Two-flavour neutrino oscillations

A neutrino is the only particle we routinely produce in one identity and detect in another. In the Standard Model the charged-current weak vertex couples a charged lepton to a fixed combination of neutrino mass eigenstates, so the electron neutrino born in a beta decay, or the muon neutrino born when a pion decays, is not a state of definite mass at all — it is a coherent superposition of the mass states ν1\nu_1 and ν2\nu_2. For two flavours that superposition is fixed by a single number, the mixing angle θ\theta, through a 2×22\times2 rotation between the flavour basis (νe,νμ)(\nu_e,\nu_\mu) and the mass basis (ν1,ν2)(\nu_1,\nu_2). Set that superposition moving. Each mass eigenstate is a plane wave that carries its own quantum phase ϕk=Ekt−pkL\phi_k=E_kt-p_kL, and because m1≠m2m_1\neq m_2 the two phases advance at different rates. The components drift out of step as the neutrino travels, so the particular blend that spelled "electron neutrino" at the source is continuously rewritten into a different blend downstream. Project the evolved state back onto the flavour basis and the probability of finding the other flavour rises and falls sinusoidally with distance — the neutrino oscillates. Everything hard about this article lives in one phase difference, Δϕ=Δm2L/2E\Delta\phi=\Delta m^2 L/2E, and everything useful follows from it: the oscillation probability depends only on the mass-squared difference Δm2\Delta m^2 and on sin⁡22θ\sin^2 2\theta, never on the absolute masses. That is why a detector kilometres from a reactor, or hundreds of kilometres from an accelerator, can weigh differences of neutrino masses far too small to measure any other way.

Key takeaways
  • The weak (flavour) states νe,νμ\nu_e,\nu_\mu are a rotation of the mass states ν1,ν2\nu_1,\nu_2 by one mixing angle θ\theta; the mass states, not the flavour states, have definite mass.
  • Mass eigenstates propagate as plane waves and accumulate phases ϕk=Ekt−pkL\phi_k=E_kt-p_kL; unequal masses give a growing phase difference Δϕ=Δm2L/2E\Delta\phi=\Delta m^2 L/2E.
  • The transition probability oscillates: P(νe→νμ)=sin⁡22θ sin⁡2 ⁣(Δm2L/4E)P(\nu_e\to\nu_\mu)=\sin^2 2\theta\,\sin^2\!\big(\Delta m^2 L/4E\big), with survival 1−P1-P.
  • Oscillation needs both a nonzero mass-squared difference and nonzero mixing — either one alone gives P=0P=0.
  • Practical form: P=sin⁡22θ sin⁡2 ⁣(1.27 Δm2[eV2] L[km]/E[GeV])P=\sin^2 2\theta\,\sin^2\!\big(1.27\,\Delta m^2[\mathrm{eV}^2]\,L[\mathrm{km}]/E[\mathrm{GeV}]\big); the oscillation length is Losc=4πE/Δm2≈2.48 E[GeV]/Δm2[eV2]L_\mathrm{osc}=4\pi E/\Delta m^2\approx 2.48\,E[\mathrm{GeV}]/\Delta m^2[\mathrm{eV}^2] km.
  • Oscillations resolved the solar and atmospheric neutrino deficits and proved that neutrinos have mass and that lepton flavour is not separately conserved.
  • Key idea: a neutrino is born in a flavour state but travels as a superposition of mass states; because the heavier and lighter components keep different quantum clocks, the interference between them periodically rebuilds the wavefunction into a different flavour.
The core insight

A neutrino is born in a flavour state but travels as a superposition of mass states; because the heavier and lighter components keep different quantum-mechanical clocks, the interference between them periodically rebuilds the wavefunction into a different flavour.

Where this lives today

The two-flavour formula is the backbone of a worldwide experimental program, even though nature needs three flavours to be described fully. Long-baseline accelerator experiments — T2K in Japan and NOvA in the United States — send muon-neutrino beams hundreds of kilometres and measure both νμ\nu_\mu disappearance and νe\nu_e appearance, using the survival dip to pin Δm322\Delta m^2_{32} and θ23\theta_{23} and the appearance channel to chase the CP-violating phase and the mass ordering that lie beyond the two-flavour picture. Reactor experiments work the complementary corner: Daya Bay, RENO and Double Chooz measured the small angle θ13\theta_{13} from a percent-level νˉe\bar\nu_e deficit at roughly a kilometre, and the upcoming JUNO detector will read the fine oscillatory spectral distortion at 53 km to resolve the mass ordering from vacuum oscillations alone. Atmospheric neutrinos remain a laboratory in their own right, now probed at the gigatonne scale by IceCube's DeepCore and, soon, by KM3NeT, with matter effects through the Earth in play. The flagship of the next decade, DUNE, will fire a wideband beam 1300 km through rock to a liquid-argon detector, scanning a full oscillation pattern in a single spectrum. Every one of these reads its data through the shape first written down for two flavours: an amplitude set by mixing, a frequency set by a mass-squared difference.

