12.2: The Born Approximation
( \newcommand{\kernel}{\mathrm{null}\,}\)
We can use time-dependent perturbation theory to do an approximate calculation of the crosssection. Provided that the interaction between particle and scattering center is localized to the region around r=0, we can regard the incident and scattered particles as free when they are far from the scattering center. We just need the result that we obtained for a constant perturbation, Fermi’s Golden Rule, to compute the rate of transitions between the initial state (free particle of momentum p) to the final state (free particle of momentum p′).
The Hamiltonian for a single particle being scattered by a fixed potential as
ˆH=ˆH0+ˆV(r) where ˆH0=ˆp22m, the kinetic energy operator
and treat the potential energy operator, ˆV(r), as the perturbation inducing transitions between the eigenstates of ˆH0, which are plane waves.
If we label the initial and final plane-wave states Φin= exp(ik.r−iωt) and Φscat= exp(ik′.r−iω′t) by their respective wave-vectors, then Fermi’s Golden Rule for the rate of transitions is
R=2πℏ|⟨k′|ˆV|k⟩|2g(Ek)
where g(Ek) is the density of final states; g(Ek)dEk is the number of final states with energy in the range Ek→Ek+dEk.
The quantity ⟨k′|ˆV|k⟩ is known as the matrix element of the perturbation and is usually abbreviated thus
Vk′k≡⟨k′|ˆV|k⟩=∫∫∫u∗k′(r)V(r)uk(r)dτ.
The time variation has been suppressed here. For constant potential, the only non-zero terms come from ω=ω′: elastic scattering. For a time oscillating potential (e.g. V(r)sinω0t) the non-zero contribution comes from ω=ω′±ω0: inelastic scattering where the scattered particle gains/loses a quantum of energy from/to the system providing the potential.