12.07.2015 Views

Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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Three-dimensional spin foam <strong>Quantum</strong> <strong>Gravity</strong> 301where X = X i σ i . The group elements can be concretely written asg = (P 4 + ıκ P i σ i ), P4 2 + κ2 P i P i = 1, P 4 ≥ 0. (16.27)We restrict ourselves <strong>to</strong> the “northern hemisphere” of SU(2) P 4 > 0 since this isenough <strong>to</strong> label SO(3) elements, and the plane waves are simply E g (X) = e i ⃗P(g)· ⃗X .We define a non-commutative ⋆-product on R 3 which is defined on planewaves by(E g1 ⋆ E g2 )(X) ≡ E g1 g 2(X). (16.28)This ⋆-product can be more explicitly written in terms of the momenta ase ı ⃗P 1· ⃗X ⋆ e ı ⃗P 2· ⃗X = e ı( ⃗P 1 ⊕ ⃗P 2 )· ⃗X , (16.29)where⃗P 1 ⊕ ⃗P 2 =√√1 − κ 2 | ⃗P 2 | 2 P ⃗ 1 + 1 − κ 2 | ⃗P 1 | 2 P ⃗ 2 (16.30)− κ ⃗P 1 × ⃗P 2 , (16.31)and × is the 3d vec<strong>to</strong>r cross product. By linearity this star product can be extended<strong>to</strong> any function of R 3 which can be written as a linear combination of plane waves.It can also be extended <strong>to</strong> any polynomial function of X by taking derivatives ofE g with respect <strong>to</strong> P around P = 0. Using this, it can be easily shown that thisstar product describes a non-commutative spacetime with the non-commutativecoordinates satisfying[X i , X j ]=iκɛ ijk X k ,[X i , P j ]=i √ 1 − κ 2 P 2 δ ij − iκɛ ijk P k . (16.32)The non-commutativity of the space time is directly related <strong>to</strong> the fact thatmomentum space is curved. Indeed in a quantum mechanics X ∼ i∂ P the coordinateis a derivation on momentum space, and derivatives of a curved space donot commute. 3 That a non-commutative spacetime structure arises in the quantizationof 3d gravity was first proposed by ’t Hooft [19], although the details aredifferent. The existence of plane waves pairing R 3 with SO(3) allows us <strong>to</strong> developa new Fourier transform [4; 18] F : C(SO(3)) → C κ (R 3 ) mapping functions onthe group <strong>to</strong> functions on R 3 having momenta bounded by 1/κ:∫φ(X) =dg ˜φ(g)e 12κ tr(Xg) . (16.33)3 The left ⋆-multiplication by X is realized as a right invariant derivative on momentum space S 3 .

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