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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Particle Dispersion and Decays in Media 249<br />

they are m<strong>as</strong>sless there is no operational distinction between a Majorana<br />

neutrino and the two active degrees of freedom of a Dirac neutrino.<br />

There<strong>for</strong>e, according to Eq. (6.107) the dispersion relation <strong>for</strong> the helicity<br />

± states of a Majorana neutrino is<br />

E ± = (m 2 + p 2 ) 1/2 ∓ V, (6.124)<br />

where the medium-induced potential V w<strong>as</strong> given in Eq. (6.108). For<br />

ν e it is V = √ 2G F (n e − 1n 2 n) with the electron and neutron densities<br />

n e and n n , respectively.<br />

This dispersion relation implies that the medium is “optically active”<br />

with regard to the neutrino helicities, just <strong>as</strong> some media are<br />

birefringent with regard to the photon circular polarization. In the<br />

optical c<strong>as</strong>e the left-right symmetry (parity) is broken by the medium<br />

constituents which must have a definite handedness; sugar molecules<br />

are a well-known example. In the neutrino c<strong>as</strong>e parity is broken by the<br />

structure of the interaction; the medium itself is unpolarized.<br />

Because there is an energy difference between the Majorana helicity<br />

states ν ± <strong>for</strong> a given momentum, decays ν − → ν + χ are kinematically<br />

allowed. For relativistic neutrinos the squared matrix element is found<br />

to be |M| 2 = 4h 2 P 1 · P 2 with the four-momenta P 1,2 of the initial and<br />

final neutrino state. The differential decay rate is then<br />

dΓ = 4h2<br />

2E 1<br />

d 3 p 2<br />

2E 2 (2π) 3<br />

d 3 k<br />

2ω(2π) 3 P 1 · P 2 (2π) 4 δ 4 (P 1 − P 2 − K)<br />

(6.125)<br />

with the majoron four-momentum K. Integrating out the d 3 k variable<br />

removes the momentum δ function. The remaining differential decay is<br />

∫<br />

dΓ<br />

+1<br />

= α χ dx P 1 · P 2 p 2 2<br />

dE 2 −1 E 1 E 2 ω δ(E 1 − E 2 − ω), (6.126)<br />

where x = cos θ <strong>for</strong> the angle between p 1 and p 2 and α χ ≡ h 2 /4π<br />

is the majoron “fine-structure constant.” In the δ function one must<br />

use ω = k = |p 1 − p 2 | = (p 2 1 + p 2 2 − 2p 1 p 2 x) 1/2 . With ∫ dx δ[f(x)] =<br />

|df/dx| −1 = ω/p 1 p 2 and with energy-momentum conservation which<br />

yields P 1 − P 2 = K and thus P 1 · P 2 = 1(P 2 2 1 + P2 2 ) one finds<br />

dΓ<br />

dE 2<br />

= α χ<br />

(E 2 1 + E 2 2 − p 2 1 − p 2 2) p 2<br />

2E 1 E 2 p 1<br />

. (6.127)

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