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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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286 A. PerezA spin foam representation of the previous expression is obtained by splitting thet-parameter in discrete steps and writinge it ̂M = limn→∞ [eit ̂M/n ] n = lim [1 + it ̂M/n] n . (15.21)n→∞The spin foam representation follows from the fact that the action of the basicopera<strong>to</strong>r 1+it ̂M/n on a spin network can be written as a linear combination of newspin networks whose graphs and labels have been modified by the creation of newnodes (in a way qualitatively analogous <strong>to</strong> the local action shown in Fig. 15.11).An explicit derivation of the physical inner product of 4d LQG along these lines isunder current investigation.Spin foam representation: the covariant perspectiveIn four dimensions the spin foam representation of LQG has also been motivatedby lattice discretizations of the path integral of gravity in the covariant formulation(for recent reviews see [7; 8] and Chapter 16 by Freidel). In four dimensions thereare two main lines of approach; both are based on classical formulations of gravitybased on modifications of the BF-theory action.The first approach is best represented by the Barrett–Crane model [11] andcorresponds<strong>to</strong> the quantization attempt of the classical formulation of gravity basedon the Plebanski action∫S[B, A,λ]= Tr [B ∧ F(A) + λ B ∧ B] , (15.22)where B is an so(3, 1)-valued two-form λ is a Lagrange multiplier imposing aquadratic constraint on the Bs whose solutions include the sec<strong>to</strong>r B = ⋆(e ∧ e),for a tetrad e, corresponding <strong>to</strong> gravity in the tetrad formulation. The key idea inthe definition of the model is that the path integral for BF-theory, whose action isS[B, A, 0],∫P <strong>to</strong>po =[ ∫D[B]D[A] exp i]Tr [B ∧ F](15.23)can be defined in terms of spin foams by a simple generalization of the constructionof Section 15.3 [13]. Notice that the formal structure of the action S[B, A, 0] isanalogous <strong>to</strong> that of the action of 2 + 1 gravity (15.2) (see[12]). The Barrett–Crane model aims at providing a definition of the path integral of gravity formallywritten as∫P GR =[ ∫D[B]D[A] δ [B → ⋆(e ∧ e)] exp i]Tr [B ∧ F] , (15.24)where the measure D[B]D[A]δ[B → ⋆(e∧e)] restricts the sum in (15.23) <strong>to</strong> thoseconfigurations of the <strong>to</strong>pological theory satisfying the constraints B = ⋆(e ∧ e) for

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