We modify and generalize the known solution for the electromagnetic field when a vacuum, stationary, axisymmetric black hole is immersed in a uniform magnetic field to the case of nonvacuum black holes (of modified gravity) and determine all linear terms of the vector potential in powers of the magnetic field and the rotation parameter
I. INTRODUCTION The Meissner effect of black holes describes their property to expel any exterior ...
AbstractIn this Letter, we extend the Parikh–Wilczek tunnelling framework to calculate the emission ...
We construct the general electrically charged, rotating black hole solution in the heterotic string ...
We modify and generalize the known solution for the electromagnetic field when a vacuum, stationary,...
We extend the Wald solution to a black hole that is also moving at constant velocity. More specifica...
Stationary axisymmetric magnetic fields are expelled from outer horizons of black holes as they beco...
In the background of a stationary black hole, the "conserved current" of a particular spinor field a...
We revisit the Blandford-Znajek process and solve the fundamental equation that governs the structur...
We study stationary black holes in the presence of an external strong magnetic field. In the case wh...
We study the vacuum polarization of a massless minimally coupled scalar field at the horizon of four...
Recently, it was claimed by King & Pringle that accretion of electric charge by a black hole rotatin...
AbstractWe show the existence of D=4 non-Abelian solutions approaching asymptotically a dilatonic Me...
We consider the Maxwell equation in the exterior of a very slowly rotating Kerr black hole. For this...
The idea that black hole spin is instrumental in the generation of powerful jets in active galactic ...
AbstractBased on the Lagrangian of the steady axisymmetric force-free magnetosphere (FFM) equation a...
I. INTRODUCTION The Meissner effect of black holes describes their property to expel any exterior ...
AbstractIn this Letter, we extend the Parikh–Wilczek tunnelling framework to calculate the emission ...
We construct the general electrically charged, rotating black hole solution in the heterotic string ...
We modify and generalize the known solution for the electromagnetic field when a vacuum, stationary,...
We extend the Wald solution to a black hole that is also moving at constant velocity. More specifica...
Stationary axisymmetric magnetic fields are expelled from outer horizons of black holes as they beco...
In the background of a stationary black hole, the "conserved current" of a particular spinor field a...
We revisit the Blandford-Znajek process and solve the fundamental equation that governs the structur...
We study stationary black holes in the presence of an external strong magnetic field. In the case wh...
We study the vacuum polarization of a massless minimally coupled scalar field at the horizon of four...
Recently, it was claimed by King & Pringle that accretion of electric charge by a black hole rotatin...
AbstractWe show the existence of D=4 non-Abelian solutions approaching asymptotically a dilatonic Me...
We consider the Maxwell equation in the exterior of a very slowly rotating Kerr black hole. For this...
The idea that black hole spin is instrumental in the generation of powerful jets in active galactic ...
AbstractBased on the Lagrangian of the steady axisymmetric force-free magnetosphere (FFM) equation a...
I. INTRODUCTION The Meissner effect of black holes describes their property to expel any exterior ...
AbstractIn this Letter, we extend the Parikh–Wilczek tunnelling framework to calculate the emission ...
We construct the general electrically charged, rotating black hole solution in the heterotic string ...
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