Proton radiation damage and annealing of COSI p-type cross-strip HPGe detectors

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 × 1 0 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.

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Publication Details

Journal
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment
Published
2025-04-29
DOI
https://doi.org/10.1016/j.nima.2025.170538
Citations
1
Primary Topic
Particle Detector Development and Performance
Type
article
Field-Weighted Citation Impact
1.87

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Proton radiation damage and annealing of COSI p-type cross-strip HPGe detectors

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Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment
Particle Detector Development and Performance
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article

Proton radiation damage and annealing of COSI p-type cross-strip HPGe detectors

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article en
1 citations

Abstract

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 × 1 0 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.

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated EquipmentVol. 1077
Goddard Space Flight Center (US), Lawrence Berkeley National Laboratory (US), University of California San Diego (US), University of California, Berkeley (US)
U.S. Department of Energy, National Aeronautics and Space Administration, Loma Linda University, Nuclear Safety and Security Commission, Goddard Space Flight Center, Laboratory Directed Research and Development, Astrophysics Science Division, Astrophysics Division, Lawrence Berkeley National Laboratory
Openalex Percentile: Top 14%
Particle Detector Development and Performance
1.87
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