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Avalanche Photodiodes

Author: the photonics expert

Acronym: APD; SPAD = single-photon avalanche diode

Definition: photodiodes with internal signal amplification through an avalanche process

More general term: photodiodes

Categories: article belongs to category photonic devices photonic devices, article belongs to category light detection and characterization light detection and characterization, article belongs to category optoelectronics optoelectronics, article belongs to category optical metrology optical metrology

DOI: 10.61835/pbn   Cite the article: BibTex plain textHTML

An avalanche photodiode is a semiconductor-based photodetector (photodiode) which is operated with a relatively high reverse voltage (typically tens or even hundreds of volts), sometimes just below breakdown. In this regime, carriers (electrons and holes) excited by absorbed photons are strongly accelerated in the strong internal electric field so that they can generate secondary carriers. The avalanche process, which may take place over a distance of only a few micrometers, for example, effectively amplifies the photocurrent by a significant factor, although not as much as in a photomultiplier. Therefore, avalanche photodiodes can be used for very sensitive detectors, which need less electronic signal amplification and are thus less susceptible to electronic noise.

Typical applications of avalanche photodiodes include receivers in optical fiber communications, range finding, imaging, high-speed laser scanners, laser microscopy, and optical-time domain reflectometers (OTDR).


avalanche photodiodes
Figure 1: Avalanche photodiodes. Source: Excelitas Technologies

The current amplification process strongly increases the responsivity of an APD. Note, however, that the amplification factor and thus the responsivity depends strongly on the reverse voltage, and may also substantially vary from device to device. Therefore, it is common to specify a certain voltage range within which all devices reach a certain responsivity. For precise measurements of low light powers, avalanche diodes are hardly suitable, since their responsivity is not nearly as well-defined as that of a p–i–n diode, for example.

Quantum Efficiency

Despite the high responsivity, the quantum efficiency of an APD is not necessarily high – certainly below 100% and possibly lower than for other photodiodes. This means that some of the incident photons do not contribute to the photocurrent, even though other photons do very much so, triggering an electron avalanche.

Materials and Wavelength Ranges

Silicon-based avalanche photodiodes are sensitive in the wavelength region from ≈ 450 to 1000 nm (sometimes up to 1100 nm), with the maximum responsivity occurring around 600–800 nm, i.e., at somewhat shorter wavelengths than for silicon p–i–n diodes. Depending on the device and the reverse voltage applied, the multiplication factor (also called gain) of silicon APDs can vary between 50 and 1000. For longer wavelengths up to roughly 1.7 μm, APDs based on germanium or indium gallium arsenide (InGaAs) are used. These have lower current multiplication factors of 10 to 40. InGaAs APDs are significantly more expensive than those based on germanium, but exhibit superior noise performance and a higher detection bandwidth. Their high absorption coefficient allows the use of a rather thin absorbing layer. Another possibility is to use germanium/silicon (GeSi) devices, where radiation is absorbed in germanium, and the carriers are transferred into a silicon region for charge multiplication [10, 14].

Less common semiconductor materials for APDs are gallium nitride (GaN) for ultraviolet light and HgCdTe for the mid-infrared up to wavelength of ≈14 μm (used under cryogenic conditions).

Detection Bandwidth

The detection bandwidth achievable with avalanche diodes can be quite high, although there is an inherent trade-off between bandwidth and amplification factor. On the other hand, the enhanced responsivity can allow the operation with a smaller shunt resistor than usable with an ordinary photodiode, and that effect may compensate for a possible speed disadvantage of an avalanche diode.

Detection Noise

The large responsivity of an APD can help to reduce detection noise, since it much reduces the impact of electronic noise in the subsequently used photodiode preamplifier. Therefore, the noise performance of photodetectors with APDs can be better than that of devices with ordinary p–i–n photodiodes when electronic noise is a limiting factor.

