Utilize este identificador para referenciar este registo: https://hdl.handle.net/10316/109407
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dc.contributor.authorAngloher, G.-
dc.contributor.authorBento, A.-
dc.contributor.authorBucci, C.-
dc.contributor.authorCanonica, L.-
dc.contributor.authorErb, A.-
dc.contributor.authorvon Feilitzsch, F.-
dc.contributor.authorIachellini, N. Ferreiro-
dc.contributor.authorGorla, P.-
dc.contributor.authorGütlein, A.-
dc.contributor.authorHauff, D.-
dc.contributor.authorHuff, P.-
dc.contributor.authorJochum, J.-
dc.contributor.authorKiefer, M.-
dc.contributor.authorKister, C.-
dc.contributor.authorKluck, H.-
dc.contributor.authorKraus, H.-
dc.contributor.authorLanfranchi, J.-C.-
dc.contributor.authorLoebell, J.-
dc.contributor.authorMünster, A.-
dc.contributor.authorPetricca, F.-
dc.contributor.authorPotzel, W.-
dc.contributor.authorPröbst, F.-
dc.contributor.authorReindl, F.-
dc.contributor.authorRoth, S.-
dc.contributor.authorRottler, K.-
dc.contributor.authorSailer, C.-
dc.contributor.authorSchäffner, K.-
dc.contributor.authorSchieck, J.-
dc.contributor.authorSchmaler, J.-
dc.contributor.authorScholl, S.-
dc.contributor.authorSchönert, S.-
dc.contributor.authorSeidel, W.-
dc.contributor.authorvon Sivers, M.-
dc.contributor.authorStodolsky, L.-
dc.contributor.authorStrandhagen, C.-
dc.contributor.authorStrauß, R.-
dc.contributor.authorTanzke, A.-
dc.contributor.authorUffinger, M.-
dc.contributor.authorUlrich, A.-
dc.contributor.authorUsherov, I.-
dc.contributor.authorWawoczny, S.-
dc.contributor.authorWillers, M.-
dc.contributor.authorWüstrich, M.-
dc.contributor.authorZöller, A.-
dc.date.accessioned2023-10-13T08:22:36Z-
dc.date.available2023-10-13T08:22:36Z-
dc.date.issued2014-
dc.identifier.issn1434-6044pt
dc.identifier.issn1434-6052pt
dc.identifier.urihttps://hdl.handle.net/10316/109407-
dc.description.abstractThe CRESST-II cryogenic dark matter search aims for the detection of WIMPs via elastic scattering off nuclei in CaWO4 crystals. We present results from a lowthreshold analysis of a single upgraded detector module. This module efficiently vetoes low energy backgrounds induced by α-decays on inner surfaces of the detector. With an exposure of 29.35 kg live days collected in 2013 we set a limit on spin-independent WIMP-nucleon scattering which probes a new region of parameter space for WIMP masses below 3 GeV/c2, previously not covered in direct detection searches. A possible excess over background discussed for the previous CRESST-II phase 1 (from 2009 to 2011) is not confirmed.pt
dc.description.sponsorshipThis work was supported by funds of the German Federal Ministry of Science and Education (BMBF), the Munich Cluster of Excellence (Origin and Structure of the Universe), the Maier- Leibnitz-Laboratorium (Garching), the Science and Technology Facilities Council (STFC) UK, as well as theHelmholtz Alliance forAstroparticle Physics. We gratefully acknowledge the work of Michael Stanger from the crystal laboratory of the TU Munich.We are grateful to LNGS for their generous support of CRESST, in particular to Marco Guetti for his constant assistance.pt
dc.language.isoengpt
dc.publisherSpringer Naturept
dc.rightsopenAccesspt
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/pt
dc.titleResults on low mass WIMPs using an upgraded CRESST-II detectorpt
dc.typearticle-
degois.publication.issue12pt
degois.publication.titleEuropean Physical Journal Cpt
dc.peerreviewedyespt
dc.identifier.doi10.1140/epjc/s10052-014-3184-9pt
degois.publication.volume74pt
dc.date.embargo2014-01-01*
uc.date.periodoEmbargo0pt
item.fulltextCom Texto completo-
item.languageiso639-1en-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypearticle-
item.grantfulltextopen-
item.cerifentitytypePublications-
crisitem.author.orcid0000-0002-3817-6015-
Aparece nas coleções:FCTUC Física - Artigos em Revistas Internacionais
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