2001
DOI: 10.1016/s0022-0248(01)01467-1
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Al Ga1−N for solar-blind UV detectors

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Cited by 104 publications
(47 citation statements)
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“…6 Fig . 5 illustrates the plot of the responsivity versus dark current for the state-of-the-art solar blind (230-290 nm) UV detectors reported [4][5][6]8,[10][11]16,[30][31][32][33][34][35][36][37] for the devices based on Al x Ga 1-x N as well as on β-Ga 2 O 3 . The detectors reported in this work have excellent responsivity while maintaining a very low dark current for 230-240 nm range.…”
mentioning
confidence: 99%
“…6 Fig . 5 illustrates the plot of the responsivity versus dark current for the state-of-the-art solar blind (230-290 nm) UV detectors reported [4][5][6]8,[10][11]16,[30][31][32][33][34][35][36][37] for the devices based on Al x Ga 1-x N as well as on β-Ga 2 O 3 . The detectors reported in this work have excellent responsivity while maintaining a very low dark current for 230-240 nm range.…”
mentioning
confidence: 99%
“…The natural ambient light in this range is very low, therefore the noise level at the receiver is very low. 2 The deep-UV portion of the spectrum is also ideal for fluorescence of chemical compounds in bacteria. This fluorescence spectrum can then be used to identify the bacteria, and warn of the presence of dangerous bacteria.…”
Section: Introductionmentioning
confidence: 99%
“…In the past decade, there have been several reports on GaN-AlGaN based photodetectors, such as photoconductors [2], p-n junction [3], p-i-n [4] and p-p-n [5], Schottky barrier [6][7][8], metal-semiconductor-metal [9], metal-insulator-semiconductor [10], field-effect transistors, bipolar junction transistor [11] and avalanche photodiode [12]. Peak responsivities and corresponding quantum efficiencies scatter in a wide range depending on the device design and material qualities.…”
Section: Introductionmentioning
confidence: 99%