A demagnetizing factor relates a component of demagnetizing field to magnetization. The three principal factors of a uniformly magnetized ellipsoid sum to one in the International System of Units. Factors quoted in a different unit convention need conversion; state the convention and measurement geometry before applying them.

Couple the nucleon isospin $1/2$ to the pion isospin $1$. The highest state $|3/2,3/2⟩=|p{\pi }^{+}⟩$ is normalized. One application of the total isospin lowering operator gives $|3/2,1/2⟩=\sqrt{2/3}|p{\pi }^0⟩+\sqrt{1/3}|n{\pi }^{+}⟩$. For a common isospin-invariant two-body decay amplitude, the partial decay rates relative to the ${\Delta }^{++}$ channel are $2/3$ and $1/3$. The lowest state gives ${\Delta }^{-}\to n{\pi }^{-}$. Exact relations assume isospin-degenerate masses and common kinematic factors; electromagnetic and quark-mass differences cause corrections.

A delayed feedback characteristic root solves the characteristic equation of a delay differential equation and supplies an exponential function mode. Its real part determines decay or growth of that mode.

The degree sequence of a labelled graph records the degree of a vertex at each label. The handshaking lemma gives ${\sum }_i{d}_i=2|E|$. A nonincreasing list forgets the assignment of degrees to labels unless a particular ordering is specified.

The reference configuration is a chosen arrangement used to label a body's material particles and measure their subsequent deformation. A particle at $\mathbf{X}$ in the chosen reference has position $\mathbf{x}=\mathbf{\chi }(\mathbf{X},t)$ in the current configuration. The reference coordinates are Lagrangian coordinates and remain attached to the particles.

The initial shape of a specimen is a convenient reference, but a reference configuration need not be stress-free. A preloaded or residually stressed specimen can also be chosen as the reference. For example, engineering strain compares length with the chosen original gauge length, while the deformation gradient compares infinitesimal material line elements. Current and reference mass densities satisfy $\rho J={\rho }_0$ for conserved mass, with $J$ the local volume ratio. Keeping this choice explicit prevents mixing stress or strain measures based on different areas and lengths.

The current configuration is the spatial arrangement of a material body at the time being studied. A deformation map $\mathbf{x}=\mathbf{\chi }(\mathbf{X},t)$ gives the current position $\mathbf{x}$ of the particle labelled by reference position $\mathbf{X}$. Fields expressed as functions of $\mathbf{x}$ use Eulerian coordinates.

A marked rubber strip illustrates the distinction: its original marks identify material particles, while their observed positions after stretching form the current configuration. A current length or area can differ from the corresponding quantity in the reference configuration. The Cauchy stress tensor measures force per current area, and mass density per current volume changes under compression even though each marked material region retains its mass. Specifying the configuration is therefore part of specifying a measurement, rather than a change in the underlying physical body.

Let $E$ be a finite normal closure of the number field $K$. The permutation representation of its Galois group on the embeddings of $K$ into $E$ has one trivial constituent, because the action is transitive. At a prime, the inertia group invariant basis consists of sums over inertia orbits of embeddings; Frobenius automorphism permutes them in cycles of lengths equal to the residue degrees of the primes of $K$. A cycle of length $f$ contributes $\det (1-T\rho (\mathrm{Frob}))=1-T^f$. Hence the local factors equal those of the Dedekind zeta function, including at ramified primes. If nontrivial irreducible Artin L-functions are holomorphic and nonzero at one, this factorization and the simple pole of the Riemann zeta function show that ${\zeta }_K$ has a simple pole there.

The invariant decay amplitude is the transition matrix element for one incoming particle and a specified on-shell final state, with the overall momentum delta function factored out. For covariantly normalized states, write the connected S-matrix element as $i(2\pi {)}^4{\delta }^4(p_i-p_f)\mathcal{M}(i\to f)$. Its overall phase does not affect the decay width. The rate is $\Gamma =(2M_i{)}^{-1}{\sum }_{\mathrm{spins}}\int d{\Phi }_f|\mathcal{M}{|}^2$, with the initial spin average included when the initial state is unpolarized. For a spin-zero parent and an angle-independent two-body amplitude, the two-body Lorentz-invariant phase space gives $\Gamma =|\mathbf{k}|\sum |\mathcal{M}{|}^2/(8\pi M_i^2)$. In leptonic pion decay, contracting the axial hadronic matrix element with the chiral weak charged current makes this amplitude proportional to the charged-lepton mass, proving helicity suppression.

