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Nuclear, particle & quantum-information sequence · Interactive lesson

Nuclear radius from the charge form factor

Electron scattering is the cleanest ruler physics has for the nucleus: a structureless probe, an interaction we can write down exactly, first-order perturbation theory good enough to use. This lesson is about what that ruler hands back — a squared modulus over a finite range of q — and how much of the density survives the trip home.

UPV-14.02 · Lesson 2 of 9 in this unit. Position is not a completion score.
Starting model: Nuclear radius from the charge form factorLog plot of |F(q)|² against momentum transfer q for a uniform sphere of half-density radius c = 6.60 fm folded with a Gaussian surface of width σ = 0.90 fm. This σ is not the Fermi diffuseness a: the same 90-to-10 thickness t needs σ = 1.71a, so a = 0.55 fm corresponds to σ ≈ 0.94 fm. Zeros stand where qc = 4.49, 7.73, 10.90, so the first is at q₁ = 0.68 per fm and the open circle marks it on the axis. The dashed vertical line is the cutoff q_max = 3.0 per fm, beyond which nothing is measured.|F(q)|² = [3 j₁(qc)/(qc)]² exp(−q²σ²)q₁c = 6.60 fm σ = 0.90 fmπ/qmax = 1.05 fm110⁻²10⁻⁴10⁻⁶q (fm⁻¹) 0 to 3cutoff qmax = 3.0 /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

You measure |F(q)|². You want F(q). Everything hard here follows from that.

The key idea

The charge form factor F(q) is the normalised Fourier transform of a nucleus's charge density, defined so that the elastic electron cross-section is the point-charge Mott cross-section multiplied by |F(q)|², with F(0) = 1.

Example. For ¹²C at 200 MeV and θ = 20°, q = 2E sin(θ/2)/ħc = 0.352 fm⁻¹, and a measured ratio to Mott of 0.778 gives F = 0.882 — a 12% dip below unity that the low-q expansion turns into a radius of about 2.4 fm.

The complete physical model and assumptions

Accelerate electrons until their reduced wavelength is smaller than a nucleus and the first Born approximation applies: the amplitude is the point-charge amplitude times the normalised Fourier transform of the charge distribution, so the measured cross-section is the point-charge Mott cross-section times |F(q)|², with F that transform sampled at momentum transfer q = 2k sin(θ/2). Sweep the angle, sweep q, and you are reading off the transform of ρch. That is the promise. The bill arrives in three parts. A detector counts rates, so what is recorded is |F|² and never F — for a real spherical density F is real and flips sign at every diffraction zero, and those signs are not measured. The beam energy caps q at qₘₐₓ = 2E/ħc, so the transform is truncated and structure finer than about π/qₘₐₓ is simply absent. And the Born approximation itself fails for heavy nuclei, where the electron is pulled tens of MeV deeper before it scatters. What comes out is therefore never the density but a fitted shape — a two-parameter Fermi profile, or a Fourier–Bessel series carrying a stated incompleteness band — from which a half-density radius near 1.1 A¹⁄³ fm, a surface thickness near 2.4 fm and a saturated interior near 0.16 nucleons per fm³ follow. Only one length escapes the convention: the rms radius, which the slope of F at q → 0 pins down whatever shape ρ has.

1Divide by Mott before you interpret anything

The electron is the right probe because it has no strong interaction and no structure of its own, so the whole vertex is electromagnetic and one order of perturbation theory is enough. In the first Born approximation the amplitude is the Fourier transform of the potential, so for a static charge distribution the cross-section factorises: dσ/dΩ = (dσ/dΩ)Mott |F(q)|². The Mott factor is the point-charge answer — Rutherford, with the relativistic spin factor cos²(θ/2) and a recoil denominator — and it holds no nuclear structure whatever. Everything the nucleus contributes lives in |F(q)|². So the first operation on any data set is a division: plot measured cross-section over Mott and you have |F|² on a scale where F(0) = 1 by construction. Nothing has yet been assumed about ρ beyond a static, spherical source.

