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TES-Based Light Detectors for the CRESST Direct Dark Matter Search

dc.contributor.authorRothe, J.
dc.contributor.authorAngloher, G.
dc.contributor.authorBauer, P.
dc.contributor.authorBento, A.
dc.contributor.authorBucci, C.
dc.contributor.authorD’Addabbo, A.
dc.contributor.authorDefay, X.
dc.contributor.authorErb, A.
dc.contributor.authorFeilitzsch, F. v
dc.contributor.authorFerreiro Iachellini, N.
dc.contributor.authorGorla, P.
dc.contributor.authorGütlein, A.
dc.contributor.authorHauff, D.
dc.contributor.authorJochum, J.
dc.contributor.authorKiefer, M.
dc.contributor.authorKluck, H.
dc.contributor.authorKraus, H.
dc.contributor.authorLanfranchi, J.-C.
dc.contributor.authorLangenkämper, A.
dc.contributor.authorLoebell, J.
dc.contributor.authorMancuso, M.
dc.contributor.authorMondragon, E.
dc.contributor.authorMünster, A.
dc.contributor.authorPagliarone, C.
dc.contributor.authorPetricca, F.
dc.contributor.authorPotzel, W.
dc.contributor.authorPröbst, F.
dc.contributor.authorPuig, R.
dc.contributor.authorReindl, F.
dc.contributor.authorSchäffner, K.
dc.contributor.authorSchieck, J.
dc.contributor.authorSchipperges, V.
dc.contributor.authorSchönert, S.
dc.contributor.authorSeidel, W.
dc.contributor.authorStahlberg, M.
dc.contributor.authorStodolsky, L.
dc.contributor.authorStrandhagen, C.
dc.contributor.authorStrauss, R.
dc.contributor.authorTanzke, A.
dc.contributor.authorTrinh Thi, H. H
dc.contributor.authorTürkoğlu, C.
dc.contributor.authorUlrich, A.
dc.contributor.authorUsherov, I.
dc.contributor.authorWawoczny, S.
dc.contributor.authorWillers, M.
dc.contributor.authorWüstrich, M.
dc.contributor.authorCanonica, Lucia
dc.date.accessioned2018-06-21T18:19:35Z
dc.date.available2018-06-21T18:19:35Z
dc.date.issued2018-05
dc.date.submitted2017-11
dc.identifier.issn0022-2291
dc.identifier.issn1573-7357
dc.identifier.urihttp://hdl.handle.net/1721.1/116506
dc.description.abstractThe CRESST experiment uses cryogenic detectors based on transition-edge sensors to search for dark matter interactions. Each detector module consists of a scintillating CaWO₄ crystal and a silicon-on-sapphire (SOS) light detector which operate in coincidence (phonon-light technique). The 40-mm-diameter SOS disks (2 g mass) used in the data taking campaign of CRESST-II Phase 2 (2014–2016) reached absolute baseline resolutions of σ = 4–7 eV. This is the best performance reported for cryogenic light detectors of this size. Newly developed silicon beaker light detectors (4 cm height, 4 cm diameter, 6 g mass), which cover a large fraction of the target crystal surface, have achieved a baseline resolution of σ = 5.8 eV. First results of further improved light detectors developed for the ongoing low-threshold CRESST-III experiment are presented. Keywords: Transition-edge sensor; Cryogenic light detector; Direct dark matter searchen_US
dc.publisherSpringer-Verlagen_US
dc.relation.isversionofhttps://doi.org/10.1007/s10909-018-1944-xen_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringer USen_US
dc.titleTES-Based Light Detectors for the CRESST Direct Dark Matter Searchen_US
dc.typeArticleen_US
dc.identifier.citationRothe, J. et al. “TES-Based Light Detectors for the CRESST Direct Dark Matter Search.” Journal of Low Temperature Physics (May 2018): 1-7 © 2018 The Author(s)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.mitauthorCanonica, Lucia
dc.relation.journalJournal of Low Temperature Physicsen_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.updated2018-05-11T04:01:30Z
dc.language.rfc3066en
dc.rights.holderThe Author(s)
dspace.orderedauthorsRothe, J.; Angloher, G.; Bauer, P.; Bento, A.; Bucci, C.; Canonica, L.; D’Addabbo, A.; Defay, X.; Erb, A.; Feilitzsch, F. v.; Ferreiro Iachellini, N.; Gorla, P.; Gütlein, A.; Hauff, D.; Jochum, J.; Kiefer, M.; Kluck, H.; Kraus, H.; Lanfranchi, J.-C.; Langenkämper, A.; Loebell, J.; Mancuso, M.; Mondragon, E.; Münster, A.; Pagliarone, C.; Petricca, F.; Potzel, W.; Pröbst, F.; Puig, R.; Reindl, F.; Schäffner, K.; Schieck, J.; Schipperges, V.; Schönert, S.; Seidel, W.; Stahlberg, M.; Stodolsky, L.; Strandhagen, C.; Strauss, R.; Tanzke, A.; Trinh Thi, H. H.; Türkoğlu, C.; Ulrich, A.; Usherov, I.; Wawoczny, S.; Willers, M.; Wüstrich, M.en_US
dspace.embargo.termsNen_US
mit.licensePUBLISHER_CCen_US


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