DARWIN: towards the ultimate dark matter detector
- Aalbers, J.
- Agostini, F.
- Alfonsi, M.
- Amaro, D.
- Amsler, C.
- Aprile, E.
- Arazi, L.
- Arneodo, F.
- Barrow, P.
- Baudis, L.
- Benabderrahmane, M. L.
- Berger, Thierry
- Beskers, B.
- Breskin, A.
- Breur, A.
- Brown, A.
- Brown, E.
- Bruenner, S.
- Bruno, G.
- Budnik, R.
- Bütikofer, L.
- Calvén, J.
- Cardoso, J. M. R.
- Cichon, D.
- Coderre, D.
- Colijn, A. P.
- Conrad, J.
- Cussonneau, Jean-Pierre
- Decowski, P.
- Diglio, Sara
- Drexlin, G.
- Duchovni, E.
- Erdal, E.
- Eurin, G.
- Ferella, A.
- Fieguth, A.
- Fulgione, W.
- Rosso, A. Gallo
- Gangi, P.
- Giovanni, A.
- Galloway, M.
- Garbini, M.
- Geis, C.
- Glueck, F.
- Grandi, L.
- Greene, Z.
- Grignon, C.
- Hasterok, C.
- Hannen, V.
- Hogenbirk, E.
- Howlett, J.
- Hilk, D.
- Hils, C.
- James, A.
- Kaminsky, B.
- Kazama, S.
- Kilminster, B.
- Kish, A.
- Krauss, M.
- Landsman, H.
- Lang, R. F.
- Lin, Q.
- Linde, L.
- Lindemann, S.
- Lindner, M.
- Lopes, J. A. M.
- Undagoitia, T. Marrodan
- Masbou, Julien
- Massoli, F. V.
- Mayani, D.
- Messina, M.
- Micheneau, K.
- Molinario, A.
- Morå, K.
- Morteau, E.
- Murra, M.
- Naganoma, J.
- Newstead, J. L.
- Ni, K.
- Oberlack, U.
- Pakarha, P.
- Pelssers, B.
- de Perio, P.
- Persiani, R.
- Piastra, F.
- Piro, C.
- Plante, G.
- Rauch, L.
- Reichard, S.
- Rizzo, A.
- Rupp, N.
- Santos, J. M. F. Dos
- Sartorelli, G.
- Scheibelhut, M.
- Schindler, S.
- Schumann, M.
- Schreiner, J.
- Lavina, L. Scotto
- Selvi, M.
- Shagin, P.
- Silva, C.
- Simgen, H.
- Sissol, P.
- Sivers, M. Von
- Thers, Dominique
- Thurn, J.
- Tiseni, A.
- Trotta, R.
- Tunnell, C. D.
- Valerius, K.
- Vargas, M. A.
- Wang, H.
- Wei, Y.
- Weinheimer, C.
- Wester, T.
- Wulf, J.
- Zhang, Y.
- Zhu, T.
- Zuber, K.
- Amaro, F. D.
- Breur, P. A.
- Buetikofer, L.
- Calven, J.
- Decowski, M. P.
- Di Gangi, P.
- Di Giovanni, A.
- Krauss, L. M.
- Linde, F. L.
- Mora, K. D.
- Piro, M. C.
- Silva, M. C.
- von Sivers, M.
DOIAbstract
36 pages, 11 figuresInternational audienceDARk matter WImp search with liquid xenoN (DARWIN) 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/c2, such a detector with its large mass, low-energy threshold...
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