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Etudes des proprietes des neutrinos dans les contextes ...

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tel-00450051, version 1 - 25 Jan 2010<br />

p<br />

k<br />

νe e −<br />

e −<br />

W ±<br />

Figure 1.3: Charged-current interactions bewteen electrons and <strong>neutrinos</strong>.<br />

where x is the spatial variable. In order to separate the neutrino and electron<br />

contributions, we apply the Fierz transformation and obtain:<br />

νe<br />

H CC GF<br />

eff (x) = √2 [¯νe(x)γ µ (1 − γ5)νe(x)] [ē(x)γµ(1 − γ5)e(x)]. (1.27)<br />

To obtain the coherent forward scattering contribution to the energy of νe in matter<br />

(i.e. the matter-induced potential for νe) we fix the variab<strong>les</strong> corresponding<br />

to νe and integrate over all the variab<strong>les</strong> that correspond to the electron. For<br />

coherent forward scattering we have p = p ′ = pν and therefore k = k ′ = pe. The<br />

helicities of the electrons also remain unchanged after the scattering because the<br />

interaction must leave the medium unchanged in order to contribute coherently<br />

to the neutrino potential 7 . The average of the effective Hamiltonian over the<br />

electron background in the medium rest frame is given by<br />

HCC GF<br />

eff (x) = √2 ¯νe(x)γ µ <br />

(1 − γ5)νe(x) d 3 pef(Ee, T) (1.28)<br />

× 1 <br />

〈e<br />

2<br />

− (pe, he) | e(x)γµ(1 − γ5)e(x) | e − (pe, he)〉.<br />

he=±1<br />

For simplicity, we consider for the electron background a finite normalization<br />

volume V with the one electron states | e − (pe, he)〉 :<br />

k ′<br />

p ′<br />

| e − (pe, he)〉 = 1<br />

2EeV ahe†<br />

e (pe) | 0〉 (1.29)<br />

The function f(Ee, T) is the statistical distribution of the electron energy Ee,<br />

which depends on the temperature T of the electron background and is normalized<br />

7 Indeed the spin of the electrons is not changed therefore the helicities are conserved.<br />

17

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