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Feynman Path Integral Formulation

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226 7 Analytical Lattice Expansion Methods<br />

I R ∝<br />

∑ δ(l) A(l) , (7.1)<br />

hinges<br />

to quadratic order in the lattice weak fields one needs first and second variations<br />

with respect to the edge lengths. In four dimensions the first variation of the lattice<br />

Regge action is given by<br />

δI R ∝<br />

( )<br />

∂A<br />

∑ δ · ∑<br />

hinges edges<br />

∂l δl<br />

, (7.2)<br />

since Regge has shown that the term involving the variation of the deficit angle<br />

δ vanishes (here the variation symbol should obviously not be confused with the<br />

deficit angle). Furthermore in flat space all the deficit angles vanish, so that the<br />

second variation is given simply by<br />

δ 2 I R ∝<br />

∑<br />

hinges<br />

(<br />

∑<br />

edges<br />

) ( )<br />

∂δ<br />

∂l δl ∂A<br />

· ∑<br />

edges<br />

∂l δl<br />

. (7.3)<br />

Next a specific lattice structure needs to be chosen as a background geometry. A<br />

natural choice is to use a flat hypercubic lattice, made rigid by introducing face<br />

diagonals, body diagonals and hyperbody diagonals, which results into a subdivision<br />

of each hypercube into d! (here 4!=24) simplices. This subdivision is shown in<br />

Fig. 7.1.<br />

Fig. 7.1 A four-dimensional<br />

hypercube divided up into<br />

four-simplices.<br />

By a simple translation, the whole lattice can then be constructed from this one<br />

elemental hypercube. Consequently there will be 2 d −1 = 15 lattice fields per point,<br />

corresponding to all the edge lengths emanating in the positive lattice directions<br />

from any one vertex. Note that the number of degrees per lattice point is slightly<br />

larger than what one would have in the continuum, where the metric g μν (x) has<br />

d(d + 1)/2 = 10 degrees of freedom per spacetime point x in four dimensions<br />

(perturbatively, the physical degrees of freedom in the continuum are much less:<br />

1<br />

2 d(d + 1) − 1 − d − (d − 1) = 1 2d(d − 3), for a traceless symmetric tensor, and after

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