Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/102222
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dc.contributor.authorGütlein, A.-
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.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.authorWillers, M.-
dc.contributor.authorWüstrich, M.-
dc.contributor.authorZöller, A.-
dc.date.accessioned2022-09-28T09:28:00Z-
dc.date.available2022-09-28T09:28:00Z-
dc.date.issued2017-
dc.identifier.issn1742-6588pt
dc.identifier.issn1742-6596pt
dc.identifier.urihttps://hdl.handle.net/10316/102222-
dc.description.abstractUnderstanding the nature and origin of dark matter is one of the most important challenges for modern particle physics. During the previous decade the sensitivities of direct dark matter searches have improved by several orders of magnitude. These experiments focus their work mainly on the search for dark-matter particles interacting with nuclei (e.g. Weakly Interacting Massive Particles, WIMPs). However, there exists a large variety of different candidates for dark-matter particles. One of these candidates, the so-called dark photon, is a long-lived vector boson with a kinetic mixing to the standard-model photon. In this work we present the preliminary results of our search for dark photons. Using data from the direct dark matter search CRESST-II Phase 2 we can improve the existing constraints for the kinetic mixing for dark-photon masses between 0.3 and 0.5 keV/c2. In addition, we also present projected sensitivities for the next phases of the CRESST-III experiment showing great potential to improve the sensitivity for dark-photon masses below 1 keV.pt
dc.language.isoengpt
dc.relationDFG 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.titleSearch for dark photons using data from CRESST-II Phase 2pt
dc.typearticle-
degois.publication.firstPage012208pt
degois.publication.titleJournal of Physics: Conference Seriespt
dc.peerreviewedyespt
dc.identifier.doi10.1088/1742-6596/888/1/012208pt
degois.publication.volume888pt
dc.date.embargo2017-01-01*
uc.date.periodoEmbargo0pt
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextCom Texto completo-
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
crisitem.author.orcid0000-0002-3817-6015-
Appears in Collections:FCTUC Física - Artigos em Revistas Internacionais
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This item is licensed under a Creative Commons License Creative Commons