The physical picture

Picture the two mass eigenstates as two waves launched together from the source, perfectly in step at the moment of production. That shared starting phase is exactly what encodes the flavour: aligned in one particular way, the pair spells "muon neutrino". But the heavier state carries slightly more energy at the same momentum, so its phase turns a little faster, and the two waves slide apart as they run. When they have drifted half a beat out of step, the blend no longer spells "muon neutrino" — it spells "tau neutrino". The flavour we would measure is the running interference between two clocks ticking at almost, but not quite, the same rate. The first figure shows that drift and names the phase that drives it.

Figure
Two mass eigenstates ν₁ and ν₂ leave the source in phase, then drift apart because the heavier state turns its quantum phase faster: the accumulated difference is Δφ = (m₂² − m₁²)L / 2E = Δm² L / 2E, and where they fall out of step the flavour has changed from ν_μ toward ν_τ
Two clocks, almost in step: the phase difference Δφ = Δm² L / 2E drives the flavour change ν₁ ν₂ in phase → ν_μ flavour at production half a beat out → ν_τ flavour has flipped distance travelled L

Turn the drift into the quantity an experiment measures and you get the oscillation curve: the probability of finding the far-flavour, plotted against the ratio L/EL/E of baseline to energy. Its shape is fixed by just two numbers. The amplitude of the wiggle is sin⁡22θ\sin^2 2\theta — how completely the flavours can interchange, set entirely by the mixing angle — and the frequency of the wiggle along the L/EL/E axis is set by Δm2\Delta m^2. Experiments are built by choosing LL and EE so that the neutrino arrives near the first crest, where the conversion is largest. The second figure is that curve for the atmospheric mass splitting, drawn to scale.

Figure
Oscillation probability P(ν_μ → ν_τ) = sin²2θ · sin²(1.27 Δm² L/E) against L/E in km/GeV, for the atmospheric splitting Δm² = 2.5×10⁻³ eV² and maximal mixing sin²2θ = 1: the first maximum sits at L/E ≈ 495 km/GeV and one full oscillation length is L/E ≈ 992 km/GeV
The punchline: P(ν_μ → ν_τ) for Δm² = 2.5×10⁻³ eV², sin²2θ = 1 1.0 0.75 0.5 0.25 0 0 500 1000 1500 L / E (km / GeV) probability P amplitude sin²2θ = 1 first maximum L/E ≈ 495 L_osc 992 km/GeV

The core equations

The whole subject is a chain of six relations, each a short step from the last. Start with the fact that flavour is a rotation of mass. For two flavours the unitary mixing matrix is a single rotation through the angle θ\theta, tying the states the weak interaction makes and detects to the states that propagate cleanly.

(νeνμ)=(cos⁡θsin⁡θ−sin⁡θcos⁡θ)(ν1ν2)(1)\begin{pmatrix}\nu_e\\ \nu_\mu\end{pmatrix}=\begin{pmatrix}\cos\theta & \sin\theta\\ -\sin\theta & \cos\theta\end{pmatrix}\begin{pmatrix}\nu_1\\ \nu_2\end{pmatrix} \qquad (1)

where: νe,νμ\nu_e,\nu_\mu — flavour (weak) eigenstates, produced and detected by the charged current; ν1,ν2\nu_1,\nu_2 — mass eigenstates with masses m1,m2m_1,m_2; θ\theta — mixing angle. At θ=0\theta=0 flavour and mass coincide and nothing oscillates. Each mass eigenstate propagates as a plane wave, picking up a phase set by its own energy and momentum. This is the only place the dynamics enters — after this it is all interference.

∣νk(t)⟩=e−i(Ekt−pkL) ∣νk⟩=e−iϕk ∣νk⟩(2)|\nu_k(t)\rangle=e^{-i(E_k t-p_k L)}\,|\nu_k\rangle=e^{-i\phi_k}\,|\nu_k\rangle \qquad (2)

where: ϕk=Ekt−pkL\phi_k=E_kt-p_kL — the phase of mass state kk after time tt over baseline LL; Ek=pk2+mk2E_k=\sqrt{p_k^2+m_k^2} — its energy. Because m1≠m2m_1\neq m_2 the two phases advance unequally, and their difference is what survives. Prepare a νe\nu_e, evolve, and project onto νμ\nu_\mu; the modulus-squared of that amplitude is the appearance probability. This is the central result of the article.

