Oscillations · Part 3 of 7

Three Flavours and the PMNS Matrix

With three neutrinos, mixing is described by a single 3×3 matrix — three angles and a phase. Those few numbers encode every oscillation, including the possibility that neutrinos and antineutrinos behave differently.

9 min read · Updated June 19, 2026

Nature uses three neutrino flavours, so the two-flavour rotation becomes a rotation in three dimensions. The object that performs it is the Pontecorvo–Maki– Nakagawa–Sakata (PMNS) matrix — the leptonic counterpart of the CKM matrix that mixes quarks.

The matrix

Each flavour state is a superposition of the three mass states, with the coefficients collected in the unitary PMNS matrix UU:

(νeνμντ)=(Ue1Ue2Ue3Uμ1Uμ2Uμ3Uτ1Uτ2Uτ3)(ν1ν2ν3).\begin{pmatrix} \nu_e \\ \nu_\mu \\ \nu_\tau \end{pmatrix} = \begin{pmatrix} U_{e1} & U_{e2} & U_{e3} \\ U_{\mu 1} & U_{\mu 2} & U_{\mu 3} \\ U_{\tau 1} & U_{\tau 2} & U_{\tau 3} \end{pmatrix} \begin{pmatrix} \nu_1 \\ \nu_2 \\ \nu_3 \end{pmatrix}.

A general 3×3 unitary mixing matrix of this kind is parameterised by three mixing angles and one CP-violating phase:

  • θ12\theta_{12} — the “solar” angle, dominant in solar-neutrino oscillation;
  • θ23\theta_{23} — the “atmospheric” angle, dominant for atmospheric and accelerator muon neutrinos;
  • θ13\theta_{13} — the smallest angle, the last to be measured, which links the other two sectors and gates access to the phase;
  • δCP\delta_{\mathrm{CP}} — the CP-violating phase, which can make neutrinos and antineutrinos oscillate differently.

(If neutrinos are their own antiparticles, two further “Majorana phases” exist, but they do not affect oscillation.)

Two mass splittings

Three masses define two independent mass-squared differences:

  • Δm212≈7.5×10−5 eV2\Delta m^2_{21} \approx 7.5\times 10^{-5}\,\mathrm{eV}^2 — the small “solar” splitting;
  • Δm312≈2.5×10−3 eV2\Delta m^2_{31} \approx 2.5\times 10^{-3}\,\mathrm{eV}^2 — the large “atmospheric” splitting, about thirty times larger.

The hierarchy of scales is what allows the two-flavour approximation to work so well in practice: most experiments are sensitive to one splitting at a time. The measured angles are large compared with their quark counterparts — leptonic mixing is “big,” a fact still not fully understood.

Why θ₁₃ mattered so much

For years θ13\theta_{13} was consistent with zero, and its smallness was a genuine obstacle. It matters because the CP-violating phase δCP\delta_{\mathrm{CP}} only shows up in oscillation multiplied by θ13\theta_{13}: if θ13\theta_{13} were zero, leptonic CP violation would be inaccessible through oscillation. The 2012 discovery that θ13\theta_{13} is comfortably non-zero (Part 5) therefore did more than complete the table of angles — it opened the door to searching for the matter–antimatter asymmetry in neutrinos.

CP violation in one line

CP violation means a difference between P(νμ→νe)P(\nu_\mu \rightarrow \nu_e) and P(νˉμ→νˉe)P(\bar\nu_\mu \rightarrow \bar\nu_e). In the PMNS framework this difference is controlled by δCP\delta_{\mathrm{CP}} and is only non-zero if all three angles are non-zero. It is of deep interest because a matter–antimatter asymmetry in the lepton sector could, through the mechanism of leptogenesis, help explain why the universe is made of matter at all.

In context. The PMNS framework assumes neutrinos travel through empty space. In real experiments they often pass through the Sun or the Earth, where interactions with matter modify oscillation dramatically — the MSW effect, next.

Key takeaways

  • Three-flavour mixing is encoded in the unitary PMNS matrix.
  • It has three angles (θ12,θ23,θ13\theta_{12},\theta_{23},\theta_{13}) and one CP-violating phase (δCP\delta_{\mathrm{CP}}).
  • Two independent mass splittings exist: solar Δm212\Delta m^2_{21} and the ~30× larger atmospheric Δm312\Delta m^2_{31}.
  • A non-zero θ13\theta_{13} is the gateway to measuring δCP\delta_{\mathrm{CP}}.
  • Leptonic CP violation could help explain the matter–antimatter asymmetry of the universe.

References

  1. 1.S. Navas et al. (Particle Data Group), Review of Particle Physics — Neutrino Masses, Mixing, and Oscillations, Phys. Rev. D (2024). DOI: 10.1103/PhysRevD.110.030001.
  2. 2.Z. Maki, M. Nakagawa, S. Sakata, Remarks on the Unified Model of Elementary Particles, Prog. Theor. Phys. (1962). DOI: 10.1143/PTP.28.870.