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    Circular orbit of a particle and weak gravitational lensing

    Zonghai Li1,*, Guodong Zhang2,†, and Ali Övgün3,‡

    • 1MOE Key Laboratory of Artificial Micro- and Nano-structures, School of Physics and Technology, Wuhan University, Wuhan 430072, China
    • 2Chengguan Middle School, LuoNan 726100, China
    • 3Physics Department, Arts and Sciences Faculty, Eastern Mediterranean University, Famagusta, North Cyprus 99628 via Mersin 10, Turkey

    • *lzh@my.swjtu.edu.cn
    • †yashangluzhu@snnu.edu.cn
    • ‡ali.ovgun@emu.edu.tr

    Phys. Rev. D 101, 124058 – Published 26 June, 2020

    DOI: https://doi.org/10.1103/PhysRevD.101.124058

    Abstract

    The purpose of this paper is twofold. First, we introduce a geometric approach to study the circular orbit of a particle in static and spherically symmetric spacetime based on Jacobi metric. Second, we apply the circular orbit to study the weak gravitational deflection of null and timelike particles based on Gauss-Bonnet theorem. By this way, we obtain an expression of deflection angle and extend the study of deflection angle to asymptotically nonflat black hole spacetimes. Some black holes as lens are considered such as a static and spherically symmetric black hole in the conformal Weyl gravity and a Schwarzschild-like black hole in bumblebee gravity. Our results are consistent with the previous literature. In particular, we find that the connection between Gaussian curvature and the radius of a circular orbit greatly simplifies the calculation.

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