The DarkSide Experiment: Present Status and Future

G. Zuzel,P. Agnes,I. F. M. Albuquerque,T. Alexander,A. Alton,D. M. Asner,H. O. Back, B. Baldin, K. Biery,V. Bocci,G. Bonfini,W. Bonivento, M. Bossa,B. Bottino,A. Brigatti,J. Brodsky, F. Budano,S. Bussino,M. Cadeddu,L. Cadonati,M. Cadoni, F. Calaprice,N. Canci,A. Candela,M. Caravati, M. Cariello, M. Carlini, S. Catalanotti, P. Cavalcante, A. Chepurnov, C. Cicalò,A. G. Cocco,G. Covone,D. D’Angelo,M. D’Incecco,S. Davini,S. De Cecco,M. De Deo,M. De Vincenzi,A. Derbin,A. Devoto,F. Di Eusanio,G. Di Pietro,C. Dionisi, E. Edkins, A. Empl,A. Fan,G. Fiorillo, K. Fomenko,G. Forster,D. Franco,F. Gabriele,C. Galbiati,S. Giagu,C. Giganti,G. K. Giovanetti, A. Goretti,F. Granato, L. Grandi,M. Gromov,M. Guan, Y. Guardincerri, B. Hackett, K. Herner,D. Hughes,P. Humble,E. Hungerford,Al. Ianni,An. Ianni,I. James,T. N. Johnson, C. Jollet, K. Keeter, C. Kendziora, G. Koh, D. Korablev, G. Korga,A. Kubankin,X. Li,M. Lissia,B. Loer,P. Lombardi,G. Longo,Y. Ma, I. Machulin, A. Mandarano,S. M. Mari,J. Maricic,L. Marini,C. J. Martoff,A. Meregaglia,P. D. Meyers, R. Milincic, J. D. Miller, D. Montanari,A. Monte, B. J. Mount,V. Muratova, P. Musico,J. Napolitano,A. Navrer Agasson, S. Odrowski, M. Orsini,F. Ortica,L. Pagani,M. Pallavicini, E. Pantic, S. Parmeggiano,K. Pelczar, N. Pelliccia,A. Pocar, S. Pordes,D. A. Pugachev,H. Qian, K. Randle,G. Ranucci,M. Razeti,A. Razeto,B. Reinhold,A. Renshaw, M. Rescigno,Q. Riffard,A. Romani,B. Rossi,N. Rossi, D. Rountree, D. Sablone,P. Saggese,R. Saldanha, W. Sands,C. Savarese,B. Schlitzer,E. Segreto, D. Semenov,E. Shields,P. N. Singh, M. Skorokhvatov,O. Smirnov,A. Sotnikov,C. Stanford,Y. Suvorov,R. Tartaglia, J. Tatarowicz, G. Testera, A. Tonazzo,P. Trinchese,E. Unzhakov,M. Verducci,A. Vishneva,B. Vogelaar,M. Wada,S. Walker, H. Wang,Y. Wang,A. W. Watson,S. Westerdale,M. Wojcik,Xi Xiang,X. Xiao,J. Xu,C. Yang, A. Zec,W. Zhong,C. Zhu

Journal of Physics Conference Series(2017)

引用 7|浏览31
暂无评分
摘要
DARKSIDE is a multi-stage program devoted to direct searches of Dark Matter particles with detectors based on double phase liquid Argon Time Projection Chamber. The DARKSIDE-50 setup is running underground at the Laboratori Nazionali del Gran Sasso. First it was operated with Atmospheric Argon and during that run (1422 +/- 67) kgxd of truly background-free exposure has been accumulated. Obtained data made it possible to set a 90% C.L. upper limit on the WIMP-nucleon cross section of 6.1 x 10(-44) cm(2) (for a WIMP mass of 100 GeV/c(2)). Presently the detector is filled with Underground Argon, which is depleted in Ar-39 by a factor of (1.4 +/- 0.2) x 10(3) with respect to Atmospheric Argon. Acquired so far (2616 +/- 43) kgxd (71 live days) in combination with the data from the Atmospheric Argon run give us the 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section of 2.0 x 10(-44) cm(2) for a WIMP mass of 100 GeV/c(2). Up to date this is the best limit obtained with an argon target.
更多
查看译文
关键词
darkside experiment
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要