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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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Loop quantum gravity 249a definite, universal value. This is possible because in LQG geometrical opera<strong>to</strong>rssuch as volumes, areas and lengths of regions, surfaces (such as the horizon) andcurves have discrete spectrum [43; 44; 45; 46] with a gap away from zero (otherwisethe entropy would be infinite). 13 One may speculate whether the discretenessof the spectra hints at a combina<strong>to</strong>rical, distributional Planck scale structure ofspacetime with no meaning <strong>to</strong> notions like smoothness or metrics which shouldemerge only on large scales.Finally, certain minisuperspace approximations <strong>to</strong> LQG have been developed inorder <strong>to</strong> perform approximate quantum cosmology [48]. The results obtained aresubject <strong>to</strong> the usual restriction that a truncated model might not display the truebehaviour of the full theory due <strong>to</strong> artificial suppression of degrees of freedomwhich might have large fluctuations in the full theory. See e.g. [49; 50] where it isshown that (big bang) singularity avoidance of the models is due <strong>to</strong> a mechanismwhich is only available in those models. On the other hand, as shown, in the fulltheory singularity avoidance could possibly be obtained by a more subtle featureof LQG. In any case, the models indicate that LQG indeed might be able <strong>to</strong> resolvethe singularities of full GR.To summarise: LQG is a mathematically rigorous approach <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong>which is conceptually clear and simple. It only uses the principles of General Relativityand <strong>Quantum</strong> Mechanics and no experimentally unverified assumptions. Itis fully background independent as every <strong>Quantum</strong> <strong>Gravity</strong> theory must be. Now<strong>to</strong>ols have have been developed that enable one <strong>to</strong> make contact with experimentand thus <strong>to</strong> falsify the theory.References[1] C. Rovelli, <strong>Quantum</strong> <strong>Gravity</strong> (Cambridge, Cambridge University Press, 2004).[2] T. Thiemann, Modern Canonical <strong>Quantum</strong> General Relativity (Cambridge,Cambridge University Press, 2007),[3] A. Ashtekar, J. Lewandowski, “Background independent quantum gravity: a statusreport”, Class. Quant. Grav. 21 (2004) R53, [gr-qc/0404018].[4] L. Smolin, “<strong>Quantum</strong> gravity with a positive cosmological constant”,hep-th/0209079[5] C. Rovelli, “Loop quantum gravity”, Living Rev. Rel. 1 (1998) 1, gr-qc/9710008[6] T. Thiemann,“Lectures on loop quantum gravity”, Lecture Notes in Physics, 631(2003) 41–135, gr-qc/0210094[7] R. Haag, Local <strong>Quantum</strong> Physics, 2nd edn (Berlin, Springer Verlag, 1996).13 Actually, there are two unequivalent Volume Opera<strong>to</strong>rs, one due <strong>to</strong> Rovelli and Smolin (RS) and the other onedue <strong>to</strong> Ashtekar and Lewandowski (AL) [43; 44; 45; 46] which are both derived using background independenttechniques from the fundamental flux opera<strong>to</strong>r. In a recent non-trivial consistency check [47] theRSandALvolume opera<strong>to</strong>rs have been shown <strong>to</strong> be inconsistent and consistent respectively with the flux opera<strong>to</strong>r. Thisis a first example for an analysis which uses internal mathematical consistency in order <strong>to</strong> improve the degreeof uniqueness of LQG.

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