Past exam of the particle and nuclear physics course of the University of Cambridge / 2016 / Paper 1 / 2 / c

The Standard Model is a gauge theory with group $SU(3{)}_c\times SU(2{)}_L\times U(1{)}_Y$, 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 $m_D^2/M$. 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.