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Observational properties of coherent quantum black holes
We consider null and timelike geodesics around a spherically symmetric, nonrotating coherent quantum black hole (CQBH). The classical limit of the geometry of a CQBH departs from that of the Schwarzschild spacetime at short scales and depends on one parameter Rs which can be interpreted as the physical radius of the “quantum” core. We study circular orbits, photon rings, and lensing effects and compare them with the Schwarzschild metric.
Constraining deviations from spherical symmetry using $\ensuremath{\gamma}$-metric
Abstract The γ-spacetime metric is a static and axially symmetric vacuum solution of the Einstein equation. This spacetime represents a naked singularity and it has an extra parameter γ which signifies deviations from spherical symmetry. In this work, we study the possibility of constraining the deformation parameter with astrophysical observations.
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