Sean N. Pike, Steven E. Boggs, Gabriel Brewster, Sophia E. Haight, Jarred M. Roberts, Albert Y. Shih, Joanna Szornel, John A. Tomsick, Andreas Zoglauer
{"title":"锗交叉带探测器中质子辐照产生空穴阱的特性研究。","authors":"Sean N. Pike, Steven E. Boggs, Gabriel Brewster, Sophia E. Haight, Jarred M. Roberts, Albert Y. Shih, Joanna Szornel, John A. Tomsick, Andreas Zoglauer","doi":"10.1007/s10686-025-09978-8","DOIUrl":null,"url":null,"abstract":"<div><p>We present an investigation into the effects of high-energy proton damage on charge trapping in germanium cross-strip detectors with the goal of accomplishing three important measurements. First, we calibrated and characterized the spectral resolution of a spare COSI-balloon detector in order to determine the effects of intrinsic trapping, finding that electron trapping due to impurities dominates over hole trapping in the undamaged detector. Second, we performed two rounds of proton irradiation of the detector in order to quantify, for the first time, the rate at which charge traps are produced by proton irradiation. We find that the product of the hole trap density and cross-sectional area, <span>\\([n\\sigma ]_\\textrm{h}\\)</span>, follows a linear relationship with the proton fluence, <span>\\(F_\\textrm{p}\\)</span>, with a slope of <span>\\((5.4\\pm 0.4)\\times 10^{-11}\\,\\mathrm {cm/p^{+}}\\)</span>. Third, by utilizing our measurements of physical trapping parameters, we performed calibrations which corrected for the effects of trapping and mitigated degradation to the spectral resolution of the detector.</p></div>","PeriodicalId":551,"journal":{"name":"Experimental Astronomy","volume":"59 1","pages":""},"PeriodicalIF":2.7000,"publicationDate":"2025-01-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11757935/pdf/","citationCount":"0","resultStr":"{\"title\":\"Characterizing hole trap production due to proton irradiation in germanium cross-strip detectors\",\"authors\":\"Sean N. Pike, Steven E. Boggs, Gabriel Brewster, Sophia E. Haight, Jarred M. Roberts, Albert Y. Shih, Joanna Szornel, John A. Tomsick, Andreas Zoglauer\",\"doi\":\"10.1007/s10686-025-09978-8\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>We present an investigation into the effects of high-energy proton damage on charge trapping in germanium cross-strip detectors with the goal of accomplishing three important measurements. First, we calibrated and characterized the spectral resolution of a spare COSI-balloon detector in order to determine the effects of intrinsic trapping, finding that electron trapping due to impurities dominates over hole trapping in the undamaged detector. Second, we performed two rounds of proton irradiation of the detector in order to quantify, for the first time, the rate at which charge traps are produced by proton irradiation. We find that the product of the hole trap density and cross-sectional area, <span>\\\\([n\\\\sigma ]_\\\\textrm{h}\\\\)</span>, follows a linear relationship with the proton fluence, <span>\\\\(F_\\\\textrm{p}\\\\)</span>, with a slope of <span>\\\\((5.4\\\\pm 0.4)\\\\times 10^{-11}\\\\,\\\\mathrm {cm/p^{+}}\\\\)</span>. Third, by utilizing our measurements of physical trapping parameters, we performed calibrations which corrected for the effects of trapping and mitigated degradation to the spectral resolution of the detector.</p></div>\",\"PeriodicalId\":551,\"journal\":{\"name\":\"Experimental Astronomy\",\"volume\":\"59 1\",\"pages\":\"\"},\"PeriodicalIF\":2.7000,\"publicationDate\":\"2025-01-24\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11757935/pdf/\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Experimental Astronomy\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s10686-025-09978-8\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Experimental Astronomy","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10686-025-09978-8","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
我们研究了高能质子损伤对锗交叉带探测器中电荷捕获的影响,目的是完成三个重要的测量。首先,我们对一个备用的cosi -气球探测器的光谱分辨率进行了校准和表征,以确定内在俘获的影响,发现由于杂质引起的电子俘获比未损坏的探测器中的空穴俘获更重要。其次,我们对探测器进行了两轮质子辐照,首次量化了质子辐照产生电荷阱的速率。我们发现,空穴阱密度与横截面积的乘积[n σ] h与质子通量F p呈线性关系,斜率为(5.4±0.4)× 10 - 11 cm / p +。第三,利用我们对物理捕获参数的测量,我们进行了校准,修正了捕获的影响,减轻了探测器光谱分辨率的下降。
Characterizing hole trap production due to proton irradiation in germanium cross-strip detectors
We present an investigation into the effects of high-energy proton damage on charge trapping in germanium cross-strip detectors with the goal of accomplishing three important measurements. First, we calibrated and characterized the spectral resolution of a spare COSI-balloon detector in order to determine the effects of intrinsic trapping, finding that electron trapping due to impurities dominates over hole trapping in the undamaged detector. Second, we performed two rounds of proton irradiation of the detector in order to quantify, for the first time, the rate at which charge traps are produced by proton irradiation. We find that the product of the hole trap density and cross-sectional area, \([n\sigma ]_\textrm{h}\), follows a linear relationship with the proton fluence, \(F_\textrm{p}\), with a slope of \((5.4\pm 0.4)\times 10^{-11}\,\mathrm {cm/p^{+}}\). Third, by utilizing our measurements of physical trapping parameters, we performed calibrations which corrected for the effects of trapping and mitigated degradation to the spectral resolution of the detector.
期刊介绍:
Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments.
Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields.
Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.