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dc.contributor.authorArmatol, A.
dc.contributor.authorArmengaud, E.
dc.contributor.authorArmstrong, W.
dc.contributor.authorAugier, C.
dc.contributor.authorAvignone, F. T.
dc.contributor.authorAzzolini, O.
dc.contributor.authorBarabash, A.
dc.contributor.authorBari, G.
dc.contributor.authorBarresi, A.
dc.contributor.authorBaudin, D.
dc.contributor.authorBellini, F.
dc.contributor.authorBenato, G.
dc.contributor.authorBeretta, M.
dc.contributor.authorBergé, L.
dc.contributor.authorBiassoni, M.
dc.contributor.authorBillard, J.
dc.contributor.authorBoldrini, V.
dc.contributor.authorBranca, A.
dc.contributor.authorBrofferio, C.
dc.contributor.authorBucci, C.
dc.contributor.authorCamilleri, J.
dc.contributor.authorCapelli, S.
dc.contributor.authorCappelli, L.
dc.contributor.authorCardani, L.
dc.contributor.authorCarniti, P.
dc.contributor.authorCasali, N.
dc.contributor.authorCazes, A.
dc.contributor.authorCeli, E.
dc.contributor.authorChang, C.
dc.contributor.authorChapellier, M.
dc.contributor.authorCharrier, A.
dc.contributor.authorChiesa, D.
dc.contributor.authorClemenza, M.
dc.contributor.authorColantoni, I.
dc.contributor.authorCollamati, F.
dc.contributor.authorCopello, S.
dc.contributor.authorCremonesi, O.
dc.contributor.authorJ. Creswick, R.
dc.contributor.authorCruciani, A.
dc.contributor.authorD’Addabbo, A.
dc.contributor.authorD’Imperio, G.
dc.contributor.authorDafinei, I.
dc.contributor.authorA. Danevich, F.
dc.contributor.authorde Combarieu, M.
dc.contributor.authorDe Jesus, M.
dc.contributor.authorde Marcillac, P.
dc.contributor.authorDell’Oro, S.
dc.contributor.authorDi Domizio, S.
dc.contributor.authorDompè, V.
dc.contributor.authorDrobizhev, A.
dc.contributor.authorDumoulin, L.
dc.contributor.authorFantini, G.
dc.contributor.authorFaverzani, M.
dc.contributor.authorFerri, E.
dc.contributor.authorFerri, F.
dc.contributor.authorFerroni, F.
dc.contributor.authorFigueroa-Feliciano, E.
dc.contributor.authorFormaggio, J.
dc.contributor.authorFranceschi, A.
dc.contributor.authorFu, C.
dc.contributor.authorFu, S.
dc.contributor.authorFujikawa, B. K.
dc.contributor.authorGascon, J.
dc.contributor.authorGiachero, A.
dc.contributor.authorGironi, L.
dc.contributor.authorGiuliani, A.
dc.contributor.authorGorla, P.
dc.contributor.authorGotti, C.
dc.contributor.authorGras, P.
dc.contributor.authorGros, M.
dc.contributor.authorGutierrez, T. D.
dc.contributor.authorHan, K.
dc.contributor.authorHansen, E. V.
dc.contributor.authorHeeger, K. M.
dc.contributor.authorHelis, D. L.
dc.contributor.authorHuang, H. Z.
dc.contributor.authorHuang, R. G.
dc.contributor.authorImbert, L.
dc.contributor.authorJohnston, J.
dc.contributor.authorJuillard, A.
dc.contributor.authorKarapetrov, G.
dc.contributor.authorKeppel, G.
dc.contributor.authorKhalife, H.
dc.contributor.authorKobychev, V. V.
dc.contributor.authorKolomensky, Yu. G.
dc.contributor.authorKonovalov, S.
dc.contributor.authorLiu, Y.
dc.contributor.authorLoaiza, P.
dc.contributor.authorMa, L.
dc.contributor.authorMadhukuttan, M.
dc.contributor.authorMancarella, F.
dc.contributor.authorMariam, R.
dc.contributor.authorMarini, L.
dc.contributor.authorMarnieros, S.
dc.contributor.authorMartinez, M.
dc.contributor.authorMaruyama, R. H.
dc.contributor.authorMauri, B.
dc.contributor.authorMayer, D.
dc.contributor.authorMei, Y.
dc.contributor.authorMilana, S.
dc.contributor.authorMisiak, D.
dc.contributor.authorNapolitano, T.
dc.contributor.authorNastasi, M.
dc.contributor.authorNavick, X. F.
dc.contributor.authorNikkel, J.
dc.contributor.authorNipoti, R.
dc.contributor.authorNisi, S.
dc.contributor.authorNones, C.
dc.contributor.authorNorman, E. B.
dc.contributor.authorNovosad, V.
dc.contributor.authorNutini, I.
dc.contributor.authorO’Donnell, T.
