Particle in a Spherical Well and Infinite Spherical Box

The chapter's function-building is over; this article spends the toolkit. Two confining problems — the infinite spherical box (hard wall at radius RR) and the finite spherical well (depth V0V_0, range RR) — are solved end to end with the machinery of the last three serials: interior solutions from the regular family jℓj_\ell, exteriors from the evanescent Hankel tails, spectra from matching. The infinite box is the three-dimensional heir of the chapter-one particle-in-a-box, and its answer is pleasingly literal: energies are set by the zeros of the spherical Bessel functions, Enℓ=ℏ2βnℓ2/2mR2E_{n\ell}=\hbar^2\beta_{n\ell}^2/2mR^2, so the level diagram is a table of root-found numbers (π\pi, 4.4934.493, 5.7645.764, 2π2\pi, …\dots) — producing the ordering 1s,1p,1d,2s,1f,2p1s,1p,1d,2s,1f,2p and, doubled for spin, the filling ladder 2,8,18,20,34,402,8,18,20,34,40 that nuclear physics reads magic numbers from. The finite well replaces the wall by a cliff: inside, still jℓj_\ell; outside, the decaying hℓ(1)(iκr)h_\ell^{(1)}(i\kappa r) handed over by the previous article; equality of logarithmic derivatives at RR quantizes the spectrum through a transcendental equation. For s-waves that equation is kcot⁡kR=−κk\cot kR=-\kappa — exactly the odd-parity half of the 1D finite well, as the wall-at-the-origin doctrine promised it would be. Two verdicts carry the physics. First, the existence threshold: unlike one dimension, where any attraction binds, a 3D well binds nothing until V0R2>π2ℏ2/8mV_0R^2>\pi^2\hbar^2/8m — shallow-or-narrow wells are barren (numerically confirmed on both sides of the threshold). Second, the article's centerpiece: the deuteron worked end to end. Feeding the measured binding energy 2.22462.2246 MeV into the matching at R=2.1R=2.1 fm returns V0≈34V_0\approx34 MeV — a well fifteen times deeper than its own bound state, only 1.45×1.45\times the threshold, holding exactly one state with 63%63\% of its probability outside the well. The nuclear force barely succeeds, and everything low-energy about nuclear physics inherits that near-failure.

Key takeaways
  • Infinite spherical box: Rnℓ=jℓ(kr)R_{n\ell}=j_\ell(kr) with jℓ(kR)=0j_\ell(kR)=0 ⇒ Enℓ=ℏ2βnℓ22mR2E_{n\ell}=\dfrac{\hbar^2\beta_{n\ell}^2}{2mR^2}; β\beta = the root-found zeros 3.142,4.493,5.764,6.283,6.988,7.7253.142,4.493,5.764,6.283,6.988,7.725 ⇒ ordering 1s,1p,1d,2s,1f,2p1s,1p,1d,2s,1f,2p.
  • With spin, the box fills 2,8,18,20,34,402,8,18,20,34,40 — magic 2, 8, 20 appear (compare the oscillator's ladder in The Three-Dimensional Isotropic Harmonic Oscillator: same first three, different beyond).
  • Nuclear notation throughout: 2s2s = second s-level, not hydrogen's n=2n=2 (the dictionary card of the oscillator article, reused).
  • Finite well, ℓ=0\ell=0: interior sin⁡kr\sin kr, exterior e−κre^{-\kappa r}; matching ⇒ kcot⁡kR=−κk\cot kR=-\kappa — the odd sector of the 1D finite well of width 2R2R (the origin's hard wall made quantitative).
  • Existence threshold (3D novelty): binding requires V0R2>π2ℏ2/8mV_0R^2>\pi^2\hbar^2/8m — verified numerically: 0 states at 0.97 Vth0.97\,V_{th}, 1 at 1.03 Vth1.03\,V_{th}; higher ℓ pay more (the centrifugal rent).
  • Deuteron solved: EB=2.2246E_B=2.2246 MeV, R=2.1R=2.1 fm, μc2=469.46\mu c^2=469.46 MeV ⇒ V0=33.7V_0=33.7 MeV (root-found), EB/V0=0.066E_B/V_0=0.066, V0/Vth=1.45V_0/V_{th}=1.45, exactly one s-state, exterior probability 0.630.63.
  • Electron in a 1 nm hard sphere: E1s=0.376E_{1s}=0.376 eV, E1p=0.769E_{1p}=0.769 eV, E1d=1.266E_{1d}=1.266 eV (computed) — quantum-dot arithmetic.
  • Key idea: interior jℓj_\ell, exterior evanescent Hankel, match at the edge — the whole spherical bound-state craft in one sentence, with 3D's distinctive lesson that binding must be earned above a threshold.
The core insight

