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Event Reconstruction in a Liquid Xenon Time Projection Chamber with an Optically-Open Field Cage

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arxiv 2009.10231 v2 pith:ORUAAXAA submitted 2020-09-22 physics.ins-det

T. Stiegler , S. Sangiorgio , J.P. Brodsky , M. Heffner , S. Al Kharusi , G. Anton , I.J. Arnquist , I. Badhrees
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P.S. Barbeau D. Beck V. Belov T. Bhatta A. Bolotnikov P.A. Breur E. Brown T. Brunner E. Caden G.F. Cao L. Cao C. Chambers B. Chana S.A. Charlebois M. Chiu B. Cleveland M. Coon A. Craycraft J. Dalmasson T. Daniels L. Darroch A. De St. Croix A. Der Mesrobian-Kabakian K. Deslandes R. DeVoe M.L. Di Vacri J. Dilling Y.Y. Ding M.J. Dolinski A. Dragone J. Echevers F. Edaltafar M. Elbeltagi L. Fabris D. Fairbank W. Fairbank J. Farine S. Ferrara S. Feyzbakhsh G. Gallina P. Gautam G. Giacomini D. Goeldi R. Gornea G. Gratta E.V. Hansen E.W. Hoppe J. Hö{ss}l A. House M. Hughes A. Iverson A. Jamil M.J. Jewell X.S. Jiang A. Karelin L.J. Kaufman T. Koffas R. Krücken A. Kuchenkov K.S. Kumar Y. Lan A. Larson K.G. Leach B.G. Lenardo D.S. Leonard G. Li S. Li Z. Li C. Licciardi P. Lv R. MacLellan N. Massacret T. McElroy M. Medina-Peregrina T. Michel B. Mong D.C. Moore K. Murray P. Nakarmi C.R. Natzke R.J. Newby K. Ni Z. Ning O. Njoya F. Nolet O. Nusair K. Odgers A. Odian M. Oriunno J.L. Orrell G.S. Ortega I. Ostrovskiy C.T. Overman S. Parent A. Piepke A. Pocar J.-F. Pratte V. Radeka E. Raguzin S. Rescia F. Retière M. Richman A. Robinson T. Rossignol P.C. Rowson N. Roy R. Saldanha K. Skarpaas VIII A.K. Soma G. St-Hilaire V. Stekhanov X.L. Sun M. Tarka S. Thibado A. Tidball J. Todd T.I. Totev R. Tsang T. Tsang F. Vachon V. Veeraraghavan S. Viel G. Visser C. Vivo-Vilches J.-L. Vuilleumier M. Wagenpfeil T. Wager M. Walent Q. Wang W. Wei L.J. Wen U. Wichoski M. Worcester S.X. Wu W.H. Wu X. Wu Q. Xia H. Yang L. Yang O. Zeldovich J. Zhao Y. Zhou T. Ziegler (nEXO Collaboration)
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classification physics.ins-det
keywords skinbackgroundbetacagefieldchamberdecayionization
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abstract

nEXO is a proposed tonne-scale neutrinoless double beta decay ($0\nu\beta\beta$) experiment using liquid ${}^{136}Xe$ (LXe) in a Time Projection Chamber (TPC) to read out ionization and scintillation signals. Between the field cage and the LXe vessel, a layer of LXe ("skin" LXe) is present, where no ionization signal is collected. Only scintillation photons are detected, owing to the lack of optical barrier around the field cage. In this work, we show that the light originating in the skin LXe region can be used to improve background discrimination by 5% over previous published estimates. This improvement comes from two elements. First, a fraction of the $\gamma$-ray background is removed by identifying light from interactions with an energy deposition in the skin LXe. Second, background from ${}^{222}Rn$ dissolved in the skin LXe can be efficiently rejected by tagging the $\alpha$ decay in the ${}^{214}Bi-{}^{214}Po$ chain in the skin LXe.

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  1. Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter

    nucl-ex 2025-06 conditional novelty 6.0 of 10

    A new delayed-coincidence tag from 136Cs isomers could let the nEXO detector reject backgrounds down to 10^-9 and measure CNO solar neutrinos, the 7Be neutrino energy, and sub-MeV fermionic dark matter.

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