Epicyclic frequencies in the equatorial plane around stationary and axially symmetric wormhole geometries
arXiv:2307.03151 · doi:10.1103/PhysRevD.108.024051
Abstract
Epicyclic frequencies are usually observed in X-ray binaries and constitute a powerful astrophysical mean to probe the strong gravitational field around a compact object. We consider them in the equatorial plane around a general stationary and axially symmetric wormhole. We first search for the wormholes' existence, distinguishing them from a Kerr black hole. Once there will be available observational data on wormholes, we present a strategy to reconstruct the related metrics. Finally, we discuss the implications of our approach and outline possible future perspectives.
arXiv comment10 pages, 2 figures, 2 Tables; accepted for publication in Phys. Rev. D
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