2003
DOI: 10.1109/tns.2003.820749
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Proton-induced transients and charge collection measurements in a LWIR HgCdTe focal plane array

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Cited by 11 publications
(7 citation statements)
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“…A connection between and the level of displacement damage can be established by assuming a linear increase in the defect concentration with , which the data from these experiments supports. Recall that when dominated by Shockley-Read-Hall (SRH) recombination and assuming a single active recombination level, is related to according to (4) where is the minority carrier capture cross-section, is the carrier thermal velocity equal to , is Boltzmann's constant and is effective mass. [ …”
Section: A Degradation Rates and Damage Factorsmentioning
confidence: 99%
See 1 more Smart Citation
“…A connection between and the level of displacement damage can be established by assuming a linear increase in the defect concentration with , which the data from these experiments supports. Recall that when dominated by Shockley-Read-Hall (SRH) recombination and assuming a single active recombination level, is related to according to (4) where is the minority carrier capture cross-section, is the carrier thermal velocity equal to , is Boltzmann's constant and is effective mass. [ …”
Section: A Degradation Rates and Damage Factorsmentioning
confidence: 99%
“…Here, will be diffusion-limited, but is dominated by SRH-recombination, according to (4), and thus is still limited by . In the regime, which is expected for unipolar barrier detectors at lower , where is expected to be lowest, the diffusion-limited, dark current density is given by (7) where is the absorber thickness, is the intrinsic carrier concentration and is the doping concentration.…”
Section: B Dark Current Density Damage Factormentioning
confidence: 99%
“…The effective ionization potential for long-wavelength cutoff HgCdTe is ∼1.04 eV∕e − , corresponding to an efficiency of converting energy into electron-hole pairs of about 10% (the band gap energy is about 0.1 eV). 16 The total charge generated by high-energy protons is approximately 17 E Q -T A R G E T ; t e m p : i n t r a l i n k -; e 0 0 3 ; 6 3 ; 1 8 7 charge ≈ pathlength à ðdE∕dxÞ∕ionization energy per e − :…”
Section: Proton Stopping Powermentioning
confidence: 99%
“…For space applications, it is important to understand the effects of radiation on these devices. Radiation damage of HgCdTe photodiode arrays without avalanche gain have been studied extensively [21]- [28] and the results show they are much less susceptible to radiation damage than their silicon counterparts [29]- [31]. However, due to the relatively high electron multiplication gain, HgCdTe APDs are expected to be more susceptible to space radiation damage.…”
Section: Introductionmentioning
confidence: 99%