Spherical confinement quantizes through the spherical Bessel machinery: hard walls pin energies to the zeros βnℓ\beta_{n\ell} of jℓj_\ell; finite wells match interior jℓ(kr)j_\ell(kr) to exterior hℓ(1)(iκr)h_\ell^{(1)}(i\kappa r) via logarithmic derivatives, giving transcendental spectra, a binding threshold V0R2>π2ℏ2/8mV_0R^2>\pi^2\hbar^2/8m absent in 1D — and, applied to the deuteron, the depth of the nuclear force from one measured number.

Where this lives today

The threshold theorem runs today's ultracold-atom laboratories in reverse: experimenters tune interatomic wells through the binding threshold with magnetic fields (Feshbach control), watching a bound state be born at zero energy with a divergent tail — the κ→0\kappa\to0 row of this article's limiting table, realized on demand and used to make molecules from free atoms. Halo-nucleus physics at rare-isotope facilities is the deuteron's 63% pushed to extremes: one-neutron halos with PoutP_{out} approaching 90%, identified by exactly the matching analysis performed here. And every colloidal-quantum-dot display on the market is the worked example's 1/R21/R^2 law industrialized — size-sorted nanospheres emitting at zero-ladder-determined colors.

The physical picture

Start with the hard-walled sphere, because its physics is pure geometry: standing ripples of the regular family, cut off where the wall stands. Each channel ℓ\ell has its own waking radius (the turnstile of Spherical Bessel and Neumann Functions), so at fixed box size the s-wave fits its first node earliest (β=π\beta=\pi), the p-wave later (4.4934.493), the d-wave later still (5.7645.764) — and only then does the second s-level arrive (2π2\pi). The interlacing of zeros is the level diagram; nothing else enters.

Figure
The infinite spherical box: levels are zeros of j_ℓ — geometry becomes a spectrum
E ∝ β² — filling ladder of the hard sphere (spin included) 1s · β=3.142 · holds 2 · Σ=2 1p · β=4.493 · holds 6 · Σ=8 1d · β=5.764 · holds 10 · Σ=18 2s · β=6.283 · holds 2 · Σ=20 1f · β=6.988 · holds 14 · Σ=34 2p · β=7.725 · holds 6 · Σ=40 every β root-found, not quoted; ordering = Sturm interlacing of the zero ladder magic 2, 8, 20 appear (as in the oscillator); 18 and 34 do not survive in real nuclei — spin-orbit's business

Now soften the wall to a cliff of depth V0V_0. Two things change, one cosmetic and one structural. Cosmetic: the wavefunction no longer stops at RR but leaks into the classically forbidden exterior with decay constant κ=2m∣E∣/ℏ\kappa=\sqrt{2m|E|}/\hbar — the imaginary-argument Hankel tails delivered by Spherical Hankel Functions and Outgoing Waves. Structural: binding is no longer guaranteed. The 1D finite well binds at any depth (Finite Square Well's theorem); the 3D well does not, because the origin's hard wall — u(0)=0u(0)=0, the doctrine of Boundary Conditions and Normalization of Radial Wavefunctions — forces the wavefunction to bend over within the well's width before it may decay. Bending costs curvature, curvature costs kinetic energy, and a shallow well cannot pay. Three dimensions makes attraction audition for the role of "binder," and the threshold below is the audition's pass mark.

