We present black hole uniqueness theorems for the C-metric and Ernst solution. The proof follows a similar strategy as that used to prove the uniqueness of the Kerr-Newman solution, however the presence of an acceleration horizon provides some critical differences. We also show how to derive the Bunting/Mazur result (on the positivity of a suitable divergence required in the proof) using new methods. We briefly explain the importance of the uniqueness of the Ernst solution in relation to the proposed black hole monopole pair creation mediated by the related instanton
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
Einstein's Theory of General Relativity has proven remarkably successful at modelling a wide range ...
We make use of an internal symmetry of a truncation of the bosonic sector of the superstring and N=4...
The Ernst method of removing nodal singularities from the charged C-metric representing a uniformly ...
We show that a stationary asymptotically flat electro-vacuum solution of Einstein's equations that i...
A straightforward generalization of the celebrated uniqueness theorem to dimensions greater than fou...
We show that a stationary asymptotically flat electro-vacuum solution of Einstein's equations that i...
We examine the effects of accelerating both isolated and coupled black holes in a variety of contex...
I examine the pair creation of black holes in spacetimes with a cosmological constant of either sign...
The pair creation of black holes with event horizons of non-trivial topology is described. The space...
WOS:000272458700010 (Nº de Acesso Web of Science)We prove uniqueness of the Kerr black holes within ...
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
The complete family of exact solutions representing accelerating and rotating black holes with possi...
A class of exact solutions of the Einstein–Maxwell equations is presented which describes an acceler...
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
Einstein's Theory of General Relativity has proven remarkably successful at modelling a wide range ...
We make use of an internal symmetry of a truncation of the bosonic sector of the superstring and N=4...
The Ernst method of removing nodal singularities from the charged C-metric representing a uniformly ...
We show that a stationary asymptotically flat electro-vacuum solution of Einstein's equations that i...
A straightforward generalization of the celebrated uniqueness theorem to dimensions greater than fou...
We show that a stationary asymptotically flat electro-vacuum solution of Einstein's equations that i...
We examine the effects of accelerating both isolated and coupled black holes in a variety of contex...
I examine the pair creation of black holes in spacetimes with a cosmological constant of either sign...
The pair creation of black holes with event horizons of non-trivial topology is described. The space...
WOS:000272458700010 (Nº de Acesso Web of Science)We prove uniqueness of the Kerr black holes within ...
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
The complete family of exact solutions representing accelerating and rotating black holes with possi...
A class of exact solutions of the Einstein–Maxwell equations is presented which describes an acceler...
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
WOS:000273677900011 (Nº de Acesso Web of Science)We obtain a classification of stationary, I+-regula...
Einstein's Theory of General Relativity has proven remarkably successful at modelling a wide range ...