Andre' Quanta said:
During a course of QFT my teacher said that in this theory is not possible to use the operator X for the position in order to construct with the momentum P and the spin S a set of irreducible operators that charachterize particles, and that we need a different point of wiev: the irreducible unitary rappresentations of the Poincare Group?
Why is this true? Why i can' t use the operator X, P and S in QFT to describe particles as in the normal Q.M.?
The problem follows from the fact that QFT is not a single particle QM. So, in order to define a position operator one has to restrict oneself to the space of positive energy solutions of the equation of motion (as they are physically realizable by a free single particle). Even then, the usual definition of the position operator fails to be Hermitian and hence does not correspond to a measurable property, and when we define it to be Hermitian, the (localized) states, formed from its eigen-functions, fail to be Lorentz covariant.
To see this, consider the positive energy solutions of the KG equation. The space of such covariant solutions consists of all amplitudes \phi (x) of the form \phi (x) = \frac{\sqrt{2}}{(2 \pi)^{3/2}} \int d^{4}p \ e^{- i p \cdot x} \theta (p_{0}) \delta (p^{2} - m^{2}) \Phi (p) , or, by doing the p_{0} integration, \phi (x) = \frac{1}{\sqrt{2} (2 \pi)^{3/2}} \int \frac{d^{3}p}{p_{0}} \ e^{- i p \cdot x} \ \Phi (\mathbf{p}) , where p_{0} = + \sqrt{\mathbf{p}^{2} + m^{2}} and \Phi(\mathbf{p}) is (like \phi(x)) a scalar because d^{3}p/p_{0} is the invariant measure over the hyperboloid p^{2} = m^{2} and p \cdot x is Lorentz invariant.
Clearly, the space of positive energy solution is a linear vector space. So, in order to turn it into a Hilbert space, we need to define a suitable (i.e. Lorentz-invariant and time-independent) scalar product. Let us define the scalar product of two positive energy amplitudes by \left( \phi , \psi \right)_{\sigma} \equiv i \int_{\sigma} d \sigma^{\mu}(x) \ \phi^{*}(x) \overleftrightarrow{\partial_{\mu}} \psi (x) , \ \ \ \ (1) where \sigma is an arbitrary space-like hypersurface. The 4-vector surface element d\sigma^{\mu} (x) = n^{\mu}(x) d\sigma, (where n^{\mu}(x) is the unit normal to \sigma at x) has the components d\sigma^{\mu} = \{ dx^{1} dx^{2} dx^{3} , dt dx^{2}dx^{3}, dt dx^{1}dx^{3}, dt dx^{1}dx^{2} \} . For the hyperplane \sigma = t = \mbox{const.} equation (1) reduces to \left( \phi , \psi \right)_{t} \equiv i \int_{t} d^{3}x \ \phi^{*}(x) \overleftrightarrow{\partial_{t}} \psi (x) . \ \ \ \ (2) Going over to momentum space, the scalar product, (2), becomes \left( \phi , \psi \right) = \int_{+} \frac{d^{3}p}{p_{0}} \ \Phi^{*}(\mathbf{p}) \Psi (\mathbf{p}) . \ \ \ \ \ (3) This shows that (\phi , \phi) is positive definite if \phi \neq 0. It is also evident that ( \phi , \psi ) = ( \psi , \phi )^{*} and ( \phi + \chi , \psi ) = ( \phi , \psi ) + ( \chi , \psi ). Thus, our scalar product satisfies all the properties required of a scalar product.
Clearly the scalar product, eq(1), is Lorentz invariant. Also, it is easy to show that \frac{\delta}{\delta \sigma (x)} \left( \phi , \psi \right)_{\sigma} = 0 , if \phi and \psi satisfy the KG equation. This means that the scalar product does not depend on the space-like surface \sigma used to calculate it. Therefore, it is time-independent.
Now, it is easy to show that the usual quantum mechanical expression for the position operator \hat{X} = i \vec{\nabla}_{\mathbf{p}} is not Hermitian. Indeed, integrating by parts and ignoring a surface term gives
\int_{+} \frac{d^{3}p}{p_{0}} \ \Phi^{*}(\mathbf{p}) ( i \vec{\nabla}) \Psi (\mathbf{p}) = \int_{+} \frac{d^{3}p}{p_{0}} \left(- i \vec{\nabla} \Phi^{*}(\mathbf{p}) \right) \Psi (\mathbf{p}) + \int_{+} \frac{d^{3}p}{p_{0}} \Phi^{*}(\mathbf{p}) \frac{ i \mathbf{p}}{p_{0}^{2}} \Psi (\mathbf{p}) . \ \ (4) Thus, (\phi , \hat{X}\psi) \neq (\hat{X}\phi , \psi). It follows that the wave function \phi (x) cannot be a probability amplitude for finding the particle at (t , \mathbf{x}).
Equation (4), allows us to define the following Hermitian operator \hat{Q} = i \vec{\nabla}_{\mathbf{p}} - \frac{i \mathbf{p}}{2 p_{0}^{2}} , which agrees with the definition of the centre of mass in special relativity. It is the so-called Newton-Wigner position operator: they derived it from certain physical conditions on localized states. It turns out that the localized states do not form a Lorentz covariant manifold. They only have the symmetry properties in the hyperplane t = \mbox{constant} in spacetime.