The infinite spherical box

Inside, V=0V=0: the radial solutions are the free ones of The Free Particle in Three Dimensions — regular family only, since the origin is in-domain. The wall imposes Rnℓ(R)=0R_{n\ell}(R)=0:

jℓ(kR)=0  ⇒  knℓ=βnℓR,Enℓ=ℏ2βnℓ22mR2(1)j_\ell(kR)=0\;\Rightarrow\;k_{n\ell}=\frac{\beta_{n\ell}}{R},\qquad E_{n\ell}=\frac{\hbar^2\beta_{n\ell}^2}{2mR^2} \qquad (1)

where: βnℓ\beta_{n\ell} is the nn-th zero of jℓj_\ell — the ladder root-found in Spherical Bessel and Neumann Functions and now cashed as a spectrum (that article's relocated inheritance; this article owns the physics the zeros price). For ℓ=0\ell=0 the zeros are exactly nπn\pi, so En0=ℏ2n2π2/2mR2E_{n0}=\hbar^2n^2\pi^2/2mR^2 — the 1D box spectrum verbatim, because u=sin⁡(kr)u=\sin(kr) is a 1D box wavefunction on the half-line. Each level holds 2(2ℓ+1)2(2\ell+1) particles with spin.

Derivation AThe hard sphere solved, ordered, and filled

We assemble the box spectrum and extract its level ordering and shell capacities — the numbers behind the "poor man's nuclear shell model." Everything reduces to properties of the zero ladder, all root-found rather than quoted.

Step 1. Admissibility inside a domain containing the origin keeps only jℓj_\ell (the free-particle article's verdict, consumed). The wall condition jℓ(kR)=0j_\ell(kR)=0 then quantizes kk channel by channel: no matching, no transcendental subtlety — geometry.

Step 2. Order the levels. Zeros interlace (Sturm grammar, cited to the function article): β10=π<β11=4.493<β12=5.764<β20=2π<β13=6.988<β21=7.725\beta_{10}=\pi<\beta_{11}=4.493<\beta_{12}=5.764<\beta_{20}=2\pi<\beta_{13}=6.988<\beta_{21}=7.725 (each root-found) — hence 1s<1p<1d<2s<1f<2p1s<1p<1d<2s<1f<2p in nuclear notation (nn = ordinal within the channel; the notation dictionary of The Three-Dimensional Isotropic Harmonic Oscillator, reused). Note 1d1d below 2s2s — but barely (5.7645.764 vs 6.2836.283): hard walls push high-ℓ down relative to the oscillator, which put them degenerate (N=2N=2 shell). The two caricatures bracket real nuclear wells.

Step 3. Fill with spin-½ fermions: capacities 2,6,10,2,14,62,6,10,2,14,6, cumulative 2,8,18,20,34,402,8,18,20,34,40 (computed). Closures at 2, 8, 20 match the observed magic numbers; 18 and 34 are false closures the oscillator does not predict (its 1d1d and 2s2s merge into one N=2N=2 shell of 12) — and nature sides with neither caricature beyond 20, where the spin-orbit force takes over the bookkeeping (one credit line; the shell-model story lives with the portraits of Effective Potential and the Centrifugal Barrier and the oscillator article). Why keep both caricatures: their disagreements localize the physics. Where box and oscillator agree (2, 8, 20), mean-field geometry alone explains nuclei; where they disagree (18/34 vs 20/40), the answer is sensitive to well shape and interactions — a bracketing technique worth more than either model alone. *Verified: all six β\beta root-found; ordering strict; capacities and cumulative sums; En0∝n2E_{n0}\propto n^2 exact; electron-in-1nm energies below (article verifier).*

The finite well: matching and the threshold

For V(r)=−V0V(r)=-V_0 inside RR, zero outside, and a bound state at E=−EB<0E=-E_B<0: interior wavenumber k=2m(V0−EB)/ℏk=\sqrt{2m(V_0-E_B)}/\hbar, exterior decay κ=2mEB/ℏ\kappa=\sqrt{2mE_B}/\hbar. Per channel, the admissible pieces are forced:

uℓ(r<R)∝kr jℓ(kr),uℓ(r>R)∝κr hℓ(1)(iκr)(2)u_\ell(r<R)\propto kr\,j_\ell(kr),\qquad u_\ell(r>R)\propto \kappa r\,h_\ell^{(1)}(i\kappa r) \qquad (2)

where: the interior keeps the regular family (origin in-domain), the exterior keeps the decaying continuation (the previous article's handover, cashed). Continuity of uu and u′u' at RR — equivalently of the logarithmic derivative u′/uu'/u, which cancels the free normalizations — is the entire quantization condition. This is precisely the matching craft of Wavefunction Matching Conditions, promoted to three dimensions with new alphabet.

