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Physics IV course sequence · Interactive lesson

Central potentials and the 3D Schrödinger equation

Before hydrogen can have an energy level, it has to become a solvable problem. Two moving bodies collapse to one fictitious particle of reduced mass; three coordinates collapse to one ordinary differential equation plus a table of angular functions you solve once and reuse for the rest of the course. This lesson is that reduction.

UPIV-10.01 · Lesson 1 of 9 in this unit. Position is not a completion score.
Starting model: Central potentials and the 3D Schrödinger equationLeft: two bodies orbiting their shared centre of mass, the light one on a circle 0.888 of the separation, the heavy one 0.112 of it. Right: the same physics as one particle of mass μ = 0.8882 m at that same separation r from a fixed centre. Every transition energy of the pair falls 11.182% short of the infinite-mass value.two bodies, one CMone particle of mass μM/m = 8μ/m = 0.8882orbits 0.888 : 0.112r and V(r) unchanged
Start with a picture. Change the model in the lab below.
1

Build the model

Two bodies become one, and the angles leave before the potential is named.

The key idea

A central potential depends only on the distance r between two particles, which lets the two-body problem reduce exactly to one particle of reduced mass μ moving in V(r), with a wavefunction that factors as ψ = R(r)Yₗₘ(θ, φ).

Example. For hydrogen μ = mₑ mₚ/(mₑ + mₚ) = mₑ/(1 + 1/1836.15) = 0.9994557 mₑ, which lowers the Rydberg energy from the infinite-mass 13.6057 eV to 13.5983 eV — a 7.4 meV shift that moves Lyman-α by 0.066 nm.

The complete physical model and assumptions

An atom is two bodies, and a two-body wavefunction lives on six coordinates. Two exact moves cut that down. Because the interaction depends only on r₁ − r₂, the Hamiltonian splits cleanly into a free centre-of-mass piece and a relative piece in which a single fictitious particle of reduced mass μ = m₁m₂/(m₁ + m₂) moves in V(r); the atom's entire internal spectrum belongs to that second piece, and nothing has been approximated to get there. Then, because V depends on the length of r and not its direction, the angular derivatives in the Laplacian appear only inside L², divided by exactly r² — so multiplying through by r² quarantines them, ψ = R(r)Y(θ, φ) goes through, and the angular half of the problem is solved once for every central potential there will ever be. The cost is worth stating up front. The reduction is exact for two bodies and dies at three, where a mass-polarisation term survives and helium never separates. Any potential with a direction in it — an applied field, a second electron, a deformed nucleus — destroys the factorisation immediately. And the familiar −e²/4πε₀r is a further idealisation stacked on top, one the separation never asked for: what it buys is not the spherical harmonics but the 1/n² spectrum and the degeneracy in l.

1Six coordinates, and the move that removes three

An isolated atom is two particles, so its wavefunction lives on six coordinates: Ψ(r₁, r₂), with H = −(ℏ²/2m₁)∇₁² − (ℏ²/2m₂)∇₂² + V(r₁ − r₂). Nothing separates in these variables, because V couples them. Change to the centre of mass R = (m₁r₁ + m₂r₂)/(m₁ + m₂) and the separation r = r₁ − r₂. The kinetic energy — the one piece of algebra worth doing by hand once — becomes −(ℏ²/2M)∇²R − (ℏ²/2μ)∇²ᵣ, with M = m₁ + m₂ and 1/μ = 1/m₁ + 1/m₂, and the cross terms cancel identically. Now Ψ = e(iK⋅R)ψ(r) works: the centre of mass is a free particle carrying kinetic energy ℏ²K²/2M, and every level, every orbital and every spectral line of the atom belongs to the second factor. The only thing used was that V depends on the difference of the positions, which is translation invariance — so this reduction is exact, not a model.

2Reduced mass is what an exact reduction leaves behind

μ = m₁m₂/(m₁ + m₂) is smaller than either mass and is dominated by the lighter one: for hydrogen μ = mₑ × 1836.15/1837.15 = 0.9994557 mₑ. Let the nucleus grow without limit and μ → mₑ, which is the clamped-nucleus picture — so nailing the proton down is the approximation, and μ is the exact answer, not the other way round. The correction is small but never invisible. Every level of a hydrogenic system carries one factor of μ and every length one factor of 1/μ, so hydrogen's Rydberg energy is 13.5983 eV against the infinite-mass 13.6057 eV, and Lyman-α sits at 121.568 nm rather than 121.502 nm. Deuterium, with a nucleus twice as heavy, has μ = 0.9997276 mₑ, and the 0.18 nm gap between the two Balmer-α lines near 656 nm is how Urey identified deuterium in 1932 — a new isotope found in a mass ratio. Positronium, where the two masses are equal, gives μ = mₑ/2 exactly: half the binding, twice the radius.