On the other hand, the avalanche process itself is subject to quantum noise and amplification noise, which can offset the mentioned advantage. The excess noise due to those effects is quantified with the excess noise factor <$F$>; that is the factor by which the electronic noise power is increased compared with that of an ideal photodetector. The amount of excess noise depends on many factors: the magnitude of the reverse voltage, material properties (in particular, the ionization coefficient ratio <$\kappa$>), and the device design. The excess noise factor increases with increasing amplification factor, as obtained for increasing reverse voltage. Therefore, the reverse voltage is often chosen such that the multiplication noise approximately equals the noise of the electronic amplifier because that setting minimizes the overall noise.

Geiger Mode for Single Photon Counting

When operated in the so-called Geiger mode with carefully designed electronics, avalanche photodiodes can be used even for single photon counting with dark count rates well below 1 kHz and with a quantum efficiency of several tens of percent, sometimes even well above 50%. The Geiger mode means that the diode is operated slightly above the breakdown threshold voltage, where a single electron–hole pair (generated by absorption of a photon or by a thermal fluctuation) can trigger a strong avalanche. In the case of such an event, an electronic quenching circuit reduces the voltage at the diode below the threshold voltage for a short time, so that the avalanche is stopped, and the detector is ready for detection of further photons after some recovery time of e.g. 100 ns. That dead time constitutes a substantial limitation of this technology. It limits the count rate to the order of 10 MHz, whereas an avalanche diode in linear mode (i.e., operated with lower reverse voltage) may be operated with a bandwidth of many gigahertz. So that such devices have a limited quantum efficiency, i.e., not every incident photon can trigger an avalanche.

Photon-counting APDs are also called SPADs = single-photon avalanche diodes. When optimized for high quantum efficiencies, they can be used in quantum optics experiments (for example, for quantum cryptography) and in some of the applications mentioned above if an extremely high responsivity is required. SPADs with optimized amplifier electronics are also available in CMOS integrated form, even as large photodiode arrays, e.g. for use as image sensors for single-photon 3D imaging via time-resolved detection [9].

Surprisingly, it is even possible to measure the number of photons absorbed within a certain short time interval in the active region of an avalanche photodiode [8]. For that purpose, it is necessary to precisely measure the rise of photocurrent at the beginning of the avalanche.

Avalanche Diode Modules

Avalanche diodes are available as part of modules, which apart from the photodiode also contain additional electronic components. In particular, there can be a current amplifier (transimpedance amplifier) integrated into the package, which not only reduces the number of parts required on a circuit board, but also improves the noise performance and results in a better combination of bandwidth and responsivity. Some modules have been specifically optimized for use in optical fiber communications systems and are fiber-coupled. It is also possible to integrate the quenching electronics required for Geiger mode operation.

Silicon Photomultipliers

An important difference between an avalanche photodiode and a photomultiplier is that the latter has a much larger active area. However, it is possible to construct so-called silicon photomultipliers, containing arrays of silicon-based avalanche diodes, where the combined active area can be fairly large.

Apart from the large active area, silicon photomultipliers are also suitable for measuring photon numbers [12], even if the single diodes are not: one may count the total number of diodes which are triggered by a weak incident optical pulse. That number approximates well the photon number (multiplied with the quantum efficiency) provided that the probability of more than one photon hitting a single diode is sufficiently small.


Another type of semiconductor-based photodetector, which also uses some kind of photocurrent amplification, is the phototransistor. Here, however, the amplification is based on different principles, and the operating characteristics are also quite different.

More to Learn

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The RP Photonics Buyer's Guide contains 27 suppliers for avalanche photodiodes. Among them:


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[15]A. H. Jones et al., “Low-noise high-temperature AlInAsSb/GaSb avalanche photodiodes for 2-μm applications”, Nature Photonics 14, 559 (2020); https://doi.org/10.1038/s41566-020-0637-6
[16]I. Straka et al., “Counting statistics of actively quenched SPADs under continuous illumination”, J. Lightwave Technol. 38 (17), 4765 (2020)
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