- Open Access
PhotoniX volume 1, Article number: 22 (2020)
High-performance vacuum-ultraviolet (VUV) photodetectors are of great significance to space science, radiation monitoring, electronic industry and basic science. Due to the absolute advantages in VUV selective response and radiation resistance, ultra-wide bandgap semiconductors such as diamond, BN and AlN attract wide interest from researchers, and thus the researches on VUV photodetectors based on these emerging semiconductor materials have made considerable progress in the past 20 years. This paper takes ultra-wide bandgap semiconductor filterless VUV photodetectors with different working mechanisms as the object and gives a systematic review in the aspects of figures of merit, performance evaluation methods and research progress. These miniaturized and easily-integrated photodetectors with low power consumption are expected to achieve efficient VUV dynamic imaging and single photon detection in the future.
Vacuum-ultraviolet (VUV) spectrum is known to be in the wavelength range of 10–200 nm [1, 2], where the ultraviolet light is strongly absorbed by oxygen in the air and can only propagate in a vacuum, and that is the origin of its name. High-sensitivity detection of VUV light is of great significance to space science (space exploration, cosmic physics, etc.), radiation monitoring (synchrotron radiation, free electron laser, etc.), electronic industry (semiconductor lithography, surface technology, etc.) and basic science (analysis instrument, spectral physics, etc.) as shown in Fig. 1.
It is well-known that the sun tends to cause aurora, magnetic storms and ionospheric disturbance on the earth [3,4,5,6,7] in a period of intense activity, which will affect human life and even bring serious attacks on the earth. For example, in the famous Carrington Event in 1859, the solar storm destroyed the first primitive power system, leading to severe fire accident in a large number of telegraph systems and getting them burnt down . In the maximum solar spectrum of 2003 (solar storms struck the earth and induced powerful magnetic storms) and the minimum solar spectrum of 2008 , a significant difference can be observed in the VUV region, which indicates that VUV light detection is probably the most effective way to monitor space weather and track star evolution .
As the most direct tool for studying the interaction between light and atoms, molecules and condensed matter, VUV light is involved in many fields of basic science such as spectroscopy and photochemistry, which has become an important driving force for the development of various VUV photodetectors. More importantly, high-performance VUV photodetectors are essential to high-resolution semiconductor lithography  (such as 193 nm and 157 nm excimer lithography, 13.5 nm extreme ultraviolet (EUV) lithography), synchrotron and free-electron lasers (FEL) beam monitors .
Due to the limitation of atmosphere and the lack of related technologies, it’s difficult to carry out the researches on VUV photodetectors. At the end of the twentieth century, some solar-terrestrial physicists and cosmologists tried to load a combined system of Rowland chromatograph and microchannel plate [13, 14] on satellites for real-time solar VUV detection. However, these conventional detection systems require a driving voltage of several thousand volts, which imposes excessive burden of power supply on the operation of satellites. In the past 20 years, due to the advantages of miniaturization and ease of integration , VUV detectors based on the emerging ultra-wide bandgap (UWB) semiconductors have attracted researchers’ attention. A typical case is in 2009 when an ultraviolet diamond detector was applied to space for the first time and the vacuum ultraviolet solar radiometer Large Yield Radiometer (LYRA) was released on the European Space Agency’s PROBA2 [9, 16]. This on-board test first demonstrated the application potential of UWB semiconductor-based VUV photodetectors in solar physics research. Encouragingly, in the summer of 2018, NASA launched the first solar probe to complete the significant mission of exploring the mysteries of the sun at a distance of 7 million kilometers from its surface. A year later, the first research results of the Parker Solar Probe on the corona and solar wind were announced [17,18,19,20]. There is no doubt that the UWB semiconductor VUV detector definitely plays an indispensable role in this difficult task.
Photodetectors in the VUV region generally have to operate in a clean and ultra-high vacuum environment, and cannot interact or degrade in the presence of radiation. In addition, low level of background noise is needed to help detect relatively weak signals. Silicon photodiodes originally designed for the visible spectrum range can be used in the VUV region [21,22,23], but the significant disadvantage lies in the inherent wide-band response from X-ray to near-infrared and radiation degradation. The direct method to fabricate highly-selective VUV detectors with high radiation hardness is to use UWB semiconductors . Compared with the silicon-based detectors with relatively mature production technologies, UWB semiconductor-based detectors are still at a stage of rapid development, and significant improvements in terms of quantum efficiency, responsivity, response time, spectral response, and detection are required. Nevertheless, their absolute advantages in terms of VUV selective response and tolerance to harsh environments still attract a lot of interest from researchers [15, 25]. Their efforts like designing different device structures and studying different types or sizes of photosensitive materials to improve light absorption efficiency, carrier transmission efficiency and device lifetime have brought considerable development to UWB semiconductor-based VUV photodetectors and to the emergence of new VUV detection technologies.
In this review, we roughly divide UWB semiconductor detectors into three categories: photoconductive, photovoltaic, and avalanche based on the dominant working mechanism of devices in specific researches. Although the structure of the prepared device is clear, its actual working mechanism is often too complicated to be judged if without the help of experimental results. In a review published before, various VUV detection technologies such as photomultiplier tubes, scintillator detectors, Si-based photodetectors and gaseous detectors have been introduced . This review will focus on the ultra-wide bandgap semiconductor-based filterless VUV photodetectors, especially the figures of merit under different working mechanisms, performance evaluation methods and research progress.