3Why r-dependence alone lets the angles leave

In spherical coordinates ∇² = (1/r²)∂ᵣ(r²∂ᵣ) + (1/r²sinθ)∂θ(sinθ ∂θ) + (1/r²sin²θ)∂²φ. The two angular terms are not a mess to be endured: together they are exactly −L²/ℏ², an operator built only from θ and φ, and they sit divided by exactly r². So H = −(ℏ²/2μ)(1/r²)∂ᵣ(r²∂ᵣ) + L²/(2μr²) + V(r). If V depends on r alone, then L² commutes with every term — it cannot see V(r), and the radial derivatives cannot see θ or φ. Put ψ = R(r)Y(θ, φ), divide by RY and multiply by −2μr²/ℏ². The r² cancels the 1/r² carried by the angular block, and what is left is a function of r alone on one side and a function of θ and φ alone on the other. Two such functions can be equal only if both are the same constant, and that constant is written l(l + 1). That step, and only that step, is where separability comes from.

4One boundary condition per separation constant

Separation manufactures constants; boundary conditions choose their values, and each of the three comes from a different demand. Take φ first: d²Φ/dφ² = −m²Φ gives Φ = e(imφ), and going once round the axis must return the same wavefunction, Φ(φ + 2π) = Φ(φ), so m is an integer. The θ equation then has solutions that diverge at cosθ = ±1 unless its series terminates; demanding a finite ψ on the polar axis forces l to be a non-negative integer with l ≥ |m|, so each l carries 2l + 1 values of m. Only the third constant, E, comes from the radial equation, where R must stay finite at the origin and normalisable at infinity. Notice what that ordering means: two of the three quantum numbers are fixed by geometry before the potential has even been named, and they come out the same for a nuclear well as for hydrogen. E is the only one that ever knows what V is.

5The angular half is universal; only the radial half knows V

The saving is large. Yₗₘ(θ, φ) is the answer for every central potential there is: the three-dimensional isotropic oscillator, the finite spherical well, the Woods-Saxon potential of a nucleus, the Yukawa and Thomas-Fermi screened forms, the confinement of a spherical quantum dot, and the Coulomb 1/r. That is why the s, p, d labels and the 2l + 1 counting carry across from atoms to nuclei to nanocrystals with no rederivation. Rotational symmetry also hands you a degeneracy for free: because H contains no preferred direction, the 2l + 1 states of a given l share one energy in any V(r), which is exactly why something with a direction in it — an applied field — is what splits them. What the potential controls is the radial equation, and through it E(n, l) and the node count. The extra l-degeneracy of hydrogen is not generic: move the exponent off −1 and states of different l separate at once, while every Yₗₘ stays untouched.

6Where the reduction stops

Three limits are worth naming in advance. First, two bodies only. Remove the centre of mass from a three-body atom and you are left not merely with reduced masses but with a mass-polarisation term, −(ℏ²/M)∇₁⋅∇₂ with M the nuclear mass, coupling the electrons through the recoiling nucleus; helium has no exact one-particle reduction even before the repulsion between its electrons is counted. Second, central means central. An external electric field, the r₁₂ repulsion between two electrons, a quadrupole-deformed nucleus — each puts a direction into V and kills the factorisation on the spot. Third, spherical symmetry is a far weaker requirement than a point charge. A proton of radius 0.84 fm gives a potential that is not −e²/4πε₀r inside the nucleus, yet it is still a function of r alone, so ψ = R Yₗₘ survives intact and only the radial equation changes. Keep the two ideas apart: separation is a statement about symmetry, and 1/r is a statement about the source.

2

Key equations

Read the units, assumptions and limits before substituting.

Reduced mass

1/μ = 1/m₁ + 1/m₂, so μ = m₁m₂/(m₁ + m₂)

Hydrogen: μ = 0.9994557 mₑ. Positronium: μ = mₑ/2 exactly.

m₁, m₂ and μ in kg, or all as multiples of mₑ; μ is always smaller than either mass.

Two-body Hamiltonian after the split

H = −(ℏ²/2M)∇²R − (ℏ²/2μ)∇²ᵣ + V(r)

The R term is a free particle. Every atomic level lives in the r term.

M = m₁ + m₂ in kg; R is the centre of mass and r = r₁ − r₂, both in m.

Laplacian in spherical coordinates

∇² = (1/r²)∂ᵣ(r²∂ᵣ) − L²/(ℏ²r²)

Every angular derivative sits inside L², divided by exactly r². That is the whole trick.

L² acts on θ and φ only and carries units of ℏ², that is J² s²; r in m.

Separation with ψ = R(r)Y(θ, φ)

(1/R) d/dr(r² dR/dr) − (2μr²/ℏ²)[V(r) − E] = l(l + 1)

Two functions of independent variables can only agree by both being one constant.

The left side depends on r only; V and E in J; l(l + 1) is dimensionless.

The angular equations and their constants

L²Yₗₘ = ℏ²l(l + 1)Yₗₘ · LzYₗₘ = mℏYₗₘ

Solved once. The same Yₗₘ serve every central potential, hydrogen included.

m is an integer from 2π-periodicity in φ; l = 0, 1, 2, … with |m| ≤ l from regularity at the poles.

