Bianchi-I cosmological model and crossing singularities
arXiv:1702.02314 · doi:10.1103/PhysRevD.95.083503
Abstract
We consider a rather simple method for the description of the Big Bang - Big Crunch cosmological singularity crossing. For the flat Friedmann universe this method gives the same results as more complicated methods, using Weyl symmetry or the transitions between the Jordan and Einstein frames. It is then easily generalized for the case of a Bianchi-I anisotropic universe. We also present early-time and late-time asymptotic solutions for a Bianchi-I universe, filled with a conformally coupled massless scalar field.
11 pages, v2: accepted for publication in Phys. Rev. D
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