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Etudes des proprietes des neutrinos dans les contextes ...

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

Consequently, the vector Q in flavour space plays the role of a spherical pendulum<br />

in that its length is conserved so that it can move only on a sphere of radius<br />

Q. Actually, looking at Eqs.(5.27) and (5.31), we realize that the pendulum’s<br />

subsequent oscillations, represented by the vector Q, are confined in a plane<br />

defined by B and the z-axis. Indeed, in vacuum the vectors P and ¯ P evolve<br />

in the same way except that they rotate in opposite directions, therefore, their<br />

respective y−component cancels each other. Consequently, the vector Q has only<br />

two evolving components on the x− and z− axis. Therefore, we can define Q<br />

such as:<br />

⎛<br />

Q = ⎝<br />

sin ϕx<br />

0y<br />

cosϕz<br />

⎞<br />

⎠ (5.34)<br />

where ϕ is the tilt angle of Q relative to the z-axis. Finally, the problem variab<strong>les</strong><br />

are:<br />

˙ϕ = µD ,<br />

˙D = −ωQ sin(ϕ + 2θV ) . (5.35)<br />

Noticing from Eqs.(5.35), that ϕ is a coordinate and D its canonically conjugate<br />

momentum, we can obtain the form of the corresponding Hamiltonian, namely:<br />

where<br />

H(ϕ, D) = κ2<br />

1 − cos(ϕ + 2θV )<br />

µ<br />

+ 1<br />

2 µ D2 = V + T<br />

= ωB · Q + µ<br />

2 D2 , (5.36)<br />

κ 2 = ωµQ . (5.37)<br />

It corresponds to the motion of a simple pendulum where the first term V =<br />

ωB · Q is the potential energy in a homogeneous field and the second term T =<br />

µ2D 2 /2 is the kinetic energy. We now study the influence of the hierarchy on the<br />

pendulum behaviour.<br />

The importance of the hierarchy<br />

We first consider the normal hierarchy case and then investigate the inverted<br />

hierarchy case. Assuming a small vacuum mixing angle θ0 and a small excursion<br />

angle ϕ of the pendulum, the potential can be expanded to the second order:<br />

V (ϕ) = κ 2 [1 − cos(ϕ + 2θV )]<br />

= κ2<br />

2 (ϕ + 2θV ) 2 + . . . . (5.38)<br />

100

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