DarkSide-50, a background free experiment for dark matter searches

Agnes, P.; Alexander, 1 T.; Alton, 2 A.; Arisaka, 3 K.; Back, 4 H. O.; Baldin, 5 B.; Biery, 6 K.; Bonfini, 6 G.; Bossa, 7 M.; Brigatti, 8 A.; Brodsky, 9 J.; Budano, 5 F.; Cadonati, 10 L.; Calaprice, 2 F.; Canci, 5 N.; Candela, 4 A.; Cao, 7 H.; Cariello, 5 M.; Cavalcante, 11 P.; Chavarria, 7 A.; Chepurnov, 12 A.; Cocco, 13 A. G.; Crippa, 14 L.; D’Angelo, 9 D.; D’Incecco, 9 M.; Davini, 7 S.; De Deo, 15 M.; Derbin, 7 A.; Devoto, 16 A.; Di Eusanio, 17 F.; Di Pietro, 5 G.; Edkins, 9 E.; Empl, 18 A.; Fan, 15 A.; Fiorillo, 4 G.; Fomenko, 14 K.; Forster, 19 G.; Franco, 2 D.; Gabriele, 1 F.; Galbiati, 7 C.; Goretti, 5 A.; Grandi, 5 L.; Gromov, 12 M.; Guan, 13 M. Y.; Guardincerri, 20 Y.; Hackett, 6 B.; Herner, 18 K.; Hungerford, 6 E. V.; Ianni, 15 A. l.; Ianni, 7 A. n.; Jollet, 5 C.; Keeter, 21 K.; Kendziora, 22 C.; Kidner, 6 S.; 23,; Kobychev, a. V.; Koh, 24 G.; Korablev, 5 D.; Korga, 19 G.; Kurlej, 15 A.; 2 P. X., Li; Loer, 20 B.; Lombardi, 5 P.; Love, 9 C.; Ludhova, 25 L.; Luitz, 9 S.; 26 Y. Q., Ma; Machulin, 20 I.; 27,; Mandarano, 28 A.; 10,; Mari, Stefano Maria; Maricic, 10 J.; Marini, 18 L.; Martoff, 10 C. J.; Meregaglia, 25 A.; Meroni, 21 E.; Meyers, 9 P. D.; Milincic, 5 R.; Montanari, 18 D.; Montuschi, 6 M.; Monzani, 7 M. E.; Mosteiro, 26 P.; Mount, 5 B.; Muratova, 22 V.; Musico, 16 P.; Nelson, 11 A.; Odrowski, 5 S.; Okounkova, 7 M.; Orsini, 5 M.; Ortica, 7 F.; Pagani, 29 L.; Pallavicini, 11 M.; Pantic, 11 E.; 4,; Papp, 30 L.; Parmeggiano, 23 S.; Parsells, 9 R.; Pelczar, 5 K.; Pelliccia, 31 N.; Perasso, 29 S.; Pocar, 1 A.; Pordes, 2 S.; Pugachev, 6 D.; Qian, 27 H.; Randle, 5 K.; Ranucci, 2 G.; Razeto, 9 A.; Reinhold, 7 B.; Renshaw, 18 A.; Romani, 4 A.; Rossi, 29 B.; 5,; Rossi, 14 N.; Rountree, 7 S. D.; Sablone, 23 D.; Saggese, 15 P.; Saldanha, 7 R.; Sands, 12 W.; Sangiorgio, 5 S.; Segreto, 32 E.; Semenov, 7 D.; Shields, 16 E.; Skorokhvatov, 5 M.; 27,; Smirnov, 28 O.; Sotnikov, 19 A.; Stanford, 19 C.; Suvorov, 5 Y.; Tartaglia, 4 R.; Tatarowicz, 7 J.; Testera, 25 G.; Tonazzo, 11 A.; Unzhakov, 1 E.; Vogelaar, 16 R. B.; Wada, 23 M.; Walker, 5 S.; Wang, 14 H.; Wang, 4 Y.; Watson, 20 A.; Westerdale, 25 S.; Wojcik, 5 M.; Wright, 31 A.; Xiang, 5 X.; 5 J., Xu; Yang, 5 C. G.; Yoo, 20 J.; Zavatarelli, 6 S.; Zec, 11 A.; Zhu, 2 C.; 5,; Zuzel31, G.

doi:10.1088/1748-0221/9/01/C01034

The existence of dark matter is inferred from gravitational effects, but its nature remains a deep mystery. One possibility, motivated by considerations in elementary particle physics, is that dark matter consists of elementary particles, such as the hypothesized Weakly Interacting Massive Particles (WIMPs), with mass ~ 100 GeV and cross-section ~ 10−47 cm2, that can be gravitationally trapped inside our galaxy and revealed by their scattering on nuclei. It should be possible to detect WIMPs directly, as the orbital motion of the WIMPs composing the dark matter halo pervading the galaxy should result in WIMP-nucleus collisions of sufficient energy to be observable in the laboratory. The DarkSide-50 experiment is a direct WIMP search using a Liquid Argon Time Projection Chamber (LAr-TPC) with an active mass of 50 kg with a high sensitivity and an ultra-low background detector.

P., A., 1 T., A., 2 A., A., 3 K., A., 4 H. O., B., 5 B., B., et al. (2014). DarkSide-50, a background free experiment for dark matter searches. JOURNAL OF INSTRUMENTATION, 9 [10.1088/1748-0221/9/01/C01034].