The holographic bound in the scalar-tensor and gravities
arXiv:1301.2769 · doi:10.1140/epjc/s10052-013-2595-3
Abstract
The holographic bound has been extended to the different theory of gravities such as scalar-tensor gravity and gravity according to the Noether charge definition of the entropy for a black hole surface. We have introduced some popular examples of the flat FRW cosmology in order to investigate holographic bound in scalar-tensor and gravity. Using the holographic bound, we put an additional constraint on the scalar-tensor gravity and gravity parameters. We also discuss about the transformation from Jordan frame to Einstein frame.
accepted in European Physical Journal C (epjc), a section added to the paper
References in corpus (6)
- The (pseudo)issue of the conformal frame revisited
- Black hole entropy in modified gravity models
- The conformal transformation's controversy: what are we missing?
- Noether Charge and Black Hole Entropy in Modified Theories of Gravity
- Cardy-Verlinde formula in FRW Universe with inhomogeneous generalized fluid and dynamical entropy bounds near the future singularity
- The horizon-entropy increase law for causal and quasi-local horizons and conformal field redefinitions