The Richardson-Dushman law models the magnitude of emitted electric current density asHere is absolute thermodynamic temperature, is the work function, is the Boltzmann constant, and is the Thermionic Richardson constant. The signed electric current density points opposite to the outgoing Electron motion; here is positive. For uniform emission over area , the emitted electric current magnitude is .
The Richardson-Dushman law assumes an emitter close to thermal equilibrium, a surface with a well-defined and approximately constant work function over the fitted temperature range, and predominantly thermal escape over the barrier. Interpreting a measured collector electric current with this law additionally requires an emission-limited thermionic current, known emitting area, and negligible return emission from the collector. Strong electric fields can lower the surface barrier or enable quantum tunnelling; then this zero-field expression is insufficient.
For a deliberately chosen teaching model, take and , expressing the barrier in electronvolts. These are illustrative parameters, not measured properties of a named material. Using , at the Boltzmann factor is about , yetA 20 percent increase in temperature raises the predicted electric current density by about 69 times. For a chosen emitting area , these correspond to approximately and if collection is complete. The small escaping fraction is replenished by the external electrical circuit.
The sensitivity is especially clear from the logarithmic derivative at fixed :In the chosen model at , a rise changes by about 2.5 percent to first order. Accurate temperature measurement matters even when electric current measurement is easy.
The coefficient has dimensions of electric current density divided by squared temperature. For ideal nonrelativistic particles with the free electron mass, two spin states, a planar uniform surface, and unit escape transmission, the thermionic tail-flux derivation giveswhere is the positive elementary charge and is the Planck constant. The two area units differ by a factor of . A fitted need not equal : reflection at the surface, the electronic band structure, and uncertain emitting area affect the inferred coefficient. A constant escape transmission would give in this simple model; an energy-dependent transmission generally requires an integral instead.
The name joins Owen Willans Richardson with Saul Dushman. Dushman's 1923 paper develops a thermodynamic treatment of Electron emission analogous to evaporation and evaluates the prefactor using quantum ideas.[ref]
Electron Emission from Metals as a Function of Temperature by Saul Dushman. Abstract, general equation and theoretical evaluation of A
Choose a fixed positive reference with the same units as . Taking the natural logarithm of a dimensionless ratio givesThus the Richardson plot is a straight line when and are constant, with slope and intercept . The familiar notation silently chooses units; the reference makes that choice explicit. Changing shifts the intercept and leaves the inferred work function unchanged. If the horizontal axis instead uses , its slope is .
For the chosen example, choose . Then and . Their slope is approximately , giving . Two temperatures determine a line algebraically; several temperatures allow curvature and drift to be detected. These values are calculated, rather than experimental observations.
A straight trace alone does not establish a unique surface work function. Adsorption, changing surface coverage, or a mixture of regions with different barriers can change the inferred slope. For independent emitting patches with area fractions , constant and barriers ,Lower barriers contribute disproportionately. Even with fixed patches, the slope of the Richardson plot gives a temperature-dependent weighted mean of the , rather than their simple area average. If or themselves vary with temperature, the apparent slope-derived barrier becomesCheck collection, temperature calibration, and surface stability before assigning curvature to a new emission mechanism.
Consider a planar surface with outward normal along . For an auxiliary equilibrium electron gas just outside it, let be the total number density, counting both signs of . Its Maxwell-Boltzmann velocity distribution has normal-component densityAn Electron with crosses more area per unit time when it moves faster. The outgoing number flux therefore uses , rather than just the probability of :This integral contributes only . Holding a classical bulk number density fixed and imposing a normal kinetic energy threshold would instead give ; that argument alone does not produce .
For the ideal surface model, measure external Electron energies from the metal's chemical potential . A freely propagating external state has . When , its Fermi-Dirac distribution reduces to the Maxwell–Boltzmann statistics tail. Counting two spin states per phase space cell of volume givesEach of the three Gaussian integrals supplies . Combining this state count with the crossing factor givesThe auxiliary atmosphere supplies an equilibrium state-counting argument; an operating collector removes the outgoing Electrons. It need not maintain a real equilibrium gas throughout the gap. Unit transmission and the ideal free Electron state count are substantive assumptions, so this calculation does not determine an arbitrary real surface's measured .
In particular, Electrons inside a metal generally form a degenerate Fermi gas. A classical distribution for the escaping tail does not imply a classical distribution for the whole interior. Richardson himself emphasized this distinction in his lecture.[ref]
Thermionic Phenomena and the Laws which Govern Them by Owen Willans Richardson. Nobel Lectures, Physics 1922–1941; pp. 230–231, internal versus external electron statistics
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