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Novella, P.; Sorel, M.; Usón, A.; Adams, C.; Almazán, H.; Álvarez, V.; Aranburu, A. I.; Arazi, L.; Arnquist, I. J.; Auria-Luna, F.; Ayet, S.; Azevedo, C. D. R.; Ballester, F.; Bayo, A.; Benlloch-Rodríguez, J. M.; Borges, F. I. G. M.; Bounasser, S.; Cárcel, S.; Carrión, J. V.; Cebrián, S.; Cid, L.; Conde, C. A. N.; Contreras, T.; Dey, E.; Dickel, T.; Elorza, M.; Escada, J.; Esteve, R.; Fahs, A.; Felkai, R.; Fernandes, L. M. P.; Ferrario, P.; Ferreira, A. L.; Foss, F. W.; Freitas, E. D. C.; Freixa, Z.; Generowicz, J.; Goldschmidt, A.; Gómez-Cadenas, J. J.; González, R.; Grocott, J.; Guenette, R.; Haefner, J.; Hafidi, K.; Hauptman, J.; Hernando Morata, J. A.; Herrero-Gómez, P.; Herrero, V.; Hervés Carrete, C.; Ho, J.; Ho, P.; Ifergan, Y.; Jones, B. J. P.; Labarga, L.; Larizgoitia, L.; Larumbe, A.; Lebrun, P.; Lopez, F.; Lopez Gutierrez, D.; López-March, N.; Martínez-Lema, G.; Martínez-Vara, M.; Meziani, Z. E.; Miller, R. L.; Mistry, K.; Molina-Canteras, J.; Monrabal, F.; Monteiro, C. M. B.; Mora, F. J.; Muñoz Vidal, J.; Navarro, K.; Nuñez, A.; Nygren, D. R.; Oblak, E.; Odriozola-Gimeno, M.; Palacio, J.; Palmeiro, B.; Para, A.; Parmaksiz, I.; Pelegrin, J.; Pérez Maneiro, M.; Querol, M.; Redwine, A. B.; Renner, J.; Rivilla, I.; Rogero, C.; Rogers, L.; Romeo, B.; Romo-Luque, C.; Santos, F. P.; dos Santos, J. M. F.; Simón, A.; Soleti, S. R.; Stanford, C.; Teixeira, J. M. R.; Toledo, J. F.; Torrent, J.; Vuong, T. T.; Waiton, J.; White, J. T.
The journal of high energy physics, 09/2023, Letnik: 2023, Številka: 9Journal Article
A bstract The NEXT experiment aims at the sensitive search of the neutrinoless double beta decay in 136 Xe, using high-pressure gas electroluminescent time projection chambers. The NEXT-White detector is the first radiopure demonstrator of this technology, operated in the Laboratorio Subterráneo de Canfranc. Achieving an energy resolution of 1% FWHM at 2.6 MeV and further background rejection by means of the topology of the reconstructed tracks, NEXT-White has been exploited beyond its original goals in order to perform a neu- trinoless double beta decay search. The analysis considers the combination of 271.6 days of 136 Xe-enriched data and 208.9 days of 136 Xe-depleted data. A detailed background modeling and measurement has been developed, ensuring the time stability of the radiogenic and cosmogenic contributions across both data samples. Limits to the neutrinoless mode are obtained in two alternative analyses: a background-model-dependent approach and a novel direct background-subtraction technique, offering results with small dependence on the background model assumptions. With a fiducial mass of only 3.50 ± 0.01 kg of 136 Xe-enriched xenon, 90% C.L. lower limits to the neutrinoless double beta decay are found in the T 1 / 2 0 ν > 5 . 5 × 10 23 − 1 . 3 × 10 24 yr range, depending on the method. The presented techniques stand as a proof-of-concept for the searches to be implemented with larger NEXT detectors.
