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Robust statistics studies procedures whose behavior remains controlled under outliers and deviations from an assumed model.

A stationary axisymmetric spacetime has commuting stationary and axial Killing vector fields, with the axial field having closed spacelike orbits.

A static spacetime has a timelike Killing vector that is hypersurface orthogonal. Coordinates adapted to it can be chosen with no time-space cross terms.

A strictly stationary spacetime has a globally defined Killing vector that is timelike everywhere.

If the phase derivative has no zero on the support of a smooth amplitude, repeated integration by parts makes the oscillatory integral decay faster than any prescribed inverse power, subject to corresponding decay and regularity of the amplitude.

If ${\psi }^{\prime }(k_0)=0$, ${\psi }^{\prime \prime }(k_0)\ne 0$, and $A$ is smooth near $k_0$, thenContributions from distinct stationary points add.

A stationary point $x_0$ of a smooth phase $\varphi$ is nondegenerate when its Hessian matrix at $x_0$ is an invertible matrix. In one dimension, this condition is ${\varphi }^{\prime \prime }(x_0)\ne 0$.

A macrostate groups microstates sharing prescribed coarse data. The grouping depends on what is retained: here retain only total energy. For the two distinguishable two-level systems, the macrostates $E=0,\Delta ,2\Delta$ have state degeneracies $1,2,1$. Although two units are not macroscopic in size, they make this loss of information visible: knowing $E=\Delta$ does not tell us which unit is excited.

At inverse temperature $\beta \Delta =\ln 3$, each unit's excited-state probability is $p=1/4$. Their independence gives microstate probabilities $9/16,3/16,3/16,1/16$ in the order above. Adding within each macrostate givesThe total expected value of energy is therefore $\Delta (6/16)+2\Delta (1/16)=\Delta /2$, matching two units each with expected value of energy $\Delta /4$. Equal state degeneracies would give the wrong answer: macrostate probabilities combine counting with the Boltzmann factor. At very high positive temperature, all four microstates become equally likely, but these three macrostate probabilities approach $1/4,1/2,1/4$.

A microstate is a complete microscopic specification within the chosen model. For two distinguishable, noninteracting two-level systems, label the units $A,B$ and their states $0,1$, with energies $0,\Delta$ and $\Delta >0$. The four microstates arewith total energies $0,\Delta ,\Delta ,2\Delta$. Distinguishability matters: $(0,1)$ and $(1,0)$ describe different assignments to the labeled units. Noninteraction matters too: their energies add without an extra coupling term.

For a classical particle model, a microstate can instead be a point in phase space, specifying every position and momentum. In the quantum canonical ensemble, the sum uses energy eigenstates; a general quantum state may also contain quantum coherence, which an energy label alone does not specify.

A degeneracy factor counts the distinct microscopic states that share the same macroscopic quantum numbers or energy.

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.

The electroweak interaction is the $SU(2{)}_L\times U(1{)}_Y$ gauge theory that unifies the weak and electromagnetic interactions.

An instructive tension motivates the unification: the photon is massless, while the W boson and Z boson are massive; electromagnetic interaction and weak interaction also have different observed low-energy strengths and chiral couplings. A gauge theory can relate their interactions while the Higgs field gives different masses after electroweak symmetry breaking. The resulting theory predicts relationships between processes, not merely a common name for observed phenomena.

Its useful organizing principle is the combination of weak isospin and hypercharge. The surviving electromagnetic generator is $Q=T_3+Y$ in the convention used here. The photon and Z boson are different mixtures of neutral gauge fields, while the charged current uses the charged combinations. The electroweak doublet gauge-boson mass matrix explains why one neutral mixture stays massless. At low energies, a massive W boson propagator instead produces the approximate Fermi interaction, withHere $g$ is the $SU(2{)}_L$ gauge coupling and $v$ the Higgs doublet vacuum expectation value. The inverse squared mediator mass suppresses low-energy weak rates. Unification does not require setting $g$ equal to the electromagnetic coupling $e$: their relation is $e=g\sin {\theta }_W$.

A striking experimental consequence is a neutral current in addition to the familiar charged current. The Gargamelle experiment tests this extra channel through visible charged secondaries, with a background problem fundamentally different from directly identifying a Z boson. The muon-neutrino electron recoil spectrum shows how the same Weinberg angle enters another process quantitatively.

A nonlinear sigma model has fields valued in a curved target space such as a vacuum manifold $G/H$. Its leading action is quadratic in spacetime derivatives but nonlinear in any unconstrained coordinates used for the target.

In a local quantum field theory obeying special relativity, with a positive physical state space, a conserved continuous internal global symmetry in field theory and a selected Lorentz-invariant ground state, a broken generator requires a massless Goldstone boson. For $G\to H$, there are $\dim G-\dim H$ symmetry-required Goldstone bosons in this setting; additional accidental massless excitations are possible. Jeffrey Goldstone's institutional biography identifies his work with Abdus Salam and Steven Weinberg on the zero-mass theorem.^[ref]

The Goldstone directions in the scalar mass matrix give a short classical proof at a smooth minimum. The quantum argument uses a conserved current $j^{\mu }$ and a scalar local operator $O$ whose expectation changes under the broken generator. The Ward identity for the current–local operator correlation function then has a nonzero contact term. After a Fourier transform, its divergence remains nonzero as four-momentum tends to zero. Lorentz invariance forces the vector–scalar correlator to have the form $p^{\mu }F(p^2)$, so $F$ must have a pole at $p^2=0$. The spectral representation associates that pole with a physical zero-mass excitation. A properly regulated spatial integral of the conserved current implements the broken generator; a well-defined global charge acting on the broken ground state cannot simply be assumed.

The hypotheses explain the boundaries of the result. A discrete symmetry has no infinitesimal generator and need not give a Goldstone boson. A gauge redundancy does not supply the physical global generator assumed here. In nonrelativistic matter the type-B Goldstone boson shows why one cannot universally count one independent mode per broken generator. Long-wavelength fluctuations can also prevent an assumed broken state from existing, as in the Mermin-Wagner theorem.

The vacuum manifold is the space of field configurations that minimize the energy. If a group $G$ acts transitively and a chosen vacuum has stabilizer $H$, its connected component is the homogeneous space $G/H$.

A rotationally invariant rank-two tensor is a scalar multiple of ${\delta }_{ij}$; taking its trace determines the scalar.

For an element $a$ of a complex Banach algebra,

Mantle convection is the slow buoyancy-driven motion of a rocky planetary mantle. On geological timescales the solid mantle behaves as a highly viscous Newtonian fluid to first approximation.

The largest prime factor $P^{+}(n)$ of an integer $n>1$ is the greatest prime number dividing $n$.

For a finite set $S$ of primes, an integer is $S$-smooth when every prime dividing it belongs to $S$. Bounding the largest prime factor is equivalent to restricting the integer to be $S$-smooth for a suitable finite $S$.