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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

General relativity from Einstein-Gauss-Bonnet gravity

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Autor(es):
Canfora, Fabrizio [1] ; Cisterna, Adolfo [2] ; Fuenzalida, Sebastian [3] ; Henriquez-Baez, Carla [4] ; Oliva, Julio [4]
Número total de Autores: 5
Afiliação do(s) autor(es):
[1] Ctr Estudios Cient, Casilla 1469, Valdivia - Chile
[2] Univ Tarapaca, Sede Esmeralda, Ave Luis Emilio Recabarren 2477, Iquique - Chile
[3] Univ Tecn Federico Santa Maria, Dept Fis, Casilla 110-V, Valparaiso - Chile
[4] Univ Concepcion, Dept Fis, Casilla 160-C, Concepcion - Chile
Número total de Afiliações: 4
Tipo de documento: Artigo Científico
Fonte: Physical Review D; v. 104, n. 4 AUG 11 2021.
Citações Web of Science: 0
Resumo

In this work we show that Einstein gravity in four dimensions can be consistently obtained from the compactification of a generic higher curvature Lovelock theory in dimension D = 4 + p, (p >= 1). The compactification is performed on a direct product space M-D = M-4 x K-p, where K-p is a Euclidean internal manifold of constant curvature. The process is carried out in such a way that no fine tuning between the coupling constants is needed. The compactification requires us to dress the internal manifold with the flux of suitable p-forms whose field strengths are proportional to the volume form of the internal space. We explicitly compactify Einstein-Gauss-Bonnet theory from dimension six to Einstein theory in dimension four and sketch out a similar procedure for this compactification to take place starting from dimension five. Several black string/p-branes solutions are constructed, among which, a five dimensional asymptotically flat black string composed of a Schwarzschild black hole on the brane is particularly interesting. Finally, the thermodynamic of the solutions is described and we find that the consistent compactification modifies the entropy by including a constant term, which may induce a departure from the usual behavior of the Hawking-Page phase transition. New scenarios are possible in which large black holes dominate the canonical ensemble for all temperatures above the minimal value. (AU)

Processo FAPESP: 19/13231-7 - Rede Chile - São Paulo de holografia
Beneficiário:Horatiu Stefan Nastase
Modalidade de apoio: Auxílio à Pesquisa - Regular