arXiv · 0709.3738
Thermodynamics of Large AdS Black Holes
Abstract
We consider leading order quantum corrections to the geometry of large AdS black holes in a spherical reduction of four-dimensional Einstein gravity with negative cosmological constant. The Hawking temperature grows without bound with increasing black hole mass, yet the semiclassical back-reaction on the geometry is relatively mild, indicating that observers in free fall outside a large AdS black hole never see thermal radiation at the Hawking temperature. The positive specific heat of large AdS black holes is a statement about the dual gauge theory rather than an observable property on the gravity side. Implications for string thermodynamics with an AdS infrared regulator are briefly discussed.
Explore related subjects
Keep this discovery
Samuli Hemming, Larus Thorlacius. 2007-10-10. Thermodynamics of Large AdS Black Holes. https://doi.org/10.1088/1126-6708%2F2007%2F11%2F086
Cite the original work for its findings. Save a collection to share your selection of sources.