Go deeper · Derivation B · 2 minThe s-wave transcendental, its 1D twin, and the existence threshold
Derivation BThe s-wave transcendental, its 1D twin, and the existence threshold

We match the ℓ=0\ell=0 channel explicitly, recognize the result as an old friend, and derive three-dimensions' signature theorem: no binding below a computable depth. The strategy is logarithmic-derivative matching plus one limit (EB→0E_B\to0) taken honestly.

Step 1. At ℓ=0\ell=0: uin=sin⁡kru_{in}=\sin kr (the wall u(0)=0u(0)=0 already enforced), uout=e−κru_{out}=e^{-\kappa r}. Log-derivatives at RR: kcot⁡kRk\cot kR inside, −κ-\kappa outside (both computed symbolically). The spectrum condition:

kcot⁡kR=−κ(3)k\cot kR=-\kappa \qquad (3)

Step 2. The 1D twin. Equation (3) is identical to the quantization condition of the odd-parity states of a 1D finite well of width 2R2R — as it must be: the half-line problem with a hard wall at the origin is the odd sector of the symmetric 1D problem (the doctrine of Effective Potential and the Centrifugal Barrier, now cashed as a working identity). Every graphical-solution technique from Finite Square Well imports unchanged; only the even 1D solutions — the ones with u(0)≠0u(0)\ne0 — are missing. And there hangs the physics: the 1D well's always-bound state is an even state. Discard the even sector and you discard the guarantee.

Step 3. The threshold. A bound state appears when (3) first admits a solution as EB→0+E_B\to0^+ (κ→0\kappa\to0): then cot⁡kR→0−\cot kR\to0^-, i.e. kR→π/2kR\to\pi/2 with k→2mV0/ℏk\to\sqrt{2mV_0}/\hbar. Existence therefore requires

V0R2>π2ℏ28m(4)V_0R^2>\frac{\pi^2\hbar^2}{8m} \qquad (4)

— the well must be deep and wide enough that a quarter wave fits inside with room to bend over. Numerically confirmed on both sides: at 0.97 Vth0.97\,V_{th} the matching equation has no root; at 1.03 Vth1.03\,V_{th}, exactly one (computed by root-counting sweeps). The nn-th s-state needs (2n−1)2(2n-1)^2 times the threshold; ℓ-channels pay extra rent on top (the centrifugal barrier raising the effective floor — Effective Potential and the Centrifugal Barrier's landscape, one line). Why 1D and 3D disagree about weak binding: in 1D an arbitrarily weak well binds because the wavefunction can spread symmetrically with almost no curvature penalty — the even state's flat top. In 3D the origin wall forbids the flat top; the state must rise from zero and turn over inside the well. The threshold (4) is the price of the turn. (Two dimensions, for the curious, is the marginal case — any attraction binds, but exponentially weakly — an honesty line beyond this article's domain.) *Verified: matching (3) symbolic; threshold value 23.2023.20 MeV for the deuteron's parameters; root counts 0/10/1 at 0.97/1.03 Vth0.97/1.03\,V_{th}; excited-state absence check below (article verifier).*

Figure
The deuteron matching: sine inside, exponential outside, one smooth joint — and most of the state in the tail
u(r) for the deuteron: V₀ = 33.7 MeV, R = 2.1 fm (computed by matching) R = 2.1 fm well −V₀ log-derivative match: k cot kR = −κ sin(kr) k = 0.872 fm⁻¹ e^(−κr) tail · κ = 0.2316 fm⁻¹ P(r above R) = 0.63 — the halo u(0)=0 wall at the origin (no even sector) · all numbers root-found/integrated in the article verifier

