Invariant Correlations in Simplicial Gravity
arXiv:hep-th/9311024 · doi:10.1103/PhysRevD.50.3932
Abstract
Some first results are presented regarding the behavior of invariant correlations in simplicial gravity, with an action containing both a bare cosmological term and a lattice higher derivative term. The determination of invariant correlations as a function of geodesic distance by numerical methods is a difficult task, since the geodesic distance between any two points is a function of the fluctuating background geometry, and correlation effects become rather small for large distances. Still, a strikingly different behavior is found for the volume and curvature correlation functions. While the first one is found to be negative definite at large geodesic distances, the second one is always positive for large distances. For both correlations the results are consistent in the smooth phase with an exponential decay, turning into a power law close to the critical point at . Such a behavior is not completely unexpected, if the model is to reproduce the classical Einstein theory at distances much larger than the ultraviolet cutoff scale.
27 pages, conforms to published version
References in corpus (4)
Cited by in corpus (30)
- Spin Networks and Quantum Gravity
- Observables in effective gravity
- Discrete approaches to quantum gravity in four dimensions
- Observables, gravitational dressing, and obstructions to locality and subsystems
- Nonlocal Effective Gravitational Field Equations and the Running of Newton's G
- Scaling in four dimensional quantum gravity
- Newtonian Potential in Quantum Regge Gravity
- On the Gravitational Scaling Dimensions
- Fluctuating geometries, q-observables, and infrared growth in inflationary spacetimes
- Gauge Invariance in Simplicial Gravity
- Non-Perturbative Gravity and the Spin of the Lattice Graviton
- Scaling Exponents for Lattice Quantum Gravity in Four Dimensions
- Two-point functions in 4D dynamical triangulation
- Discrete Wheeler-DeWitt Equation
- Decoherence in Quantum Gravity: Issues and Critiques
- Renormalization Group Running of Newton's G: The Static Isotropic Case
- Vacuum Condensate Picture of Quantum Gravity
- On the absence of localized curvature in the weak-coupling phase of quantum gravity
- One-loop quantum gravitational corrections to the scalar two-point function at fixed geodesic distance
- Scale-Dependent Newton's Constant G in the Conformal Newtonian Gauge
- Cosmological Density Perturbations with a Scale-Dependent Newton's G
- On the structure of a background independent quantum theory: Hamilton function, transition amplitudes, classical limit and continuous limit
- Static Quark Potentials in Quantum Gravity
- Heat kernel coefficients for massive gravity
- Gravitational Fluctuations as an Alternative to Inflation
- Phase diagram of Regge quantum gravity coupled to SU(2) gauge theory
- Correlation functions in lattice formulations of quantum gravity
- Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum
- A Reasonable Ab Initio Cosmological Constant Without Holography
- Combinatorial Dark Energy