2The variable is q, and the beam energy caps it

Angle is what the apparatus turns; q is what the physics depends on. For an ultrarelativistic electron k = E/ħc, and elastic scattering through θ transfers q = 2k sin(θ/2), so with ħc = 197.33 MeV fm a 200 MeV beam at 20° gives q = 0.352 fm⁻¹. Two consequences follow. The reach is largest at backscattering, qₘₐₓ = 2E/ħc: 2.03 fm⁻¹ at 200 MeV, 5.07 fm⁻¹ at 500 MeV. And a truncated transform cannot resolve structure finer than roughly δr ≈ π/qₘₐₓ — 1.55 fm at 200 MeV, 0.62 fm at 500 MeV. That is why radius work is done at several hundred MeV and above: run it lower and you are measuring a blurred nucleus, and no fitting procedure invents detail the kinematics never delivered.

3Two reads of a radius, answering different questions

Expand the transform at small q: F(q) = 1 − q²⟨r²⟩/6 + q⁴⟨r⁴⟩/120 − …, a series in q², so ⟨r²⟩ = −6 dF/d(q²) at q = 0 is model-independent — the slope is the radius whatever shape ρ has. That is the number quoted as the rms charge radius: 2.470 fm for ¹²C, 5.501 fm for ²⁰⁸Pb, and it carries no convention at all. The second read is the diffraction pattern. A uniform sphere has F = 3[sin(qR) − qR cos(qR)]/(qR)³, vanishing at qR = 4.4934, so the first minimum gives R = 4.4934/q₁ from angles alone. For ²⁰⁸Pb at 250 MeV, once Coulomb distortion is corrected for, that minimum sits at θ = 30.5°, q₁ = 0.667 fm⁻¹, hence R = 6.74 fm and √(3/5)R = 5.22 fm — 5% short of 5.50. The reads disagree because the second assumed a shape and the first did not.

4The phase problem, and what a fit is really doing

A detector counts rates, so the measurement is |F(q)|², while for a real spherical density F is real and changes sign at every zero. Those signs are supplied by the model, not by the experiment. Add truncation at qₘₐₓ and the inversion is ill-posed twice over: densities whose transforms agree below qₘₐₓ and differ above it fit the data identically, and so do densities whose transforms differ by a sign flip on one lobe. Practice takes one of two routes. Fit a shape with few parameters — the two-parameter Fermi profile — and quote c and a with their covariance, accepting the shape as an assumption. Or expand ρ in a Fourier–Bessel series inside a fixed cutoff radius, fit the coefficients qₘₐₓ supports, and bound the unmeasured tail, quoting the resulting incompleteness error as a band around ρ(r). Both are honest. Neither is an inversion.

5Saturation, and why two radii give two densities

Fit the Fermi profile across the chart and c comes out near 1.1 A¹⁄³ fm with a near 0.55 fm, so the 90-to-10 surface thickness t = 4a ln3 ≈ 2.4 fm hardly changes from carbon to lead: nuclear matter saturates, and the interior density is close to A-independent. But the number you quote for that interior depends on which radius convention you used, and the two in common use are different lengths. For ²⁰⁸Pb the Fermi fit c = 6.60 fm, a = 0.55 fm gives ρ₀ = 3A/(4πc³[1 + (πa/c)²]) = 0.162 nucleons fm⁻³. The sharp-sphere convention R = 1.2 A¹⁄³ fm = 7.11 fm reproduces the same rms radius (√0.6 × 7.11 = 5.51 fm) but spreads 208 nucleons through a bigger volume: 0.138 fm⁻³, 15% lower. Each is right inside its own definition; taking c from one and a density from the other is not.