P(νe→νμ)=sin⁡22θ sin⁡2 ⁣(Δm2 L4E),Δm2≡m22−m12(3)P(\nu_e\to\nu_\mu)=\sin^2 2\theta\,\sin^2\!\left(\frac{\Delta m^2\,L}{4E}\right),\qquad \Delta m^2\equiv m_2^2-m_1^2 \qquad (3)

where: sin⁡22θ\sin^2 2\theta — the oscillation amplitude, fixed by mixing; Δm2\Delta m^2 — mass-squared difference in eV2\mathrm{eV}^2; LL — baseline; EE — neutrino energy. The probability depends on Δm2\Delta m^2, never on m1m_1 or m2m_2 separately, and the sign of Δm2\Delta m^2 drops out because sin⁡2\sin^2 is even. Probability is conserved, so what does not appear as νμ\nu_\mu survives as νe\nu_e. The survival probability is the complement, and it is what a disappearance experiment measures directly.

P(νe→νe)=1−sin⁡22θ sin⁡2 ⁣(Δm2 L4E)(4)P(\nu_e\to\nu_e)=1-\sin^2 2\theta\,\sin^2\!\left(\frac{\Delta m^2\,L}{4E}\right) \qquad (4)

where: the two channels sum to one, P(νe→νe)+P(νe→νμ)=1P(\nu_e\to\nu_e)+P(\nu_e\to\nu_\mu)=1, as unitarity demands for two flavours. A reactor experiment counts the νˉe\bar\nu_e that fail to arrive; an accelerator experiment can count either channel. Restoring the factors of ℏ\hbar and cc that natural units hid turns equation (3) into the form every experimentalist actually uses, with the baseline in kilometres and the energy in GeV.

P=sin⁡22θ sin⁡2 ⁣(1.267 Δm2[eV2] L[km]E[GeV])(5)P=\sin^2 2\theta\,\sin^2\!\left(1.267\,\frac{\Delta m^2[\mathrm{eV}^2]\,L[\mathrm{km}]}{E[\mathrm{GeV}]}\right) \qquad (5)

where: the constant 1.2671.267 packages ℏc\hbar c and the unit conversions (derived below); the same number holds for LL in metres and EE in MeV. This is the working formula behind every oscillation plot. Finally, the distance over which the pattern repeats defines the oscillation length, the natural yardstick for choosing a baseline.

Losc=4πEΔm2≈2.48 E[GeV]Δm2[eV2] km(6)L_\mathrm{osc}=\frac{4\pi E}{\Delta m^2}\approx 2.48\,\frac{E[\mathrm{GeV}]}{\Delta m^2[\mathrm{eV}^2]}\ \mathrm{km} \qquad (6)

where: LoscL_\mathrm{osc} — one full period of the oscillation; the first appearance maximum sits at Losc/2L_\mathrm{osc}/2. Matching L/EL/E to LoscL_\mathrm{osc} for a given Δm2\Delta m^2 is the whole art of designing an oscillation experiment.

Derivation AFrom flavour mixing to the oscillation probability

The goal is to turn the physical story into equation (3) with no gaps: start from a neutrino produced as a pure flavour state, write it in the mass basis where propagation is simple, let each mass eigenstate accumulate its plane-wave phase, project the evolved state back onto the other flavour, and square the amplitude. Every step is elementary quantum mechanics of a two-state system; the only physics input is that the mass eigenstates, not the flavour states, are what propagate with definite phase. We keep two flavours throughout so the algebra stays a single rotation.

Step 1. Produce a νe\nu_e at L=0L=0, t=0t=0. Using equation (1), write it in the mass basis: ∣ν(0)⟩=∣νe⟩=cos⁡θ ∣ν1⟩+sin⁡θ ∣ν2⟩|\nu(0)\rangle=|\nu_e\rangle=\cos\theta\,|\nu_1\rangle+\sin\theta\,|\nu_2\rangle. Why: the weak interaction makes a flavour state, but only the mass states have a definite energy–momentum relation, so we must change basis before we can propagate anything.

Step 2. Evolve each mass component with its own phase from equation (2): ∣ν(t)⟩=cos⁡θ e−iϕ1∣ν1⟩+sin⁡θ e−iϕ2∣ν2⟩|\nu(t)\rangle=\cos\theta\,e^{-i\phi_1}|\nu_1\rangle+\sin\theta\,e^{-i\phi_2}|\nu_2\rangle. Why: superposition means each eigenstate evolves independently; the two phases ϕ1,ϕ2\phi_1,\phi_2 are the only things that change, and their difference is the entire physics.

