Quantum deformation of quantum gravity
Seth Major, Lee Smolin
TL;DR
The paper proposes a q-deformation of the loop representation of quantum gravity by elevating loops to framed loops, with the deformation parameter $q = e^{ i \hbar^2 G^2 \Lambda /6}$ tied to the cosmological constant. It develops a framed-loop algebra $\mathcal{LA}^f$ and a $q$-spin-net basis that yields a closed, commuting operator algebra $\hat{T}_q[\alpha]$ and a $q$-deformed area operator with discrete spectra, together with eigenstates of $\hat{T}_q[\alpha]$ and potential pathways to a $q$-deformed connection representation. The framework connects Chern–Simons/Kauffman-bracket topology to nonperturbative quantum gravity, suggesting a Kodama phase where framing counts twist and offering a diffeomorphism-invariant infrared regulator. These constructions may illuminate nonperturbative vacuum structure in quantum gravity with a cosmological constant and provide practical tools for calculations via recoupling theory in the $q$-deformed setting.
Abstract
We describe a deformation of the observable algebra of quantum gravity in which the loop algebra is extended to framed loops. This allows an alternative nonperturbative quantization which is suitable for describing a phase of quantum gravity characterized by states which are normalizable in the measure of Chern-Simons theory. The deformation parameter, q, depends on the cosmological constant. The Mandelstam identities are extended to a set of relations which are governed by the Kauffman bracket so that the spin network basis is deformed to a basis of SU(2)q spin networks. Corrections to the actions of operators in non-perturbative quantum gravity may be readily computed using recoupling theory; the example of the area observable is treated here. Finally, eigenstates of the q-deformed Wilson loops are constructed, which may make possible the construction of a q-deformed connection representation through an inverse transform.
