Dirac, Majorana masses, and lepton number
Distinguish neutrino mass operators and their symmetries, derive a one-generation seesaw estimate, and separate oscillation evidence from mass-nature evidence.
On this page
The question for today
What you’ll understand
- Identify lepton-number conservation or violation in a mass term.
- Obtain light and heavy scales in a controlled one-generation seesaw.
- Separate absolute-mass observables from tests of Majorana nature.
Neutrino oscillations establish nonzero mass-squared differences, but they do not identify the symmetry of the mass term. A neutral fermion can have a Dirac mass linking independent chiral fields or a Majorana mass linking a field to its charge conjugate. These alternatives differ in lepton-number symmetry and possible processes, even when their ordinary relativistic oscillation probabilities coincide. We will inspect the operators, derive a simple seesaw hierarchy, and state precisely what an absolute-mass measurement would and would not resolve.
Symmetry assignments distinguish two mass constructions
A Dirac term links an active left-handed neutrino to an independent right-handed gauge singlet. Assign both fields lepton number one and the term conserves total lepton number. A Majorana term can instead couple a neutral chiral field to itself through charge conjugation, changing lepton number by two under the same assignment. The factor one half avoids counting identical field contractions twice. A nonzero electric charge would forbid such a same-field mass term by gauge invariance; neutrino neutrality makes the possibility available.
These are low-energy mass structures, not complete electroweak gauge-invariant ultraviolet theories by themselves. An active left-handed Majorana mass requires additional symmetry-breaking structure or an effective operator before the Higgs field gains its expectation value. A sterile right-handed Majorana mass is gauge allowed already. An exactly Dirac description requires the lepton-number-violating terms to be absent through a symmetry or another specified construction. Merely setting them numerically small in one displayed matrix does not explain why quantum corrections in a larger theory should preserve that choice.
A large sterile Majorana scale produces a small light mass
For this real one-generation matrix, the ordinary algebraic eigenvalues are . One is negative. Physical Majorana masses are nonnegative singular values obtained by a Takagi transformation of the complex symmetric mass matrix; a field phase converts that negative sign into a positive mass while carrying the associated phase information. In the limit , the light mass magnitude is approximately m D squared over M R, while the heavy mass is approximately M R.
The small active-sterile mixing angle is approximately m D over M R in this same hierarchical limit. This explains why a heavy state can alter the light mass while having an extremely small admixture in low-energy charged currents. It does not prove that nature uses this mechanism or fix a unique heavy scale. Several generations introduce matrix structure, cancellations, and additional parameters; a one-generation numerical estimate cannot reconstruct them. If the hierarchy is absent, the approximation must be replaced by the exact diagonalization rather than extrapolated beyond its expansion parameter.
Existing evidence establishes masses without identifying their nature
The two distinct nonzero oscillation-splitting scales imply at least two nonzero neutrino masses in the three-active-state interpretation. They leave the lightest mass undetermined and cancel possible Majorana phases from ordinary oscillations. A beta-endpoint spectrum instead probes an incoherent weighted mass-squared combination because the emitted mass alternatives are unobserved orthogonal final states. The KATRIN result published in 2025, based on 259 measurement days, reports at ninety percent confidence. This is a bound on an effective kinematic mass, not a detection of a nonzero absolute mass or a Majorana signal.
Cosmological mass constraints involve neutrino effects on cosmic evolution and require a cosmological model and data assumptions. They do not by themselves identify lepton-number violation. A Majorana mass would permit such violation in principle, but relativistic weak production and detection select helicities and can suppress the accessible rates enormously. Calling neutrino and antineutrino the same Majorana particle therefore does not imply that a laboratory beam immediately converts into an unsuppressed opposite-charge weak signal. The next lesson examines a dedicated lepton-number-violating search and the assumptions needed to interpret its absence or discovery.
Work it through
A hierarchical mass estimate with unit conversion
In the real one-generation seesaw model take and . Estimate the light mass in electronvolts, heavy mass, and active-sterile mixing angle.
The expansion parameter is , so the assumed hierarchy is excellent. The heavy mass is approximately .
The light mass magnitude is . Multiplying by one billion electronvolts per GeV gives .
The mixing angle magnitude is approximately radians. Its squared admixture is of order ; the signed algebraic light eigenvalue is not a negative physical rest mass.
The light mass is about 0.001 eV, the heavy mass about 10^14 GeV, and the active-sterile mixing angle about 10^−13 radians in this illustrative model.
The living notebook
Explore the model
Interactive lab · quantum
Small amplitude angles give quadratically small weights
Reset and set BOTH Mixing angle θ = 10° and Relative phase φ = 0°; predict P(1) = sin²5° ≈ 0.0076, shown as about 0.8%. For a fresh comparison, Reset and set θ = 20° and φ = 0°; predict sin²10° ≈ 0.0302, shown as about 3.0%.
- 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 nearly fourfold change illustrates squared small-angle amplitudes; the lab uses θ/2. These are reachable illustrative angles, not the tiny seesaw estimate, and the instrument does not diagonalize a Dirac or Majorana mass matrix.
Pause & reason
Check your understanding
Your turn
Try it yourself
Assume the same one-generation hierarchy and choose . What sterile Majorana scale gives , and what mixing angle does this imply?
Take a moment to make a prediction or work it out on paper. Open a hint when you need one.
Give me a hint
Convert the light mass to GeV before solving for the heavy scale; then check the expansion parameter.
Compare with the solution
The requested light mass is . Solving the leading relation gives . The mixing estimate is radians, validating the hierarchy. This scale is conditional on the chosen Dirac mass and simple mass texture; the light mass alone would not determine it if those inputs were unknown or additional generations contributed.
Keep the idea
Take it with you
- Dirac and Majorana mass terms differ through lepton-number symmetry.
- The seesaw estimate requires a declared mass texture and a large hierarchy.
- Oscillation splittings and kinematic mass bounds do not establish Majorana nature.
Read further
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