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Feynman Path Integral Formulation

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6.4 Rotations, Parallel Transports and Voronoi Loops 173<br />

Next, in order to introduce curvature, one needs to define the dihedral angle between<br />

faces in an n-simplex. In an n-simplex s two n − 1-simplices f and f ′ will intersect<br />

on a common n − 2-simplex h, and the dihedral angle at the specified hinge h is<br />

defined as<br />

cosθ( f , f ′ )= ω( f ) n−1 · ω( f ′ ) n−1<br />

V n−1 ( f )V n−1 ( f ′ , (6.10)<br />

)<br />

where the scalar product appearing on the r.h.s. can be re-written in terms of squared<br />

edge lengths using<br />

ω n · ω ′ n = 1<br />

(n!) 2 det(e i · e ′ j) , (6.11)<br />

and e i · e ′ j in turn expressed in terms of squared edge lengths by the use of Eq. (6.3).<br />

(Note that the dihedral angle θ would have to be defined as π minus the arccosine<br />

of the expression on the r.h.s. if the orientation for the e’s had been chosen in such<br />

a way that the ω’s would all point from the face f inward into the simplex s). As an<br />

example, in two dimensions and within a given triangle, two edges will intersect at<br />

a vertex, giving θ as the angle between the two edges. In three dimensions within<br />

a given simplex two triangles will intersect at a given edge, while in four dimension<br />

two tetrahedra will meet at a triangle. For the special case of an equilateral<br />

n-simplex, one has simply θ = arccos 1 n<br />

. A related and often used formula for the<br />

sine of the dihedral angle θ is<br />

sinθ( f , f ′ )=<br />

n V n (s)V n−2 (h)<br />

n − 1 V n−1 ( f )V n−1 ( f ′ ) , (6.12)<br />

but is less useful for practical calculations, as the sine of the angle does not unambiguously<br />

determine the angle itself, which is needed in order to compute the local<br />

curvature.<br />

In a piecewise linear space curvature is detected by going around elementary<br />

loops which are dual to a (d − 2)-dimensional subspace. From the dihedral angles<br />

associated with the faces of the simplices meeting at a given hinge h one can compute<br />

the deficit angle δ(h), defined as<br />

δ(h) =2π − ∑ θ(s,h) , (6.13)<br />

s⊃h<br />

where the sum extends over all simplices s meeting on h. It then follows that the<br />

deficit angle δ is a measure of the curvature at h. The two-dimensional case is illustrated<br />

in Fig. 6.4, while the three- and four-dimensional cases are shown in Fig. 6.5.<br />

6.4 Rotations, Parallel Transports and Voronoi Loops<br />

Since the interior of each simplex s is assumed to be flat, one can assign to it a<br />

Lorentz frame Σ(s). Furthermore inside s one can define a d-component vector

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