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Dimensionless Parameters Table

Dimensionless parameters are the knobs that actually control a canonical wave-mechanics problem. Mass, length, field strength, barrier width, and energy may look independent in dimensional form, but the physics usually depends on combinations such as kLkL, κa\kappa a, V0/ELV_0/E_L, x/ℓx/\ell, r/a0r/a_0, or A/(2πℓB2)A/(2\pi\ell_B^2).

This page is a lookup table. The derivation of scaling conventions is Dimensionless Variables and Scaling; the table below records the combinations most often needed when reading, solving, or numerically checking canonical model pages.

For a one-dimensional problem with a geometric length LL, define

EL=ℏ22mL2,ξ=xL,ε=EEL.E_L=\frac{\hbar^2}{2mL^2}, \qquad \xi=\frac{x}{L}, \qquad \varepsilon=\frac{E}{E_L}.

If a potential has characteristic height V0V_0, a standard strength parameter is

λ=V0EL=2mV0L2ℏ2.\lambda=\frac{V_0}{E_L} =\frac{2mV_0L^2}{\hbar^2}.

Different authors may choose LL to be a full width, half-width, oscillator length, Bohr radius, or magnetic length. The exact numerical factors depend on that choice, but the physical question is stable: how large is the potential, phase, action, or flux compared with the natural quantum scale?

System Natural variables Main dimensionless parameters What they control Check in limits
Free particle kxkx, Et/ℏEt/\hbar kLkL, pL/ℏpL/\hbar, Et/ℏEt/\hbar phase accumulation over a length or time kL≪1kL\ll1 means little phase variation over the region; kL≫1kL\gg1 means rapid oscillation
Infinite square well ξ=x/L\xi=x/L, ε=E/EL\varepsilon=E/E_L quantum number nn, eigenvalue εn=n2π2\varepsilon_n=n^2\pi^2 node count and energy scale all dimensional energies scale as 1/L21/L^2
Finite square well x/Lx/L, E/ELE/E_L depth λ=V0/EL\lambda=V_0/E_L, decay length ratio L/ℓtailL/\ell_{\mathrm{tail}} number of bound states and leakage outside the well λ→∞\lambda\to\infty approaches the infinite well; shallow wells lose excited states
Delta potential x/ℓδx/\ell_\delta, with ℓδ=ℏ2/(mα)\ell_\delta=\hbar^2/(m\alpha) for V=−αδ(x)V=-\alpha\delta(x) kℓδk\ell_\delta in scattering bound-state size and scattering strength small kℓδk\ell_\delta gives strong low-energy scattering from the point interaction
Potential step k1xk_1x, k2xk_2x E/V0E/V_0, k2/k1k_2/k_1 impedance mismatch between asymptotic regions V0→0V_0\to0 gives no reflection; current ratios still matter
Rectangular barrier kaka, κa\kappa a, E/V0E/V_0 opacity κa=a2m(V0−E)/ℏ\kappa a=a\sqrt{2m(V_0-E)}/\hbar for E<V0E\lt V_0 tunneling suppression and resonance widths κa≫1\kappa a\gg1 gives exponential suppression; a→0a\to0 at fixed height gives transparency
Transfer-matrix chains region phases kjajk_ja_j interface ratios kj+1/kjk_{j+1}/k_j, total phase, determinant checks interference, resonances, and current conservation for ordinary amplitudes det⁡M=kL/kR\det M=k_L/k_R; flux-normalized amplitudes give unit determinant
Gaussian wave packet (x−x0)/σx(x-x_0)/\sigma_x, t/t0t/t_0 σxσp/ℏ\sigma_x\sigma_p/\hbar, t/t0t/t_0 with t0=2mσx2/ℏt_0=2m\sigma_x^2/\hbar for the common minimum packet convention spreading and near-plane-wave behavior broad packets have small momentum spread; long times require boundary checks
Harmonic oscillator ξ=x/ℓ\xi=x/\ell, τ=ωt\tau=\omega t, ℓ=ℏ/(mω)\ell=\sqrt{\hbar/(m\omega)} ε=E/(ℏω)\varepsilon=E/(\hbar\omega), coherent-state amplitude α\alpha universal oscillator shape, spectrum, and classicality ∣α∣2≫1\lvert\alpha\rvert^2\gg1 gives large action compared with ℏ\hbar
Coupled oscillators normal coordinates Qa/ℓaQ_a/\ell_a frequency ratios ωa/ωb\omega_a/\omega_b, coupling-to-detuning ratios normal-mode splitting and degeneracy integer frequency relations permit degeneracies; weak coupling can strongly mix nearly resonant modes
Two-level system dimensionless time Ωt/ℏ\Omega t/\hbar, for H=ϵσz+ΔσxH=\epsilon\sigma_z+\Delta\sigma_x and Ω=ϵ2+Δ2\Omega=\sqrt{\epsilon^2+\Delta^2} ϵ/Ω\epsilon/\Omega, Δ/Ω\Delta/\Omega, gap time 2Ωt/ℏ2\Omega t/\hbar mixing angle, transition probability, and adiabaticity estimates large detuning suppresses transitions; near degeneracy invalidates nondegenerate perturbation
Three-dimensional box xi/Lix_i/L_i aspect ratios Lx/LyL_x/L_y, Ly/LzL_y/L_z, scaled energy E/ELxE/E_{L_x} degeneracy patterns and density of states taking one length to infinity makes only that direction continuous
Central potentials r/Lr/L, dimensionless reduced radial amplitude L1/2uL^{1/2}u angular parameter ℓ(ℓ+1)\ell(\ell+1), strength 2mL2V0/ℏ22mL^2V_0/\hbar^2 centrifugal barrier and radial localization large ℓ\ell pushes probability away from the origin
Hydrogenic Coulomb problem ρ=Zr/a0\rho=Zr/a_0, E/EHE/E_{\mathrm H} Zr/a0Zr/a_0, principal quantum number nn, Coulomb strength encoded in a0/Za_0/Z orbital size, binding energy, and Rydberg scaling radii grow like n2a0/Zn^2a_0/Z and energies scale as −Z2/n2-Z^2/n^2
Rigid rotor angles on S2S^2 E/BrotE/B_{\mathrm{rot}}, JJ, with Brot=ℏ2/(2I)B_{\mathrm{rot}}=\hbar^2/(2I) rotational ladder and degeneracy J≫1J\gg1 approaches classical angular momentum magnitude
Minimal coupling kinetic momentum scale, gauge phase flux phase qΦB/ℏq\Phi_B/\hbar, length ratio L/ℓBL/\ell_B if BB is uniform gauge-covariant phase and magnetic localization only gauge-invariant quantities should survive physical comparisons
Landau levels x/ℓBx/\ell_B, ωct\omega_ct, ℓB=ℏ/(∣q∣B)\ell_B=\sqrt{\hbar/(\lvert q\rvert B)} A/(2πℓB2)A/(2\pi\ell_B^2), E/(ℏωc)E/(\hbar\omega_c) cyclotron radius scale, level spacing, and degeneracy B→0B\to0 requires tracking both vanishing spacing and vanishing degeneracy density
Semiclassical checks action divided by ℏ\hbar S0/ℏS_0/\hbar, de Broglie wavelength over variation length WKB validity and classical correspondence large action alone is not enough near turning points

