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USSR Computational Mathematics and Mathematical Physics

Asymptotic expansions in wave mechanics

В. А. Дубровский, G. A. Skuridin

Published Jan 1, 1964• 4 citations
Publisher
DOI
10.1016/0041-5553(64)90142-9

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Exactly solvable quantum systems are rare—the harmonic oscillator, the hydrogen atom, the square well—and the physics of everything else is the physics of approximation. This article presents a narrative review of the primary literature that built quantum mechanics' approximation methods, from Rayleigh's Theory of Sound, whose treatment of slightly perturbed vibrating systems gave perturbation theory its name and scheme, and Ritz's 1909 variational method, which converted boundary-value problems into energy minimizations, through Schrödinger's 1926 wave mechanics, which equipped the new quantum theory with perturbation theory from the start, Born and Oppenheimer's 1927 adiabatic separation of electronic and nuclear motion, the 1926 papers of Wentzel, Kramers, and Brillouin that independently derived the semiclassical expansion bearing their initials, Hartree's 1928 self-consistent field and Hylleraas's 1929 variational computation of helium, which made the many-electron atom calculable, Kato's 1949 mathematical foundation of the perturbation method's convergence, Landau and Lifshitz's codifying textbook, and Bender and Wu's 1969 demonstration that the anharmonic oscillator's perturbation series diverges—the asymptotic character that defines the method's limits. The synthesis is organized around three themes: the perturbation program, in which small parameters turned the solvable cases into engines for the unsolvable; the variational program, in which upper bounds and trial functions turned minimization into the many-body atom's working instrument; and the semiclassical bridge, in which the WKB expansion connected wave mechanics to action-angle quantization and exposed tunneling. It is concluded that the three programs are complementary solutions to one problem—the gap between what can be solved and what must be calculated—and that their asymptotic character, made precise by Bender and Wu, is not a defect but the field's realistic self-understanding.

•Aug 29, 2026•0 citations
Since Kato proved his singularity condition for Coulomb potentials in 1957, there has been interest in the creation of wave functions that meet the prescriptions of the cusp conditions, necessary for high-precision quantum-mechanical calculations. It is well known, that wave-function expansions based on Slater determinants of one-electron functions are poorly convergent with respect to satisfying the electron-electron cusp condition. In this contribution we show that with the wavelet expansion of density operators even the local form of the electron-electron cusp condition is easily representable by Slater determinants of one-electron wavelet functions with a proper asymptotics of the expansion coefficients, which is explicitly calculated for Haar wavelets.
Exactly solvable quantum systems are rare—the harmonic oscillator, the hydrogen atom, the square well—and the physics of everything else is the physics of approximation. This article presents a narrative review of the primary literature that built quantum mechanics' approximation methods, from Rayleigh's Theory of Sound, whose treatment of slightly perturbed vibrating systems gave perturbation theory its name and scheme, and Ritz's 1909 variational method, which converted boundary-value problems into energy minimizations, through Schrödinger's 1926 wave mechanics, which equipped the new quantum theory with perturbation theory from the start, Born and Oppenheimer's 1927 adiabatic separation of electronic and nuclear motion, the 1926 papers of Wentzel, Kramers, and Brillouin that independently derived the semiclassical expansion bearing their initials, Hartree's 1928 self-consistent field and Hylleraas's 1929 variational computation of helium, which made the many-electron atom calculable, Kato's 1949 mathematical foundation of the perturbation method's convergence, Landau and Lifshitz's codifying textbook, and Bender and Wu's 1969 demonstration that the anharmonic oscillator's perturbation series diverges—the asymptotic character that defines the method's limits. The synthesis is organized around three themes: the perturbation program, in which small parameters turned the solvable cases into engines for the unsolvable; the variational program, in which upper bounds and trial functions turned minimization into the many-body atom's working instrument; and the semiclassical bridge, in which the WKB expansion connected wave mechanics to action-angle quantization and exposed tunneling. It is concluded that the three programs are complementary solutions to one problem—the gap between what can be solved and what must be calculated—and that their asymptotic character, made precise by Bender and Wu, is not a defect but the field's realistic self-understanding.