Photon Detection Efficiency Calculator (SiPM)
Work out a silicon photomultiplier's photon detection efficiency: detected photon events divided by incident photons, before dark-count corrections.
Photon Detection Efficiency Calculator (SiPM)
Background.
A silicon photomultiplier, or SiPM, is a grid of hundreds to tens of thousands of microscopic avalanche photodiodes wired in parallel and biased just above their breakdown voltage. In that state a single absorbed photon can set off a self-sustaining avalanche in one cell, which a series resistor then quenches, so the device can count individual photons. How many of the photons that reach it it actually counts is its photon detection efficiency, and that one figure decides how much light a PET scanner crystal, a LiDAR receiver or a scintillator in a physics experiment needs before a signal stands out.
Three probabilities multiply to give it. Quantum efficiency is the chance a photon creates an electron-hole pair in the sensitive silicon. Fill factor is the share of the surface that is actually sensitive, rather than given over to trenches, quench resistors and wiring between cells. Triggering probability is the chance that the freed carrier starts an avalanche, and it rises with the overvoltage, the bias above breakdown. So PDE is never a single number for a device: it changes with wavelength, with bias and, through the breakdown voltage, with temperature.
The figure here is the plain measured ratio: detected events divided by incident photons, times 100. Typically the incident number comes from a calibrated reference photodiode and the detected number from the SiPM's own pulse count.
That ratio is only as clean as the counts. Dark counts, optical crosstalk between cells and afterpulsing all add events that were not new photons, pushing the result up; dead time and saturation of the cells at high light levels push it down. None of these is corrected, so unless you remove them first the answer is an apparent PDE. A result above 100% is a sure sign that extra counts have crept in.
What is photon detection efficiency calculator (sipm)?
Photon detection efficiency (PDE) is the probability that a photon arriving at a silicon photomultiplier's surface produces a counted signal, expressed as a percentage. It is the product of quantum efficiency, geometric fill factor and avalanche triggering probability, so it varies with wavelength and with the overvoltage applied above breakdown. Measured directly, it is the number of detected photon events divided by the number of incident photons over the same exposure.
How to use this calculator.
- Enter the detected photon events: the SiPM counts recorded during the exposure, after subtracting the dark counts from a run of equal length with the light blocked.
- Enter the incident photons for the same exposure and the same area, usually taken from a calibrated reference photodiode: optical power divided by the energy per photon, hc/λ, multiplied by the exposure time.
- Use totals or rates for both inputs, as long as they share the same basis: both per second, both per light pulse, or both over the whole run.
- Read the PDE in percent, and record the wavelength, overvoltage and temperature with it, since each of them changes the result.
The formula.
PDE = N_detected ÷ N_incident × 100%. N_detected is the number of photon events the SiPM registered and N_incident the number of photons that reached its surface in the same interval; their ratio is a probability, and multiplying by 100 turns it into a percentage. Physically, the ratio estimates the product QE × FF × P_trigger of quantum efficiency, fill factor and triggering probability. The division is exact, but the inputs rarely are. The incident count normally comes from a reference detector, so its calibration error passes straight into the answer: an incident count 3% too high makes the PDE roughly 3% too low. Correlated noise inflates N_detected, while cell saturation at high light levels deflates it.
A worked example.
A test bench illuminates a SiPM with light at 420 nm. A calibrated reference photodiode shows that 100,000 photons reach the sensor during the exposure, and the SiPM registers 42,000 photon events. The ratio is 42,000 ÷ 100,000 = 0.42, and multiplying by 100 gives a PDE of 42%: a little over four photons in every ten are counted. That 42 is a raw figure. Suppose a dark run of the same length, with the shutter closed, had produced 1,500 counts. Subtracting them leaves 40,500 events, and 40,500 ÷ 100,000 × 100 = 40.5%, so the uncorrected figure overstated the efficiency by 1.5 percentage points. Crosstalk and afterpulsing would need a separate correction on top.
Frequently asked questions.
How do I find out how many photons actually hit the SiPM?
Why did I get a PDE above 100%?
Why does the PDE rise as I increase the overvoltage?
Why do careful PDE measurements count the light pulses that produced nothing?
Is photon detection efficiency the same as quantum efficiency?
References& sources.
- [1]IEC 60747-19-1:2019, Semiconductor devices — Smart sensors — Photodetectors (BIBLIOGRAPHIC/PAYWALL).
- [2]Hamamatsu Photonics, MPPC technical information.
- [3]BIPM, The International System of Units (SI Brochure), 9th ed., version 3.01, coherent derived units and quantity equations.
How this page was produced
- Published by
- Quanta Calculator
- Overseen by
- Daniel, Quanta Calculator Researcher
- Primary sources
- 3 cited below
- Method
- PDE = N_detected / N_incident × 100%
- Published
- Last verified
Built with AI assistance and verified by automated tests against the cited sources — every worked example on this page is computed by the same code that runs the calculator. How we build and check calculators.
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