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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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130 F. Markopoulouhas been claimed <strong>to</strong> be the case, in different systems, by Dreyer ([8] and this volume),Lloyd [19], Kribs and Markopoulou [16], and Konopka, Markopoulou andSmolin [14].As can be seen from the above, this new direction is in fact orthogonal <strong>to</strong> all previousapproaches and so it comes with its own set of promises and challenges. Weshall discuss these but we also wish <strong>to</strong> outline the choices involved in the answers <strong>to</strong>our two questions above. It is normally difficult <strong>to</strong> have an overview of the choicesinvolved in picking different directions in <strong>Quantum</strong> <strong>Gravity</strong> because the mathematicalrealizations are intricate and all different. Luckily, for the present purposes,we find that we can base the discussion on the formalism of <strong>Quantum</strong> CausalHis<strong>to</strong>ries (QCH), a locally finite directed graph of finite-dimensional quantumsystems. 1A QCH, depending on the physical interpretation of its constituents, can modela discrete analog of <strong>Quantum</strong> Field Theory, a traditional, quantum geometry basedbackground independent system, or the new, pre-geometric background independenttheories. This will allow us <strong>to</strong> keep an overview of the forks on the road<strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong>. It will also be ideal for analyzing the newest kind of backgroundindependent systems and obtaining some first results on their effectiveproperties. In particular, we shall see how one can extract conserved quantities inpre-geometric systems using a straightforward map between a QCH and a quantuminformation processing system.The outline of this chapter is as follows. In section 9.2 we give the definitionof a <strong>Quantum</strong> Causal His<strong>to</strong>ry, <strong>to</strong>gether with a simple example, locallyevolving networks in subsection 9.2.1. At this point we have not restricted ourselves<strong>to</strong> any particular physical interpretation of the QCH and the options arelisted in 9.2.2. In section 9.3 we give the necessary definitions of BackgroundIndependence. The following three sections contain three distinct physical interpretationsof a QCH: as a discrete analog of <strong>Quantum</strong> Field Theory (a backgrounddependent theory) in section 9.4, a quantum geometry theory in section 9.5 witha discussion of advantages and challenges (9.5.1) and finally the new type ofbackground independent systems in section 9.6. Their advantages and challengesare discussed in 9.6.2. In section 9.6.3, we map a QCH <strong>to</strong> a quantum informationprocessing system and use this <strong>to</strong> derive conserved quantities with noreference <strong>to</strong> a background spacetime, complete with a simple example of such conservedquantities. We conclude with a brief discussion of these new directions insection 9.7.1 The finiteness is a simple implementation of the expectation that there really are only a finite number of degreesof freedom in a finite volume, arguments for which are well-known and we have reviewed them elsewhere [25].

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