Large-area Si(Li) detectors for X-ray spectrometry and particle tracking in the GAPS experiment

F. Rogers, M. Xiao, K. M. Perez, S. Boggs, T. Erjavec, L. Fabris, H. Fuke, C. J. Hailey, M. Kozai, A. Lowell, N. Madden, M. Manghisoni, S. McBride, V. Re, E. Riceputi, N. Saffold, Y. Shimizu

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22 Scopus citations

Abstract

The first lithium-drifted silicon (Si(Li)) detectors to satisfy the unique geometric, performance, and cost requirements of the General Antiparticle Spectrometer (GAPS) experiment have been produced by Shimadzu Corporation. The GAPS Si(Li) detectors will form the first large-area, relatively high-temperature Si(Li) detector system with sensitivity to X-rays to operate at high altitude. These 10 cm-diameter, 2.5 mm-thick, 4- or 8-strip detectors provide the active area, X-ray absorption efficiency, energy resolution, and particle tracking capability necessary for the GAPS exotic-atom particle identification technique. In this paper, the detector performance is validated on the bases of X-ray energy resolution and reconstruction of cosmic minimum ionizing particle (MIP) signals. We use the established noise model for semiconductor detectors to distinguish sources of noise due to the detector from those due to signal processing electronics. We demonstrate that detectors with either 4 strips or 8 strips can provide the required ≤4 keV (FWHM) X-ray energy resolution at flight temperatures of -35 to -45°C, given the proper choice of signal processing electronics. Approximately 1000 8-strip detectors will be used for the first GAPS Antarctic balloon flight, scheduled for late 2021.

Original languageEnglish
Article numberP10009
JournalJournal of Instrumentation
Volume14
Issue number10
DOIs
StatePublished - Oct 2019

Funding

We thank SUMCO Corporation and Shimadzu Corporation for their cooperation in detector development. We also thank the GAPS collaboration for their consultation and support. K. Perez receives support from the Heising-Simons Foundation and the Alfred P. Sloan Foundation. F. Rogers is supported through the National Science Foundation Graduate Research Fellowship under Grant No. 1122374. M. Kozai is supported by the JSPS KAKENHI under Grant No. JP17K14313. H. Fuke is supported by the JSPS KAKENHI under Grant Nos. JP2670715 and JP17H01136. M. Manghisoni, V. Re, and E. Riceputi are supported by the Agenzia Spaziale Italiana (ASI). This work was partially supported by the NASA APRA program through Grant Nos. NNX17AB44G and NNX17AB46G.

FundersFunder number
SUMCO Corporation
Shimadzu Corporation
National Science Foundation
Directorate for Education and Human Resources1122374
National Aeronautics and Space AdministrationNNX17AB46G, NNX17AB44G
Alfred P. Sloan Foundation
Heising-Simons Foundation
Japan Society for the Promotion of ScienceJP17H01136, JP17K14313, JP2670715
Agenzia Spaziale Italiana

    Keywords

    • Balloon instrumentation
    • Dark Matter detectors (WIMPs, axions, etc.)
    • Particle tracking detectors (Solid-state detectors)
    • X-ray detectors

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