The DarkSide Multiton Detector for the Direct Dark Matter Search

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dc.contributor.authorAalseth, C. E.en
dc.contributor.authorAgnes, P.en
dc.contributor.authorAlton, A. K.en
dc.contributor.authorArisaka, K.en
dc.contributor.authorAsner, D. M.en
dc.contributor.authorBack, H. O.en
dc.contributor.authorBaldin, B.en
dc.contributor.authorBiery, K.en
dc.contributor.authorBonfini, G.en
dc.contributor.authorBossa, M.en
dc.contributor.authorBrigatti, A.en
dc.contributor.authorBrodsky, J.en
dc.contributor.authorBudano, F.en
dc.contributor.authorCadonati, L.en
dc.contributor.authorCadoni, M.en
dc.contributor.authorCalaprice, F.en
dc.contributor.authorCanci, N.en
dc.contributor.authorCandela, A.en
dc.contributor.authorCao, H.en
dc.contributor.authorCariello, M.en
dc.contributor.authorCavalcante, P.en
dc.contributor.authorChepurnov, A.en
dc.contributor.authorCocco, A. G.en
dc.contributor.authorCondon, C.en
dc.contributor.authorCrippa, L.en
dc.contributor.authorD'Angelo, D.en
dc.contributor.authorD'Incecco, M.en
dc.contributor.authorDavini, S.en
dc.contributor.authorDe Deo, M.en
dc.contributor.authorDerbin, A. V.en
dc.contributor.authorDevoto, A.en
dc.contributor.authorDi Eusanio, F.en
dc.contributor.authorEdkins, E.en
dc.contributor.authorEmpl, A.en
dc.contributor.authorFan, A.en
dc.contributor.authorFiorillo, G.en
dc.contributor.authorFomenko, K.en
dc.contributor.authorForster, G.en
dc.contributor.authorFoxe, M.en
dc.contributor.authorFranco, D.en
dc.contributor.authorGabriele, Federicoen
dc.contributor.authorGalbiati, C.en
dc.contributor.authorGoretti, A.en
dc.contributor.authorGrandi, L.en
dc.contributor.authorGromov, M.en
dc.contributor.authorGuan, M. Y.en
dc.contributor.authorGuardincerri, Y.en
dc.contributor.authorHackett, B.en
dc.contributor.authorHerner, K.en
dc.contributor.authorHime, A.en
dc.contributor.authorHumble, P.en
dc.contributor.authorHungerford, Ed V.en
dc.contributor.authorIanni, A.en
dc.contributor.authorIanni, A.en
dc.contributor.authorJaffe, D. E.en
dc.contributor.authorJollet, C.en
dc.contributor.authorKeeter, K.en
dc.contributor.authorKendziora, C. L.en
dc.contributor.authorKidner, S.en
dc.contributor.authorKobychev, V.en
dc.contributor.authorKoh, G.en
dc.contributor.authorKorablev, D.en
dc.contributor.authorKorga, G.en
dc.contributor.authorKurlej, A.en
dc.contributor.authorLi, P. X.en
dc.contributor.authorLissia, M.en
dc.contributor.authorLombardi, Paoloen
dc.contributor.authorLudhova, L.en
dc.contributor.authorLuitz, S.en
dc.contributor.authorLukyachenko, G.en
dc.contributor.authorMa, Y. Q.en
dc.contributor.authorMachulin, I. N.en
dc.contributor.authorMandarano, A.en
dc.contributor.authorMari, S. M.en
dc.contributor.authorMaricic, Jelenaen
dc.contributor.authorMarini, L.en
dc.contributor.authorMarkov, D.en
dc.contributor.authorMartoff, J.en
dc.contributor.authorMeregaglia, A.en
dc.contributor.authorMeroni, E.en
dc.contributor.authorMeyers, P. D.en
dc.contributor.authorMiletic, T.en
dc.contributor.authorMilincic, R.en
dc.contributor.authorMontuschi, M.en
dc.contributor.authorMonzani, M. E.en
dc.contributor.authorMosteiro, P.en
dc.contributor.authorMount, B.en
dc.contributor.authorMuratova, V. N.en
dc.contributor.authorMusico, P.en
dc.contributor.authorMontanari, D.en
dc.contributor.authorNelson, A.en
dc.contributor.authorOdrowski, S.en
dc.contributor.authorOdrzywolek, A.en
dc.contributor.authorOrrell, J. L.en
