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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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530 J. Collins, A. Perez and D. Sudarskypropose that it is the measurement process that picks out the modified 4-momentumopera<strong>to</strong>rs as the measurable quantities.We will also <strong>to</strong>uch on an aspect with important connections <strong>to</strong> the general fieldof QG: the problem of a physical regularization and construction of <strong>Quantum</strong> FieldTheories (QFT).27.2 Phenomenological modelsMethodical phenomenological explorations can best be quantified relative <strong>to</strong> adefinite theoretical context. In our case, of Lorentz invariance violation (LIV) ataccessible energies, the context should minimally incorporate known microscopicphysics, including <strong>Quantum</strong> Mechanics and Special Relativity (in order <strong>to</strong> considersmall deviations therefrom). This leads <strong>to</strong> the use of a conventional interacting<strong>Quantum</strong> Field Theory but with the inclusion of Lorentz violating terms in theLagrangian.One proposal is the Standard Model Extension (SME) of Colladay & Kostelecký[20] and Coleman & Glashow [19]. This incorporates within the Standard Modelof particle physics all the possible renormalizable Lorentz violating terms, whilepreserving SU(3) × SU(2) × U(1) gauge symmetry and the standard field content.For example, the terms in the free part of the Lagrangian density for a free fermionfield ψ are:L free = i ¯ψ(γ μ + c μν γ ν + d μν γ 5 γ ν + e μ + if μ γ 5 + 1 2 g μνρσ νρ )∂ μ ψ− ¯ψ(m + a ν γ ν + b ν γ 5 γ ν + 1 2 H νρσ νρ )ψ. (27.3)Here the quantities a μ , b μ , c μν , d μν , e μ , f μ , g μνρ and H μν are numerical quantitiescovariantly characterizing LIV, and can be thought of as arising from the VEV ofotherwise dynamical gravitational fields. The interacting theory is then obtainedin the same way as usual, with SU(3) × SU(2) × U(1) gauge fields and a Higgsfield. The expected renormalizability was shown by Kostelecký and Mewes [46]and Kostelecký et al. [47].A second approach, as used by Myers and Pospelov [54] is <strong>to</strong> take the LIV termsas higher dimension non-renormalizable opera<strong>to</strong>rs. This is a natural proposal if onesupposes that LIV is produced at the Planck scale with power suppressed effectsat low energy; it gives modified dispersion relations at tree approximation. Forexample, there are dimension-5 terms with 1/M Pl suppression in the free part ofthe Lagrangian, such as1M PlW μ W ν W ρ ¯ψ(ξ f + ξ 5 f γ 5 )γ μ ∂ ν ∂ ρ ψ, (27.4)

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