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Limiting cases are physical error checks. A formula for a canonical system should reduce to a simpler model when a wall becomes infinite, a barrier disappears, a packet becomes broad, a magnetic field turns off, or a quantum number becomes large. If it does not, either the calculation has a mistake or the limit has been taken while holding the wrong quantity fixed.

This table is a diagnostic layer. The canonical derivations live on the linked model pages; the entries here state what behavior should be recovered and what subtlety usually causes wrong answers.

Before trusting a result, identify the dimensionless control parameter and ask what happens in the small, large, or degenerate limit. The most useful checks are often qualitative:

  • a finite wall should not become a hard wall until the penetration length becomes negligible;
  • a tunneling barrier should become transparent when its width or height disappears;
  • a discrete spectrum should become dense when the confining length goes to infinity;
  • a quantum probability distribution should approach a classical time-spent distribution only after suitable averaging;
  • a singular limit, such as a delta potential, depends on which product of parameters is held fixed.

The last point is important. The limit a→0a\to0 of a rectangular barrier is not unique: if the height stays fixed the barrier disappears, while if V0aV_0a stays fixed it becomes a delta interaction.

Model or result Limit Expected behavior Good diagnostic Common trap
Infinite square well from a finite well well depth V0→∞V_0\to\infty at fixed width LL exterior penetration length goes to zero and energies measured from the well bottom approach n2π2ℏ2/(2mL2)n^2\pi^2\hbar^2/(2mL^2); if the interior potential is −V0-V_0, this means En+V0E_n+V_0 compare the lowest finite-well energies with the hard-wall spectrum imposing hard-wall boundary conditions before the depth is actually infinite
Shallow finite well V0→0+V_0\to0^+ for an attractive one-dimensional well only the lowest bound state survives; excited states disappear through threshold track bound-state count as depth increases expecting every infinite-well level to have a shallow-well descendant
Delta potential from a narrow well width a→0a\to0, depth V0→∞V_0\to\infty, area V0aV_0a fixed the wavefunction remains continuous but its derivative has a finite jump recover the matching rule for V(x)=λδ(x)V(x)=\lambda\delta(x) with λ=−V0a\lambda=-V_0a letting both width and area vanish, which gives the free particle instead
Potential step V0→0V_0\to0 or E≫V0E\gg V_0 reflection tends to zero and transmission tends to one check probability current, not just amplitude using ∣A∣2\lvert A\rvert^2 ratios when incoming and transmitted wave numbers differ
Rectangular barrier, transparent limit barrier width a→0a\to0 at fixed height, or height V0→0V_0\to0 T→1T\to1 and R→0R\to0 global plane-wave coefficients give the identity; endpoint-referenced coefficients retain free-propagation phases at fixed width confusing this with the fixed-area delta-barrier limit
Rectangular barrier, opaque limit κa≫1\kappa a\gg1 for E<V0E\lt V_0 transmission is exponentially small, with leading scale T∝e−2κaT\propto e^{-2\kappa a} plot log⁡T\log T against aa treating an evanescent wave as an ordinary probability density moving through the barrier
Resonant barrier or well propagating interior phase equals an integer multiple of π\pi, with equal exterior potentials transmission can approach one even with nonzero interfaces look for zeros of the reflection amplitude assuming every barrier suppresses transmission monotonically
Free particle from a box L→∞L\to\infty level spacing tends to zero and sums over nn become integrals over kk verify the density of states before replacing sums by integrals keeping box-normalized amplitudes while using continuum normalization
Gaussian wave packet initial width σx→∞\sigma_x\to\infty at fixed mean momentum momentum probability density tends weakly to a delta function; the unit-normalized position amplitude tends to zero locally check σxσp=ℏ/2\sigma_x\sigma_p=\hbar/2 for the minimum packet identifying a unit-normalized amplitude with a nonzero plane wave; matching shapes requires amplitude rescaling
Harmonic oscillator, large quantum number n≫1n\gg1 turning points approach An≃2En/(mω2)A_n\simeq \sqrt{2E_n/(m\omega^2)} and the coarse-grained density approaches the classical time-spent distribution compare support near the classical turning points expecting pointwise convergence of the oscillatory wavefunction
Harmonic oscillator, weak confinement ω→0\omega\to0 spacing ℏω\hbar\omega goes to zero and oscillator length ℓ=ℏ/(mω)\ell=\sqrt{\hbar/(m\omega)} diverges state which energy, coordinate scale, or quantum number is held fixed calling the limit a free particle without tracking the widening states
Coherent state large amplitude ∣α∣≫1\lvert\alpha\rvert\gg1 center follows the classical oscillator orbit while the packet shape stays Gaussian compare ⟨x(t)⟩\langle x(t)\rangle and ⟨p(t)⟩\langle p(t)\rangle with the classical solution mistaking small relative uncertainty for zero absolute uncertainty
Two-level avoided crossing coupling Δ→0\Delta\to0 eigenvalues cross and eigenvectors become diabatic basis states away from degeneracy diagonalize a0I+b⋅σa_0I+\mathbf b\cdot\boldsymbol\sigma as Δ\Delta changes using nondegenerate perturbation theory at the crossing
Rabi oscillations detuning ∣δ∣≫Ω\lvert\delta\rvert\gg\Omega transition amplitude is suppressed by the small mixing angle check the maximum transition probability, not only the oscillation frequency assuming large detuning merely changes the period
Three-dimensional box one side length Lz→∞L_z\to\infty the zz spectrum becomes continuous while transverse levels remain discrete replace ∑nz\sum_{n_z} by an integral only in that direction treating the whole spectrum as continuous too early
Central radial problem angular momentum ℓ≫1\ell\gg1 centrifugal barrier pushes probability away from the origin inspect the effective potential Veff(r)V_{\mathrm{eff}}(r) forgetting the radial measure and judging only R(r)R(r)
Hydrogen atom, Rydberg limit n≫1n\gg1 at fixed ZZ radius scale grows like n2a0/Zn^2a_0/Z and binding energy approaches zero as −1/n2-1/n^2 check both the energy and radial scale treating large-nn states as small corrections to the ground state
Hydrogen atom, continuum threshold n→∞n\to\infty bound levels accumulate at E=0−E=0^-; scattering states form the distinct continuum at E>0E>0 verify the sign convention for the zero of energy expecting equally spaced levels near ionization
Rigid rotor J≫1J\gg1 energy grows as J2J^2 and angular momentum becomes approximately classical in magnitude compare EJ=ℏ2J(J+1)/(2I)E_J=\hbar^2J(J+1)/(2I) with L2/(2I)L^2/(2I) replacing J(J+1)J(J+1) by J2J^2 at small JJ
Landau levels B→0B\to0 cyclotron spacing ℏωc\hbar\omega_c and degeneracy density 1/(2πℓB2)1/(2\pi\ell_B^2) go to zero; the free-particle continuum is recovered after summing many levels track both spacing and degeneracy looking at one fixed Landau level and expecting the full free continuum
Strong magnetic field increase BB while ℏωc≪mc2\hbar\omega_c\ll mc^2 magnetic length ℓB=ℏ/(∣q∣B)\ell_B=\sqrt{\hbar/(\lvert q\rvert B)} shrinks and Landau-level spacing grows compare the physical length scale with ℓB\ell_B extrapolating the nonrelativistic model to arbitrarily large fields

