Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/108670
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dc.contributor.authorPetricca, F.-
dc.contributor.authorAngloher, G.-
dc.contributor.authorBento, A.-
dc.contributor.authorBucci, C.-
dc.contributor.authorCanonica, L.-
dc.contributor.authorDefay, X.-
dc.contributor.authorErb, A.-
dc.contributor.authorv Feilitzsch, F.-
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.authorLoebell, J.-
dc.contributor.authorMünster, A.-
dc.contributor.authorPagliarone, C.-
dc.contributor.authorPotzel, W.-
dc.contributor.authorPröbst, F.-
dc.contributor.authorReindl, F.-
dc.contributor.authorSchäffner, K.-
dc.contributor.authorSchieck, J.-
dc.contributor.authorSchönert, S.-
dc.contributor.authorSeidel, W.-
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.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.accessioned2023-09-07T11:14:37Z-
dc.date.available2023-09-07T11:14:37Z-
dc.date.issued2016-
dc.identifier.issn1742-6588pt
dc.identifier.issn1742-6596pt
dc.identifier.urihttps://hdl.handle.net/10316/108670-
dc.description.abstractThe CRESST-II experiment is searching for dark matter particles via their elastic scattering off nuclei in a target material. The CRESST target consists of scintillating CaWO4 crystals which are operated as cryogenic calorimeters at millikelvin temperatures and read out by transition edge sensors. Each interaction in the CaWO4 target crystal produces a phonon signal and also a light signal that is measured by a secondary cryogenic calorimeter. The low energy thresholds of these detectors, combined with the presence of light nuclei in the target material, allow to probe the low-mass region of the parameter space for spin-independent dark matter-nucleon scattering with high sensitivity. In this contribution results from a blind analysis of one detector module operated in the latest measurement campaign are presented. An unprecedented sensitivity for the light dark matter has been obtained with 52kg live days and a threshold of 307eV for nuclear recoils, extending the reach of direct dark matter searches to the sub-GeV/c2 region.pt
dc.language.isoengpt
dc.publisherInstitute of Physics Publishingpt
dc.relationWe are grateful to LNGS for their generous support of CRESST, in particular to Marco Guetti for his constant assistance. This work was supported by the DFG cluster of excellence: Origin and Structure of the Universe, by the Helmholtz Alliance for Astroparticle Physics, and by the BMBF: Project 05A11WOC EURECA-XENON.pt
dc.rightsopenAccesspt
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/pt
dc.titleNew results on low-mass dark matter from the CRESST-II experimentpt
dc.typearticle-
degois.publication.firstPage042044pt
degois.publication.issue4pt
degois.publication.titleJournal of Physics: Conference Seriespt
dc.peerreviewedyespt
dc.identifier.doi10.1088/1742-6596/718/4/042044pt
degois.publication.volume718pt
dc.date.embargo2016-01-01*
uc.date.periodoEmbargo0pt
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextopen-
item.openairetypearticle-
item.languageiso639-1en-
item.fulltextCom Texto completo-
item.cerifentitytypePublications-
crisitem.author.orcid0000-0002-3817-6015-
Appears in Collections:FCTUC Física - Artigos em Revistas Internacionais
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