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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Oscillations of Trapped Neutrinos 323<br />

After a lengthy but straight<strong>for</strong>ward calculation one arrives at the<br />

NC collision term (Sigl and Raffelt 1993)<br />

∫<br />

˙ρ p,coll = 1 dp ′[ W<br />

2<br />

P ′ ,P Gρ p ′G(1 − ρ p ) − W P,P ′ρ p G(1 − ρ p ′)G<br />

+ W −P ′ ,P (1 − ρ p )G(1 − ρ p ′)G − W P,−P ′ρ p Gρ p ′G + h.c. ] ,<br />

(9.22)<br />

where P and P ′ are neutrino four momenta with physical (positive) energies<br />

P 0 = |p| and P ′ 0 = |p ′ |. The nonnegative transition probabilities<br />

W K ′ ,K = W (K ′ , K) are Wick contractions of medium operators of the<br />

<strong>for</strong>m<br />

W (K ′ , K) = 1 8 G2 F S µν (K ′ − K) N µν (K ′ , K) , (9.23)<br />

where K and K ′ correspond to neutrino four-momenta with K 0 and K 0<br />

′<br />

positive or negative. The “medium structure function” is<br />

S µν (∆) ≡<br />

∫ +∞<br />

−∞<br />

dt e i∆ 0t ⟨B µ (t, ∆)B ν (0, −∆)⟩ , (9.24)<br />

where the energy transfer ∆ 0 can be both positive and negative. In the<br />

ultrarelativistic limit the neutrino tensor can be written <strong>as</strong><br />

N µν = 1 2 (U µ U ′ν + U ′µ U ν − U · U ′ g µν − iϵ µναβ U α U ′ β), (9.25)<br />

where U ≡ K/K 0 and U ′ ≡ K ′ /K 0 are the neutrino four velocities.<br />

There<strong>for</strong>e, N µν is an even function of K and K ′ . Note that the definition<br />

Eq. (9.25) differs slightly from the corresponding Eq. (4.17).<br />

The first two terms of the collision integral Eq. (9.22) are due to<br />

neutrino scattering off the medium. The positive term represents gains<br />

from scatterings ν p ′ → ν p while the negative one is from losses by the<br />

inverse reaction. The third and fourth expressions account <strong>for</strong> pair<br />

processes, i.e. the creation or absorption of ν p ν p ′ by the medium. The<br />

pair terms are found by direct calculation or from the scattering ones<br />

by “crossing,”<br />

P → −P and ρ p → (1 − ρ p ) . (9.26)<br />

For example, the reaction ν p X → X ′ ν p ′ trans<strong>for</strong>ms to X → X ′ ν p ν p ′<br />

under this operation where X and X ′ represent medium configurations.<br />

The collision integral <strong>for</strong> ρ p is found by direct calculation or by<br />

applying the crossing operation Eq. (9.26) to all neutrinos and antineutrinos<br />

appearing in Eq. (9.22). The neutrino gain terms then trans<strong>for</strong>m<br />

to the antineutrino loss terms and vice versa.

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