Scalar perturbations in scalar field quantum cosmology

DOI10.1103/PhysRevD.79.023507zbMath1222.83066arXiv0810.3542MaRDI QIDQ3093664

F. T. Falciano, Nelson Pinto-Neto

Publication date: 18 October 2011

Published in: Physical Review D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0810.3542

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantization of the gravitational field (83C45)

Related Items (7)

Benefits of objective collapse models for cosmology and quantum gravity ⋮ Cosmological models with asymmetric quantum bounces ⋮ Non-oscillating power spectra in loop quantum cosmology ⋮ BOUNCING AND QUANTUM THEORY ⋮ Gauge invariant canonical cosmological perturbation theory with geometrical clocks in extended phase-space — A review and applications ⋮ Bianchi type I, Schutz perfect fluid and evolutionary quantum cosmology ⋮ Bohmian quantization of the big-brake singularity

Cites Work

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• Quantization of Friedmann cosmological models with two fluids: dust plus radiation
• The accelerated expansion of the Universe as a quantum cosmological effect
• Quantum cosmological perfect fluid models
• The consistency of causal quantum geometrodynamics and quantum field theory
• Notes on semiclassical gravity
• Hamiltonian formalism and gauge invariance for linear perturbations in inflation
• Scalar and vector perturbations in quantum cosmological backgrounds
• THE CAUSAL INTERPRETATION OF QUANTUM MECHANICS AND THE SINGULARITY PROBLEM AND TIME ISSUE IN QUANTUM COSMOLOGY
• Tensor perturbations in quantum cosmological backgrounds

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