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dc.contributor.authorCampani, Alice
dc.contributor.authorAdams, D. Q
dc.contributor.authorAlduino, C.
dc.contributor.authorAlfonso, K.
dc.contributor.authorAvignone, F. T
dc.contributor.authorAzzolini, O.
dc.contributor.authorBari, G.
dc.contributor.authorBellini, F.
dc.contributor.authorBenato, G.
dc.contributor.authorBiassoni, M.
dc.contributor.authorBranca, A.
dc.contributor.authorBrofferio, C.
dc.contributor.authorBucci, C.
dc.contributor.authorCaminata, A.
dc.contributor.authorCanonica, L.
dc.contributor.authorCao, X. G
dc.date.accessioned2021-09-20T17:17:28Z
dc.date.available2021-09-20T17:17:28Z
dc.date.issued2020-06-10
dc.identifier.urihttps://hdl.handle.net/1721.1/131528
dc.description.abstractAbstract CUORE is a tonne-scale cryogenic experiment located at the Laboratori Nazionali del Gran Sasso that exploits bolometric technique to search for neutrinoless double beta decay of $$^{130}{\hbox {Te}}$$ 130 Te . Thanks to its very low background and large mass, CUORE is also a powerful tool to study a broad class of phenomena, such as solar axions and WIMP scattering. The ability to conduct such sensitive searches crucially depends on the energy threshold, which has to be kept as low as possible. In this contribution, we show how the trigger algorithm affects the sensitivity to low-energy phenomena and the interpretation of the energy spectrum. In particular, we focus on the impact that the trigger algorithm has on the identification of the coincidence events among different crystals and, consequently, on the reconstruction of the background.en_US
dc.publisherSpringer USen_US
dc.relation.isversionofhttps://doi.org/10.1007/s10909-020-02487-2en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourceSpringer USen_US
dc.titleLowering the Energy Threshold of the CUORE Experiment: Benefits in the Surface Alpha Events Reconstructionen_US
dc.typeArticleen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2020-09-24T21:29:16Z
dc.language.rfc3066en
dc.rights.holderSpringer Science+Business Media, LLC, part of Springer Nature
dspace.embargo.termsY
dspace.date.submission2020-09-24T21:29:16Z
mit.licenseOPEN_ACCESS_POLICY
mit.metadata.statusAuthority Work and Publication Information Needed


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