On an alternative mechanism for the black hole echoes
Hang Liu, Wei-Liang Qian, Yunqi Liu, Jian-Pin Wu, Bin Wang, and Rui-Hong Yue

TL;DR
This paper proposes an alternative mechanism for black hole echoes based on a discontinuity in the black hole metric, supported by numerical and analytical analysis, with implications for understanding quantum gravity and astrophysical observations.
Contribution
It introduces a novel mechanism for black hole echoes involving metric discontinuities, expanding the theoretical framework and providing analytical and numerical evidence.
Findings
Echoes persist even with distant and weak discontinuities.
The period of echoes relates to the pole spacing in quasinormal modes.
Discontinuities modify the asymptotic behavior of quasinormal frequencies.
Abstract
Gravitational wave echoes from the black holes have been suggested as a crucial observable to probe the spacetime in the vicinity of the horizon. In particular, it was speculated that the echoes are closely connected with specific characteristics of the exotic compact objects, and moreover, possibly provide an access to the quantum nature of gravity. Recently, it was shown that the discontinuity in the black hole metric substantially modifies the asymptotical behavior of quasinormal frequencies. In the present study, we proceed further and argue that a discontinuity planted into the metric furnishes an alternative mechanism for the black hole echoes. Physically, the latter may correspond to an uneven matter distribution inside the surrounding halo. To demonstrate the results, we first numerically investigate the temporal evolution of the scalar perturbations around a black hole that…
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