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6.11. More Details on Scattering and Structure 177<br />

is built up from delta functions, δ(r ′ ), each with a weight (2m/� 2 )V (r ′ )ψ(r ′ )so<br />

that<br />

ψs(r) = 2m<br />

� 2<br />

�<br />

d 3 r ′ G(r,r ′ )V (r ′ )ψ(r ′ ), (6.85)<br />

where G(r,r ′ ) is the Green’s function for a delta function potential, Eq. (6.80). The<br />

appropriate solution of the homogeneous Schrödinger equation describes a particle<br />

that impinges on the target along the z axis; the general solution is therefore<br />

ψ(r) =e ikz + 2m<br />

� 2<br />

�<br />

d 3 r ′ G(r,r ′ )V (r ′ )ψ(r ′ ). (6.86)<br />

The original Schrödinger differential equation for the wave function ψ has been<br />

transformed into an integral equation, called the scattering integral equation. For<br />

many problems, it is more convenient to start from such an integral equation rather<br />

than from the differential equation.<br />

In scattering experiments, the incident beam is prepared far outside the scattering<br />

potential, and the scattered particles are also analyzed and detected far away.<br />

The detailed form of the wave function inside the scattering region is consequently<br />

not investigated, and what is needed is the asymptotic form of the scattered wave,<br />

ψs(x). With ˆr = r/r and k = kˆr, asindicatedinFig.6.26,|r − r ′ | becomes<br />

|r − r ′ �<br />

2r · r′<br />

| = r 1 −<br />

r2 r′2<br />

+<br />

r2 �1/2<br />

and the Green’s function takes on the asymptotic value<br />

G(r,r ′ ) ∼<br />

r→∞<br />

−→ r − ˆr · r′<br />

r→∞<br />

(6.87)<br />

−1 exp(ikr)<br />

exp(−ik · r<br />

4π r<br />

′ ). (6.88)<br />

Inserting G(r,r ′ ) into Eq. (6.85) and comparing with Eq. (6.76) yields the expression<br />

for the scattering amplitude,<br />

f(θ, ϕ) = −m<br />

2π�2 �<br />

d 3 r ′ e ik·r′<br />

V (r ′ )ψ(r ′ ).• (6.89)<br />

The First Born Approximation The first Born approximation corresponds to<br />

the case of a weak interaction. If the interaction were negligible, the scattering<br />

amplitude would vanish and ψ(r ′ ) would be given by exp(ikz ′ ) ≡ exp(ik0 · r ′ ). As<br />

a first approximation, this value of the wave function is inserted in Eq. (6.89), with<br />

the result<br />

f(θ, ϕ) = −m<br />

2π�2 �<br />

d 3 r ′ V (r ′ )exp(iq · r ′ /�), (6.90)

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