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22 November 7, 2013<br />

The function S(ϕ) is called the action of the particular quantum field theory :<br />

in a sense, it is the theory. For the probability density to be acceptable, S(ϕ)<br />

must go to infinity sufficiently fast as |ϕ| → ∞. The normalization factor N is<br />

defined by 1 N −1 =<br />

∫<br />

exp ( − S(ϕ) ) dϕ . (1.2)<br />

It is of course also possible to have more than one field associated with the single<br />

spacetime point. If there are K fields ϕ 1 , ϕ 2 , . . . , ϕ K , they will have a combined<br />

probability density<br />

P (ϕ 1 , ϕ 2 , . . . , ϕ K ) = N exp ( − S(ϕ 1 , ϕ 2 , . . . , ϕ K ) ) , (1.3)<br />

with 2 ∫<br />

N −1 =<br />

∫<br />

· · ·<br />

exp ( − S(ϕ 1 , ϕ 2 , . . . , ϕ K ) ) dϕ 1 dϕ 2 · · · dϕ K . (1.4)<br />

In the special case where the action is separable, that is,<br />

S(ϕ 1 , ϕ 2 , . . . , ϕ K ) = S 1 (ϕ 1 ) + S 2 (ϕ 2 ) + · · · + S K (ϕ K ) ,<br />

the fields are actually independent random variables.<br />

1.2.2 Green’s functions, sources and the path integral<br />

Since the quantum field is a random variable, the most that can be computed<br />

about it 3 is the collection of its moments, in the jargon called Green’s functions 4 :<br />

∫<br />

G n ≡ 〈ϕ n 〉 ≡ N exp ( − S(ϕ) ) ϕ n dϕ , n = 0, 1, 2, 3, . . . . (1.5)<br />

We shall assume that G n exists for all n. By construction, we must always have<br />

G 0 = 〈 ϕ 0〉 = 〈1〉 = 1 . (1.6)<br />

1 If not explicitly indicated otherwise, integrals run from −∞ to +∞.<br />

2 In the following, multiple integrals will be denoted by a single integral sign for simplicity.<br />

This is usually clear from the context.<br />

3 You are here approaching a career decision. You may decide simply to measure the value<br />

of ϕ : in that case you have decided to become an eperimentalist rather than a theorist.<br />

4 A clarifying remark must be made here. In this text, the Green’s functions are simply<br />

defined to be expectation values. This may appear to contrast with the use of Green’s functions<br />

in the solution of inhomogeneous linear differential equations such as are encountered in<br />

classical elctrodynamics where one uses them to compute the electromagnetic field configurations<br />

for given sources. The difference is only apparent since, as we shall recognize, the latter<br />

type of Green’s functions are in our treatment simply the two-point Green’s functions ; and<br />

for theories such as electrodynamics, where the electromagnetic fields do not undergo selfinteraction,<br />

the two-point functions are in fact the only nonzero connected Green’s functions.<br />

Be not, therefore, misled into thinking that there are somehow two sorts of Green’s functions.<br />

The Green’s function formulation of electrodynamics will in fact appear as the classical limit<br />

of the Schwinger-Dyson equation discussed below.

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