Two formalisms, one renormalized stress-energy tensor
arXiv:1112.0489 · doi:10.1103/PhysRevD.85.084001
Abstract
We explicitly compare the structure of the renormalized stress-energy tensor (RSET) of a massless scalar field in a (1+1) curved spacetime as obtained by two different strategies: normal-mode construction of the field operator and one-loop effective action. We pay special attention to where and how it is encoded the information related to the choice of vacuum state in both formalisms. By establishing a clear translation map between both procedures, we show that these two potentially different RSET are actually equal, when using vacuum-state choices related by this map. One specific aim of the analysis is to facilitate the comparison of results regarding semiclassical effects in gravitational collapse as obtained within these different formalisms.
9 pages, no figures; v2: minor changes, version accepted for publication
References in corpus (6)
- Fate of gravitational collapse in semiclassical gravity
- Macroscopic Effects of the Quantum Trace Anomaly
- Quantum Gowdy model: A uniqueness result
- Hawking radiation by Kerr black holes and conformal symmetry
- Short-distance contribution to the spectrum of Hawking radiation
- New Horizons in Gravity: Dark Energy and Condensate Stars
Cited by in corpus (13)
- Stellar equilibrium in semiclassical gravity
- Classical mass inflation vs semiclassical inner horizon inflation
- The Equivalence Principle at Work in Radiation from Unaccelerated Atoms and Mirrors
- Semiclassical instability of inner-extremal regular black holes
- Tidal and nonequilibrium Casimir effects in free fall
- Semiclassical gravity effects near horizon formation
- Boulware Vacuum vs. Regularity: Thoughts on Anomaly-Induced Effective Action
- Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity
- The boundary effect of anomaly-induced action
- Quantum corrected Einstein-Yang-Mills black holes in semiclassical gravity
- An Ultra-compact Object from Semi-classical Gravity
- Dynamical wormholes
- Imprints of quantum vacuum fluctuations on the gravitational field of a spherical mass