Development of Large-area Lithium-drifted Silicon Detectors for the GAPS Experiment
M. Kozai, H. Fuke, M. Yamada, T. Erjavec, C. J. Hailey, C. Kato, N., Madden, K. Munakata, K. Perez, F. Rogers, N. Saffold, Y. Shimizu, K. Tokuda, and M. Xiao

TL;DR
This paper reports the development of large-area lithium-drifted silicon detectors designed specifically for the GAPS experiment, aiming to detect cosmic-ray antinuclei with high energy resolution at relatively high temperatures.
Contribution
The paper introduces a novel fabrication process for large-area Si(Li) detectors with improved leakage current suppression suitable for balloon-borne cosmic-ray detection.
Findings
Achieved <4 keV energy resolution at -35 to -45°C
Developed a high-yield production process for 10-cm diameter detectors
Successfully suppressed leakage current with guard ring and surface etching
Abstract
We have developed large-area lithium-drifted silicon (Si(Li)) detectors to meet the unique requirements of the General Antiparticle Spectrometer (GAPS) experiment. GAPS is an Antarctic balloon-borne mission scheduled for the first flight in late 2020. The GAPS experiment aims to survey low-energy cosmic-ray antinuclei, particularly antideuterons, which are recognized as essentially background-free signals from dark matter annihilation or decay. The GAPS Si(Li) detector design is a thickness of 2.5 mm, diameter of 10 cm and 8 readout strips. The energy resolution of <4 keV (FWHM) for 20 to 100 keV X-rays at temperature of -35 to -45 C, far above the liquid nitrogen temperatures frequently used to achieve fine energy resolution, is required. We developed a high-quality Si crystal and Li-evaporation, diffusion and drift methods to form a uniform Li-drifted layer. Guard ring structure and…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle Detector Development and Performance · Neutrino Physics Research
