1999
DOI: 10.1088/0268-1242/14/7/201
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Semiconductor near-ultraviolet photoelectronics

Abstract: After a brief review of classification, application and sources of near-ultraviolet (UV) radiation the methods for fabricating UV photodetectors and characteristics of the photoconductive cells, p-n junction structure and Schottky barrier photodiodes are discussed. Characteristics of some light filters used in photodetectors and measuring devices are also reported. Now Si p-n structures are commonly used but Schottky diodes based on wide-gap (GaAsP, GaP, GaN, AlGaN, SiC) semiconductors are very attractive. The… Show more

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Cited by 121 publications
(66 citation statements)
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“…The ultra-fast , where τ dif , τ dr and τ c are carrier diffusion time from generated area to junction region, drift time in the junction region, and parasitic circuit time constant, respectively. 56 Due to atomic layer thickness and high mobility of graphene, the diffusion time in graphene τ dif (Gr) is estimated to be less than 1 ps. As the UV light penetration depth l is much less than the depletion region width W, τ dif (Si) in Si substrate for UV light can also be neglected according to τ dif = d 2 /(2D c ) and d~0, where d is the diffusion length and D c is the diffusion coefficient.…”
Section: Resultsmentioning
confidence: 99%
“…The ultra-fast , where τ dif , τ dr and τ c are carrier diffusion time from generated area to junction region, drift time in the junction region, and parasitic circuit time constant, respectively. 56 Due to atomic layer thickness and high mobility of graphene, the diffusion time in graphene τ dif (Gr) is estimated to be less than 1 ps. As the UV light penetration depth l is much less than the depletion region width W, τ dif (Si) in Si substrate for UV light can also be neglected according to τ dif = d 2 /(2D c ) and d~0, where d is the diffusion length and D c is the diffusion coefficient.…”
Section: Resultsmentioning
confidence: 99%
“…The Sun radiates over the entire ultraviolet (UV) spectrum, however, ozone in the Earth's atmosphere strongly absorbs wavelengths between 200 nm and 300 nm [1,2]. Solar-blind UV detectors are sensitive only to wavelengths in the UV-C region (200 nm to 280 nm) and therefore only respond to terrestrial sources radiating in this region [3].…”
Section: Introductionmentioning
confidence: 99%
“…UV research began in the latter half of the 19th century and the development of electro-optic systems for studying objects emitting in the UV region (10 nm to 400 nm) was stimulated after World War II, because of their military, industrial and scientific applications [1,2,4]. These systems and their components need to be robust, withstand UV radiation, and have good signalto-noise ratios (S/N).…”
Section: Introductionmentioning
confidence: 99%
“…These include absorption and emission spectrometers, flame detectors, surface defect detectors, satellite cameras, surveillance cameras and so on [1,2,3,4,5,6,7,8,9,10,11,12,13,14]. These instruments are used in a variety of scientific and engineering fields: chemical, life scientific and medical analyses, material science and semiconductor manufacturing, factory automation, environmental assessment and space vision [1,2,3,4,5,6,7,8,9,10,11,12,13,14]. Image sensors used in these fields are required to have high sensitivity through 200 to 1000 nm or selected waveband of these.…”
Section: Introductionmentioning
confidence: 99%