2015
DOI: 10.1016/j.sse.2015.02.019
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Surface treatment to improve responsivity of MgZnO UV detectors

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Cited by 14 publications
(8 citation statements)
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“…The detector was compared with other detectors, and the relevant data is shown in Table 1. By comparison with the reference (Zhao et al, 2014), it can be seen that the responsivity of the detector in this paper is far greater than that of the MSM structure detector mentioned in the reference under the same bias voltage, the MSM detectors in some other articles (Wang et al, 2009;Zhao et al, 2015;Zhang W. et al, 2018), even if they work under a relatively high bias voltage, their responsivity is only comparable to the detectors in this article. It should be noted that the responsivity in the above-mentioned articles is the maximum value of its responsivity.…”
Section: Device Performance Measurements Resultsmentioning
confidence: 67%
“…The detector was compared with other detectors, and the relevant data is shown in Table 1. By comparison with the reference (Zhao et al, 2014), it can be seen that the responsivity of the detector in this paper is far greater than that of the MSM structure detector mentioned in the reference under the same bias voltage, the MSM detectors in some other articles (Wang et al, 2009;Zhao et al, 2015;Zhang W. et al, 2018), even if they work under a relatively high bias voltage, their responsivity is only comparable to the detectors in this article. It should be noted that the responsivity in the above-mentioned articles is the maximum value of its responsivity.…”
Section: Device Performance Measurements Resultsmentioning
confidence: 67%
“…Wide band gap semiconductor materials are considered to be suitable for solar-blind photodetectors, such as AlN, AlGaN, , ZnMgO, diamond, cubic BN, and Ga 2 O 3 . However, a complex buffer layer is needed to reduce the lattice mismatch between the AlGaN film and the substrate. , Although MgZnO has a wide tunable range band gap (3.3–7.8 eV) by adjusting the composition of Mg, the problem of phase segregation at high Mg concentration needs to be further solved. , The band gap of diamond is fixed at 5.5 eV, which limits its detection wavelength range shorter than 225 nm. , Significantly, Ga 2 O 3 with a natural band gap of ∼4.9 eV without the alloying process has the advantages of low cost and excellent chemical and physical stabilities, which make it suitable for solar-blind photodetection. ,, …”
Section: Introductionmentioning
confidence: 99%
“…Varma et al studied the performance of UV detectors based on ZnO thin‐film Schottky diodes with Au and Pd contacts by RF magnetron sputtering technique 20 . Zhao et al prepared MSM UV detectors based on MgZnO films, showing that the surface treatment of ZnO particles plays a key role in enhancing the responsivity of detector 21 . Xu et al reported ZnO thin film based on MSM UV detector with gold Schottky contact by hydrothermal method, indicating that the performance of the UV device depends on the structure of the ZnO materials 22 .…”
Section: Introductionmentioning
confidence: 99%