Inhomogeneities, loop quantum gravity corrections, constraint algebra and general covariance
arXiv:1311.1297 · doi:10.1088/0264-9381/31/5/055010
Abstract
Loop quantum gravity corrections, in the presence of inhomogeneities, can lead to a deformed constraint algebra. Such a deformation implies that the effective theory is no longer generally covariant. As a consequence, the geometrical concepts used in the classical theory lose their meaning. In the present paper we propose a method, based on canonical transformation on the phase space of the spherically symmetric effective theory, to systematically recover the classical constraint algebra in the presence of the inverse triad corrections as well as in the presence of the holonomy corrections. We show, by way of explicit example, that this also leads to the recovery of general covariance of the theory in the presence of inverse triad corrections, implying that one can once again use the geometrical concepts to analyze the solutions in the presence of these quantum gravity corrections.
22 pages, 2 figures, matches published version
References in corpus (6)
- Spherically Symmetric Quantum Geometry: States and Basic Operators
- Anomaly freedom in perturbative loop quantum gravity
- Loop quantum gravity corrections to gravitational wave dispersion
- Loop quantization of spherically symmetric midi-superspaces
- Non-marginal LTB-like models with inverse triad corrections from loop quantum gravity
- Lemaitre-Tolman-Bondi collapse from the perspective of loop quantum gravity
Cited by in corpus (33)
- Quantum cosmology: a review
- Polymer Schwarzschild black hole: An effective metric
- Anomaly-free cosmological perturbations in effective canonical quantum gravity
- Hypersurface-deformation algebroids and effective space-time models
- Non-singular black holes and the Limiting Curvature Mechanism: A Hamiltonian perspective
- Black Holes and Covariance in Effective Quantum Gravity
- Absorption, Scattering, Geodesics, Shadows and Lensing Phenomena of Black Holes in Effective Quantum Gravity
- Emergent modified gravity: Covariance regained
- Gravitational lensing effect of black holes in effective quantum gravity
- Protected Symmetry in Quantum Cosmology
- Non-covariance of "covariant polymerization" in models of loop quantum gravity
- A covariant polymerized scalar field in loop quantum gravity
- Black holes and covariance in effective quantum gravity: A solution without Cauchy horizons
- Effective constraint algebras with structure functions
- Emergent modified gravity: The perfect fluid and gravitational collapse
- Emergent Modified Gravity
- Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models
- Group quantization of the black hole minisuperspace
- Loop Quantum Corrected Einstein Yang-Mills Black Holes
- Space-time physics in background-independent theories of quantum gravity
- Fourth order deformed general relativity
- Formation of nonsingular spherical black holes with holonomy corrections
- Testing general covariance in effective models motivated by Loop Quantum Gravity
- Covariant effective spacetimes of spherically symmetric electrovacuum with a cosmological constant
- New second derivative theories of gravity for spherically symmetric spacetimes
- Lessons for loop quantum gravity from emergent modified gravity
- The general scalar-tensor Hamiltonian with deformed covariance
- Hamiltonian consistency of the gravitational constraint algebra under deformations
- Dynamically implementing the -scheme in cosmological and spherically symmetric models in an extended phase space model
- Deformed general relativity
- Midisuperspace quantization: possibilities for fractional and emergent spacetime dimensions
- Symmetries of space-time
- Singularities in loop quantum cosmology