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20 April 2024

» arxiv » 1412.2969

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The Electronics and Data Acquisition System of the DarkSide Dark Matter Search
DarkSide Collaboration - P. Agnes ; T. Alexander ; A. Alton ; K. Arisaka ; H. O. Back ; B. Baldin ; K. Biery ; G. Bonfini ; M. Bossa ; A. Brigatti ; J. Brodsky ; F. Budano ; L. Cadonati ; F. Calaprice ; N. Canci ; A. Candela ; H. Cao ; M. Cariello ; P. Cavalcante ; A. Chavarria ; A. Chepurnov ; A. G. Cocco ; L. Crippa ; D. D'Angelo ; M. D'Incecco ; S.Davini ; M. De Deo ; A. Derbin ; A. Devoto ; F. Di Eusanio ; G. Di Pieto ; E. Edkins ; A. Empl ; A. Fan ; G. Fiorillo ; K. Fomenko ; G. Forster ; D. Franco ; F. Gabriele ; C. Galbiati ; A. Goretti ; L. Grandi ; M. Gromov ; M. Y. Guan ; Y. Guardincerri ; B.Hackett ; K. Herner ; E. Hungerford ; Al. Ianni ; An. Ianni ; C. Jollet ; K. Keeter ; C. Kendziora ; S. Kidner ; V. Kobychev ; G. Koh ; D. Korablev ; G. Korga ; A. Kurlej ; P. X. Li ; B. Loer ; P. Lombardi ; C. Love ; L.Ludhova ; S. Luitz ; Y. Q. Ma ; I. Machulin ; A. Mandarano ; S.M. Mari ; J. Maricic ; L. Marini ; J. Martoff ; A. Meregaglia ; E. Meroni ; P. D. Meyers ; R. Milincic ; D. Montanari ; M. Montuschi ; M. E. Monzani ; P. Mosteiro ; B. Mount ; V. Muratova ; P. Musico ; A. Nelson ; S. Odrowski ; M. Okounkoa ; M. Orsini ; F. Ortica ; L. Pagani ; M. Pallavicini ; E. Pantic ; L. Papp ; S. Parmeggiano ; Bob Parsells ; K. Pelczar ; N. Pelliccia ; S. Perasso ; A. Pocar ; S. Pordes ; D. Pugachev ; H. Qian ; K. Randle ; G. Ranucci ; A. Razeto ; B. Reinhold ; A. Renshaw ; A. Romani ; B. Rossi ; N. Rossi ; S. D. Rountree ; D. Sablone ; P. Saggese ; R. Saldanha ; W. Sands ; S. Sangiorgio ; E. Segreto ; D. Semenov ; E. Shields ; M. Skorokhvatov ; O. Smirnov ; A. Sotnikov ; C. Stanford ; Suvorov ; R. Tartaglia ; J. Tatarowicz ; G. Testera ; A. Tonazzo ; E. Unzhakov ; R. B. Vogelaar ; M. Wada ; S. E. Walker ; H. Wang ; Y. Wang ; A. Watson ; S. Westerdale ; M. Wojcik ; A. Wright ; X. Xiang ; J. Xu ; C. G. Yang ; J. Yoo ; S. Zavatarelli ; A. Zec ; C. Zhu ; G. Zuzel ;
Date:	9 Dec 2014
Abstract:	It is generally inferred from astronomical measurements that Dark Matter (DM) comprises approximately 27\% of the energy-density of the universe. If DM is a subatomic particle, a possible candidate is a Weakly Interacting Massive Particle (WIMP), and the DarkSide-50 (DS) experiment is a direct search for evidence of WIMP-nuclear collisions. DS is located underground at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, and consists of three active, embedded components; an outer water veto (CTF), a liquid scintillator veto (LSV), and a liquid argon (LAr) time projection chamber (TPC). This paper describes the data acquisition and electronic systems of the DS detectors, designed to detect the residual ionization from such collisions.
Source:	arXiv, 1412.2969
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