Quantifying the performance of VUV photodetectors
The major physical mechanism of semiconductor photodetectors is photon absorption which changes the electrical properties of electronic systems. The performance of a photodetector depends on the optical absorption process, carrier transport and its interaction with the circuit system. The main performance indicators include quantum efficiency, responsivity, spectral response, response time, noise equivalent power and detectivity. But for VUV radiation, the radiation resistance of photodetectors, that is, the degree of decline in the above performance indicators after a certain amount of radiation, is also a figure of merit worthy of consideration and attention.
The internal quantum efficiency of photodetectors is defined as the number of carriers generated with per photon absorbed. In order to measure the number of carriers produced by each electron-hole pair, there is another widely-used concept called “photoconductive gain”, which depends on the carrier lifetime and the ratio of carrier transit time between the two electrodes. Generally, without considering the recombination loss, the internal quantum efficiency is equal to 1, but this value may be greater for photodetectors with internal gain mechanism. In practice, incomplete absorption will cause the number of photons absorbed by the detector to be less than that of incident photons, and the external quantum efficiency (EQE) is thus defined as the ratio of the number of generated carriers to that of incident photons.
Responsivity is another important parameter to describe the photoelectric conversion efficiency of photodetectors, which is defined as the ratio of the output signal of photodetectors to the unit incident light power. According to the difference of various output signals, responsivity can be divided into the current one and voltage one. Most photodetectors are selectively responsive to spectra, which is called spectral response, namely a property that the responsivity varies with the wavelength of incident light. For a filterless VUV photodetector, the responsivity in the VUV region should be much greater than the long-wave region (or no response in the long-wave region).
In many fields of application, the response speed of photodetectors should be faster enough to meet the working requirements when compared with the data rate of digital transmission. Thus, response time is another important parameter of photodetectors. The response time of photoconductive detectors is determined by the carrier lifetime which is related to the characteristics of semiconductors. When the illumination stops, the carrier concentration will decay with time in a certain rule.
Noise equivalent power is an important parameter to describe the detection capability of photodetectors. Its value is equal to the incident light power when the output voltage of photodetectors is exactly equal to the output noise voltage. When the photodetector operates in a condition that the background flux is smaller than the light (signal) flux, its ultimate performance will be determined by the signal fluctuation limit. Detectivity is defined as the reciprocal of noise equivalent power, which reflects the detection capability of detectors more intuitively. Since detectivity is proportional to the square root of illuminated area of the detector and the square root of amplifier bandwidth, the concept of normalized detectivity is introduced to eliminate this effect. The larger the normalized detectivity is, the stronger the detector’s ability to detect weak light will be.
Expression for photoresponsivity
For both photoconductive and photovoltaic detectors, photoresponsivity is the primary core evaluation indicator among all the parameters. In fact, this key parameter can be strictly described by mathematical formula if.with an ideal model.
For photoconductive detectors, the photoresponsivity depends on: 1) the intrinsic properties of photosensitive materials, such as carrier collection efficiency μτ (τ is the carrier lifetime, μ is the carrier mobility); 2) device structure, such as the spacing between positive and negative electrodes. Photoconductive gain (G) can be used as a bridge to deduce the specific expression. The current responsivity Rλ can be defined as Rλ = Iph/Pin (Iph is the photocurrent, Pin is the input optical power), which can be specifically expressed by the following formula .
In this formula, η stands for quantum efficiency (η = ηabsηtrans, ηabs: light absorption efficiency; ηtrans: charge transmission efficiency), V the driving voltage imposed on carriers, L the electrode spacing, e the electron charge, λ the wavelength and hc/λ the energy per photon. Therefore, the EQE of photoconductive devices can be described as EQE =η G.
Absorption coefficient, carrier transfer and collection efficiency are three indicators positively correlated with photoresponsivity, which are mainly determined by photosensitive materials. Therefore, semiconductor materials with excellent photoelectric properties are the primary choice in the design of high-responsivity photodetectors. Furthermore, in the design of device structure, vertical structure has more advantages than the horizontal one in reducing the spacing between positive and negative electrodes.
As for photovoltaic detectors, the photoresponsivity can also be described by Rλ = Iph/Pin. Generally speaking, the gain of photovoltaic detectors is 1, that is to say, the number of photo-generated electron-hole pairs equals to that of carriers contributing to the current. Therefore, the expression of photoresponsivity for photovoltaic detectors is Rλ = ηeλ/hc, in which the EQE of photovoltaic devices is expressed as EQE =η. The analysis of the working mechanism of photovoltaic detectors mainly focuses on the carrier drift and diffusion processes. In theory, it can be deduced from simplified ideal models, such as Poisson equation and continuity equation; but in practice, the mechanism of devices tends to be much more complex because of the existence of defects in semiconductors and dislocations at heterojunctions. Therefore, in addition to the optimized design of device structure, the growth of high-quality semiconductor materials is also a decisive factor that influences the performance of photovoltaic detectors.
Balance between photoresponsivity and response time
For photoconductive detectors, external bias voltage is required for the device to work. In theory, there is no upper limit for R as well as for the corresponding external quantum efficiency. The photoresponsivity of the device is positively correlated with the response time: Rλ ∝ f(t), Rλ = I0 + Is/Pin, where I0 refers to transient photocurrent and Is is persistent photocurrent . The longer the lifetime of trap state is, the larger the Is and Rλ of the device will be, but at the same time, the recovery time of the device from on to off will also be longer .