dc.contributor.authorOrsini, M.en
dc.contributor.authorOrtica, F.en
dc.contributor.authorPagani, L.en
dc.contributor.authorPallavicini, M.en
dc.contributor.authorPantic, E.en
dc.contributor.authorParmeggiano, S.en
dc.contributor.authorParsells, B.en
dc.contributor.authorPelczar, K.en
dc.contributor.authorPelliccia, N.en
dc.contributor.authorPerasso, S.en
dc.contributor.authorPerasso, L.en
dc.contributor.authorPocar, A.en
dc.contributor.authorPordes, S.en
dc.contributor.authorPugachev, D. A.en
dc.contributor.authorQian, H.en
dc.contributor.authorRandle, K.en
dc.contributor.authorRanucci, G.en
dc.contributor.authorRazeto, A.en
dc.contributor.authorRecine, K.en
dc.contributor.authorReinhold, B.en
dc.contributor.authorRenshaw, A. L.en
dc.contributor.authorRomani, A.en
dc.contributor.authorRossi, Nicolaen
dc.contributor.authorRossi, B.en
dc.contributor.authorRountree, S. D.en
dc.contributor.authorSablone, D.en
dc.contributor.authorSaggese, P.en
dc.contributor.authorSaldanha, R.en
dc.contributor.authorSands, W.en
dc.contributor.authorSangiorgio, S.en
dc.contributor.authorSegreto, E.en
dc.contributor.authorSemenov, D. A.en
dc.contributor.authorShields, E.en
dc.contributor.authorSkorokhvatov, Mikhail D.en
dc.contributor.authorSmallcomb, M.en
dc.contributor.authorSmirnov, O. Y.en
dc.contributor.authorSotnikov, A.en
dc.contributor.authorSuvurov, Y.en
dc.contributor.authorTartaglia, R.en
dc.contributor.authorTatarowicz, J.en
dc.contributor.authorTestera, G.en
dc.contributor.authorTonazzo, A.en
dc.contributor.authorUnzhakov, E. V.en
dc.contributor.authorVogelaar, R. Bruceen
dc.contributor.authorWada, M.en
dc.contributor.authorWalker, S. E.en
dc.contributor.authorWang, H.en
dc.contributor.authorWang, Y.en
dc.contributor.authorWatson, A. W.en
dc.contributor.authorWesterdale, S.en
dc.contributor.authorWilliams, R.en
dc.contributor.authorWojcik, M. M.en
dc.contributor.authorXu, J.en
dc.contributor.authorYang, C. G.en
dc.contributor.authorYoo, J.en
dc.contributor.authorYu, B.en
dc.contributor.authorZavatarelli, S.en
dc.contributor.authorZhong, W. L.en
dc.contributor.authorZuzel, G.en
dc.contributor.departmentPhysicsen
dc.date.accessioned2017-09-18T09:41:03Zen
dc.date.available2017-09-18T09:41:03Zen
dc.date.issued2015-01-20en
dc.date.updated2017-09-18T09:41:03Zen
dc.description.abstractAlthough the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (ud_less_than100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide-50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.en
dc.description.versionPublished versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.citationC. E. Aalseth, P. Agnes, A. Alton, et al., “The DarkSide Multiton Detector for the Direct Dark Matter Search,” Advances in High Energy Physics, vol. 2015, Article ID 541362, 8 pages, 2015. doi:10.1155/2015/541362en
dc.identifier.doihttps://doi.org/10.1155/2015/541362en
dc.identifier.urihttp://hdl.handle.net/10919/78956en
dc.language.isoenen
dc.publisherHindawien
dc.rightsCreative Commons Attribution 4.0 Internationalen
dc.rights.holderCopyright © 2015 C. E. Aalseth et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP3.en
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en
dc.titleThe DarkSide Multiton Detector for the Direct Dark Matter Searchen
dc.title.serialAdvances in High Energy Physicsen
dc.typeArticle - Refereeden
dc.type.dcmitypeTexten

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