Dilatonic (quasi-) black holes without scalar charge
- Authors: Bronnikov K.A.1,2,3, Israpilov D.I.2
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Affiliations:
- VNIIMS
- Institute of Gravitation and Cosmology
- National Research Nuclear University “MEPhI” (Moscow Engineering Physics Institute)
- Issue: Vol 22, No 3 (2016)
- Pages: 281-287
- Section: Article
- URL: https://journals.rcsi.science/0202-2893/article/view/176038
- DOI: https://doi.org/10.1134/S020228931603004X
- ID: 176038
Cite item
Abstract
We consider static, spherically symmetric configurations of electrically charged dust in Einstein-Maxwell-dilaton gravity where the Lagrangian contains the interaction term P(χ)FμνFμν with an arbitrary function P(χ). Unlike previous studies, we assume that the scalar field χ (which can be canonical or phantom) does not have a charge of its own and exists only due to this interaction. We discuss possible solutions to the field equations, in particular, those describing black holes (BHs) and quasi-black holes (QBHs). The latter are globally regular configurations whose size is very close to that of a BH of the same mass and which therefore are almost indistinguishable from BHs for a distant observer. Some general features are revealed, a family of explicitly integrable models is found, and some explicit examples are presented.
About the authors
K. A. Bronnikov
VNIIMS; Institute of Gravitation and Cosmology; National Research Nuclear University “MEPhI” (Moscow Engineering Physics Institute)
Author for correspondence.
Email: kb20@yandex.ru
Russian Federation, Ozyornaya ul. 46, Moscow, 119361; ul. Miklukho-Maklaya 6, Moscow, 117198; Kashirskoe sh. 31, Moscow, 115409
D. I. Israpilov
Institute of Gravitation and Cosmology
Email: kb20@yandex.ru
Russian Federation, ul. Miklukho-Maklaya 6, Moscow, 117198