Sensitivity of a tonne-scale NEXT detector for neutrinoless double-beta decay searches

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Adams, C.
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Álvarez Puerta, Vicente
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Arazi, L.
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Arnquist, I.J.
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Azevedo, C.D.R.
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Bailey, K.
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Ballester Merelo, Francisco José
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Benlloch Rodríguez, J.M.
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Borges, Filipa I.G.M.
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Byrnes, N.
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Cárcel García, Sara
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Carrión, J.V.
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Cebrián, Susana
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Church, E.
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Conde, Carlos A.N.
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Contreras, T.
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Denisenko, A.A.
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Díaz López, G.
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Díaz Medina, José
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Escada, J.
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Esteve, Raúl
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Felkai, R.
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Fernandes, L.M.P.
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Ferrario, Paola
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Ferreira, Antonio Luis
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Foss, F.
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Freitas, Elisabete D.C.
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Freixa, Zoraida
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Generowicz, J.
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Goldschmidt, Azriel
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Gómez Cadenas, Juan José
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González, R.
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González-Díaz, Diego
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Ghosh, S.
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Guenette, R.
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Gutiérrez, Rafael María
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Haefner, J.
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Hafidi, K.
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Hauptman, John M.
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Henriques, C.A.O.
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Hernando Morata, J.A.
orcId Herrero i Viñas, Pau​ ​ ​ ​
Herrero i Viñas, Pau
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Herrero, Vicente
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Ho, J.
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Ifergan, Y.
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Jones, Benjamin J.P.
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Kekic, M.
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Labarga, Luis A.
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Laing, Andrew
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Lebrun, P.
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López-March, N.
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Losada, Marta
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Mano, R.D.P.
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Martín-Albo Simón, Justo
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Martínez Pérez, Alberto
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Martínez-Vara, M.
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Martínez Lema, Gonzalo
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McDonald, Alison D.
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Meziani, Z.E.
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Monrabal Capilla, Francesc
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Monteiro, Cristina M.B.
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Mora, Francisco José
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Muñoz Vidal, J.
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Newhouse, C.
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Novella, P.
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Nygren, David R.
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Oblak, E.
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Palmeiro, B.
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Para, A.
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Pérez Pérez, Javier
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Querol, M.
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Redwine, A.B.
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Renner, Joshua
orcId Ripoll Masferrer, Lluís​ researcherId Ripoll Masferrer, Lluís​ scopusId Ripoll Masferrer, Lluís​ ​
Ripoll Masferrer, Lluís
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Rivilla, I.
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Rodríguez García, Y.
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Rodríguez Samaniego, Javier
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Rogero, C.
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Rogers, L.
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Romeo, B.
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Romo-Luque, C.
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Santos, Filomena P.
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dos Santos, Joaquim M.F.
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Simón Estévez, Ander
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Sorel, Michel
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Stanford, C.
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Teixeira, J.M.R.
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Thapa, P.
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Toledo, J.F.
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Torrent Collell, Jordi
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Usón, A.
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Veloso, João F.C.A.
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Vuong, T.T.
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Webb, R.C.
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Weiss-Babai, R.
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White, James T.
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Woodruff, K.
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Yahlali Haddou, Nadia
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The Neutrino Experiment with a Xenon TPC (NEXT) searches for the neutrinoless double-beta (0νββ) decay of 136Xe using high-pressure xenon gas TPCs with electroluminescent amplification. A scaled-up version of this technology with about 1 tonne of enriched xenon could reach in less than 5 years of operation a sensitivity to the half-life of 0νββ decay better than 1027 years, improving the current limits by at least one order of magnitude. This prediction is based on a well-understood background model dominated by radiogenic sources. The detector concept presented here represents a first step on a compelling path towards sensitivity to the parameter space defined by the inverted ordering of neutrino masses, and beyond ​
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