2020
DOI: 10.48550/arxiv.2008.12244
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Deflection angle of a light ray reflected by a general marginally unstable photon sphere in a strong deflection limit

Naoki Tsukamoto

Abstract: We investigate the deflection angle in a strong deflection limit for a marginally unstable photon sphere in a general asymptotically flat, static and spherically symmetric spacetime under some assumptions to calculate observables. The deflection angle of a light ray reflected by the marginally unstable photon sphere diverges nonlogarithmically while the one reflected by a photon sphere diverges logarithmically. We apply our formula to a Reissner-Nordström spacetime and Hayward spacetime.

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Cited by 2 publications
(2 citation statements)
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“…Furthermore, it has recently been shown [25,26] that the existence of KT can be related to important characteristics of spacetime, such as photon spheres and their generalizations: fundamental photon surfaces [27][28][29][30][31][32][33][34][35][36][37][38], which are compact submanifolds paved by null geodesics. Such surfaces are important for strong gravitational lensing and black hole shadows [39][40][41][42][43][44][45][46][47][48][49][50][51]. They are equally useful in the analysis of the black hole uniqueness [52][53][54][55][56][57][58][59][60][61] and in deriving the area bounds [62][63][64].…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, it has recently been shown [25,26] that the existence of KT can be related to important characteristics of spacetime, such as photon spheres and their generalizations: fundamental photon surfaces [27][28][29][30][31][32][33][34][35][36][37][38], which are compact submanifolds paved by null geodesics. Such surfaces are important for strong gravitational lensing and black hole shadows [39][40][41][42][43][44][45][46][47][48][49][50][51]. They are equally useful in the analysis of the black hole uniqueness [52][53][54][55][56][57][58][59][60][61] and in deriving the area bounds [62][63][64].…”
Section: Introductionmentioning
confidence: 99%
“…This purely geometric property can serve as a constructive definition for analyzing photon surfaces instead of solving geodesic equations and plays a decisive role in the analysis of the black hole uniqueness [24][25][26][27][28][29][30][31][32][33] and area bounds [34][35][36]. Photon surfaces find applications in the description of optical properties and gravitational shadows [37][38][39][40][41][42][43][44][45][46][47].…”
Section: Introductionmentioning
confidence: 99%