In general, when photoconductive detectors absorb photons and generate electron-hole pairs, the majority of carriers (electrons) will have higher mobility with a shorter transit time than carrier lifetime; while the minority of carriers (holes) move slowly with a longer transit time than carrier lifetime. In this case, the electrons are quickly swept out of the detector, and the holes inside are redundant, and the other electrode needs to provide electrons to maintain electrical neutrality. Through such behavior, electrons can go back and forth for multiple times during the carrier lifetime, and the photodetector can thus obtain a larger gain, which is commonly understood as persistent photoconductivity. The longer the recombination life of the carriers is, the greater the responsivity of the photodetector will be. However, this mechanism will inevitably lead to an increase in switching response time, as shown in Fig. 2a, b.
Therefore, in practical application, it is necessary to make a trade-off between the two key indicators of responsivity and response time. The carrier lifetime is not only related to the properties of semiconductors, but also to the lifetime of trap states. For high-quality semiconductors with smooth surface and low defect density, when the illumination is stopped, carriers can recombine more rapidly, thus inhibiting the persistent photoconductive effect caused by excess carriers, so a faster response speed is easier to be achieved.
For photovoltaic detectors, the gain is 1 in general. Thus, in the absence of bias voltage, the photoresponsivity has an upper limit of Rλ = eλ/hc, corresponding to EQE = 100%. Semiconductor depletion region with high electric field, which is used to separate photo-generated electrons from holes, is the most important factor to the performance of photovoltaic detectors. On the one hand, the depletion region must be kept very thin to shorten the transit time; one the other hand, it must be thick enough to absorb most of the incident light. Therefore, in practical application, the thickness of depletion layer must be adjusted appropriately to obtain the optimal quantum efficiency and frequency response. For photovoltaic detectors with a certain structure (with certain width of depletion layer, the detection performance of the device mainly depends on the physical properties of semiconductor materials whose photoresponsivity is negatively correlated with the response time: Rλ ∝ f(1/t). As illustrated in Fig. 2c, d, the existence of trap states in semiconductors not only reduces the collection efficiency of photo-generated carriers, which leads to a decrease in photoresponsivity, but also increases the response decay time of the device. Thus, it is easier for the photovoltaic detectors based on high-quality semiconductor with low defect density to achieve high responsivity and fast response speed at the same time.
Avalanche gain mechanism
When a large reverse bias voltage is applied to the junction region, the carriers moving in a strong electric field obtain electric field energy and thereby generate new electron-hole pairs through collisional ionization. The newly-generated secondary electrons and holes move to the opposite direction with the influence of electric field, and a new collision ionization can be generated in the movement. A series of collision ionization causes the avalanche multiplication of the number of carriers. Obviously, devices that operate under an avalanche gain mechanism have greater responsivity and are more suitable for detecting weak optical signals. The multiplication factor is an important parameter used to describe the avalanche effect on the device current amplification factor. In addition, the noise equivalent power is also a key parameter to measure the performance of the avalanche detector. The low noise can be achieved by using two materials with large difference in ionization ability of carriers, that is, carriers with higher ionization ability are injected into the depletion layer. Overall, low-noise and high-gain avalanche detectors have extremely high requirements for the quality of materials and the uniformity of structures.
For the test of the indicators of the photodetector mentioned above, harsh experimental conditions like vacuum environment, VUV light source, special optical components and high-precision electrical instruments are required. One common method to obtain the figure of merit of a photodetector is using a standard synchrotron radiation source (Fig. 3a). Another method is to use a standard detector as the transfer testing standard in the laboratory (Fig. 3b). Typical laboratory VUV light sources include deuterium lamps (continuous spectrum), low-pressure mercury lamps (185 nm), xenon excimer lamps (172 nm), ArF excimer lasers (193 nm) and F2 excimer lasers (157 nm). Simultaneously, since conventional optical research materials have a strong absorption effect on VUV light, special windows, gratings, filters, etc. are needed, which leaves many physical difficulties and challenges to the performance evaluation of VUV photodetectors. Therefore, the development of related technologies for detector testing has also received increasing attention.
VUV-sensitive UWB semiconductors
Diamond with excellent physical properties such as high thermal conductivity, small dielectric constant, and large bandgap energy (~ 5.5 eV, corresponding to the absorption edge of ~ 225 nm) has become an ideal choice for many electronic and optoelectronic applications . In addition, it has been proven to withstand high temperatures, high ionized particle flow as well as intense X-ray and VUV radiation [31,32,33,34]. Attempts have been made long before to apply natural or synthetic diamonds to VUV detection technology [35, 36]. However, photodetectors require diamond films to have sufficiently low defect and concentration of n-type and p-type dopants, otherwise the satisfactory detection performance cannot be achieved. Since natural and high-quality diamonds are very expensive and rare, many research teams are committed to exploring how to grow high-quality single crystal diamond films at a low cost [37, 38].
As one of the III-V nitrides materials, cubic BN (c-BN) manifests a series of extreme properties similar to or even better than those of diamond. In sphalerite structure, the atomic density of cubic BN with sp3 atomic bond is only 4.3% less. Its thermal conductivity is only inferior to diamond, while its oxidation and graphitization temperatures are much higher than those of diamond . More importantly, c-BN’s bandgap (~ 6.3 eV) is larger than the diamond’s [40, 41], and c-BN can be doped to form n-type and p-type conductivity, which is still difficult for diamond [42, 43]. Unfortunately, the application of c-BN to VUV photodetectors is seriously hampered by the poor quality of available materials (random orientation, limited thickness of films, poor crystallinity and adhesion to substrates caused by non-cubic BN interlayer) . Therefore, similar to the case of diamond, the research on c-BN-based VUV detectors also focuses on how to prepare high-quality film materials . The similarity of structure, properties, technical development and application between diamond and c-BN demonstrates that the synthetic methods of these materials are of mutual referential significance.