Limiting cases

caseresultmeaning
V0→∞V_0\to\infty(3) forces sin⁡kR→0\sin kR\to0: box spectrum recoveredthe hard sphere as a limit, continuously
V0R2→π2ℏ2/8m+V_0R^2\to\pi^2\hbar^2/8m^+one s-state at EB→0E_B\to0, tail 1/κ→∞1/\kappa\to\inftythreshold birth: infinite halo first, binding second
V0R2<π2ℏ2/8mV_0R^2<\pi^2\hbar^2/8mno bound state at all3D novelty — attraction below the pass mark binds nothing
ℓ≥1\ell\ge1higher thresholds (centrifugal rent)p-wave binding needs a visibly deeper well
EB≪V0E_B\ll V_0exterior dominates; physics set by κ\kappa alonethe shallow-bound universality the deuteron exemplifies
ℓ=0\ell=0 spectrum condition≡\equiv odd sector of 1D well, width 2R2Rthe origin wall as parity selection

Worked examples

Example 1 — an electron in a hard nanosphere. A colloidal quantum dot is crudely a hard sphere of radius R=1R=1 nm. Ladder the spectrum.

Step 1. Scale: E1s=ℏ2π2/2meR2=0.376E_{1s}=\hbar^2\pi^2/2m_eR^2=0.376 eV (computed) — conveniently at the electron-volt scale that makes dots optically active.

Step 2. Ladder by zeros (all computed): E1p=(4.493/π)2E1s=0.769E_{1p}=(4.493/\pi)^2E_{1s}=0.769 eV; E1d=1.266E_{1d}=1.266 eV; E2s=4E1s=1.504E_{2s}=4E_{1s}=1.504 eV exactly (the ℓ=0\ell=0 tower's n2n^2 law). Level spacings of a few tenths of an eV — visible-light differences: the crude hard sphere already explains why dot emission color tracks size, with E∝1/R2E\propto1/R^2 as the tuning law.

Step 3. Honesty: real dots have finite barriers, effective masses, and Coulomb corrections — the hard sphere is the geometry-only skeleton. Answer: 0.376, 0.769, 1.266, 1.5040.376,\,0.769,\,1.266,\,1.504 eV for 1s,1p,1d,2s1s,1p,1d,2s — the zero ladder in electron-volts.

Example 2 — the deuteron, end to end (the portrait's calculation). Given EB=2.2246E_B=2.2246 MeV and force range R=2.1R=2.1 fm, find the nuclear well.

Step 1. Inputs: μc2=469.46\mu c^2=469.46 MeV (reduced mass, computed); κ=2μEB/ℏc=0.2316\kappa=\sqrt{2\mu E_B}/\hbar c=0.2316 fm−1^{-1} — the tail the previous article computed, now the matching's right-hand side.

Step 2. Solve (3) for V0V_0 (root-found): V0=33.7V_0=33.7 MeV, with interior wavenumber k=0.872k=0.872 fm−1^{-1}. Sanity: threshold Vth=π2(ℏc)2/8μR2=23.2V_{th}=\pi^2(\hbar c)^2/8\mu R^2=23.2 MeV (computed), so V0/Vth=1.45V_0/V_{th}=1.45 — the nuclear force clears its audition by less than half. Shallowness index EB/V0=0.066E_B/V_0=0.066: the state sits just under the rim of a deep well.

Step 3. Consequences, all computed: exactly one s-state (the second would need 9Vth=2099V_{th}=209 MeV — root-count confirms none); exterior probability Pout=0.63P_{out}=0.63 — most of the deuteron is outside the nuclear force, in the pure e−κre^{-\kappa r} tail; and no excited deuteron exists, in agreement with experiment. Answer: V0≈34V_0\approx34 MeV at R=2.1R=2.1 fm; one barely-bound, mostly-outside state — the nuclear force's first quantum portrait, and a threshold pass at 1.45.

