WKB Approximation
Consider a particle of mass and energy moving through some slowly-varying
potential, . The particle's wavefunction satisfies
|
(11.116) |
where
|
(11.117) |
Let us try a solution to Equation (11.116) of the form
|
(11.118) |
where is a complex constant. Note that this solution represents
a particle propagating in the positive -direction [because the full
wavefunction is multiplied by
, where
] with the continuously-varying wavenumber
.
It follows that
|
(11.119) |
and
|
(11.120) |
where
. A comparison of Equations (11.116) and (11.120)
reveals that Equation (11.118) represents an approximate solution to
Equation (11.116) provided that the first term on the right-hand side of Equation (11.120)
is negligible compared to the second. This yields
the validity criterion
, or
|
(11.121) |
In other words, the variation lengthscale of , which is
approximately the same as the variation lengthscale of , must
be much greater than the particle's de Broglie wavelength (which
is of order ). Let us suppose that this is the case. Incidentally,
the approximation involved in dropping the first term on the right-hand side
of Equation (11.120) is generally known as the WKB approximation, after G. Wentzel, H.A. Kramers, and L. Brillouin. (See Section 6.10.)
Similarly, Equation (11.118) is termed a WKB solution.
According to the WKB solution, (11.118), the probability
density remains constant; that is,
|
(11.122) |
as long as the particle
moves through a region in which , and is consequently real (i.e., an allowed region
according to classical physics).
Suppose, however, that the particle encounters a potential barrier (i.e., a region from which the particle is excluded according to classical
physics). By definition, inside such a barrier, and
is consequently imaginary. Let the barrier extend from to , where
. The WKB solution inside the barrier is written
|
(11.123) |
where
|
(11.124) |
Here, we have neglected the unphysical exponentially-growing solution.
According to the WKB solution, (11.123), the probability
density decays exponentially inside the barrier; that is,
|
(11.125) |
where
is the probability density at the left-hand
side of the barrier (i.e., ). It follows that the
probability density at the right-hand side of the barrier (i.e., ) is
|
(11.126) |
Note that
. Of course, in the region to the right of the
barrier (i.e., ), the probability density takes the
constant value
.
We can interpret the ratio of the probability densities to the right and to the left of the potential barrier as the probability, , that a particle
incident from the left will tunnel through the barrier and
emerge on the other side; that is,
|
(11.127) |
It is easily demonstrated that the probability of a particle incident from the
right tunneling through the barrier is the same.
Note that the criterion (11.121) for the validity of the WKB approximation
implies that the previous transmission probability is very small. Hence,
the WKB approximation only applies to situations in which there is
very little chance of a particle tunneling through the potential barrier in question.
Unfortunately, the validity criterion (11.121) breaks down completely
at the edges of the barrier (i.e., at and ), because
at these points. However, it can be demonstrated that the
contribution of those regions, around and , in which the WKB
approximation breaks down to the integral in Equation (11.127)
is fairly negligible (Schiff 1955). Hence, the previous expression for the tunneling
probability is a reasonable approximation provided that the incident particle's
de Broglie wavelength is much smaller than the spatial extent of the potential
barrier.