As a van der Waals material with excellent long-term stability and electric insulation, two-dimensional (2D) h-BN (Eg = 5.955 eV) with layered structure is an ideal material for VUV detection [46, 47]. In recent years, h-BN has attracted wide attention in the field of vacuum ultraviolet detection due to its low-dimensional conductive channel, high trap state surface density and high photocurrent gain. Current methods available for preparing atomic-scale h-BN nanosheets for VUV detectors include mechanical exfoliation, metal organic chemical vapor deposition, short pulse plasma beam deposition and ion beam sputtering deposition [48,49,50,51,52,53].
Aluminum nitride (AlN) with ultra-wide direct bandgap (~ 6.2 eV, corresponding to the absorption edge of ~ 200 nm) is another photosensitive material with VUV detection potential among III-V nitrides, which can suppress background noise internally. The high thermal and chemical stability  and excellent radiation resistance make it an ideal material for luminescence [55, 56] and VUV detection . Previous studies have shown that AlN epitaxial layers with optical quality comparable to GaN can be grown on sapphire through metal organic chemical vapor deposition (MOCVD) [58,59,60,61], which lays the foundation for the research of detectors based on high quality AlN films.
In addition to the widely-reported semiconductor materials, many other materials with ultra-wide bandgap are also worthy of exploration and further application especially nitrides [62, 63] and oxides. 2D MgO is an example. It has an ultra-wide energy bandgap of about 7.3 eV . In view of that it does not have the same layered structure as h-BN, thus a two-step conformal anneal synthesis method has been proposed to provide a universally applicable way for the growth of other two-dimensional oxides with layered precursors, such as NiO, CaO, CrO, etc. What’s more, this is also an effective method to obtain VUV-sensitive materials with specific band gaps through the mixed growth of two different band-gap semiconductors such as MgGaO and MgZnO.
It should be noted that although some UWB semiconductors such as AlGaN, GaN, ZnO, Ga2O3 and SiC have also been demonstrated to have the potential for VUV detection, filters are still required in some applications due to bandgap limitations. The semiconductor materials with larger bandgaps (diamond, BN, AlN, etc.) as a focus of this review do not require filtering in practice.
Photoconductive VUV photodetectors
As we all know, the structure of photoconductive detector is usually a semiconductor with two ohmic contacts, which represents a simple and low-cost structural design. In the past decade, considerable progress has been made in the development of photoconductive photodetectors based on these emerging semiconductor materials, and film-structure and nano-structure materials with high quality have been successfully prepared (the quality of materials is the key factor limiting their development).
Chemical vapor deposition (CVD) and high-pressure high-temperature (HPHT) are the two common methods for diamond film growth. In 2005, Z. Remes et al  reported the experimental results of photocurrent spectra and instantaneous decay of photocurrent of intrinsic CVD diamond films grown on natural (100) oriented and single-crystal IIA diamond substrates in the same epitaxial manner. The long effective lifetime of photogenerated carriers led to a typical sensitivity that is about 10− 2 A/W at 200 nm, and a response time less than 0.1 ms. Concurrently, Balducci et al  reported the photoresponse characteristics of single-crystal diamond-based VUV detectors by microwave CVD. The photocurrent of the device at 30.4 nm and 58.4 nm proves the photoelectric detection ability of as-fabricated detectors in the extreme ultraviolet spectral region. Moreover, the diamond thin-film detector exhibited long-term stability over 98 h under VUV radiation of 10 mW/cm2 . Excellent long-term stability is one of the important factors for transfer standard detectors in the VUV band .
Metal-semiconductor-metal (MSM) diamond photodetectors have been used in the LYRA  of the vacuum ultraviolet solar radiometer. LYRA can provide four ultraviolet bands of solar radiation data with a temporal resolution up to 10 ms, which provides an effective technical support for space solar activity monitoring. In order to evaluate the usability of photoconductive diamond detectors in lithography, measurements were performed by using various VUV light sources, including low-pressure mercury lamp, xenon excimer lamp, ArF excimer laser and synchrotron radiation (EUV) . The device can detect a 193 nm laser with a pulse width of 5 ns and has a good linear output within a certain energy range. In addition, it is found that the diamond ultraviolet detector has a higher spectral responsivity in the wavelength range of 10-33 nm. These results disclose that diamond detectors have great application potential both for 193 nm and EUV lithography. Since photodetectors are usually packaged in grounded metal vacuum chambers for detection, the photoemission current contributes to the output current. Especially for short-wavelength detection in the VUV range, the photoemission current is not negligible . It is found that in the 10–60 nm wavelength range, the light emission current dominates when the wavelength is greater than 40 nm, while the internal photocurrent plays a major role when the wavelength is less than about 25 nm . In recent years, the development of new device structures mainly focus on improving the light absorption efficiency and carrier transmission efficiency of diamond detectors, including the use of electrodes of different materials, the design of electrodes of different shapes and sizes, and the construction of three-dimensional structures [71,72,73,74]. Among them, an all-carbon diamond photodetector achieves the best photoresponsivity of 21.8 A/W (218 nm, 50 V bias) .
Compared with traditional bulk and thin-film structure materials, low-dimensional nanostructured detectors that have a quantum confinement effect on carriers [75,76,77] are more likely to have higher response rates and faster response speed. Moreover, nano-scale materials have a strong self-exclusion effect of impurities, which makes defects fewer and crystalline quality higher .