Step 3. Ask for the amplitude to detect a νμ\nu_\mu. With ⟨νμ∣=−sin⁡θ ⟨ν1∣+cos⁡θ ⟨ν2∣\langle\nu_\mu|=-\sin\theta\,\langle\nu_1|+\cos\theta\,\langle\nu_2| and orthonormal mass states, ⟨νμ∣ν(t)⟩=sin⁡θcos⁡θ (e−iϕ2−e−iϕ1)\langle\nu_\mu|\nu(t)\rangle=\sin\theta\cos\theta\,(e^{-i\phi_2}-e^{-i\phi_1}). Why: the detector, like the source, couples to a flavour state, so the observable amplitude is the projection of the evolved state onto νμ\nu_\mu — and it vanishes unless the two phases differ.

Step 4. Square the amplitude. Using ∣e−iϕ2−e−iϕ1∣2=2−2cos⁡(ϕ1−ϕ2)=4sin⁡2 ⁣(ϕ1−ϕ22)|e^{-i\phi_2}-e^{-i\phi_1}|^2=2-2\cos(\phi_1-\phi_2)=4\sin^2\!\big(\tfrac{\phi_1-\phi_2}{2}\big) and sin⁡2θcos⁡2θ=14sin⁡22θ\sin^2\theta\cos^2\theta=\tfrac14\sin^2 2\theta, the factors of four cancel: P(νe→νμ)=sin⁡22θ sin⁡2 ⁣(Δϕ2)P(\nu_e\to\nu_\mu)=\sin^2 2\theta\,\sin^2\!\big(\tfrac{\Delta\phi}{2}\big), with Δϕ=ϕ1−ϕ2\Delta\phi=\phi_1-\phi_2. Why: this is the interference term made real — the mixing sets how much can interfere, and the phase difference sets where in the cycle the interference lands.

Step 5. Insert the phase difference Δϕ=Δm2L/2E\Delta\phi=\Delta m^2 L/2E from the next derivation to reach P(νe→νμ)=sin⁡22θ sin⁡2 ⁣(Δm2L/4E)P(\nu_e\to\nu_\mu)=\sin^2 2\theta\,\sin^2\!\big(\Delta m^2 L/4E\big). Why: with the phase evaluated, the abstract two-state result becomes the concrete oscillation formula, depending only on Δm2\Delta m^2, θ\theta, and L/EL/E.

Go deeper · Derivation B · 1 minThe propagation phase and why equal energy, equal momentum, and equal velocity all agree
Derivation BThe propagation phase and why equal energy, equal momentum, and equal velocity all agree

The aim is to justify the single most important line in the subject, Δϕ=Δm2L/2E\Delta\phi=\Delta m^2 L/2E, and to defuse a genuine confusion: the raw phase ϕk=Ekt−pkL\phi_k=E_kt-p_kL mixes an energy term and a momentum term, and the two mass eigenstates strictly have different energies, momenta, times of flight, and velocities. The reassuring fact is that in the ultra-relativistic limit that always applies to real neutrinos, three different simplifying assumptions — equal momenta, equal energies, or equal velocities — deliver the identical answer, and a full wave-packet treatment confirms it. We show the two cleanest routes converge.

Step 1. Write the difference of phases exactly: Δϕ=ϕ1−ϕ2=(E1−E2)t−(p1−p2)L\Delta\phi=\phi_1-\phi_2=(E_1-E_2)t-(p_1-p_2)L. Neutrinos are ultra-relativistic, mk≪Em_k\ll E, and both components share essentially one path, so t≈Lt\approx L and E≈pE\approx p. Why: no honest simplification is available until we commit to m≪Em\ll E, which is spectacularly well satisfied — sub-eV masses against MeV–GeV energies.

Step 2. Take the equal-momentum assumption p1=p2=pp_1=p_2=p. Then Δϕ=(E1−E2)t\Delta\phi=(E_1-E_2)t, and expanding Ek=p2+mk2≈p+mk2/2pE_k=\sqrt{p^2+m_k^2}\approx p+m_k^2/2p gives E1−E2=(m12−m22)/2pE_1-E_2=(m_1^2-m_2^2)/2p. With t≈Lt\approx L and p≈Ep\approx E, ∣Δϕ∣=Δm2L/2E|\Delta\phi|=\Delta m^2 L/2E. Why: this is the textbook shortcut; the momentum term dies and the energy splitting is purely the mass term.

