Photoconductor response time

ID: photoconductor-response-time

Photoconductor response time describes how quickly the electrical signal follows a change in illumination under stated bias, temperature, background and readout conditions. A rise time, fall time and modulation bandwidth summarize different features and require definitions. The manufacturer’s PbS description notes that sensitivity, response speed and dark resistance vary with temperature, so a timing number is not independent of operating conditions.[ref]
An original one-lifetime model takes excess carrier density to obey
With constant mobility and fixed detector bias, suppose the excess current is proportional to . After a step from zero to generation , the normalized signal is . The times to reach ten and ninety percent of its final value are and , giving
The time from zero to ninety percent is instead . A quoted rise time without its thresholds is therefore incomplete.
For small sinusoidal generation changes, the normalized frequency response is
The half-power frequency is , so this single-pole model gives . This relationship is a consequence of the stated model, not a universal identity for arbitrary detectors.
For , the rise time is about and the cutoff about . At , the signal amplitude is about of its low-frequency value and its phase lags by . The signal can therefore have a substantial phase delay before reaching the half-power point.
A readout adds its own dynamics. If the detector response is cascaded with a separate first-order electronic response of the same time constant, the overall magnitude is . Its half-power frequency is , about times the single-pole cutoff. Assigning that combined bandwidth entirely to the material would give an incorrect carrier-lifetime estimate.
Photoconductor rise and fall asymmetry tests another limitation of the simple model: linear one-lifetime dynamics predict equal normalized rise and fall behavior, but trap occupancy, changing background or a nonlinear circuit can produce different transients. A long relaxation tail should be measured rather than compressed into an unsupported single time constant.
A proposed experiment switches or modulates a monitored optical source, records detector current and actual bias, and measures ten-to-ninety and ninety-to-ten crossings after settling the initial illumination state. Repeat the modulation sweep with a characterized faster readout or independently measured amplifier response. Vary temperature and optical background while holding the wavelength and spot fixed. Agreement between step and frequency-response fits tests the one-pole approximation; disagreement identifies missing dynamics without by itself proving which physical mechanism caused them.

New to topics? Read the docs here!