In order to prepare a VUV photodetector based on low-dimensional AlN, a two-step physical vapor transport method is designed to break the bottleneck of growing defect-free and high-quality micro/nanowires . The method includes a high-temperature process for growing AlN single crystal and a temperature-optimized auxiliary annealing process for reducing defects in nanostructures . Photodetectors based on AlN micro/nanowires are constructed by depositing Au (20 nm) electrodes at an interval of 10 μm onto the micro/nanowires on sapphire substrates, in which the tail of AlN micro/nanowires is covered with indium to improve the physical contact between metal and semiconductor (Inset of Fig. 4a). In addition to the expected low dark current and high breakdown voltage, the spectral response curve indicates that when the energy of incident light exceeds the threshold of 200 nm (6.2 eV), the detector exhibits significant photocurrent gain with a cut-off wavelength of 208 nm (Fig. 4a).
2D materials can efficiently collect photo-generated carriers, which benefits from the low-dimensional conductive channel for fast carrier collection and the high surface state density for photocurrent gain absorption. Typically, VUV photodetectors based on 2D h-BN and MgO with MSM structure are constructed [27, 80] and their VUV detection performance is tested by using synchrotron radiation. The detectors are not only capable of identifying VUV signals of very weak pw power levels, but also achieving external quantum efficiencies up to 2133% and 1539% respectively at certain bias voltages (Fig. 4b, c). This ultra-high photoconductivity gain is mainly due to the contribution of the sustained photoconductivity effect to the photocurrent. The trap centers on the surface of the 2D material to capture the photogenerated carriers and to help form additional electron transport channels (Fig. 4d). Compared with photoconductive detectors based on bulk and film materials, these two two-dimensional materials have been greatly improved when it comes to the response speed (milliseconds).
Although the universal applicability for VUV detection of the photoconductive detectors mentioned above has been proven, further research is necessary on these UWB semiconductors and related technologies to improve the device performance, so as to meet the requirements of practical application in VUV detection. Especially for photoresponse dynamics, methods such as deliberately introducing recombination centers can be implemented to reduce the carrier lifetime and to avoid the nonlinear response.
Photovoltaic VUV photodetectors
Compared with photoconductive VUV detectors, the advantage of photovoltaic VUV detectors exists in the possibility of achieving zero power consumption. Also, because of the built-in electric field used to separate photogenerated carriers, the photovoltaic device can achieve ultra-fast response speed, which is expected to replace the bulky and high-power-consumption conventional VUV detection system in the future.
Single Schottky-barrier photodiodes
For p-doped diamond with boron, the construction of the Schottky structure is feasible. Both planar and vertical configurations can implement Schottky barrier photodiodes. Liao et al. proposed a single Schottky barrier photodiode with interdigitated ohmic contact and Schottky contact (Fig. 5a), which can operate with high gain in photoconductive mode and achieve fast response speed in depletion mode . The homoepitaxial diamond layer was grown on a HPHT synthetic Ib (100) diamond substrate containing typically 100 ppm nitrogen by using a microwave plasma-enhanced CVD technique. Under 220 nm irradiation, the EQE reached 20% at a reverse bias of 30 V and a responsivity more than 18 A/W was obtained at a forward bias of − 23 V. Another vertical structure was constructed by Almaviva et al [82, 84]. Similarly, a conductive boron-doped diamond homoepitaxial layer was grown on a low-cost synthetic HPHT-Ib single crystal diamond substrate by microwave plasma-enhanced CVD and then an intrinsic diamond with a thickness of about 2 μm was uniformly epitaxially grown on the doped layer as a light absorbing layer (PIM structure, Fig. 5b). The diamond detector’s responsivity and EQE under two different bias voltages in the 20-80 nm wavelength range are shown in Fig. 5c . The dependence of the device’s response on the applied bias voltage varies with the incident wavelength, which may be due to the increase in surface and volume recombination caused by the change in penetration depth. In order to compare the performance of the planar and vertical structure detectors above, the p-type diamond interdigitated electrode was used to construct ohmic contact to control the variables (IDT-PIM structure) . The responsivity of these two different structures varies with wavelength in opposite directions, and it is obvious that the vertical structure is more advantageous in the short wavelength band (Fig. 5d). In addition to the Al electrodes, vertical TiN electrodes have also been used to construct diamond detectors by DC magnetron sputtering and lift-off methods . The detector achieves a responsivity of 0.325 A/W (30 V, 210 nm) and a decay time of ~ 1.2 ms. The EQE of the device exceeds 100% at 60 V bias, which indicates the existence of a certain gain mechanism.
Back-to-back MSM photodiodes
The MSM photovoltaic detector consists of two interdigitated back-to-back diodes, which does not require p-type doping of the semiconductor, and has the advantages like simple structure (planar structure), high sensitivity and easy integration. This structure is often implemented by UWB semiconductor-based detectors for which doping is hard to be achieved.
