Cosmological equations and Thermodynamics on Apparent Horizon in Thick Braneworld
arXiv:0710.5394 · doi:10.1007/s10714-010-0932-5
Abstract
We derive the generalized Friedmann equation governing the cosmological evolution inside the thick brane model in the presence of two curvature correction terms: a four-dimensional scalar curvature from induced gravity on the brane, and a five-dimensional Gauss-Bonnet curvature term. We find two effective four-dimensional reductions of the Friedmann equation in some limits and demonstrate that they can be rewritten as the first law of thermodynamics on the apparent horizon of thick braneworld.
25 pages, no figure, a definition corrected, several references added, more motivation and discussion
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Cited by in corpus (13)
- Hawking Radiation of Apparent Horizon in a FRW Universe
- Corrected Entropy-Area Relation and Modified Friedmann Equations
- Horizon Thermodynamics and Gravitational Field Equations in Horava-Lifshitz Gravity
- Surface Density of Spacetime Degrees of Freedom from Equipartition Law in theories of Gravity
- Thermodynamics of Apparent Horizon in Brane World Scenarios
- Thermodynamics in gravity in the Palatini formalism
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- The Unified First law in "Cosmic Triad" Vector Field Scenario