Step 3. Take instead the equal-energy assumption E1=E2=EE_1=E_2=E. Then Δϕ=−(p1−p2)L\Delta\phi=-(p_1-p_2)L, and pk=E2−mk2≈E−mk2/2Ep_k=\sqrt{E^2-m_k^2}\approx E-m_k^2/2E gives p1−p2=(m22−m12)/2Ep_1-p_2=(m_2^2-m_1^2)/2E, so again ∣Δϕ∣=Δm2L/2E|\Delta\phi|=\Delta m^2 L/2E. Why: the two assumptions look physically different but land on the same phase, because to leading order in m2/E2m^2/E^2 only the on-shell relation E2=p2+m2E^2=p^2+m^2 matters, not how we split the small difference between the EE and pp channels.

Step 4. Note the robustness. The apparent factor-of-two ambiguities that plague careless "equal time" arguments cancel once t≈Lt\approx L is imposed consistently, and a treatment with genuine wave packets — where each mass eigenstate is a localized bump moving at its own group velocity — reproduces Δϕ=Δm2L/2E\Delta\phi=\Delta m^2 L/2E and additionally predicts loss of coherence once the packets separate. Why: the plane-wave result is not an accident of a convenient assumption; it is the leading term of the correct wave-packet calculation, which is why it survives.

Go deeper · Derivation C · 1 minRestoring ħ and c to get the practical factor 1.267
Derivation CRestoring ħ and c to get the practical factor 1.267

The purpose here is to explain where the mysterious 1.2671.267 in equation (5) comes from, because it is not a physical constant but a bookkeeping factor that lets you feed in eV², kilometres, and GeV and read out a pure number in radians. In natural units the oscillation phase is Δm2L/4E\Delta m^2 L/4E; we reinsert the powers of ℏ\hbar and cc needed to make the three mismatched units cancel, then evaluate the resulting constant. The exercise also fixes, once and for all, that the same constant works for metres with MeV.

Step 1. Reinstate the constants. Dimensionally the phase must be Δm2c4 L4 ℏc E\dfrac{\Delta m^2 c^4\,L}{4\,\hbar c\,E}, since Δm2c4\Delta m^2 c^4 is an energy-squared, ℏc\hbar c carries the energy times length, and EE is an energy, leaving a dimensionless argument. Why: only this combination makes the units cancel; ℏc\hbar c is the single conversion constant between the natural-unit answer and laboratory units.

Step 2. Insert ℏc=1.973×10−7 eV m\hbar c=1.973\times10^{-7}\ \mathrm{eV\,m} and choose lab units Δm2\Delta m^2 in eV2\mathrm{eV}^2, LL in km =103=10^3 m, EE in GeV =109=10^9 eV. The numerical prefactor is 1034 (1.973×10−7) 109=1.267\dfrac{10^3}{4\,(1.973\times10^{-7})\,10^9}=1.267. Why: this is just arithmetic on the powers of ten and the value of ℏc\hbar c — nothing physical, but it is the number you cannot afford to get wrong.

Step 3. Read off equation (5): P=sin⁡22θ sin⁡2 ⁣(1.267 Δm2[eV2]L[km]/E[GeV])P=\sin^2 2\theta\,\sin^2\!\big(1.267\,\Delta m^2[\mathrm{eV}^2]L[\mathrm{km}]/E[\mathrm{GeV}]\big). Because km/GeV and m/MeV carry the same ratio of powers of ten, the identical 1.2671.267 serves for LL in metres and EE in MeV — the combination reactor and short-baseline experiments live in. Why: recognizing the scale invariance saves re-deriving the constant for every experiment; one number covers reactors, accelerators, and atmospheric neutrinos alike.

Limiting cases

CaseResultMeaning
No mixing, θ=0\theta=0P=0P=0flavour and mass bases coincide; each flavour propagates unchanged
Degenerate masses, Δm2=0\Delta m^2=0P=0P=0the two phases stay locked; no interference, even with full mixing
Maximal mixing, θ=45∘\theta=45^\circP=sin⁡2 ⁣(Δm2L/4E)P=\sin^2\!\big(\Delta m^2 L/4E\big)amplitude reaches 1; complete flavour conversion at the crest (atmospheric νμ→ντ\nu_\mu\to\nu_\tau)
Very short baseline, Δm2L/4E≪1\Delta m^2 L/4E\ll1P≈sin⁡22θ (Δm2L/4E)2P\approx\sin^2 2\theta\,\big(\Delta m^2 L/4E\big)^2probability rises quadratically from zero; near-detectors see no oscillation
Oscillation maximum, Δm2L/4E=π/2\Delta m^2 L/4E=\pi/2P=sin⁡22θP=\sin^2 2\thetafirst and largest peak; experiments are tuned to sit here
Long baseline / broad spectrum (averaged)⟨P⟩=12sin⁡22θ\langle P\rangle=\tfrac12\sin^2 2\thetafast oscillations wash out with energy resolution; only the mean amplitude survives

