Skip to content

Canonical Systems Formulas

Canonical systems are reusable test problems: their spectra and states anchor perturbation theory, semiclassical limits, numerical benchmarks, and local approximations to more complicated Hamiltonians. These cards make their most used formulas available without detaching them from boundary conditions, normalization conventions, degeneracies, or energy-zero choices.

Each card is a lookup layer. Follow its canonical link for the derivation and full physical interpretation.

TaskCard
Quantize a particle between hard wallsParticle-in-a-Box Spectrum
Solve a finite attractive square well by parityFinite Square-Well Equations
Look up oscillator energies, eigenfunctions, or momentsHarmonic Oscillator Spectrum
Evaluate oscillator matrix elements with creation and annihilation operatorsHarmonic Oscillator Ladder Operators
Expand, overlap, displace, or evolve a coherent stateCoherent-State Expansion
Compute Coulomb bound energies, transitions, or degeneracyHydrogen Spectrum
Look up normalized Coulomb radial functions, nodes, or radial momentsHydrogen Radial Wavefunctions
Convert molecular inertia into ideal rotational levels or linesRigid-Rotor Spectrum
Compute magnetic scales, orbital levels, or flux degeneracyLandau Levels
SystemCore Hamiltonian or conditionDiscrete labelSpectrum or level equation
Infinite square wellψ(0)=ψ(L)=0\psi(0)=\psi(L)=0n=1,2,…n=1,2,\ldotsEn=π2ℏ2n2/(2mL2)E_n=\pi^2\hbar^2n^2/(2mL^2)
Symmetric finite wellV=−V0V=-V_0 for ∣x∣<a\lvert x\rvert<aparity and bound-state rootztan⁡z=z02−z2z\tan z=\sqrt{z_0^2-z^2} or −zcot⁡z=z02−z2-z\cot z=\sqrt{z_0^2-z^2}
Harmonic oscillatorP2/(2m)+mω2X2/2P^2/(2m)+m\omega^2X^2/2n=0,1,2,…n=0,1,2,\ldotsEn=ℏω(n+1/2)E_n=\hbar\omega(n+1/2)
Hydrogenic Coulomb problemp2/(2μ)−Ze2/(4πϵ0r)p^2/(2\mu)-Ze^2/(4\pi\epsilon_0r)n,ℓ,mn,\ell,mEn=−μc2(Zα)2/(2n2)E_n=-\mu c^2(Z\alpha)^2/(2n^2)
Linear rigid rotorL2/(2I)L^2/(2I)J,MJ,MEJ=ℏ2J(J+1)/(2I)E_J=\hbar^2J(J+1)/(2I)
Spinless Landau problem(p−qA)2/(2m)(\mathbf p-q\mathbf A)^2/(2m)nn plus guiding centerEn=ℏωc(n+1/2)E_n=\hbar\omega_c(n+1/2)

The labels in the third column do not all play the same role. The box label nn identifies a nondegenerate one-dimensional level. Hydrogenic ℓ,m\ell,m labels resolve a Coulomb degeneracy. The Landau guiding-center label changes the orbital state while leaving the cyclotron energy fixed.

The Particle-in-a-Box Spectrum uses impenetrable Dirichlet walls. It includes normalized eigenfunctions, matrix elements, parity in a centered interval, multidimensional products, and revival scales. Its familiar n2n^2 spectrum does not survive unchanged when a wall becomes finite.

The Finite Square-Well Equations use a symmetric attractive well of width 2a2a, with exterior potential chosen as zero. Bound energies are roots of parity-resolved transcendental equations, not a closed polynomial spectrum. Check the width and energy-zero conventions before importing equations from a source that uses a well from 00 to LL or sets the interior potential to zero.

The Hydrogen Spectrum collects reduced-mass scales, Z2/n2Z^2/n^2 energies, transition wavenumbers, degeneracy, virial identities, and the limits of the ideal Coulomb model.

The Hydrogen Radial Wavefunctions separate three objects that are often conflated:

Rnℓ(r),unℓ(r)=rRnℓ(r),Pnℓ(r)=r2∣Rnℓ(r)∣2.R_{n\ell}(r), \qquad u_{n\ell}(r)=rR_{n\ell}(r), \qquad P_{n\ell}(r)=r^2\lvert R_{n\ell}(r)\rvert^2.

Use the spectrum card for energy and transition calculations; use the radial card for normalization, shell probabilities, nodes, moments, and radial matrix elements.

Three cards form one connected toolkit:

  1. Harmonic Oscillator Spectrum gives the exact levels, coordinate-space states, natural scales, moments, and multidimensional extensions.
  2. Harmonic Oscillator Ladder Operators gives operator definitions, repeated actions, matrix elements, commutators, and Heisenberg evolution.
  3. Coherent-State Expansion gives the number expansion, Poisson statistics, displacement identities, overlaps, resolution of identity, quadrature moments, and exact ideal evolution.

