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 [itex]\phi (x)[/itex] of the form [tex]\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) ,[/tex] or, by doing the [itex]p_{0}[/itex] integration, [tex]\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}) ,[/tex] where [itex]p_{0} = + \sqrt{\mathbf{p}^{2} + m^{2}}[/itex] and [itex]\Phi(\mathbf{p})[/itex] is (like [itex]\phi(x)[/itex]) a scalar because [itex]d^{3}p/p_{0}[/itex] is the invariant measure over the hyperboloid [itex]p^{2} = m^{2}[/itex] and [itex]p \cdot x[/itex] 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 [tex]\left( \phi , \psi \right)_{\sigma} \equiv i \int_{\sigma} d \sigma^{\mu}(x) \ \phi^{*}(x) \overleftrightarrow{\partial_{\mu}} \psi (x) , \ \ \ \ (1)[/tex] where [itex]\sigma[/itex] is an arbitrary space-like hypersurface. The 4-vector surface element [itex]d\sigma^{\mu} (x) = n^{\mu}(x) d\sigma[/itex], (where [itex]n^{\mu}(x)[/itex] is the unit normal to [itex]\sigma[/itex] at [itex]x[/itex]) has the components [tex]d\sigma^{\mu} = \{ dx^{1} dx^{2} dx^{3} , dt dx^{2}dx^{3}, dt dx^{1}dx^{3}, dt dx^{1}dx^{2} \} .[/tex] For the hyperplane [itex]\sigma = t = \mbox{const.}[/itex] equation (1) reduces to [tex]\left( \phi , \psi \right)_{t} \equiv i \int_{t} d^{3}x \ \phi^{*}(x) \overleftrightarrow{\partial_{t}} \psi (x) . \ \ \ \ (2)[/tex] Going over to momentum space, the scalar product, (2), becomes [tex]\left( \phi , \psi \right) = \int_{+} \frac{d^{3}p}{p_{0}} \ \Phi^{*}(\mathbf{p}) \Psi (\mathbf{p}) . \ \ \ \ \ (3)[/tex] This shows that [itex](\phi , \phi)[/itex] is positive definite if [itex]\phi \neq 0[/itex]. It is also evident that [itex]( \phi , \psi ) = ( \psi , \phi )^{*}[/itex] and [itex]( \phi + \chi , \psi ) = ( \phi , \psi ) + ( \chi , \psi )[/itex]. 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 [tex]\frac{\delta}{\delta \sigma (x)} \left( \phi , \psi \right)_{\sigma} = 0 ,[/tex] if [itex]\phi[/itex] and [itex]\psi[/itex] satisfy the KG equation. This means that the scalar product does not depend on the space-like surface [itex]\sigma[/itex] 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 [itex]\hat{X} = i \vec{\nabla}_{\mathbf{p}}[/itex] is not Hermitian. Indeed, integrating by parts and ignoring a surface term gives
[tex]\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)[/tex] Thus, [itex](\phi , \hat{X}\psi) \neq (\hat{X}\phi , \psi)[/itex]. It follows that the wave function [itex]\phi (x)[/itex] cannot be a probability amplitude for finding the particle at [itex](t , \mathbf{x})[/itex].
Equation (4), allows us to define the following Hermitian operator [tex]\hat{Q} = i \vec{\nabla}_{\mathbf{p}} - \frac{i \mathbf{p}}{2 p_{0}^{2}} ,[/tex] 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 [itex]t = \mbox{constant}[/itex] in spacetime.