Add to ORKGA class of exact solutions of the Einstein–Maxwell equations is presented which describes an accelerating and rotating charged black hole in an asymptotically de Sitter or anti-de Sitter universe. The metric is presented in a new and convenient form in which the meaning of the parameters is clearly identified, and from which the physical properties of the solution can readily be interpreted
Kerrr in the title is not a typo. The third \u201cr\u201d stands for regular, in the sense of pathol...
We construct several new families of vacuum solutions that describe black holes in uniformly acceler...
The core of this thesis is the analysis of accelerating black hole solution with the NUT parameter, ...
A class of exact solutions of the Einstein-Maxwell equations is presented which describes an acceler...
The complete family of exact solutions representing accelerating and rotating black holes with possi...
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...
A class of exact solutions of Einstein’s equations is analysed which describes uniformly acceleratin...
The complete family of exact solutions representing accelerating and rotating black holes with possi...
The Ernst method of removing nodal singularities from the charged C-metric representing a uniformly ...
Einstein-Maxwell equations with a cosmological constant are analyzed in a stationary spacetime admit...
AbstractKerrr in the title is not a typo. The third “r” stands for regular, in the sense of patholog...
In this thesis we investigate gravitational lensing in two different families of black hole spacetim...
The curvature scalar invariants of the Riemann tensor are important in General Relativity because th...
We construct several new families of vacuum solutions that describe black holes in uniformly acceler...
Kerrr in the title is not a typo. The third \u201cr\u201d stands for regular, in the sense of pathol...
We construct several new families of vacuum solutions that describe black holes in uniformly acceler...
The core of this thesis is the analysis of accelerating black hole solution with the NUT parameter, ...
A class of exact solutions of the Einstein-Maxwell equations is presented which describes an acceler...
The complete family of exact solutions representing accelerating and rotating black holes with possi...
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...
A class of exact solutions of Einstein’s equations is analysed which describes uniformly acceleratin...
The complete family of exact solutions representing accelerating and rotating black holes with possi...
The Ernst method of removing nodal singularities from the charged C-metric representing a uniformly ...
Einstein-Maxwell equations with a cosmological constant are analyzed in a stationary spacetime admit...
AbstractKerrr in the title is not a typo. The third “r” stands for regular, in the sense of patholog...
In this thesis we investigate gravitational lensing in two different families of black hole spacetim...
The curvature scalar invariants of the Riemann tensor are important in General Relativity because th...
We construct several new families of vacuum solutions that describe black holes in uniformly acceler...
Kerrr in the title is not a typo. The third \u201cr\u201d stands for regular, in the sense of pathol...
We construct several new families of vacuum solutions that describe black holes in uniformly acceler...
The core of this thesis is the analysis of accelerating black hole solution with the NUT parameter, ...