A Concise Introduction to Quantum Field Theory 201
The subspace spanned by the vectorsφ(f 1 )φ(f 2 )···φ(fn)| 0 〉for arbitrary
test functionsf 1 ,f 2 ,···fn∈S(R^3 ) is a dense subspace ofH.
- P6Poincar ́e covariance: Letf ̃∈S(R^4 ) be a test function defined in
Minkowski space-time and
φ(f ̃)=
∫
R^4
d^4 xφ(x)f ̃(x),
whereφ(x)=φ(x,t)=eitP^0 φ(x)e−itP^0 .Then^4 ,
U(Λ,a)φ(f ̃)U(Λ,a)†=φ(f ̃(Λ,a)),
with
f ̃(Λ,a)(x)=f ̃(Λ−^1 (x−a)).
- P7(Bosonic) local causality:For anyf,g∈S(R^3 ) the corresponding field
operatorsφ(f),φ(g)commute^5 ,
[φ(f),φ(g)] = 0. (3.12)
3.3.1 Canonicalquantization
As in the case of quantum mechanics, there are special cases where the quantum
field theory arises from the quantization of a classical field theory^6.
Let us consider a scalar real fieldφin Minkowski space-timeR^4. The classical
field theory is defined according to the variational principle by stationary field
configurationsφ(x) of the classical action functional
S[φ(x)]≡
∫
d^4 xL(φ, ∂μφ)=
∫
d^4 x
( 1
2 ∂μφ∂
μφ−V(φ)). (3.13)
The equations of motion are obtained, thus, from the Euler-Lagrange equations
∂μ
[
δL
δ(∂μφ)
]
−δL
δφ
=0 =⇒ φ+δV
δφ
=0, (3.14)
where=∂μ∂μ. Notice that the Poincar ́e invariance of the action implies the
Poincar ́e invariance of the equations of motion.
(^4) For higher spin fields, the Poincar ́e representation satisfies the covariant transfomation law
U(Λ,a)φ(f)U(Λ,a)†=S(Λ)−^1 φ(f(Λ,a)), whereSis a linear n-dimensional representation of
Lorentz group andφis a field with n-components.
(^5) In the fermionic case, the commutator [·,·] is replaced by an anticommutator{·,·}.
(^6) See section 1.3.