Numerical evolution of squeezed and non-Gaussian states in loop quantum cosmology

DOI10.1088/0264-9381/31/16/165006zbMath1298.83126arXiv1406.1486OpenAlexW2093174556WikidataQ62273555 ScholiaQ62273555MaRDI QIDQ3190749

Brajesh Gupt, Peter Diener, Parampreet Singh, Miguel Megevand

Publication date: 19 September 2014

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1406.1486

zbMATH Keywords

numerical simulationloop quantum cosmologyquantum evolutionquantum bounce

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of statistics to physics (62P35) Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45) Space-time singularities, cosmic censorship, etc. (83C75) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Related Items (7)

A diffeomorphism invariant family of metric-affine actions for loop cosmologies ⋮ Pulsation of black holes ⋮ From black holes to white holes: a quantum gravitational, symmetric bounce ⋮ Noncommutative Friedmann equations in effective LQC ⋮ Generic absence of strong singularities in loop quantum Bianchi-IX spacetimes ⋮ von-Neumann stability and singularity resolution in loop quantized Schwarzschild black hole ⋮ Basis function method for numerical loop quantum cosmology: the Schwarzschild black hole interior

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