How μ rescales the whole answer

Eₙ ∝ μ · a ∝ 1/μ · λ ∝ 1/μ

Hydrogen: 0.054% shallower. Muonic hydrogen: 10.1%. Positronium: 50%.

M is the nuclear mass and m the orbiting one. Against the M → ∞ values, binding energies shrink by exactly the fraction 1/(1 + M/m) and lengths grow by m/M.
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

0.9
0 to 3.6; steps of 0.1.
45 °
0 to 360 °; steps of 15.

Try this. Set the mass-ratio slider to 0 and the two bodies are twins: equal orbits, μ exactly m/2, positronium. Drag right to 3.3 and the heavy body's orbit collapses to 0.0005 of the separation while μ climbs to 0.9995 m — the clamped nucleus is the limit M → ∞, not an assumption you get for free.

Live results

MASS RATIO M/m
8
REDUCED MASS μ/m
0.8882
HEAVY-BODY ORBIT
0.1118 of r
SHIFT FROM INFINITE MASS
11.182 %

Results follow this lesson’s model and assumptions. Displayed values are rounded.

Interactive Physics IV modelLeft: two bodies orbiting their shared centre of mass, the light one on a circle 0.888 of the separation, the heavy one 0.112 of it. Right: the same physics as one particle of mass μ = 0.8882 m at that same separation r from a fixed centre. Every transition energy of the pair falls 11.182% short of the infinite-mass value.two bodies, one CMone particle of mass μM/m = 8μ/m = 0.8882orbits 0.888 : 0.112r and V(r) unchanged
Left: two bodies orbiting their shared centre of mass, the light one on a circle 0.888 of the separation, the heavy one 0.112 of it. Right: the same physics as one particle of mass μ = 0.8882 m at that same separation r from a fixed centre. Every transition energy of the pair falls 11.182% short of the infinite-mass value.

Predict → change one variable → check

Plan a change before running it. Every other input stays at the saved baseline.

Saved baseline. Mass ratio, log₁₀(M/m): 0.9; Orbital phase: 45 °

Baseline 0.9; choose 0 to 3.6, in steps of 0.1.
4. Compared with the saved baseline, this result will…

This experiment is kept only while this page is open. It does not change saved course progress.

4

Catch the common trap

The reduced mass gets filed as a correction and the factorisation as an approximation, and both are backwards. μ is what an exact change of variables produces from any V(r₁ − r₂); the clamped nucleus is the approximation, recovered by letting M → ∞. And ψ = R(r)Yₗₘ(θ, φ) is no trial form that happens to suit hydrogen: H, L² and Lz commute for every central potential, so their common eigenfunctions are a complete basis. The error this breeds is treating spherical harmonics as a Coulomb result. They are not — angular momentum produces them, so they survive the finite-size proton, the screening in a many-electron atom and the Woods-Saxon well of a nucleus. What 1/r buys is narrower: the 1/n² spectrum and the accidental l-degeneracy, both of which vanish the moment the exponent moves off −1, while every Yₗₘ stays put.

5

Practice & worked examples

3 authored examples. Make an attempt, then reveal the reasoning one step at a time.

EasyExample 1

Take mₚ/mₑ = 1836.15 and the infinite-nuclear-mass Rydberg energy as 13.6057 eV. Find the reduced mass of hydrogen as a multiple of mₑ, then the ground-state energy and the size of the correction. Finally quote that correction as a wavelength shift on the Lyman-α line, whose infinite-mass value is 121.502 nm.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 4 steps revealed.

MediumExample 2

A deuterium nucleus has mass 3670.48 mₑ. Hydrogen's Balmer-α line (n = 3 → 2) lies at 656.28 nm. Predict deuterium's Balmer-α wavelength and the splitting between the two lines, and state the resolving power a spectrograph needs to separate them.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 4 steps revealed.

HardExample 3

Muonic hydrogen replaces the electron with a muon, mμ = 206.77 mₑ, bound to a proton of 1836.15 mₑ. Find the reduced mass, the ground-state energy and the Bohr radius of the system, taking a₀ = 52918 fm and the Rydberg energy as 13.6057 eV. Then repeat with mμ used unreduced in place of mₑ, and say how large the difference is and why it dwarfs the one in ordinary hydrogen.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

6

Quick check

Select an answer and explain it before checking.

An electron is bound to a nucleus by the screened potential V(r) = −(A/r)e(−r/d), with A and d fixed constants. What happens when you try to separate its three-dimensional Schrödinger equation?
7

Review & continue

A central potential depends only on the distance r between two particles, which lets the two-body problem reduce exactly to one particle of reduced mass μ moving in V(r), with a wavefunction that factors as ψ = R(r)Yₗₘ(θ, φ).

  • Explain the relationship without looking at the equation.
  • Check a sign, a unit and a model assumption in your working.
  • Return to the lab or worked example if a step is still unclear.

Extra challenging questions

Connect several ideas, explore supplied data, and compare your reasoning with a worked solution.