20.01.2015 Views

Feynman Path Integral Formulation

Feynman Path Integral Formulation

Feynman Path Integral Formulation

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

7.6 Discrete Gravity in the Large-d Limit 265<br />

Here we have further allowed for the possibility that the average lattice spacing<br />

l 0 = 〈l 2 〉 1/2 is not equal to one (in other words, we have restored the appropriate<br />

overall scale for the average edge length, which is in fact largely determined by the<br />

value of λ 0 ).<br />

The average lattice spacing l 0 can easily be estimated from the following argument.<br />

The volume of a general equilateral simplex is given by Eq. (7.133), multiplied<br />

by an additional factor of l0 d . In the limit of small k the average volume of a<br />

simplex is largely determined by the cosmological term, and can therefore be computed<br />

from<br />

< V >= − ∂ ∫<br />

log [dl 2 ]e −λ 0V (l 2) , (7.148)<br />

∂λ 0<br />

with V (l 2 )=( √ d + 1/d!2 d/2 )l d ≡ c d l d . After doing the integral over l 2 with measure<br />

dl 2 and solving this last expression for l0 2 one obtains<br />

[ ] 2/d<br />

l0 2 = 1 2 d!2 d/2<br />

λ 2/d √ , (7.149)<br />

d d + 1<br />

0<br />

(which, for example, gives l 0 = 2.153 for λ 0 = 1 in four dimensions, in reasonable<br />

agreement with the actual value l 0 ≈ 2.43 found near the transition point).<br />

This then gives for λ 0 = 1 the estimate k c = √ 3/(16·5 1/4 )=0.0724 in d = 4, to<br />

be compared with k c = 0.0636(11) obtained in (Hamber, 2000) by direct numerical<br />

simulation in four dimensions. Even in d = 3 one finds again for λ 0 = 1, from<br />

Eqs. (7.147) and (7.149), k c = 2 5/3 /27 = 0.118, to be compared with k c = 0.112(5)<br />

obtained in (Hamber and Williams, 1993) by direct numerical simulation.<br />

Using Eq. (7.149) inserted into Eq. (7.147) one obtains in the large d limit for<br />

the dimensionless combination k/λ (d−2)/d<br />

0<br />

k c<br />

λ 1−2/d<br />

0<br />

= 21+2/d<br />

d 3<br />

[ Γ (d)<br />

√<br />

d + 1<br />

] 2/d<br />

. (7.150)<br />

To summarize, an expansion in powers of 1/d can be developed, which relies on a<br />

combined use of the weak field expansion. It can be regarded therefore as a double<br />

expansion in 1/d and ε, valid wherever the fields are smooth enough and the geometry<br />

is close to flat, which presumably is the case in the vicinity of the lattice critical<br />

point at k c .<br />

A somewhat complementary 1/d expansion can be set up, which does not require<br />

weak fields, but relies instead on the strong coupling (small k = 1/8πG, or large<br />

G) limit. As such it will be a double expansion in 1/d and k. Its validity will be<br />

in a regime where the fields are not smooth, and in fact will involve lattice field<br />

configurations which are very far from smooth at short distances.<br />

The general framework for the strong coupling expansion for pure quantum gravity<br />

was outlined in the previous section, and is quite analogous to what one does in<br />

gauge theories (Balian, Drouffe and Itzykson, 1975). One expands Z latt in powers<br />

of k as in Eq. (7.68)

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!