On the initial conditions and solutions of the semiclassical Einstein equations in a cosmological scenario
DOI10.1007/s00220-011-1268-zzbMath1223.83056arXiv1001.0864OpenAlexW2164564549MaRDI QIDQ635816
Publication date: 23 August 2011
Published in: Communications in Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1001.0864
Relativistic cosmology (83F05) Gravitational interaction in quantum theory (81V17) Quantization of the gravitational field (83C45) Renormalization group methods applied to problems in quantum field theory (81T17) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Initial value problems for second-order hyperbolic equations (35L15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (21)
Cites Work
- Unnamed Item
- Unnamed Item
- Particle creation by black holes
- On the derivation of Hawking radiation associated with the formation of a black hole
- Perturbative algebraic quantum field theory and the renormalization groups
- Theorems on the uniqueness and thermal properties of stationary, nonsingular, quasifree states on spacetimes with a bifurcate Killing horizon
- Cosmological horizons and reconstruction of quantum field theories
- On the Casimir energy for a massive quantum scalar field and the cosmological constant
- Radiation damping in a gravitational field
- Conformal generally covariant quantum field theory: the scalar field and its Wick products
- Wave equations on Lorentzian manifolds and quantization.
- Quantum out-states holographically induced by asymptotic flatness: invariance under spacetime symmetries, energy positivity and Hadamard property
- Equivalence of the (generalised) Hadamard and microlocal spectrum condition for (generalised) free fields in curved spacetime
- Uniqueness theorem for BMS-invariant states of scalar QFT on the null boundary of asymptotically flat spacetimes and bulk-boundary observable algebra correspondence
- The back reaction effect in particle creation in curved spacetime
- Algebras of local observables on a manifold
- Axiomatic renormalization of the stress tensor of a conformally invariant field in conformally flat spacetimes
- The generally covariant locality principle -- a new paradigm for local quantum field theory
- On the renormalization group in curved spacetime
- Microlocal analysis and interacting quantum field theories: renormalization on physical back\-grounds.
- Local quasiequivalence and adiabatic vacuum states
- Adiabatic vacuum states on general spacetime manifolds: Definition, construction, and physical properties.
- Existence of local covariant time ordered products of quantum fields in curved spacetime
- Comments on the stress-energy tensor operator in curved spacetime
- Micro-local approach to the Hadamard condition in quantum field theory on curved space-time
- The microlocal spectrum condition and Wick polynomials of free fields on curved spacetimes
- A new type of isotropic cosmological models without singularity
- Fourier integral operators. II
- DYNAMICAL BACKREACTION IN ROBERTSON–WALKER SPACETIME
- Distinguished quantum states in a class of cosmological spacetimes and their Hadamard property
- Quantum Field Theory on Curved Backgrounds
- Effective action of vacuum: the semiclassical approach
- Backreaction from non-conformal quantum fields in de Sitter spacetime
- The inverse function theorem of Nash and Moser
- EFFECTIVE ACTION FOR CONFORMAL SCALARS AND ANTIEVAPORATION OF BLACK HOLES
- MICROLOCAL SPECTRUM CONDITION AND HADAMARD FORM FOR VECTOR-VALUED QUANTUM FIELDS IN CURVED SPACETIME
- A general worldline quantum inequality
- Microlocal analysis of quantum fields on curved space–times: Analytic wave front sets and Reeh–Schlieder theorems
- Cosmological particle creation in states of low energy
- CONSERVATION OF THE STRESS TENSOR IN PERTURBATIVE INTERACTING QUANTUM FIELD THEORY IN CURVED SPACETIMES
- States of low energy on Robertson–Walker spacetimes
- RIGOROUS STEPS TOWARDS HOLOGRAPHY IN ASYMPTOTICALLY FLAT SPACETIMES
- Quantized Fields and Particle Creation in Expanding Universes. I
- Stochastic gravity: theory and applications
- Quantum annihilation of anti-de Sitter universe
- Local Wick polynomials and time ordered products of quantum fields in curved spacetime
- Massive fields temper anomaly-induced inflation: the clue to graceful exit?
This page was built for publication: On the initial conditions and solutions of the semiclassical Einstein equations in a cosmological scenario