Sensors of light or other electromagnetic energy From Wikipedia, the free encyclopedia
Photodetectors, also called photosensors, are sensors of light or other electromagnetic radiation.[1] There are a wide variety of photodetectors which may be classified by mechanism of detection, such as photoelectric or photochemical effects, or by various performance metrics, such as spectral response. Semiconductor-based photodetectors typically
use a p–n junction that converts photons into charge. The absorbed photons make electron–hole pairs in the depletion region. Photodiodes and photo transistors are a few examples of photo detectors. Solar cells convert some of the light energy absorbed into electrical energy.
This article's lead sectionmay be too short to adequately summarize the key points. (January 2020)
A photodetector salvaged from a CD-ROM drive. The photodetector contains three photodiodes, visible in the photo (in center).
Photodetectors can be classified based on their mechanism of operation and device structure. Here are the common classifications:
Based on mechanism of operation
A commercial amplified photodetector for use in optics research
Photoconductive effect: These detectors work by changing their electrical conductivity when exposed to light. The incident light generates electron-hole pairs in the material, altering its conductivity. Photoconductive detectors are typically made of semiconductors.[5]
Photoemission or photoelectric effect: Photons cause electrons to transition from the conduction band of a material to free electrons in a vacuum or gas.
Thermal: Photons cause electrons to transition to mid-gap states then decay back to lower bands, inducing phonon generation and thus heat.
Polarization: Photons induce changes in polarization states of suitable materials, which may lead to change in index of refraction or other polarization effects.
Photochemical: Photons induce a chemical change in a material.
Weak interaction effects: photons induce secondary effects such as in photon drag[6][7] detectors or gas pressure changes in Golay cells.
Photodetectors may be used in different configurations. Single sensors may detect overall light levels. A 1-D array of photodetectors, as in a spectrophotometer or a Line scanner, may be used to measure the distribution of light along a line. A 2-D array of photodetectors may be used as an image sensor to form images from the pattern of light before it.
A photodetector or array is typically covered by an illumination window, sometimes having an anti-reflective coating.
Based on device structure
Based on device structure, photodetectors can be classified into the following categories:
MSM Photodetector: A metal-semiconductor-metal (MSM) photodetector consists of a semiconductor layer sandwiched between two metal electrodes. The metal electrodes are interdigitated, forming a series of alternating fingers or grids. The semiconductor layer is typically made of materials such as silicon (Si), gallium arsenide (GaAs), indium phosphide (InP) or antimony selenide (Sb2Se3).[5] Various methods are employed together to improve its characteristics, such as manipulating the vertical structure, etching, changing the substrate, and utilizing plasmonics.[8] The best achievable efficiency is shown by Antimony Selenide photodetectors.
Photodiodes: Photodiodes are the most common type of photodetectors. They are semiconductor devices with a PN junction. Incident light generates electron-hole pairs in the depletion region of the junction, producing a photocurrent. Photodiodes can be further categorized into: a. PIN Photodiodes: These photodiodes have an additional intrinsic (I) region between the P and N regions, which extends the depletion region and improves the device's performance. b. Schottky Photodiodes: In Schottky photodiodes, a metal-semiconductor junction is used instead of a PN junction. They offer high-speed response and are commonly used in high-frequency applications.
Avalanche Photodiodes (APDs): APDs are specialized photodiodes that incorporate avalanche multiplication. They have a high electric field region near the PN junction, which causes impact ionization and produces additional electron-hole pairs. This internal amplification improves the detection sensitivity. APDs are widely used in applications requiring high sensitivity, such as low-light imaging and long-distance optical communication.[9]
Phototransistors: Phototransistors are transistors with a light-sensitive base region. Incident light causes a change in the base current, which controls the transistor's collector current. Phototransistors offer amplification and can be used in applications that require both detection and signal amplification.
Charge-Coupled Devices (CCDs): CCDs are imaging sensors composed of an array of tiny capacitors. Incident light generates charge in the capacitors, which is sequentially read and processed to form an image. CCDs are commonly used in digital cameras and scientific imaging applications.
