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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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316 Chapter 9<br />

(Dolgov 1981)<br />

ρ ij (p) = ⟨ a † j(p)a i (p) ⟩ and ρ ij (p) = ⟨ b † i(p)b j (p) ⟩ , (9.3)<br />

where a i (p) and a † i(p) are the destruction and creation operators <strong>for</strong><br />

neutrinos of flavor i in mode p while b is <strong>for</strong> antineutrinos which otherwise<br />

are referred to by overbarred quantities. The reversed order of the<br />

flavor indices in the definition of ρ(p) guarantees that both matrices<br />

trans<strong>for</strong>m in the same way under a unitary trans<strong>for</strong>mation in flavor<br />

space. Also, <strong>for</strong> brevity ⟨ | . . . | ⟩ is always written <strong>as</strong> ⟨. . .⟩.<br />

The diagonal elements of ρ p and ρ p are the usual occupation numbers<br />

while the off-diagonal ones represent relative ph<strong>as</strong>e in<strong>for</strong>mation.<br />

In the nondegenerate limit, up to a normalization ρ p plays the role of<br />

the previously defined single-particle density matrix. There<strong>for</strong>e, the<br />

ρ p ’s and ρ p ’s are well suited to account simultaneously <strong>for</strong> oscillations<br />

and collisions. In fact, one can argue that a homogeneous neutrino<br />

ensemble is completely characterized by these “matrices of densities”<br />

(Sigl and Raffelt 1993). It remains to derive an equation of motion<br />

which in the appropriate limits should reduce to the previous precession<br />

equation, to a Boltzmann collision equation, and to Stodolsky’s<br />

damping equation (9.1), respectively.<br />

9.2.3 Free Evolution: Flavor Oscillations<br />

The creation and annihilation operators which appear in the definition<br />

of ρ p are the time-dependent coefficients of a spatial Fourier expansion<br />

of the neutrino field [notation dp ≡ d 3 p/(2π) 3 ]<br />

∫<br />

Ψ(t, x) = dp [ a p (t)u p + b † ]<br />

−p(t)v −p e ip·x . (9.4)<br />

More precisely, a p is an annihilation operator <strong>for</strong> negative-helicity neutrinos<br />

of momentum p while b † p is a creation operator <strong>for</strong> positivehelicity<br />

antineutrinos. The Dirac spinors u p and v p refer to m<strong>as</strong>sless<br />

negative-helicity particles and positive-helicity antiparticles, respectively;<br />

the spinor normalization is taken to be unity. For n flavors,<br />

a p and b † p are column vectors of components a i (p) and b † i(p), respectively.<br />

They satisfy the anticommutation relations {a i (p), a † j(p ′ )} =<br />

{b i (p), b † j(p ′ )} = δ ij (2π) 3 δ (3) (p − p ′ ).<br />

In the m<strong>as</strong>sless limit and when only left-handed (l.h.) interactions<br />

are present one may ignore the right-handed (r.h.) field entirely. However,<br />

in order to include flavor mixing one needs to introduce a n × n

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