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Nuclear, particle & quantum-information sequence · Interactive lesson

Nucleons, isospin and the two-nucleon system

Nature made exactly one bound state out of two nucleons, and it is a strange one: barely held, mostly outside its own potential, and not spherical. This topic hands you the bookkeeping that makes all three follow from a single antisymmetry rule, rather than from a table of measured numbers you have to trust.

UPV-14.01 · Lesson 1 of 9 in this unit. Position is not a completion score.
Starting model: Nucleons, isospin and the two-nucleon systemZero-energy S-wave function u(r) above the square well that produces it, for depth 21.5 MeV and radius 2.10 fm. Inside, u is a sine of phase k₀R = 1.512 rad; outside it is a straight line whose dashed extension meets the axis at the scattering length a = -21.5 fm. Threshold depth here is 23.20 MeV.zero-energy S-wave u(r)a = −21.5 fmRV₀ = 21.5 MeV02 fm4 fm6 fm
Start with a picture. Change the model in the lab below.

Nuclear, particle & quantum-information sequence. These units continue into nuclear and particle physics and quantum information. Follow your university’s prerequisites, mathematical depth and assessment; this independent pathway is not a universal programme specification.

1

Build the model

The strong force barely notices charge; the exclusion principle notices everything.

The key idea

Isospin is a two-valued internal label that treats the proton and the neutron as one particle, acted on by operators Tᵢ = τᵢ/2 obeying the same SU(2) algebra as spin, and approximately conserved by the strong interaction alone.

Example. The two nucleons of a deuteron sit in the isospin singlet |0,0⟩ = (|pn⟩ − |np⟩)/√2, so T = 0; its T = 1 partner (|pn⟩ + |np⟩)/√2 is the ¹S₀ state, unbound by about 66 keV, and its charged relatives pp and nn are unbound too.

The complete physical model and assumptions

Heisenberg's move was to stop treating the proton and the neutron as two particles and start treating them as two states of one, separated by a label the strong interaction cannot read. Give the nucleon an internal two-dimensional space, |p⟩ = (1, 0)ᵀ and |n⟩ = (0, 1)ᵀ, act on it with Tᵢ = τᵢ/2 built from the very Pauli matrices spin already uses, and the whole SU(2) apparatus transfers untouched: ladder operators T_± that turn a neutron into a proton, Clebsch-Gordan addition, total-T multiplets. Charge independence then becomes a statement about operators, [Hₛ, Tᵢ] = 0 for i = 1, 2, 3, so the strong Hamiltonian reads a pair's total isospin and never its projection; charge symmetry, invariance under the π rotation exp(−iπT₂) alone, is the weaker claim that equates only pp with nn. The evidence is that the three ¹S₀ scattering lengths agree to a few fermi out of twenty; the cost is that they agree only to a few fermi, because Coulomb and the up-down quark mass difference make this a percent-level symmetry rather than an exact one. What it buys is a counting rule. Two nucleons are now identical fermions, so space, spin and isospin must be antisymmetric together, (−1)(L+S+T) = −1. At L = 0 that leaves exactly two channels — ³S₁ with T = 0 and ¹S₀ with T = 1 — and since pp and nn are stuck at T = 1, they are locked out of the only one that binds.

1Two states of one particle, and the operators that say so

Heisenberg's observation was arithmetic: mₚ c² = 938.272 MeV and mₙ c² = 939.565 MeV differ by 1.293 MeV, one part in 726. Treat that near-degeneracy as a symmetry and give the nucleon an internal two-dimensional space, |p⟩ = (1, 0)ᵀ and |n⟩ = (0, 1)ᵀ, with operators Tᵢ = τᵢ/2 built from the same Pauli matrices spin uses. The algebra is identical: [Tᵢ, Tⱼ] = i εᵢⱼₖ Tₖ, T² = ¾ on the doublet, and T_± = T₁ ± iT₂ move you along it, T+|n⟩ = |p⟩. Charge depends on the third component alone, Q = e(T₃ + B/2) with B the baryon number, which fixes the proton at T₃ = +½ in the convention used here. Nothing has yet been assumed about the force. This is a relabelling, and its entire content is the claim that the two labels can be rotated into each other.

