β⁻ Decay: Electron Spectrum

In β⁻ decay a nucleus emits an electron and an electron antineutrino, sharing energy and momentum with the recoiling daughter. For an allowed transition the electron kinetic-energy spectrum is continuous from zero up to an endpoint Q (the maximum electron kinetic energy when the antineutrino carries essentially none). A standard Fermi “golden rule” phase-space cartoon gives dΓ/dE ∝ p (Q − E)² with relativistic electron momentum p(E) = √(E² + 2 m_e c² E). Coulomb distortion F(Z,E) near the nucleus is omitted here, so the curve is schematic but shows the key qualitative shape: rising from threshold, peaking, then falling to zero at E = Q. The mean kinetic energy ⟨E⟩ for the displayed shape is shown for comparison when you change Q.

Who it's for: Modern physics and introductory nuclear physics courses discussing neutrinos, lepton number, and kinematics of three-body decay.

Key terms

  • Beta Decay
  • Fermi Golden Rule
  • Endpoint Energy
  • Antineutrino
  • Continuous Spectrum

How it works

Electron kinetic-energy spectrum in β⁻ decay is continuous up to an endpoint Q: the antineutrino carries the missing energy and momentum — Pauli’s 1930 hypothesis, confirmed by experiment.

Frequently asked questions

Why is the spectrum not symmetric around Q/2?
The (Q − E)² factor favors lower electron energies because more phase space opens when the light antineutrino takes more energy; the electron momentum factor p(E) also shapes the low-energy rise. Real nuclei add a Coulomb correction that modifies the low-energy end.