Under , one Standard Model fermion generation including a right-handed neutrino is
The Standard Model is a gauge theory with group , matter quarks and leptons, gauge bosons and a Higgs field. It combines Quantum chromodynamics with the electroweak interaction. Its successes do not make its field content a complete account of nature. Established missing phenomena should be distinguished from theoretical questions about its parameters.
neutrino oscillation demonstrates nonzero mass-squared differences and mixing of flavor states. The minimal renormalizable Standard Model has no right-handed neutrino and no neutrino mass term. The atmospheric experiment compared zenith-angle distributions of muon-like and electron-like events in a large water Cherenkov detector. A direction-dependent muon-neutrino deficit, with different path lengths through Earth and comparison samples, discriminated against a uniform flux-normalization error.[ref] One extension adds right-handed neutrinos and small Dirac Yukawa couplings; another has a Majorana mass term and seesaw mechanism, with light eigenvalue of order . Oscillations alone do not decide whether neutrinos are Majorana neutrinos.
dark matter is inferred from gravitational observations such as galactic motions and gravitational lensing; Standard Model particles do not supply the required dominant cold component. Active neutrinos contribute some matter but cannot constitute all the cold dark matter. A new stable weakly interacting particle, an axion, or other hidden-sector states are possible explanations, with different scattering, production and astrophysical signals. Dark-matter evidence does not identify a particular new particle. The institutional account distinguishes gravitational evidence from proposed particle candidates.[ref]
The matter-antimatter imbalance poses a different problem. Dynamical baryogenesis needs Sakharov conditions, including baryon-number violation, CP violation and departure from thermal equilibrium. Although the Standard Model contains relevant ingredients in principle, they do not generate the observed asymmetry in its conventional thermal history with measured parameters. Additional CP phases, a stronger electroweak transition, or leptogenesis from heavy Majorana neutrinos are possible extensions. Each needs a quantitative mechanism.
gravity is absent as a dynamical quantum interaction, motivating quantum gravity and unification. The hierarchy problem asks why the Higgs mass scale is small compared with much higher scales when scalar masses receive sensitive quantum corrections. supersymmetry can cancel particular contributions between partner fields if its breaking pattern is suitable; compositeness gives another interpretation of the Higgs sector. Neither motivation proves that the corresponding new particles exist. The Strong CP problem asks why the allowed QCD CP-violating parameter is so small; an axion mechanism is one possible answer.
A grand unified theory embeds the separate gauge factors in a larger group and can relate couplings or fermion representations, sometimes predicting proton decay. Its tests differ from dark-matter or neutrino-mass searches. A useful extension must explain a specified deficiency, preserve successful low-energy predictions and supply distinguishable experimental consequences. Attractive new symmetries alone are not evidence.
The known active neutrinos are too light and too fast to supply the dominant cold dark matter. Their relativistic decoupling leaves substantial free streaming, which erases rather than seeds sufficiently small-scale structure; their allowed mass density is also inadequate for the dominant cold component. Changing a light active neutrino from Dirac to Majorana does not remove those problems. What can change the picture is an enlarged neutral-fermion sector containing sterile states with different masses, production and decay rates. A sufficiently long-lived sterile neutrino in a Majorana state can be a dark-matter candidate; Majorana character alone supplies neither stability nor the correct abundance.
For the spinor calculation, put and define , . Applying the given chiral projectors gives
Consequently
where the last equality uses . Same-chirality Lorentz scalar products instead vanish: for example . The nonzero overlaps demonstrate the Lorentz scalar structures coupling left and right chirality. For to this is a particle-number-preserving Dirac coupling; for to the charge-conjugate sector it can describe a lepton-number-violating Majorana coupling.
There is a normalization subtlety: both displayed overlaps equal the on-shell mass parameter used to define the spinors. A chiral scalar spinor overlap verifies a coupling structure without fixing an independent Lagrangian coefficient . Repeating the on-shell construction with mass parameter would instead give the corresponding overlap ; this is a different input, rather than a newly derived parameter. The independent coefficients of a Dirac mass term and a Majorana mass term are defined by
The Majorana terms connect a field with its charge conjugate and violate the corresponding continuous lepton phase symmetry by two units. With only unbroken Standard Model gauge symmetry, a left-handed Majorana mass also requires electroweak symmetry breaking or an appropriate higher-dimensional operator; it is not an arbitrary gauge-invariant bare mass for a lepton doublet.
Use an all-left-handed Weyl basis . For real parameters the one-family Dirac-Majorana mass matrix is
Writing gives an orthogonal diagonalization, with up to the rotation-sign convention. Massive-particle chirality and helicity are not identical; the familiar left/right helicity language becomes an approximation in the relativistic regime.
