Published August 17, 2015 | Version v1
Journal article

Surface purity control during XMASS detector refurbishment

  • 1. Kavl Institute for the Physics and Mathematics of the Universe (WPI), the University of Tokyo, Kashiwa, Chiba, 277-8582 (Japan)
  • 2. Kamioka observatory, Institute for Cosmic Ray Research, the University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205 (Japan)

Description

The XMASS project aims at detecting dark matter, pp and 7Be solar neutrinos, and neutrino less double beta decay using large volume of pure liquid xenon. The first physics target of the XMASS project is to detect dark matter with 835 kg liquid xenon. After the commissioning runs, XMASS detector was refurbished to minimize the background contribution mainly from PMT sealing material and we restarted data taking in November 2013. We report how we control surface purity, especially how we prevent radon daughter accumulation on the detector copper surface, during XMASS detector refurbishment. The result and future plan of XMASS are also reported

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1672
Journal Issue
1
Journal Page Range
p. 050003-050003.6
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
5. international workshop in low radioactivity techniques
Acronym
LRT 2015
Dates
18-20 Mar 2015
Place
Seattle, WA (United States)

Optional Information

Notes
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