English

Canonical quantum gravity in the Vassiliev invariants arena: I. Kinematical structure

General Relativity and Quantum Cosmology 2009-10-31 v1 High Energy Physics - Theory

Abstract

We generalize the idea of Vassiliev invariants to the spin network context, with the aim of using these invariants as a kinematical arena for a canonical quantization of gravity. This paper presents a detailed construction of these invariants (both ambient and regular isotopic) requiring a significant elaboration based on the use of Chern-Simons perturbation theory which extends the work of Kauffman, Martin and Witten to four-valent networks. We show that this space of knot invariants has the crucial property -from the point of view of the quantization of gravity- of being loop differentiable in the sense of distributions. This allows the definition of diffeomorphism and Hamiltonian constraints. We show that the invariants are annihilated by the diffeomorphism constraint. In a companion paper we elaborate on the definition of a Hamiltonian constraint, discuss the constraint algebra, and show that the construction leads to a consistent theory of canonical quantum gravity.

Keywords

Cite

@article{arxiv.gr-qc/9911009,
  title  = {Canonical quantum gravity in the Vassiliev invariants arena: I. Kinematical structure},
  author = {Cayetano Di Bartolo and Rodolfo Gambini and Jorge Griego and Jorge Pullin},
  journal= {arXiv preprint arXiv:gr-qc/9911009},
  year   = {2009}
}

Comments

21 Pages, RevTex, many figures included with psfig