Abstract Various aspects of the C-metric representing two rotating charged black holes accelerated in opposite directions are summarized and its limits are considered. A particular attention is paid to the special-relativistic limit in which the electromag-netic field becomes the “magic field ” of two oppositely accelerated rotating charged relativistic discs. When the acceleration vanishes the usual electromagnetic magic field of the Kerr–Newman black hole with gravitational constant set to zero arises. Properties of the accelerated discs and the fields produced are studied and illustrated graphically. The charges at the rim of the accelerated discs move along spiral trajec-tories with the speed of light. If the magic field has some deeper...
In this paper, considering the nonlinear electromagnetic field coupled to Einstein gravity, we obtai...
The near horizon geometry of the rotating C-metric, describing accelerating Kerr–Newman black holes,...
Cosmic black holes can act as agents of particle acceleration. We study properties of a system consi...
Various aspects of the C-metric representing two rotating charged black holes accelerated in opposit...
Various aspects of the C-metric representing two rotating charged black holes accelerated in opposit...
The Ernst method of removing nodal singularities from the charged C-metric representing a uniformly ...
This paper examines the general relativistic model of a geometrically thick configuration of an accr...
An exact solution of Einstein's equations which represents a pair of accelerating and rotating black...
An exact solution of Einstein’s equations which represents a pair of accelerating and rotating black...
Strong gravity and magnetic fields are key ingredients that power processes of accretion and ejectio...
When the equatorial spin velocity, $v$, of a charged conducting sphere approaches $c$, the Lorentz f...
Abstract It is demonstrated that the Melvin universe representing the spacetime with a strong ‘homog...
To test the role of large-scale magnetic fields in accretion processes, we study the dynamics of the...
AbstractThe near horizon geometry of the rotating C-metric, describing accelerating Kerr–Newman blac...
Cosmic black holes can act as agents of particle acceleration. We study properties of a system consi...
In this paper, considering the nonlinear electromagnetic field coupled to Einstein gravity, we obtai...
The near horizon geometry of the rotating C-metric, describing accelerating Kerr–Newman black holes,...
Cosmic black holes can act as agents of particle acceleration. We study properties of a system consi...
Various aspects of the C-metric representing two rotating charged black holes accelerated in opposit...
Various aspects of the C-metric representing two rotating charged black holes accelerated in opposit...
The Ernst method of removing nodal singularities from the charged C-metric representing a uniformly ...
This paper examines the general relativistic model of a geometrically thick configuration of an accr...
An exact solution of Einstein's equations which represents a pair of accelerating and rotating black...
An exact solution of Einstein’s equations which represents a pair of accelerating and rotating black...
Strong gravity and magnetic fields are key ingredients that power processes of accretion and ejectio...
When the equatorial spin velocity, $v$, of a charged conducting sphere approaches $c$, the Lorentz f...
Abstract It is demonstrated that the Melvin universe representing the spacetime with a strong ‘homog...
To test the role of large-scale magnetic fields in accretion processes, we study the dynamics of the...
AbstractThe near horizon geometry of the rotating C-metric, describing accelerating Kerr–Newman blac...
Cosmic black holes can act as agents of particle acceleration. We study properties of a system consi...
In this paper, considering the nonlinear electromagnetic field coupled to Einstein gravity, we obtai...
The near horizon geometry of the rotating C-metric, describing accelerating Kerr–Newman black holes,...
Cosmic black holes can act as agents of particle acceleration. We study properties of a system consi...