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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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The group field theory approach <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong> 325gravity: quantum Regge calculus (see chapter 19 by Williams) and dynamical triangulations(see chapter 18 by Ambjørn et al.)? The first of the above uses a fixedtriangulation of spacetime, and thus should be reproduced at the level of the GFTFeynman amplitudes for a given Feynman diagram. Given the geometric interpretationof the GFT variables [28; 9; 10], each amplitude should correspond <strong>to</strong> a firs<strong>to</strong>rder path integral quantization of discrete gravity, i.e. treating on equal footing(D − 2)-volumes and dihedral angles (equivalently, appropriate parallel transportsof a Lorentz connection) as fundamental variables, as opposed <strong>to</strong> the second orderformulation of traditional Regge calculus in terms of edge lengths. This, however,may be consider a somewhat minor difference. The main issue <strong>to</strong> be clarified inorder <strong>to</strong> establish a clear link with the quantum Regge calculus approach has <strong>to</strong> dowith the fact that the quantum amplitudes of the latter approach are given by theexponential of the Regge action for discrete gravity, while in the most studied spinfoam models the connection between the quantum amplitudes and the Regge actionis clear only in a particular regime and rather involved. However, it seems plausiblethat the new generalized models of [24], or a suitably modification of the same, canindeed give amplitudes with the same structure as in quantum Regge calculus, witha measure being uniquely determined by the choice of GFT action, thus clarifyingthe connection with discrete gravity and at the same time subsuming the quantumRegge calculus approach within the GFT formalism. The same type of amplitudesis needed also <strong>to</strong> establish a solid link with the dynamical triangulations approach,where the Regge action weights this time the combina<strong>to</strong>rial structure of the triangulationitself, which is treated as the only true dynamical variable within a sumover all possible triangulations of a given <strong>to</strong>pology. The dynamical triangulationsapproach would then once more arise as a subsec<strong>to</strong>r of the GFT formalism, if onecould find the right way of trivializing the extra structure associated <strong>to</strong> each triangulation(thus dropping the sum over geometric data). Of course, more work wouldbe needed then <strong>to</strong> impose the extra conditions (fixed slicing structure, absence ofbaby universe nucleation, etc) that seem <strong>to</strong> be needed in the modern version of theapproach (see chapter 18 by Ambjørn et al.) <strong>to</strong> have a good continuum limit. Workon this is in progress [30].It is well known that a covariant path integral quantization is more general thanthe corresponding canonical/Hamil<strong>to</strong>nian one, and that this is even more true ina third quantization formalism with its sum over <strong>to</strong>pologies. One expects <strong>to</strong> beable <strong>to</strong> reproduce from a GFT the results of a canonical <strong>Quantum</strong> <strong>Gravity</strong> withgroup elements and group representations as basic variables, and spin networks asquantum states, i.e. loop quantum gravity. We have discussed above how this canindeed be realized [2]. The main differences between the particular version of theLQG formalism that the GFT approach reproduces, and the traditional one (see thechapter by Thiemann), are: (1) the spin networks appearing as boundary states or

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