III
Schrodinger and Klein-Gordon Equations for
One-Electron Atoms in a Magnetic Field
Introduction
Summary.
The most interesting problems in the theory of linear and
homogeneous partial differential equations are the eigenvalue problems.
Their essential feature is that they have solutions only exceptionally.
Examples of lagrangian problems having the same feature are given in
this chapter. These problems assume
1 = 3, Z(3) = X Q+ X*,
X = X* = E3 (euclidean space).
They concern the lagrangian operator a associated to some convenient
hamiltonian: this hamiltonian gives rise to a Hamilton system admitting
two first integrals defined on Z(3), namely, the length L and") one of the
components M of the vector x A p in V.
H may be the hamiltonian(2) of the nonrelativistic or relativistic electron
under the simultaneous influence of the electric field of a stationary atomic
nucleus and a constant magnetic field (Zeeman effect). Then H depends
on a parameter: the energy level E of the electron. The operator a is the
Schrodinger or (in the relativistic case) the Klein-Gordon operator. The
energy levels for which our lagrangian problems have a solution coincide
with those defined by the problems that are classically studied regarding
these operators.
The advantage of the lagrangian point of view is its simplicity. By applying
theorem 7.1 of II, §3, these energy levels are obtained in §1 by a quadrature.
The latter is easily calculated in the Schrodinger and Klein-Gordon cases
using the method of residues.
In §1, we determine solutions defined mod(1/v) on a compact lagrangian
manifold of the lagrangian system:
a U = (aL2 - const.) U = (aM - const.) U = 0 mod
1
1,
(1)
V11
where aL= and am are the lagrangian operators associated to the first
integrals L2 and M. Here theorem 7.1 is applied. Three integers introduced
by the Maslov quantization,
1, m, n such that I m < I < n,
'The author uses A - to denote the vector product in V. [Translator's note]
'Or the hamiltonian of the harmonic operator: see §3, remark 4.3.