Abstract: The solution of the null non-radial geodesic in a Schwarzschild-de Sitter background is revisited. The gravitational bending of a light ray is affected by the cosmological constant, in agreement with the findings of some previous investigations. The present study confirms that the leading correction term depends directly not only on Λ but also on the impact parameter and on the angular distance to the source. Using the resulting lens equation, the projected mass of the lens was estimated for several systems di… Show more

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Cited by 35 publications
(46 citation statements)
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References 14 publications
(29 reference statements)
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“…The Equation (25) is similar and comparable with previous results, that is, the third term of Equation (13) in [20], and the fourth term of Equation (25) in [22].…”
Section: Effect Of the Cosmological Constant On Light Deflectionsupporting
confidence: 89%
See 3 more Smart Citations
“…The Equation (25) is similar and comparable with previous results, that is, the third term of Equation (13) in [20], and the fourth term of Equation (25) in [22].…”
Section: Effect Of the Cosmological Constant On Light Deflectionsupporting
confidence: 89%
“…Our result seems to be similar and comparable with the third term of Equation (13) in [20], and the fourth term of Equation (25) in [22]. Also, as [13,14,[20][21][22]24,25], the cosmological constant leads to diminishing the bending angle due to the mass of the central body M.…”
supporting
confidence: 84%
See 2 more Smart Citations
“…We expect that different lens density profiles would lead to different results in the mass estimates also from the point of view of the cosmological corrections, as shown in Ref. [10] for the case of the Kottler metric. Figure A1.…”
Section: Discussionmentioning
confidence: 80%