The high surface energy and small atom spacing of c-BN  hinder its formation on heterogeneous substrates. Therefore, the selection of substrate materials for depositing c-BN thin films becomes an arduous task of repeated experiments. Some people have tried to grow c-BN on silicon , aluminum nitride  and diamond [89,90,91] substrates, among which diamond has been proved to be the optimal substrate for the heteroepitaxial growth of c-BN. Subsequent studies have shown that diamond can be deposited as a general intermediate layer on a variety of materials with good adhesion and crystallinity to form composite structures for the growth of pure (i.e. not in the form of non-cubic BN) and adhesive c-BN films on all these materials [92,93,94]. It has been reported that with the help of He-Ar-N2-BF3-H2 gas mixture, a VUV photodetector based on c-BN films was fabricated by depositing c-BN films on diamond-coated silicon substrates in an electron cyclotron resonance microwave plasma CVD system (Fig. 6a) . The collimating and tunable monochromatic beams were used to measure the spectral response of a c-BN-based photodetector and the spectral responsivity curve was plotted by using AXUV silicon photodiode for calibration. It can be observed from Fig. 6b that under the bias voltages of − 20, − 30 and -35 V, the maximum response at about 180 nm is 12, 23 and 32 mA/W respectively. At about 193 nm, the device has a very sharp cut-off wavelength corresponding to the bulk c-BN bandgap. The measured rejection ratio (the ratio of responsivity between 180 and 250 nm) exceeds four orders of magnitude, suggesting that c-BN-based detectors are able to directly detect VUV radiation and eliminate any mid-ultraviolet noise.
For AlN with difficult p-type doping, the back-to-back MSM structure is a comprehensive optimal choice. Researchers demonstrate the development and utilization of high-quality AlN thin films in VUV photodetectors, and their outstanding characteristics are reported . Figure 6c shows a schematic diagram of the device layer structure used in this study, which adopts an undoped 1.5-um-thick AlN epitaxial layer as the active layer. The device presents extremely low dark current of about 100 fA at a bias voltage of 200 V (system limitation). The peak response of 200 nm, pretty sharp cut-off wavelength of 207 nm, and VUV to UV/visible light rejection ratio of more than four orders of magnitude all indicate that AlN-based photodetectors are promising in the application of VUV detection. Later, Tsai et al. fabricated a MSM photodetector by deposing the AlN film on Si (100) substrates, which showed high temperature resistance and radiation tolerance for harsh environments .
It is well-known that high-density threading dislocations (TDs) and inverted domains (IDs) with N polarity significantly reduce the performance of III nitride-based devices. Pantha et al have observed a strong correlation between the dark current and sensitivity of MSM photodetectors in MOCVD AlN and the TD density . In order to investigate the effect of ID on the photoelectric properties of AlN-based MSM photodetectors, Large-area MSM photodetectors based on AlN layers with different densities of IDs have been fabricated, and the effects of ammonia molecular beam epitaxy growth conditions on the structure and morphology of AlN have been studied . The results show that the smallest root-mean-square (rms) roughness and the optimal crystal integrity are generated by nitriding at high ammonia flow rate. Subsequent TEM measurements verify that the ID originates from the sapphire/AlN interface. After the growth of nucleating layers of AlN, two AlN/GaN short-period super-lattices are introduced to significantly reduce the ID density by an order of magnitude, while the TD density is basically unchanged. Both low-density and high-density ID samples are used to fabricate MSM photodetectors. Athough the device with ID density of 106 cm− 2 (low density) has a performance comparable to that with AlN grown by MOCVD, its responsivity is very poor. This is because illumination or photo-degradation will result in a decrease of photocurrent, which can be attributed to the formation of metastable defects of positioning carriers [101,102,103].
Similar to diamond, the well-known parasitic phenomenon is that when the photo-generated electrons have enough energy, they will emanate photoemission from the device. In order to verify the applicability of AlN-based MSM photodetectors for VUV detection, Ben Moussa et al  studied the influence of photoemission current on output signals. At the PTB-Bessy II Synchrotron Radiation Beam (B), the AlN MSM photodiode is mounted in the operating stage bracket. It is concluded that the whole circuit is biased to the energy higher than the maximum kinetic energy (e.g. dozens of electron volts) that can be obtained after electrons leave the surface. In other words, the AlN MSM detector is operated at positively high bias voltages to maximize output signals and to reduce the escape probability of electrons, which thus proves that photodetectors based on wide band-gap semiconductors have the advantages of high rejection ratio and high output signal in VUV solar observations. For practical application, the optical components of detectors are usually directly exposed to solar radiation, so ionization and atomic displacement damage effects are the main reasons for the degradation of space instruments. In order to explore their effects, the same research group  manufactured a large-area AlN circular MSM detector with diameter of 1.1–4.3 mm by using an interdigital electrode with a width of 2 μm and a spacing of 5 μm (Fig. 6d), and it was mounted in a ceramic package with a removable glass protective device. The spectral responsivity and irradiation stability of the device in the wavelength range of 40–700 nm are measured. As shown in Fig. 6e, the detector exhibits a high rejection ratio of about five orders of magnitude between 200 nm and 450 nm, which meets the strict requirement for unfiltered VUV solar observations. After the exposure to protons with 14.4 MeV energy, no significant reduction in detector performance is observed (Fig. 6f), which shows good radiation tolerance and further proves the universal feasibility of AlN MSM detectors for space application.
Heterojunction photovoltaic photodetectors
The selection and optimization of the functional layer is the key to the preparation of heterojunction photovoltaic vacuum ultraviolet detectors, which is involved in energy band engineering. Typically, several PIN diamond photodiodes of circular shape have been fabricated for the solar mission LYRA [105, 106]. The p-type and n-type doping of diamond was achieved by boron and phosphorus, respectively, and a thin Al layer (< 10 nm) with a transmittance of typically 20% to 50% was deposited for the top contact. The responsivity of the detector is 27.2 mA/W at 200 nm, displaying a UV/visible ratio (200 nm/500 nm) of six orders of magnitude. In the wavelength range of interest, PIN photodiodes are reasonably homogeneous, linear and stable under brief irradiation, which have the potential to meet the requirements of LYRA.
