Quantum Riemannian geometry of the discrete interval and q-deformation
arXiv:2204.12212 · doi:10.1063/5.0133982
Abstract
We solve for quantum Riemannian geometries on the finite lattice interval with nodes (the Dynkin graph of type ) and find that they are necessarily -deformed with . This comes out of the intrinsic geometry and not by assuming any quantum group in the picture. Specifically, we discover a novel `boundary effect' whereby, in order to admit a quantum-Levi Civita connection, the `metric weight' at any edge is forced to be greater pointing towards the bulk compared to towards the boundary, with ratio given by at node , where is a -integer. The Christoffel symbols are also q-deformed. The limit likewise forces the quantum Riemannian geometry of the natural numbers to have rational metric multiples in the direction of increasing . In both cases, there is a unique Ricci-scalar flat metric up to normalisation. Elements of quantum field theory and quantum gravity are exhibited for and for the continuum limit of the geometry of . The Laplacian for the scalar-flat metric becomes the Airy equation operator in so far as a limit exists. Scaling this metric by a conformal factor gives a limiting Ricci scalar curvature proportional to .
arXiv comment35 pages AMS latex, 8 figures. Some corrections to the formulae in Sections 5,6 for the Laplacian and Ricci
References in corpus (13)
- The quantum structure of spacetime at the Planck scale and quantum fields
- Bicrossproduct structure of -Poincare group and non-commutative geometry
- Loop quantum cosmology of k=1 FRW models
- Quantization of Point Particles in 2+1 Dimensional Gravity and Space-Time Discreteness
- Dynamically Triangulating Lorentzian Quantum Gravity
- Connections on central bimodules
- Gravity induced from quantum spacetime
- Quantum gravity on a square graph
- Quantum Riemannian geometry and particle creation on the integer line
- Path Integral Quantisation of Finite Noncommutative Geometries
- Quantum gravity on polygons and FLRW model
- Fuzzy and discrete black hole models
- Riemannian Geometry of a Discretized Circle and Torus