Quantum Theory at Planck Scale, Limiting Values, Deformed Gravity and Dark Energy Problem
arXiv:1102.5084 · doi:10.1142/S0218271812500137
Abstract
Within a theory of the existing fundamental length on the order of Planck's a high-energy deformation of the General Relativity for the space with horizon has been constructed. On this basis, Markov's work of the early eighties of the last century has been given a new interpretation to show that the heuristic model considered by him may be placed on a fundamental footing. The obtained results have been applied to solving of the dark energy problem, making it possible to frame the following hypothesis: a dynamic cosmological term is a measure of deviation from a thermodynamic identity (the first law of thermodynamics) of the high-energy (Planck's) deformation of Einstein equations for horizon spaces in their thermodynamic interpretation.
30 pages, Latex. arXiv admin note: substantial text overlap with arXiv:1003.4523, arXiv:0911.5597, arXiv:1006.4979
References in corpus (18)
- Thermodynamical Aspects of Gravity: New insights
- Thermodynamic route to Field equations in Lanczos-Lovelock Gravity
- Dark Energy and Gravity
- Infrared-modified gravities and massive gravitons
- Quantum-corrected black hole thermodynamics to all orders in the Planck length
- The Generalized Uncertainty Principle in (A)dS Space and the Modification of Hawking Temperature from the Minimal Length
- Decay of Vacuum Energy
- Entropy of Null Surfaces and Dynamics of Spacetime
- Prospects for constraining quantum gravity dispersion with near term observations
- Holography of Gravitational Action Functionals
- Running Coupling with Minimal Length
- Gravity: A New Holographic Perspective
- Time and M-theory
- Infrared Modified Gravity with Dynamical Torsion
- A revision of the Generalized Uncertainty Principle
- Entropy bound of local quantum field theory with generalized uncertainty principle
- Why there is something so close to nothing: towards a fundamental theory of the cosmological constant
- Entropy In The Present And Early Universe: New Small Parameters And Dark Energy Problem