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Dilaton Black Holes in de Sitter or Anti-de Sitter Universe

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arxiv hep-th/0411104 v4 pith:XN5U74QL submitted 2004-11-10 hep-th astro-ph

Chang Jun Gao , Shuang Nan Zhang This is my paper · ORCID
classification hep-thastro-ph
keywords sitterdilatonanti-deblackuniversebackgroundholeliouville-type
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Poletti and Wiltshire have shown that, with the exception of a pure cosmological constant, the solution of a dilaton black hole in the background of de Sitter or anti-de Sitter universe, does not exist in the presence of one Liouville-type dilaton potential. Here with the combination of three Liouville-type dilaton potentials, we obtain the dilaton black hole solutions in the background of de Sitter or anti-de Sitter universe.

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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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