An alpha particle sits inside the nucleus behind a Coulomb barrier built by the repulsion from the daughter's Z−2 protons. Classically it cannot escape — its energy Q is below the barrier peak — but quantum mechanically it tunnels through with a probability set by the WKB approximation (Gamow, 1928):
V(r) = 2(Z−2)e²/(4πε₀ r) Coulomb barrier outside R = r₀A^(1/3)
r_c: V(r_c) = Q classically-forbidden zone is R → r_c
G = (2/ħ)·√(2m)·∫[R,r_c] √(V(r) − Q) dr Gamow factor (WKB integral)
T = e^(−G) transmission probability per assault
f = v/(2R), v = √(2Q/m) assault frequency on the barrier wall
λ = f·T, T₁/₂ = ln(2)/λ decay constant → half-life
This two-parameter model (Z, Q — with R fixed by A) reproduces the real half-life range correctly to within a few orders of magnitude across 30+ orders of magnitude of half-lives, from Po-212's 0.3 μs to U-238's 4.5 billion years — the entire spread comes from Q sitting inside an exponential. Real values also depend on nuclear-structure corrections (spin, parity, preformation factor) this simplified model omits.
Escape animation: attempts are shown on a fixed demo clock (not the real assault frequency f, which is ~10²¹ Hz — far too fast to render). The escape/reflect outcome of each shown attempt is drawn from a probability rescaled from the real Gamow factor G, so a thinner barrier (lower G) still escapes more often here, just as it would in reality — only the timescale is compressed to be watchable.