Abstract
DarkSide-50 is a detector for dark matter candidates in the form of weakly interacting massive particles. It utilizes a liquid argon time projection chamber for the inner main detector, surrounded by a liquid scintillator veto (LSV) and a water Cherenkov veto detector (WCV). The LSV and WCV act as the neutron and cosmogenic muon veto detectors for DarkSide-50. This paper describes the electronics and data acquisition system used for these two detectors. The system is made of a custom built front end electronics and commercial National Instruments high speed digitizers. The front end electronics, the DAQ, and the trigger system have been used to acquire data in the form of zero-suppressed waveform samples from the 110 PMTs of the LSV and the 80 PMTs of the WCV. The veto DAQ system has proven its performance and reliability. This electronics and DAQ system can be scaled and used as it is for the veto of the next generation DarkSide-20k detector.
| Original language | English (US) |
|---|---|
| Article number | P12007 |
| Journal | Journal of Instrumentation |
| Volume | 11 |
| Issue number | 12 |
| DOIs | |
| State | Published - Dec 12 2016 |
All Science Journal Classification (ASJC) codes
- Mathematical Physics
- Instrumentation
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The electronics and data acquisition system for the DarkSide-50 veto detectors. / Agnes, P.; Agostino, L.; Albuquerque, I. F.M.; Alexander, T.; Alton, A. K.; Arisaka, K.; Back, H. O.; Baldin, B.; Biery, K.; Bonfini, G.; Bossa, M.; Bottino, B.; Brigatti, A.; Brodsky, J.; Budano, F.; Bussino, S.; Cadeddu, M.; Cadoni, M.; Calaprice, F.; Canci, N.; Candela, A.; Cao, H.; Cariello, M.; Carlini, M.; Catalanotti, S.; Cavalcante, P.; Chepurnov, A.; Cocco, A. G.; Covone, G.; Crippa, L.; D'Angelo, D.; D'Incecco, M.; Davini, S.; DeCecco, S.; De Deo, M.; De Vincenzi, M.; Derbin, A.; Devoto, A.; Di Eusanio, F.; Di Pietro, G.; Edkins, E.; Empl, A.; Fan, A.; Fiorillo, G.; Fomenko, K.; Foster, G.; Franco, D.; Gabriele, F.; Galbiati, C.; Giganti, C.; Goretti, A. M.; Granato, F.; Grandi, L.; Gromov, M.; Guan, M.; Guardincerri, Y.; Hackett, B. R.; Herner, K. R.; Hungerford, E. V.; Ianni, Aldo; Ianni, Andrea; James, I.; Jollet, C.; Keeter, K.; Kendziora, C. L.; Kobychev, V.; Koh, G.; Korablev, D.; Korga, G.; Kubankin, A.; Li, X.; Lissia, M.; Lombardi, P.; Luitz, S.; Ma, Y.; Machulin, I. N.; Mandarano, A.; Mari, S. M.; Maricic, J.; Marini, L.; Martoff, C. J.; Meregaglia, A.; Meyers, P. D.; Miletic, T.; Milincic, R.; Montanari, D.; Monte, A.; Montuschi, M.; Monzani, M. E.; Mosteiro, P.; Mount, B. J.; Muratova, V. N.; Musico, P.; Napolitano, J.; Nelson, A.; Odrowski, S.; Orsini, M.; Ortica, F.; Pagani, L.; Pallavicini, M.; Pantic, E.; Parmeggiano, S.; Pelczar, K.; Pelliccia, N.; Pocar, A.; Pordes, S.; Pugachev, D. A.; Qian, H.; Randle, K.; Ranucci, G.; Razeto, A.; Reinhold, B.; Renshaw, A. L.; Riffard, Q.; Romani, A.; Rossi, B.; Rossi, N.; Rountree, S. D.; Sablone, D.; Saggese, P.; Saldanha, R.; Sands, W.; Sangiorgio, S.; Savarese, C.; Segreto, E.; Semenov, D. A.; Shields, E.; Singh, P. N.; Skorokhvatov, M. D.; Smirnov, O.; Sotnikov, A.; Stanford, C.; Suvorov, Y.; Tartaglia, R.; Tatarowicz, J.; Testera, G.; Tonazzo, A.; Trinchese, P.; Unzhakov, E. V.; Vishneva, A.; Vogelaar, R. B.; Wada, M.; Walker, S.; Wang, H.; Wang, Y.; Watson, A. W.; Westerdale, S.; Wilhelmi, J.; Wojcik, M. M.; Xiang, X.; Xu, J.; Yang, C.; Yoo, J.; Zavatarelli, S.; Zec, A.; Zhong, W.; Zhu, C.; Zuzel, G.
