Dynamically and thermodynamically stable black holes in Einstein-Maxwell-Dilaton gravity

DOI10.1007/JHEP07(2020)063zbMath1451.83061arXiv1912.02192MaRDI QIDQ2215359

Dumitru Astefanesei, Eugen Radu, Nicolas Sanchis-Gual, Jose Luis Blázquez-Salcedo, Carlos A. R. Herdeiro

Publication date: 11 December 2020

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1912.02192

zbMATH Keywords

black holes in string theoryblack holes

Mathematics Subject Classification ID

Black holes (83C57) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)

Related Items (8)

Horizon acoustics of the GHS black hole and the spectrum of \( \mathrm{AdS}_2\) ⋮ Higher dimensional Reissner-Nordström black holes supporting static scalar shells ⋮ Time evolution of Einstein-Maxwell-scalar black holes after a thermal quench ⋮ Hairy black holes, scalar charges and extended thermodynamics ⋮ De-singularizing the extremal GMGHS black hole via higher derivatives corrections ⋮ Spontaneously vectorized Einstein-Gauss-Bonnet black holes ⋮ Thermodynamically stable asymptotically flat hairy black holes with a dilaton potential: the general case ⋮ Exact holographic RG flows in extended SUGRA

Uses Software

• Einstein Toolkit

Cites Work

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