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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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112 R. PercacciIn section 8.2 I introduce the general idea of asymp<strong>to</strong>tic safety; the reader isreferred <strong>to</strong> [46] for a more detailed discussion. In section 8.3 I describe some peculiaritiesof the gravitational RG, which derive from the dual character of the metricas a dynamical field and as definition of lengths. Recent evidence for a FP, comingmainly from the ERGE, is reviewed in section 8.4. Some relations <strong>to</strong> otherapproaches <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong> are briefly mentioned in section 8.5.8.2 The general notion of asymp<strong>to</strong>tic safetyThe techniques of effective QFT have been recognized as being of great generalityand are now quite pervasive in particle physics. An effective field theory isdescribed by an effective action Ɣ k which can be thought of as the result of havingintegrated out all fluctuations of the fields with momenta larger than k. Weneed not specify here the physical meaning of k: for each application of the theoryone will have <strong>to</strong> identify the physically relevant variable acting as k (in particlephysics it is usually some external momentum). One convenient definition of Ɣ kthat we shall use here is as follows. We start from a (“bare”) action S[φ A ] formultiplets of quantum fields φ A , describing physics at an energy scale k 0 .Weadd<strong>to</strong> it a term S k [φ A ], quadratic in the φ A , which in Fourier space has the form:S k [φ] = ∫ d d qφ A RkAB (q 2 )φ B .ThekernelRkAB (q 2 ), henceforth called the cu<strong>to</strong>fffunction, is chosen in such a way that the propagation of field modes φ A (q) withmomenta q < k is suppressed, while field modes with momenta k < q < k 0 areunaffected. We formally define a k-dependent generating functional of connectedGreen functions∫ (∫ )W k [J A ]=−log (dφ A ) exp −S[φ A ]−S k [φ A ]− J A φ A (8.1)and a modified k-dependent Legendre transform∫Ɣ k [φ A ]=W k [J A ]− J A φ A − S k [φ A ] , (8.2)where S k has been subtracted. The “classical fields” δW kare denoted again φδ J AAfor notational simplicity. This functional interpolates continuously between S, fork = k 0 , and the usual effective action Ɣ[φ A ], the generating functional of oneparticleirreducible Green functions, for k = 0. It is similar in spirit, but distinctfrom, the Wilsonian effective action. In the following we will always use thisdefinition of Ɣ k , but much of what will be said should be true also with otherdefinitions.In the case of gauge theories there are complications due <strong>to</strong> the fact that the cu<strong>to</strong>ffinterferes with gauge invariance. One can use a background gauge condition, whichcircumvents these problems by defining a functional of two fields, the background

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