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Feynman Path Integral Formulation

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222 6 Lattice Regularized Quantum Gravity<br />

To actually show this, it will be useful to introduce an artificial integration ∫ [dΩ]<br />

over the gauge group parameters, by writing for the Euclidean partition function<br />

∫<br />

Z = [dA]e −S(A)<br />

∫<br />

= const. [dΩ][dA]e −S(A)<br />

∫<br />

= const. [dΩ][dA Ω ]e −S(A)<br />

∫<br />

= const. [dΩ][dA]e −S(A Ω −1 ) . (6.213)<br />

To take into account the effect of the Ω variables one first integrates over them, and<br />

then deduces from this procedure an effective action for the A fields,<br />

S eff (A) =S 0 (A)+δS inv (A) . (6.214)<br />

The new effective action is made out of the original invariant contribution S 0 (A),<br />

plus a correction from δS inv (A), which is obtained from<br />

∫<br />

exp{−δS inv (A)} = [dΩ] exp{−S(A Ω −1)} . (6.215)<br />

In general there is no guarantee that the additional contribution δS inv (A) will be<br />

local, i.e. of the form<br />

∫<br />

δS inv (A) = dx δL inv [A(x)] . (6.216)<br />

But the δS inv (A) term will indeed be local provided certain conditions are met, i.e.<br />

that the correlations in the Ω variables will be sufficiently short ranged. Then at<br />

distances large compared to the correlation length ξ Ω of the Ω variables it is possible<br />

to expand δL inv [A(x)] in terms of locally gauge invariant terms of the type<br />

tr(F μν ) 2 ,tr(∇ σ F μν ) 2 , etc. At sufficiently large distances one expects only terms<br />

with the lowest dimensions to be important, the leading one being tr(F μν ) 2 , whose<br />

effect will be just to renormalize the bare gauge coupling.<br />

Clearly the argument for the decoupling of the Ω variables only works if there<br />

are long range correlations in the unperturbed gauge variables A μ (so that the<br />

two correlation lengths can be compared to each other, and thus the notion of<br />

“short range” makes sense) which implies g ≫ 1 in an asymptotically free gauge<br />

theory, or in general that one is close to an ultraviolet fixed point of the gauge<br />

theory.<br />

In summary, the expectation is that if the non-invariant correction is small there<br />

are no significant changes compared to the invariant theory, which is a rather remarkable<br />

result. On the other hand if the non-invariant correction is large then a<br />

phase transition appears and one moves into a qualitatively new phase. The argument<br />

is nice because of its simplicity, but still leaves one major issue open: namely

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