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DARWIN: towards the ultimate dark matter detector
Vise andre og tillknytning
Rekke forfattare: 1192016 (engelsk)Inngår i: Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, E-ISSN 1475-7516, nr 11, artikkel-id 017Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

DARk matter WImp search with liquid xenoN (DARWIN(2)) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally accessible parameter space for Weakly Interacting Massive Particles (WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background. The prompt scintillation light and the charge signals induced by particle interactions in the xenon will be observed by VUV sensitive, ultra-low background photosensors. Besides its excellent sensitivity to WIMPs above a mass of 5 GeV/c(2), such a detector with its large mass, low-energy threshold and ultra-low background level will also be sensitive to other rare interactions. It will search for solar axions,galactic axion-like particles and the neutrinoless double-beta decay of Xe-136, as well as measure the low-energy solar neutrino flux with <1% precision, observe coherent neutrino-nucleus interactions, and detect galactic supernovae. We present the concept of the DARWIN detector and discuss its physics reach, the main sources of backgrounds and the ongoing detector design and R&D efforts.

sted, utgiver, år, opplag, sider
2016. nr 11, artikkel-id 017
Emneord [en]
dark matter detectors, neutrino detectors, double beta decay, solar and atmospheric neutrinos
HSV kategori
Identifikatorer
URN: urn:nbn:se:su:diva-142425DOI: 10.1088/1475-7516/2016/11/017ISI: 000397734100017OAI: oai:DiVA.org:su-142425DiVA, id: diva2:1092424
Tilgjengelig fra: 2017-05-02 Laget: 2017-05-02 Sist oppdatert: 2017-11-29bibliografisk kontrollert

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Calvén, JakobConrad, JanFerella, AlfredoMorå, Knut D.Pelssers, Bart
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