Keep the oscillator length convention visible. This compendium uses

ℓ=ℏmω,\ell = \sqrt{\frac{\hbar}{m\omega}},

so the ground-state Gaussian is proportional to e−x2/(2ℓ2)e^{-x^2/(2\ell^2)}. Some sources call ℓ/2\ell/\sqrt2 the oscillator length, which shifts factors of 2\sqrt2 in ladder and variance formulas without changing the physics.

The Rigid-Rotor Spectrum uses scalar wavefunctions on S2S^2 and integer JJ. It distinguishes the rotational constant in energy, frequency, and wavenumber units, and it explains why ideal adjacent dipole lines are equally spaced even though the energy levels are not.

The Landau Levels card separates cyclotron excitation from guiding-center degeneracy. It gives both Landau-gauge wavefunctions and gauge-independent algebra, bulk flux counting, the three-dimensional dispersion, and a signed-charge Zeeman extension.

These two systems both organize states into degenerate multiplets, but for different reasons:

  • rotor MM degeneracy follows ordinary rotational invariance;
  • Landau guiding-center degeneracy follows magnetic translation structure and flux density.
SystemEnergy scaleLength or inertia scaleMain scaling
Infinite wellℏ2/(2mL2)\hbar^2/(2mL^2)LLEn∝n2/(mL2)E_n\propto n^2/(mL^2)
Finite wellℏ2/(2ma2)\hbar^2/(2ma^2) and V0V_0aaroots depend on z0=a2mV0/ℏz_0=a\sqrt{2mV_0}/\hbar
Oscillatorℏω\hbar\omegaℓ=ℏ/(mω)\ell=\sqrt{\hbar/(m\omega)}equally spaced levels
Hydrogenic ionμc2(Zα)2/2\mu c^2(Z\alpha)^2/2aZ=ℏ/(μcZα)a_Z=\hbar/(\mu cZ\alpha)E∝μZ2E\propto\mu Z^2, r∝1/(μZ)r\propto1/(\mu Z)
Linear rotorℏ2/(2I)\hbar^2/(2I)I=μRe2I=\mu R_e^2E∝1/(μRe2)E\propto1/(\mu R_e^2)
Landau levelℏ∣q∣B/m\hbar\lvert q\rvert B/mℓB=ℏ/(∣q∣B)\ell_B=\sqrt{\hbar/(\lvert q\rvert B)}gap ∝B\propto B, area per state ∝1/B\propto1/B

Dimensionless control parameters make comparisons safer. Examples are the finite-well strength z0z_0, the hydrogenic coupling ZαZ\alpha, and ratios such as a perturbation energy to ℏω\hbar\omega or BEB_E.

Before applying a canonical-system formula, identify:

  1. Configuration space: line, interval, half-line, sphere, plane, or three- dimensional space.
  2. Boundary conditions: hard wall, decaying tail, periodic identification, regular radial endpoint, or magnetic boundary condition.
  3. Energy zero: finite-well depths and ionization energies depend on it.
  4. Mass parameter: particle mass, reduced mass, effective mass, or moment of inertia.
  5. Charge convention: qq is signed, while ωc\omega_c and ℓB\ell_B use ∣q∣\lvert q\rvert.
  6. Normalization measure: dxdx, r2drr^2dr, dΩd\Omega, box normalization, or continuum delta normalization.
  7. Degeneracy count: orbital only, spin resolved, or including additional symmetry and exchange weights.
  8. Approximation boundary: infinite wall, rigid bond, point nucleus, quadratic potential, or uniform field.

Several formulas recur because one canonical system reduces locally or algebraically to another:

  • a smooth potential near a stable minimum becomes a harmonic oscillator to quadratic order;
  • Landau cyclotron motion is an oscillator built from noncommuting kinetic momenta;
  • the rigid rotor is the angular part of a fixed-radius particle on a sphere;
  • hydrogenic states combine a Coulomb radial equation with spherical-harmonic angular states;
  • the deep finite well approaches hard-wall behavior for low-lying states, but retains exponentially decaying tails at every finite depth.

These connections justify reusing methods. They do not erase differences in domain, measure, degeneracy, or boundary conditions.

  • A familiar spectrum is not portable without its Hamiltonian and domain.
  • Degeneracy is part of a level specification, not an optional annotation.
  • Gauge-dependent labels may organize states without being observables.
  • A normalized radial factor need not be normalized with ordinary drdr.
  • Spectroscopic constants must carry units until the final conversion.
  • Reduced and effective masses must be stated rather than silently replaced by a bare mass.
  • The ideal model should be named before any correction is appended.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
  • C. Cohen-Tannoudji, B. Diu, and F. Laloe, Quantum Mechanics, Wiley, 1977.
  • L. D. Landau and E. M. Lifshitz, Quantum Mechanics: Non-Relativistic Theory, 3rd ed., Pergamon, 1977.
  • R. N. Zare, Angular Momentum: Understanding Spatial Aspects in Chemistry and Physics, Wiley, 1988.