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Schottky effect and modified Richardson equation

Short answer

The Schottky effect is the lowering of the metal's work function by an applied electric field. For an electron at distance x, the image potential is -e^2/(16 pi epsilon0 x) and field E adds -eEx. The barrier maximum gives an effective work function Phi_eff = Phi - sqrt(e^3 E/(4 pi epsilon0)). The modified Richardson equation is J = B0 T^2 exp[-(Phi - beta_s sqrt(E))/kT].

What is Schottky effect? Derive the modified Richardson's equation that shows the reduction in barrier potential due to the application of external field.

Schottky effect is the lowering of the work function (potential barrier) of a metal surface when a strong accelerating electric field is applied to it. Because the barrier is lowered, the thermionic emission current increases with field even at constant temperature.

Barrier without field (image force)

An electron at distance xx outside a metal surface induces an image charge +e+e at distance xx inside. The attractive image force and its potential energy are

F=−e24πε0(2x)2=−e216πε0x2,PEim=−e216πε0xF = -\frac{e^2}{4\pi\varepsilon_0(2x)^2} = -\frac{e^2}{16\pi\varepsilon_0 x^2}, \qquad PE_{im} = -\frac{e^2}{16\pi\varepsilon_0 x}

Taking energies from the Fermi level, the electron's PE outside is

PE(x)=Φ−e216πε0xPE(x) = \Phi - \frac{e^2}{16\pi\varepsilon_0 x}

which approaches Φ\Phi at large xx. So the full barrier to be crossed is Φ\Phi.

Barrier with applied field

An applied field E\mathcal{E} that pulls electrons out adds PE =−eEx= -e\mathcal{E}x:

PE(x)=Φ−e216πε0x−eExPE(x) = \Phi - \frac{e^2}{16\pi\varepsilon_0 x} - e\mathcal{E}x
 PE
  ^   no field: -> Phi
  | Phi .......___________
  |  dPhi{  .-''-.
  |       /        '-._  with E
  |      /             '-._
  | EF  /___________________> x
     surface   xm

Finding the lowered barrier

The peak is where d(PE)/dx=0d(PE)/dx = 0:

e216πε0xm2=eE⇒xm=(e16πε0E)1/2\frac{e^2}{16\pi\varepsilon_0 x_m^2} = e\mathcal{E} \quad\Rightarrow\quad x_m = \left(\frac{e}{16\pi\varepsilon_0\mathcal{E}}\right)^{1/2}

Putting xmx_m back:

PEmax=Φ−e216πε0xm−eExm=Φ−(e3E16πε0)1/2−(e3E16πε0)1/2=Φ−(e3E4πε0)1/2\begin{aligned} PE_{max} &= \Phi - \frac{e^2}{16\pi\varepsilon_0 x_m} - e\mathcal{E}x_m \\ &= \Phi - \left(\frac{e^3\mathcal{E}}{16\pi\varepsilon_0}\right)^{1/2} - \left(\frac{e^3\mathcal{E}}{16\pi\varepsilon_0}\right)^{1/2} \\ &= \Phi - \left(\frac{e^3\mathcal{E}}{4\pi\varepsilon_0}\right)^{1/2} \end{aligned}

So the barrier is reduced by

ΔΦ=βSE,βS=(e34πε0)1/2=6.08×10−24 J (V/m)−1/2\Delta\Phi = \beta_S\sqrt{\mathcal{E}}, \qquad \beta_S = \left(\frac{e^3}{4\pi\varepsilon_0}\right)^{1/2} = 6.08 \times 10^{-24}\ \text{J}\,(\text{V/m})^{-1/2}

and the effective work function is Φeff=Φ−βSE\Phi_{eff} = \Phi - \beta_S\sqrt{\mathcal{E}}.

Modified Richardson equation

The Richardson-Dushman equation J=B0T2exp⁡(−Φ/kT)J = B_0T^2\exp(-\Phi/kT) now uses Φeff\Phi_{eff}:

J=B0T2exp⁡[−Φ−βSEkT]=J0exp⁡(βSEkT)J = B_0 T^2 \exp\left[-\frac{\Phi - \beta_S\sqrt{\mathcal{E}}}{kT}\right] = J_0 \exp\left(\frac{\beta_S\sqrt{\mathcal{E}}}{kT}\right)

where J0=B0T2e−Φ/kTJ_0 = B_0T^2e^{-\Phi/kT} is the zero-field emission and B0=4πmek2/h3≈1.2×106 A m−2K−2B_0 = 4\pi mek^2/h^3 \approx 1.2 \times 10^{6}\ \text{A m}^{-2}\text{K}^{-2}.

Remarks: ln⁡J\ln J is linear in E\sqrt{\mathcal{E}} (Schottky plot). For E=108 V/m\mathcal{E} = 10^8\ \text{V/m}, ΔΦ≈0.38 eV\Delta\Phi \approx 0.38\ \text{eV} and xm≈1.9 nmx_m \approx 1.9\ \text{nm}. At much higher fields (>109>10^9 V/m) the barrier becomes thin enough for tunnelling, i.e. field emission.

✓ Answer checked by Claude Opus 5.5 (high effort)

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