MISC

2016年

Dark matter search project PICO-LON

XIV INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP 2015), PTS 1-7
  • K. Fushimi
  • H. Ejiri
  • R. Hazama
  • H. Ikeda
  • K. Imagawa
  • K. Inoue
  • G. Kanzaki
  • A. Kozlov
  • R. Oritol
  • T. Shima
  • Y. Takemoto
  • Y. Teraoka
  • S. Umehara
  • K. Yasuda
  • S. Yoshida
  • 全て表示

718
記述言語
英語
掲載種別
機関テクニカルレポート,技術報告書,プレプリント等
DOI
10.1088/1742-6596/718/4/042022
出版者・発行元
IOP PUBLISHING LTD

The PICO-LON project aims at search for cold dark matter by means of highly radio-pure and large volume NaI(Tl) scintillator. The Nal powder was purified by chemical processing to remove lead isotopes and selecting a high purity graphite crucible. The concentrations of radioactive impurities of Ra-226 and Th-228 were effectively reduced to 58 +/- 4 mu Bq/kg and 1.5 +/- 1.9 beta Bq/kg, respectively. It should be remarked that the concentration of zio-, r D which is crucial for the sensitivity to dark matter, was reduced to 24 +/- 2 beta Bq/kg. The total background rate at 10 keV(ee) was as low as 8 keV(-1)kg(-1)day(-1), which was sufficiently low to search for dark matter. Further purification of NaI(Tl) ingot and future prospect of PICO-LON project is discussed.

リンク情報
DOI
https://doi.org/10.1088/1742-6596/718/4/042022
arXiv
http://arxiv.org/abs/arXiv:1512.04645
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000391490200048&DestApp=WOS_CPL
URL
http://arxiv.org/abs/1512.04645v1
ID情報
  • DOI : 10.1088/1742-6596/718/4/042022
  • ISSN : 1742-6588
  • arXiv ID : arXiv:1512.04645
  • Web of Science ID : WOS:000391490200048

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