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The Enriched Xenon Observatory
Conference proceeding   Peer reviewed

The Enriched Xenon Observatory

M. J. Dolinski and EXO Collaboration
INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS, v 1182(1), pp 92-95
01 Jan 2009

Abstract

Physical Sciences Physics Physics, Nuclear Physics, Particles & Fields Science & Technology
The Enriched Xenon Observatory (EXO) experiment will search for neutrinoless double beta decay of Xe-136. The EXO Collaboration is actively pursuing both liquid-phase and gas-phase Xe detector technologies with scalability to the ton-scale. The search for neutrinoless double beta decay of Xe-136 is especially attractive because of the possibility of tagging the resulting Ba daughter ion, eliminating all sources of background other than the two neutrino decay mode. EXO-200, the first phase of the project, is a liquid Xe time projection chamber with 200 kg of Xe enriched to 80% in Xe-136. EXO-200, which does not include Ba-tagging, will begin taking data in 2009, with two-year sensitivity to the half-life for neutrinoless double beta decay of 6.4 x 10(25) years. This corresponds to an effective Majorana neutrino mass of 0.13 to 0.19 eV.

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