In a photoconductive
detector an
electric potential is applied across the absorbing region and causes a current to flow in proportion
to the irradiance if the photon energy exceeds the energy gap between the
valence and the
conduction band. Depending on their
spectral responsivity function, photoconductive detectors are divided into photoconductive detectors for the
visiblewavelength range e.g. cadmium sulfide or
CdS photoconductive detectors, photoconductive detectors for the near
infraredwavelength range e.g. lead sulfide or
PbS photoconductive detectors, photoconductive detectors for the
infraredwavelength range e.g. silicon doped with arsenide or
Si:
As photoconductive detectors, and the mercury-cadmium-telluride or
HgCdTe photoconductive detector.
Source:
PAC, 1995, 67, 1745
(Nomenclature, symbols, units and their usage in spectrochemical analysis-XI. Detection
of radiation (IUPAC Recommendations 1995))
on page 1754
Cite as:
IUPAC. Compendium of Chemical Terminology, 2nd ed. (the "Gold Book"). Compiled by
A. D. McNaught and A. Wilkinson. Blackwell Scientific Publications, Oxford (1997).
XML on-line corrected version: http://goldbook.iupac.org (2006-) created by M. Nic,
J. Jirat, B. Kosata; updates compiled by A. Jenkins. ISBN 0-9678550-9-8.
https://doi.org/10.1351/goldbook.