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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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Spacetime symmetries in his<strong>to</strong>ries canonical gravity 71which is a time-ordered sequence of properties of the physical system, each onerepresented by a single-time projection opera<strong>to</strong>r on the standard Hilbert space. Theemphasis is given on his<strong>to</strong>ries rather than states at a single time.The probabilities and the dynamics are contained in the decoherence functional,a complex-valued function on the space of his<strong>to</strong>rieswhere ρ t0 is the initial quantum state and whered H,ρ (α, β) = tr( ˜C † α ρ t 0C β ), (5.2)˜C α := U(t 0 , t 1 ) ˆα t1 U(t 1 , t 2 )...U(t n−1 , t n ) ˆα tn U(t n , t 0 ) (5.3)is the class opera<strong>to</strong>r that represents the his<strong>to</strong>ry α.When a set of his<strong>to</strong>ries satisfies a decoherence condition, d H,ρ (α , β) = 0thenα,βare in the consistent set, which means that we have zero interference betweendifferent his<strong>to</strong>ries, and then it is possible <strong>to</strong> consistently assign probabilities <strong>to</strong> eachhis<strong>to</strong>ry in that set; it is called a consistent set.Then we can assign probabilities <strong>to</strong> each his<strong>to</strong>ry in the consistent setd H,ρ (α , α) = Prob(α; ρ t0 ) = tr( ˜C † α ρ t 0C α ). (5.4)One of the aims of the his<strong>to</strong>ries formalism is <strong>to</strong> provide a generalised quantummechanics definition, so that, one may deal with systems possessing a non-trivialcausal structure, including perhaps <strong>Quantum</strong> <strong>Gravity</strong>. In particular, Hartle has providedexamples of how this procedure would work, based mainly on a path integralexpression of the decoherence functional [10].5.2.2 HPO formalism – basicsIn the His<strong>to</strong>ry Projection Opera<strong>to</strong>r (HPO) approach <strong>to</strong> consistent his<strong>to</strong>ries theorythe emphasis is given on the temporal quantum logic. Thus it offers the possibilityof handling the ideas of space and time in a significantly new way within thequantum theory.A his<strong>to</strong>ry is represented by a tensor product of projection opera<strong>to</strong>rsˆα := ˆα t1 ⊗ˆα t2 ⊗ ... ⊗ˆα tn , (5.5)each opera<strong>to</strong>r ˆα ti being defined on a copy of the single-time Hilbert space H ti at thattime t i and corresponding <strong>to</strong> some property of the system at the same time indicatedby the t-label. Therefore – in contrast <strong>to</strong> the sum over his<strong>to</strong>ries formalism – ahis<strong>to</strong>ry is itself a genuine projection opera<strong>to</strong>r defined on the his<strong>to</strong>ry Hilbert spaceV n , which is a tensor product of the single-time Hilbert spacesV n := H t1 ⊗ H t2 ⊗ ... ⊗ H tn . (5.6)

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