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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.)

Charged black holes in a generalized scalar-tensor gravity model

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Autor(es):
Brihaye, Yves [1] ; Hartmann, Betti [2]
Número total de Autores: 2
Afiliação do(s) autor(es):
[1] Univ Mons, Phys Theor & Math, Pl Parc, B-7000 Mons - Belgium
[2] Univ Sao Paulo, IFSC, BR-13560970 Sao Carlos, SP - Brazil
Número total de Afiliações: 2
Tipo de documento: Artigo Científico
Fonte: Physics Letters B; v. 772, p. 476-482, SEP 10 2017.
Citações Web of Science: 1
Resumo

We study 4-dimensional charged and static black holes in a generalized scalar-tensor gravity model, in which a shift symmetry for the scalar field exists. For vanishing scalar field the solution corresponds to the Reissner-Nordstrom (RN) solution, while solutions of the full scalar-gravity model have to be constructed numerically. We demonstrate that these black holes support Galilean scalar hair up to a maximal value of the scalar-tensor coupling that depends on the value of the charge and can be up to roughly twice as large as that for uncharged solutions. The Hawking temperature T-H of the hairy black holes at maximal scalar-tensor coupling decreases continuously with the increase of the charge and reaches T-H = 0 for the highest possible charge that these solutions can carry. However, in this limit, the scalar-tensor coupling needs to vanish. The limiting solution hence corresponds to the extremal RN solution, which does not support regular Galileanscalar hair due to its AdS(2) x S-2 near-horizon geometry. (C) 2017 The Author(s). Published by Elsevier B.V. (AU)

Processo FAPESP: 16/12605-2 - Instabilidade/Estabilidade e excitação de modos nos espaços-tempos (assintoticamente) Anti-de Sitter com vista a correspondência AdS/CFT
Beneficiário:Betti Hartmann
Linha de fomento: Auxílio à Pesquisa - Regular