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Optimum Timing Solutions for Scintillation Detectors In
scintillation/photomultiplier timing systems, jitter is influenced
by the generation rate of photons in the scintillator, variations in
the photon transit times through the scintillator, the transit time
variations of photo electrons from the photocathode to the first
dynode, statistical fluctuations in the gains of the individual
dynodes, and, to a much smaller degree, the width of the
single-electron response of the PMT. Normally, the signal amplitude
at the anode output is large enough to make the input noise of the
succeeding electronics a negligible contributor. Best time
resolutions are obtained from scintillators with small mechanical
size, efficient light collection, high light output, and short
fluorescence decay times. The photomultiplier should be chosen for
high photocathode yield, small photocathode diameter, high
first-dynode yield, minimal transit-time spread, and a reasonably
narrow single-electron response. With a 14-stage PMT the anode
output pulse is usually large enough to be connected directly to the
input of the timing discriminator. Eight- or ten-stage PMTs may
require some amplification, as described in the introduction to
Preamplifiers and
Amplifiers. |