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- W2023113112 abstract "Three-dimensional (3D) loop quantum gravity with a vanishing cosmological constant can be related to the quantization of the SU(2) BF theory discretized on a lattice. At the classical level, this discrete model characterizes discrete flat geometries and its phase space is built from ${T}^{*}mathrm{SU}(2)$. In a recent paper [Bonzom et al., arXiv:1402.2323], this discrete model was deformed using the Poisson-Lie group formalism and was shown to characterize discrete hyperbolic geometries while still being topological. Hence, it is a good candidate to describe the discretization of SU(2) BF theory with a (negative) cosmological constant. We proceed here to the quantization of this model. At the kinematical level, the Hilbert space is spanned by spin networks built on ${mathcal{U}}_{q}(mathfrak{su}(2))$ (with $q$ real). In particular, the quantization of the discretized Gauss constraint leads naturally to ${mathcal{U}}_{q}(mathfrak{su}(2))$ intertwiners. We also quantize the Hamiltonian constraint on a face of degree 3 and show that physical states are proportional to the quantum 6j symbol. This suggests that the Turaev-Viro amplitude with $q$ real is a solution of the quantum Hamiltonian. This model is therefore a natural candidate to describe 3D loop quantum gravity with a (negative) cosmological constant." @default.
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- W2023113112 date "2014-11-24" @default.
- W2023113112 modified "2023-10-18" @default.
- W2023113112 title "Towards the Turaev-Viro amplitudes from a Hamiltonian constraint" @default.
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- W2023113112 doi "https://doi.org/10.1103/physrevd.90.104038" @default.
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