{"title":"Submillimeter detection with Hg1-xCdxTe","authors":"J. Giles, M. Kimmitt, G. C. Lopez, H. Röser","doi":"10.1109/irmm.1983.9126404","DOIUrl":null,"url":null,"abstract":"In recent papers [1] and [2] Weber and Kulpa have reported on the usefulness of the alloy semiconductor Hg1-xCdxTe as a long wavelength electron bolometer detector. Although our main interest is in the use of this semiconductor as a mixer for far infrared heterodyne experiments [3], we have inevitably also studied its wider response. Although this research is at a fairly early stage, and some of the results are not easy to interpret, our best detector has a good detectivity (NEP < 1 × 10−11 WHz−½ at 500 μm and < 5 × 10−12 WHz−½ at 900 μm), with a significantly faster response than n-InSb. Moreover, construction of the detector is very simple compared with n-InSb where considerable ingenuity is required to make high impedance, high voltage responsivity detectors without employing magnetic fields.","PeriodicalId":314918,"journal":{"name":"1983 Eighth International Conference on Infrared and Millimeter Waves","volume":"22 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1983-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"1983 Eighth International Conference on Infrared and Millimeter Waves","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/irmm.1983.9126404","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
In recent papers [1] and [2] Weber and Kulpa have reported on the usefulness of the alloy semiconductor Hg1-xCdxTe as a long wavelength electron bolometer detector. Although our main interest is in the use of this semiconductor as a mixer for far infrared heterodyne experiments [3], we have inevitably also studied its wider response. Although this research is at a fairly early stage, and some of the results are not easy to interpret, our best detector has a good detectivity (NEP < 1 × 10−11 WHz−½ at 500 μm and < 5 × 10−12 WHz−½ at 900 μm), with a significantly faster response than n-InSb. Moreover, construction of the detector is very simple compared with n-InSb where considerable ingenuity is required to make high impedance, high voltage responsivity detectors without employing magnetic fields.