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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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482 S. Majid<strong>to</strong> complete the structure of U λ (poinc 1,1 ) ≡ U(so 1,1 )⊲◭C[R>⊳R] along with(24.18). Note that as λ → 0 we obtain the 2D Poincaré algebra with the usual additivecoproduct of U(poinc 1,1 ) as expected. Moreover, the deformed norm (24.24)isnecessarily a constant of motion and hence killed by the vec<strong>to</strong>r Ñ (one may checkthis easily enough). Hence it is central (a Casimir) for the deformed algebra.In the 4D case the fac<strong>to</strong>risation SO 4,1 ≈ (R 3 >⊳R).SO 3,1 leading <strong>to</strong> Poincaréquantum group U(so 3,1 )⊲◭C[R 3 >⊳R] is <strong>to</strong>o complicated <strong>to</strong> give explicitly but hassimilar global issues, likewise for SO 3,2 . It was instead constructed in [23] by identifyingthe solution of the matched pair equations at the differentiated level as aresult of finding the Hopf algebra itself (we have seen that only the differentials ofthe actions ⊲, ⊳ enter in<strong>to</strong> the Hopf algebra itself) and integrating these. The Hopfalgebra now has commuting translation genera<strong>to</strong>rs p μ , rotations M i and boosts N iwith cf. [23] but in opposite conventions for the coproduct:[p μ , p ν ]=0, [M i , M j ]=ıɛ ij k M k , [N i , N j ]=−ıɛ ij k M k[M i , N j ]=ıɛ ij k N k , [p 0 , M i ]=0, [p i , M j ]=ıɛ i jkp k , [p 0 , N i ]=−ıp i ,as usual, and the modified relations and coproduct[p i , N j ]=− ı 2 δi j(1 − e −2λp0λ+ λ ⃗p 2 )+ ıλp i p j ,N i = N i ⊗ 1 + e −λp0 ⊗ N i + λɛ ij k p j ⊗ M k ,p i = p i ⊗ 1 + e −λp0 ⊗ p iand the usual additive coproducts on p 0 , M i . The deformed Minkowski norm nowhas the same form as stated in (24.3) with the same picture as in Figure 24.2 exceptthat now the horizontal axis is any one of the p i (there is a suppressed rotationalsymmetry among them). As before, for the same fundamental reasons of nonlinearityof the matched pair equations (24.10), we have a Planckian bound |⃗p| 0 mass-shell but we also have finite boosts sending off-shellor retarded momenta off <strong>to</strong> infinitely negative ‘energy’.We have skipped over the 3D case, which is of a similar form but without asmany rotations and boosts. It was the first example in the general family <strong>to</strong> befound, by the author in [9; 12; 16; 21] as the bicrossproduct U(so 3 )◮⊳C[R 2 >⊳R](initially in a Hopf–von Neumann algebra setting), from the fac<strong>to</strong>risation SO 3,1 =(R 2 >⊳R).SO 3 . We have similarlySO m,n ≈ (R m+n−2 >⊳R).SO m,n−1

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