Impact Ionisation Group

## Indium Phosphide Ionisation Coefficients

The figure shows the impact ionization coefficients for the III-V binary semiconductor material, Indium Phosphide (InP), as a function of inverse electric field at room temperature. These ionization coefficients were obtained from photomultiplication measurements undertaken on a range of PIN and NIP diodes of different avalanching widths.

The electron (hole) ionization coefficients, α (β) plotted in the diagram above can be expressed as

$$\alpha(\beta)=A\exp{\bigg[-\left({\frac{B}{F}}\right)^c\bigg]}$$

where F is electric field strength. The constants A, B and c are tabulated as below.

F (kV/cm)Coefficient TypeA (x105 cm-1)B(x105 cm-1)c
240-380α11231.11
β47.925.51
380-560α29.326.41
β16.221.11
560-1250α2.328.462
β2.487.892

α(β) can be can be used in simple analytical expressions to determine the avalanche multiplication (or gain) and the breakdown voltage. In thin avalanching structures, α(β) overestimate the multiplication as they ignore "dead-space" effects. They also cannot accurately predict the excess noise due to the impact ionization process. Models to predict the multiplication and excess noise in thin avalanching structure require knowledge of enabled ionization coefficients, α*(β*).

α*(β*) can be approximated from α(β) using

$$\frac{1}{\alpha^*}=\frac{1}{\alpha}-\frac{2E_{the}}{F}$$ $$\frac{1}{\beta^*}=\frac{1}{\beta}-\frac{2E_{thh}}{F}$$
where Ethe (Ethh) corresponds to the InP electron (hole) threshold energy and is given as 2.8 (3.0) eV1. A full description on model which uses α*(β*) (recursive model) is given by Saleh et. al. 2 and the numerical equivalent model (RPL model) is by Ong et. al.3

The above data is from Tan et. al.4 Other authors who have published InP ionisation coefficients are Cook5, Umebu6 and Armiento et. al.7. Details of ionisation coefficients over a wide electric field range can be found in Cheong et. al. for Indium Phosphide and other popular semiconductor materials8