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Approaches to Quantum Gravity

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<strong>Quantum</strong> Regge calculus 373<br />

where ξ is the correlation length, was approximately 1/3. When scalar matter was<br />

included in the simulations, the effect on the critical exponents was small, but the<br />

results suggested that gravitational interactions could increase with distance [31].<br />

In an investigation of the New<strong>to</strong>nian potential in quantum Regge gravity, Hamber<br />

and Williams [32] computed correlations on the lattice between Wilson lines associated<br />

with two massive particles. In the smooth anti-de Sitter-like phase, the only<br />

region where a sensible lattice continuum limit could be constructed in the model,<br />

the shape and mass dependence of the attractive potential were studied close <strong>to</strong> the<br />

critical point in G. It was found that non-linear gravitational interactions gave rise<br />

<strong>to</strong> a Yukawa-like potential, with mass parameter decreasing <strong>to</strong>wards the critical<br />

point where the average curvature vanished.<br />

The other pioneer of these methods, Berg, did early simulations keeping the<br />

<strong>to</strong>tal volume constant [8]. His results indicated that an exponentially decreasing<br />

entropy fac<strong>to</strong>r in the measure might cure the problem of the unboundedness of the<br />

gravitaional action [9].<br />

The group in Vienna has, over the years, explored many aspects of Regge lattice<br />

gravity. Recently, a Z 2 model, in which edge lengths could take just two discrete<br />

values, was compared with the standard Regge model with a continuous range of<br />

values for the edge lengths [11]. The results of the two models were similar. An<br />

extension of this [62] also included the model of Caselle et al. [13], where gravity<br />

is treated as a gauge theory, and the action involves the sine of the deficit angle.<br />

Evidence was found in all models of a continuous phase transition, and the results<br />

were compatible with the existence of massless spin-2 excitations. These types<br />

of comparison should be pursued as a means of investigating the very important<br />

question of the relationship between the universality classes of Regge calculus and<br />

dynamical triangulations.<br />

More details and discussion of numerical work on quantum Regge calculus are<br />

given in the review by Loll [53].<br />

19.7 Canonical quantum Regge calculus<br />

By way of contrast, we mention finally some approaches <strong>to</strong> canonical <strong>Quantum</strong><br />

<strong>Gravity</strong> using Regge calculus.<br />

Immirzi set out <strong>to</strong> relate the canonical approach of loop quantum gravity<br />

<strong>to</strong> Regge calculus. He defined the Ashtekar variables for a Regge lattice, and<br />

introduced the Liouville form and Poisson brackets [44]. He found that it was<br />

impossible <strong>to</strong> quantise the model directly using complex variables, and leave the<br />

second class constraints <strong>to</strong> fix the metric of the quantum Hilbert space, because one<br />

cannot find a metric which makes the area variables hermitian [45].<br />

In a long series of papers, Khatsymovsky has confronted many of the problems<br />

arising in setting up a canonical quantisation of Regge calculus [48]. Topics he has

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