Charged Lifshitz black holes from general covariance breaking
arXiv:2307.07305 · doi:10.1088/1361-6382/ad1d47
Abstract
In this work we use a general covariance breaking method to obtain a class of topological charged black holes whose background geometry asymptotically approaches Lifshitz spacetimes. We discuss how this mechanism affects Einstein's equations and explore the thermodynamics and critical behavior of the solution found.
Text and figures improvements, corrected typos, references added. Published in Classical and Quantum Gravity
References in corpus (23)
- Quantum Gravity at a Lifshitz Point
- Non-relativistic holography
- Horava-Lifshitz gravity: a status report
- Black holes in asymptotically Lifshitz spacetime
- Lifshitz Gravity for Lifshitz Holography
- Generalised tensor fluctuations and inflation
- Thermodynamics of Lifshitz Black Holes
- No Cauchy Horizon Theorem for Nonlinear Electrodynamics Black Holes with Charged Scalar Hairs
- Nonlinearly charged Lifshitz black holes for any exponent
- Hamiltonian formulation of an effective modified gravity with nondynamical background fields
- Universal thermal and electrical conductivity from holography
- Radially symmetric scalar solitons
- On the thermodynamics of Lifshitz black holes
- Gravity Theories with Background Fields and Spacetime Symmetry Breaking
- Evading Derrick's theorem in curved space: Static metastable spherical domain wall
- Gravity with Explicit Diffeomorphism Breaking
- Solitons in curved spacetime
- Localized scalar structures around static black holes
- Non-relativistic Josephson Junction from Holography
- BPS equations and solutions for Maxwell-scalar theory
- Scalar fields and Lifshitz black holes from Derrick's theorem evasion
- Lifshitz and hyperscaling violated Yang-Mills-dilaton black holes
- Holographic complexity for nonlinearly charged Lifshitz black holes