Large-area Si(Li) detectors for X-ray spectrometry and particle tracking in the GAPS experiment
Creators
- 1. Department of Physics, Massachusetts Institute of Technology, 77 Massachusetts Ave, Cambridge, MA 02139 (United States)
- 2. Department of Physics, University of California at San Diego, 9500 Gilman Dr, La Jolla, CA 92093 (United States)
- 3. Oak Ridge National Laboratory, P.O. Box 2008, Oak Ridge, TN 37831 (United States)
- 4. Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210 (Japan)
- 5. Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027 (United States)
- 6. Center for Astrophysics and Space Sciences, University of California at San Diego, 9500 Gilman Dr, La Jolla, CA 92093 (United States)
- 7. Department of Engineering and Applied Sciences, University of Bergamo, Viale Marconi 5, Dalmine I-24044, Bergamo (Italy)
- 8. Space Sciences Laboratory, University of California at Berkeley, 7 Gauss Way, Berkeley, CA 94720 (United States)
- 9. Department of Physics, Faculty of Technology, Kanagawa University, 3-27-1 Rokkakubashi, Kanagawa-ku, Yokohama, Kanagawa 221-8686 (Japan)
Description
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 −45oC, 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.
Availability note (English)
Available from http://dx.doi.org/10.1088/1748-0221/14/10/P10009Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Instrumentation
- Journal Volume
- 14
- Journal Issue
- 10
- Journal Page Range
- p. P10009
- ISSN
- 1748-0221
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51058709
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- ABSORPTION; ANTIPARTICLES; ENERGY RESOLUTION; HADRONIC ATOMS; LI-DRIFTED SI DETECTORS; PARTICLE IDENTIFICATION; SENSITIVITY; SPECTROMETERS; X-RAY SPECTROSCOPY
- Descriptors DEC
- ANTIMATTER; ATOMS; ELEMENTARY PARTICLES; LI-DRIFTED DETECTORS; MATTER; MEASURING INSTRUMENTS; RADIATION DETECTORS; RESOLUTION; SEMICONDUCTOR DETECTORS; SI SEMICONDUCTOR DETECTORS; SORPTION; SPECTROSCOPY