6Where plane waves fail: Coulomb distortion

The Born approximation treats both electron waves as plane waves, which needs Zα ≪ 1. For lead Zα = 82/137 = 0.60, and the failure is quantitative, not cosmetic. An electron at the centre of a uniformly charged sphere sits 3Zαħc/2R ≈ 24.9 MeV deeper than at infinity, so its local wavenumber inside exceeds the asymptotic k — a 10% effect at 250 MeV, 5% at 500 MeV. The diffraction minima therefore appear at smaller angles than plane-wave Born predicts, and such a fit reads the radius about 10% high: 0.7 fm on 7.1 fm, against data good to thousandths of a femtometre. Distortion also partly fills the minima, so they stop being true zeros. The cure is to stop approximating — solve the Dirac equation for the electron in the electrostatic potential of the extended nuclear charge, do a phase-shift analysis, and adjust ρ until the computed cross-section matches.

2

Key equations

Read the units, assumptions and limits before substituting.

Born cross-section, structure factored out

dσ/dΩ = (dσ/dΩ)Mott |F(q)|²

Divide the data by Mott and every nuclear property left in the plot sits inside |F|².

Mott carries the point charge Ze, the spin factor cos²(θ/2) and recoil, in mb/sr

Momentum transfer set by the angle

q = 2k sin(θ/2) with k = E/ħc

200 MeV at 20° is q = 0.352 fm⁻¹; the resolvable detail is δr ≈ π/qₘₐₓ, 1.55 fm at 200 MeV.

ħc = 197.33 MeV fm, so E in MeV gives q in fm⁻¹, and qₘₐₓ = 2E/ħc at backscattering

Form factor of a spherical density

F(q) = (4π/(Ze⋅q)) ∫₀^∞ r ρch(r) sin(qr) dr

One sine transform in one variable — invertible in principle, if you had F over all q with its signs.

ρch in e fm⁻³ normalised to ∫ρch d³r = Ze, so F(0) = 1, with q in fm⁻¹

Low-q slope gives the rms radius

F(q) = 1 − q²⟨r²⟩/6 + q⁴⟨r⁴⟩/120 − …⟨r²⟩ = −6 dF/d(q²) at q = 0

The one model-independent length in the topic: no shape is assumed to get it.

⟨r²⟩ in fm², and the series is usable only while q²⟨r²⟩ stays well below 6

Uniform sphere and its diffraction zeros

F(q) = 3[sin(qR) − qR cos(qR)]/(qR)³zeros at qR = 4.4934, 7.7253, 10.9041

The minima locate R from angles alone — no absolute normalisation of the beam is needed.

⟨r²⟩ = 3R²/5, and the convention R = 1.2 A¹⁄³ fm is tuned to reproduce measured ⟨r²⟩

Two-parameter Fermi profile

ρ(r) = ρ₀/(1 + exp[(r − c)/a])t = 4a ln3

Two numbers fit almost every measured nucleus — and hide the model dependence inside a choice of shape.

c ≈ 1.1 A¹⁄³ fm, a ≈ 0.55 fm, t ≈ 2.4 fm, ρ₀ ≈ 0.16 nucleons fm⁻³
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

6.6 fm
2 to 8 fm; steps of 0.1.
0.90 fm
0.1 to 1.2 fm; steps of 0.05.
3.0 fm⁻¹
1 to 3 fm⁻¹; steps of 0.1.

Try this. Drag c and every minimum slides together — their spacing measures the radius and nothing else. Then drag σ: the minima stay put while the envelope tilts, which is how surface thickness is read. Pull qₘₐₓ left and count the lobes you lose.

