XMASS detector
K. Abe, K. Hieda, K. Hiraide, S. Hirano, Y. Kishimoto, K. Kobayashi,, S. Moriyama, K. Nakagawa, M. Nakahata, H. Nishiie, H. Ogawa, N. Oka, H., Sekiya, A. Shinozaki, Y. Suzuki, A. Takeda, O. Takachio, K. Ueshima, D., Umemoto, M. Yamashita, B. S. Yang, S. Tasaka, J. Liu
TL;DR
The XMASS detector is a highly pure liquid xenon setup designed to detect dark matter, solar neutrinos, and neutrinoless double beta decay, with detailed descriptions of its configuration and calibration.
Contribution
This paper provides a comprehensive description of the XMASS detector's design, configuration, and calibration system for dark matter and neutrino detection.
Findings
Successful detector configuration and calibration
Enhanced sensitivity for dark matter detection
Detailed system overview for future research
Abstract
The XMASS project aims to detect dark matter, pp and Be solar neutrinos, and neutrinoless double beta decay using ultra pure liquid xenon. The first phase of the XMASS experiment searches for dark matter. In this paper, we describe the XMASS detector in detail, including its configuration, data acquisition equipment and calibration system.
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