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Feynman Path Integral Formulation

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3.4 Self-coupled Fermion Model 83<br />

3.4 Self-coupled Fermion Model<br />

The non-linear sigma model is not an isolated example of a field theory that is<br />

not perturbatively renormalizable above two dimensions, although it is certainly by<br />

far the most thoroghly explored one. Here it seems worthwhile to mention a second<br />

example of a theory which naively is not perturbatively renormalizable in d > 2, and<br />

yet whose critical properties can again be worked out both in the 2 + ε expansion,<br />

and in the large N limit. It is described by an U(N)-invariant action containing a set<br />

of N massless self-coupled Dirac fermions (Wilson, 1973; Gross and Neveu, 1974)<br />

∫<br />

S(ψ, ¯ψ)=− d d x[ ¯ψ· ̸∂ψ+ 1 2 Λ d−2 u( ¯ψ · ψ) 2 ] . (3.69)<br />

In even dimensions the discrete chiral symmetry ψ → γ 5 ψ, ¯ψ →−¯ψγ 5 prevents the<br />

appearance of a fermion mass term. Interest in the model resides in the fact that it<br />

exhibits a mechanism for dynamical mass generation and chiral symmetry breaking.<br />

In two dimensions the fermion self-coupling constant is dimensionless, and after<br />

setting d = 2+ε one is again ready to develop the full machinery of the perturbative<br />

expansion in u and ε, as was done for the non-linear σ-model, since the model is<br />

again believed to be multiplicatively renormalizable in the framework of the 2 + ε<br />

expansion. For the β-function one finds to three loops<br />

β(u)=εu − ¯N − 2<br />

2π u2 + ¯N − 2<br />

4π 2 u3 + ( ¯N − 2)( ¯N − 7)<br />

32π 3 u 4 + ... (3.70)<br />

with the parameter ¯N = N tr1, where the last quantity is the identity matrix in the γ-<br />

matrix algebra. In two dimensions ¯N = 2N and the model is asymptotically free; for<br />

¯N = 2 the interaction is proportional to the Thirring one and the β-function vanishes<br />

identically.<br />

As for the case of the non-linear σ-model, the solution of the renormalization<br />

group equations involves an invariant scale, which can be obtained (up to a constant<br />

which cannot be determined from perturbation theory alone) by integrating<br />

Eq. (3.70)<br />

[ ∫ u<br />

ξ −1 du ′ ]<br />

(u)=m(u)=const.Λ exp −<br />

β(u ′ . (3.71)<br />

)<br />

In two dimensions this scale is, to lowest order in u, proportional to<br />

[<br />

m(u) ∼ Λ exp −<br />

2π ]<br />

, (3.72)<br />

u→0 ( ¯N − 2)u<br />

and thus non-analytic in the bare coupling u. Above two dimensions a non-trivial<br />

ultraviolet fixed point appears at<br />

u c =<br />

2π<br />

¯N − 2 ε + 2π<br />

( ¯N − 2) 2 ε2 + ( ¯N + 1)π<br />

2( ¯N − 2) 3 ε3 + ... (3.73)

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