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It might be that spacetime is not fully quantized in a standard sense. Spacetime physics may be quantized by a a series lagrangian of the form
R α'R_{abcd}R^{abcd} α'^2 O(R^4) ...
Where the R is a classical background and the string parameter α' give corrections in order of the string tension; similar to O(ħ) as the string tension is due to the Heisenberg uncertainty principle. Of course this is a sticking point for the LQG folks, and this background independence issue is the one big card they hold in their hand.
However, a full quantum theory of spacetime in the LQG sense runs into trouble by placing lots of degrees of freedom in spacetime, and by corollary a huge entropy. The classical limit of LQG is not physically tenable. So any quantization of spacetime curvature may simply only work as an effective theory, whether that be with orders in string parameter or with LQG Sen connection terms.
The hyperbolic plane, or the anti de Sitter spacetime, is S-dual to a Thirring fermion field. The horizon limit of an AdS_n spacetime containing a black hole his an AdS_2 ~ H_2. This contains all the conformal machinery of CFT_1, which is the Hartle-Hawking vacuum. The S-dual to the soliton dynamics in H_2 is the Thirring Fermions, which in the interior of the AdS defines the "graviton." The Thirring field has the Lagrangian
L = {bar-ψ}γ^a∂_aψ g|ψψ|^2
Where we might think of the graviton as having a substratum of quantized fermions.
Cheers LC