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32 Chapter 5. The Eikonal F<strong>in</strong>al State<br />

approximation (RDWIA). Next, we will <strong>in</strong>troduce a consistent relativistic model for<br />

the description of A(e, e ′ p) processes <strong>in</strong> the eikonal approximation. With the term<br />

“consistent” we refer to a procedure <strong>in</strong> which the bound <strong>and</strong> scatter<strong>in</strong>g states are<br />

derived from the same Dirac equation. The consistent approach possesses the virtue<br />

of obey<strong>in</strong>g orthogonality <strong>and</strong> unitarity constra<strong>in</strong>ts but will soon be observed to<br />

provide poor descriptions of the experimental data. In a next step, we will improve<br />

our model by implement<strong>in</strong>g complex optical potentials for the description of proton<br />

distortion <strong>in</strong> the f<strong>in</strong>al state. F<strong>in</strong>ally, we develop a scheme that allows to perform fully<br />

relativistic <strong>and</strong> unfactorized A(e, e ′ p) calculations <strong>in</strong> a Glauber multiple-scatter<strong>in</strong>g<br />

framework.<br />

5.1 The Relativistic Distorted Wave Approximation<br />

We will now briefly outl<strong>in</strong>e the RDWIA scheme to solve the Dirac equation of<br />

Eq. (3.3). With<strong>in</strong> a relativistic framework the bound state wave functions with<br />

well def<strong>in</strong>ed angular quantum numbers κ <strong>and</strong> m were of the form<br />

ψ nκm (⃗r) =<br />

[ ]<br />

ıGnκt (r)/r Y κm<br />

−F nκt (r)/r Y −κm<br />

. (5.1)<br />

These solutions are eigenstates of the total Hamiltonian <strong>and</strong> the total angular momentum<br />

with eigenvalue j = |κ| − 1/2,<br />

Y κm = ∑ 1<br />

< lm l<br />

m l m s<br />

2 m s|l 1 2 jm > Y l,m l<br />

χ 1<br />

2 ms ,<br />

j = |κ| − 1 2 , l = {<br />

κ, κ > 0<br />

−(κ + 1), κ < 0 .<br />

(5.2)<br />

The wave function for the outgo<strong>in</strong>g proton Ψ f is a scatter<strong>in</strong>g solution of the same<br />

Dirac equation of Eq. (3.3). In the RDWIA approach it is obta<strong>in</strong>ed as a partial wave<br />

expansion <strong>in</strong> configuration space [17, 18, 52, 53],<br />

Ψ f (⃗r) = 4π<br />

√<br />

E f + M<br />

2M<br />

∑<br />

1<br />

e −ıδ∗ κ<br />

< lm l<br />

κ,m,m l<br />

2 m s|l 1 2 jm > Y lm ∗<br />

l<br />

(ˆk f )ψ κm (⃗r) . (5.3)<br />

The phase shifts δ κ are calculated with a procedure as for example outl<strong>in</strong>ed <strong>in</strong><br />

Ref. [54]. Basically, one expresses the <strong>in</strong>cident, or bound, wave as a sum of partial<br />

waves <strong>and</strong> one can then compare the asymptotic radial functions of Eq. (5.3) with<br />

this plane wave expansion to determ<strong>in</strong>e the phase-shifts.

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