CMOS Image Sensors (CIS): CMOS image sensors are based on complementary metal-oxide-semiconductor (CMOS) technology. They integrate photodetectors and signal processing circuitry on a single chip. CMOS image sensors have gained popularity due to their low power consumption, high integration, and compatibility with standard CMOS fabrication processes.
Photomultiplier Tubes (PMTs): PMTs are vacuum tube-based photodetectors. They consist of a photocathode that emits electrons when illuminated, followed by a series of dynodes that multiply the electron current through secondary emission. PMTs offer high sensitivity and are used in applications that require low-light detection, such as particle physics experiments and scintillation detectors.
These are some of the common photodetectors based on device structure. Each type has its own characteristics, advantages, and applications in various fields, including imaging, communication, sensing, and scientific research.
There are a number of performance metrics, also called figures of merit, by which photodetectors are characterized and compared[2][3]
Responsivity: The output current divided by total light power falling upon the photodetector.
Noise-equivalent power: The amount of light power needed to generate a signal comparable in size to the noise of the device.
Detectivity: The square root of the detector area divided by the noise equivalent power.
Gain: The output current of a photodetector divided by the current directly produced by the photons incident on the detectors, i.e., the built-in current gain.
Dark current: The current flowing through a photodetector even in the absence of light.
Response time: The time needed for a photodetector to go from 10% to 90% of final output.
Noise spectrum: The intrinsic noise voltage or current as a function of frequency. This can be represented in the form of a noise spectral density.
Nonlinearity: The RF-output is limited by the nonlinearity of the photodetector[10]
Spectral response: The response of a photodetector as a function of photon frequency.
Grouped by mechanism, photodetectors include the following devices:
Photoemission or photoelectric
Gaseous ionization detectors are used in experimental particle physics to detect photons and particles with sufficient energy to ionize gas atoms or molecules. Electrons and ions generated by ionization cause a current flow which can be measured.
Microchannel plate detectors use a porous glass substrate as a mechanism for multiplying electrons. They can be used in combination with a photocathode like the photomultiplier described above, with the porous glass substrate acting as a dynode stage
Cadmium zinc telluride radiation detectors can operate in direct-conversion (or photoconductive) mode at room temperature, unlike some other materials (particularly germanium) which require liquid nitrogen cooling. Their relative advantages include high sensitivity for x-rays and gamma-rays, due to the high atomic numbers of Cd and Te, and better energy resolution than scintillator detectors.
HgCdTe infrared detectors. Detection occurs when an infrared photon of sufficient energy kicks an electron from the valence band to the conduction band. Such an electron is collected by a suitable external readout integrated circuits (ROIC) and transformed into an electric signal.
Photoresistors or Light Dependent Resistors (LDR) which change resistance according to light intensity. Normally the resistance of LDRs decreases with increasing intensity of light falling on it.[11]
Bolometers measure the power of incident electromagnetic radiation via the heating of a material with a temperature-dependent electrical resistance. A microbolometer is a specific type of bolometer used as a detector in a thermal camera.
Pyroelectric detectors detect photons through the heat they generate and the subsequent voltage generated in pyroelectric materials.
Thermopiles detect electromagnetic radiation through heat, then generating a voltage in thermocouples.
Golay cells detect photons by the heat they generate in a gas-filled chamber, causing the gas to expand and deform a flexible membrane whose deflection is measured.
Chemical detectors, such as photographic plates, in which a silver halide molecule is split into an atom of metallic silver and a halogen atom. The photographic developer causes adjacent molecules to split similarly.
A graphene/n-type silicon heterojunction has been demonstrated to exhibit strong rectifying behavior and high photoresponsivity. Graphene is coupled with silicon quantum dots (Si QDs) on top of bulk Si to form a hybrid photodetector. Si QDs cause an increase of the built-in potential of the graphene/Si Schottky junction while reducing the optical reflection of the photodetector. Both the electrical and optical contributions of Si QDs enable a superior performance of the photodetector.[20]
Bishop, P.; Gibson, A.; Kimmitt, M. (October 1973). "The performance of photon-drag detectors at high laser intensities". IEEE Journal of Quantum Electronics. 9 (10): 1007–1011. Bibcode:1973IJQE....9.1007B. doi:10.1109/JQE.1973.1077407.
