arXiv Analytics

Sign in

arXiv:1001.2663 [gr-qc]AbstractReferencesReviewsResources

Cosmic recall and the scattering picture of Loop Quantum Cosmology

Wojciech Kaminski, Tomasz Pawlowski

Published 2010-01-15Version 1

The global dynamics of a homogeneous universe in Loop Quantum Cosmology is viewed as a scattering process of its geometrodynamical equivalent. This picture is applied to build a flexible (easy to generalize) and not restricted just to exactly solvable models method of verifying the preservation of the semiclassicality through the bounce. The devised method is next applied to two simple examples: (i) the isotropic Friedman Robertson Walker universe, and (ii) the isotropic sector of the Bianchi I model. For both of them we show, that the dispersions in the logarithm of the volume ln(v) and scalar field momentum ln(p_phi) in the distant future and past are related via strong triangle inequalities. This implies in particular a strict preservation of the semiclassicality (in considered degrees of freedom) in both the cases (i) and (ii). Derived inequalities are general: valid for all the physical states within the considered models.

Comments: RevTex4, 19 pages, 3 figures
Journal: Phys.Rev.D81:084027,2010
Categories: gr-qc
Related articles: Most relevant | Search more
arXiv:1207.5601 [gr-qc] (Published 2012-07-24, updated 2012-12-31)
Dynamical eigenfunctions and critical density in loop quantum cosmology
arXiv:0811.2790 [gr-qc] (Published 2008-11-17)
Comment on "Quantum bounce and cosmic recall" [arXiv:0710.4543]
arXiv:0906.3751 [gr-qc] (Published 2009-06-22)
Physical evolution in Loop Quantum Cosmology: The example of vacuum Bianchi I