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The DarkSide awakens

Authors :
B. Bottino
R. Tartaglia
A. K. Alton
K. Randle
A. Vishneva
Mariano Cadoni
Denis Korablev
P. Cavalcante
P. J. Mosteiro
J. Brodsky
Michele Montuschi
L. Marini
M. Bossa
P. Saggese
I. N. Machulin
Samuele Sangiorgio
B. J. Mount
N. Rossi
L. Agostino
E. Pantic
A. M. Goretti
N. Canci
C. L. Kendziora
Irina James
B. Rossi
M. Orsini
D. Montanari
S. Catalanotti
Marco Pallavicini
D. D'Angelo
M. Cariello
E. Shields
A. G. Cocco
Jingke Xu
Alan Watson
A. Mandarano
P Trinchese
V. N. Muratova
K. Biery
Yanchu Wang
L. Pagani
K. Pelczar
Cristiano Galbiati
S. Perasso
M. D. Skorokhvatov
S. De Cecco
P. D. Meyers
S. Bussino
Nicomede Pelliccia
L. Grandi
K. Arisaka
G. Korga
C. Stanford
B. Vogelaar
G. Fiorillo
Anton Empl
B. Reinhold
M. M. Wojcik
Chung-Yao Yang
E. Edkins
Paolo Musico
A. V. Derbin
A. Razeto
J. Wilhelmi
A. Fan
M. Wada
Y. Guardincerri
D. A. Pugachev
M. D'Incecco
Anselmo Meregaglia
J. Yoo
M. Lissia
H. Qian
F. Gabriele
G. Zuzel
E. V. Hungerford
G. Testera
D. Sablone
A. Candela
O. Smirnov
M. Gromov
G. Di Pietro
Giovanni Covone
A. Sotnikov
Jim Napolitano
A. S. Kubankin
F. Di Eusanio
A. Tonazzo
S. Parmeggiano
J. Maricic
Aldo Romani
E. V. Unzhakov
P. Agnes
S. Walker
Yanhui Ma
C. Savarese
M. De Deo
W. Sands
Thomas Alexander
M. E. Monzani
Andrea Ianni
Sandra Zavatarelli
A. Pocar
M. Cadeddu
Xiujiang Li
D. Franco
Gioacchino Ranucci
K. Herner
T. Miletic
W. Zhong
Griffin Foster
R. Saldanha
J. Tatarowicz
D. A. Semenov
Caoxiang Zhu
H. Cao
S. Luitz
F. Granato
Cécile Jollet
Han Wang
A. Devoto
Y. Suvorov
S. Westerdale
B. Baldin
S. M. Mari
A. S. Chepurnov
S. Davini
Henning O. Back
S. D. Rountree
Paolo Lombardi
E. Segreto
A. Monte
V. V. Kobychev
B. R. Hackett
A. Brigatti
C. J. Martoff
G. Bonfini
K. J. Keeter
Frank Calaprice
X. Xiang
A. Zec
S. Pordes
R. Milincic
G. Koh
A. L. Renshaw
Aldo Ianni
M. Carlini
P. N. Singh
K. Fomenko
F. Budano
C. Giganti
Laura Cadonati
Fausto Ortica
Min-Xin Guan
M. De Vincenzi
Ivone F. M. Albuquerque
Davini, S.
Agnes, P.
Agostino, L.
M. Albuquerque, I. F.
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, Federico
Bussino, Severino Angelo Maria
Cadeddu, M.
Cadonati, L.
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.
D'Angelo, D.
D'Incecco, M.
De Cecco, S.
De Deo, M.
DE VINCENZI, Mario
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, Irina
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, Stefano Maria
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.
Orsini, M.
Ortica, F.
Pagani, L.
Pallavicini, M.
Pantic, E.
Parmeggiano, S.
Pelczar, K.
Pelliccia, N.
Perasso, S.
Pocar, A.
Pordes, S.
Pugachev, D. A.
Qian, H.
Randle, K.
Ranucci, G.
Razeto, A.
Reinhold, B.
Renshaw, A. L.
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, 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.
Gran Sasso Science Institute (GSSI)
Istituto Nazionale di Fisica Nucleare (INFN)
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585))
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Institut Pluridisciplinaire Hubert Curien (IPHC)
Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
DarkSide
Albuquerque, I. F. M.
Back, H.
Budano, F.
Bussino, S.
Catalanotti, Sergio
Cocco, ALFREDO GIUSEPPE
Covone, Giovanni
De Vincenzi, M.
Di Pietra, G.
Fiorillo, Giuliana
James, I.
Mari, S. M.
Muratova, N.
Walker, Susan Elizabeth
Source :
Journal of Physics: Conference Series, XIV International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015), XIV International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015), Sep 2015, Torino, Italy. pp.042016, ⟨10.1088/1742-6596/718/4/042016⟩
Publication Year :
2016

Abstract

International audience; The DarkSide program at LNGS aims to perform background-free WIMP searches using two phase liquid argon time projection chambers, with the ultimate goal of covering all parameters down to the so-called neutrino floor. One of the distinct features of the program is the use of underground argon with has a reduced content of the radioactive $^{39}$Ar compared to atmospheric argon. The DarkSide Collaboration is currently operating the DarkSide-50 experiment, the first such WIMP detector using underground argon. Operations with underground argon indicate a suppression of $^{39}$Ar by a factor (1.4 ± 0.2) × 10$^3$ relative to atmospheric argon. The new results obtained with DarkSide-50 and the plans for the next steps of the DarkSide program, the 20t fiducial mass DarkSide-20k detector and the 200 t fiducial Argo, are reviewed in this proceedings.

Details

Language :
English
Database :
OpenAIRE
Journal :
Journal of Physics: Conference Series, XIV International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015), XIV International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015), Sep 2015, Torino, Italy. pp.042016, ⟨10.1088/1742-6596/718/4/042016⟩
Accession number :
edsair.doi.dedup.....6757df23a8ae61e4368ffd957a16bff6
Full Text :
https://doi.org/10.1088/1742-6596/718/4/042016⟩