For UWB semiconductors as photosensitive layers, it is difficult to obtain an optimal upper window layer (conductive transmission layer) that is transparent to VUV light. Although the VUV transmittance can be improved by reducing the thickness of the metal electrode, the transmittance of even a thin layer (≤10 nm) is not large enough. Graphene (Gr) is widely used as electrode material because of its high mobility. Recently, Gr has been revealed to have a transmittance up to 96% by ultraviolet spectrum transmission experiments  in the VUV band due to its weak resistance to electromagnetic waves  (Fig. 7a). Therefore, graphene is an excellent candidate for the conductive window layer of VUV photovoltaic detectors.
The construction of a heterojunction photovoltaic device (Fig. 7b) with a PN characteristic vertical structure by using p-type graphene as a transparent electrode to collect carriers confirms the availability of graphene studied by Zheng et al.  With the back-to-back heterojunction structure of p-Gr/AlN/p-GaN, the thermal diffusion of carriers is effectively suppressed , resulting in a lower noise voltage density, which contributes to the detection of ultra-weak VUV signals. Under the irradiation of 185 nm monochromatic light (from the characteristic spectral line of low-voltage mercury lamp), an electromotive force of 1.7 V will be formed at both ends of the device and a stable open-circuit voltage can be output, but in dark state and under 250 nm light no response is seen (Fig. 7c). A thick space charge region is formed in the heterojunction composed of high-carrier-concentration p-Gr and low-carrier-concentration i-AlN. When VUV photons penetrate graphene into the absorption layer of AlN, most of them are absorbed in the space charge region near the p-Gr side of AlN to produce photo-generated electron-hole pairs. Then, electrons and holes are separated by the built-in electric field: the holes drift to the p-Gr side, while the electrons drift to the opposite direction, resulting in an open-circuit voltage of 1.7 V. Time response test is conducted by using 193 nm nanosecond pulses to simulate ultra-fast changing VUV signal sources, showing that the device has an encouraging ultra-fast rise time of only 80 ns (Fig. 7d) which is 104–106 times faster than that of the VUV detectors reported currently.
Drawing on the work above, VUV detectors based on other UWB photosensitive materials are also introduced. As we know, the band gap can be controlled by adjusting the composition of the compound. For example, the compound with a band gap between 4.8–7.3 eV can be obtained by the mixed growth of MgO and Ga2O3. Amorphous MgGaO (~ 6.0 eV) is grown on n-type GaN  and n-type SiC  substrates respectively, and the responsivity of 2 mA/W and 10 mA/W (under 185 nm radiation) are obtained by using graphene as window layer. In addition, graphene has also been used to construct diamond heterojunction detectors . The research results above prove the universality of using graphene to construct heterojunction VUV detectors, and provide a new scheme for the development of integrated VUV photodetectors with zero power consumption, ultra-high speed and high sensitivity.
Improvement of photovoltaic performance
We have noticed that in the impulse response experimental results of the above studies, the decay time of the device at room temperature is still much longer than the ultrafast rise time of photoresponse. In order to explore the response time mechanism of the device for the reduction in decay time, a p-Gr/AlN/n-ZnO heterojunction photovoltaic detector with PIN characteristics is constructed . According to the previous description, the rise time of photodetectors mainly depends on the transit time of the uncaptured photo-generated carriers drifting to the electrodes, while the exponential response attenuation mainly results from the capture of photo-generated carriers by internal defects and/or surface states, that is, the lifetime of so-called trap states directly determines the decay time of photo-response. Therefore, it is theoretically possible to use external heating to provide active energy for trap carrier escape and accelerate the annihilation of trap states, and then the carriers can be quickly collected instead of being captured by trap centers to reduce decay time. Temperature-dependent time response tests (Fig. 8a) confirm the effectiveness of the proposed strategy. With the increase of temperature, the photocurrent of the device gradually increases, while the decay time of the device decreases rapidly (Fig. 8b). Furthermore, the proposed instantaneous response mechanism of thermally-enhanced wide-bandgap semiconductor-based photovoltaic devices is universally applicable.
As we all know, for photovoltaic detectors, increasing the open-circuit voltage of the device is useful to obtain a larger voltage signal output and higher external quantum efficiency [116, 117]. For vertical structure heterojunction detectors, efficient energy band assembly is the key method to increase the potential difference across the device and then to increase the open-circuit voltage . The optimized device structure is designed through comparison of different electrode materials by Jia et al., and an open-circuit voltage of up to 2.45 V was realized for the first time (Fig. 8c) . Under irradiation, the holes generated by the AlN absorption layer are injected into the graphene, so that the density of the hole state of the graphene increases significantly, resulting in the Fermi level’s being lowered. Predictably, this detector exhibits high EQE (56.1%) and fast response speed (rise time≈45 ns). This work clarifies the various possibilities brought by the unique properties of graphene to improve the performance of the device through the effective comparison experiment of control variables for the first time.
Obviously, one of the significant advantages of semiconductor detectors is their ease of integration, which is also the ultimate development trend of UWB semiconductor-based VUV detectors for a wide range of applications. For example, the most intuitive way to monitor solar storms is to use VUV detectors for imaging . In order to realize VUV imaging, ultra-fast response speed is the primary requirement. Moreover, the array structure of detectors is also needed. AlN-based VUV detectors have been demonstrated in the aspect of their integrability: Twenty p-Gr / AlN / p-Si composite heterostructure arrays are fabricated on silicon wafers (the size of each unit is 200 μm × 5 μm) . The circular VUV spots of a certain diameter are obtained through the focus of quartz objective lens for imaging test. When the y-axis is fixed, a linear image can be obtained first. Later, with the movement of the device along the y-axis, the final VUV image can be obtained by the detection of interline currents (Fig. 8d). The excellent detection performance of the device unit is a prerequisite for obtaining the expected imaging, and further research on the large-area process technology still requires researchers’ great efforts.
