Weak deflection angle of a dirty black hole
arXiv:2003.00764 · doi:10.1016/j.cjph.2020.06.015
Abstract
In this paper, we present the weak deflection angle in a Schwarzschild black hole of mass surrounded by the dark matter of mass and thickness . The Gauss-Bonnet theorem, formulated for asymptotic spacetimes, is found to be ill-behaved in the third-order of for very large . Using the finite-distance for the radial locations of the source and the receiver, we derived the expression for the weak deflection angle up to the third-order of using Ishihara (\textit{et al.}) method. The result showed that the required dark matter thickness is for the deviations in the weak deflection angle to occur. Such thickness requirement is better by a factor of 2 as compared to the deviations in the shadow radius (). It implies that the use of the weak deflection angle in detecting dark matter effects in one's galaxy is better than using any deviations in the shadow radius.
arXiv comment6 pages, 1 figure; expressions in section 4 simplified thoroughly; accepted for publication in Chinese Journal of Physics
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