Silicon Photomultiplier (SiPM)

Take ten thousand Geiger counters, each the size of a red blood cell, and wire them together in parallel. Now they can count single photons of light — and tell you how many landed.

Detects light pulses ranging from a single photon to tens of thousands of photons per nanosecond with rise times under 1 ns. Unlike a vacuum photomultiplier tube, a SiPM is a few-mm² silicon chip that operates from a single 25–55 V bias, weighs almost nothing, is unaffected by magnetic fields, cannot be damaged by ambient light, and costs a fraction of a comparable PMT. SiPMs now form the photon-counting front-end of medical PET scanners, automotive LiDAR receivers, neutrino observatories, dark-matter detectors, and the high-luminosity LHC's CMS hadronic calorimeter.

The chip is etched into roughly 10,000 microcells per square millimetre, each microcell ~10–50 µm across. Every microcell is an avalanche photodiode reverse-biased a few volts above its breakdown voltage — so-called Geiger mode. In this regime a single photon-induced electron-hole pair triggers a self-sustaining avalanche that briefly draws 100 µA through the cell, producing a binary 'fired' signal. Each microcell is wired to a passive quenching resistor (typically 100 kΩ–1 MΩ polysilicon) in series; when the avalanche current develops, the resistor drops enough voltage to quench the avalanche in 1–10 ns, and the cell recharges to its operating point in 20–100 ns, ready for the next photon. All microcell outputs are connected in parallel on the chip, so the total output current is the sum of however many microcells fired in the same pulse — giving a quasi-analog 'photon counting' waveform whose pulse height resolves individual photon-number peaks (1, 2, 3, ... photoelectrons) up to roughly 100 photons per ~30 ns window before pile-up saturates the device.

In plain terms

Imagine a rain detector made of ten thousand tiny buckets — but each bucket only knows two things: 'a raindrop landed in me' or 'no raindrop yet'. By counting how many of the ten thousand buckets got hit in the same second, you can measure how heavy the rain is. A SiPM does the same trick with light: each tiny bucket is a 'micro-Geiger counter' that flashes when struck by a single photon, and adding them up tells you how bright the light pulse was.

Also called: SiPM, MPPC, Geiger-mode APD array, solid-state photomultiplier.

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A short history

Geiger-mode avalanche behaviour in silicon p-n junctions was first studied by Haitz at Shockley Laboratory in the early 1960s. Sergio Cova's group at Politecnico di Milano established practical single-photon avalanche diodes through the 1980s, building on McIntyre's 1966 theory of avalanche multiplication in silicon and introducing the active quenching circuit in 1981. Through the 1990s, Russian groups (Sadygov, Golovin, Buzhan) showed that arrays of SPAD microcells coupled by quenching resistors and read out on a common bus produced a quasi-analog photon-counting device — the silicon photomultiplier. Hamamatsu Photonics commercialised the multi-pixel photon counter (MPPC) in the mid-2000s. By the mid-2010s, SiPMs had reached parity with PMTs in single-photon timing and detection efficiency at far lower cost, weight, and operating voltage, opening the door to mass deployment in medical imaging, LiDAR, and high-energy physics. The transition was largely complete by 2020, with PMTs retaining a niche only in very-large-area (m²-class) applications where SiPM tiling remains cost-prohibitive.

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