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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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The spin foam representation of loop quantum gravity 287some tetrad e. The remarkable fact is that the constraint B = ⋆(e∧e) can be directlyimplemented on the spin foam configurations of P <strong>to</strong>po by appropriate restriction onthe allowed spin labels and intertwiners. All this is possible if a regularization isprovided, consisting of a cellular decomposition of the spacetime manifold. Thekey open issue is, however, how <strong>to</strong> get rid of this regula<strong>to</strong>r. A proposal for a regula<strong>to</strong>rindependent definition is that of the group field theory formulation presentedin Chapter 17 by Oriti.A second proposal is the one recently introduced by Freidel and Starodubtsev[14] based on the formulation McDowell–Mansouri action of Riemannian gravitygiven by∫S[B, A] = Tr[B ∧ F(A) − α 4 B ∧ Bγ 5], (15.25)where B is an so(5)-valued two-form, A an so(5) connection, α = G/3 ≈10 −120 a coupling constant, and the γ 5 in the last term produces the symmetrybreaking SO(5) → SO(4). The idea is <strong>to</strong> define P GR as a power series in α, namely∞∑ (−iα) n ∫[ ∫ ]P GR =D[B]D[A](Tr[B ∧ Bγ4 n 5 ]) n exp i Tr[B ∧ F] . (15.26)n!n=0Notice that each term in the sum is the expectation value of a certain power of Bsinthe well unders<strong>to</strong>od <strong>to</strong>pological BF field theory. A regula<strong>to</strong>r in the form of a cellulardecomposition of the spacetime manifold is necessary <strong>to</strong> give a meaning <strong>to</strong> the formerexpression. Because of the absence of local degrees of freedom of BF-theoryit is expected that the regula<strong>to</strong>r can be removed in analogy <strong>to</strong> the 2 + 1 gravitycase. It is important <strong>to</strong> show that removing the regula<strong>to</strong>r does not produce anuncontrollable set of ambiguities (see remarks below regarding renormalizability).15.4.1 The UV problem in the background independent contextIn the spin foam representation, the functional integral for gravity is replaced bya sum over amplitudes of combina<strong>to</strong>rial objects given by foam-like configurations(spin foams). This is a direct consequence of the background independent treatmen<strong>to</strong>f the gravitational field degrees of freedom. As a result there is no place for the UVdivergences that plague standard <strong>Quantum</strong> Field Theory. The combina<strong>to</strong>rial natureof the fundamental degrees of freedom of geometry appears as a regula<strong>to</strong>r of allthe interactions. This seem <strong>to</strong> be a common feature of all the formulations referred<strong>to</strong> in this chapter. Does it mean that the UV problem in LQG is resolved? Theanswer <strong>to</strong> this question remains open for the following reason. All the definitionsof spin foams models require the introduction of some kind of regula<strong>to</strong>r genericallyrepresented by a space (e.g. in the canonical formulation of 2 + 1 gravity or in the

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