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声学史瓦西黑洞的引力弯曲。

The gravitational bending of acoustic Schwarzschild black hole.

作者信息

Qiao Chen-Kai, Zhou Mi

机构信息

College of Science, Chongqing University of Technology, Banan, Chongqing, 400054 China.

出版信息

Eur Phys J C Part Fields. 2023;83(4):271. doi: 10.1140/epjc/s10052-023-11376-3. Epub 2023 Apr 2.

Abstract

Acoustic black hole is becoming an attractive topic in recent years, for it open-up new direction for experimental/observational explorations of black holes. In this work, the gravitational bending of acoustic Schwarzschild black hole is investigated. The gravitational deflection angle of particles traveling along null geodesics, weak gravitational lensing and Einstein ring for acoustic Schwarzschild black hole are carefully studied and analyzed. Particularly, in the calculation of gravitational deflection angle, we resort to two approaches-the Gauss-Bonnet theorem and the geodesic method. The results show that the gravitational bending effect in acoustic Schwarzschild black hole is enhanced, compared with conventional Schwarzschild black hole. This result indicates that the acoustic black holes may be more easily detectable in gravitational bending effects and weak gravitational lensing observations.

摘要

近年来,声学黑洞正成为一个引人关注的课题,因为它为黑洞的实验/观测探索开辟了新方向。在这项工作中,我们研究了声学史瓦西黑洞的引力弯曲。仔细研究并分析了沿类光测地线传播的粒子的引力偏转角、声学史瓦西黑洞的弱引力透镜效应和爱因斯坦环。特别地,在引力偏转角的计算中,我们采用了两种方法——高斯-博内定理和测地线方法。结果表明,与传统史瓦西黑洞相比,声学史瓦西黑洞中的引力弯曲效应增强了。这一结果表明,在引力弯曲效应和弱引力透镜观测中,声学黑洞可能更容易被探测到。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8ab4/10067517/2a733ac9391e/10052_2023_11376_Fig1_HTML.jpg

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