Worked examples

1 · Choosing a baseline from the oscillation length (confidence builder)

Reactor antineutrinos of energy E=4E=4 MeV are studied with the solar mass splitting Δm212=7.5×10−5 eV2\Delta m^2_{21}=7.5\times10^{-5}\ \mathrm{eV}^2. Over what distance does the oscillation develop, and why did KamLAND sit its detectors near 180 km?

Step 1. Use equation (6) with E=4 MeV=0.004 GeVE=4\ \mathrm{MeV}=0.004\ \mathrm{GeV}: Losc=2.48×(0.004)/(7.5×10−5)=2.48×53.3=132 kmL_\mathrm{osc}=2.48\times(0.004)/(7.5\times10^{-5})=2.48\times53.3=\mathbf{132\ km}. The first appearance maximum, at Losc/2L_\mathrm{osc}/2, sits near 66 km.

Step 2. A flux-weighted baseline of roughly 180 km is about 1.4 Losc1.4\,L_\mathrm{osc}, so KamLAND's reactor antineutrinos arrive well past the first minimum, where the survival probability is strongly suppressed and — crucially — energy-dependent, imprinting an oscillatory distortion across the spectrum rather than a flat deficit. A single deficit could be absorbed into flux uncertainty; a spectral wiggle is the fingerprint that fixed Δm212\Delta m^2_{21}.

Step 3. The same equation explains the atmospheric case: for Δm322=2.5×10−3 eV2\Delta m^2_{32}=2.5\times10^{-3}\ \mathrm{eV}^2 and E=1E=1 GeV, Losc=2.48/(2.5×10−3)=992 kmL_\mathrm{osc}=2.48/(2.5\times10^{-3})=\mathbf{992\ km} — comparable to distances through the Earth, which is precisely why upward-going GeV atmospheric νμ\nu_\mu that cross the planet are seen to disappear while downward-going ones are not.

2 · The T2K disappearance at the oscillation maximum (fully worked)

The T2K experiment fires a νμ\nu_\mu beam of mean energy E=0.6E=0.6 GeV to a detector L=295L=295 km away. Taking the atmospheric parameters Δm322=2.5×10−3 eV2\Delta m^2_{32}=2.5\times10^{-3}\ \mathrm{eV}^2 and near-maximal mixing sin⁡22θ23=1.0\sin^2 2\theta_{23}=1.0, find the νμ\nu_\mu survival probability.

Step 1. Evaluate the phase argument of equation (5): 1.267×(2.5×10−3)(295)0.6=1.267×0.73750.6=1.267×1.229=1.557 rad1.267\times\dfrac{(2.5\times10^{-3})(295)}{0.6}=1.267\times\dfrac{0.7375}{0.6}=1.267\times1.229=\mathbf{1.557\ rad}.

Step 2. This sits almost exactly at π/2=1.5708\pi/2=1.5708 — T2K's baseline and beam energy were chosen so the neutrinos reach the detector at the first oscillation maximum. Then sin⁡2(1.557)=(0.99991)2=0.99982\sin^2(1.557)=(0.99991)^2=\mathbf{0.99982}.

Step 3. The transition probability is P(νμ→ντ)=sin⁡22θ⋅sin⁡2(1.557)=1.0×0.99982=0.9998P(\nu_\mu\to\nu_\tau)=\sin^2 2\theta\cdot\sin^2(1.557)=1.0\times0.99982=0.9998, so the survival probability is P(νμ→νμ)=1−0.9998=0.0002P(\nu_\mu\to\nu_\mu)=1-0.9998=\mathbf{0.0002}.

Step 4. In this idealized maximal-mixing, single-splitting picture almost every muon neutrino has converted by the time it reaches Super-Kamiokande. At the oscillation maximum the νμ\nu_\mu beam essentially vanishes — the dramatic disappearance that long-baseline experiments are built to catch. (Real T2K mixing is close to but not exactly maximal, and the finite beam spectrum softens the dip, so the measured survival minimum is a few percent rather than zero.)

Physics of the portrait

Neutrino oscillations were a theorist's conjecture for forty years before an experiment forced them on the world. The idea belongs to one restless, brilliant, and politically improbable figure who kept asking whether the neutrino might be less simple than it looked.

