PMNS mixing and vacuum oscillations
Derive neutrino flavor interference with explicit PMNS conjugations, practical oscillation units, and limitations on ordering and Majorana-phase inference.
On this page
The question for today
What you’ll understand
- Construct flavor propagation amplitudes using a declared PMNS convention.
- Convert the vacuum oscillation phase into km, GeV, and electronvolt-squared units.
- Identify what two-flavor and phase-averaged observations cannot determine.
A neutrino created with a charged lepton has a weak flavor label, but its coherent components propagate with different masses. Their relative phases change the flavor-dependent detection amplitude. Oscillation experiments measure those phase differences and mixing combinations, rather than tracking a particle that classically changes an internal label. We will define the PMNS matrix and its conjugations explicitly, derive a two-flavor limit, and keep practical baseline units separate from natural-unit formulas. Production and detection coherence are assumptions to be examined later.
Flavor states and propagation fix the conjugations
Use , with alpha labeling electron, muon, or tau flavor and i the mass eigenstate. For ultrarelativistic neutrinos of common characteristic energy E, remove an irrelevant common phase and evolve the mass components with in natural units. Projecting on flavor beta gives an amplitude with , not two unconjugated entries. Unitarity makes the zero-baseline amplitude the appropriate Kronecker delta and conserves total probability across the three active flavors.
Choose , with real rotations having positive sine above and negative sine below the relevant diagonal. The 13 complex entry is , and contains possible Majorana phases. Each column phase cancels between the two U factors in an ordinary oscillation amplitude. For antineutrinos in vacuum replace U by its complex conjugate. A three-flavor CP asymmetry can depend on delta, whereas these Majorana phases cannot be extracted from ordinary flavor oscillation probabilities.
The phase contains a specific factor of four
In a real two-flavor reduction, define the signed splitting and mixing angle theta through the same real rotation convention. Subtracting the two propagation amplitudes yields a sine of half their relative phase. The transition probability therefore contains , not the sine squared of the full relative phase. Squaring makes this two-flavor vacuum probability insensitive to the sign of the splitting. It cannot by itself establish a mass ordering or exhibit intrinsic CP violation.
For practical units, the sine argument is 1.267 times the splitting in electronvolts squared times baseline in kilometres divided by energy in GeV. Using metres and MeV gives the same numerical coefficient because their ratios are equal. An extra conversion factor of a thousand would be an error. Oscillation wavelengths grow with energy and shrink with splitting magnitude. The first transition maximum sets the phase to pi over two, while the full probability period corresponds to a phase increase of pi. Always identify which of these distances a quoted oscillation length denotes.
Experimental averaging is part of the prediction
A detector generally records a distribution of production points, energies, and reconstructed resolutions. Averaging a rapidly varying sine squared gives one half when the phase is well sampled, leaving a transition probability of one half times the mixing prefactor. This need not be one half for nonmaximal mixing. Such averaging is different from a proof that each neutrino lost microscopic coherence. A sufficiently resolved spectrum can retain oscillatory information even when a coarse total count does not. The wavepacket lesson separates these physical and statistical mechanisms.
For three-flavor naming choose : normal ordering means , and inverted ordering means . This labeling does not determine the lightest mass. Several splittings, appearance channels, and neutrino-antineutrino comparisons constrain the angles and CP phase jointly. Matter effects must also enter long-baseline analyses. The T2K and NOvA joint analysis released in October 2025 reported no statistically significant preference between mass orderings; its strongest CP evidence was conditional on inverted ordering. This dated result illustrates why a preferred fit value is not a settled ordering or an unconditional CP discovery. The elementary two-state formulas here explain phase scales, not that full experimental inference.
Work it through
Locate a first vacuum maximum
Use and . Find the first-maximum L/E and the corresponding baseline for energy 2 GeV in the two-flavor vacuum approximation.
The first maximum requires . The units in this equation are km per GeV for L over E.
Solving gives . This is half the full probability-period baseline per unit energy.
At 2 GeV the baseline is approximately 992 km. The phase factor is one at that point, so the transition probability equals its mixing prefactor, 0.80.
The first maximum is at about 496 km/GeV, or 992 km for 2 GeV, with transition probability 0.80 in the stated vacuum model.
The living notebook
Explore the model
Interactive lab · quantum
Relative phase need not change the chosen basis probabilities
Reset and set BOTH Mixing angle θ = 60° and Relative phase φ = 0°; predict P(1) = 0.25 and positive Bloch x. For a fresh comparison, Reset and set θ = 60° and φ = 180°; predict the same P(1) and opposite Bloch x. Inspect both readouts at Reset time.
- Probability |0⟩
- 71.1%
- Probability |1⟩
- 28.9%
- Bloch (x, y, z)
- 0.78, 0.45, 0.42
A normalized two-level pure state, not an interacting field simulation. Playback adds one radian per second to the relative phase; basis probabilities stay fixed. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.
Look forThe pure-state lab displays phase-sensitive geometry and fixed computational-basis populations. Its playback does not rotate between neutrino flavor and mass bases or solve PMNS propagation.
Pause & reason
Check your understanding
Your turn
Try it yourself
For two-flavor vacuum mixing with , average over many unresolved oscillation phases. Find transition and survival probabilities. Does this establish complete microscopic decoherence?
Take a moment to make a prediction or work it out on paper. Open a hint when you need one.
Give me a hint
Average the oscillatory sine squared before multiplying by the mixing prefactor.
Compare with the solution
The mixing prefactor is , while the phase average is one half. Transition probability is therefore and survival probability . Their sum is one. These unequal values reflect nonmaximal mixing, not missing probability. An unresolved energy or baseline distribution can produce this same average from individually coherent events, so the averaged probabilities alone do not identify microscopic wavepacket separation or another physical decoherence mechanism.
Keep the idea
Take it with you
- The stated flavor-state convention fixes the U conjugations in propagation amplitudes.
- The practical vacuum sine argument uses 1.267 with eV squared, km, and GeV.
- Two-flavor vacuum data and unresolved phase averages have specific limits on ordering, CP, and coherence inference.
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