Entropy-Area Relations in Field Theory
arXiv:hep-th/0204038 · doi:10.1088/1126-6708/2002/06/008
Abstract
We consider the contribution to the entropy from fields in the background of a curved time-independent metric. To account for the curvature of space, we postulate a position-dependent UV cutoff. We argue that a UV cutoff on energy naturally implies an IR cutoff on distance. With this procedure, we calculate the scalar contribution in a background anti-de Sitter space, the exterior of a black hole, and de Sitter space. In all cases, we find results that can be simply interpreted in terms of local energy and proper volume, yielding insight into the apparent reduced dimensionality of systems with gravity.
20 pages, 1 figure
References in corpus (4)
Cited by in corpus (10)
- Scale-invariant resonance tagging in multijet events and new physics in Higgs pair production
- A negative S parameter from Holographic Technicolor
- Gravity-mediated (or Composite) Dark Matter
- Running of Gauge Couplings in AdS5 via Deconstruction
- The fifth dimension as an analogue computer for strong interactions at the LHC
- Gravity-mediated (or Composite) Dark Matter Confronts Astrophysical Data
- D-Sitter Space: Causal Structure, Thermodynamics, and Entropy
- Discretizing Gravity in Warped Spacetime
- Exploring holographic Composite Higgs models
- On the compatibility of the diboson excess with a gg-initiated composite sector