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First underground results with NEWAGE-0.3a direction-sensitive dark matter detector
Authors:Kentaro Miuchi  Hironobu Nishimura  Kaori Hattori  Naoki Higashi  Chihiro Ida  Satoshi Iwaki  Shigeto Kabuki  Hidetoshi Kubo  Shunsuke Kurosawa  Kiseki Nakamura  Joseph Parker  Tatsuya Sawano  Michiaki Takahashi  Toru Tanimori  Kojiro Taniue  Kazuki Ueno  Hiroyuki Sekiya  Atsushi Takeda  Ken'ichi Tsuchiya  Atsushi Takada
Affiliation:1. Cosmic-Ray Group, Department of Physics, Graduate School of Science, Kyoto University Kitashirakawa-oiwakecho, Sakyo-ku, Kyoto, 606-8502, Japan;2. Kamioka Observatory, ICRR, The University of Tokyo Higashi-Mozumi, Kamioka cho, Hida 506-1205, Japan;3. National Research Institute of Police Science 6-3-1 Kashiwanoha, Kashiwa, Chiba, 277-0882, Japan;4. Scientific Balloon Laboratory, ISAS, JAXA Yoshinodai 3-1-1, Sagamihara, Kanagawa, 229-8510, Japan
Abstract:A direction-sensitive dark matter search experiment at Kamioka underground laboratory with the NEWAGE-0.3a detector was performed. The NEWAGE-0.3a detector is a gaseous micro-time-projection chamber filled with CF4 gas at 152 Torr. The fiducial volume and target mass are 20×25×31 cm320×25×31 cm3 and 0.0115 kg, respectively. With an exposure of 0.524 kg days, improved spin-dependent weakly interacting massive particle (WIMP)-proton cross section limits by a direction-sensitive method were achieved including a new record of 5400 pb for 150 GeV/c2/c2 WIMPs. We studied the remaining background and found that ambient γ-rays contributed about one-fifth of the remaining background and radioactive contaminants inside the gas chamber contributed the rest.
Keywords:Time projection chamber   Micro pattern detector   Dark matter   WIMP   Direction-sensitive
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