Both the classical and tunneling WKB approximations of addendum
{A.26} fail near so-called “turning points”
where the classical kinetic energy
becomes zero. This note
explains how the problem can be fixed.
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The trick is to use a different approximation near turning points. In
a small vicinity of a turning point, it can normally be assumed that
the
-derivative
of the potential is about constant, so that
the potential varies linearly with position. Under that condition,
the exact solution of the Hamiltonian eigenvalue problem is known to
be a combination of two special functions Ai and Bi that are called
the “Airy” functions. These functions are shown in
figure A.17. The general solution near a turning point
is:
The second step is to relate this solution to the normal WKB
approximations away from the turning point. Now from a macroscopic
point of view, the WKB approximation follows from the assumption that
Planck’s constant
is very small. That implies that the
validity of the Airy functions normally extends to region where
is relatively large. For example, if you focus
attention on a point where
is a finite multiple of
,
is small, so the value of
will deviate
little from its value at the turning point: the assumption of linearly
varying potential remains valid. Still, if
is a finite multiple
of
,
will be proportional to
, and that is large. Such regions of large, but not
too large,
are called “matching regions,” because in them both the Airy function
solution and the WKB solution are valid. It is where the two meet and
must agree.
It is graphically depicted in figures A.18 and
A.19. Away from the turning points, the classical or
tunneling WKB approximations apply, depending on whether the total
energy is more than the potential energy or less. In the vicinity of
the turning points, the solution is a combination of the Airy
functions. If you look up in a mathematical handbook like
[1] how the Airy functions can be approximated
for large positive respectively negative
, you find the
expressions listed in the bottom lines of the figures. (After you
rewrite what you find in table books in terms of useful quantities,
that is!)
The expressions in the bottom lines must agree with what the
classical, respectively tunneling WKB approximation say about the
matching regions. At one side of the turning point, that relates the
coefficients
and
of the tunneling
approximation to the coefficients of
and
of
the Airy functions. At the other side, it relates the coefficients
and
(or
and
) of
the classical WKB approximation to
and
. The
net effect of it all is to relate, “connect,” the
coefficients of the classical WKB approximation to those of the
tunneling one. That is why the formulae in figures
A.18 and A.19 are called the “connection formulae.”
You may have noted the appearance of an additional constant
in
figures A.18 and A.19. This nasty
constant is defined as
As an example of how the connection formulae are used, consider a
right turning point for the harmonic oscillator or similar. Near such
a turning point, the connection formulae of figure
A.18 apply. In the tunneling region towards the
right, the term
better be zero, because it
blows up at large
, and that would put the particle at infinity for
sure. So the constant
will have to be zero. Now the
matching at the right side equates
to
so
will have to be zero. That
means that the solution in the vicinity of the turning point will have
to be a pure Ai function. Then the matching towards the left shows
that the solution in the classical WKB region must take the form of a
sine that, when extrapolated to the turning point
,
stops short of reaching zero by an angular amount
. Hence the
assertion in addendum {A.26} that the angular range of the
classical WKB solution should be shortened by
for each end at
which the particle is trapped by a gradually increasing potential
instead of an impenetrable wall.
As another example, consider tunneling as discussed in chapter
7.12 and 7.13. Figure A.20
shows a sketch. The WKB approximation may be used if the barrier
through which the particle tunnels is high and wide. In the far right
region, the energy eigenfunction only involves a term
with a forward wave speed. To simplify
the analysis, the constant
can be taken to be one,
because it does not make a difference how the wave function is
normalized. Also, the integration constant in
can be chosen
such that
at turning point 2; then the connection
formulae of figure A.19 along with the Euler formula
(2.5) show that the coefficients of the Airy functions at
turning point 2 are
and
. Next, the
integration constant in
can be taken such that
at
turning point 2; then the connection formulae of figure
A.19 imply that
and
.
Next consider the connection formulae for turning point 1 in figure
A.18. Note that
can be written as
, where
, because the
integration constant in
was chosen such that
.
The advantage of using
instead of
is
that it is independent of the choice of integration constant.
Furthermore, under the typical conditions that the WKB approximation
applies, for a high and wide barrier,
will be a very
large number. It is then seen from figure A.18 that
near turning point 1,
which is large
while
is small and will be ignored. And that then
implies, using the Euler formula to convert Ai’s sine into
exponentials, that
. As
discussed in chapter 7.13, the transmission coefficient
is given by