Gravity's rainbow: a bridge between LQC and DSR
arXiv:1606.00910 · doi:10.1016/j.physletb.2016.12.023
Abstract
The doubly special relativity (DSR) theories are investigated in order to take into account an observer-independent length scale in special relativity framework. It is widely believed that any quantum theory of gravity would reduce to a DSR model at the flat limit when purely gravitational and quantum mechanical effects are negligible. Gravity's rainbow is a simple generalization of DSR theories to incorporate gravity. In this paper, we show that the effective Friedmann equations that are suggested by loop quantum cosmology (LQC) can be exactly reobtained in rainbow cosmology setup. The deformed geometry of LQC then completely fixes the modified dispersion relation and results in unique DSR model. In comparison with standard LQC scenario where only the geometry is modified, both of the geometry and matter parts get modifications in our setup. In this respect, we find that the total number of microstates for the universe is finite which suggests the statistical origin for the energy and entropy density bounds. These results explicitly show that the DSR theories are appropriate candidates for the flat limit of loop quantum gravity.
10 pages, 4 figures, Refs. added
References in corpus (14)
- Quantum Nature of the Big Bang: Improved dynamics
- Quantum Nature of the Big Bang
- Universality of Quantum Gravity Corrections
- Remnant for all Black Objects due to Gravity's Rainbow
- Absence of Black Holes at LHC due to Gravity's Rainbow
- Critical behavior of charged black holes in Gauss-Bonnet gravity`s rainbow
- Speed of particles and a relativity of locality in -Minkowski quantum spacetime
- Vaidya Spacetime for Galileon Gravity's Rainbow
- Spacetime-noncommutativity regime of Loop Quantum Gravity
- Photon Gas Thermodynamics in Doubly Special Relativity
- Thermodynamics of Photon Gas with an Invariant Energy Scale
- Deformed Special Relativity in Position Space
- Could deformed special relativity naturally arise from the semiclassical limit of quantum gravity?
- Early universe thermostatistics in curved momentum spaces
Cited by in corpus (13)
- Recent progress on the description of relativistic spin: vector model of spinning particle and rotating body with gravimagnetic moment in General Relativity
- Thermal fluctuations of charged black holes in gravity's rainbow
- Quantum corrected thermodynamics of nonlinearly charged BTZ black holes in massive gravity's rainbow
- Inflation from theories in gravity's rainbow
- Quantum Configuration and Phase Spaces: Finsler and Hamilton Geometries
- Quantum corrections to the thermodynamics and phase transition of a black hole surrounded by a cavity in the extended phase space
- The extended phase space thermodynamics of Planck-scale-corrected Reissner-Nordström-anti-de Sitter black hole
- Equilibrium properties of blackbody radiation with an ultraviolet energy cut-off
- 5-Dimensional -Invariant Action as an Origin to the Magueijo-Smolin Doubly Special Relativity Proposal
- Observational Constraints on Asymptotic Safety Inflation in Gravity Rainbow
- Gravitational baryogenesis in gravity's rainbow
- Thermodynamic analysis of a compact object in Rastall-Rainbow gravity
- The effect of loop quantum gravitational rainbow functions on the formation of naked singularities