Numerical Analysis of the Big Bounce in Loop Quantum Cosmology

dc.creatorLaguna, Pablo
dc.date2006-08-28
dc.date2007-01-29
dc.date.accessioned2026-07-07T10:24:28Z
dc.date.available2026-07-07T10:24:28Z
dc.descriptionLoop quantum cosmology homogeneous models with a massless scalar field show that the big-bang singularity can be replaced by a big quantum bounce. To gain further insight on the nature of this bounce, we study the semi-discrete loop quantum gravity Hamiltonian constraint equation from the point of view of numerical analysis. For illustration purposes, we establish a numerical analogy between the quantum bounces and reflections in finite difference discretizations of wave equations triggered by the use of nonuniform grids or, equivalently, reflections found when solving numerically wave equations with varying coefficients. We show that the bounce is closely related to the method for the temporal update of the system and demonstrate that explicit time-updates in general yield bounces. Finally, we present an example of an implicit time-update devoid of bounces and show back-in-time, deterministic evolutions that reach and partially jump over the big-bang singularity.
dc.description5 pages, 3 figures, new title, replaced with version accepted for publication
dc.identifierhttps://arxiv.org/abs/gr-qc/0608117
dc.identifierhttp://arxiv.org/abs/gr-qc/0608117
dc.identifierPhys.Rev.D75:024033,2007
dc.identifierdoi:10.1103/PhysRevD.75.024033
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176197
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleNumerical Analysis of the Big Bounce in Loop Quantum Cosmology
dc.typetext

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