| タイトル | Demonstration of the First 4H-SiC EUV Detector with Large Detection Area |
| 本文（外部サイト） | http://hdl.handle.net/2060/20090022809 |
| 著者（英） | Zhao, Jian H.; Xin, Xiaobin; Hu, Jun; Yan, Feng; Koeth, Timothy W. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2005-09-18 |
| 言語 | eng |
| 内容記述 | Ultraviolet (UV) and Extreme Ultraviolet (EUV) detectors are very attractive in astronomy, photolithography and biochemical applications. For EUV applications, most of the semiconductor detectors based on PN or PIN structures suffer from the very short penetration depth. Most of the carries are absorbed at the surface and recombined there due to the high surface recombination before reach the depletion region, resulting very low quantum efficiency. On the other hand, for Schottky structures, the active region starts from the surface and carriers generated from the surface can be efficiently collected. 4H-Sic has a bandgap of 3.26eV and is immune to visible light background noise. Also, 4H-Sic detectors usually have very good radiation hardness and very low noise, which is very important for space applications where the signal is very weak. The E W photodiodes presented in this paper are based on Schottky structures. Platinum (Pt) and Nickel (Ni) are selected as the Schottky contact metals, which have the highest electron work functions (5.65eV and 5.15eV, respectively) among all the known metals on 4H-Sic. |
| NASA分類 | Space Radiation |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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