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Etudes des proprietes des neutrinos dans les contextes ...

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

with the motion of D. Since a large µ means also that all Pω are aligned, using<br />

Eq.(5.54), one realize that the motion of D is essentially a precession around B<br />

and one can define a frame with the two vectors B and D that moves around B.<br />

According to Eq. (5.53) all Hω obviously lie in the plane spanned by B and D<br />

which we call the “co-rotating plane.” If we assume that µ varies slowly enough<br />

with time, then we are in the adiabatic limit: each of Pω follows Hω and stays<br />

mainly in this plane which seems the right frame to see an adiabatic evolution.<br />

Consequently M, also evolves in that plane and therefore we can decompose:<br />

and rewrite the EOM of Eq.(5.54) as<br />

M = bB + ωcD (5.56)<br />

∂tD = ωc B × D. (5.57)<br />

Therefore D and the co-rotating plane precess around B with the common or<br />

“co-rotation frequency” ωc. Projecting Eq.(5.56) on the transverse plane one<br />

has:<br />

ωc =<br />

+∞<br />

−∞ dω sω ω Pω⊥<br />

+∞<br />

dω sωPω⊥<br />

−∞<br />

=<br />

+∞<br />

−∞ dω sω ω Pω⊥<br />

D⊥<br />

. (5.58)<br />

ωc is clearly a function of µ. When µ → ∞ and all Pω are aligned, this is identical<br />

with the synchronization frequency Eq. (5.55).<br />

The corotating frame<br />

To study the feature of the spectral split, it is easier to work in a corotating<br />

frame. To do so, we apply the same method used in the previous subsection<br />

(see appendix D) for studying the neutrino evolution in a new frame. Therefore<br />

writing the E.O.M. given in Eq.(5.52) in the corotating frame yields:<br />

∂tPω = Hω × Pω − ωcB × Pω<br />

= ((ω − ωc)B + µD) × Pω<br />

(5.59)<br />

Initially when µ is very large, all individual Hamiltonians are essentially aligned<br />

with D. In turn, D is aligned with the weak-interaction direction if initially<br />

all polarization vectors Pω are aligned with that direction. In other words, all<br />

<strong>neutrinos</strong> are prepared in interaction eigenstates and initially Pω ∝ Hω. The<br />

adiabatic evolution would imply that if µ changes slowly enough, Pω follows<br />

Hω(µ) and therefore remains aligned with Hω(µ) at later times as well. So the<br />

adiabatic solution of the EOMs for our initial condition is given by<br />

Pω(µ) = ˆ Hω(µ) Pω , (5.60)<br />

107

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