Light Deflection and Gauss-Bonnet Theorem: Definition of Total Deflection Angle and its Applications
arXiv:1708.04011 · doi:10.1007/s10714-018-2368-2
Abstract
In this paper, we re-examine the light deflection in the Schwarzschild and the Schwarzschild-de Sitter spacetime. First, supposing a static and spherically symmetric spacetime, we propose the definition of the total deflection angle of the light ray by constructing a quadrilateral on the optical reference geometry determined by the optical metric . On the basis of the definition of the total deflection angle and the Gauss-Bonnet theorem, we derive two formulas to calculate the total deflection angle ; (i) the angular formula that uses four angles determined on the optical reference geometry or the curved subspace being a slice of constant time and (ii) the integral formula on the optical reference geometry which is the areal integral of the Gaussian curvature in the area of a quadrilateral and the line integral of the geodesic curvature along the curve . As the curve , we introduce the unperturbed reference line that is the null geodesic on the background spacetime such as the Minkowski or the de Sitter spacetime, and is obtained by projecting vertically onto the curved subspace . We demonstrate that the two formulas give the same total deflection angle for the Schwarzschild and the Schwarzschild--de Sitter spacetime. In particular, in the Schwarzschild case, the result coincides with Epstein--Shapiro's formula when the source and the receiver of the light ray are located at infinity. In addition, in the Schwarzschild--de Sitter case, there appear order terms in addition to the Schwarzschild-like part, while order terms disappear.
23 pages, 7 figures
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