Specific detectivity

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Specific detectivity, or D*, for a photodetector is a figure of merit used to characterize performance, equal to the reciprocal of noise-equivalent power (NEP), normalized per square root of the sensor's area and frequency bandwidth (reciprical of its sampling rate).

Specific detectivity is given by D^{*}={\frac  {{\sqrt  {Af}}}{NEP}}, where A is the area of the photosensitive region of the detector and f is the frequency bandwidth. It is commonly expressed in Jones units (cm\cdot {\sqrt  {Hz}}/W)in honor of R. Clark Jones who originally defined it.[1][2]

Given that noise-equivalent power can be expressed as a function of the responsivity {\mathfrak  {R}} (in units of A/W or V/W) and the noise spectral density S_{n} (in units of A/Hz^{{1/2}} or V/Hz^{{1/2}}) as NEP={\frac  {S_{n}}{{\mathfrak  {R}}}}, it's common to see the specific detectivity expressed as D^{*}={\frac  {{\mathfrak  {R}}\cdot {\sqrt  {A}}}{S_{n}}}.

It is often useful to express the specific detectivity in terms of relative noise levels present in the device. A common expression is given below.

D^{*}={\frac  {q\lambda \eta }{hc}}\left[{\frac  {4kT}{R_{0}A}}+2q^{2}\eta \Phi _{b}\right]^{{-1/2}}

With q as the electronic charge, \lambda is the wavelength of interest, h is Planck's constant, c is the speed of light, k is Boltzmann's constant, T is the temperature of the detector, R_{0}A is the zero-bias dynamic resistance area product (often measured experimentally, but also expressible in noise level assumptions), \eta is the quantum efficiency of the device, and \Phi _{b} is the total flux of the source (often a blackbody) in photons/sec/cm².

References

  1. R. C. Jones, "Quantum efficiency of photoconductors," Proc. IRIS 2, 9 (1957)
  2. R. C. Jones, "Proposal of the detectivity D** for detectors limited by radiation noise," J. Opt. Soc. Am. 50, 1058 (1960), doi:10.1364/JOSA.50.001058)

 This article incorporates public domain material from the General Services Administration document "Federal Standard 1037C".

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