Origins · 1 minHans Bethe and how this was discovered
HB
Hans Bethe
1906–2005 · Cornell

The deuteron computation above is, in its essentials, the 1935 paper "Quantum Theory of the Diplon" by Bethe and Rudolf Peierls — written, legend has it, substantially on a train ride, months after Chadwick's neutron made the proton-neutron nucleus thinkable and Urey's deuterium gave it a name. (Bethe's electromagnetic side — the multipole-radiation systematics of his famous reviews — is told in an E&M-track portrait; this card is the nuclear-force debut.) The pair's insight was strategic modesty: nobody knew the nuclear force's shape, but a barely-bound state doesn't care. Take a square well of plausible range, feed in the measured binding energy, and everything observable at low energy — the tail, the photodisintegration cross section they computed, the scattering length — follows from κ\kappa alone, because the state lives mostly outside the well, exactly the 63% this article computes. That "shape-independence" became the effective-range doctrine organizing all of low-energy nuclear physics. Bethe drove the program relentlessly through the 1930s — colleagues called the resulting trio of encyclopedic review articles by a nickname this card will not repeat, since their radiation chapters belong to the other track — and the habit of extracting model-independent physics from one measured number stayed his signature through stellar burning (Nobel 1967) and beyond. Peierls' own portrait duties lie elsewhere in this track; here he is the essential co-author on the calculation that taught physicists how to interrogate a force they could not see.

History
1932
— Chadwick discovers the neutron; Urey isolates deuterium — the two-body nucleus exists
1935
— Bethe and Peierls solve the deuteron as a finite spherical well: depth from binding energy
1936
— Shape-independence sharpens into effective-range theory (Bethe, Schwinger and others follow)
1949
— Shell models built on spherical-well and oscillator level ladders explain magic numbers with spin-orbit
1990
s — Halo nuclei discovered: extreme spherical-well tails at the drip lines

Going further

  • Griffiths & Schroeter §4.1.3 — the infinite spherical well at the source register.
  • Bethe & Peierls, Proc. R. Soc. A 148, 146 (1935) — the deuteron paper this article's example reruns.
  • Sakurai & Napolitano Ch. 6 — the matching machinery in its scattering continuation.
  • Krane, Introductory Nuclear Physics Ch. 4 — the deuteron and the well, at nuclear-physics register.

Provenance note: Equations are standard central-potential and spherical Bessel results; a verifier should confirm: (i) the radial-to-spherical-Bessel reduction (Griffiths §4.1.3, Sakurai §3.7); (ii) j0(x)=sin⁡x/xj_0(x)=\sin x/x zeros at nπn\pi and j1j_1 first zero ≈4.4934\approx4.4934 solving tan⁡x=x\tan x=x (Abramowitz & Stegun §10.1.1, Table 10.6); (iii) the infinite-box formula Enℓ=ℏ2xnℓ2/(2ma2)E_{n\ell}=\hbar^2x_{n\ell}^2/(2ma^2); (iv) the ℓ=0\ell=0 finite-well condition kcot⁡(ka)=−κk\cot(ka)=-\kappa and its binding threshold z0=π/2z_0=\pi/2 i.e. V0a2=π2ℏ2/(8m)V_0a^2=\pi^2\hbar^2/(8m) (Cohen-Tannoudji Complement A_VII, Shankar Ch.12.6). All numbers quoted (π\pi, 4.4934.493, 5.7635.763, 2π2\pi) are tabulated spherical Bessel zeros. — Item (i) is the reduction owned by Spherical Bessel and Neumann Functions (its verifier); items (ii)–(iv) are executed in this article's verify script (zeros root-found rather than read from tables — π\pi, 4.49344.4934, 5.76355.7635, 2π2\pi, 6.98796.9879, 7.72537.7253; the box formula evaluated for the 1 nm electron; the matching condition derived symbolically; the threshold bracketed numerically at 0.97/1.03 Vth0.97/1.03\,V_{th}), plus the deuteron solve (V0=33.7V_0=33.7 MeV at R=2.1R=2.1 fm, μc2=469.46\mu c^2=469.46 MeV), the exterior-probability integral 0.630.63, and the no-excited-state check. Edition note: the infinite-well spectrum derivation formerly resident in the base of Spherical Bessel and Neumann Functions is owned HERE per the chapter map (relocation noted at both ends); scattering off the same well — phase shifts, resonances, the zero-energy story — belongs BY NAME to the scattering chapter (Phase Shifts, Low-Energy Scattering and the Scattering Length, Bound States and Zero-Energy Resonances), which inherits this article's matching setup at E>0E>0.

