meopemuk said:
There are two things that look very similar, but have very different physical interpretations. One of them I denote a(x) and call "operator annihilating particle at space point x". The other one I denote \psi(x) and call "particle annihilation field".
Thanks for the clarification. Let me rewrite what you said in covariant notation. For simplicity, I only consider neutral scalar fields, and take hbar=c=1. I use the inner product with signature +---, and write Dp for the appropriately normalized invariant measure on the mass shell. I write a(p) for the annihilation operator with 4-momentum p, scaled such that the smeared annihilators
a(f):=\int Dp f(p) a(p)
satisfy
[a(f),a(g)^*]=\int Dp f(p) g(p)^*
for square integrable test functions f,g on the mass shell.
(This differs from Weinberg's annihilation operators by a factor proportional to sqrt(p_0) but has the advantage of making everything manifestly covariant.) Then we have several kinds of quantum fields:
A. The annihilation field
\psi^+(x) = \int Dp e^{ip\cdot x}a(p)
that annihilates the vacuum. It satisfies covariance but violates causality. The adjoint creation field
\psi^-(x) = \int Dp e^{-ip\cdot x}a(p)^*
creates 1-particle states from the vacuum and also satisfies covariance but violates causality.
B. The Heisenberg field (as it is commonly called)
\psi(x) = \psi^+(x) + \psi^-(x)
that figures in the interaction density. It satisfies covariance and causality, hence can be used to define an interaction density.
C. For each future-pointing velocity 4-vector u with u^2=1, a Newton-Wigner field
a_u(x) = \int Dp \sqrt{u\cdot p} e^{ip\cdot x}a(p)
and its adjoint. They are frame-dependent and violate covariance but satisfy a CCR of the form
[a_u(x),a_u(y)^*]=0~~~~~~~ (u\cdot x=u\cdot y,~~ x\ne y).
An observer moving along the world line x(s) with velocity u(s)=\dotx(s) has at each moment s its private time coordinate t(s)=u(s)\cdot x(s), its private 3-space defined by the hyperplane u(s)\cdot x=t(s), and its private Newton-Wigner field a(s)=a_{u(s)} (dependence on x suppressed). Because of the CCR, the latter can in principle be prepared and measured independently at each point of the private 3-space.
D. For every sufficiently nice kernel K(p,q) the composite field
N_K(x) = \int Dp Dq K(p,q) e^{i(q-p)\cdot x}a(p)^*a(q)
It transforms covariantly iff K(p,q) is Lorentz invariant, and its commutation properties can be worked out; I'll do this another time. Some of these fields - which ones we'll have to discuss - deserve to be called mass density field, energy density field, etc..
According to the traditional terminology, all these fields deserve to be called quantum fields, since they are operator-valued distributions.
''In physics, a field is a physical quantity associated to each point of spacetime. [...] a field can be either a classical field or a quantum field, depending on whether it is characterized by numbers or quantum operators respectively.'' (
http://en.wikipedia.org/wiki/Quantum_field )