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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Oscillations of Trapped Neutrinos 327<br />

physically most transparent to work always in the weak interaction<br />

b<strong>as</strong>is.<br />

In order to derive an equation of motion <strong>for</strong> ˜ρ p one evaluates the<br />

collision term in Eq. (9.32) by inserting ˜ρ p ’s under the integral. Expanding<br />

the result in Pauli matrices leads to an expression of the <strong>for</strong>m<br />

1<br />

(a 2 p + A p · σ). In general, the polarization vector A p produced by the<br />

collision term is not parallel to v p = (s p , 0, c p ) because the collision<br />

term couples modes with different mixing angles. However, the <strong>as</strong>sumed<br />

f<strong>as</strong>t oscillations average to zero the A p component perpendicular to v p .<br />

There<strong>for</strong>e, the r.h.s. of Eq. (9.32) is of the <strong>for</strong>m 1[a 2 p+(v p·A p ) (v p·σ)].<br />

With a matrix of coupling constants in the weak b<strong>as</strong>is of<br />

( ) ge 0<br />

G =<br />

(9.36)<br />

0 g x<br />

the collision integral Eq. (9.32) becomes explicitly<br />

∫<br />

f˙<br />

p x = 1 dp { ]<br />

′ w(ν x 4<br />

p → νp x ′)[ (4 − s 2 p)gx 2 + (2 − s 2 p)t p t p ′g e g x<br />

]<br />

+ w(νp e → νp x ′)[ −s 2 pgx 2 − s 2 pt p t p ′g e g x<br />

where<br />

+ w(ν x p → ν e p ′)[ s 2 pg 2 e − (2 − s 2 p)t p t p ′g e g x<br />

]<br />

+ w(ν e p → ν e p ′)[ s 2 pg 2 e + s 2 pt p t p ′g e g x<br />

]}<br />

, (9.37)<br />

w(νp a → νp b ′) ≡ W P ′ P fp b ′(1 − f p) a − W P P ′fp(1 a − fp b ′) (9.38)<br />

(Raffelt and Sigl 1993). The equation <strong>for</strong> fp e is the same if one exchanges<br />

e ↔ x everywhere. In the absence of mixing s p = t p = 0, leading to<br />

the usual collision integral <strong>for</strong> each species separately.<br />

If ν x is neither ν µ nor ν τ but rather some hypothetical sterile species<br />

its coupling constant is g x = 0 by definition. In this c<strong>as</strong>e the collision<br />

integral simplifies to<br />

˙ f x p = 1 4 s2 pg 2 e<br />

∫<br />

dp ′[ W P ′ P fp e ′(2 − f p e − fp)<br />

x<br />

− W P P ′(f e p + f x p)(1 − f e p ′)] . (9.39)<br />

If the ν e stay approximately in thermal equilibrium, detailed balance<br />

yields<br />

∫<br />

f˙<br />

p x = 1 4 s2 pge<br />

2 dp ′[ W P ′ P fp e ′(1 − f p) x − W P P ′ fp(1 x − fp e ′)] . (9.40)<br />

If in addition the mixing angle is so small that the ν x freely escape one<br />

may set f x p = 0 on the r.h.s. so that the integral expression becomes<br />

∫ dp ′ W P ′ P f e p ′.

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