nEXO Pre-Conceptual Design Report
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 perfected in the course of a dedicated R&D program. Hence the risk which is inherent to the construction of a large, ultra-low background detector is reduced, as the intrinsic radioactive contamination requirements are generally not beyond those demonstrated with the present generation decay experiments. Indeed, most of the required materials have been already assayed or reasonable estimates of their properties are at hand. The details described herein represent the base design of the detector configuration as of early 2018. Where potential design improvements are possible, alternatives are discussed. This design for nEXO presents a compelling path towards a next generation search for , with a substantial possibility to discover physics beyond the Standard Model.
Cite
@article{arxiv.1805.11142,
title = {nEXO Pre-Conceptual Design Report},
author = {nEXO Collaboration and S. Al Kharusi and A. Alamre and J. B. Albert and M. Alfaris and G. Anton and I. J. Arnquist and I. Badhrees and P. S. Barbeau and D. Beck and V. Belov and T. Bhatta and F. Bourque and J. P. Brodsky and E. Brown and T. Brunner and A. Burenkov and G. F. Cao and L. Cao and W. R. Cen and C. Chambers and S. A. Charlebois and M. Chiu and B. Cleveland and R. Conley and M. Coon and M. Côté and A. Craycraft and W. Cree and J. Dalmasson and T. Daniels and D. Danovitch and L. Darroch and S. J. Daugherty and J. Daughhetee and R. DeVoe and S. Delaquis and A. Der Mesrobian-Kabakian and M. L. Di Vacri and J. Dilling and Y. Y. Ding and M. J. Dolinski and A. Dragone and J. Echevers and L. Fabris and D. Fairbank and W. Fairbank and J. Farine and S. Ferrara and S. Feyzbakhsh and P. Fierlinger and R. Fontaine and D. Fudenberg and G. Gallina and G. Giacomini and R. Gornea and G. Gratta and G. Haller and E. V. Hansen and D. Harris and J. Hasi and M. Heffner and E. W. Hoppe and J. Hößl and A. House and P. Hufschmidt and M. Hughes and Y. Ito and A. Iverson and A. Jamil and C. Jessiman and M. J. Jewell and X. S. Jiang and A. Karelin and L. J. Kaufman and C. Kenney and R. Killick and D. Kodroff and T. Koffas and S. Kravitz and R. Krücken and A. Kuchenkov and K. S. Kumar and Y. Lan and A. Larson and B. G. Lenardo and D. S. Leonard and C. M. Lewis and G. Li and S. Li and Z. Li and C. Licciardi and Y. H. Lin and P. Lv and R. MacLellan and K. McFarlane and T. Michel and B. Mong and D. C. Moore and K. Murray and R. J. Newby and T. Nguyen and Z. Ning and O. Njoya and F. Nolet and O. Nusair and K. Odgers and A. Odian and M. Oriunno and J. L. Orrell and G. S. Ortega and I. Ostrovskiy and C. T. Overman and S. Parent and M. Patel and A. Peña-Perez and A. Piepke and A. Pocar and J. -F. Pratte and D. Qiu and V. Radeka and E. Raguzin and T. Rao and S. Rescia and F. Retière and A. Robinson and T. Rossignol and P. C. Rowson and N. Roy and J. Runge and R. Saldanha and S. Sangiorgio and S. Schmidt and J. Schneider and A. Schubert and J. Segal and K. Skarpaas~VIII and A. K. Soma and K. Spitaels and G. St-Hilaire and V. Stekhanov and T. Stiegler and X. L. Sun and M. Tarka and J. Todd and T. Tolba and T. I. Totev and R. Tsang and T. Tsang and F. Vachon and B. Veenstra and V. Veeraraghavan and G. Visser and P. Vogel and J. -L. Vuilleumier and M. Wagenpfeil and Q. Wang and M. Ward and J. Watkins and M. Weber and W. Wei and L. J. Wen and U. Wichoski and G. Wrede and S. X. Wu and W. H. Wu and Q. Xia and L. Yang and Y. -R. Yen and O. Zeldovich and X. Zhang and J. Zhao and Y. Zhou and T. Ziegler},
journal= {arXiv preprint arXiv:1805.11142},
year = {2018}
}
Comments
182 pages, minor revisions