12.07.2015 Views

Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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New directions in background independent <strong>Quantum</strong> <strong>Gravity</strong> 135A 1=A 2=(9.7)A 3=Fig. 9.1. The three genera<strong>to</strong>rs of evolution on the network space H. Theyarecalled expansion, contraction and exchange moves.where the sum is over all <strong>to</strong>pologically distinct embeddings of all such networks in with the natural inner product 〈S i |S i ′〉=δ Si S i ′ .Local dynamics on H can be defined by excising pieces of S and replacing themwith new ones with the same boundary [21; 26]. The genera<strong>to</strong>rs of such dynamicsare given graphically in Fig. 9.1. Given a network S, application of A i results in i |S〉 = ∑ α|S αi ′ 〉, (9.8)where S ′ αiare all the networks obtained from S by an application of one move oftype i (i = 1, 2, 3). Together with the identity 1, these moves generate the evolutionalgebraA evol = {1, A i } , i = 1, 2, 3 (9.9)on H.Finally, changing the network S by the above local moves produces a directedgraph Ɣ. The vertices of S are also the vertices of Ɣ. The genera<strong>to</strong>r moves correspond<strong>to</strong> complete pairs and hence unitary opera<strong>to</strong>rs, however, the opera<strong>to</strong>rsbetween individual vertices are CP and the resulting system of locally evolvingnetworks is a <strong>Quantum</strong> Causal His<strong>to</strong>ry. For example, in this change of S <strong>to</strong> S ′we have operated with A 3 between complete pair sets ξ and ζ and with A 1 betweencomplete pairs η and ɛ.Themapfromx <strong>to</strong> y is a CP map.

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