Recently, Bueno, Cano, and Hennigar [Regular black holes from pure gravity, arxiv:
2403.04827.] proposed a generic approach for incorporating an infinite tower of higher …

We compute precise values of quasinormal modes of a massive scalar field in the
background of the Schwarzschild-like brane-localised black holes. It is shown that the …

A recent development involves an intriguing model of a quantum‐corrected black hole,
established through the application of the quantum Oppenheimer–Snyder model within loop …

In this paper, we investigate quasinormal modes of scalar and electromagnetic fields in the
background of Einstein–scalar–Gauss–Bonnet (EsGB) black holes. Using the scalar and …

In this paper, we thoroughly explore two crucial aspects of a quantum Schwarzschild black
solution within four-dimensional space–time:(i) the weak deflection angle,(ii) the rigorous …

Recently, a covariant spherically symmetric model of a black hole within the framework of
loop quantum gravity (LQG), characterized by a quantum parameter r 0 or λ, has been …

As the fingerprints of black holes, quasinormal modes are closely associated with many
properties of black holes. Especially, the ringdown phase of gravitational waveforms from …

Two quantum-corrected black hole models have recently been proposed within the
Hamiltonian constraints approach to quantum gravity, maintaining general covariance\cite …

The Reissner-Nordström metric encompasses three distinct interpretations: firstly, as a
charged static black hole in the Einstein-Maxwell theory; secondly, within the brane world …

Abstract We compute the Quasi-Normal Mode (QNM) frequencies for scalar perturbations for
modified Schwarzschild black holes in Loop Quantum Gravity. We study the singularity-free …