Almost commutative Riemannian geometry: wave operators

preprint2011arXivOpen access

Abstract

Associated to any (pseudo)-Riemannian manifold MM of dimension nn is an n+1n+1-dimensional noncommutative differential structure $(Ω^1,\extd)$ on the manifold, with the extra dimension encoding the classical Laplacian as a noncommutative `vector field'. We use the classical connection, Ricci tensor and Hodge Laplacian to construct $(Ω^2,\extd)$ and a natural noncommutative torsion free connection (∇,σ)(\nabla,σ) on Ω1Ω^1. We show that its generalised braiding $σ:Ω^1\tensΩ^1\to Ω^1\tensΩ^1$ obeys the quantum Yang-Baxter or braid relations only when the original MM is flat, i.e their failure is governed by the Riemann curvature, and that $σ^2=\id$ only when MM is Einstein. We show that if MM has a conformal Killing vector field ττ then the cross product algebra C(M)⋊τRC(M)\rtimes_τ\R viewed as a noncommutative analogue of M×RM\times\R has a natural n+2n+2-dimensional calculus extending Ω1Ω^1 and a natural spacetime Laplacian now directly defined by the extra dimension. The case M=R3M=\R^3 recovers the Majid-Ruegg bicrossproduct flat spacetime model and the wave-operator used in its variable speed of light preduction, but now as an example of a general construction. As an application we construct the wave operator on a noncommutative Schwarzschild black hole and take a first look at its features. It appears that the infinite classical redshift/time dilation factor at the event horizon is made finite.

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