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Particle motion around a static axially symmetric wormhole

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arxiv 2105.09174 v2 pith:JCIZG77W submitted 2021-05-19 gr-qc

Bakhtiyor Narzilloev , Daniele Malafarina , Ahmadjon Abdujabbarov , Bobomurat Ahmedo , Cosimo Bambi This is my paper · ORCID
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keywords motionwormholeblackparticleaxiallydistinguishholestatic
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We consider the properties of a static axially symmetric wormhole described by an exact solution of Einstein's field equations and investigate how we can distinguish such a hypothetical object from a black hole. To this aim, we explore the motion of test particles and photons in the wormhole's space-time and compare it with the particle dynamics in the well known space-times of Schwarzschild and Kerr black holes. We show that precise simultaneous measurement of test particle motion and photon motion may provide the means to distinguish the wormhole geometry from that of a black hole.

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  1. Constraining quadrupole deformations with relativistic effects

    gr-qc 2025-06 reject novelty 6.0 of 10

    In the Zipoy-Voorhees spacetime, the Shapiro time delay and the Shirokov oscillation frequencies acquire corrections from the quadrupole deformation parameter q, with the delay correction appearing at first order in q.

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