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Coalescing massive black hole binaries are produced by the mergers of galaxies. The final stages of the black hole coalescence produce strong gravitational radiation that can be detected by the space-borne LISA. In cases where the black…

The instability of rotating Kerr black holes due to massive scalar perturbations is investigated. It is well known that a bosonic field impinging on a Kerr black hole can be amplified as it scatters off the hole. This superradiant…

General Relativity and Quantum Cosmology · Physics 2015-06-05 Shahar Hod

Photons propagating in a plasma acquire an effective mass $\mu$, which is given by the plasma frequency and which scales with the square root of the plasma density. As noted previously by Conlon and Herdeiro, for electron number densities…

General Relativity and Quantum Cosmology · Physics 2020-08-07 Alexandru Dima , Enrico Barausse

Massive bosonic fields in the background of a Kerr black hole can either trigger superradiant instabilities (black-hole bombs) or form equilibrium configurations corresponding to pure bound states, known as stationary scalar clouds. Here,…

General Relativity and Quantum Cosmology · Physics 2021-02-10 Marzena Ciszak , Francesco Marino

Gravitational signatures of black hole superradiance are a unique probe of ultralight particles that are weakly-coupled to ordinary matter. The existence of an ultralight boson would lead spinning black holes with size comparable to the…

General Relativity and Quantum Cosmology · Physics 2023-05-03 Nils Siemonsen , Taillte May , William E. East

We study the evaporation of black holes in space-times with extra dimensions of size L. We first obtain a description which interpolates between the expected behaviors of very large and very small black holes and then show that the…

High Energy Physics - Theory · Physics 2008-11-26 Roberto Casadio , Benjamin Harms

Relativistic axions are good candidates for the dark radiation for which there are mounting observational hints. The primordial decays of heavy fields produce axions which are ultra-energetic compared to thermalised matter and inelastic…

High Energy Physics - Phenomenology · Physics 2015-06-15 Joseph P. Conlon , M. C. David Marsh

In this work, we study the luminosity that results from the conversion of QCD axion particles into photons in the magnetic field of the plasma accreting onto black holes (BHs). For the luminosities to be large two conditions need to be met:…

High Energy Physics - Phenomenology · Physics 2024-04-22 Ricardo Z. Ferreira , Ángel Gil Muyor

Detection of gravitational waves (GWs) paves the beginning of a new era of gravitational wave astronomy. Black holes (BHs) in their ringdown phase provide the cleanest signal of emitted GWs that imprint the fundamental nature of BHs under…

General Relativity and Quantum Cosmology · Physics 2025-10-28 Rajesh Karmakar , Debaprasad Maity

Kerr Sen black holes possess stretchon parameters and hidden conformal symmetries. The superradiant stability and steady state resonance of such black holes warrant further investigation and form the primary motivation for this study. In…

General Relativity and Quantum Cosmology · Physics 2025-08-05 Wen-Xiang Chen

Black holes in binary systems execute patterns of outburst activity where two characteristic X-ray states are associated with different behaviours observed at radio wavelengths. The hard state is associated with radio emission indicative of…

The rate of gravitational wave bursts from the mergers of massive primordial black holes in clusters is calculated. Such clusters of black holes can be formed through phase transitions in the early Universe. The central black holes in…

Cosmology and Nongalactic Astrophysics · Physics 2010-03-23 V. I. Dokuchaev , Yu. N. Eroshenko , S. G. Rubin

Supermassive black holes can be seen as an agent of galaxy transformation. In particular, a supermassive black hole can cause a triaxial galaxy to evolve toward axisymmetry by inducing chaos in centrophilic orbit families. This is one way…

Astrophysics · Physics 2007-05-23 Kelly Holley-Bockelmann

We propose a new model of Fast Radio Bursts (FRBs) based on stellar mass black hole-massive star binaries. We argue that the inhomogeneity of the circumstellar materials or/and the time varying wind activities of the stellar companion will…

High Energy Astrophysical Phenomena · Physics 2018-12-12 Shu-Xu Yi , K. S. Cheng , Rui Luo

In Ho\v{r}ava and Einstein-{\AE}ther theories of modified gravity, in spite of the violation of Lorentz invariance, spherically-symmetric stationary black hole solutions possess an inner universal horizon which separates field…

General Relativity and Quantum Cosmology · Physics 2015-07-10 Florent Michel , Renaud Parentani

Gamma-ray bursts (GRBs) appear as the brightest transient phenomena in the Universe. The nature of the central engine in GRBs is a missing link in the theory of fireballs to their stellar mass progenitors. Here it is shown that rotating…

Astrophysics · Physics 2008-11-26 Maurice H. P. M. van Putten

Based on the hyperboloidal framework, we research the dynamical process of charged de Sitter black holes scattered by a charged scalar field. From the linear perturbation analysis, with the coupling strength within a critical interval, the…

General Relativity and Quantum Cosmology · Physics 2025-02-17 Zhen-Tao He , Qian Chen , Yu Tian , Cheng-Yong Zhang , Hongbao Zhang

Vorticity has recently been suggested to be a property of highly-spinning black holes. The connection between vorticity and limiting spin represents a universal feature shared by objects of maximal microstate entropy, so-called saturons.…

High Energy Physics - Phenomenology · Physics 2024-04-16 Gia Dvali , Oleg Kaikov , Florian Kuhnel , Juan Sebastián Valbuena-Bermúdez , Michael Zantedeschi

The spectrum of the quasinormal modes of the gravitational waves emitted during the ringdown phase following the merger of two black holes is of primary importance in gravitational astronomy. However, the spectrum is extremely sensitive to…

General Relativity and Quantum Cosmology · Physics 2024-07-30 A. Ianniccari , A. J. Iovino , A. Kehagias , P. Pani , G. Perna , D. Perrone , A. Riotto

We consider the case of rotating black holes in a dark-matter-emulating theory of gravity called MOG. The latter introduces a gravitational vector field with an associated gravitational charge proportional to the black hole mass and a…

General Relativity and Quantum Cosmology · Physics 2018-12-14 Michael F. Wondrak , Piero Nicolini , John W. Moffat
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