On black hole area quantization and echoes

In this work we argue that black hole (BH) area quantization of Bekenstein and Mukhanov should not give rise to measurable effects in terms of so-called gravitational wave echoes during BH mergers. We outline that the quantum spectrum of a BH should be washed out during and after BH mergers, and hence one should not expect echoes in this scenario. The extreme broadening of the spectrum is due to the large particle emission rate during ringdown. Our results question key assumptions being made in recent literature on this topic.

Automated summary

This work argues that the black hole area quantization theory proposed by Bekenstein and Mukhanov should not result in measurable gravitational wave echoes during black hole mergers. The quantum spectrum of a black hole is expected to be washed out during and after mergers, thus eliminating the possibility of echoes. The broadening of the spectrum is attributed to the high rate of particle emission during ringdown. The findings of this study question key assumptions in recent literature on this topic.