Playground

Adjust A and Z to see the five SEMF terms compete: volume, surface, Coulomb, asymmetry, and pairing.

Variables

SymbolNameSIDimensionRange
BBBinding energyoutput
Total nuclear binding energy
JM·L²·T⁻²0 – 1e-9
AAMass number
Total number of nucleons
111 – 300
ZZAtomic number
Number of protons
111 – 120
aVa_VVolume coefficient
Volume term coefficient
MeVM·L²·T⁻²15 – 16
aSa_SSurface coefficient
Surface term coefficient
MeVM·L²·T⁻²17 – 19
aCa_CCoulomb coefficient
Coulomb repulsion term coefficient
MeVM·L²·T⁻²0.6 – 0.8
aAa_AAsymmetry coefficient
Proton-neutron asymmetry coefficient
MeVM·L²·T⁻²22 – 24

Deep dive

Derivation
Treat the nucleus as a charged liquid drop. Volume term (a_V·A): each nucleon interacts with nearest neighbors via the strong force, giving energy proportional to A. Surface term (−a_S·A^{2/3}): nucleons at the surface have fewer neighbors, reducing binding. Coulomb term (−a_C·Z²/A^{1/3}): proton-proton electrostatic repulsion scales as Z² divided by nuclear radius ∝ A^{1/3}. Asymmetry term (−a_A·(A−2Z)²/A): the Pauli exclusion principle penalizes unequal proton/neutron numbers. Pairing term (δ): empirical correction favoring even-even nuclei.
Experimental verification
Aston's mass spectrograph (1920s) first showed systematic mass defects. Modern atomic mass evaluations (AME2020) provide masses of ~3400 nuclides. The SEMF reproduces these to within ~1% for A > 20, confirming the liquid drop picture. Deviations at magic numbers led to the nuclear shell model.
Common misconceptions
  • The formula does NOT predict magic numbers — these require the shell model.
  • The pairing term δ is NOT simply +δ for even-even; it depends on whether A is odd or even, and the sign convention varies by textbook.
  • The coefficients are NOT universal constants — they are fitted to experimental data and vary slightly between different fitting sets.
Real-world applications
  • Predicting nuclear stability and drip lines
  • Estimating fission barrier heights
  • Nucleosynthesis calculations in stellar evolution
  • Nuclear reactor fuel cycle analysis

Worked examples

Binding energy of ⁵⁶Fe (Z=26, A=56)

Given:
A:
56
Z:
26
a_V:
15.8
a_S:
18.3
a_C:
0.714
a_A:
23.2
δ:
0
Find: B
Solution

B ≈ 493.4 MeV → B/A ≈ 8.81 MeV/nucleon

Binding energy of ²³⁸U (Z=92, A=238)

Given:
A:
238
Z:
92
a_V:
15.8
a_S:
18.3
a_C:
0.714
a_A:
23.2
δ:
+0.78
Find: B
Solution

B ≈ 1802 MeV → B/A ≈ 7.57 MeV/nucleon

Scenarios

What if…
  • scenario:
    What if we ignore the Coulomb term?
    answer:
    Binding energy would increase monotonically with A, and there would be no upper limit on nuclear size. The Coulomb term is what makes superheavy nuclei unstable and drives fission.
  • scenario:
    What if N ≠ Z for a light nucleus?
    answer:
    The asymmetry term penalizes the imbalance. For example, ¹⁴C (Z=6, N=8) has a lower binding energy than ¹⁴N (Z=7, N=7) partly due to this term, making ¹⁴C radioactive.
  • scenario:
    What if a nucleus sits at a magic number?
    answer:
    Shell closures add extra binding not captured by the SEMF. For example, ²⁰⁸Pb (Z=82, N=126 — doubly magic) has ~10 MeV more binding than the SEMF predicts.
Limiting cases
  • condition:
    A → large, Z ≈ A/2
    result:
    B/A peaks near A ≈ 56 then decreases
    explanation:
    The Coulomb term grows faster than the volume term for large A, reducing binding energy per nucleon and making heavy nuclei less stable.
  • condition:
    Z = A/2 (symmetric nuclei)
    result:
    Asymmetry term vanishes
    explanation:
    When proton and neutron numbers are equal, the (A−2Z)² term is zero, maximizing binding for light nuclei.
  • condition:
    A → small
    result:
    Surface term dominates over volume
    explanation:
    Small nuclei have a large surface-to-volume ratio, so the negative surface correction significantly reduces binding energy per nucleon.

Context

Carl von Weizsäcker & Hans Bethe · 1935

Weizsäcker proposed the liquid drop model for nuclear masses; Bethe refined it, producing a formula that predicts binding energies across the chart of nuclides.

Hook

Why is iron-56 the end of the line for stellar fusion?

Estimate the binding energy of ⁵⁶Fe (Z=26, A=56) using the SEMF.

Dimensions:
lhs:
B → [Energy] = MeV
rhs:
a_V·A → [MeV]·[1] = [MeV]; a_S·A^{2/3} → [MeV]; a_C·Z²/A^{1/3} → [MeV]·[1]/[1] = [MeV]; a_A·(A−2Z)²/A → [MeV]
check:
All terms have dimensions of [Energy] = MeV. ✓
Validity: Valid for nuclei with A ≳ 12 (breaks down for very light nuclei where shell effects dominate). Accuracy is ~1% for most nuclei but deviates near magic numbers (2, 8, 20, 28, 50, 82, 126). The pairing term δ(A,Z) requires separate treatment for even-even, odd-odd, and odd-A nuclei.

Related formulas