Hawking radiation from AdS black holes
By V. Hubeny, D. Marolf, M. Rangamani. 2009
146 citations recorded by the source corpus.
We study Hartle–Hawking-like states of quantum field theories on asymptotically AdS black hole backgrounds, with particular regard to the phase structure of interacting theories. By a suitable analytic continuation we show that the equilibrium dynamics of field theories on large asymptotically AdS black holes can be related to the low-temperature states of the same field theory on the AdS soliton (or pure AdS) background. This allows us to gain insight into Hartle–Hawking-like states on large-radius Schwarzschild- or rotating-AdS black holes. Furthermore, we exploit the AdS/CFT correspondence to explore the physics of strongly coupled large N theories on asymptotically AdS black holes. In particular, we exhibit a plausibly complete set of phases for the M2-brane world-volume superconformal field theory on a BTZ black hole background. Our analysis partially resolves puzzles previously raised in connection with Hawking radiation on large AdS black holes.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ed858a5e9db7e00b3f91f6dd3e9b211a29b0883e
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Citations in the corpus
- Brownian Motion in AdS/CFT (2008, unknown): “The fact that the outgoing and ingoing modes have the same amplitude means that the AdS black hole, which Hawking radiates, can be in thermal equilibrium at temperature T [35].”
- Numerical methods for finding stationary gravitational solutions (2015, unknown): “[317] V.”
- Static patch solipsism: conformal symmetry of the de Sitter worldline (2011, background): “The conformal map (63) has appeared before in different contexts, such as [47].”
- A Holographic View on Physics out of Equilibrium (2010, methodology): “For a discussion when the boundary metric describes a black hole with various asymptotics, see [27, 28, 29]; in the high temperature regime the conjectured bulk solution, christened ‘black funnel’, would be a bulk black hole whose horizon stretches all the way out to the boundary.”