With
denoting here the elementary charge, the Coulomb potential
between two point particles with charges
and masses
separated by a distance
is
,
where
are atomic numbers,
is the electric constant,
is the fine structure constant,
and
is the reduced Planck’s constant.
The reduced mass is
,
and at energy of relative motion
with relative orbital angular momentum
,
the Schrödinger equation for the radial wave function
is given by
The
-scaled variables
and
of §33.2 are
given by
At positive energies
,
, and:
| Attractive potentials: |
|
|---|---|
|
Zero potential ( |
|
| Repulsive potentials: |
|
The
-scaled variables
and
of §33.14 are given
by
For
and
, the electron mass, the scaling factors in (33.22.5)
reduce to the Bohr radius,
,
and to a multiple of the Rydberg constant,
.
| Attractive potentials: |
|
|---|---|
|
Zero potential ( |
|
| Repulsive potentials: |
|
The
-scaled variables
and
of §13.2
are given by
| Attractive potentials: |
|
|---|---|
|
Zero potential ( |
|
| Repulsive potentials: |
|
Customary variables are
in atomic physics and
in
atomic and nuclear physics. Both variable sets may be used for attractive and
repulsive potentials: the
set cannot be used for a zero
potential because this would imply
for all
, and the
set cannot be used for zero energy
because this would imply
always.
The relativistic motion of spinless particles in a Coulomb field, as encountered in pionic atoms and pion-nucleon scattering (Backenstoss (1970)) is described by a Klein–Gordon equation equivalent to (33.2.1); see Barnett (1981a). The motion of a relativistic electron in a Coulomb field, which arises in the theory of the electronic structure of heavy elements (Johnson (2007)), is described by a Dirac equation. The solutions to this equation are closely related to the Coulomb functions; see Greiner et al. (1985).
The Coulomb solutions of the Schrödinger and Klein–Gordon equations are almost always used in the external region, outside the range of any non-Coulomb forces or couplings.
For scattering problems, the interior solution is then matched to a linear
combination of a pair of Coulomb functions,
and
, or
and
, to determine the scattering
-matrix and
also the correct normalization of the interior wave solutions; see
Bloch et al. (1951).
For bound-state problems only the exponentially decaying solution is required,
usually taken to be the Whittaker function
. The functions
defined by (33.14.14) are the hydrogenic bound states in
attractive Coulomb potentials; their polynomial components are often called
associated Laguerre functions; see Christy and Duck (1961) and
Bethe and Salpeter (1977).
The penetrability of repulsive Coulomb potential barriers is normally expressed
in terms of the quantity
(Mott and Massey (1956, pp. 63–65)). The WKBJ approximations of
§33.23(vii) may also be used to estimate the penetrability.
The Coulomb functions given in this chapter are most commonly evaluated for
real values of
,
,
,
and nonnegative integer values
of
, but they may be continued analytically to complex arguments and
order
as indicated in §33.13.
Examples of applications to noninteger and/or complex variables are as follows.
Scattering at complex energies. See for example McDonald and Nuttall (1969).
Searches for resonances as poles of the
-matrix in the complex
half-plane
. See for example Csótó and Hale (1997).
Regge poles at complex values of
. See for example
Takemasa et al. (1979).
Eigenstates using complex-rotated coordinates
,
so that resonances have square-integrable eigenfunctions. See for example
Halley et al. (1993).
Gravitational radiation. See for example Berti and Cardoso (2006).
For further examples see Humblet (1984).