A Quantum Complete Prelude to Inflation
arXiv:1901.04492 · doi:10.1103/PhysRevD.99.065012
Abstract
It is shown that the inflationary paradigm admits quantum complete extensions of space-time. The extended inflationary spacetimes still have geodesic borders, but quantum fields are prohibited from migrating across these borders by their evolution semigroups. The geodesic singularities lurking across the borders lack a physical description because the evolution semigroups give vanishing probabilistic support to quantum fields for populating regions bordering on these singularities. As an example, anisotropic Bianchi type-I cosmologies are shown to be quantum complete preludes to inflation. They admit Kasner-like geometries close to their geodesic borders. Quantum fields enjoy a contractive evolution in these asymptotic regions and ultimately become free. As a consequence, quantum probes cannot migrate across the geodesic border of Bianchi type-I cosmologies.
8 pages
References in corpus (12)
- Loop quantum cosmology of Bianchi I models
- Theory of cosmological perturbations in an anisotropic universe
- Inflationary perturbations in anisotropic backgrounds and their imprint on the CMB
- No smooth beginning for spacetime
- Perfect Quantum Cosmological Bounce
- A Hamiltonian Formulation of the BKL Conjecture
- Unitarity and ultraviolet regularity in cosmology
- Gravity Waves Signatures from Anisotropic pre-Inflation
- Hamiltonian General Relativity and the Belinskii, Khalatnikov, Lifshitz Conjecture
- Classical versus quantum completeness
- Perturbations of generic Kasner spacetimes and their stability
- Non-Gaussian ground-state deformations near a black-hole singularity
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- Geometric flavours of Quantum Field theory on a Cauchy hypersurface. Part II: Methods of quantization and evolution
- Geometric flavours of Quantum Field theory on a Cauchy hypersurface. Part I: Gaussian analysis and other Mathematical aspects
- A local diagnostic program for unitary evolution in general space-times
- Unitarity in the Schroedinger Formalism of QFT in Curved Space-Time