期刊
PHYSICAL REVIEW D
卷 104, 期 12, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.104.124010
关键词
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资金
- China Scholarship Council
- China Postdoctoral Science Foundation [2019M660278, 2020T130020]
- National Natural Science Foundation of China [11905157, 11935009]
The study presents a distinct shadow mechanism from the asymmetric thin-shell wormhole and investigates the appearance of an accretion disk around it. The analysis reveals additional photon rings and a potential lensing band between highly demagnified photon rings, providing an observational signature to distinguish asymmetric thin-shell wormholes from black holes.
Recently, a distinct shadow mechanism was proposed by Wang et al. from the asymmetric thin-shell wormhole (ATW) [X. Wang et aL, Phys. Lett. B 811, 135930 (2020)]. On the other hand, Gralla, Holz, and Wald's work [Phys. Rev. D 100, 024018 (2019)] represented a nice description of photon rings in the presence of an accretion disk around a black hole. In this paper, we are inspired to thoroughly investigate the observational appearance of an accretion disk around the ATW. Although the spacetime outside an ATW with a throat could be identical to that containing a black hole with its event horizon, we show evident additional photon rings from the ATW spacetime. Moreover, a potential lensing band between two highly demagnified photon rings is found. Our analysis provides an optically observational signature to distinguish ATWs from black holes.
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