5.4 Barrier penetration

In order to understand quantum mechanical tunnelling in fission it makes sense to look at the simplest fission process: the emission of a He nucleus, so called α radiation. The picture is as in Fig. 5.12.


alpha˙decay


Figure 5.12: The potential energy for alpha decay

Suppose there exists an α particle inside a nucleus at an (unbound) energy > 0. Since it isn’t bound, why doesn’t it decay immediately? This must be tunnelling. In the sketch above we have once again shown the nuclear binding potential as a square well, but we have included the Coulomb tail,

V Coulomb(r) = (Z 2)2e2 4π𝜖0r . (5.20)

. The height of the barrier is exactly the coulomb potential at the boundary, which is the nuclear radius, RC = 1.2A1.3 fm, and thus BC = 2.4(Z 2)A13. The decay probability across a barrier can be given by the simple integral expression P = e2γ, with

γ = (2μα)12 RCb[V (r) E α]12dr = (2μα)12 RCb 2(Z 2)e2 4π𝜖0r Eα 12dr = 2(Z 2)e2 2π𝜖0v arccos(EαBC) (EαBC)(1 EαBC), (5.21)

(here v is the velocity associated with Eα). In the limit that BC Eα we find

P = exp 2(Z 2)e2 2𝜖0v . (5.22)

This shows how sensitive the probability is to Z and v!