2017/10/31 by nEXO Collaboration, J. B. Albert, G. Anton +147 · 186 citations
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Detector #Double beta decay #Homogeneous #Neutrino Physics Research #Observatory #Projection (relational algebra) #Radioactive Decay and Measurement Techniques #Sensitivity (control systems) #nucl-ex #physics.ins-det
paper · pdf · doi:10.1103/physrevc.97.065503
published in Physical Review C 97(6) (American Institute of Physics) · v2 as published
openalex created_date 2016/06/24 · openalex publication_date 2018/06/15 · arxiv created 2018/10/19 · arxiv updated 2018/10/23 · openalex updated_date 2026/08/05
The next-generation Enriched Xenon Observatory (nEXO) is a proposed experiment to search for neutrinoless double-\ensuremathβ (0\ensuremathν\ensuremathβ\ensuremathβ) decay in 136Xe with a target half-life sensitivity of approximately 1028 yr using 5\ifmmode×\else\texttimes\fi103 kg of isotopically enriched liquid-xenon in a time projection chamber. This improvement of two orders of magnitude in sensitivity over current limits is obtained by a significant increase of the 136Xe mass, the monolithic and homogeneous configuration of the active medium, and the multiparameter measurements of the interactions enabled by the time projection chamber. The detector concept and anticipated performance are presented based upon demonstrated realizable background rates.