Avalanche VUV photodetectors
Broadly speaking, avalanche detector also belongs to a photovoltaic detector according to its structure. However, since its working mode and mechanism are special, it is discussed separately here. Avalanche photodetectors have the advantages of high sensitivity, fast speed and high optical gain. The reverse bias applied to the junction is close to the breakdown voltage to stimulate the avalanche effect. Because the realization of avalanche VUV detectors has high requirements for the quality of UWB materials and construction processes, and it is limited by cost and technical difficulties, thus there is still few researches in this field. Nonetheless, the application potential of UWB semiconductor-based avalanche VUV detectors in many cutting-edge technologies such as single photon detection should still be valued.
Avalanche multiplication effect in diamond
High breakdown voltage or field is considered as a major advantage of diamond. So far, the charge multiplication effect has been observed in intrinsic, p-type and n-type doped CVD diamond structures [120,121,122]. Due to the difference in doping concentration and device structure or insufficient design, the data reported in various literature are different. Among them, the result of a high breakdown field of 20 MV/cm is relatively reliable and reproducible. Atsushi Hiraiwa et al. established a method to extract the ionization coefficient from the arbitrary relationship between breakdown voltage and doping density and developed a method to simplify the ionization integration . It is found that the breakdown field of diamond is more dependent on the doping density than other materials. Although the enhanced activation of impurities at high temperature significantly improves the performance of diamond, the problem of thermal runaway still needs attention. An accurate understanding of these physical processes is essential to the design and application of high-performance detectors. At present, the application demonstration of diamond-based avalanche detectors is mostly in the field of particle detection. More evaluation on the VUV detection performance of diamond-based avalanche detectors are still in demand.
AlN avalanche photodetectors
The growth of high-quality crystals and the lattice matching of different functional layers are the prerequisites for achieving low-noise and high-gain detectors. The high-quality AlN and SiC interface and good lattice matching (the mismatch rate is 1%) [124, 125], as well as the presence of a conductive SiC substrate, provide feasibility for the preparation of AlN / n-SiC vertical avalanche detectors. An avalanche detector based on AlN / n-SiC Schottky diode structure has been reported [126, 127], and its schematic diagram is shown in Fig. 9a. Schottky contact area is defined by evaporating a 6 nm thick Pt layer followed by photolithography and lift-off. The peak response wavelength and cut-off wavelength are 200 nm and 210 nm, respectively. At a reverse bias of − 250 V (Eb = 2.8 MV/cm), a photocurrent gain of 1200 is achieved (Fig. 9b) . In order to realize the device working in Geiger mode, further researches on reducing the dislocation density, optimizing the device size and geometric structure still need to be carried out.
Photosensitive materials such as diamond, c-BN, AlN, etc. with the advantages of high radiation hardness, low dark current, high chemical stability and room temperature thermal stability have great application prospects in vacuum ultraviolet detection. Researches on photodetectors based on these emerging semiconductor materials have made considerable progress. The film-structure VUV detector may move faster towards practical productization due to its high stability with more integration process achieved. Future work should still focus on the growth of high-quality thin films, the free control of carriers, and the design of optimized integrated structures. Although emerging nanostructured devices have unique advantages in terms of VUV detection performance, their stability and integration technology still wait for a breakthrough. In addition, the development of new UWB semiconductor materials (in different dimensions) also brings more possibilities for VUV photodetectors.
The general characteristics of these photodetectors and the EQE of some representative results have been summarized in Fig. 10. For different applications’ needs, a reasonable trade-off between high quantum efficiency and high frequency response is necessary. For example, in space exploration, it is usually required to minimize the power consumption and response time because the former one is often the most direct and effective way to reduce equipment costs. Meanwhile, in order to monitor solar activity in real time, ultra-fast response time is also indispensable. Therefore, heterojunction photovoltaic detectors with ultra-fast response speed are the best choice in this field.
In the future, researchers should devote their work to the development of imaging technology of flat panel detectors. It has long been expected by scientists to take pictures of ultra-fast dynamic processes in celestial activities, such as recording the early evolution of the original orbit and detecting the chemical composition of coronal jets in solar storms. Especially, achieving single photon detection is also the ultimate goal of VUV photodetectors. At present, only few studies have reported the avalanche detectors based on UWB semiconductors, and the research on single-photon detection performance is still blank. Accordingly, the development of related technologies for detection performance evaluation also needs to be further promoted. The characteristics currently exhibited by UWB semiconductor-based VUV photodetectors shed light on their huge application potential in the frontier field, and related research still has a long way to go.
Availability of data and materials
Data sharing is not applicable to this article as no new data were created or analysed in this study.
Large Yield Radiometer
External quantum efficiency
Chemical vapor deposition
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This work is supported by the National Natural Science Foundation of China (NSFC) (61427901, 61604178, 91333207, U1505252).
The authors declare that they have no competing interests.
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Jia, L., Zheng, W. & Huang, F. Vacuum-ultraviolet photodetectors. PhotoniX 1, 22 (2020). https://doi.org/10.1186/s43074-020-00022-w
- Vacuum-ultraviolet detection
- Ultra-wide bandgap semiconductors
- Selective response