Mixmaster universe in the z=3 deformed Hořava-Lifshitz gravity

Details Mixmaster universe in the z=3 deformed Hořava-Lifshitz gravity Mixmaster universe in the z=3 deformed Hořava-Lifshitz gravity

2010-01-22

arxiv.org/abs/1001.3921v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, 7 figures, version to appear in JHEP

Scientific paper

The z=3 deformed Horava-Lifshitz gravity with coupling constants \omega and \epsilon leads 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.

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