Lessons for loop quantum gravity from emergent modified gravity
arXiv:2411.17545 · doi:10.1103/PhysRevD.111.086027
Abstract
Most of the potential physical effects of loop quantum gravity have been derived in effective models that modify the constraints of canonical general relativity in specific forms. Emergent modified gravity evaluates important conditions that ensure the existence of a compatible geometrical space-time interpretation of canonical solutions, as well as phase-space covariance under different choices of canonical variables. This setting, specialized to modifications suggested by loop quantum gravity, is therefore an important contribution to physical evaluations of this approach to quantum gravity. Here, it is shown that emergent modified gravity restricts several ambiguities that existed in previous formulations, rules out several specific candidates, and provides a unified treatment of different types of (holonomy) modifications that had been thought to be physically distinct.
31 pages
References in corpus (39)
- The Dynamics of General Relativity
- Quantum Nature of the Big Bang: Improved dynamics
- Loop quantization of the Schwarzschild black hole
- Quantum Oppenheimer-Snyder and Swiss Cheese models
- The Area Operator in the Spherically Symmetric Sector of Loop Quantum Gravity
- Quantum Symmetry Reduction for Diffeomorphism Invariant Theories of Connections
- Spherically Symmetric Quantum Geometry: States and Basic Operators
- Spherically Symmetric Quantum Geometry: Hamiltonian Constraint
- Deformed General Relativity and Effective Actions from Loop Quantum Gravity
- Effective loop quantum gravity framework for vacuum spherically symmetric space-times
- Effective line elements and black-hole models in canonical (loop) quantum gravity
- Loop quantum cosmology and inhomogeneities
- Lattice refining loop quantum cosmology, anisotropic models and stability
- Covariance in models of loop quantum gravity: Spherical symmetry
- An effective model for the quantum Schwarzschild black hole
- Anomaly-free cosmological perturbations in effective canonical quantum gravity
- Quantum gravity of dust collapse: shock waves from black holes
- Some implications of signature-change in cosmological models of loop quantum gravity
- Observational Exclusion of a Consistent Quantum Cosmology Scenario
- Covariance in models of loop quantum gravity: Gowdy systems
- Spherically symmetric Einstein-Maxwell theory and loop quantum gravity corrections
- Spherically symmetric canonical quantum gravity
- Inhomogeneities, loop quantum gravity corrections, constraint algebra and general covariance
- Emergent modified gravity: Covariance regained
- Anomaly-free deformations of spherical general relativity coupled to matter
- Hawking radiation from a spherical loop quantum gravity black hole
- Singularity resolution by holonomy corrections: Spherical charged black holes in cosmological backgrounds
- Shell-crossings and shock formation during gravitational collapse in effective loop quantum gravity
- Non-covariance of "covariant polymerization" in models of loop quantum gravity
- Holonomy and inverse-triad corrections in spherical models coupled to matter
- Loop Quantization of Polarized Gowdy Model on : Classical Theory
- Preinflationary perturbations from the closed algebra approach in loop quantum cosmology
- Emergent modified gravity: The perfect fluid and gravitational collapse
- Emergent modified gravity coupled to scalar matter
- Emergent Modified Gravity
- A new type of large-scale signature change in emergent modified gravity
- Inequivalence of mimetic gravity with models of loop quantum gravity
- Uniqueness of Galilean and Carrollian limits of gravitational theories and application to higher derivative gravity
- Emergent modified gravity: Polarized Gowdy model on a torus