nEXO Pre-Conceptual Design Report
nEXO Collaboration: S. Al Kharusi, A. Alamre, J.B. Albert, M. Alfaris,, G. Anton, I.J. Arnquist, I. Badhrees, P.S. Barbeau, D. Beck, V. Belov, T., Bhatta, F. Bourque, J.P. Brodsky, E. Brown, T. Brunner, A. Burenkov, G.F., Cao, L. Cao, W.R. Cen, C. Chambers, S.A. Charlebois

TL;DR
The nEXO pre-conceptual design aims to build a large, low-background liquid xenon detector to significantly improve the sensitivity of neutrinoless double beta decay searches, potentially revealing new physics beyond the Standard Model.
Contribution
This report presents the initial design and projected performance of the nEXO detector, a next-generation experiment for neutrinoless double beta decay using enriched liquid xenon.
Findings
Projected half-life sensitivity of ~10^28 years
Active mass of about 5000 kg of enriched xenon
Background dominated by external radiation sources
Abstract
The projected performance and detector configuration of nEXO are described in this pre-Conceptual Design Report (pCDR). nEXO is a tonne-scale neutrinoless double beta () decay search in Xe, based on the ultra-low background liquid xenon technology validated by EXO-200. With 5000 kg of xenon enriched to 90% in the isotope 136, nEXO has a projected half-life sensitivity of approximately years. This represents an improvement in sensitivity of about two orders of magnitude with respect to current results. Based on the experience gained from EXO-200 and the effectiveness of xenon purification techniques, we expect the background to be dominated by external sources of radiation. The sensitivity increase is, therefore, entirely derived from the increase of active mass in a monolithic and homogeneous detector, along with some technical advances…
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Taxonomy
TopicsNeutrino Physics Research · Dark Matter and Cosmic Phenomena · Astrophysics and Cosmic Phenomena