The characteristic polynomial is
Its roots are
For Majorana fermions the nonnegative physical masses, as explained by physical Majorana mass and signed eigenvalue, are after a possible field rephasing; a negative real eigenvalue is not a negative physical rest mass. When ,
The light state is predominantly , while the heavy state is predominantly . Each mass eigenstate combines its Weyl component and charge conjugate to form a Majorana field.
For , the heavy mass is approximately . In the type-I limit ,
The seesaw light-mass estimate needs a Dirac scale: no unique numerical light mass follows because the Dirac mass and were not supplied. As an explicitly conditional illustration, choosing and gives ; this is an assumed Dirac scale, not additional exam data or a prediction from alone. A heavy seesaw state is also not automatically stable enough to be dark matter.
Figure 1.
A large right-handed mass produces reciprocal light and heavy scales
. Original exact one-family eigenvalues for , expressed relative to an unspecified fixed Dirac mass. Negative signed eigenvalues are shown by their positive physical masses; no numerical Dirac mass is assumed. Details.
The conventional minimal Pati-Salam model gauge group is
The group printed in this paper is different: it contains two factors and only one . This is a discrepancy in the original PDF, not just in the transcription. The standard-model discussion below uses the conventional intended Pati-Salam model model. A literal theory with the printed product would require additional fermion representations and symmetry-breaking data that are not specified.
The Pati-Salam model unifies the three quark color charges with lepton number as a fourth color charge. A family forms left-handed and right-handed multiplets, including a right-handed neutrino. The extended color charge group contains quark-lepton gauge bosons, while the right-handed weak factor supplies right-handed charged currents after symmetry breaking. The Pati-Salam charge embedding is
The original paper explicitly develops the smaller local subgroup , as well as a larger underlying global structure; neither distinction licenses silently replacing the printed group.[ref] The product group is a quark-lepton unification scheme rather than a simple gauge group with one automatically common coupling. Breaking the right-handed and symmetries can generate a large and light/heavy Majorana neutrinos through the seesaw. The gauge group alone does not uniquely fix their masses or guarantee a dark-matter lifetime.
The most important laboratory test of Majorana character is neutrinoless double beta decay,
with no outgoing neutrinos. Under light-neutrino exchange, the amplitude involves
The coherent squared mixing elements allow phase cancellations. A null result constrains this combination within the assumed mechanism, rather than proving that all neutrinos are Dirac.
The observable is a peak in summed electron energy at the decay Q value, unlike the continuous two-neutrino spectrum. Enriched source material, large exposure, good energy resolution, underground operation and radiopure construction suppress backgrounds. germanium arrays use the source as a semiconductor detector; xenon time-projection chambers combine ionization, light and event-position information; bolometers measure deposited energy through a temperature rise. The GERDA collaboration's Phase-I study is a concrete example of an enriched-germanium source-detector search with background suppression.[ref] energy calibration, resolution tails, radon and material backgrounds, cosmic-ray vetoes, signal-like event topology and sideband fits all need independent checks before a Q-value excess is convincing. Collider same-sign dilepton processes can test heavier Majorana states, but require a specified production and decay mechanism. Lepton-number violation, absolute-mass measurements and oscillation data provide complementary information; oscillations alone do not settle Majorana character.
Pati-Salam model Created 2026-10-20 Updated 2026-10-25
A quark-lepton unification framework with conventional minimal gauge group . leptons supply a fourth color charge, and a right-handed neutrino completes each family. fermion masses additionally depend on symmetry breaking and Yukawa couplings.
Pati-Salam neutrino hypercharge cancellation Created 2026-10-20 Updated 2026-11-05
For the right-handed neutrino, and , so . Its colour-singlet and left-weak-singlet assignments make it sterile under the Standard Model after symmetry breaking.
Right-handed neutrino Created 2026-09-24 Updated 2026-11-05
A right-handed neutrino transforms as under , so it is neutral under every Standard Model gauge interaction.
Standard Model fermion Created 2026-09-24 Updated 2026-11-05
A Standard Model generation contains left-handed quark and lepton doublets and right-handed up-quark, down-quark and charged-lepton singlets. A right-handed neutrino may be added as a gauge singlet.
Standard Model gauge singlet neutrino Created 2026-10-20 Updated 2026-11-05
A right-handed neutrino can transform as under colour, weak isospin and hypercharge. It has no direct Standard Model gauge coupling, but may mix with active neutrinos. Sterility under the low-energy group does not imply sterility under an enlarged unbroken gauge group.