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Constructing black holes in Einstein-Maxwell-scalar theory

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arxiv 2005.14476 v2 pith:O6I34Q54 submitted 2020-05-29 gr-qc hep-th

Shuang Yu , Jianhui Qiu , Changjun Gao This is my paper · ORCID
classification gr-qchep-th
keywords blackeinstein-maxwell-scalarholesscalarsittertheoryanticonstructed
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Exact black hole solutions in the Einstein-Maxwell-scalar theory are constructed. They are the extensions of dilaton black holes in de Sitter or anti de Sitter universe. As a result, except for a scalar potential, a coupling function between the scalar field and the Maxwell invariant is present. Then the corresponding Smarr formula and the first law of thermodynamics are investigated.

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Cited by 1 Pith paper

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  1. Phase Transition and Critical Phenomena of Charged Einstein-Maxwell-Scalar Black Holes

    gr-qc 2025-05 conditional novelty 5.0 of 10

    Charged EMs black holes show van der Waals-type phase transitions with mean-field critical exponents, and the phase transition disappears above a threshold scalar charge.

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