Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/111801
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dc.contributor.authorAgostini, F.-
dc.contributor.authorMaouloud, S. E. M. Ahmed-
dc.contributor.authorAlthueser, L.-
dc.contributor.authorAmaro, F. D.-
dc.contributor.authorAntunovic, B.-
dc.contributor.authorAprile, E.-
dc.contributor.authorBaudis, L.-
dc.contributor.authorBaur, D.-
dc.contributor.authorBiondi, Y.-
dc.contributor.authorBismark, A.-
dc.contributor.authorBreur, P.A.-
dc.contributor.authorBrown, A-
dc.contributor.authorBruno, G.-
dc.contributor.authorBudnik, R.-
dc.contributor.authorCapelli, C.-
dc.contributor.authorCardoso, J.-
dc.contributor.authorCichon, D.-
dc.contributor.authorClark, M.-
dc.contributor.authorColijn, A P-
dc.contributor.authorCuenca-García, J. J.-
dc.contributor.authorCussonneau, J. P.-
dc.contributor.authorDecowski, M. P.-
dc.contributor.authorDepoian, A.-
dc.contributor.authorDierle, J.-
dc.contributor.authorGangi, P. Di-
dc.contributor.authorGiovanni, A. Di-
dc.contributor.authorDiglio, S.-
dc.contributor.authorSantos, J. M. F. dos-
dc.contributor.authorDrexlin, G.-
dc.contributor.authorEitel, K.-
dc.contributor.authorEngel, R.-
dc.contributor.authorFerella, A. D.-
dc.contributor.authorFischer, H.-
dc.contributor.authorGalloway, M.-
dc.contributor.authorGao, F.-
dc.contributor.authorGirard, F.-
dc.contributor.authorGlück, F.-
dc.contributor.authorGrandi, L.-
dc.contributor.authorGrößle, R.-
dc.contributor.authorGumbsheimer, R.-
dc.contributor.authorHansmann-Menzemer, S.-
dc.contributor.authorJörg, F.-
dc.contributor.authorKhundzakishvili, G.-
dc.contributor.authorKopec, A.-
dc.contributor.authorKuger, F.-
dc.contributor.authorKrauss, L.M.-
dc.contributor.authorLandsman, H.-
dc.contributor.authorLang, R. F.-
dc.contributor.authorLindemann, S.-
dc.contributor.authorLindner, M.-
dc.contributor.authorLopes, J. A. M.-
dc.contributor.authorVillalpando, A. Loya-
dc.contributor.authorMacolino, C.-
dc.contributor.authorManfredini, A.-
dc.contributor.authorUndagoitia, T. Marrodán-
dc.contributor.authorMasbou, J.-
dc.contributor.authorMasson, E.-
dc.contributor.authorMeinhardt, P.-
dc.contributor.authorMilutinovic, S.-
dc.contributor.authorMolinario, A.-
dc.contributor.authorMonteiro, C. M. B.-
dc.contributor.authorMurra, M.-
dc.contributor.authorOberlack, U. G.-
dc.contributor.authorPandurovic, M.-
dc.contributor.authorPeres, R.-
dc.contributor.authorPienaar, J.-
dc.contributor.authorPierre, M.-
dc.contributor.authorPizzella, V-
dc.contributor.authorQin, J.-
dc.contributor.authorGarcía, D. Ramírez-
dc.contributor.authorReichard, S.-
dc.contributor.authorRupp, N.-
dc.contributor.authorSanchez-Lucas, P.-
dc.contributor.authorSartorelli, G.-
dc.contributor.authorSchulte, D.-
dc.contributor.authorSchumann, M.-
dc.contributor.authorLavina, L. Scotto-
dc.contributor.authorSelvi, M.-
dc.contributor.authorSilva, M.-
dc.contributor.authorSimgen, H.-
dc.contributor.authorSteidl, M.-
dc.contributor.authorTerliuk, A.-
dc.contributor.authorTherreau, C.-
dc.contributor.authorThers, D.-
dc.contributor.authorThieme, K.-
dc.contributor.authorTrotta, R.-
dc.contributor.authorTunnell, C.D.-
dc.contributor.authorValerius, K.-
dc.contributor.authorVolta, G.-
dc.contributor.authorVorkapic, D.-
dc.contributor.authorWeinheimer, C.-
dc.contributor.authorWittweg, C.-
dc.contributor.authorWolf, J.-
dc.contributor.authorZopounidis, J. P.-
dc.contributor.authorZuber, K.-
dc.date.accessioned2024-01-10T12:54:28Z-
dc.date.available2024-01-10T12:54:28Z-
dc.date.issued2023-
dc.identifier.issn1434-6052-
dc.identifier.urihttps://hdl.handle.net/10316/111801-
dc.description.abstractWe correct an overestimation of the production rate of 137Xe in the DARWIN detector operated at LNGS. This formerly dominant intrinsic background source is now at a level similar to the irreducible background from solar 8B neutrinos, thus unproblematic at the LNGS depth. The projected half-life sensitivity for the neutrinoless double beta decay (0νββ) of 136Xe improves by 22% compared to the previously reported number and is now T 0ν 1/2 = 3.0 × 1027 yr (90% C.L.) after 10 years of DARWIN operation.pt
dc.language.isoengpt
dc.publisherSpringer Naturept
dc.relationSCOAP3pt
dc.rightsopenAccesspt
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/pt
dc.titleErratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$Xept
dc.typearticlept
degois.publication.firstPage996pt
degois.publication.issue11pt
degois.publication.titleEuropean Physical Journal Cpt
dc.peerreviewedyespt
dc.identifier.doi10.1140/epjc/s10052-023-12036-2-
degois.publication.volume83pt
dc.date.embargo2023-01-01*
uc.date.periodoEmbargo0pt
item.fulltextCom Texto completo-
item.grantfulltextopen-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairetypearticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
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.orcid0000-0001-7315-0550-
crisitem.author.orcid0000-0002-8841-6523-
crisitem.author.orcid0000-0002-1912-2804-
Appears in Collections:LIBPhys - Artigos em Revistas Internacionais
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