A generalized Kasner transition for bouncing Bianchi I models in modified gravity theories
arXiv:1910.03616 · doi:10.1088/1475-7516/2019/12/039
Abstract
We derive transition rules for Kasner exponents in bouncing Bianchi I models with generic perfect fluid matter fields for a broad class of modified gravity theories where cosmological singularities are resolved and replaced by a non-singular bounce. This is a generalization of results obtained previously in limiting curvature mimetic gravity and loop quantum cosmology. A geometric interpretation is provided for the transition rule as a linear map in the Kasner plane. We show that the general evolution of anisotropies in a Bianchi I universe -- including during the bounce phase -- is equivalent to the motion of a point particle on a sphere, where the sphere is the one-point compactification of the Kasner plane. In addition, we study the evolution of anisotropies in a large family of bouncing Bianchi I space-times. We also present a novel explicit solution to the Einstein equations for a Bianchi I universe with ekpyrotic matter with a constant equation of state .
28 pages, 2 figures; v2: references added; accepted for publication in JCAP
References in corpus (13)
- Resummation of Massive Gravity
- Covariant Galileon
- Imperfect Dark Energy from Kinetic Gravity Braiding
- Towards a Nonsingular Bouncing Cosmology
- Galilean Genesis: an alternative to inflation
- A Matter Bounce By Means of Ghost Condensation
- Anisotropy in a Nonsingular Bounce
- The behavior of non-linear anisotropies in bouncing Bianchi I models of loop quantum cosmology
- Quantum gravitational Kasner transitions in Bianchi-I spacetime
- Classical and Quantum Features of the Mixmaster Singularity
- Non-Singular Bounces Catalysed by Dark Energy
- Reconstruction of mimetic gravity in a non-singular bouncing universe from quantum gravity
- Mixmaster dynamics in the dust time gauge