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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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260 Chapter 7<br />

The expansion rate and thus the energy density of the universe are<br />

well “me<strong>as</strong>ured” at the epoch of nucleosynthesis (T ≈ 0.3 MeV) by<br />

the primordial light-element abundances (Yang et al. 1984). This bigbang<br />

nucleosynthesis (BBN) argument h<strong>as</strong> been used to constrain the<br />

number of light neutrino families to N ν ∼ < 3.4 (Yang et al. 1984; Olive<br />

et al. 1990). Even though the me<strong>as</strong>ured Z ◦ decay width h<strong>as</strong> established<br />

N ν = 3 (Particle Data <strong>Group</strong> 1994) the BBN bound remains of interest<br />

<strong>as</strong> a m<strong>as</strong>s limit because m<strong>as</strong>sive neutrinos contribute more than a m<strong>as</strong>sless<br />

one to the expansion rate at BBN. For a lifetime exceeding about<br />

100 s this argument excludes 500 keV ∼ < m ν ∼ < 35 MeV (Kolb et al. 1991;<br />

Dolgov and Rothstein 1993; Kaw<strong>as</strong>aki et al. 1994), with even more restrictive<br />

limits <strong>for</strong> Dirac neutrinos (Fuller and Malaney 1991; Enqvist<br />

and Uibo 1993; Dolgov, Kainulainen, and Rothstein 1995). In Fig. 7.2<br />

the region thus excluded is hatched and marked “BBN.”<br />

Kaw<strong>as</strong>aki et al. (1994) have considered the majoron mode ν → ν ′ χ<br />

(Sect. 15.7) <strong>as</strong> a specific model <strong>for</strong> the neutrino decay. Including the<br />

energy density of the scalar χ they find even more restrictive limits<br />

which exclude the region between the d<strong>as</strong>hed lines in Fig. 7.2.<br />

7.2 Neutrino Mixing and Decay<br />

7.2.1 Flavor Mixing<br />

One of the most mysterious features of the particle zoo is the threefold<br />

repetition of families (or “flavors”) shown in Fig. 7.1. The fermions in<br />

each column have been arranged in a sequence of incre<strong>as</strong>ing m<strong>as</strong>s which<br />

appears to be the only significant difference between them. There is no<br />

indication <strong>for</strong> higher sequential families; the m<strong>as</strong>ses of their neutrinos<br />

would have to exceed 1 2 m Z = 46 GeV according to the CERN and SLAC<br />

me<strong>as</strong>urements of the Z ◦ decay width (Particle Data <strong>Group</strong> 1994). If<br />

the origin of m<strong>as</strong>ses is indeed the interaction with the vacuum Higgs<br />

field, the only difference between the fermions of a given column in<br />

Fig. 7.1 is their Yukawa coupling to Φ.<br />

If the only difference between, say, an electron and a muon is the<br />

vacuum refraction, any superposition between them is an equally legitimate<br />

charged lepton except <strong>for</strong> the practical difficulty of preparing it<br />

experimentally. When such a mixed state propagates, the two components<br />

acquire different ph<strong>as</strong>es along the beam exactly like two photon<br />

helicities in an optically active medium, leading to a rotation of the<br />

plane of polarization. Of course, now this “polarization” is understood<br />

in the abstract flavor space rather than in coordinate space.

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