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42 November 7, 2013<br />

1.4.3 The classical limit<br />

Since in perturbation theory ¯h is taken to be an infinitesimally small quantity,<br />

the limit ¯h → 0 is of automatic interest. This limit has to be taken with some<br />

care since ¯h = 0 strictly would imply that only Green’s functions with E +L = 1<br />

would survive 24 . Instead, the classical limit ¯h → 0 is meant to be the result of<br />

leaving out diagrams containing closed loops. The diagrammatic SDe will, for<br />

the ϕ 3/4 theory, then take the form<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000<br />

11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

= +<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

+<br />

000000<br />

111111<br />

000000<br />

111111<br />

000000<br />

111111<br />

000000<br />

111111<br />

000000<br />

111111<br />

000000<br />

111111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

00000 11111<br />

0000 1111<br />

0000 1111<br />

0000 1111<br />

11110000<br />

11110000<br />

11110000<br />

11110000<br />

0000 1111<br />

0000 1111<br />

0000 1111<br />

. (1.76)<br />

The corresponding solution will be denoted by φ c (J) (with c for ‘classical’), and<br />

the classical SDe is written as<br />

φ c (J) = J µ − λ 3<br />

2µ φ c(J) 2 − λ 4<br />

6µ φ c(J) 3 . (1.77)<br />

The classical field function is exclusively built up from tree diagrams : this is<br />

called the tree approximation. Note that it obeys an algebraic, rather than a<br />

differential, equation, that can be written as<br />

S ′ (φ c (J)) = J . (1.78)<br />

This is called the classical field equation. This is not to be confused with equations<br />

from classical, nonquantum physics. In fact, the classical field equations<br />

will turn out to be the Klein-Gordon, Dirac, Proca and Maxwell equations. Of<br />

these, only the Maxwell equations can be considered classical, since they do not<br />

contain a particle mass.. Note that such equations have, in general, more than<br />

a single solution. Here, however, we are interested in that solution that vanishes<br />

as J → 0, which may be written out using Lagrange expansion :<br />

φ c (J) = J µ + ∑ n≥1<br />

1 ∂ n−1 ( J<br />

[(S<br />

n! µn−1 ′ (∂J) n−1 µ<br />

)) n ]<br />

. (1.79)<br />

Let us now look at the path-integral picture of the classical limit.<br />

becomes small, the fluctuations in the path integrand<br />

(<br />

exp − 1¯h<br />

( ))<br />

S(ϕ) − Jϕ<br />

When ¯h<br />

become extremely exaggerated. The main contribution to 〈ϕ〉 therefore comes<br />

from that value where the probability distribution attains its maximum, that<br />

is,<br />

〈ϕ〉 J<br />

≈ ϕ c , where S ′ (ϕ c ) = J , S ′′ (ϕ c ) > 0 . (1.80)<br />

Also in the classical limit, we therefore have φ c (J) = ϕ c .<br />

24 Later on, the discussion about truncation will clarify how this is not inconsistent.

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