Live results

FIRST ZERO q1
0.681 fm⁻¹
RMS RADIUS (model)
5.34 fm
SURFACE 90-10 t
2.31 fm
DETAIL LIMIT π/qmax
1.05 fm

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

Interactive Physics V modelLog plot of |F(q)|² against momentum transfer q for a uniform sphere of half-density radius c = 6.60 fm folded with a Gaussian surface of width σ = 0.90 fm. This σ is not the Fermi diffuseness a: the same 90-to-10 thickness t needs σ = 1.71a, so a = 0.55 fm corresponds to σ ≈ 0.94 fm. Zeros stand where qc = 4.49, 7.73, 10.90, so the first is at q₁ = 0.68 per fm and the open circle marks it on the axis. The dashed vertical line is the cutoff q_max = 3.0 per fm, beyond which nothing is measured.|F(q)|² = [3 j₁(qc)/(qc)]² exp(−q²σ²)q₁c = 6.60 fm σ = 0.90 fmπ/qmax = 1.05 fm110⁻²10⁻⁴10⁻⁶q (fm⁻¹) 0 to 3cutoff qmax = 3.0 /fm
Log plot of |F(q)|² against momentum transfer q for a uniform sphere of half-density radius c = 6.60 fm folded with a Gaussian surface of width σ = 0.90 fm. This σ is not the Fermi diffuseness a: the same 90-to-10 thickness t needs σ = 1.71a, so a = 0.55 fm corresponds to σ ≈ 0.94 fm. Zeros stand where qc = 4.49, 7.73, 10.90, so the first is at q₁ = 0.68 per fm and the open circle marks it on the axis. The dashed vertical line is the cutoff qₘₐₓ = 3.0 per fm, beyond which nothing is measured.

Predict → change one variable → check

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

Saved baseline. Half-density radius c: 6.6 fm; Gaussian surface width σ: 0.90 fm; Data cutoff qₘₐₓ: 3.0 fm⁻¹

Baseline 6.6; choose 2 to 8, 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 tempting move is to Fourier-transform the measured curve and call the result the charge density. It cannot be done, and not because the arithmetic is hard. What is measured is |F(q)|², so the sign F carries between successive zeros is missing, and the transform needs it. A finite beam energy also stops the data at qₘₐₓ, so the tail is missing too. Two densities whose form factors differ only above qₘₐₓ, or by a sign flip on one lobe, reproduce the same data exactly — which is why every published nuclear density is a fitted shape with a stated model or incompleteness error. The quieter version of the same error is quoting R = 1.2 A¹⁄³ fm as the nuclear radius and then dividing A by (4/3)πR³. That convention is tuned to reproduce ⟨r²⟩, and it returns 0.138 nucleons fm⁻³ for lead, where the half-density radius convention returns 0.162. Two conventions, not one measurement.

5

Practice & worked examples

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

EasyExample 1

Elastic scattering of 200 MeV electrons from ¹²C at θ = 20° gives a cross-section 0.778 times the Mott value. Take ħc = 197.33 MeV fm. Find the momentum transfer, the form factor, and the rms charge radius from the leading term of the low-q expansion — then say what that truncation costs.

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

Elastic scattering of 250 MeV electrons from ²⁰⁸Pb, once corrected for Coulomb distortion, puts the first minimum of |F(q)|² at θ = 30.5°. Read a sharp-sphere radius from it and convert to an rms radius. Compare with the accepted 5.501 fm and with the convention R = 1.2 A¹⁄³ fm, and decide whether one sharp sphere can satisfy both.

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

For ²⁰⁸Pb a two-parameter Fermi fit gives c = 6.60 fm and a = 0.55 fm. (a) Find the central density ρ₀ in nucleons fm⁻³. (b) Find the density implied instead by R = 1.2 A¹⁄³ fm and account for the difference. (c) Estimate how badly a plane-wave analysis of a 250 MeV measurement would misread the radius, and name the fix.

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.

A measurement on ²⁰⁸Pb reaches qₘₐₓ = 2.0 fm⁻¹ and resolves three diffraction minima. The beam energy is doubled, qₘₐₓ reaches 4.0 fm⁻¹, and four more minima appear. What does the extra data most directly buy?
7

Review & continue

The charge form factor F(q) is the normalised Fourier transform of a nucleus's charge density, defined so that the elastic electron cross-section is the point-charge Mott cross-section multiplied by |F(q)|², with F(0) = 1.

  • 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.