2Charge independence is the stronger of two symmetries

Two distinct claims hide behind "the strong force ignores charge". Charge symmetry is invariance under the π rotation exp(−iπT₂), which sends |p⟩ → |n⟩ and |n⟩ → −|p⟩ and therefore equates only pp with nn. Charge independence is [Hₛ, Tᵢ] = 0 for all three i: full SU(2) invariance, so Hₛ may depend on a pair's total T but never on T₃, and it brings np in a T = 1 state into the same equality. Different data test the two. Coulomb-corrected ¹S₀ scattering lengths give aₚₚ = −17.3 fm and aₙₙ = −18.9 fm, a 1.6 fm gap measuring charge-symmetry breaking; aₙₚ = −23.74 fm sits 5.6 fm from their mean, measuring the larger charge-independence breaking. Both look enormous as lengths and are tiny as forces: fitted as square wells of radius 2.1 fm they are 21.12, 21.28 and 21.65 MeV deep, a spread of 2.5%.

3Antisymmetry now runs over three labels at once

Once proton and neutron are one particle, two nucleons are identical fermions, and what must be antisymmetric is the product of space, spin and isospin. Exchange multiplies the spatial factor by (−1)L; the spin triplet is symmetric and the singlet antisymmetric, giving (−1)(S+1); isospin does the same, giving (−1)(T+1). The product is (−1)(L+S+T), so L + S + T must be odd. Apply it. At L = 0 exactly two channels survive, ¹S₀ with T = 1 and ³S₁ with T = 0. At L = 1, S + T must be even, so ¹P₁ carries T = 0 while ³P₀, ³P₁ and ³P₂ carry T = 1. Now use the projection: a pp or nn pair has |T₃| = 1, hence T = 1, and is barred from ³S₁ and ¹P₁ outright. The deuteron is Jπ = 1⁺, so L is even and S = 1, making L + S odd and forcing T = 0. A T = 0 state has T₃ = 0 only. It can have no charged partners, and none is observed.

4One channel binds, and only just

Put numbers on it with the crudest model that works. With μ = mₚ mₙ/(mₚ + mₙ), ħ²/2μ = (ħc)²/2μc² = 38938/938.9 = 41.47 MeV fm². For a square well of radius R the first S-wave bound state appears when a quarter wavelength just fits, k₀R = π/2, so Vcrit = π²(41.47)/4R² = 102.3/R², or 23.20 MeV at R = 2.1 fm. Fit the triplet: matching u = sin kr inside to exp(−κr) outside gives k cot kR = −κ, and with κ = √(B/41.47) = 0.2316 fm⁻¹ the solution is kR = 1.8305, V₀ = 33.73 MeV. That one well then returns a zero-energy scattering length of 5.41 fm against the measured 5.424 fm, so a single parameter fits two independent numbers. Fit the singlet to a = −23.74 fm instead and V₀ = 21.65 MeV, 6.7% under threshold. The deuteron survives on a few MeV of margin in a 34 MeV well, and it shows: 1/κ = 4.32 fm, so most of the pair sits outside the 1.41 fm range of the force holding it.

5The tensor force is what makes the deuteron non-spherical

A pure ³S₁ state is spherical and has a strictly zero quadrupole moment, yet Qd = +0.2859 fm². Something must mix in L = 2, and the only static operator that can is the tensor S₁₂ = 3(σ₁⋅r̂)(σ₂⋅r̂) − σ₁⋅σ₂, which commutes with J², S² and parity but not with L², and whose matrix elements in the (|³S₁⟩, |³D₁⟩) basis are 0, 2√2 and −2. The radial problem is therefore two coupled equations for u(r) and w(r), with a 6ħ²/2μr² centrifugal term in the D channel, boundary conditions u(0) = w(0) = 0 and both decaying as exp(−κr); in Python it is a 2N × 2N Hermitian matrix passed to numpy.linalg.eigh, or a two-channel shooting problem. Q = (1/20)∫r²w(√8u − w)dr is linear in w to leading order, which is why a 4 to 6% probability — a 20 to 25% amplitude — yields a measurable Q. The magnetic moment gives a rough independent estimate: μd = 0.857438 μN against μₚ + μₙ = 0.879804 μN gives PD ≈ 3.9% in the impulse approximation, which ignores meson-exchange currents and relativistic terms; PD is model-dependent, not an observable.