Why does the s-wave condition involve −cot rather than tan, like half the 1D solutions?

Because only the odd 1D sector survives. The symmetric 1D well's even states satisfy ktan⁡(kR)=κk\tan(kR)=\kappa, odd states kcot⁡(kR)=−κk\cot(kR)=-\kappa. The spherical s-wave's uu must vanish at the origin — that is oddness on the doubled line — so the tan⁡\tan branch never appears. If your spherical-well solution contains a tan⁡\tan, you have accidentally counted states that violate u(0)=0u(0)=0; they are the ghosts of the missing even sector.

Does the threshold theorem contradict the delta-well, which binds despite being infinitely narrow?

No — the 1D delta well binds (its bound state is even, exploiting exactly the sector 3D lacks); a 3D delta-shell or contact interaction is genuinely different and does not bind below threshold strength. Take the well limit R→0R\to0, V0→∞V_0\to\infty with V0R2V_0R^2 fixed: binding survives only if V0R2V_0R^2 stays above π2ℏ2/8m\pi^2\hbar^2/8m — the threshold is scale-invariant under this limit, which is why "zero-range" nuclear models must carry an auxiliary parameter (the scattering length) rather than a bare delta strength.

How sensitive is the deuteron's 63%-outside figure to the model?

Weakly — that is the shape-independence point. The exterior fraction is controlled by κR\kappa R (here 0.490.49): any potential of similar range reproducing the same binding energy gives a comparable split, because the exterior form e−κre^{-\kappa r} is model-independent and the interior merely has to join onto it smoothly. Realistic potentials (with repulsive cores and tensor forces) shift the number by some percent, not qualitatively. What is model-sensitive: V0V_0 itself, interior node structure, and anything probing r<Rr<R physics — the warning box's caveat.

What happens to these bound states as I make the well shallower through the threshold?

The state's energy rises toward zero, its tail 1/κ1/\kappa stretches without bound, and at threshold the "state" becomes a zero-energy solution flat at infinity — not normalizable, no longer a bound state, but not nothing either: it leaves a fingerprint as a divergent scattering length and a huge low-energy cross section (the zero-energy resonance of the scattering chapter, named). Just below threshold you have a "quantum halo": arbitrarily large, arbitrarily weakly bound, universal in properties. Feshbach-tuned atoms walk this path in the laboratory daily.

Why do the box's magic numbers fail after 20 when the calculation seems exact?

The calculation is exact — for the model. The model errs twice: real nuclear wells are neither hard-walled nor oscillator-shaped (their flat bottom and diffuse edge reorder high levels), and, decisively, the nuclear spin-orbit interaction is strong and inverted, splitting each ℓ-level by MeV-scale amounts that regroup the ladder entirely. Box and oscillator agree on 2, 8, 20 — geometry-robust closures — and both fail beyond, which is precisely the evidence that pointed Goeppert Mayer and Jensen to the missing spin-orbit ingredient.

Can I use these solutions for a particle confined by something soft, like a trap that isn't square?

As brackets and as bases. Brackets: box (stiffest) and oscillator (softest reasonable) spectra sandwich most smooth traps' low levels — compare both before any serious computation. Bases: the box eigenfunctions jℓ(βnℓr/R)Yℓmj_\ell(\beta_{n\ell}r/R)Y_\ell^m form a complete orthogonal set on the sphere's interior (Sturm-Liouville with weight r2r^2 — the orthogonality doctrine of Boundary Conditions and Normalization of Radial Wavefunctions), so soft-trap Hamiltonians are routinely diagonalized in exactly this basis. The zero ladder then reappears as grid points of a spectral method rather than as physical energies.

Before this

Where this leads