On the transition from the quantum to the classical regime for massive scalar particles: A spatiotemporal approach

摘要

If the classical structure of space-time is assumed to define an a priori scenario for the formulation of quantum theory (QT), the coordinate representation of the solutions psi((x) over right arrow, t) (psi((x) over right arrow (1), ..., (x) over right arrow (N), t)) of the Schroedinger equation of a quantum system containing one (N) massive scalar particle has a preferred status. Let us consider all of the solutions admitting a multipolar expansion of the probability density function rho((x) over right arrow, t) = vertical bar psi((x) over right arrow, t)vertical bar(2) (and more generally of the Wigner function) around a space-time trajectory (x) over right arrow (c)(t) to be properly selected. For every normalized solution ( integral d(3) x rho((x) over right arrow, t) = 1) there is a privileged trajectory implying the vanishing of the dipole moment of the multipolar expansion: it is given by the expectation value of the position operator si(t)vertical bar(x) over right arrow vertical bar psi(t) = (x) over right arrow (c)(t). Then, the special subset of solutions psi((x) over right arrow, t) which satisfy Ehrenfest's Theorem (named thereby Ehrenfest monopole wave functions (EMWF)), have the important property that this privileged classical trajectory (x) over right arrow (c)(t) is determined by a closed Newtonian equation of motion where the effective force is the Newtonian force plus non-Newtonian terms (of order (h) over bar (2) or higher) depending on the higher multipoles of the probability distribution rho. Note that the superposition of two EMWFs is not an EMWF, a result to be strongly hoped for, given the possible unwanted implications concerning classical spatial perception. These results can be extended to N-particle systems in such a way that, when N classical trajectories with all the dipole moments vanishing and satisfying Ehrenfest theorem are associated with the normalized wave functions of the N-body system, we get a natural transition from the 3N-dimensional configuration space to the space-time. Moreover, these results can be extended to relativistic quantum mechanics. Consequently, in suitable states of N quantum particle which are EMWF, we get the "emergence" of corresponding "classical particles" following Newton-like trajectories in space-time. Note that all this holds true in the standard framework of quantum mechanics, i.e. assuming, in particular, the validity of Born's rule and the individual system interpretation of the wave function (no ensemble interpretation). These results are valid without any approximation (like (h) over bar -> 0, big quantum numbers, etc.). Moreover, we do not commit ourselves to any specific ontological interpretation of quantum theory (such as, e. g., the Bohmian one). We will argue that, in substantial agreement with Bohr's viewpoint, the macroscopic description of the preparation, certain intermediate steps and the detection of the final outcome of experiments involving massive particles are dominated by these classical "effective" trajectories. This approach can be applied to the point of view of de-coherence in the case of a diagonal reduced density matrix rho(red) (an improper mixture) depending on the position variables of a massive particle and of a pointer.