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arxiv: 1512.01076 · v1 · pith:YX37S5HJnew · submitted 2015-12-03 · 🌌 astro-ph.IM

The Methods for Direct Detection of WIMP with Mass <0.5 GeV

classification 🌌 astro-ph.IM
keywords detectionchamberdirectwimpargonliquidmassaddition
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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 .

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