arXiv · 1001.3921
Mixmaster universe in the z=3 deformed Ho\v{r}ava-Lifshitz gravity
Abstract
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.
Explore related subjects
Keep this discovery
Yun Soo Myung, Yong-Wan Kim, Woo-Sik Son, Young-Jai Park. 2010-01-22. Mixmaster universe in the z=3 deformed Ho\v{r}ava-Lifshitz gravity. https://doi.org/10.1007/jhep03(2010)085
Cite the original work for its findings. Save a collection to share your selection of sources.