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For a p-n junction, biasing with the p-type semiconductor at negative electric potential difference relative to the n-type semiconductor.

For a p-n junction, biasing with the p-type semiconductor at positive electric potential difference relative to the n-type semiconductor.

The valley of stability is the region of nuclear masses near the minima with respect to proton-neutron imbalance. Its beta-stable band bends toward neutron excess for heavier nuclei, as nuclear Coulomb energy competes with the cost of neutron-proton asymmetry. The band is distinct from the particle-emission boundaries set by nuclear separation energies.

The spin-independent vector contribution to an allowed beta decay. The isospin operator ${\tau }_k^{\pm }$ changes a neutron into a proton or the reverse; the sign convention depends on the assigned nucleon isospin projection. Its rotational rank is zero, so $J_f=J_i$ and the parity is unchanged. The phrase Fermi-type forbidden contribution extends the $S=0$ classification to higher orbital angular momentum.

The spin-dependent axial-vector contribution to an allowed beta decay. Its rotational rank is one, permitting $\Delta J=0,1$ with unchanged parity, but excluding $0\to 0$. Here ${\mathbf{\sigma }}_k$ acts on nucleon spin and ${\tau }_k^{\pm }$ on isospin. Higher-orbital spin-dependent contributions are conventionally described as Gamow-Teller-type forbidden transitions.

A beta decay transition whose leading lepton orbital term has $l=0$. Fermi transitions allow $\Delta J=0$ and Gamow-Teller transitions allow $\Delta J=0,1$, excluding a Gamow-Teller $0\to 0$ transition. Both preserve nuclear parity. Allowed describes the selection rules; cancellations in the nuclear matrix element can still make an allowed transition slow.

A beta decay transition for which the leading $l=0$ lepton orbital term vanishes by the angular momentum or parity selection rules. The least contributing orbital order $l=n\ge 1$ gives the name $n$th forbidden. First-forbidden transitions change parity and can carry total lepton angular momentum $0,1,2$; second-forbidden transitions preserve parity and can carry $1,2,3$, with Fermi-type $S=0$ contributions restricted to $J=l$. Forbidden is suppression by higher powers of lepton momentum times nuclear size, rather than an absolute prohibition.

The product of a dimensionless beta-decay statistical phase-space factor $f$ and the partial half-life $t$ for the transition. The tabulated $\log ft$ normally means ${\log }_{10}[ft/(1\mathrm{s})]$. Factoring out this approximate phase space dependence allows comparisons of nuclear weak matrix elements. Strong superallowed Fermi transitions have small $\log ft$; forbidden beta decays generally have larger values, with nuclear-structure exceptions and overlaps between categories.

With the Fourier transform convention $\hat{f}(\omega )={\int }_{\mathbb{R}}f(t)e^{-i\omega t}dt$, the regular order-zero Bessel function of the first kind has the tempered distribution transformThe density is integrable despite its endpoint singularities. Fourier inversion gives the equivalent integral representationThe second formula follows by $\omega =\cos \theta$ and cancellation of the odd imaginary part. It is the standard real integral representation of $J_0$.^[ref]

Indeed, transforming the order-zero Bessel differential equation $t{y}^{\prime \prime }+y^{\prime }+ty=0$ gives $(1-{\omega }^2)Y^{\prime }-\omega Y=0$. Inside $(-1,1)$, its solutions are $C(1-{\omega }^2{)}^{-1/2}$. The compactly supported choice also solves the equation as a distribution: rewrite it as $[(1-{\omega }^2)Y{]}^{\prime }+\omega Y=0$, and observe that $(1-{\omega }^2)Y=C\sqrt{1-{\omega }^2}{1}_{(-1,1)}$ is continuous and zero at the two endpoints. Its distributional derivative has no endpoint Dirac delta terms. The inverse is regular at $t=0$, and $y(0)=1$ fixes $C=2$.

The transformed equation alone also allows separate constants on $\omega <-1$ and $\omega >1$. Selecting the compactly supported density amounts to selecting the solution regular at the origin, rather than every possible singular solution of the Bessel differential equation.

For fixed $\beta$, move the order term of the Bessel equation to the right: $x^2{y}^{\prime \prime }+x{y}^{\prime }+{\beta }^2{x}^{2}y=n^{2}y$. The integrating factor for its leading differential expression is $1/x$, giving the displayed Sturm-Liouville theory form with coefficient $p=x$, potential $q={\beta }^{2}x$, weight $w=1/x$ and eigenvalue $n^2$. The origin is a singular endpoint. The integrating factor must be normalized from a positive reference point; its defining logarithmic integral cannot literally start at zero. Boundary conditions are needed before this differential identity becomes a specified self-adjoint spectral problem.

A Bell test compares experimental probabilities or expectation values with a Bell inequality. In a two-setting photon polarization test, each station chooses a polarizer orientation and records an outcome. A coincidence circuit identifies candidate pairs using an agreed timing rule. The choice of which trials enter the statistic is part of the experiment: correlations calculated only from detected pairs can differ from correlations of all emitted pairs. The Polarization CHSH count model separates ideal expectation values from this experimental selection problem.