In: Journal of Instrumentation, Vol. 11, No. 12, P12007, 12.12.2016.Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - The electronics and data acquisition system for the DarkSide-50 veto detectors
AU - Agnes, P.
AU - Agostino, L.
AU - Albuquerque, I. F.M.
AU - Alexander, T.
AU - Alton, A. K.
AU - Arisaka, K.
AU - Back, H. O.
AU - Baldin, B.
AU - Biery, K.
AU - Bonfini, G.
AU - Bossa, M.
AU - Bottino, B.
AU - Brigatti, A.
AU - Brodsky, J.
AU - Budano, F.
AU - Bussino, S.
AU - Cadeddu, M.
AU - Cadoni, M.
AU - Calaprice, F.
AU - Canci, N.
AU - Candela, A.
AU - Cao, H.
AU - Cariello, M.
AU - Carlini, M.
AU - Catalanotti, S.
AU - Cavalcante, P.
AU - Chepurnov, A.
AU - Cocco, A. G.
AU - Covone, G.
AU - Crippa, L.
AU - D'Angelo, D.
AU - D'Incecco, M.
AU - Davini, S.
AU - DeCecco, S.
AU - De Deo, M.
AU - De Vincenzi, M.
AU - Derbin, A.
AU - Devoto, A.
AU - Di Eusanio, F.
AU - Di Pietro, G.
AU - Edkins, E.
AU - Empl, A.
AU - Fan, A.
AU - Fiorillo, G.
AU - Fomenko, K.
AU - Foster, G.
AU - Franco, D.
AU - Gabriele, F.
AU - Galbiati, C.
AU - Giganti, C.
AU - Goretti, A. M.
AU - Granato, F.
AU - Grandi, L.
AU - Gromov, M.
AU - Guan, M.
AU - Guardincerri, Y.
AU - Hackett, B. R.
AU - Herner, K. R.
AU - Hungerford, E. V.
AU - Ianni, Aldo
AU - Ianni, Andrea
AU - James, I.
AU - Jollet, C.
AU - Keeter, K.
AU - Kendziora, C. L.
AU - Kobychev, V.
AU - Koh, G.
AU - Korablev, D.
AU - Korga, G.
AU - Kubankin, A.
AU - Li, X.
AU - Lissia, M.
AU - Lombardi, P.
AU - Luitz, S.
AU - Ma, Y.
AU - Machulin, I. N.
AU - Mandarano, A.
AU - Mari, S. M.
AU - Maricic, J.
AU - Marini, L.
AU - Martoff, C. J.
AU - Meregaglia, A.
AU - Meyers, P. D.
AU - Miletic, T.
AU - Milincic, R.
AU - Montanari, D.
AU - Monte, A.
AU - Montuschi, M.
AU - Monzani, M. E.
AU - Mosteiro, P.
AU - Mount, B. J.
AU - Muratova, V. N.
AU - Musico, P.
AU - Napolitano, J.
AU - Nelson, A.
AU - Odrowski, S.
AU - Orsini, M.
AU - Ortica, F.
AU - Pagani, L.
AU - Pallavicini, M.
AU - Pantic, E.
AU - Parmeggiano, S.
AU - Pelczar, K.
AU - Pelliccia, N.
AU - Pocar, A.
AU - Pordes, S.
AU - Pugachev, D. A.
AU - Qian, H.
AU - Randle, K.
AU - Ranucci, G.
AU - Razeto, A.
AU - Reinhold, B.
AU - Renshaw, A. L.
AU - Riffard, Q.
AU - Romani, A.
AU - Rossi, B.
AU - Rossi, N.
AU - Rountree, S. D.