Several different-looking parameters express the same comparison:

  • phase parameters such as kLkL compare a wavelength with a length scale;
  • opacity parameters such as κa\kappa a compare an evanescent decay length with a barrier width;
  • strength parameters such as V0/ELV_0/E_L compare potential energy with localization kinetic energy;
  • flux parameters such as A/(2πℓB2)A/(2\pi\ell_B^2) compare area with the flux quantum scale;
  • action parameters such as S0/ℏS_0/\hbar compare classical action with the quantum of action;
  • detuning parameters such as δ/Ω\delta/\Omega compare an energy mismatch with a coupling.

The notation can vary. What matters is that each parameter is dimensionless and tied to a physical question.

For a finite square well, some authors use the full width LL while others use the half-width a=L/2a=L/2. A depth parameter written with LL differs by a factor of four from one written with aa. Both are acceptable if the convention is stated.

For the harmonic oscillator, some derivations write the stationary equation with energy E/(ℏω)E/(\hbar\omega), while others multiply through by 22 and use 2E/(ℏω)2E/(\hbar\omega). The physics is unchanged; the oscillator length ℓ=ℏ/(mω)\ell=\sqrt{\hbar/(m\omega)} is the key scale.

In the hydrogen row, a0=4πϵ0ℏ2/(μe2)a_0=4\pi\epsilon_0\hbar^2/(\mu e^2) includes the chosen reduced mass μ\mu, so the ionic length is a0/Za_0/Z. Check whether a source instead defines a0a_0 using the electron mass. Do not compare radial plots or expectation values until the convention is clear.

For Landau levels, the magnetic length sets the wavefunction scale, while the flux count sets degeneracy. A calculation can get ℏωc\hbar\omega_c right and still get the state count wrong if it ignores boundary conditions.

  • Calling a quantity dimensionless because it has been written in natural units without naming the scale.
  • Mixing full-width and half-width conventions in square-well formulas.
  • Treating κa\kappa a and kaka as interchangeable.
  • Reporting a numerical grid spacing without comparing it to the smallest physical length scale.
  • Comparing two oscillator plots without checking whether xx is measured in ℓ\ell.
  • Forgetting that A/(2πℓB2)A/(2\pi\ell_B^2) is a degeneracy estimate, not a single-particle energy.
  • Hiding the control parameter by setting too many constants to one at the start.
  1. A finite square well is written with full width LL and depth V0V_0. Define a natural kinetic energy and a dimensionless depth.
Solution

A convenient kinetic scale is

EL=ℏ22mL2.E_L=\frac{\hbar^2}{2mL^2}.

The dimensionless depth is

λ=V0EL=2mV0L2ℏ2.\lambda=\frac{V_0}{E_L} =\frac{2mV_0L^2}{\hbar^2}.

If a half-width a=L/2a=L/2 is used instead, the numerical value of the strength parameter changes by a factor of four, so the convention must be stated.

  1. For a rectangular barrier with E<V0E\lt V_0, explain the meaning of κa\kappa a.
Solution

Inside the barrier, the evanescent decay constant is

κ=2m(V0−E)ℏ.\kappa=\frac{\sqrt{2m(V_0-E)}}{\hbar}.

Thus κa\kappa a is the barrier width measured in decay lengths. When κa≫1\kappa a\gg1, transmission is exponentially suppressed; when κa≪1\kappa a\ll1, the barrier is thin on the evanescent scale.

  1. A Landau-level calculation reports the correct spacing ℏωc\hbar\omega_c but no degeneracy estimate. Which dimensionless parameter is missing?
Solution

The missing parameter is the number of flux-scale area units,

Nϕ≃A2πℓB2.N_\phi \simeq \frac{A}{2\pi\ell_B^2}.

It controls the ideal bulk degeneracy of each Landau level in area AA. The energy spacing alone does not determine the number of available states.

  • 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.
  • N. J. Higham, Accuracy and Stability of Numerical Algorithms, 2nd ed., SIAM, 2002.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.