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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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268 Chapter 7<br />

Much larger values would obtain with direct r.h. neutrino interactions.<br />

For example, in left-right symmetric models there exist heavier<br />

gauge bosons which mediate r.h. interactions; parity violation would<br />

occur because of the m<strong>as</strong>s difference between the l.h. and r.h. gauge<br />

bosons. For a neutrino ν l (flavor l = e, µ or τ) the dipole moment in<br />

such models is (Kim 1976; Marciano and Sanda 1977; Bég, Marciano,<br />

and Ruderman 1978)<br />

µ ν = eG [<br />

)<br />

)]<br />

F<br />

2 √ m<br />

2 π 2 l<br />

(1 − m2 W 1<br />

sin 2ζ + 3<br />

m m 2 4 ν l<br />

(1 + m2 W 1<br />

,<br />

W 2<br />

m 2 W 2<br />

(7.18)<br />

where ζ is the left-right mixing angle between the gauge bosons W L<br />

and W R ; W 1,2 are their m<strong>as</strong>s eigenstates.<br />

Because of the smallness of the m<strong>as</strong>s-induced standard dipole moments<br />

any evidence <strong>for</strong> neutrino electromagnetic interactions would represent<br />

evidence <strong>for</strong> interactions beyond the standard model. There<strong>for</strong>e,<br />

the quest <strong>for</strong> neutrino electromagnetic interactions is more radical than<br />

that <strong>for</strong> m<strong>as</strong>ses and mixings.<br />

In a dense medium even standard m<strong>as</strong>sless neutrinos interact with<br />

photons by an effective coupling which is mediated by the ambient electrons.<br />

This coupling can be expressed in terms of an effective neutrino<br />

charge radius. Presently I focus on neutrino interactions in vacuum,<br />

leaving a discussion of their properties in media to Sect. 6.6.<br />

7.3.2 Single-Photon Coupling<br />

There are many possible extensions of the standard model which would<br />

give sizeable neutrino dipole and transition moments by some novel r.h.<br />

interaction. For the purposes of this book the underlying new physics<br />

is of no concern; all we need is a generic representation of its observable<br />

effects in terms of neutrino electromagnetic <strong>for</strong>m factors.<br />

The most general interaction structure of a fermion field ψ with the<br />

electromagnetic field can be expressed <strong>as</strong> an effective Lagrangian<br />

L int = −F 1 ψγ µ ψA µ − G 1 ψγ µ γ 5 ψ ∂ µ F µν<br />

− 1 2 ψσ µν(F 2 + G 2 γ 5 )ψF µν , (7.19)<br />

where A µ is the electromagnetic vector potential and F µν the field<br />

strength tensor. The interpretation of the coupling constants is that<br />

of an electric charge <strong>for</strong> F 1 , an anapole moment <strong>for</strong> G 1 , a magnetic

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