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Master Dissertation

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Note that<br />

〈Woutφ, ψ〉 = 〈 lim<br />

t→∞ U(0, t)e −iH0t φ, ψ〉<br />

= lim<br />

t→∞ 〈U(0, t)e −iH0t φ, ψ〉<br />

= lim<br />

t→∞ 〈φ, e iH0t U(0, t) ∗ ψ〉<br />

= 〈φ, lim<br />

t→∞ e iH0t U(t, 0)ψ〉.<br />

Hence W ∗ out = s- limt→∞ e iH0t U(t, 0). Further<br />

W ∗ outWinψ = lim<br />

t→∞ lim<br />

s→−∞ eiH0t U(t, 0)U(0, s)e −iH0s ψ<br />

This leads us to the following definition.<br />

= lim<br />

t→∞ lim<br />

s→−∞ eiH0t U(t, s)e −iH0s ψ.<br />

Definition 3.3. The scattering matrix is defined as follows<br />

S = W ∗ outWin = s- lim<br />

t→∞ s- lim<br />

s→−∞ eiH0t U(t, s)e −iH0s .<br />

The physical meaning of the scattering matrix is now apparent. A<br />

normalized initial asymptotic state ψ considered at time t = 0, say, is first<br />

transformed to s = −∞ by free dynamics, then it is evolved from −∞ to<br />

t = ∞ by full interacting dynamics and finally it is transformed back from<br />

∞ to t = 0 again by free dynamics. Thus Sψ is in fact the outgoing<br />

scattering state transformed to t = 0 by free dynamics. The probability for<br />

a transition form ψ to φ is given by<br />

P (ψ → φ) = |〈φ, Sψ〉| 2 .<br />

Now ψ(t) as given by equation (3.1) is the solution to the Schrödinger<br />

equation<br />

i d<br />

dt ψ(t) = (H0 + V (t))ψ(t).<br />

If we go over to the interaction picture 2 by substituting φ = e iH0t ψ, we get<br />

i d d<br />

φ(t) = i<br />

dt dt (eiH0tψ(t)) = −H0e iH0t iH0t<br />

ψ(t) + e (H0 + V (t))ψ(t)<br />

= e iH0t −iH0t<br />

V e φ(t)<br />

= ˜ V (t)φ(t).<br />

FIXME: Make sure you can differentiate like this.<br />

2 See [8] page 318.<br />

20

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