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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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70 N. Savvidouof time. The development of the His<strong>to</strong>ries Projection Opera<strong>to</strong>r (HPO) approach inparticular, showed that it is characterised by two distinctive features. First, a his<strong>to</strong>ryis a temporally extended object that it is represented quantum mechanically by asingle projection opera<strong>to</strong>r, on a suitably constructed Hilbert space [12]. Second,the theory possesses a novel temporal structure [21], since time is implemented bytwo distinct parameters, one of which refers <strong>to</strong> the kinematics of the theory, whilethe other refers <strong>to</strong> its dynamical behavior. At the classical level the two parameterscoincide for all his<strong>to</strong>ries that correspond <strong>to</strong> the solutions of the equations of motion.Hence, the HPO theory is endowed with a rich kinematical structure. In the caseof General Relativity this results in the fact that different ‘canonical’ descriptionsof the theory, corresponding <strong>to</strong> different choices of spacelike foliation, coexist inthe space of his<strong>to</strong>ries and may be related by a properly defined transformation.This allows the preservation of the spacetime description of the theory, even if onechooses <strong>to</strong> work with canonical variables.The General Relativity his<strong>to</strong>ries theory suggests a quantum mechanical treatmen<strong>to</strong>f the full Lorentzian metric. Other programmes also put emphasis on thespacetime description, namely the causal set approach [6], and the Lorentziandynamical triangulations [1]. The twis<strong>to</strong>r programme has the same avowed aims.The HPO formalism, however, allows the incorporation of other theories, enrichingthem with a spacetime kinematical description, while preserving the main featuresof their dynamical behavior.A his<strong>to</strong>ries-based quantisation of General Relativity, like the canonical theory,has <strong>to</strong> address the issue of defining an appropriate Hamil<strong>to</strong>nian constraint opera<strong>to</strong>r.Loop quantum gravity has made the greatest progress so far in the construction ofsuch an opera<strong>to</strong>r, therefore it would be very interesting <strong>to</strong> exploit a his<strong>to</strong>ries versionof this theory.5.2 His<strong>to</strong>ry Projection Opera<strong>to</strong>r theory5.2.1 Consistent his<strong>to</strong>ries theoryThe consistent his<strong>to</strong>ries formalism was originally developed by Griffiths [9] andOmnés [17; 18], as an interpretation of quantum theory for closed systems.Gell-Mann and Hartle [8] elaborated this scheme in the case of quantum cosmology– the Universe being regarded as a closed system. They emphasised inparticular that a theory of <strong>Quantum</strong> <strong>Gravity</strong> that is expected <strong>to</strong> preserve the spacetimecharacter of General Relativity would need a quantum formalism in which theirreducible elements are temporally extended objects, namely his<strong>to</strong>ries.The basic object in the consistent his<strong>to</strong>ries approach is a his<strong>to</strong>ryα := ( ˆα t1 , ˆα t2 , ..., ˆα tn ), (5.1)

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