The responsivity ( 1) of a photon counting detector
can be determined using pairs of correlated photons by positioning
two detectors to intercept each of photons in the pair. The counting rate
of each detector (N1 and N2) is recorded along with the coincidence rate
(NC) between the
two detectors. The ratio of the coincidence rate to the single rate of
one detector is the absolute quantum efficiency of the other detector
and vice versa. The rate of photon production (N) cancels in this procedure.
Put another way, the output pulses of one of the detectors
can be thought of as a trigger which indicates the existence of a second
photon headed for the other detector. The quantum efficiency of the
detector is then just the fraction of photons detected at the second
detector in conjunction with a trigger from the first.
Figure 1: Schematic of the absolute responsivity scheme
To test this method, a parametric down-conversion source has been set
up to allow the absolute spatial responsivity of a photomultiplier to be
measured at a range of wavelengths in the visible. The method was
verified using independent calibration methods available within the
division. The goal is to determine the ultimate accuracy that may be
achieved with this method. The first results showed agreement at the
0.5% level, which was the estimated 1-sigma uncertainty of that
comparison. Improvements are underway to test this comparison at the
0.1% level.
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