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Feynman Path Integral Formulation

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298 8 Numerical Studies<br />

ξ ξ ξ<br />

Fig. 8.11 The lattice quantum continuum limit is gradually approached by considering sequences<br />

of lattices with increasingly larger correlation lengths ξ in lattice units. Such a limit requires the<br />

existence of an ultraviolet fixed point, where quantum field correlations extend over many lattice<br />

spacing.<br />

appears here as a consequence of the relatively small value of the lattice k c in four<br />

dimensions.<br />

The renormalization group invariance of the physical quantity m requires that<br />

the running gravitational coupling G(μ) varies in the vicinity of the fixed point in<br />

accordance with the above equation, with Λ → μ, where μ is now an arbitrary scale,<br />

( ) 1 ν [ ] G(μ) ν<br />

m = μ<br />

− 1 . (8.80)<br />

a 0 G c<br />

The latter is equivalent to the renormalization group invariance requirement<br />

μ d m[μ,G(μ)] = 0 , (8.81)<br />

d μ<br />

provided G(μ) is varied in a specific way. Indeed this type of situation was already<br />

encountered before, for example in Eqs. (3.62) and (3.122). Eq. (8.81) can therefore<br />

be used to obtain, if one so wishes, a β-function for the coupling G(μ) in units of<br />

the ultraviolet cutoff,<br />

μ ∂ G(μ) =β [G(μ)] , (8.82)<br />

∂μ<br />

with β(G) given in the vicinity of the non-trivial fixed point, using Eq. (8.80), by<br />

β(G) ≡ μ ∂<br />

∂μ G(μ)<br />

∼<br />

G→G c<br />

− 1 ν (G − G c)+... (8.83)<br />

The above procedure is in fact in complete analogy to what was done for the nonlinear<br />

σ-model, for example in Eq. (3.64). But the last two steps are not really<br />

necessary, for one can obtain the scale dependence of the gravitational coupling

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