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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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Algebraic approach <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong> II 479λp 0 2–21A0BC–1D–2 –1 0 12λp 1Fig. 24.2. Deformed orbits under the Lorentz group in the bicrossproduct modelmomentum group. Increasing θ moves anticlockwise along an orbit in regionsA, D and clockwise in regions B, C.which deforms the Minkowski norm in momentum space. It is also invariant underinversion in the curved momentum group and hence under the antipode S. Note thatthis has nothing <strong>to</strong> do with the Poincaré algebra which we have not constructed yet;it is part of the nonlinear geometry arising from the fac<strong>to</strong>risation.Theorem 2 (i) The actions ⊲, ⊳ are defined for all θ if and only if (p 0 , p 1 ) lies inthe upper mass shell (region A).(ii) For any other (p 0 , p 1 ) there exists a finite boost θ c that sends p 0 → −∞, afterwhich ⊲ breaks down.(iii) For any θ there exists a critical curve not in region (A) such that approachingit sends θ → ±∞, after which ⊳ breaks down.For the proof we use the shorthand q ≡ e −λp0 . We analyse the situation for thetwo cases S > 0andS < 0; if S = 0 then the condition (24.23) always holds.Doing the first case, <strong>to</strong> lie in regions A, C means λp 1 + 1 − q ≥ 0. HenceC + S(λp 1 − q) = (C − S) + S(λp 1 + 1 − q) >0which also implies that the other fac<strong>to</strong>r in (24.23) is also positive, so the conditionholds. But conversely, strictly inside regions B, D mean that q − λp 1 > 1andC +S(λp 1 −q) = 0 has a solution θ c > 0 according <strong>to</strong> coth( θ c2) = q −λp 1 . We alsonote that our assumption C + Sλp 1 > 0 holds here and for all smaller θ.Asθ → θ cfrom below, the denomina<strong>to</strong>r or argument of log in the actions (24.20)–(24.21) → 0and the transformed p 0′ → −∞. IfS < 0thenλp 1 + q − 1 ≤ 0 in regions A, B

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