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Etudes des proprietes des neutrinos dans les contextes ...

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

where we introduced the total proton loss rate λp = λ¯νe + λe− and the total<br />

neutron loss rate λn = λνe + λe +. It has been shown that when the rates of<br />

these processes are rapid as compared to the outflow rate a “weak chemical<br />

equilibrium” is established [99]. The weak freeze-out radius is defined to be<br />

where the neutron-to-proton conversion rate is <strong>les</strong>s than the outflow rate of the<br />

material. If the plasma reaches a weak equilibrium stage then Ye is no longer<br />

changing: dYe/dt = 0. From Eq.(3.35) one can write the equilibrium value of the<br />

electron fraction<br />

+ 1 λp − λn<br />

Xα. (3.36)<br />

2<br />

Ye = λn<br />

λp + λn<br />

λp + λn<br />

At high temperatures alpha partic<strong>les</strong> are absent and the second term in Eq.(3.36)<br />

can be dropped10 . In the region just below where the alpha partic<strong>les</strong> are formed<br />

approximately one second after the bounce, the temperature is <strong>les</strong>s then ∼ 1<br />

MeV. Here both the electron and positron capture rates are very small and Ye<br />

can be approximated as<br />

Y (0)<br />

e =<br />

Using Eq. (3.32), we rewrite Eq. (3.37):<br />

Y (0)<br />

e (r) =<br />

<br />

1 +<br />

∞<br />

0<br />

∞<br />

0<br />

1<br />

. (3.37)<br />

1 + λ¯νe/λνe<br />

σ¯νe(E) dL¯νe(r,E)<br />

dE dE<br />

σνe(E) dLνe(r,E)<br />

dE dE<br />

−1<br />

. (3.38)<br />

This is the formula we use in our numerical simulations (see chapters 4 and<br />

6). Neutrino oscillations, since they can swap energies of different flavors, can<br />

affect the energy-dependent rates in Eqs.(3.37) and (3.38), changing the electron<br />

fraction. In the next chapter, we will show how CP-violation effects may impact<br />

the electron neutrino and anti-neutrino fluxes, and consequently the electron<br />

fraction.<br />

10 At lower temperature the alpha particle mass fraction increases. Consequently free nucleons<br />

get bound in alphas and cease interacting with <strong>neutrinos</strong>, because of the large binding energy<br />

of the alpha particle. This phenomenon is called ”alpha effect”, it can increases the value of Ye<br />

which implies fewer free neutrons, and therefore negatively impacts r-process nucleosynthesis<br />

[118]. We do not consider the alpha effect in our numerical simulation, a future work should<br />

include it.<br />

63

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