Origins · 1 minBruno Pontecorvo and how this was discovered
BP
Bruno Pontecorvo
1913–1993 · the man who proposed neutrino oscillations

Bruno Pontecorvo trained in Enrico Fermi's Rome group in the 1930s — one of the "Via Panisperna boys" — and made his early name on slow-neutron physics and on the idea, later industrialized, of detecting neutrinos by inverse beta decay. In 1957, inspired by the newly discovered K0K^0–Kˉ0\bar K^0 oscillations, he proposed that neutrinos too might oscillate; with only one known neutrino species at the time he first framed it as a ν↔νˉ\nu\leftrightarrow\bar\nu transition, then, after the muon neutrino was found in 1962, recast it as the flavour oscillation we now use. In parallel, Maki, Nakagawa and Sakata wrote down the flavour-mixing matrix in 1962, and the modern mixing matrix carries all their names as the PMNS matrix. Pontecorvo also foresaw, in the 1960s, that the flux of neutrinos from the Sun would arrive depleted if oscillations were real — the interpretation eventually vindicated when the solar neutrino deficit measured by Davis was resolved. His life was as singular as his physics: in 1950, at the height of the Cold War, he defected from the West to the Soviet Union, where he continued to work at Dubna and where his oscillation idea was long treated as a curiosity. He did not live to see the 1998 Super-Kamiokande result that turned his conjecture into established fact, but the effect is, by any fair reading, his.

History
1957
— Pontecorvo proposes that neutrinos oscillate, by analogy with kaon mixing
1962
— Maki, Nakagawa and Sakata formulate neutrino flavour mixing
1968
— Davis and Bahcall report a large deficit of solar neutrinos at Homestake
1998
— Super-Kamiokande discovers atmospheric neutrino oscillations
2015
— Kajita and McDonald share the Nobel Prize for the discovery of oscillations

Going further

Texts. Thomson, Modern Particle Physics, §13.4–13.6 (neutrino oscillations and the PMNS matrix) · Griffiths, Introduction to Elementary Particles, 2nd ed., §11.6 (neutrino oscillations) · Halzen & Martin, Quarks and Leptons, Ch. 12 (weak mixing) · Perkins, Particle Astrophysics, Ch. 9 (solar and atmospheric neutrinos) · Giunti & Kim, Fundamentals of Neutrino Physics and Astrophysics (the comprehensive reference, including the wave-packet treatment). The key results of this article are: P=sin⁡22θ sin⁡2(Δm2L/4E)P=\sin^2 2\theta\,\sin^2(\Delta m^2 L/4E) from the rotate–evolve–project–square chain; Δϕ=Δm2L/2E\Delta\phi=\Delta m^2 L/2E from both the equal-momentum and equal-energy routes; the constant 1.2671.267 from ℏc=1.973×10−7 eV m\hbar c=1.973\times10^{-7}\ \mathrm{eV\,m}; Losc=2.48 E[GeV]/Δm2[eV2]L_\mathrm{osc}=2.48\,E[\mathrm{GeV}]/\Delta m^2[\mathrm{eV}^2] km; and the T2K phase argument 1.267×2.5×10−3×295/0.6=1.557≈π/21.267\times2.5\times10^{-3}\times295/0.6=1.557\approx\pi/2. The ultra-relativistic expansion Ek≈p+mk2/2pE_k\approx p+m_k^2/2p underpins the phase difference. Benchmark values used throughout are the standard global-fit numbers: Δm212≈7.5×10−5 eV2\Delta m^2_{21}\approx7.5\times10^{-5}\ \mathrm{eV}^2, Δm322≈2.5×10−3 eV2\Delta m^2_{32}\approx2.5\times10^{-3}\ \mathrm{eV}^2, sin⁡22θ12≈0.85\sin^2 2\theta_{12}\approx0.85, θ23≈45∘\theta_{23}\approx45^\circ.

Prerequisites. Mass and Weak Eigenstates · The Weak Charged Current · Non-relativistic Quantum Mechanics Review · Special-Relativistic Kinematics. Leads to. Three-flavour PMNS Mixing · Matter Effects and the MSW Resonance · Oscillation Experiments · Neutrino Mass Mechanisms.

Ask the tutor: Ask me to plug your own baseline, energy, and Δm2\Delta m^2 into the 1.267 formula, or to show how the two-flavour picture grows into the full three-flavour PMNS matrix with CP violation.

If the neutrino is emitted as one flavour, what is actually "waving" as it travels?