A branching fraction is the probability that a decay occurs through a particular mutually exclusive channel, equal to its partial decay width divided by the total decay width. Inclusive channel fractions sum to one. Rounding displayed fractions can make their numerical sum differ from one.

A streamfunction for an incompressible zonal-mean flow in the meridional-vertical plane. Its derivatives give meridional and vertical velocity, and differences in its values measure volume transport per zonal span. Constant values on closed impermeable boundaries encode zero net normal flow.

The effective meridional circulation associated with eddy buoyancy transport. In a stratified Southern Ocean, mesoscale eddies tend to flatten the isopycnals tilted by the wind-driven mean circulation, so their contribution can largely oppose the mean Deacon circulation. The residual combines mean and eddy contributions with the diabatic water-mass budget.

In a slit, a confinement blob is three-dimensional but the chain of blobs forms a two-dimensional self-avoiding walk. With $g\sim (D/b{)}^{5/3}$ and in-plane exponent $3/4$, $R_{\parallel }\sim D(N/g{)}^{3/4}$. There is no single preferred axial extension as in a tube. A strictly planar chain confined further to a narrow strip is a different geometry and gives $X\sim L(b/D{)}^{1/3}$ under the two-dimensional blob estimate.

For two incompressible fluids separated by a planar material front $X(t)$, the Darcy flux is uniform and the pressure drop sums the resistances of the two layers: $U=k\Delta P/[\mu X+{\mu }_h(L-X)]$. The front moves at the pore velocity $X^{\prime }=U/\varphi$. Integrating from $X(0)=0$ yields the displayed relation. The formula holds up to breakthrough $X=L$, with either sign of the viscosity difference; equal viscosities give constant speed.

For constant wall heat-flux density $F>0$, effective thermal conductivity $k_e$, buoyancy mobility $B={\rho }_{0}g\alpha K/\mu$ and thermal transport coefficient $\kappa =k_e/({\rho }_0{c}_f)$, a slender Darcy flow boundary layer has width $\delta =(\kappa k_{e}z/(BF){)}^{1/3}$. Writing $\eta =y/\delta$, $\psi =\kappa zf(\eta )/\delta$ and $T-T_a=(F\delta /k_e)f^{\prime }(\eta )$ gives the displayed equation with $f(0)=0$, $f^{\prime \prime }(0)=-1$ and $f^{\prime }(\infty )=0$. The exact integral is ${\int }_0^{\infty }(f^{\prime }{)}^{2}d\eta =1$. Consequently its kinematic Darcy momentum flux is $\int w^{2}dy=B\kappa Fz/k_e$ and its buoyancy flux is $g\alpha \kappa Fz/k_e$. These are per span on one heated face.

Darcy flow is slow flow through a porous medium whose averaged flux obeys the Darcy law. The Darcy velocity is the fluid volume flux per total cross-sectional area; it differs from the velocity averaged only over pore space.

Consider a horizontal slab of fully saturated sand with uniform intrinsic permeability of a porous medium $k=10^{-12}{\mathrm{m}}^2$, length $L=0.50\mathrm{m}$, total cross-sectional area $A=0.020{\mathrm{m}}^2$, and porosity $\varphi =0.25$. Use one Newtonian fluid with mass density $\rho =1000\mathrm{kg}{\mathrm{m}}^{-3}$ and dynamic viscosity $\mu =10^{-3}\mathrm{Pa}\mathrm{s}$. Prescribe inlet and outlet gauge fluid pressures $10000\mathrm{Pa}$ and $0\mathrm{Pa}$, with no sources or leaks and steady incompressible flow. The two ends have the same elevation, so gravity has no component along the slab. Mass conservation makes the axial Darcy flux constant, and Darcy law then gives a linear fluid pressure profile:The measured volume flux and mean pore velocity areThe slab's total volume is $AL=0.010{\mathrm{m}}^3$, of which $\varphi AL=0.0025{\mathrm{m}}^3=2.5\mathrm{L}$ is pore volume. In the ideal uniform advective model, a nonreacting tracer has transit time $L/v=6250\mathrm{s}\simeq 1.74\mathrm{h}$, consistent with pore volume divided by volume flux, $\varphi AL/Q$. The incorrect substitution of Darcy velocity for pore velocity would give $25000\mathrm{s}$, four times too long. Real passages have different path lengths and local speeds; these numbers describe a bulk mean rather than every particle's journey.