Several canonical limits do not commute. A long-time wave-packet limit taken before a large-box limit can show boundary recurrence, while the same packet on the line disperses indefinitely. A narrow-barrier limit at fixed area gives a delta interaction, while a narrow-barrier limit at fixed height gives no interaction. A classical limit of the oscillator can mean n→∞n\to\infty at fixed ℏω\hbar\omega, ℏ→0\hbar\to0 at fixed classical energy, or a coherent state with large action compared with ℏ\hbar.

When writing a derivation or notebook, state the limiting variables explicitly. Good phrases are “at fixed width,” “at fixed area,” “after coarse graining,” “with energy measured relative to the continuum threshold,” and “with the box-normalized density of states included.”

Use these checks when debugging formulas:

  • Does the answer have the correct dimension after the limiting parameter is removed?
  • Does a reflection coefficient vanish when the interface disappears?
  • For a short-range potential, does the bound-state tail shorten as the energy moves farther below the continuum threshold?
  • Does a continuum result include a density-of-states factor after a box limit?
  • Does a large-quantum-number result require averaging before comparison with classical mechanics?
  • Does a gauge-dependent wavefunction claim reduce to a gauge-invariant observable in a physical limit?

For numerical work, pair each limit with convergence data. A finite-difference square well should approach the analytic hard-wall spectrum as both the grid spacing and the finite-wall penetration error are reduced. A tunneling notebook should show norm conservation separately from asymptotic reflection and transmission accounting.

  • Taking a limit without saying what is held fixed.
  • Using the right limiting formula with the wrong normalization convention.
  • Assuming a finite barrier becomes an infinite wall merely because E<V0E\lt V_0.
  • Forgetting that classical correspondence can require coarse graining.
  • Comparing one member of a degenerating spectrum with an entire continuum.
  • Treating a singular limit as if it were a smooth perturbation.
  • Calling a numerical trend a limit without checking more than one parameter value.
  1. A rectangular barrier has height V0V_0 and width aa. Explain why the limits a→0a\to0 at fixed V0V_0 and a→0a\to0, V0→∞V_0\to\infty at fixed V0aV_0a give different physics.
Solution

At fixed height, the area of the barrier goes to zero, so the transfer matrix approaches the free-particle transfer matrix and the barrier becomes transparent. At fixed area, the barrier becomes singular rather than disappearing. The limiting interaction is a delta potential, which leaves the wavefunction continuous but produces a finite derivative jump.

  1. Why is the statement “the large-nn harmonic oscillator becomes the classical oscillator” incomplete?
Solution

The wavefunction remains oscillatory and does not converge pointwise to a classical trajectory. The useful statement is that the probability density, after suitable coarse graining, approaches the classical time-spent distribution between the turning points, while wave packets such as coherent states can have expectation values that follow classical motion.

  1. In the limit B→0B\to0, why is it misleading to follow only the lowest Landau level?
Solution

The Landau-level spacing goes to zero, but so does the degeneracy density of each level. The free-particle continuum is recovered by considering the combined contribution of many levels, not by tracking one fixed level in isolation.

  • C. Cohen-Tannoudji, B. Diu, and F. Laloë, Quantum Mechanics, Wiley, 1977.
  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
  • L. D. Landau and E. M. Lifshitz, Quantum Mechanics: Non-Relativistic Theory, 3rd ed., Pergamon, 1977.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.