dc.contributor.authorOlivieri, E.
dc.contributor.authorOriol, C.
dc.contributor.authorOuellet, J. L.
dc.contributor.authorPagan, S.
dc.contributor.authorPagliarone, C.
dc.contributor.authorPagnanini, L.
dc.contributor.authorPari, P.
dc.contributor.authorPattavina, L.
dc.contributor.authorPaul, B.
dc.contributor.authorPavan, M.
dc.contributor.authorPeng, H.
dc.contributor.authorPessina, G.
dc.contributor.authorPettinacci, V.
dc.contributor.authorPira, C.
dc.contributor.authorPirro, S.
dc.contributor.authorV. Poda, D.
dc.contributor.authorPolakovic, T.
dc.contributor.authorPolischuk, O. G.
dc.contributor.authorPozzi, S.
dc.contributor.authorPrevitali, E.
dc.contributor.authorPuiu, A.
dc.contributor.authorRessa, A.
dc.contributor.authorRizzoli, R.
dc.contributor.authorRosenfeld, C.
dc.contributor.authorRusconi, C.
dc.contributor.authorSanglard, V.
dc.contributor.authorScarpaci, J. A.
dc.contributor.authorSchmidt, B.
dc.contributor.authorSharma, V.
dc.contributor.authorShlegel, V.
dc.contributor.authorSingh, V.
dc.contributor.authorSisti, M.
dc.contributor.authorSpeller, D.
dc.contributor.authorSurukuchi, P. T.
dc.contributor.authorTaffarello, L.
dc.contributor.authorTellier, O.
dc.contributor.authorTomei, C.
dc.contributor.authorTretyak, V. I.
dc.contributor.authorTsymbaliuk, A.
dc.contributor.authorVelazquez, M.
dc.contributor.authorVetter, K. J.
dc.contributor.authorWagaarachchi, S. L.
dc.contributor.authorWang, G.
dc.contributor.authorWang, L.
dc.contributor.authorWelliver, B.
dc.contributor.authorWilson, J.
dc.contributor.authorWilson, K.
dc.contributor.authorWinslow, L. A.
dc.contributor.authorXue, M.
dc.contributor.authorYan, L.
dc.contributor.authorYang, J.
dc.contributor.authorYefremenko, V.
dc.contributor.authorYumatov, V.
dc.contributor.authorZarytskyy, M. M.
dc.contributor.authorZhang, J.
dc.contributor.authorZolotarova, A.
dc.contributor.authorZucchelli, S.
dc.date.accessioned2022-05-27T18:08:04Z
dc.date.available2021-09-20T17:41:31Z
dc.date.available2022-05-27T18:08:04Z
dc.date.issued2021-02
dc.date.submitted2020-12
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.urihttps://hdl.handle.net/1721.1/132026.2
dc.description.abstract<jats:title>Abstract</jats:title><jats:p>The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li<jats:inline-formula><jats:alternatives><jats:tex-math>$$_{2}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mrow /> <mml:mn>2</mml:mn> </mml:msub> </mml:math></jats:alternatives></jats:inline-formula><jats:inline-formula><jats:alternatives><jats:tex-math>$$^{100}$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>100</mml:mn> </mml:msup> </mml:math></jats:alternatives></jats:inline-formula>MoO<jats:inline-formula><jats:alternatives><jats:tex-math>$$_4$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mrow /> <mml:mn>4</mml:mn> </mml:msub> </mml:math></jats:alternatives></jats:inline-formula> crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of (<jats:inline-formula><jats:alternatives><jats:tex-math>$$6.7\pm 0.6$$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mn>6.7</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.6</mml:mn> </mml:mrow> </mml:math></jats:alternatives></jats:inline-formula>) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of <jats:inline-formula><jats:alternatives><jats:tex-math>$$\alpha $$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>α</mml:mi> </mml:math></jats:alternatives></jats:inline-formula> particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this <jats:inline-formula><jats:alternatives><jats:tex-math>$$\alpha $$</jats:tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>α</mml:mi> </mml:math></jats:alternatives></jats:inline-formula>-induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector.</jats:p>en_US
dc.publisherSpringer Science and Business Media LLCen_US
dc.relation.isversionofhttps://doi.org/10.1140/epjc/s10052-020-08809-8en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringer Berlin Heidelbergen_US
dc.titleCharacterization of cubic Li$$_{2}$$$$^{100}$$MoO$$_4$$ crystals for the CUPID experimenten_US
dc.typeArticleen_US
dc.identifier.citationThe European Physical Journal C. 2021 Feb 01;81(2):104en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.relation.journalEuropean Physical Journal Cen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2021-02-11T16:10:14Z
dc.language.rfc3066en
dc.rights.holderThe Author(s)
dspace.embargo.termsN
dspace.date.submission2021-02-11T16:10:14Z
mit.journal.volume81en_US
mit.journal.issue2en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work Neededen_US


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