oscillations

The PMNS Mixing Matrix: Structure of Neutrino Mixing

· 12 min read · Editorial

The 3×3 unitary matrix that relates neutrino flavor eigenstates to mass eigenstates — its parametrization, measured angles, and the CP-violating phase.

Once it was established that neutrinos oscillate, the field needed a language for the mismatch between the states that are produced by the weak interaction and the states that propagate freely through space. That language is the PMNS matrix: a 3×3 unitary matrix that rotates flavor eigenstates into mass eigenstates. Its entries are the mixing amplitudes. Its parameters are the mixing angles and the CP-violating phase. It is the central object of modern neutrino phenomenology, and its measurement has been the organizing goal of more than a dozen experiments over the past two decades.

What the matrix does

A neutrino produced by a charged-current weak interaction emerges in a definite flavor eigenstate, , or — set by the charged lepton it was produced alongside. A neutrino travelling freely through space, however, must be in an eigenstate of the Hamiltonian, which for a relativistic particle means an eigenstate of mass.

The two bases are connected by a linear transformation: where labels flavor and labels mass. The matrix with entries is the PMNS matrix. Unitarity — — is the statement that the two bases are both complete and orthonormal. Probability is conserved: the nine entries in each row or column sum to one.

The standard parametrization

Any 3×3 unitary matrix can be written in terms of three rotation angles and phases. The standard PDG parametrization of the PMNS matrix uses three mixing angles , , and a single Dirac CP-violating phase :

where and . The three matrices correspond, from left to right, to the atmospheric, reactor, and solar mixing sub-rotations — and each is anchored experimentally in a different set of measurements.

If neutrinos are Majorana particles, two further phases appear in a diagonal matrix applied on the right. These Majorana phases do not affect oscillation probabilities and can only be probed by lepton-number-violating processes, most notably neutrinoless double-beta decay.

Measured values

Three decades of oscillation experiments have produced precise measurements of the three angles and the two mass-squared differences:

Solar sector. is the solar mixing angle, measured by SNO’s neutral-current/charged-current comparison and confirmed by KamLAND’s reactor-antineutrino measurement. Current world-average value: , giving .

Atmospheric sector. is the atmospheric mixing angle, measured by Super-Kamiokande from the zenith-angle dependence of atmospheric disappearance, and now refined by accelerator experiments T2K and NOvA and by atmospheric-neutrino analyses at IceCube-DeepCore. Current value: , giving — close to maximal, with the “octant” (whether it is above or below 45°) not yet definitively resolved.

Reactor sector. is the reactor mixing angle, measured in 2012 by Daya Bay, RENO, and Double Chooz from short-baseline disappearance at reactor sites. Current value: , giving . It is the smallest of the three but is non-zero at better than 10 standard deviations — a finding that opened the door to CP-violation measurements.

CP phase. is measured by comparing and appearance rates in accelerator experiments. T2K and NOvA have published preliminary fits preferring near , but the combined global significance is still below five sigma. JUNO, DUNE, and Hyper-Kamiokande will settle it in the next decade.

Mass-squared differences. Oscillation measures two independent : The sign of — the mass ordering — is the one remaining unknown. “Normal ordering” has ; “inverted ordering” has . JUNO’s 2025 reactor-spectrum measurement is on track to settle this in the near term.

Why the structure matters

Three features of the PMNS matrix have no counterpart in the quark-mixing CKM matrix, and each tells us something about the deeper structure of the lepton sector.

Two angles are large. In the quark sector the analogous angles are all small — the largest, the Cabibbo angle, is about 13°. In the neutrino sector and are both very large, and is the only small one. No compelling flavor-model explanation of this striking contrast has yet emerged.

CP violation is potentially large. The Jarlskog invariant, the basis-independent measure of CP violation, is With the measured angles, can be as large as — more than thirty times the quark-sector value of . If turns out to be near , the leptonic CP violation is close to maximal — a hint that the matter-antimatter asymmetry of the universe may trace to lepton-sector physics via leptogenesis.

Unitarity is a testable assumption. The PMNS matrix is unitary in the Standard Model because the three active neutrinos exhaust the light-neutrino spectrum. A fourth, sterile, species would make the 3×3 sub-block non-unitary. Unitarity triangles in the lepton sector — analogous to the quark-sector triangles used to test the CKM matrix — are the subject of active experimental programs at short-baseline reactor and accelerator experiments.

Measuring CP violation

The observable for leptonic CP violation in long-baseline experiments is the difference between neutrino and antineutrino appearance probabilities: This asymmetry depends on through , with matter effects contributing an additional asymmetry of the same sign as — which means the CP and mass-ordering measurements are entangled. DUNE, with its 1300 km baseline and broad energy beam, will have enough matter sensitivity to break the degeneracy. Hyper-Kamiokande, with a shorter baseline, will complement the measurement with cleaner CP sensitivity and less matter-ordering ambiguity.

The target is a five-sigma determination of the sign of — the first observation of CP violation in the lepton sector.

Open questions

Even after the PMNS framework has been measured with sub-percent precision on most of its parameters, three open questions define the next decade:

Mass ordering. JUNO and DUNE each have independent pathways to the sign of . A determination is expected within a few years.

Octant of . Whether is above or below 45° discriminates between flavor-model classes. NOvA and T2K have mild tensions that future long-baseline data will resolve.

CP phase. The value of — and its implications for whether leptonic CP violation could account for the matter-antimatter asymmetry — is the central measurement goal of DUNE and Hyper-Kamiokande.

The PMNS matrix was written down in 1962 as a formal possibility, dismissed for decades as phenomenologically irrelevant, and then — between 1998 and 2012 — measured element by element. The next decade will complete it.

FAQ

Frequently asked

Why is the mixing matrix named PMNS?
Bruno Pontecorvo proposed neutrino oscillation in 1957. Ziro Maki, Masami Nakagawa, and Shoichi Sakata wrote down the explicit flavor-mixing structure in 1962. The acronym preserves both contributions — Pontecorvo for the idea of oscillation, MNS for the matrix form.
How does the PMNS matrix differ from the CKM quark-mixing matrix?
Structurally they are the same kind of object — a 3×3 unitary matrix parametrized by three angles and a CP phase. The difference lies in the values. Quark mixing angles are all small and hierarchical. Neutrino mixing angles are large, with two of them close to maximal. The neutrino sector is as different from the quark sector as a 3×3 unitary matrix can be.