Alpha Decay Fundamentals

Alpha decay is the emission of a helium-4 nucleus ($^4_2$He or alpha particle) from an unstable parent nucleus. It is the dominant decay mode for heavy nuclei with $Z > 82$:

$$^A_Z X \to ^{A-4}_{Z-2} Y + ^4_2\text{He}$$

The Q-value (kinetic energy released) is:

$$Q_\alpha = [M(A,Z) - M(A-4, Z-2) - M(^4\text{He})]c^2$$

Alpha decay is energetically possible when $Q_\alpha > 0$. The alpha particle carries most of the kinetic energy due to momentum conservation:

$$T_\alpha = Q_\alpha \frac{A - 4}{A}$$

The Geiger-Nuttall Law

Geiger and Nuttall (1911) empirically discovered that alpha-decay half-lives span an enormous range (from nanoseconds to billions of years) but correlate strongly with the decay energy:

$$\log_{10} t_{1/2} = a + \frac{b}{\sqrt{Q_\alpha}}$$

where $a$ and $b$ are constants that depend on the parent nucleus charge. A change in $Q_\alpha$ by a factor of 2 can change the half-life by 20 orders of magnitude! This extraordinary sensitivity is explained by quantum tunneling.

Gamow Theory of Alpha Decay

George Gamow (1928) provided the first successful quantum mechanical explanation of alpha decay using the WKB approximation for tunneling through the Coulomb barrier.

The Coulomb Barrier

Inside the nucleus ($r < R$), the alpha particle is bound by the nuclear potential. Outside, it sees the repulsive Coulomb barrier:

$$V(r) = \frac{2(Z-2)e^2}{4\pi\epsilon_0 r} = \frac{2(Z-2) \times 1.44 \text{ MeV}\cdot\text{fm}}{r} \quad \text{for } r > R$$

The barrier height at the nuclear surface is typically 25-30 MeV, while the alpha particle energy is only 4-9 MeV. Classically, escape is impossible.

WKB Tunneling Probability

The tunneling probability through the barrier using the WKB approximation is:

$$T = \exp\left(-\frac{2}{\hbar}\int_R^{r_{\text{tp}}} \sqrt{2\mu[V(r) - Q_\alpha]}\,dr\right)$$

where $r_{\text{tp}} = 2(Z-2)e^2/(4\pi\epsilon_0 Q_\alpha)$ is the classical turning point and $\mu$ is the reduced mass. Evaluating the integral analytically:

$$T = \exp\left(-\frac{2}{\hbar}\sqrt{2\mu Q_\alpha}\,r_{\text{tp}}\left[\arccos\sqrt{\rho} - \sqrt{\rho(1-\rho)}\right]\right)$$

where $\rho = R/r_{\text{tp}}$. The decay rate is then:

$$\lambda = f \cdot T, \quad f = \frac{v}{2R} \sim 10^{21} \text{ s}^{-1}$$

where $f$ is the assault frequency (how often the alpha particle hits the barrier).

Python Simulation: Gamow Tunneling

Calculates the Gamow tunneling probability and resulting half-lives as a function of alpha decay energy, demonstrating the Geiger-Nuttall relationship.

Gamow Tunneling Probability

Python

Tunneling probability and half-life vs alpha-decay energy for Z=82 daughter

script.py110 lines

Click Run to execute the Python code

Code will be executed with Python 3 on the server

Fortran Implementation

Calculates alpha-decay half-lives for specific nuclei using the Gamow tunneling formula.

Alpha Decay Half-Life Calculator

Fortran

Computes Gamow tunneling half-lives for various alpha-emitting nuclei

alpha_decay_halflife.f9073 lines

Click Run to execute the Fortran code

Code will be compiled with gfortran and executed on the server