Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/102119
DC FieldValueLanguage
dc.contributor.authorWillers, M.-
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.authorFeilitzsch, F v-
dc.contributor.authorIachellini, N Ferreiro-
dc.contributor.authorGütlein, A.-
dc.contributor.authorGorla, P-
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.authorMancuso, M-
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.authorS. Schönert-
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.authorThi, H H Trinh-
dc.contributor.authorTürkoǧlu, C-
dc.contributor.authorUffinger, M-
dc.contributor.authorUlrich, A.-
dc.contributor.authorUsherov, I.-
dc.contributor.authorWawoczny, S.-
dc.contributor.authorWüstrich, M-
dc.contributor.authorZöller, A.-
dc.date.accessioned2022-09-26T11:26:27Z-
dc.date.available2022-09-26T11:26:27Z-
dc.date.issued2017-
dc.identifier.issn1742-6588pt
dc.identifier.issn1742-6596pt
dc.identifier.urihttps://hdl.handle.net/10316/102119-
dc.description.abstractThe CRESST-III experiment, located in the Gran Sasso underground laboratory (LNGS, Italy), aims at the direct detection of dark matter (DM) particles. Scintillating CaWO4 crystals operated as cryogenic detectors are used as target material for DM-nucleus scattering. The simultaneous measurement of the phonon signal from the CaWO4 crystal and of the emitted scintillation light in a separate cryogenic light detector is used to discriminate backgrounds from a possible dark matter signal. The experiment aims to significantly improve the sensitivity for low-mass ( 5-10 GeV/c2) DM particles by using optimized detector modules with a nuclear recoil-energy threshold 100 eV. The current status of the experiment as well as projections of the sensitivity for spin-independent DM-nucleon scattering will be presented.pt
dc.description.sponsorshipDFG cluster of excellence: Origin and Structure of the Universe, by the Maier-Leibnitz-Laboratorium Garching, by the Helmholtz Alliance for Astroparticle Physics, by the BMBF: Project 05A11WOC EURECA-XENON and by the Science and Technology Facilities Council (STFC) UK-
dc.language.isoengpt
dc.rightsopenAccesspt
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/pt
dc.titleDirect dark matter search with the CRESST-III experiment - status and perspectivespt
dc.typearticle-
degois.publication.firstPage012209pt
degois.publication.issue1pt
degois.publication.titleJournal of Physics: Conference Seriespt
dc.peerreviewedyespt
dc.identifier.doi10.1088/1742-6596/888/1/012209pt
degois.publication.volume888pt
dc.date.embargo2017-01-01*
uc.date.periodoEmbargo0pt
item.grantfulltextopen-
item.fulltextCom Texto completo-
item.openairetypearticle-
item.languageiso639-1en-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.orcid0000-0002-3817-6015-
Appears in Collections:FCTUC Física - Artigos em Revistas Internacionais
Files in This Item:
File Description SizeFormat
Direct-dark-matter-search-with-the-CRESSTIII-experiment--Status-and-perspectivesJournal-of-Physics-Conference-Series.pdf377.77 kBAdobe PDFView/Open
Show simple item record

SCOPUSTM   
Citations

3
checked on Nov 17, 2022

WEB OF SCIENCETM
Citations

2
checked on May 2, 2023

Page view(s)

35
checked on Apr 24, 2024

Download(s)

20
checked on Apr 24, 2024

Google ScholarTM

Check

Altmetric

Altmetric


This item is licensed under a Creative Commons License Creative Commons