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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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17The group field theory approach <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong>D. ORITI17.1 Introduction and motivationGroup field theories (GFTs) [1; 2] were developed at first as a generalization ofmatrix models for 2d <strong>Quantum</strong> <strong>Gravity</strong> <strong>to</strong> 3 and 4 spacetime dimensions <strong>to</strong> producea lattice formulation of <strong>to</strong>pological theories. More recently, they have been developedfurther in the context of spin foam models for <strong>Quantum</strong> <strong>Gravity</strong>, as a <strong>to</strong>ol<strong>to</strong> overcome the limitations of working with a fixed lattice in the non-<strong>to</strong>pologicalcase. In our opinion, however, GFTs should be seen as a fundamental formulationof <strong>Quantum</strong> <strong>Gravity</strong> and not just as an auxiliary <strong>to</strong>ol. The bot<strong>to</strong>m line of thisperspective, here only tentatively outlined and still <strong>to</strong> be fully realized, hopefully,after much more work, can be summarized as follows: GFTs are quantum fieldtheories of spacetime (as opposed <strong>to</strong> QFTs on spacetime), that describe the dynamicsof both its <strong>to</strong>pology and geometry in local, simplicial, covariant, algebraicterms, and that encompass ideas and insights from most of the other approaches<strong>to</strong> non-perturbative <strong>Quantum</strong> <strong>Gravity</strong>. We have just began <strong>to</strong> explore the structureof these models, but there is already some evidence, in our opinion, that in the GFTframework lies the potential for important developments.The idea of defining a quantum field theory of geometry, i.e. a QFT on superspace(the space of 3-geometries) for given spatial <strong>to</strong>pology, say S 3 , was alreadyexplored in the past [3; 4; 5]. The context was then a global or “quantum cosmology”one. Such a theory would produce, in its perturbative expansion, a sumover different <strong>to</strong>pologies each corresponding <strong>to</strong> a possible Feynman graph, i.e. <strong>to</strong>a possible interaction process for “universes” represented by the basic 3-sphere.The spatial <strong>to</strong>pology change would be limited therefore <strong>to</strong> a changing numberof disjoint copies of S 3 . The field would represent a second quantization of thecanonical wave function on superspace, here describing the “one-particle sec<strong>to</strong>r”of the theory. 1 The quantum amplitude for each Feynman graph, corresponding <strong>to</strong>1 The 3-metric being itself a field, this second quantization of what is already a field theory was dubbed “thirdquantization”.<strong>Approaches</strong> <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong>: Toward a New Understanding of Space, Time and Matter, ed. Daniele Oriti.Published by Cambridge University Press. c○ Cambridge University Press 2009.

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