Unitarity of Maxwell theory on curved spacetimes in the covariant formalism
arXiv:1303.1885 · doi:10.1103/PhysRevD.87.125033
Abstract
Quantum field theory in curved spacetime may be defined either through a manifestly unitary canonical approach or via the manifestly covariant path integral formalism. For gauge theories, these two approaches have produced conflicting results, leading to the question of whether the canonical approach is covariant, and whether the path integral approach is unitary. We show the unitarity of the covariant U(1) Maxwell theory, defined via the Wick rotation of a Euclidean path integral. We begin by gauge-fixing the path integral, taking care with zero modes, large gauge transformations, and nontrivial bundles. We find an extra geometric factor in the partition function that has been overlooked in previous work, coming from the zero mode of the gauge symmetry, which affects the entropy and stress-energy tensor. With this extra factor, the covariant calculation agrees with the canonical result for ultrastatic manifolds, and in D = 2. Finally, we argue that if there exists a unitary (but not necessarily covariant) canonical formulation, then the covariant formulation must also be unitary, even if the two approaches disagree.
10 pages
References in corpus (2)
Cited by in corpus (12)
- Geometric entropy and edge modes of the electromagnetic field
- Quantum de Sitter horizon entropy from quasicanonical bulk, edge, sphere and topological string partition functions
- Cauchy Slice Holography: A New AdS/CFT Dictionary
- Physical renormalization schemes and asymptotic safety in quantum gravity
- Dynamical Edge Modes and Entanglement in Maxwell Theory
- Electromagnetic Duality and Entanglement Anomalies
- Structure of Kaluza-Klein Graviton Scattering Amplitudes from Gravitational Equivalence Theorem and Double-Copy
- A Compendium of Sphere Path Integrals
- Black Hole Horizon Edge Partition Functions
- Dynamical Edge Modes in -form Gauge Theories
- Infrared problem in the Faddeev-Popov-ghost propagator in perturbative quantum gravity in de Sitter spacetime
- Hamiltonian BRST formalism for gauge fields on black hole spacetimes