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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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From quantum reference frames <strong>to</strong> deformed special relativity 521the physical coordinates. In fact by adding two extra dimensions <strong>to</strong> phase space,we can do more, that is, see all the different deformations as different gaugefixingsor different choices of non-equivalent observers.Since we have an extra fundamental mass parameter M P inthegamewecanrewrite the MDR (26.5) asE 2 − p 2 − M(p) 2 =−M P 2 , with M(p) 2 = m 2 + F(p,μ,M P ) − M P 2 ,such that it looks like a five dimensional mass shell conditionP μ P μ − P 2 4 =−M P 2 . (26.7)), we do the scale transformationL P → L P χ = L C that can be chosen <strong>to</strong> keep the speed of light c fixed as well as. G becomes however, variable G → χ 2 G: in the particle units we have a fixedmass but a variable G. Since the mass becomes a variable (in Planck units) encodingthe QG fluctuations, it is natural <strong>to</strong> extend the configuration space <strong>to</strong> include itas a true variable. This goes naturally as encoding G as a new universal constant[33], since it allows us <strong>to</strong> transform a mass in<strong>to</strong> a length. We consider now ourextended phase space as given by a configuration space (y A = y μ , y 4 = G xc 2 4 ),where x 4 has mass dimension, and the momentum space given by P A .A DSR particle will be described by the actionP4 2 = M(p)2 can be interpreted as having a variable mass. This is something naturalfrom the GR point of view. For example an extended object has a varying massin a curved spacetime [28]. Since a quantum particle cannot be localized, curvaturemight introduce some slight variations <strong>to</strong> its mass. Note that now, momentumspace is identified with the de Sitter space, so that we are out of the usual geometricalscheme, the cotangent bundle is not a vec<strong>to</strong>r fiber bundle anymore. This willhave direct consequences on the addition of momenta as we shall see in the nextsection.From the QG point of view, one can expects the New<strong>to</strong>n constant G <strong>to</strong> berenormalized <strong>to</strong> encompass quantum corrections [31]. Instead of considering fluctuationsin G and a fixed mass, we can describe the theory in an effective wayas a fixed G, with a fluctuating mass: G(x) m → Gm(x). In fact all this isrelated <strong>to</strong> the choice of units. The notion of a variable mass in terms of unitshas already been studied in detail by Bekenstein [32]. The Planck units system(M P , L P , T P ), is independent of any particle data. All the different fundamentalconstants can be expressed in terms of these quantities, and in these units arefixed. Now consider a particle with a variable mass, that is expressed in the Planckunits we have m = χ M P . If one moves <strong>to</strong> the particle unit, for example the Comp<strong>to</strong>nunit (M C = m, L C = mc , T C = cL −1C∫S 5d = dy A P A − λ 1 (P A P A + M 2 P ) − λ 2 (P 4 − M),

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