High detectivity ZnSe-based Schottky barrier photodetectors for blue and near-ultraviolet spectral range

2000 ◽  
Vol 36 (9) ◽  
pp. 826 ◽  
Author(s):  
F. Vigué ◽  
P. de Mierry ◽  
J.-P. Faurie ◽  
E. Monroy ◽  
F. Calle ◽  
...  
Sensors ◽  
2021 ◽  
Vol 21 (8) ◽  
pp. 2758
Author(s):  
Alberto Taffelli ◽  
Sandra Dirè ◽  
Alberto Quaranta ◽  
Lucio Pancheri

Photodetectors based on transition metal dichalcogenides (TMDs) have been widely reported in the literature and molybdenum disulfide (MoS2) has been the most extensively explored for photodetection applications. The properties of MoS2, such as direct band gap transition in low dimensional structures, strong light–matter interaction and good carrier mobility, combined with the possibility of fabricating thin MoS2 films, have attracted interest for this material in the field of optoelectronics. In this work, MoS2-based photodetectors are reviewed in terms of their main performance metrics, namely responsivity, detectivity, response time and dark current. Although neat MoS2-based detectors already show remarkable characteristics in the visible spectral range, MoS2 can be advantageously coupled with other materials to further improve the detector performance Nanoparticles (NPs) and quantum dots (QDs) have been exploited in combination with MoS2 to boost the response of the devices in the near ultraviolet (NUV) and infrared (IR) spectral range. Moreover, heterostructures with different materials (e.g., other TMDs, Graphene) can speed up the response of the photodetectors through the creation of built-in electric fields and the faster transport of charge carriers. Finally, in order to enhance the stability of the devices, perovskites have been exploited both as passivation layers and as electron reservoirs.


1976 ◽  
Vol 31 ◽  
pp. 52-52
Author(s):  
A. Frey ◽  
W. Hofmann ◽  
D. Lemke ◽  
C. Thum

We report on new measurements extending the spectral range of our earlier photometry (Frey et al. 1974) to the near ultraviolet. The residual extinction caused by atmospheric ozone was found to be 0.m25 ± 0.m13 (2950 Å) and 0m36 ± 0m13 (2150 Å) at 41.5 km float altitude. Within the errors of 10-30% arising from calibration and the reduction procedure our measurements at 5000, 3450, and 2950 Å are compatible to a colour of the zodiacal light not different from that of the sun. Our result obtained at 2150 Å is an upper limit, since no reduction of airglow and integrated starlight has been done yet at that wavelength. This upper limit is 30% above a solar-like spectrum. This result is not in contradiction to the 0A0-2 measurements (Lillie 1972). The strong intensity increase he found occurs at wavelengths below 2150 Å.


1968 ◽  
Vol 23 (2) ◽  
pp. 311-314 ◽  
Author(s):  
R. W. Amberger ◽  
A. Flammersfeld

A new method of determining the thickness of transparent platelets (5 —100 μ) was combined with OBREIMOW’S interferometric method of measuring refractive indices. The dispersion of the refractive indices of anthracene, tetracene, p-terphenyl, trans-stilbene, and plastic scintillator was determined in the visible and near ultraviolet spectral range.


2000 ◽  
Vol 76 (2) ◽  
pp. 242-244 ◽  
Author(s):  
F. Vigué ◽  
E. Tournié ◽  
J.-P. Faurie

2000 ◽  
Vol 180 (1) ◽  
pp. 301-305 ◽  
Author(s):  
F. Vigu� ◽  
A. Bouill� ◽  
E. Tourni� ◽  
J.-P. Faurie

1996 ◽  
Vol 69 (24) ◽  
pp. 3662-3664 ◽  
Author(s):  
K. Solt ◽  
H. Melchior ◽  
U. Kroth ◽  
P. Kuschnerus ◽  
V. Persch ◽  
...  

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