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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Nonstandard Neutrinos 263<br />

Flavor mixing is the only possibility <strong>for</strong> members of one family (one<br />

row in Fig. 7.1) to trans<strong>for</strong>m into those of a different family. This phenomenon<br />

is known <strong>as</strong> the absence of flavor-changing neutral currents;<br />

it means that the Z ◦ coupling to quarks and leptons, like the photon<br />

coupling, leaves a given superposition of fermions unaltered. For example,<br />

muons decay only by the flavor-conserving mode µ − → ν µ e − ν e<br />

(Fig. 7.4); the experimental upper limits on the branching ratios <strong>for</strong><br />

µ − → e − γ and µ − → e − e + e − are 5×10 −11 and 1.0×10 −12 , respectively.<br />

In the absence of neutrino m<strong>as</strong>ses and mixing the individual lepton flavor<br />

numbers are conserved: a lepton can be trans<strong>for</strong>med only into its<br />

partner of the same family, or it can be created or annihilated together<br />

with an antilepton of the same family.<br />

Fig. 7.4. Allowed and <strong>for</strong>bidded µ decays.<br />

When neutrinos have m<strong>as</strong>ses and mixings, flavor-violating lepton<br />

decays become possible, but their rate would be so small that their<br />

experimentally observed absence does not yield interesting constraints<br />

on neutrino parameters. Because neutrino m<strong>as</strong>ses must be very small if<br />

they exist at all, the most significant observable effect is that of neutrino<br />

oscillations.<br />

7.2.2 Standard-Model Decays of Mixed Neutrinos<br />

For m<strong>as</strong>sive neutrinos it is kinematically possible to decay according<br />

to ν → ν ′ γ, ν → ν ′ γγ, or ν → ν ′ ν ′′ ν ′′ . In the absence of mixing, of<br />

course, all of these modes are <strong>for</strong>bidden. Even in the presence of mixing,<br />

Fig. 7.5. Allowed and <strong>for</strong>bidden tree-level decays of mixed neutrinos.

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