Tidal heating in a binary black hole system is driven by the absorption of energy and angular
momentum by the black hole's horizon. Previous works have shown that this phenomenon …

We study the tidal deformability of horizonless exotic compact objects, with implications for
area quantized black holes. Since, any such horizonless compact object, including an area …

We study the potential of gravitational wave astronomy to observe the quantum aspects of
black holes with tidal heating. According to Bekenstein's quantization, we find that black hole …

This article assesses Landauer's principle from information theory in the context of area
quantization of the Schwarzschild black hole. Within a quantum-mechanical perspective …

A classical black hole is characterized by a horizon that absorbs the radiation of all
frequencies incident on it. The perturbation of these black holes is well understood via …

Black hole echo is an important observable that can help us better understand gravitational
theories. The non-linear electrodynamic black holes can admit multi-horizon, and the …

We propose a new approach toward reconstructing the late-time near-horizon geometry of
merging binary black holes, and toward computing gravitational-wave echoes from exotic …

We investigate the ergoregion instability of area-quantized rotating quantum black holes
(QBH) under gravitational perturbation. We show that the instability can be avoided in binary …

In the black hole perturbation theory framework, two different physical pictures for echoes in
compact objects have been proposed. The first mechanism interprets echoes as repeated …

We assess the prospects for detecting gravitational wave echoes arising due to the quantum
nature of black hole horizons with LISA. In a recent proposal, Bekenstein's black hole area …