On this page
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.