Abstract
We examine the Hamiltonian dynamics of bouncing Bianchi IX cosmologies with three scale factors in Hořava-Lifshitz (HL) gravity. We assume a positive cosmological constant plus noninteracting dust and radiation as the matter content of the models. In this framework the modified field equations contain additional terms which turn the dynamics nonsingular. The six-dimensional phase space presents (i) two critical points in a finite region of the phase space, (ii) one asymptotic de Sitter attractor at infinity and (iii) a two-dimensional invariant plane containing the critical points; together they organize the dynamics of the phase space. We identify four distinct parameter domains , , and for which the pair of critical points engenders distinct features in the dynamics, connected to the presence of centers of multiplicity 2 and saddles of multiplicity 2. In the domain the dynamics consists basically of periodic bouncing orbits, or oscillatory orbits with a finite number of bounces before escaping to the de Sitter attractor. The center with multiplicity 2 engenders in its neighborhood the topology of stable and unstable cylinders of orbits, where is a saddle direction and is the center manifold of unstable periodic orbits. We show that the stable and unstable cylinders coalesce, realizing a smooth homoclinic connection to the center manifold, a rare event of regular/nonchaotic dynamics in bouncing Bianchi IX cosmologies. The presence of a saddle of multiplicity 2 in the domain engenders a high instability in the dynamics so that the cylinders emerging from the center manifold about towards the bounce have four distinct attractors: the center manifold itself, the de Sitter attractor at infinity and two further momentum-dominated attractors with infinite anisotropy. In the domain we examine the features of invariant manifolds of orbits about a saddle of multiplicity 2 . The presence of the saddle of multiplicity 2 engenders bifurcations of the invariant manifold as the energy of the system increases relative to the energy of : (i) for the invariant manifold has the topology ; (ii) for two points of pinch into the point , so that the invariant manifold contains infinitely many orbits homoclinic to ; (iii) for the center manifold bifurcates into a 3-torus; (iv) for sufficiently large the 3-torus bifurcates into three , an invariant manifold multiply connected. Such structures were not yet observed in the literature. The domain is not examined as most of its features are present already in the previous domains.
9 More- Received 31 May 2017
- Corrected 14 February 2018
DOI:https://doi.org/10.1103/PhysRevD.96.103532
© 2017 American Physical Society
Physics Subject Headings (PhySH)
Corrections
14 February 2018