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A Classic Thesis Style - Johannes Gutenberg-Universität Mainz

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128 theoretical background<br />

for the lepton tensor, and<br />

W 00 =<br />

� �2 |�q|<br />

W<br />

ω<br />

zz<br />

W 0i = |�q|<br />

ω Wzi<br />

(A.37)<br />

(A.38)<br />

for the hadronic tensor.<br />

Making use of these relations, we can get rid of all time components.<br />

The remaining terms in the contraction of both tensors can be<br />

conveniently grouped in the following form:<br />

LµνW µν =L xx W xx + L yy W yy − Q2<br />

ω 2 (Lzx W zx + L xz W xz ) + Q4<br />

ω 4 Lzz W zz +<br />

L xy W xy + L yx W yx − Q2<br />

ω 2 (Lyz W yz + L zy W zy )<br />

(A.39)<br />

where repeated use of the defining equation of momentum transfer<br />

Q 2 = |�q| 2 − ω 2 has been made.<br />

a.7 explicit form of the leptonic tensor<br />

According to the kinematics shown in Fig. 81 and assuming massless<br />

electrons we have:<br />

sin α = E′ e<br />

sin θe<br />

(A.40)<br />

|�q|<br />

cos α = Ee − E ′ e cos θe<br />

|�q|<br />

(A.41)<br />

Introducing these values in the defining equation for the leptonic<br />

tensor A.28 we get:<br />

Lxx = 4pexp ′ ex + Q2<br />

(A.42)<br />

Since by definition the change in the electron momentum is along the<br />

z direction, we can write:<br />

pex = p′ ex = Ee sin α = EeE ′ e sin θe<br />

|�q|<br />

Inserting these values in A.42 we get:<br />

Lxx = Q 2<br />

�<br />

4 E2eE ′2<br />

e sin 2 θe<br />

Q2 |�q| 2<br />

�<br />

+ 1<br />

(A.43)<br />

(A.44)

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