Mixmaster universe in the z=3 deformed Hořava-Lifshitz gravity
arXiv:1001.3921 · doi:10.1007/JHEP03(2010)085
Abstract
The z=3 deformed Horava-Lifshitz gravity with coupling constants ωand εleads to a nonrelativistic "mixmaster" cosmological model. The potential of theory is given by the sum of IR and UV potentials in the ADM Hamiltonian formalism. It turns out that the presence of the UV-potential cannot suppress chaotic behaviors existing in the IR-potential, which comes from curvature anisotropy.
13 pages, 7 figures, version to appear in JHEP
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- Overall observational constraints on the running parameter λof Horava-Lifshitz gravity
- Scalar graviton in the healthy extension of Hořava-Lifshitz theory
- Comment on Ricci dark energy in Chern-Simons modified gravity
- Hořava-Lifshitz gravity inspired Bianchi-II cosmology and the mixmaster universe
- Stochastic cosmology, theories of perturbations and Lifshitz gravity
- Chaos in spatially homogeneous Hořava-Lifshitz subcritical cosmologies