Phase transition to a hairy black hole in asymptotically flat spacetime
From MaRDI portal
Publication:737782
DOI10.1007/JHEP11(2013)133zbMath1342.83181arXiv1308.5280MaRDI QIDQ737782
George Siopsis, Eleftherios Papantonopoulos, George Koutsoumbas, Theodoros Kolyvaris
Publication date: 12 August 2016
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1308.5280
Related Items (10)
Extremal hairy black holes ⋮ Building a holographic superconductor with a scalar field coupled kinematically to Einstein tensor ⋮ Generalized non-minimal derivative coupling: application to inflation and primordial black hole production ⋮ Stability of black holes with non-minimally coupled scalar hair to the Einstein tensor ⋮ Black hole entropy arising from massless scalar field with Lorentz violation induced by the coupling to Einstein tensor ⋮ Four-dimensional asymptotically AdS black holes with scalar hair ⋮ Quantum effects in Galileon black holes ⋮ Quasinormal modes of scalar field coupled to Einstein's tensor in the non-commutative geometry inspired black hole ⋮ Unification of dark matter-dark energy in generalized Galileon theories ⋮ Reheating predictions in gravity theories with derivative coupling
Cites Work
- A new class of exact hairy black hole solutions
- Conformally coupled scalar black holes admit a flat horizon due to axionic charge
- The large-\(N\) limit of superconformal field theories and supergravity
- QUINTESSENTIAL AND PHANTOM POWER-LAW SOLUTIONS IN SCALAR TENSOR MODEL OF DARK ENERGY
- Introduction to Holographic Superconductors
- Scalar hair from a derivative coupling of a scalar field to the Einstein tensor
- Charged C-metric with conformally coupled scalar field
- Lectures on holographic methods for condensed matter physics
- Building a Holographic Superconductor
- Phase transitions near black hole horizons
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