Charge carrier density

The carrier density is usually obtained theoretically by integrating the density of states over the energy range of charge carriers in the material (e.g. integrating over the conduction band for electrons, integrating over the valence band for holes).

If the total number of charge carriers is known, the carrier density can be found by simply dividing by the volume. To show this mathematically, charge carrier density is a particle density, so integrating it over a volume ${\displaystyle V}$ gives the number of charge carriers ${\displaystyle N}$ in that volume

${\displaystyle N=\int _{V}n(\mathbf {r} )\,\mathrm {d} V}$.

where

${\displaystyle n(\mathbf {r} )}$ is the position-dependent charge carrier density.

If the density does not depend on position and is instead equal to a constant ${\displaystyle n_{0}}$ this equation simplifies to

${\displaystyle N=V\cdot n_{0}}$.

The carrier density is important for semiconductors, where it is an important quantity for the process of chemical doping. Using band theory, the electron density,${\displaystyle n_{0}}$ is number of electrons per unit volume in the conduction band. For holes, ${\displaystyle p_{0}}$ is the number of holes per unit volume in the valence band. To calculate this number for electrons, we start with the idea that the total density of conduction-band electrons, ${\displaystyle n_{0}}$, is just adding up the conduction electron density across the different energies in the band, from the bottom of the band ${\displaystyle E_{c}}$ to the top of the band ${\displaystyle E_{top}}$.

${\displaystyle n_{0}=\int \limits _{E_{c}}^{E_{top}}N(E)dE}$

Because electrons are fermions, the density of conduction electrons at any particular energy,${\displaystyle N(E)}$ is the product of the density of states,${\displaystyle g(E)}$ or how many conducting states are possible, with the Fermi–Dirac distribution,${\displaystyle f(E)}$ which tells us the portion of those states which will actually have electrons in ″them″

${\displaystyle N(E)=g(E)f(E)}$

In order to simplify the calculation, instead of treating the electrons as fermions, according to the Fermi–Dirac distribution, we instead treat them as a classical non-interacting gas, which is given by the Maxwell–Boltzmann distribution. This approximation has negligible effects when the magnitude ${\displaystyle |E-E_{f}|\gg k_{B}T}$, which is true for semiconductors near room temperature. This approximation is invalid at very low temperatures or an extremely small band-gap.

${\displaystyle f(E)={\frac {1}{1+e^{\frac {E-E_{f}}{kT}}}}\approx e^{\frac {-(E-E_{f})}{k_{B}T}}}$

The three-dimensional density of states is:

${\displaystyle g(E)={\frac {1}{2\pi ^{2}}}\left({\frac {2m^{*}}{\hbar ^{2}}}\right)^{\frac {3}{2}}{\sqrt {E-E_{0}}}}$

After combination and simplification, these expressions lead to:

${\displaystyle n_{0}=2\left({\frac {m^{*}k_{B}T}{2\pi \hbar ^{2}}}\right)^{3/2}}$${\displaystyle e^{\frac {-(E_{c}-E_{f})}{k_{B}T}}}$

A similar expression can be derived for holes. The carrier concentration can be calculated by treating electrons moving back and forth across the bandgap just like the equilibrium of a reversible reaction from chemistry, leading to an electronic mass action law. The mass action law defines a quantity ${\displaystyle n_{i}}$ called the intrinsic carrier concentration, which for undoped materials:

${\displaystyle n_{i}=n_{0}=p_{0}}$

The following table lists a few values of the intrinsic carrier concentration for intrinsic semiconductors.

These carrier concentrations will change if these materials are doped. For example, doping pure silicon with a small amount of phosphorus will increase the carrier density of electrons, n. Then, since n > p, the doped silicon will be a n-type extrinsic semiconductor. Doping pure silicon with a small amount of boron will increase the carrier density of holes, so then p > n, and it will be a p-type extrinsic semiconductor.

The carrier density is also applicable to metals, where it can be calculated from the simple Drude model. In this case, the carrier density (in this context, also called the free electron density) can be calculated by:[4]

${\displaystyle n={\frac {N_{A}Z\rho _{m}}{m_{a}}}}$

Where ${\displaystyle N_{A}}$ is the Avogadro constant, Z is the number of valence electrons, ${\displaystyle \rho _{m}}$ is the density of the material, and ${\displaystyle m_{a}}$ is the atomic mass.

The density of charge carriers can be determined in many cases using the Hall effect,[5] the voltage of which depends inversely on the carrier density.