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80 November 7, 2013<br />

For large m|⃗x|, the propagator therefore decreases exponentially, while for small<br />

m|⃗x|, we have<br />

Π(⃗x) ≈ ¯h ( ) 1<br />

2π log , D = 2 ,<br />

m|⃗x|<br />

Π(⃗x) ≈ ¯hΓ ( D<br />

2 − 1) x 2−D , D ≥ 3 . (2.67)<br />

4 π D/2<br />

In every dimension, the propagator is normalized in the same way :<br />

(<br />

∫<br />

Π(⃗x) d D x = ¯h ∫ ∫ exp i ⃗ )<br />

k · ⃗x<br />

(2π) D d D x d D k<br />

| ⃗ k| 2 + m 2<br />

=<br />

¯h<br />

(2π) D<br />

2.4.3 Three examples<br />

∫<br />

d D k (2π)D δ D ( ⃗ k)<br />

| ⃗ k| 2 + m 2 = ¯h m 2 . (2.68)<br />

We may consider where the evolution in Feynman rules has taken us so far.<br />

We can best illustrate this by inspecting three examples. In the first place, we<br />

of course have the lowest-order (no-loop) two-point function, the propagator,<br />

given by the diagram<br />

A 1 = x 1<br />

x 2<br />

(2.69)<br />

which equals<br />

A 1 = Π(⃗x 1 − ⃗x 2 ) . (2.70)<br />

Next, we we can look at the lowest-order contributions to the four-point function:<br />

A 2 = 〈ϕ(⃗x 1 )ϕ(⃗x 2 )ϕ(⃗x 3 )ϕ(⃗x 4 )〉 in ϕ 4 theory. According to the standard<br />

rules, we can obtain this Green’s function by writing down all Feynman diagrams<br />

with four external lines, and no source vertices. In lowest order of the<br />

loop expansion, this Green’s function contains four diagrams :<br />

x 1<br />

x 2<br />

x 1<br />

x<br />

A 2 =<br />

+<br />

x x 4<br />

3<br />

x 1<br />

x<br />

2<br />

x<br />

x<br />

+<br />

4<br />

+<br />

3<br />

x x 4<br />

3<br />

and, upon implementation of the Feynman rules, evaluate to<br />

A 2 = Π(⃗x 1 − ⃗x 2 ) Π(⃗x 3 − ⃗x 4 )<br />

+ Π(⃗x 1 − ⃗x 3 ) Π(⃗x 2 − ⃗x 4 )<br />

x<br />

x<br />

2<br />

1<br />

2<br />

y<br />

x<br />

x<br />

3<br />

4<br />

, (2.71)<br />

+ Π(⃗x 1 − ⃗x 4 ) Π(⃗x 3 − ⃗x 2 )<br />

− λ ∫<br />

4<br />

d D ⃗y Π(⃗x 1 − ⃗y) Π(⃗x 2 − ⃗y) Π(⃗x 3 − ⃗y) Π(⃗x 4 − ⃗y) . (2.72)<br />

¯h

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