Finite temperature nonlocal effective action for quantum fields in curved space
arXiv:hep-th/9807038 · doi:10.1103/PhysRevD.59.024002
Abstract
Massless and massive scalar fields and massless spinor fields are considered at arbitrary temperatures in four dimensional ultrastatic curved spacetime. Scalar models under consideration can be either conformal or nonconformal and include selfinteraction. The one-loop nonlocal effective action at finite temperature and free energy for these quantum fields are found up to the second order in background field strengths using the covariant perturbation theory. The resulting expressions are free of infrared divergences. Spectral representations for nonlocal terms of high temperature expansions are obtained.
32 pages, LaTeX
References in corpus (6)
- Thermal Fields, Entropy, and Black Holes
- Effective QED Actions: Representations, Gauge Invariance, Anomalies and Mass Expansions
- The structure of the graviton self-energy at finite temperature
- Particle creation in the effective action method
- Euclidean and Canonical Formulations of Statistical Mechanics in the Presence of Killing Horizons
- Finite Temperature Nonlocal Effective Action for Scalar Fields
Cited by in corpus (21)
- Universal temperature corrections to the free energy for the gravitational field
- The Free Energy of N=4 Super-Yang-Mills and the AdS/CFT Correspondence
- The quantum fate of black hole horizons
- One-loop effective action: nonlocal form factors and renormalization group
- Black-hole stability in non-local gravity
- Two-dimensional effective action for matter fields coupled to the dilaton
- Symmetry breaking and lattice kirigami: finite temperature effects
- Heat kernel expansion in the covariant perturbation theory
- Dual Fermion Condensates in Curved Space
- High-temperature expansion of the one-loop free energy of a scalar field on a curved background
- Finite temperature quantum field theory in the heat kernel method
- Universality and ambiguity in fermionic effective actions
- Effective action for bubble nucleation rates
- A stable static Universe?
- Non-perturbative corrections to the one-loop free energy induced by a massive scalar field on a stationary slowly varying in space gravitational background
- Nonlocal effective actions in semiclassical gravity: thermal effects in stationary geometries
- Negative Newton constant may destroy some conjectures
- Partition function for a singular background
- Can a Nonsymmetric Metric mimic NCQFT in ?
- Partition function of massless scalar field in Schwarzschild background
- Form factors and non-local Multiplicative Anomaly for fermions with background torsion