Search for low-mass dark matter WIMPs with 12 ton-day exposure of DarkSide-50
Creators: name: 50 Collaboration
name: Agnes, P.
name: Albuquerque, I. F. M.
name: Alexander, T.
name: Alton, A. K.
name: Ave, M.
name: Back, H. O.
name: Batignani, G.
name: Biery, K.
name: Bocci, V.
name: Bonivento, W. M.
name: Bottino, B.
name: Bussino, S.
name: Cadeddu, M.
name: Cadoni, M.
name: Calaprice, F.
name: Caminata, A.
name: Canci, N.
name: Caravati, M.
name: Cariello, M.
name: Carlini, M.
name: Carpinelli, M.
name: Cataudella, V.
name: Cavalcante, P.
name: Cavuoti, S.
name: Chashin, S.
name: Chepurnov, A.
name: Cicalò, C.
name: Covone, G.
name: D'Angelo, D.
name: Davini, S.
name: De Candia, A.
name: De Cecco, S.
name: De Filippis, G.
name: De Rosa, G.
name: Derbin, A. V.
name: Devoto, A.
name: D'Incecco, M.
name: Dionisi, C.
name: Dordei, F.
name: Downing, M.
name: D'Urso, D.
name: Fiorillo, G.
name: Franco, D.
name: Gabriele, F.
name: Galbiati, C.
name: Ghiano, C.
name: Giganti, C.
name: Giovanetti, G. K.
name: Goretti, A. M.
name: di Cortona, G. Grilli
name: Grobov, A.
name: Gromov, M.
name: Guan, M.
name: Gulino, M.
name: Hackett, B. R.
name: Herner, K.
name: Hessel, T.
name: Hosseini, B.
name: Hubaut, F.
name: Hungerford, E. V.
name: Ianni, An.
name: Ippolito, V.
name: Keeter, K.
name: Kendziora, C. L.
name: Kimura, M.
name: Kochanek, I.
name: Korablev, D.
name: Korga, G.
name: Kubankin, A.
name: Kuss, M.
name: La Commara, M.
name: Lai, M.
name: Li, X.
name: Lissia, M.
name: Longo, G.
name: Lychagina, O.
name: Machulin, I. N.
name: Mapelli, L. P.
name: Mari, S. M.
name: Maricic, J.
name: Messina, A.
name: Milincic, R.
name: Monroe, J.
name: Morrocchi, M.
name: Mougeot, X.
name: Muratova, V. N.
name: Musico, P.
name: Nozdrina, A. O.
name: Oleinik, A.
name: Ortica, F.
name: Pagani, L.
name: Pallavicini, M.
name: Pandola, L.
name: Pantic, E.
name: Paoloni, E.
name: Pelczar, K.
name: Pelliccia, N.
name: Piacentini, S.
name: Piacentini, S.
name: Picciau, E.
name: Pocar, A.
name: Poehlmann, D. M.
name: Pordes, S.
name: Poudel, S. S.
name: Pralavorio, P.
name: Price, D. D.
name: Ragusa, F.
name: Razeti, M.
name: Razeto, A.
name: Renshaw, A. L.
name: Rescigno, M.
name: Rode, J.
name: Romani, A.
name: Sablone, D.
name: Samoylov, O.
name: Sands, W.
name: Sanfilippo, S.
name: Sanford, E.
name: Savarese, C.
name: Schlitzer, B.
name: Semenov, D. A.
name: Shchagin, A.
name: Sheshukov, A.
name: Skorokhvatov, M. D.
name: Smirnov, O.
name: Sotnikov, A.
name: Stracka, S.
name: Suvorov, Y.
name: Tartaglia, R.
name: Testera, G.
name: Tonazzo, A.
name: Unzhakov, E. V.
name: Vishneva, A.
name: Vogelaar, R. B.
name: Wada, M.
name: Wang, H.
name: Wang, Y.
name: Westerdale, S.
name: Wojcik, M. M.
name: Xiao, X.
name: Yang, C.
name: Zuzel, G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: We report on the search for dark matter WIMPs in the mass range below 10 GeV/c$^2$, from the analysis of the entire dataset acquired with a low-radioactivity argon target by the DarkSide-50 experiment at LNGS. The new analysis benefits from more accurate calibration of the detector response, improved background model, and better determination of systematic uncertainties, allowing us to accurately model the background rate and spectra down to 0.06 keV$_{er}$. A 90% C.L. exclusion limit for the spin-independent cross section of 3 GeV/c$^2$ mass WIMP on nucleons is set at 6$\times$10$^{-43}$ cm$^2$, about a factor 10 better than the previous DarkSide-50 limit. This analysis extends the exclusion region for spin-independent dark matter interactions below the current experimental constraints in the $[1.2, 3.6]$ GeV/c$^2$ WIMP mass range.
description: 11 pages, 12 figures