2016
DOI: 10.1007/s10909-016-1484-1
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Development of Blocked-Impurity-Band-Type Ge Detectors Fabricated with the Surface-Activated Wafer Bonding Method for Far-Infrared Astronomy

Abstract: We report the current status of the development of our new detectors for far-infrared (FIR) astronomy. We develop Blocked-Impurity-Band (BIB)-type Ge detectors to realize large-format compact arrays covering a wide FIR wavelength range up to 200 µm. We fabricated Ge junction devices of different physical parameters with a BIB-type structure, using the room temperature, surface-activated wafer bonding (SAB) method. We measured the absolute responsivity and the spectral response curve of each device at low tempe… Show more

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Cited by 22 publications
(10 citation statements)
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“…Moreover, the high rate of thermal carriers has made this material unsuitable for detection at f ≤ 10 THz [29]. Other material in photon detectors can be tailored based on the nature of the interaction, such as extrinsic detectors from the Ge semiconductor [30], [31], and quantum wells (QWs) detectors made of GaAs semiconductor [32], [33]. Photon detectors have a good signal−to−noise performance and a fast response in the IR and Far-IR regions.…”
Section: B Operation Principlesmentioning
confidence: 99%
“…Moreover, the high rate of thermal carriers has made this material unsuitable for detection at f ≤ 10 THz [29]. Other material in photon detectors can be tailored based on the nature of the interaction, such as extrinsic detectors from the Ge semiconductor [30], [31], and quantum wells (QWs) detectors made of GaAs semiconductor [32], [33]. Photon detectors have a good signal−to−noise performance and a fast response in the IR and Far-IR regions.…”
Section: B Operation Principlesmentioning
confidence: 99%
“…The noise equivalent power (NEP) is calculated by taking account of shot noise of the dark current and the responsivity. The details of fabrication and characterization of the device are described elsewhere [9][10][11][12].…”
Section: Development Of Ge Bib Detectormentioning
confidence: 99%
“…However, although the Ge-based impurity detector has been developed for many years, there is still a large gap compared with other terahertz detectors in terms of array scale, performance, and maturity [14,15], due to many fabrication difficulties and problems. For example, the typical pixel sizes of the reported Ge-based THz detectors are almost over 1 mm [16,17], which are too large to be arrayed on a large scale and lead to a complex refrigeration and optical system [18]. Therefore, the ground-based popularization and application of Ge-based THz detectors are limited and not even reported.…”
Section: Introductionmentioning
confidence: 99%