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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 81The first step in the application of the his<strong>to</strong>ries formalism <strong>to</strong> loop quantum gravityis <strong>to</strong> develop the his<strong>to</strong>ries analogue of the connection formalism of GeneralRelativity. The original formulation of the programme involved the considerationof self-dual SL(2, C) connections on spacetime, <strong>to</strong>gether with a field of tetradsfor a Lorentzian metric [26; 4]. However, the mainline approach in loop quantumgravity finds it more convenient <strong>to</strong> employ in quantisation a real SU(2) connection,proposed by Barbero [5]. The Barbero connection may be obtained as a variable ina state space, extending that of canonical General Relativity; or it may be obtainedfrom a Lagrangian action (the Holst Lagrangian by [11]). However, the latter procedureinvolves gauge fixing, and it is not clear whether the connection may bedefined in its absence – see [19; 20] for related discussions.The his<strong>to</strong>ries description for classical gravity in term of the Holst Lagrangian hasbeen developed in [25]. The basic variables at the covariant level is an SL(2, C)connection and a field of tetrads on spacetime M, <strong>to</strong>gether with their conjugatevariables. The corresponding his<strong>to</strong>ry space carries a symplectic action of the groupDi f f (M) of spacetime diffeomorphisms. The introduction of an equivariant foliationfunctional allows the translation of the spacetime description in<strong>to</strong> that ofan one-parameter family of canonical structures. The results of the metric-basedtheory can be fully reproduced in this construction: the set of constraints corresponding<strong>to</strong> the Holst Lagrangian is invariant under the action of the spacetimeDi f f (M) group. Hence the genera<strong>to</strong>rs of the spacetime diffeomorphisms groupcan also be projected on<strong>to</strong> the reduced state space.The next step would involve choosing the basic variables for quantisation. Followingthe spirit of loop quantum gravity, we may try <strong>to</strong> identify a loop algebra,and then construct a his<strong>to</strong>ries Hilbert space by studying its representation theory.The obvious place <strong>to</strong> start would be the loop algebra corresponding <strong>to</strong> thespacetime SL(2, C) connection of the covariant description. This, however, wouldinvolve a representation theory for loop variables with a non-compact gauge group,which <strong>to</strong> the best of our knowledge has not yet been fully developed. Moreover,we would have <strong>to</strong> identify a new role for the tetrad fields, because at this level theycommute with the connection variables.It may be more profitable <strong>to</strong> work with ‘internal’ fields, namely the ones thatcorrespond <strong>to</strong> one-parameter families of the standard canonical variables. Thiswould allow the consideration of connections with compact gauge group. However,a complication arises, because of the gauge-dependence of the definition ofthe Barbero connection. A gauge-fixing condition, at this level, breaks the backgroundindependence of the theory. In [25] we show that a connection sharing allproperties of the Barbero connection can be defined in a gauge invariant way, albeitin a larger space than the one usually employed.A his<strong>to</strong>ry quantisation may be therefore envisioned that will employ variablesdefined with support on a two-dimensional cylinder – giving a his<strong>to</strong>ry analogue of

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