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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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320 Chapter 9<br />

9.3 Neutral-Current Interactions<br />

9.3.1 Hamiltonian<br />

In order to make Eq. (9.13) explicit one must use a specific model <strong>for</strong><br />

the interactions between neutrinos and the medium. To this end I begin<br />

with fermions which interact by virtue of an effective neutral-current<br />

(NC) Hamiltonian,<br />

H NC = G F ∑<br />

∫<br />

√ d 3 x B a µ (x) Ψ(x)G a γ µ (1 − γ 5 )Ψ(x) . (9.14)<br />

2<br />

a<br />

Here, B a<br />

µ typically is also a bilinear of the <strong>for</strong>m ψ a γ µ ψ a or ψ a γ 5 γ µ ψ a<br />

with a Dirac field ψ a which describes fermions of the medium. It is<br />

<strong>as</strong>sumed that all neutrino flavors scatter on a given species a in the<br />

same way apart from overall factors which are given <strong>as</strong> a hermitian<br />

n × n matrix G a of dimensionless coupling constants. In the absence of<br />

flavor-changing neutral currents it is diagonal in the weak interaction<br />

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

As a concrete example consider the ν e and ν µ flavors in a medium<br />

of ultrarelativistic electrons which may be cl<strong>as</strong>sified into a l.h. and a<br />

r.h. “species,” a = L or R, so that B µ L,R = 1ψ 2 eγ µ (1 ∓ γ 5 )ψ e . With the<br />

standard-model couplings given in Sect. 6.7.1 one finds in the weak<br />

interaction b<strong>as</strong>is G L = 2 sin 2 θ W + σ 3 and G R = 2 sin 2 θ W .<br />

For the calculations it is convenient to write Eq. (9.14) in momentum<br />

space,<br />

H NC = G F ∑<br />

∫<br />

√ dp dp ′ B a µ (p − p ′ ) Ψ p G a γ µ (1 − γ 5 )Ψ p ′ , (9.15)<br />

2<br />

a<br />

where B a µ (∆) = ∫ d 3 x B a µ (x)e −i∆·x is the Fourier trans<strong>for</strong>m of B a µ (x)<br />

and Ψ p = a p u p + b † −pv −p in terms of the annihilation and creation<br />

operators of Eq. (9.4).<br />

A special c<strong>as</strong>e of NC interactions are those among the neutrinos<br />

themselves with a Hamiltonian that is quartic in Ψ. In momentum<br />

space these “self-interactions” are given by<br />

H S = G ∫<br />

F<br />

√ dp dp ′ dq dq ′ (2π) 3 δ (3) (p + q − p ′ − q ′ )<br />

2<br />

× Ψ q G S γ µ (1 − γ 5 )Ψ q ′ Ψ p G S γ µ (1 − γ 5 )Ψ p ′ . (9.16)<br />

In the standard model with three sequential neutrino families G S is the<br />

3 × 3 unit matrix. For the evolution of a normal and a hypothetical<br />

sterile flavor one would have G S = diag(1, 0).

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