138Ba(d,alpha) Study of States in 136Cs: Implications for New Physics Searches with Xenon Detectors

dc.contributor.authorRebeiro, B. M.
dc.contributor.authorTriambak, S.
dc.contributor.authorGarrett, P. E.
dc.contributor.authorBall, G. C.
dc.contributor.authorBrown, B. A.
dc.contributor.authorMenéndez Sánchez, Javier
dc.contributor.authorRomeo, B.
dc.contributor.authorAdsley, P.
dc.contributor.authorLenardo, B. G.
dc.contributor.authorLindsay, R.
dc.contributor.authorBildstein, V.
dc.contributor.authorBurbadge, C.
dc.contributor.authorColeman, R.
dc.contributor.authorDiaz Varela, A.
dc.contributor.authorDubey, R.
dc.contributor.authorFaestermann, T.
dc.contributor.authorHertenberger, R.
dc.contributor.authorKamil, M.
dc.contributor.authorLeach, K. G.
dc.contributor.authorNatzke, C.
dc.contributor.authorNzobadila Ondze, J. C.
dc.contributor.authorRadich, A.
dc.contributor.authorRand, E.
dc.contributor.authorWirth, H. -F.
dc.date.accessioned2024-11-04T15:22:48Z
dc.date.available2024-11-04T15:22:48Z
dc.date.issued2023-07-31
dc.date.updated2024-11-04T15:22:48Z
dc.description.abstractWe used the 138Ba⁢( , ) reaction to carry out an in-depth study of states in 136Cs, up to around 2.5 MeV. In this Letter, we place emphasis on hitherto unobserved states below the first 1+ level, which are important in the context of solar neutrino and fermionic dark matter (FDM) detection in large-scale xenon-based experiments. We identify for the first time candidate metastable states in 136Cs, which would allow a real-time detection of solar neutrino and FDM events in xenon detectors, with high background suppression. Our results are also compared with shell-model calculations performed with three Hamiltonians that were previously used to evaluate the nuclear matrix element (NME) for 136Xe neutrinoless double beta decay. We find that one of these Hamiltonians, which also systematically underestimates the NME compared with the others, dramatically fails to describe the observed low-energy 136Cs spectrum, while the other two show reasonably good agreement.
dc.format.extent1 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec746408
dc.identifier.issn0031-9007
dc.identifier.urihttps://hdl.handle.net/2445/216202
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1103/PhysRevLett.131.052501
dc.relation.ispartofPhysical Review Letters, 2023, vol. 131, p. 052501
dc.relation.urihttps://doi.org/10.1103/PhysRevLett.131.052501
dc.rights(c) American Physical Society, 2023
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationReaccions nuclears
dc.subject.classificationMatèria fosca (Astronomia)
dc.subject.classificationNeutrins solars
dc.subject.otherNuclear reactions
dc.subject.otherDark matter (Astronomy)
dc.subject.otherSolar neutrinos
dc.title138Ba(d,alpha) Study of States in 136Cs: Implications for New Physics Searches with Xenon Detectors
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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