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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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272 Chapter 7<br />

coupling in gauge theories were per<strong>for</strong>med by Levine (1966) and Cung<br />

and Yoshimura (1975); <strong>for</strong> more recent discussions in the framework of<br />

the standard model see Nieves, Pal, and Unger (1983), Nieves (1987),<br />

Dodelson and Feinberg (1991), Liu (1991), Langacker and Liu (1992),<br />

Kuznetsov and Mikheev (1993), and Dicus and Repko (1993). This<br />

two-photon coupling leads to a higher-order contribution to the neutrino<br />

refractive index in a bath of photons (Sect. 6.7.2). However, this<br />

and other consequences do not seem to be important in any <strong>as</strong>trophysical<br />

or laboratory setting of practical interest.<br />

For neutrinos with m<strong>as</strong>ses and mixings there is a decay amplitude<br />

ν → ν ′ γγ which can dominate <strong>for</strong> a small range of neutrino m<strong>as</strong>ses<br />

below m ν = 2m e <strong>as</strong> discussed by Nieves (1983) and Ghosh (1984).<br />

Explicit results were given in Sect. 7.2.2 above.<br />

One of the photons may represent an external electric or magnetic<br />

field, i.e. one may consider the neutrino decay ν → ν ′ γ in the presence<br />

of a strong external field which would modify the propagators<br />

of the intermediate charged leptons. For very strong fields it appears<br />

that a substantial decay rate can obtain (Gvozdev, Mikheev, and V<strong>as</strong>silevskaya<br />

1992a,b, 1993, 1994a,b). From this literature it does not<br />

seem to become entirely clear under which if any circumstances these<br />

results might be of practical interest <strong>for</strong>, say, the decay of supernova or<br />

neutron-star neutrinos.<br />

7.4 Electromagnetic Processes<br />

The presence of electromagnetic dipole and transition moments implies<br />

that neutrinos couple directly to the electromagnetic field, allowing <strong>for</strong><br />

a variety of nonstandard processes (Fig. 7.8). Most obviously, neutrinos<br />

can scatter on electrons by photon exchange. The ν-e scattering cross<br />

section (electrons at rest in the laboratory frame) w<strong>as</strong> given, e.g. by<br />

Vogel and Engel (1989)<br />

dσ<br />

dT = G2 Fm e<br />

2π<br />

[(C V + C A ) 2 + (C V − C A ) 2 (1 − T E ν<br />

) 2<br />

+ (C 2 A − C 2 V ) m eT<br />

E 2 ν<br />

]<br />

+ αµ 2 ν<br />

[ 1<br />

T − 1 E ν<br />

]<br />

, (7.24)<br />

where C V and C A are the weak coupling constants given in Appendix B,<br />

T is the electron recoil energy with the limits 0 ≤ T ≤ 2E 2 ν/(2E ν +m e ),<br />

and µ ν is the neutrino dipole moment.

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