Beta decay is the transformation of a neutron into a proton (or vice versa) via the weak nuclear force, accompanied by emission of an electron (or positron) and an antineutrino (or neutrino). The Q-value (energy available) is shared among the products in a continuous spectrum, with the antineutrino carrying away a variable amount. This was historically puzzling until the neutrino was hypothesized to explain the missing energy.
Identify the Q-value from initial and final nuclear masses. Understand that the continuous energy spectrum of electrons arises from variable antineutrino carries-off. Distinguish between beta-minus (n → p), beta-plus (p → n), and electron capture decay modes.
Not all the Q-value goes to the electron (it shares energy with the neutrino, producing the continuous spectrum). Electron capture does not emit an electron; rather, the nucleus absorbs an inner-shell electron and emits a neutrino. The weak force acts on flavor-changing quark transitions, a concept beyond classical nuclear models.
From your study of radioactive decay, you know that unstable nuclei release energy by transforming into more stable configurations. In alpha and gamma decay, the energy available — the Q-value — goes into kinetic energy of the products in a well-defined way: because only two bodies emerge (the alpha particle and the daughter nucleus, or the gamma photon and the recoiling nucleus), conservation of energy and momentum dictate a unique energy for each product. Alpha particles from a given isotope are emitted with a single discrete energy. This discreteness was considered a universal feature of radioactive decay — until beta decay experiments revealed something deeply puzzling.
When physicists measured the energy of electrons emitted in beta-minus decay (n → p + e⁻ + ν̄_e), they found not a discrete line but a continuous spectrum: electrons emerged with energies ranging from near zero up to a maximum Q-value. The Q-value is calculated from the mass difference between the initial and final nuclei using mass-energy equivalence: Q = (M_parent − M_daughter − m_e)c². If only the electron and the daughter nucleus were produced, energy conservation would demand a unique electron energy just as in alpha decay. The continuous spectrum seemed to imply that energy was not conserved — a crisis serious enough that Niels Bohr temporarily proposed abandoning conservation of energy in nuclear processes.
In 1930, Wolfgang Pauli proposed a bold resolution: a third particle — he called it the neutrino (small neutral one) — is produced alongside the electron, and the two share the Q-value between them in continuously variable proportions. Because the neutrino is nearly massless and interacts extremely weakly with matter (so weakly it escaped detection in Pauli's time), it carries away the "missing" energy unobserved. The electron spectrum has a continuous shape precisely because the energy split between electron and neutrino is probabilistic, with the maximum electron energy corresponding to a neutrino carrying away near-zero energy. Fermi formalized this into a quantitative theory in 1934; the neutrino was not directly detected until 1956.
The three modes of beta decay differ in which particle is emitted and the underlying nuclear transformation. Beta-minus decay (the common form) converts a neutron to a proton and emits an electron and an electron antineutrino: n → p + e⁻ + ν̄_e. Beta-plus decay converts a proton to a neutron and emits a positron and an electron neutrino: p → n + e⁺ + ν_e; this can only occur when the Q-value exceeds 2m_ec² (≈ 1.02 MeV) because the positron mass must be created. Electron capture is a competing process to beta-plus: the nucleus absorbs an inner-shell electron and emits a neutrino (p + e⁻ → n + ν_e), without producing a positron. In all three modes, a neutrino or antineutrino carries away a portion of the Q-value, producing the characteristic continuous spectrum — a clean experimental signature of the three-body final state that vindicated Pauli's hypothesis.
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