Abstract
Perturbation theory (PT) represents one of the bridges that takes us from a simpler, exactly solvable (unperturbed) problem to a corresponding real (perturbed) problem by expressing its solutions as a series expansion in a suitably chosen “small” parameter ε in such a way that the problem reduces to the unperturbed problem when ε = 0. It originated in classical mechanics and eventually developed into an important branch of applied mathematics enabling physicists and engineers to obtain approximate solutions of various systems of differential equations [5.1,2,3,4]. For the problems of atomic and molecular structure and dynamics, the perturbed problem is usually given by the time-independent or time-dependent Schrödinger equation [5.5,6,7,8].
Abbreviations
- BW:
-
Brillouin-Wigner
- CC:
-
coupled cluster
- CCD:
-
coupled cluster doubles
- DODS:
-
different orbitals for different spins
- EOM:
-
equation of motion
- HF:
-
Hartree-Fock equations
- MBPT:
-
many-body perturbation theory
- MR:
-
multireference
- PT:
-
perturbation theory
- RSPT:
-
Rayleigh-Schrödinger perturbation theory
- UHF:
-
unrestricted Hartree-Fock
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Paldus, J. (2006). Perturbation Theory. In: Drake, G. (eds) Springer Handbook of Atomic, Molecular, and Optical Physics. Springer Handbooks. Springer, New York, NY. https://doi.org/10.1007/978-0-387-26308-3_5
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