6What breaks isospin, and what survives the breaking

Two culprits are known. Electromagnetism is the obvious one, since it couples to T₃ rather than to T. The subtler one is that the up and down quarks have different masses, md − mᵤ ≈ 2.5 MeV, which is why the neutron is heavier at all; lattice calculations split mₙ − mₚ = 1.293 MeV into roughly +2.3 MeV of quark-mass effect against −1.0 MeV of QED. Together they leave isospin good at the percent level, which is enough for T to stay a working label: isobaric analogue states, the Fermi operator Στ_±(i) of beta decay, and ΔT selection rules all survive. But do not read scattering lengths as a measure of the breaking. Near a pole a is hypersensitive, and the 27% spread from −17.3 to −23.74 fm comes from a 2.5% spread in well depth. A quantity that magnifies its input is a superb detector of small differences and a terrible ruler for them.

2

Key equations

Read the units, assumptions and limits before substituting.

Isospin doublet and its algebra

Tᵢ = τᵢ/2, [Tᵢ, Tⱼ] = i εᵢⱼₖ Tₖ, T₃|p⟩ = +½|p⟩, T₃|n⟩ = −½|n⟩

Every spin identity you own — ladders, Clebsch-Gordan, multiplets — transfers to charge with no new algebra to learn.

τᵢ the Pauli matrices; T is dimensionless; Q = e(T₃ + B/2) for a nucleon, B = 1

Charge independence against charge symmetry

[Hₛ, Tᵢ] = 0, i = 1, 2, 3 (CI)[Hₛ, exp(−iπT₂)] = 0 (CS only)

CS equates only pp with nn; CI adds np in the same T = 1 state, so the two are tested by different experiments.

exp(−iπT₂) is a π rotation about the 2-axis: |p⟩ → |n⟩, |n⟩ → −|p⟩

Generalised Pauli principle

(−1)(L+S+T) = −1, so L + S + T is odd

One line decides which channels exist: ³S₁ demands T = 0, ¹S₀ demands T = 1, and the ³P states are T = 1 only.

L, S, T the pair's orbital, spin and isospin quantum numbers, all integers

Deuteron binding from the mass table

B = [m(¹H) + mₙ − m(²H)]c² = 0.002388 u × 931.494 MeV/u = 2.2244 MeV

Gives the only energy the two-nucleon system has, and κ = √(B/41.47 MeV fm²) = 0.2316 fm⁻¹ with it.

Neutral atomic masses in u; one electron on each side, so they cancel exactly

Effective-range expansion

k cot δ₀ = −1/a + ½ r₀k²aₜ = +5.424 fm, aₛ = −23.74 fm

For a shallow attractive well the sign of a is the whole answer: positive means a bound state below threshold, negative means a virtual state, a pole on the unphysical sheet with no normalisable wavefunction.

k in fm⁻¹, δ₀ the S-wave phase shift, a and r₀ in fm; rₜ = 1.759 fm

Tensor operator and the S-D mixing

S₁₂ = 3(σ₁⋅r̂)(σ₂⋅r̂) − σ₁⋅σ₂⟨³S₁|S₁₂|³D₁⟩ = 2√2, ⟨³D₁|S₁₂|³D₁⟩ = −2

The only term that can put D-wave into a J = 1 state, so it alone accounts for Qd ≠ 0.

S₁₂ is dimensionless, acts only on S = 1, and commutes with J² and parity but not L²
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

21.50 MeV
14 to 36 MeV; steps of 0.25.
2.10 fm
1.8 to 2.2 fm; steps of 0.05.

Try this. Raise the depth through threshold and watch the exterior line flatten: a runs out to minus infinity and returns from plus infinity, and only then does the node at r = a walk in from the right. At R = 2.10 fm, 21.5 MeV is the unbound ¹S₀ channel and 33.75 MeV the bound ³S₁ one.

