학술논문

Search for dark matter annual modulation with DarkSide-50
Document Type
Working Paper
Author
Collaboration, The DarkSide-50Agnes, P.Albuquerque, I. F. M.Alexander, T.Alton, A. K.Ave, M.Back, H. O.Batignani, G.Biery, K.Bocci, V.Bonivento, W. M.Bottino, B.Bussino, S.Cadeddu, M.Cadoni, M.Calaprice, F.Caminata, A.Campos, M. D.Canci, N.Caravati, M.Cargioli, N.Cariello, M.Carlini, M.Cataudella, V.Cavalcante, P.Cavuoti, S.Chashin, S.Chepurnov, A.Cicalò, C.Covone, G.D'Angelo, D.Davini, S.De Candia, A.De Cecco, S.De Filippis, G.De Rosa, G.Derbin, A. V.Devoto, A.D'Incecco, M.Dionisi, C.Dordei, F.Downing, M.D'Urso, D.Fairbairn, M.Fiorillo, G.Franco, D.Gabriele, F.Galbiati, C.Ghiano, C.Giganti, C.Giovanetti, G. K.Goretti, A. M.di Cortona, G. GrilliGrobov, A.Gromov, M.Guan, M.Gulino, M.Hackett, B. R.Herner, K.Hessel, T.Hosseini, B.Hubaut, F.Hugues, T.Hungerford, E. V.Ianni, An.Ippolito, V.Keeter, K.Kendziora, C. L.Kimura, M.Kochanek, I.Korablev, D.Korga, G.Kubankin, A.Kuss, M.Kuźniak, M.La Commara, M.Lai, M.Li, X.Lissia, M.Longo, G.Lychagina, O.Machulin, I. N.Mapelli, L. P.Mari, S. M.Maricic, J.Messina, A.Milincic, R.Monroe, J.Morrocchi, M.Mougeot, X.Muratova, V. N.Musico, P.Nozdrina, A. O.Oleinik, A.Ortica, F.Pagani, L.Pallavicini, M.Pandola, L.Pantic, E.Paoloni, E.Pelczar, K.Pelliccia, N.Piacentini, S.Pocar, A.Poehlmann, D. M.Pordes, S.Poudel, S. S.Pralavorio, P.Price, D. D.Ragusa, F.Razeti, M.Razeto, A.Renshaw, A. L.Rescigno, M.Rode, J.Romani, A.Sablone, D.Samoylov, O.Sandford, E.Sands, W.Sanfilippo, S.Savarese, C.Schlitzer, B.Semenov, D. A.Shchagin, A.Sheshukov, A.Skorokhvatov, M. D.Smirnov, O.Sotnikov, A.Stracka, S.Suvorov, Y.Tartaglia, R.Testera, G.Tonazzo, A.Unzhakov, E. V.Vishneva, A.Vogelaar, R. B.Wada, M.Wang, H.Wang, Y.Westerdale, S.Wojcik, M. M.Xiao, X.Yang, C.Zuzel, G.
Source
Subject
High Energy Physics - Experiment
Astrophysics - Cosmology and Nongalactic Astrophysics
Language
Abstract
Dark matter induced event rate in an Earth-based detector is predicted to show an annual modulation as a result of the Earth's orbital motion around the Sun. We searched for this modulation signature using the ionization signal of the DarkSide-50 liquid argon time projection chamber. No significant signature compatible with dark matter is observed in the electron recoil equivalent energy range above $40~{\rm eV_{ee}}$, the lowest threshold ever achieved in such a search.
Comment: 8 pages, 4 figures