Beta Decay Processes

Beta decay involves the transformation of a neutron into a proton (or vice versa) inside the nucleus, mediated by the weak interaction. There are three types:

$\beta^-$ Decay

$$n \to p + e^- + \bar{\nu}_e$$

Neutron-rich nuclei. Emits electron and antineutrino.

$\beta^+$ Decay

$$p \to n + e^+ + \nu_e$$

Proton-rich nuclei. Emits positron and neutrino.

Electron Capture

$$p + e^- \to n + \nu_e$$

Captures orbital electron. Competes with $\beta^+$.

Fermi Theory of Beta Decay

Enrico Fermi (1934) developed the first successful theory of beta decay, treating it as a four-fermion point interaction. The transition rate is given by Fermi's Golden Rule:

$$\lambda = \frac{2\pi}{\hbar}|M_{fi}|^2 \rho(E_f)$$

Beta Spectrum Shape

The electron energy spectrum for allowed $\beta^-$ decay is:

$$N(T_e) \propto F(Z', E_e)\,p_e\,E_e\,(Q - T_e)^2$$

where $T_e$ is the electron kinetic energy, $E_e = T_e + m_e c^2$ is the total energy, $p_e = \sqrt{E_e^2 - m_e^2 c^4}/c$ is the momentum, and $F(Z', E_e)$ is the Fermi function that accounts for the Coulomb interaction between the emitted electron and the daughter nucleus.

The Kurie Plot

The Kurie (or Fermi-Kurie) plot is a powerful tool for analyzing beta spectra. Defining the Kurie function:

$$K(T_e) = \sqrt{\frac{N(T_e)}{F(Z', E_e)\,p_e\,E_e}} \propto (Q - T_e)$$

For allowed transitions, this is a straight line that intercepts the energy axis at $T_e = Q$. Deviations from linearity indicate forbidden transitions or a non-zero neutrino mass.

ft Values and Selection Rules

The comparative half-life (ft value) removes kinematic factors:

$$ft_{1/2} = \frac{K}{g^2|M_{fi}|^2}$$

where K is a known constant. The ft value depends only on the nuclear matrix element:

  • - Superallowed: $\log ft \approx 3.5$ (e.g., $^{14}$O $\to$ $^{14}$N)
  • - Allowed: $\log ft \approx 4-7$ ($\Delta J = 0, \pm 1$, no parity change)
  • - First forbidden: $\log ft \approx 6-9$ ($\Delta J = 0, \pm 1, \pm 2$, parity change)
  • - Second forbidden: $\log ft \approx 10-13$

Connection to Neutrino Physics

Beta decay is intimately connected to neutrino physics. The continuous electron energy spectrum was the key evidence that led Pauli to postulate the neutrino (1930). Modern beta-decay experiments probe:

  • - Neutrino mass: The endpoint of the tritium beta spectrum is sensitive to $m_{\nu_e}$. The KATRIN experiment constrains $m_{\nu_e} < 0.45$ eV.
  • - Double beta decay: Neutrinoless double beta decay ($0\nu\beta\beta$) would prove neutrinos are Majorana particles.
  • - CKM matrix: Superallowed $0^+ \to 0^+$ beta decays provide the most precise determination of $V_{ud}$.

Python Simulation: Beta Spectrum & Kurie Plot

Computes the Fermi theory beta-decay electron spectra for several nuclei and demonstrates the Kurie plot analysis technique.

Beta Decay Spectrum and Kurie Plot

Python

Fermi theory prediction for beta-minus spectra of tritium, Co-60, and P-32

script.py115 lines

Click Run to execute the Python code

Code will be executed with Python 3 on the server

Fortran Implementation

Calculates the Fermi function and ft values for beta-decay transitions.

Fermi Function and ft Values

Fortran

Computes statistical rate function f and comparative half-lives for beta decays

fermi_ft_values.f9071 lines

Click Run to execute the Fortran code

Code will be compiled with gfortran and executed on the server