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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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324 D. Oritiwhere: g i ∈ G, s i ∈ R, μ =±1andα i =±1 are orientation data that allowone <strong>to</strong> reconstruct the orientation of the Feynman graph from the complex amplitudeassociated <strong>to</strong> it, φ + (g i , s i ) = φ(g 1 , s 1 ; ..., g 4 , s 4 ) and φ − (g i , s i ) = φ † (g i , s i ),P h is the projec<strong>to</strong>r imposing invariance under the SO(3) subgroup, ∇ is theD’Alembertian opera<strong>to</strong>r on the group G, θ(s) is the step function and K (g, s)is the evolution kernel for a scalar particle on the group manifold G with evolutionparameter s. The field is assumed invariant under the diagonal action of G asdescribed above. The form of the kinetic and vertex opera<strong>to</strong>r impose a non-trivialdependence on the orientation data in fully covariant way. The resulting Feynmanamplitudes [24] have all the properties wanted, being complex and orientationdependent,and have the natural interpretation as analogs of Feynman transitionamplitudes for <strong>Quantum</strong> <strong>Gravity</strong> [24; 29]. Also, when expressed in terms of thevariables conjugate <strong>to</strong> the s i , the amplitude for each vertex is given by the exponentialof the Regge action in first order formalism, times an appropriate measurefac<strong>to</strong>r [24]. It remains <strong>to</strong> be proven that this also holds for the amplitude associated<strong>to</strong> the whole Feynman graph [30; 31]. Other models based on the same formalismand same type of field, but differing, for example, in the expression for the vertexterm can also be constructed, and share similar properties [31].Other types of GFTs have been constructed in the literature, ranging from aBoula<strong>to</strong>v-like model for 3d gravity based on the quantum group DSU(2) [32],with links <strong>to</strong> models of 3d <strong>Quantum</strong> <strong>Gravity</strong> coupled <strong>to</strong> matter mentioned below,<strong>to</strong> a modified version [33] of the GFTs for the Barrett–Crane models, with a tunableextra coupling among the 4-simplices and a possible use in the renormalization ofspin foam models. For all this we refer <strong>to</strong> the literature. We refer <strong>to</strong> the literaturealso for the recent construction of group field theory models for <strong>Quantum</strong> <strong>Gravity</strong>coupled <strong>to</strong> matter fields of any mass and spin in 3d [34; 35; 36], for work inprogress concerning the 4d case (coupling of <strong>Quantum</strong> <strong>Gravity</strong> and gauge fields,of <strong>to</strong>pological gravity and strings, etc.), and for the proposal of re-interpreting theconical singularities appearing in non-manifold-like Feynman graphs of GFTs asmatter fields [37].17.4 Connections with other approachesWe would like <strong>to</strong> recapitulate here some links <strong>to</strong> other approaches, and sketch a(rather speculative, at present) broader picture of GFTs as a generalized formalismfor <strong>Quantum</strong> <strong>Gravity</strong>, in which other discrete approaches can be subsumed.GFTs seek <strong>to</strong> realize a local simplicial third quantization of gravity, withdiscrete gravity path integrals as Feyman amplitudes and a sum over simplicialspacetimes of all <strong>to</strong>pologies realized as a Feynman expansion. What is the exactrelationship with the more traditional path integral quantizations of simplicial

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