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Astron. Astrophys. 337, 299-310 (1998)
7. Conclusion
As a summary account of this paper that investigates a macroscopic
context for Schroedinger equation at the scale of the Solar System,
let us emphasize the following new results:
-
There is a `dynamical degeneracy' of any stationary quantum state
. Indeed, to each such state defined by the
energy eigenvalue E, one can associate an infinity of dynamical
states of the system that are defined through Eqs. (22) and (29-32) by
a particular value of the Wronskian A of the Schroedinger
equation.
-
These dynamical states, the existence of which is guaranteed by i)
the Planck-DeBroglie postulate stating that the phase of the
wavefunction (3) is Hamilton's characteristic (or principal) function
S of the system, and ii) the canonical Hamilton-Jacobi equation
(31), must be understood in the classical (causal) sense.
-
The quantity (averaged over the polar
angles) is the local classical statistical probability distribution
(36) of the particle position in terms of the corresponding velocity
flow derived from the radial momentum field (29-32).
-
There exists for any energy level E of the system a
particular state defined by Eqs. (40-43). It describes a
classical-like dynamical behaviour of the system within the
classically allowed region in accordance with Eq. (39). We suggest to
call this quantum state the `classical-like quantum state', and the
corresponding steady-state radial-velocity matter flow the
`classical-like static soliton mode'.
© European Southern Observatory (ESO) 1998
Online publication: August 6, 1998
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