Equivalence of Adiabatic and DeWitt-Schwinger renormalization schemes
arXiv:1412.7570 · doi:10.1103/PhysRevD.91.064031
Abstract
We prove that adiabatic regularization and DeWitt-Schwinger point-splitting provide the same result for the renormalized expectation values of the stress-energy tensor for spin- fields. This generalizes the equivalence found for scalar fields, which is here recovered in a different way. We also argue that the coincidence limit of the DeWitt-Schwinger proper time expansion of the two-point function exactly agrees with the analogous expansion defined by the adiabatic regularization method at any order (for both scalar and spin- fields). We also illustrate the power of the adiabatic method to compute higher order DeWitt coefficients in FLRW universes.
arXiv commentMisprints corrected, small change in title
References in corpus (18)
- The pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations
- A Quantum Gravity Extension of the Inflationary Scenario
- An Extension of the Quantum Theory of Cosmological Perturbations to the Planck Era
- Non-perturbative effects of vacuum energy on the recent expansion of the universe
- Adiabatic regularization and particle creation for spin one-half fields
- Perturbative Quantum Gravity Comes of Age
- Adiabatic regularization for spin-1/2 fields
- Riemann Normal Coordinate expansions using Cadabra
- Renormalized stress-energy tensor for spin-1/2 fields in expanding universes
- Revising the predictions of inflation for the cosmic microwave background anisotropies
- Particle creation and particle number in an expanding universe
- Acceleration of the universe, vacuum metamorphosis, and the large-time asymptotic form of the heat kernel
- Revising the observable consequences of slow-roll inflation
- Stress-Energy Tensor of Adiabatic Vacuum in Friedmann-Robertson-Walker Spacetimes
- Stress-Energy Tensor of the Quantized Massive Fields in Friedman-Robertson-Walker Spacetimes
- Inflation, quantum fields, and CMB anisotropies
- Spacetime correlators of perturbations in slow-roll de Sitter inflation
- Electric-magnetic duality and renormalization in curved spacetimes
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