Two loop stress-energy tensor for inflationary scalar electrodynamics
- 1. Institute for Theoretical Physics (ITF) and Spinoza Institute, Utrecht University, Leuvenlaan 4, Postbus 80.195, 3508 TD Utrecht (Netherlands)
- 2. Department of Physics, University of Crete, GR-710 03 Heraklion (Greece)
- 3. Department of Physics, University of Florida, Gainesville, Florida 32611 (United States)
Description
We calculate the expectation value of the coincident product of two field strength tensors at two loop order in scalar electrodynamics on de Sitter background. The result agrees with the stochastic formulation which we have developed in a companion paper [T. Prokopec, N. C. Tsamis, and R. P. Woodard, Ann. Phys. (N.Y.) 323, 1324 (2008)] for the nonperturbative resummation of leading logarithms of the scale factor. When combined with a previous computation of scalar bilinears [T. Prokopec, N. C. Tsamis, and R. P. Woodard, Classical Quantum Gravity 24, 201 (2007)], our current result also gives the two loop stress-energy tensor for inflationary scalar electrodynamics. This shows a secular decrease in the vacuum energy which derives from the vacuum polarization induced by the inflationary production of charged scalars.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.78.043523;
- arXiv
- arXiv:0802.3673v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 78
- Journal Issue
- 4
- Journal Page Range
- p. 043523-043523.37
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41001800
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COMPUTERIZED SIMULATION; DE SITTER GROUP; ELECTRODYNAMICS; EXPECTATION VALUE; QUANTUM GRAVITY; STOCHASTIC PROCESSES; STRESSES; TENSOR FIELDS; VACUUM POLARIZATION
- Descriptors DEC
- FIELD THEORIES; LIE GROUPS; QUANTUM FIELD THEORY; SIMULATION; SYMMETRY GROUPS
Optional Information
- Notes
- (c) 2008 The American Physical Society