perturbation-theory

Layer 1 — Physics24 concepts in this subtree

Systematic series-expansion methods for eigenvalues and eigenstates of Hamiltonians of the form H = H_0 + λV, where H_0 has a known spectrum and λ is a small formal parameter. Rayleigh 1894 secular-equation origin, Schrödinger 1926 formal…

Rayleigh-Schrödinger time-independent perturbation theory
Dyson 1949 time-ordered interaction-picture propagator series
Brillouin-Wigner self-consistent perturbation expansion
RS 1st-order energy shift for λx² perturbation of harmonic oscillator
RS 2nd-order energies for 2-level system with off-diagonal perturbation
1st-order ground-state shift for λx⁴ perturbation of harmonic oscillator
Pade-Borel resummation: convert divergent perturbative series into convergent rational approximants
WKB semiclassical expansion: psi(x) ~ A(x)*exp(i*S(x)/hbar) with S expanded in powers of hbar
Van Vleck / Lowdin quasi-degenerate perturbation: block-diagonalise H via Schur-lemma decomposition
Theorem: Pade[1/1](e^x) = (2+x)/(2-x) agrees with Taylor series through O(x^2)
Theorem: Bohr-Sommerfeld quantization gives exact E_n = hbar*omega*(n + 1/2) for harmonic oscillator
Theorem: 2x2 Van Vleck block has trace E1+E2, det E1*E2 - V^2, second-order shift V^2/(E1-E2)
Rayleigh-Schrodinger PT (1926)
Regularization (t Hooft 1972)
RG (Wilson 1971)
Borel summation (1899)
Instanton tunneling
Convergence radius
Rayleigh-Schrödinger (1926)
Brillouin-Wigner (1933)
Time-dependent (Dirac 1927)
Borel summability (Bender-Wu 1969)
WKB (Wentzel-Kramers-Brillouin-Jeffreys 1923-1926)
Instanton (Feynman 1965)
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