For example, consider the time-independent Schrödinger equation
for the function ψ ( x ) {\displaystyle \psi (\mathbf {x} )} (in dimensionless units, for simplicity). (Equivalently, consider the inhomogeneous Helmholtz equation.) If the function V ( x ) {\displaystyle V(\mathbf {x} )} in three dimensions is of the form
then it turns out that the problem can be separated into three one-dimensional ODEs for functions ψ 1 ( x 1 ) {\displaystyle \psi _{1}(x_{1})} , ψ 2 ( x 2 ) {\displaystyle \psi _{2}(x_{2})} , and ψ 3 ( x 3 ) {\displaystyle \psi _{3}(x_{3})} , and the final solution can be written as ψ ( x ) = ψ 1 ( x 1 ) ⋅ ψ 2 ( x 2 ) ⋅ ψ 3 ( x 3 ) {\displaystyle \psi (\mathbf {x} )=\psi _{1}(x_{1})\cdot \psi _{2}(x_{2})\cdot \psi _{3}(x_{3})} . (More generally, the separable cases of the Schrödinger equation were enumerated by Eisenhart in 1948.1)
Eisenhart, L. P. (1948-07-01). "Enumeration of Potentials for Which One-Particle Schroedinger Equations Are Separable". Physical Review. 74 (1). American Physical Society (APS): 87–89. Bibcode:1948PhRv...74...87E. doi:10.1103/physrev.74.87. ISSN 0031-899X. /wiki/Bibcode_(identifier) ↩