A reference blank is the comparison sample used to establish the background response in a measurement. For absorbance, it contains matching solvent and other assay ingredients without the target absorbing chemical species; it sets the reference radiant power $P_0$ under matching cuvette and wavelength conditions.

The superconducting isotope effect is the dependence of the superconducting transition temperature on isotopic mass $M$ at fixed chemical composition. Its discovery in 1950 was a crucial clue that phonons participate in conventional superconductivity.^[ref]

The model prediction can be derived from two assumptions. For harmonic motion with a fixed restoring-force constant $K$, a phonon frequency scales as $\omega \propto \sqrt{K/M}$. If the BCS dimensionless coupling is independent of $M$, the weak coupling result $k_B{T}_c\simeq 1.134\hslash {\omega }_D{e}^{-1/\lambda }$ then gives $T_c\propto M^{-1/2}$ and $\alpha =1/2$. Changes in the effective interaction can change this exponent; it is not a universal law for every material exhibiting superconductivity. For a stipulated mass ratio $M_2/M_1=1.04$, the ideal model predicts $T_{c,2}/T_{c,1}=1/\sqrt{1.04}\simeq 0.98058$. This is an original scaling example, not a pair of measured transition temperatures.

The clean isotropic weak-coupling BCS coherence length is conventionally ${\xi }_0=\hslash v_F/(\pi \Delta (0))$, with Fermi velocity $v_F$. It characterizes the spatial extent of pairing correlations.^[ref]

The scale follows from the same spectral calculation. Linearizing the normal energy near the Fermi surface gives ${\xi }_k\simeq \hslash v_F(k-k_F)$. The region $|{\xi }_k|\lesssim \Delta$ therefore has radial width $\delta k\sim \Delta /(\hslash v_F)$. Fourier analysis associates this width with a distance $\ell \sim 1/\delta k\sim \hslash v_F/\Delta$. This argument establishes the scale, not the conventional factor $1/\pi$. A small superconducting energy gap consequently permits pairing correlations over many interparticle spacings.

The BCS quasiparticle spectrum is the positive excitation energy obtained by diagonalizing the paired particle-hole block. Here the weak coupling shell model has $\Delta \ll {\Omega }_D$: the minimum lies inside the pairing shell, and states outside it cost more. To derive it for a uniform isotropic real $\Delta >0$, measure the normal-state energy from the chemical potential, ${\xi }_k={ϵ}_k-\mu$, and use the same sign convention as the BCS coherence factors:Its eigenvalues are ${\epsilon }_{\pm }=\pm E_k$, where $E_k=\sqrt{{\xi }_k^2+{\Delta }^2}$. The positive $E_k$ is the cost of creating a quasiparticle above the BCS ground state. The lower branch $-E_k$ is its particle-hole partner in this doubled matrix description, not an excitation that lowers the ground state energy without bound.

The location and value of the minimum follow directly:The unique minimum as a function of $\xi$ is $E(0)=\Delta$, at the normal-state Fermi surface. On an isotropic three-dimensional Fermi surface it occurs for every direction of $k$, rather than at a unique point of momentum space. Near that minimum,Farther away, $E(\xi )\simeq |\xi |$ when $\Delta \ll |\xi |\ll {\Omega }_D$. For the illustrative $\lambda =0.25$ example, a state at $\xi =\Delta$ costs $\sqrt{2}\Delta \simeq 1.03644\mathrm{meV}$ rather than the minimum $0.732871\mathrm{meV}$.

For smooth inviscid barotropic fluid with potential body forces, barotropic vorticity transport and $\nabla \cdot \mathbf{\omega }=0$ give $D\mathbf{\omega }/Dt=(\mathbf{\omega }\cdot \nabla )\mathbf{u}-\mathbf{\omega }\nabla \cdot \mathbf{u}$. Combine this with material surface element evolution to obtain $D(\mathbf{\omega }\cdot d\mathbf{S})/Dt=0$. Integrating over a material surface proves the flux law. Its boundary must move with the fluid; flux through a fixed open surface is generally not conserved. By Stokes theorem the same statement is Kelvin's circulation theorem around the material boundary.

For a smooth axisymmetric flow, write $u_z(r,z)=w(z)+O(r^2)$ near the axis. The incompressible flow condition is $r^{-1}{\partial }_r(r{u}_r)+{\partial }_z{u}_z=0$. Integrating radially and excluding a singular line source at the axis gives $u_r=-r{w}^{\prime }(z)/2+O(r^3)$. The signed axial velocity is essential: specifying only its magnitude does not fix the sign of the radial velocity.

In macroautophagy, a portion of cytoplasm, potentially including an organelle, is enclosed in an autophagosome before delivery to a lysosome. Sequestration precedes digestion.^[ref]