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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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416 Questions and answersthat the lattice spacing times the correlation length measured in lattice unitsis constant (equal <strong>to</strong> the inverse physical mass). This is the way <strong>to</strong> recover thecontinuum limit of the lattice theory.However, suppose we are already at the critical surface. As an explicitexample consider a free massless scalar particle (in Euclidean spacetime).Put it on the lattice in the simplest possible way. The propaga<strong>to</strong>r is nowG(p) =1sin 2 (pa/2) → 1a 2 p 2 for a → 0.Except for a prefac<strong>to</strong>r, we have directly the continuum propaga<strong>to</strong>r when thelattice spacing a → 0. No fine-tuning is needed. In other theories where masslessparticles can be put on the lattice in a natural way which does not generatea mass term, neither perturbatively nor non-perturbatively, we have the samesituation. An example is four-dimensional lattice U(1) theory. For the (lattice)coupling constant above the critical value, one has a confining lattice theorywithout a continuum limit, but for the coupling constant below the criticalvalue one is au<strong>to</strong>matically in the Coulomb phase where a trivial rescaling ofthe lattice spacing and fields leads <strong>to</strong> the continuum free field theory of thepho<strong>to</strong>n.In CDT we seem <strong>to</strong> have the same situation: for some range of the baregravitational coupling constant we obtain a lattice theory with no continuumlimit. For another range of the gravitational coupling constant we obtain acontinuum limit (<strong>to</strong> the extent one can trust the computer simulations) just bytaking the lattice spacing <strong>to</strong> zero. If one wants <strong>to</strong> use the analogy with theU(1) theory mentioned above, the interpretation would be that the gravi<strong>to</strong>nhas been incorporated in a natural way which does not lead <strong>to</strong> a mass, soone is staying on the critical surface for a range of coupling constants. It isprobably a good thing.In the “old” Euclidean DT the situation was the following: for almostall values of the gravitational couplings constant the computer simulationsshowed just a lattice theory without any obvious continuum limit. Only nearthe phase transition between a pathologically crumpled phase and an equallypathologically “stretched” phase (where the geometry degenerated <strong>to</strong> socalledbranched polymers) was there a chance <strong>to</strong> obtain something whichwas not a lattice artifact. Unfortunately the phase transition turned out <strong>to</strong> bea (weak) first order transition and the separation between the two phaseswould be sharp with increasing spacetime volume. Had it been a secondorder transition one could have hoped it would have been possible <strong>to</strong> definea continuum limit, in particular that there was a divergent correlation length

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