Construction and physical properties of Kerr black holes with scalar hair
C Herdeiro, E Radu - Classical and Quantum Gravity, 2015 - iopscience.iop.org
Kerr black holes (BHs) with scalar hair are solutions of the Einstein–Klein–Gordon field
equations describing regular (on and outside an event horizon), asymptotically flat BHs with …
equations describing regular (on and outside an event horizon), asymptotically flat BHs with …
Black-hole bombs and photon-mass bounds
Generic extensions of the standard model predict the existence of ultralight bosonic degrees
of freedom. Several ongoing experiments are aimed at detecting these particles or …
of freedom. Several ongoing experiments are aimed at detecting these particles or …
Superradiant instabilities in astrophysical systems
Light bosonic degrees of freedom have become a serious candidate for dark matter, which
seems to pervade our entire Universe. The evolution of these fields around curved …
seems to pervade our entire Universe. The evolution of these fields around curved …
Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric
We discuss a general method to study linear perturbations of slowly rotating black holes
which is valid for any perturbation field, and particularly advantageous when the field …
which is valid for any perturbation field, and particularly advantageous when the field …
Superradiant instabilities of rotating black holes in the time domain
SR Dolan - Physical Review D—Particles, Fields, Gravitation, and …, 2013 - APS
Bosonic fields on rotating black hole spacetimes are subject to amplification by
superradiance, which induces exponentially-growing instabilities (the “black hole bomb”) in …
superradiance, which induces exponentially-growing instabilities (the “black hole bomb”) in …
Massive vector fields on the Schwarzschild spacetime: quasinormal modes and bound states
We study the propagation of a massive vector or Proca field on the Schwarzschild
spacetime. The field equations are reduced to a one-dimensional wave equation for the odd …
spacetime. The field equations are reduced to a one-dimensional wave equation for the odd …
Nonlinear interactions between black holes and Proca fields
Physics beyond the standard model is an important candidate for dark matter, and an
interesting testing ground for strong-field gravity: the equivalence principle'forces' all forms of …
interesting testing ground for strong-field gravity: the equivalence principle'forces' all forms of …
Maxwell perturbations on Kerr–anti–de Sitter black holes: Quasinormal modes, superradiant instabilities, and vector clouds
M Wang, C Herdeiro - Physical Review D, 2016 - APS
Scalar and gravitational perturbations on Kerr–anti–de Sitter (Kerr-AdS) black holes have
been addressed in the literature and have been shown to exhibit a rich phenomenology. In …
been addressed in the literature and have been shown to exhibit a rich phenomenology. In …
NR/HEP: roadmap for the future
Physic in curved spacetime describes a multitude of phenomena, ranging from astrophysics
to high-energy physics (HEP). The last few years have witnessed further progress on several …
to high-energy physics (HEP). The last few years have witnessed further progress on several …
Superradiance--the 2020 Edition
Superradiance is a radiation enhancement process that involves dissipative systems. With a
60 year-old history, superradiance has played a prominent role in optics, quantum …
60 year-old history, superradiance has played a prominent role in optics, quantum …