As an independent check, gravitational acceleration magnitude $g=9.81\mathrm{m}{\mathrm{s}}^{-2}$ gives hydraulic conductivity $K=9.81\times 10^{-6}\mathrm{m}{\mathrm{s}}^{-1}$, hydraulic head drop $\Delta h=10000/(1000\times 9.81)\mathrm{m}\simeq 1.01937\mathrm{m}$, and $q=K\Delta h/L=2.0\times 10^{-5}\mathrm{m}{\mathrm{s}}^{-1}$ again. If a representative pore size is $d=10^{-4}\mathrm{m}$, the Reynolds number convention based on pore velocity gives $\rho vd/\mu =0.008$, supporting neglect of pore inertia. This size is an illustrative extra measurement, not something determined by porosity and intrinsic permeability of a porous medium alone.

Regenerate the diagram by running python ../darcy-flux-and-pore-velocity.py from _media; it writes its PNG into the current directory.

Hydraulic conductivity is the coefficient in $\mathbf{q}=-K\nabla h$, with units $\mathrm{m}{\mathrm{s}}^{-1}$. Because the gradient of hydraulic head is dimensionless, hydraulic conductivity has the dimensions of velocity, but it is not the actual Darcy velocity unless the driving gradient has magnitude one. Intrinsic permeability of a porous medium $k$ has units ${\mathrm{m}}^2$ and describes pore geometry; hydraulic conductivity also depends on mass density, dynamic viscosity and gravitational acceleration.^[ref]

For $k=10^{-12}{\mathrm{m}}^2$, $\rho =1000\mathrm{kg}{\mathrm{m}}^{-3}$, $g=9.81\mathrm{m}{\mathrm{s}}^{-2}$ and $\mu =10^{-3}\mathrm{Pa}\mathrm{s}$, hydraulic conductivity is $K=9.81\times 10^{-6}\mathrm{m}{\mathrm{s}}^{-1}$. Doubling dynamic viscosity while keeping pore geometry, mass density and gravitational acceleration fixed halves hydraulic conductivity without changing intrinsic permeability of a porous medium. Thus a value quoted as a material's hydraulic conductivity needs its fluid conditions.

Hydraulic head is the sum of elevation and pressure head, measured in metres relative to a chosen height datum. For constant mass density $\rho$ and gravitational acceleration magnitude $g$, the pressure head $p/(\rho g)$ is the height of a column of the same fluid supported by fluid pressure $p$. A water-filled open measuring tube records hydraulic head as the elevation of its water level when $p$ is gauge fluid pressure. Changing the common pressure reference or height datum adds a constant to hydraulic head and leaves its driving gradient unchanged.

For water with $\rho =1000\mathrm{kg}{\mathrm{m}}^{-3}$ and $g=9.81\mathrm{m}{\mathrm{s}}^{-2}$, a point at $z=2\mathrm{m}$ with gauge fluid pressure $p=9810\mathrm{Pa}$ has $h=3\mathrm{m}$. A second point at $z=0$ with gauge fluid pressure $29430\mathrm{Pa}$ also has $h=3\mathrm{m}$: these values are compatible with a stationary column under hydrostatic pressure. It is a difference in hydraulic head, rather than a difference in fluid pressure alone, that drives saturated Darcy flow. This form uses constant mass density; one cannot generally pull spatially varying $\rho$ through the gradient.^[ref]

For $a\ge 1$ and $p\nmid m$, the identity ${\Phi }_{p^{a}m}(X)={\Phi }_m(X^{p^a})/{\Phi }_m(X^{p^{a-1}})$ gives the displayed reduction, since taking a $p$th power equals substitution $X\mapsto X^p$ in characteristic $p$. The reduction of ${\Phi }_m$ is squarefree because it divides the separable polynomial $X^m-1$. The Kummer-Dedekind theorem therefore gives ramification index of a prime ideal $\phi (p^a)$ in the cyclotomic field. In particular, a conductor factor $2$ occurring only to the first power has index one and creates no ramification by itself.

Fix finitely many prescribed cyclotomic classes for pairwise differences. Such patterns are realized in every sufficiently large compatible finite field. For $r$ already chosen coordinates, let $M(a)$ count extensions with prescribed classes for $x-a_i$. Averaging over all $a\in {\mathbb{F}}_q^r$ gives $\mathbb{E}M=q/m^r+O(1)$ and, from the uniform two-class intersection estimate, $\mathrm{Var}M=O_{m,r}(q^{3/2})$. The Chebyshev inequality makes the fraction with $M<q/(2m^r)$ tend to zero. Inductively each fixed pattern on $r$ coordinates occupies a positive proportion of all tuples, so some positive proportion have many extensions. This proves the pattern-existence claim without an unproved greedy-extension assumption.