The Methods for Direct Detection of WIMP with Mass <0.5 GeV
Instrumentation and Methods for Astrophysics
2015-12-04 v1
Abstract
The chamber for direct detection of WIMP with mass <0.5 Gev/c2 was developed. The chamber is filled with gas mixture Ne+10%H2 (0-1bar)+0,15ppm Ge(CH3)4. For events detection used GEM+pin-anodes , which provides the energy threshold about eV. The electron background is suppressed owing to photosensitive addition Ge(CH3)4 . It is proposed also for direct detection of WIMP the liquid argon chamber with H2 dissolved in liquid argon at a concentration 100ppm+0,015ppm Ge(CH3)4 .
Keywords
Cite
@article{arxiv.1512.01076,
title = {The Methods for Direct Detection of WIMP with Mass <0.5 GeV},
author = {B. M. Ovchinnikov and I. I. Tkachev and V. V. Parusov},
journal= {arXiv preprint arXiv:1512.01076},
year = {2015}
}
Comments
4 pages,3 figures