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arXiv:hep-th/9304011 v1 Apr 5 1993

arXiv:hep-th/9304011 v1 Apr 5 1993

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vertices and is counted <strong>th</strong>ree times.) The discrete counterpart to <strong>th</strong>e Ricci scalar R at<br />

vertex i is R i = 2π(6 − N i )/N i , so <strong>th</strong>at<br />

∫ √g R →<br />

∑<br />

i<br />

4π(1 − N i /6) = 4π(V − 1 F ) = 4π(V − E + F ) = 4πχ .<br />

2<br />

Here we have used <strong>th</strong>e simplicial definition which gives <strong>th</strong>e Euler character χ in terms of<br />

<strong>th</strong>e total number of vertices, edges, and faces V , E, and F of <strong>th</strong>e triangulation (and we<br />

have used <strong>th</strong>e relation 3F = 2E obeyed by triangulations of surfaces, since each face has<br />

<strong>th</strong>ree edges each of which is shared by two faces).<br />

In <strong>th</strong>e above, triangles do not play an essential role and may be replaced by any set<br />

of polygons. General random polygonulations of surfaces wi<strong>th</strong> appropriate fine tuning of<br />

couplings may, as we shall see, have more general critical behavior, but can in particular<br />

always reproduce <strong>th</strong>e pure gravity behavior of triangulations in <strong>th</strong>e continuum limit.<br />

6.2. Matrix models<br />

We now demonstrate how <strong>th</strong>e integral over geometry in (6.1) may be performed in<br />

its discretized form as a sum over random triangulations. The trick is to use a certain<br />

matrix integral as a generating functional for random triangulations. The essential idea<br />

goes back to work [81] on <strong>th</strong>e large N limit of QCD, followed by work on <strong>th</strong>e saddle point<br />

approximation [82].<br />

We first recall <strong>th</strong>e (Feynman) diagrammatic expansion of <strong>th</strong>e (0-dimensional) field<br />

<strong>th</strong>eory integral.<br />

∫ ∞<br />

−∞<br />

dϕ<br />

√<br />

2π<br />

e −ϕ2 /2 + λϕ 4 /4! , (6.3)<br />

where ϕ is an ordinary real number. 25 In a formal perturbation series in λ, we would need<br />

to evaluate integrals such as<br />

λ n<br />

n!<br />

Up to overall normalization we can write<br />

∫<br />

ϕ<br />

e −ϕ2 /2 ϕ 2k =<br />

∂2k<br />

∫<br />

∂J 2k ∫ϕ<br />

ϕ<br />

e −ϕ2 /2 ( ϕ 4 ) n<br />

. (6.4)<br />

4!<br />

e −ϕ2 /2 + Jϕ ∣ ∣ ∣∣<br />

J=0<br />

= ∂2k<br />

∂J 2k eJ 2 /2 ∣ ∣<br />

∣∣J=0 . (6.5)<br />

25 The integral is understood to be defined by analytic continuation to negative λ.<br />

77

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