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arXiv 2501.02412physics.ins-detastro-ph.IMnucl-ex
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COSI p型交叉条HPGe探测器的质子辐射损伤与退火

Proton Radiation Damage and Annealing of COSI p-type Cross-strip HPGe Detectors

Sophia E. Haight, Steven E. Boggs, Gabriel Brewster, Sean N. Pike, Jarred M. Roberts, Albert Y. Shih, Joanna M. Szornel, John A. Tomsick, Aravind B. Valluvan, Andreas Zoglauer

AI总结:

为了解空间辐射对交叉条锗探测器的影响,研究了高能质子损伤对COSI探测器的效应及高温退火的修复能力,通过150MeV质子辐照并经高温退火修复电荷陷阱,最终能谱分辨率达辐照前37%以内,为长期维护提供依据。

摘要:

为了解空间辐射环境对交叉条锗探测器的影响,我们研究了高能质子损伤对COSI探测器的效应以及高温退火修复探测器能谱分辨率的能力。我们用150 MeV质子辐照了一个COSI气球载交叉条高纯锗(HPGe)探测器,净注量为$4.95×10^8$ p$^+$/cm²,对应COSI空间辐射环境中约10年的剂量。我们通过一系列高温退火修复了由此导致的能谱分辨率退化,最终获得4.08 keV的半高宽(FWHM),为辐照前值(2.98 keV FWHM)的37%以内。我们通过高温退火时间表征了电荷陷阱的修复情况,为COSI能谱分辨率的长期维护提供退火程序依据。

英文摘要:

In order to understand the effects of a space radiation environment on cross-strip germanium detectors, we investigated the effects of high-energy proton damage on a COSI detector and the capabilities of high-temperature annealing in repairing detector spectral resolution. We irradiated a COSI-balloon cross-strip high-purity germanium (HPGe) detector with 150 MeV protons resulting in a net fluence of $4.95\times10^8$ p$^+$/cm$^2$ and corresponding to ~10 years in COSI's space radiation environment. We repaired the resulting degradation in spectral resolution through a series of high-temperature anneals to obtain a final FWHM of 4.08 keV, within 37% of its preradiation value (2.98 keV FWHM). We characterized the repair of charge traps with time spent under high-temperature anneal to inform an annealing procedure for long-term maintenance of COSI's spectral resolution.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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