Not the flavour itself, but the relative phase of the two mass eigenstates that make it up. At production the two components ν1\nu_1 and ν2\nu_2 are locked in a particular phase relationship that spells one flavour. Because they have different masses they advance their quantum phases at slightly different rates, so that relationship rotates smoothly as the neutrino flies. When the relative phase has turned by π\pi the superposition spells the other flavour; when it has turned by 2π2\pi it spells the original flavour again. Nothing about the individual mass states changes flavour — flavour is a property of how they interfere, and the interference is what oscillates.

Why does only the mass-squared difference appear, and not the masses themselves?

Because the observable is a phase difference. Each mass eigenstate contributes a phase proportional to its energy, and in the ultra-relativistic limit that energy is Ek≈p+mk2/2pE_k\approx p+m_k^2/2p. The part common to both states, pp, contributes an overall phase that is identical for both components and cancels when you take their difference — an overall phase is unobservable in quantum mechanics. What remains is the difference of the mk2/2pm_k^2/2p terms, which is exactly Δm2/2p\Delta m^2/2p. So the mass scale and the individual masses live in the common phase that drops out, and only their squared difference survives to drive the oscillation.

Do antineutrinos oscillate the same way as neutrinos?

In two-flavour vacuum oscillations, yes, identically. The two-flavour formula depends only on sin⁡22θ\sin^2 2\theta and Δm2L/4E\Delta m^2 L/4E, none of which changes under charge conjugation, so P(νe→νμ)=P(νˉe→νˉμ)P(\nu_e\to\nu_\mu)=P(\bar\nu_e\to\bar\nu_\mu). Any difference between neutrino and antineutrino oscillation — CP violation in the lepton sector — requires at least three flavours and a nonzero complex phase in the mixing matrix, which cannot appear in a single real rotation angle. It can also be mimicked by matter effects, since ordinary matter contains electrons but not positrons and so treats νe\nu_e and νˉe\bar\nu_e differently. Both of those lie beyond this article, but their absence here is precisely why the two-flavour vacuum case is CP-symmetric.

How do you actually see an oscillation rather than just a missing flux?

A flat deficit is weak evidence: the source flux is often uncertain at the ten-percent level, so a uniform shortfall can always be blamed on the prediction. An oscillation leaves a sharper signature — the survival probability varies with L/EL/E in a specific sinusoidal way, so the deficit is energy-dependent and distance-dependent in the pattern sin⁡2(1.267 Δm2L/E)\sin^2(1.267\,\Delta m^2 L/E). KamLAND saw the reactor νˉe\bar\nu_e spectrum dip and recover across energy; Super-Kamiokande saw atmospheric νμ\nu_\mu disappear as a function of zenith angle, hence path length. Reconstructing that wiggle, not just the total count, is what distinguishes genuine oscillation from a mundane flux error and what lets a single dataset measure Δm2\Delta m^2 and θ\theta together.

Is two flavours ever enough, or is it just a warm-up for three?

It is a genuine and often excellent approximation, not merely a toy. Nature has three neutrinos, but the two mass-squared splittings are very different — the solar splitting is about thirty times smaller than the atmospheric one — so in many experiments one splitting dominates the relevant L/EL/E range and the third state decouples. Atmospheric and long-baseline νμ\nu_\mu disappearance is well described by a two-flavour νμ→ντ\nu_\mu\to\nu_\tau formula in (Δm322,θ23)(\Delta m^2_{32},\theta_{23}); solar and KamLAND data reduce to two-flavour (Δm212,θ12)(\Delta m^2_{21},\theta_{12}). The full three-flavour PMNS treatment is needed for sub-leading effects — νe\nu_e appearance driven by θ13\theta_{13}, CP violation, and the interference of the two splittings — but the two-flavour result captures the leading behaviour of most measurements to good accuracy.

What happens to the oscillation over very long distances or with a broad energy spread?

The clean sinusoid washes out into a constant. Real beams have a spread of energies, and a detector has finite energy resolution, so instead of a single value of Δm2L/4E\Delta m^2 L/4E you average sin⁡2\sin^2 over a range of phases. Once the phase varies by more than about π\pi across that range — which happens at large LL or with a broad spectrum — the oscillatory factor averages to 12\tfrac12, and the survival probability settles at 1−12sin⁡22θ1-\tfrac12\sin^2 2\theta. This is exactly the regime of solar neutrinos observed at Earth: the enormous baseline and the broad production region wash out the vacuum wiggle, leaving an averaged survival that (with matter effects included) explains the solar deficit. The information in Δm2\Delta m^2 is not lost, but it is read from where the averaging sets in, not from a resolved fringe.

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Where this leads