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Physics LibreTexts

6.4: Neutrino Oscillations

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Neutrino oscillation is a phenomenon where a specific flavour of neutrino (electron, muon or tau) is later measured to have different flavour. The probability of measuring a particular flavour varies periodically. The three neutrino states are created by a radioactive decay in a flavour eigenstate as |f1, |f2, |f3 (electron, muon, tauon). However, these are not eigenstates of energy with a definite mass |m1, |m2, |m3. We can expand the flavour eigenstate using the energy eigenstates as a basis:

|fi=jmj|fi|mj

the energy eigenstates show how the wavefunctions behave in time, mj(t)=mj(0) exp(iωjt), where ωj=mjc2/. ωij=(mimj)c2/. Consider an electron neutrino produced by a fusion reaction in the sun, Φ(t=0)=|f1, its wavefunction then varies as:

Φ(t)=j|mjmj|f1 exp(iωjt)

For real neutrinos, the mj|f1 matrix has non-zero, possibly even complex elements everywhere, but here for simplicity we suppose that

mj|fi=|ac0ca0001|

with a and c real, time independent and a2+c2=1 for normalisation. Our electron neutrono then evolves as Φ(t)=a exp(iω1t)|m1(t)+c exp(iω2t)|m2(t), so the probability that some time later it is still an electron neutrino is

|f1|Φ(t)|2=|a2 exp(iω1t)+c2 exp(iω2t)|2=a4+c4+a2c2(exp(iω21t)+a2c2 exp(iω21t)=14a2c2sin2(ω21t/2)

which is less than 1: it can somehow “turn into” a muon neutrino. Often, one writes a=sinθ in which case 4a2c2=sin2θ. θ is refered to as a “mixing angle”.

If a=c=12, then with a frequency governed by the difference in masses, the electron neutrino turns completely into a muon neutrino, then back again. With smaller c, there’s always some chance that it will still be an electron neutrino. In reality, it is also possible to oscillate into a tau neutrino. This underlies the “solar neutrino problem”. Detection of solar neutrinos was the subject of the 2002 Nobel prize. Similar oscillation occurs in the kaon system due to a symmetrybreaking effect called “CP violation” subject of the 2008 Nobel prize. Here one of the states is subject to radioactive decay, so a particle not only “turns into” something else, it also disappears when it does so!


This page titled 6.4: Neutrino Oscillations is shared under a CC BY 4.0 license and was authored, remixed, and/or curated by Graeme Ackland via source content that was edited to the style and standards of the LibreTexts platform.

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