Thermodynamics of a class of non-asymptotically flat black holes in Einstein-Maxwell-dilaton theory
DOI10.1007/S10714-013-1529-6zbMath1273.83111arXiv1206.0763OpenAlexW3100685750MaRDI QIDQ354741
Glauber Tadaiesky Marques, Manuel E. Rodrigues
Publication date: 19 July 2013
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1206.0763
Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Classical and relativistic thermodynamics (80A10) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Einstein-Maxwell equations (83C22)
Cites Work
- Unnamed Item
- Unnamed Item
- No Hawking-page phase transition in three dimensions
- Particle creation by black holes
- Hawking radiation of linear dilaton black holes
- Rotating solutions of Einstein-Maxwell-dilaton gravity with unusual asymptotics
- Geometrothermodynamics of black holes
- Contact Riemannian geometry and thermodynamics
- Charged dilaton black holes with unusual asymptotics
- Linear dilatons, \(\text{NS} 5\)-branes and holography
- Differential-geometrical methods in statistics
- General static spherical solutions of \(d\)-dimensional charged dilaton gravity theories
- Geometrothermodynamics
- Spherically symmetric solutions in dimensionally reduced spacetimes
- Conformal invariance of black hole temperature
- Asymptotically non-flat rotating dilaton black holes
- Non-asymptotically flat, non-dS/AdS dyonic black holes in dilaton gravity
- General Relativity
- Quantum Fields in Curved Space
This page was built for publication: Thermodynamics of a class of non-asymptotically flat black holes in Einstein-Maxwell-dilaton theory
