Thermodynamics and classification of cosmological models in the Horava-Lifshitz theory of gravity
arXiv:0905.4117 · doi:10.1088/1475-7516/2009/07/012
Abstract
We study thermodynamics of cosmological models in the Horava-Lifshitz theory of gravity, and systematically investigate the evolution of the universe filled with a perfect fluid that has the equation of state , where and denote, respectively, the pressure and energy density of the fluid, and is an arbitrary real constant. Depending on specific values of the free parameters involved in the models, we classify all of them into various cases. In each case the main properties of the evolution are studied in detail, including the periods of deceleration and/or acceleration, and the existence of big bang, big crunch, and big rip singularities. We pay particular attention on models that may give rise to a bouncing universe.
revtex4, 21 figures. New references added & some changes made in Introduction. Version to appear in JCAP
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- Recent advances in cosmological singularities
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- Quantization of (1+1)-dimensional Hořava-Lifshitz theory of gravity
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- Stable Singularity-free Cosmological Solutions in non-projectable Horava-Lifshitz Gravity
- Thermodynamics in Quasi-Spherical Szekeres Space-Time
- Analytical expressions for greybody factor and dynamic evolution for scalar field in Hořava-Lifshitz black hole
- The Unified First law in "Cosmic Triad" Vector Field Scenario
- Spatially homogeneous black hole solutions in Hořava-Lifshitz gravity in dimensions with Nil geometry and horizons
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- Hubble tension problem encompassed by phase-space quantum cosmology