arXiv Analytics

Sign in

arXiv:1801.05690 [gr-qc]AbstractReferencesReviewsResources

Regularization of the big bang singularity with random perturbations

Edward Belbruno, BingKan Xue

Published 2018-01-13Version 1

We show how to regularize the big bang singularity in the presence of random perturbations modeled by Brownian motion using stochastic methods. We prove that the physical variables in a contracting universe dominated by a scalar field can be continuously and uniquely extended through the big bang as a function of time to an expanding universe only for a discrete set of values of the equation of state satisfying special co-prime number conditions. This result significantly generalizes a previous result \cite{Xue:2014} that did not model random perturbations. This result implies that the extension from a contracting to an expanding universe for the discrete set of co-prime equation of state is robust, which is a surprising result. Implications for a purely expanding universe are discussed, such as a non-smooth, randomly varying scale factor near the big bang.

Related articles: Most relevant | Search more
arXiv:2202.11458 [gr-qc] (Published 2022-02-23)
Initial data on big bang singularities in symmetric settings
arXiv:1602.02456 [gr-qc] (Published 2016-02-08)
On The Big Bang Singularity in $k=0$ FLRW Cosmologies
arXiv:2002.03551 [gr-qc] (Published 2020-02-10)
Thurston boundary of the Teichmüller space is the space of big bang singularities of 2+1 gravity