Abstract
Abstract
In this work we use a general covariance breaking mechanism to obtain a class of charged black holes whose background geometry asymptotically approaches Lifshitz spacetimes. We discuss how this method affects Einstein’s equations and explore the thermodynamics and critical behavior of the solution found.
Funder
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Fundação de Apoio à Pesquisa do Estado da Paraíba
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior
Cited by
1 articles.
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