Live results

INTERIOR PHASE k₀R
1.512 rad
THRESHOLD DEPTH
23.20 MeV
SCATTERING LENGTH a
-21.5 fm
DEPTH OVER THRESHOLD
-1.70 MeV

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

Interactive Physics V modelZero-energy S-wave function u(r) above the square well that produces it, for depth 21.5 MeV and radius 2.10 fm. Inside, u is a sine of phase k₀R = 1.512 rad; outside it is a straight line whose dashed extension meets the axis at the scattering length a = -21.5 fm. Threshold depth here is 23.20 MeV.zero-energy S-wave u(r)a = −21.5 fmRV₀ = 21.5 MeV02 fm4 fm6 fm
Zero-energy S-wave function u(r) above the square well that produces it, for depth 21.5 MeV and radius 2.10 fm. Inside, u is a sine of phase k₀R = 1.512 rad; outside it is a straight line whose dashed extension meets the axis at the scattering length a = −21.5 fm. Threshold depth here is 23.20 MeV.

Predict → change one variable → check

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

Saved baseline. Well depth V₀: 21.50 MeV; Well radius R: 2.10 fm

Baseline 21.50; choose 14 to 36, in steps of 0.25.
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 usual story is that the deuteron binds because the neutron-proton force is stronger than the neutron-neutron force. It is not. Charge independence holds the T = 1 interaction equal in all three pairs to a percent or two, and the test is direct: the np ¹S₀ state, built from exactly the pair that does bind in ³S₁, is itself unbound by about 66 keV, with a = −23.74 fm against aₙₙ = −18.9 fm. The same two particles fail in one spin state and succeed in the other, so the force depends on the channel, not on the pair; what separates np from nn is channel access. L + S + T odd means an L = 0 pair with T = 1 must have S = 0, and identical nucleons are locked to T = 1; only np can reach S = 1 with T = 0, where the tensor force operates. The second half of the error is reading a = −23.74 fm as strong attraction because it is large. A large |a| says only that a pole sits close to threshold; the minus sign says which side of it.

5

Practice & worked examples

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

EasyExample 1

Neutral atomic masses are m(¹H) = 1.007825 u, mₙ = 1.008665 u and m(²H) = 2.014102 u, with 1 u = 931.494 MeV/c². Find the deuteron's binding energy and B/A, then convert B into the asymptotic decay length 1/κ of its wavefunction using ħ²/2μ = 41.47 MeV fm². Compare that length with the 1.41 fm range of one-pion exchange.

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.

MediumExample 2

Two nucleons are in a relative S or P state. (a) Write the isospin triplet and singlet and confirm their exchange symmetry with Pτ = (1 + τ₁⋅τ₂)/2. (b) Use L + S + T odd to list every allowed L = 0 and L = 1 channel. (c) Say which are open to a neutron pair, and deduce the deuteron's isospin from Jπ = 1⁺.

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.

HardExample 3

Model the S-wave np interaction as a square well of radius R = 2.1 fm, with ħ²/2μ = 41.47 MeV fm². (a) Find the depth at which the first S-wave bound state appears. (b) Find the depth reproducing B = 2.2246 MeV, and test it against the measured triplet scattering length +5.424 fm. (c) Find the depth reproducing the singlet a = −23.74 fm, and say by what margin that channel misses binding.

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

0 of 6 steps revealed.

6

Quick check

Select an answer and explain it before checking.

The np system has a bound ³S₁ state (a = +5.42 fm) and an unbound ¹S₀ state (a = −23.74 fm), built from the very same proton and neutron. A neutron pair has no bound state at all. Which account covers both facts?
7

Review & continue

Isospin is a two-valued internal label that treats the proton and the neutron as one particle, acted on by operators Tᵢ = τᵢ/2 obeying the same SU(2) algebra as spin, and approximately conserved by the strong interaction alone.

  • 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.