130_notes.dvi

(Frankie) #1
= Z 1 Z 2 e^2

2 π
−i∆

[


e−(

(^1) a+i∆)r
1
a+i∆


+

e−(

(^1) a−i∆)r
1
a−i∆


]∞

0
= Z 1 Z 2 e^2

2 π
−i∆

[

1

1
a+i∆


1

1
a−i∆

]

= Z 1 Z 2 e^2

2 π
−i∆

[ 1

a−i∆−

1
a−i∆
1
a^2 + ∆
2

]

= Z 1 Z 2 e^2

2 π
−i∆

[

− 2 i∆
1
a^2 + ∆

2

]

=

4 πZ 1 Z 2 e^2
1
a^2 + ∆
2

Since∆ =~ ~kf−~ki, we have ∆^2 =k^2 f+ki^2 − 2 kfkicosθ. For elastic scattering, ∆^2 = 2k^2 (1−cosθ).
The differential cross section is



dΩ

=

μ^2
4 π^2 ̄h^4



∣V ̃(∆)~




2

=

μ^2
4 π^2 ̄h^4



∣∣^4 πZ^1 Z^2 e

2
1
a^2 + 2k

(^2) (1−cosθ)




∣∣

2

=






μZ 1 Z 2 e^2
̄h^2
2 a^2 +p

(^2) (1−cosθ)







2

=






Z 1 Z 2 e^2
̄h^2
2 μa^2 + 4Esin

(^2) θ
2







2

In the last step we have used the non-relativistic formula for energy and 1−cosθ=^12 sin^2 θ 2.


The screened Coulomb potential gives a finite total cross section. It corresponds well with the
experiment Rutherford did in whichαparticles were scattered from atoms in a foil. If we scatter
from a bare charge where there is no screening, we can take the limitin whicha→∞.







Z 1 Z 2 e^2
4 Esin^2 θ 2






2

The total cross section diverges in due to the region around zero scattering angle.


30.2 Scattering from a Hard Sphere


Assume a low energy beam is incident upon a small, hard sphere of radiusr 0. We will assume that
̄hkr 0 < ̄hso that only theℓ= 0 partial wave is significantly affected by the sphere. As with the
particle in a box, the boundary condition on a hard surface is that the wavefunction is zero. Outside
the sphere, the potential is zero and the wavefunction solution willhave reached its form for large
r. So we set
(
e−i(kr^0 −ℓπ/2)−e^2 iδℓ(k)ei(kr^0 −ℓπ/2)


)

=

(

e−ikr^0 −e^2 iδ^0 (k)eikr^0

)

= 0

e^2 iδ^0 (k)=e−^2 ikr^0
Free download pdf