AU - Sablone, D.
AU - Saggese, P.
AU - Saldanha, R.
AU - Sands, W.
AU - Sangiorgio, S.
AU - Savarese, C.
AU - Segreto, E.
AU - Semenov, D. A.
AU - Shields, E.
AU - Singh, P. N.
AU - Skorokhvatov, M. D.
AU - Smirnov, O.
AU - Sotnikov, A.
AU - Stanford, C.
AU - Suvorov, Y.
AU - Tartaglia, R.
AU - Tatarowicz, J.
AU - Testera, G.
AU - Tonazzo, A.
AU - Trinchese, P.
AU - Unzhakov, E. V.
AU - Vishneva, A.
AU - Vogelaar, R. B.
AU - Wada, M.
AU - Walker, S.
AU - Wang, H.
AU - Wang, Y.
AU - Watson, A. W.
AU - Westerdale, S.
AU - Wilhelmi, J.
AU - Wojcik, M. M.
AU - Xiang, X.
AU - Xu, J.
AU - Yang, C.
AU - Yoo, J.
AU - Zavatarelli, S.
AU - Zec, A.
AU - Zhong, W.
AU - Zhu, C.
AU - Zuzel, G.
N1 - Funding Information: This report is based upon work supported by the US NSF (Grants PHY-0919363, PHY-1004072, PHY-1004054, PHY-1242585, PHY-1314483, PHY-1314507 and associated collaborative grants; Grants PHY-1211308 and PHY-1455351), the Italian Istituto Nazionale di Fisica Nucleare (INFN), the US DOE (Contract Nos. DE-FG02-91ER40671 and DE-AC02-07CH11359), the Polish NCN (Grant UMO-2012/05/E/ST2/02333), and the Russian Science Foundation Grant No 16-12-10369. We thank the staff of the Fermilab Particle Physics, Scientific and Core Computing Divisions for their support. We acknowledge the financial support from the UnivEarthS Labex program of Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02) and from the Sao Paulo Research Foundation (FAPESP).
PY - 2016/12/12
Y1 - 2016/12/12
N2 - DarkSide-50 is a detector for dark matter candidates in the form of weakly interacting massive particles. It utilizes a liquid argon time projection chamber for the inner main detector, surrounded by a liquid scintillator veto (LSV) and a water Cherenkov veto detector (WCV). The LSV and WCV act as the neutron and cosmogenic muon veto detectors for DarkSide-50. This paper describes the electronics and data acquisition system used for these two detectors. The system is made of a custom built front end electronics and commercial National Instruments high speed digitizers. The front end electronics, the DAQ, and the trigger system have been used to acquire data in the form of zero-suppressed waveform samples from the 110 PMTs of the LSV and the 80 PMTs of the WCV. The veto DAQ system has proven its performance and reliability. This electronics and DAQ system can be scaled and used as it is for the veto of the next generation DarkSide-20k detector.
AB - DarkSide-50 is a detector for dark matter candidates in the form of weakly interacting massive particles. It utilizes a liquid argon time projection chamber for the inner main detector, surrounded by a liquid scintillator veto (LSV) and a water Cherenkov veto detector (WCV). The LSV and WCV act as the neutron and cosmogenic muon veto detectors for DarkSide-50. This paper describes the electronics and data acquisition system used for these two detectors. The system is made of a custom built front end electronics and commercial National Instruments high speed digitizers. The front end electronics, the DAQ, and the trigger system have been used to acquire data in the form of zero-suppressed waveform samples from the 110 PMTs of the LSV and the 80 PMTs of the WCV. The veto DAQ system has proven its performance and reliability. This electronics and DAQ system can be scaled and used as it is for the veto of the next generation DarkSide-20k detector.
UR - http://www.scopus.com/inward/record.url?scp=85008219751&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85008219751&partnerID=8YFLogxK
U2 - 10.1088/1748-0221/11/12/P12007
DO - 10.1088/1748-0221/11/12/P12007
M3 - Article
AN - SCOPUS:85008219751
VL - 11
JO - Journal of Instrumentation
JF - Journal of Instrumentation
SN - 1748-0221
IS - 12
M1 - P12007
ER -