The hydrodynamic model, originally proposed by Madelung [Mad27], provides a classical picture for quantum dynamics, namely, that of the flow of an indestructible probability fluid.
Mathematically it consists in representing using polar coordinates as
(6.17) |
Substituting this ansatz into the time-dependent Schrödinger equation with constant mass and separating into real and imaginary parts, gives two equations:
(6.20) |
In these formulas the prime denotes the one-dimensional space derivative.
The quantum potential arises from the kinetic energy of the Schrödinger equation and creates the ``self-field''. Alternatively can be seen as pressure in a hydrodynamical Navier-Stokes interpretation [Har66], which is related to Nelson's stochastic interpretation of quantum mechanics.
In the classical limit (e.g., WKB approximation [Kol00], [Sch69]) Equation 6.19 becomes the Hamilton-Jacobi equation with principal function .
With the identification of the velocity
(6.21) |
(6.22) |
(6.23) |
In the deBroglie-Bohm interpretation of quantum mechanics a particle has a sharp position at each time moving along a fluid trajectory determined by Equation 6.25 (with ). Evolution in the Bohm picture is ``sharp'', but the initial condition given by the initial location of the particle is a distribution. Tunneling is explained by lowering the barrier through the additional Bohm potential . This is a hidden variables theory which singles out position as a preferred variable. The same can be done for other observables, see [Vin00].
In the stationary case we have
(6.25) |
This gives and
(6.26) | ||
(6.27) |
The hydrodynamical formulation can be extended to the mixed state case and was used for quantum mechanical simulation in [BM02], [LW99], [Dal03], [Bit00].
It is pointed out in [Wal94], that the hydrodynamical formulation needs an additional quantization constraint for equivalence with the ``standard'' Schrödinger equation.
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