Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/112001
DC FieldValueLanguage
dc.contributor.authorFernandes, L. M. P.-
dc.contributor.authorFreitas, E. D. C.-
dc.contributor.authorHenriques, C. A. O.-
dc.contributor.authorMano, R.D.P.-
dc.contributor.authorMonteiro, C. M. B.-
dc.contributor.authorSantos, J. M. F. dos-
dc.contributor.authorTeixeira, J. M. R.-
dc.contributor.authorBorges, F. I. G. M.-
dc.contributor.authorConde, C. A. N.-
dc.contributor.authorEscada, J.-
dc.contributor.authorMarques, A. P.-
dc.contributor.authorSantos, F. P.-
dc.contributor.authorNEXT Collaboration-
dc.date.accessioned2024-01-18T12:53:41Z-
dc.date.available2024-01-18T12:53:41Z-
dc.date.issued2023-05-16-
dc.identifier.issn1029-8479-
dc.identifier.urihttps://hdl.handle.net/10316/112001-
dc.description.abstractThe 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 Subterr\'aneo 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 neutrinoless 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$\pm$0.01 kg of $^{136}$Xe-enriched xenon, 90% C.L. lower limits to the neutrinoless double beta decay are found in the T$_{1/2}^{0\nu}>5.5\times10^{23}-1.3\times10^{24}$ 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.pt
dc.description.sponsorshipThe NEXT Collaboration acknowledges support from the following agencies and institutions: the European Research Council (ERC) under Grant Agreement No. 951281- BOLD; the European Union’s Framework Programme for Research and Innovation Horizon 2020 (2014–2020) under Grant Agreement No. 957202-HIDDEN; the MCIN/AEI of Spain and ERDF A way of making Europe under grants PID2021-125475NB and the Severo Ochoa Program grant CEX2018-000867-S; the Generalitat Valenciana of Spain under grants PROMETEO/2021/087 and CIDEGENT/2019/049; the Department of Education of the Basque Government of Spain under the predoctoral training program non-doctoral research personnel; the Spanish la Caixa Foundation (ID 100010434) under fellowship code LCF/BQ/PI22/11910019; the Portuguese FCT under project UID/FIS/04559/2020 to fund the activities of LIBPhys-UC; the Israel Science Foundation (ISF) under grant 1223/21; the Pazy Foundation (Israel) under grants 310/22, 315/19 and 465; the US Department of Energy under contracts number DE-AC02-06CH11357 (Argonne National Laboratory), DEAC02- 07CH11359 (Fermi National Accelerator Laboratory), DE-FG02-13ER42020 (Texas A&M), DE-SC0019054 (Texas Arlington) and DE-SC0019223 (Texas Arlington); the US National Science Foundation under award number NSF CHE 2004111; the Robert A Welch Foundation under award number Y-2031-20200401. Finally, we are grateful to the Laboratorio Subterráneo de Canfranc for hosting and supporting the NEXT experiment.pt
dc.language.isoporpt
dc.publisherSpringer Naturept
dc.rightsopenAccesspt
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/pt
dc.subjectDark Matter and Double Beta Decay (experiments)pt
dc.subjectRare Decaypt
dc.titleDemonstration of neutrinoless double beta decay searches in gaseous xenon with NEXTpt
dc.typearticlept
degois.publication.firstPage190pt
degois.publication.issue9pt
degois.publication.titleJournal of High Energy Physicspt
dc.peerreviewedyespt
dc.identifier.doi10.1007/JHEP09(2023)190-
degois.publication.volume2023pt
dc.date.embargo2023-05-16*
dc.identifier.urlhttp://arxiv.org/abs/2305.09435v4-
uc.date.periodoEmbargo0pt
item.grantfulltextopen-
item.cerifentitytypePublications-
item.languageiso639-1pt-
item.openairetypearticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextCom Texto completo-
crisitem.author.researchunitLIBPhys - Laboratory for Instrumentation, Biomedical Engineering and Radiation Physics-
crisitem.author.researchunitLIBPhys - Laboratory for Instrumentation, Biomedical Engineering and Radiation Physics-
crisitem.author.researchunitLIBPhys - Laboratory for Instrumentation, Biomedical Engineering and Radiation Physics-
crisitem.author.researchunitLIBPhys - Laboratory for Instrumentation, Biomedical Engineering and Radiation Physics-
crisitem.author.parentresearchunitUniversity of Coimbra-
crisitem.author.parentresearchunitUniversity of Coimbra-
crisitem.author.parentresearchunitUniversity of Coimbra-
crisitem.author.parentresearchunitUniversity of Coimbra-
crisitem.author.orcid0000-0001-8235-3229-
crisitem.author.orcid0000-0002-1912-2804-
crisitem.author.orcid0000-0002-8841-6523-
crisitem.author.orcid0000-0002-0214-4185-
Appears in Collections:LIP - Artigos em Revistas Internacionais
LIBPhys - Artigos em Revistas Internacionais
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