DarkSide

Bianca Bottino; M. Bossa; A. Mandarano; C. Savarese; A. Razeto; G. Bonfini; A. Candela; M. Carlini; P. Cavalcante; M. De Deo; M. D'Incecco; F. Gabriele; A. M. Goretti; A. Ianni; M. Orsini; N. Rossi; D. Sablone; R. Tartaglia; M. Pallavicini; G. Testera; M. Cariello; L. Marini; P. Musico; L. Pagani; S. Davini; S. M. Mari; F. Budano; S. Bussino; M. De Vincenzi; I. James; G. Fiorillo; S. Catalanotti; A. G. Cocco; G. Covone; F. Granato; B. Rossi; P. Trinchese; S. Walker; A. Devoto; M. Cadeddu; M. Cadoni; M. Lissia; G. Ranucci; A. Brigatti; D. D'Angelo; P. Lombardi; S. Parmeggiano; P. Saggese; D. Franco; P. Agnes; A. Tonazzo; S. De Cecco; C. Giganti; C. Galbiati; P. D. Meyers; I. F.M. Albuquerque; J. Brodsky; H. Cao; F. Calaprice; G. Koh; X. Li; H. Qian; W. Sands; E. Shields; C. Stanford; M. Wada; S. Westerdale; X. Xiang; J. Xu; C. Zhu; S. Pordes; K. Biery; G. Forster; K. Herner; Y. Guardincerri; C. L. Kendziora; J. Yoo; H. Wang; A. Fan; Y. Suvorov; A. Pocar; A. Monte; K. Randle; J. Maricic; E. Edkins; B. R. Hackett; R. Milincic; B. Reinhold; E. V. Hungerford; A. L. Renshaw; N. Canci; A. Empl; G. Korga; P. N. Singh; C. J. Martoff; J. Napolitano; T. Miletic; A. W. Watson; E. Pantic; T. Johnson; A. Chepurnov; M. Gromov; O. Smirnov; K. Fomenko; D. Korablev; A. Sotnikov; A. Wishneva; M. M. Wojcik; K. Pelczar; G. Zuzel; A. Derbin; V. N. Muratova; D. A. Semenov; E. V. Unzhakov

DarkSide

Bianca Bottino, M. Bossa, A. Mandarano, C. Savarese, A. Razeto, G. Bonfini, A. Candela, M. Carlini, P. Cavalcante, M. De Deo, M. D'Incecco, F. Gabriele, A. M. Goretti, A. Ianni, M. Orsini, N. Rossi, D. Sablone, R. Tartaglia, M. Pallavicini, G. TesteraM. Cariello, L. Marini, P. Musico, L. Pagani, S. Davini, S. M. Mari, F. Budano, S. Bussino, M. De Vincenzi, I. James, G. Fiorillo, S. Catalanotti, A. G. Cocco, G. Covone, F. Granato, B. Rossi, P. Trinchese, S. Walker, A. Devoto, M. Cadeddu, M. Cadoni, M. Lissia, G. Ranucci, A. Brigatti, D. D'Angelo, P. Lombardi, S. Parmeggiano, P. Saggese, D. Franco, P. Agnes, A. Tonazzo, S. De Cecco, C. Giganti, C. Galbiati, P. D. Meyers, I. F.M. Albuquerque, J. Brodsky, H. Cao, F. Calaprice, G. Koh, X. Li, H. Qian, W. Sands, E. Shields, C. Stanford, M. Wada, S. Westerdale, X. Xiang, J. Xu, C. Zhu, S. Pordes, K. Biery, G. Forster, K. Herner, Y. Guardincerri, C. L. Kendziora, J. Yoo, H. Wang, A. Fan, Y. Suvorov, A. Pocar, A. Monte, K. Randle, J. Maricic, E. Edkins, B. R. Hackett, R. Milincic, B. Reinhold, E. V. Hungerford, A. L. Renshaw, N. Canci, A. Empl, G. Korga, P. N. Singh, C. J. Martoff, J. Napolitano, T. Miletic, A. W. Watson, E. Pantic, T. Johnson, A. Chepurnov, M. Gromov, O. Smirnov, K. Fomenko, D. Korablev, A. Sotnikov, A. Wishneva, M. M. Wojcik, K. Pelczar, G. Zuzel, A. Derbin, V. N. Muratova, D. A. Semenov, E. V. Unzhakov

Research output: Contribution to journal › Conference article › peer-review

Abstract

The DarkSide project at Laboratori Nazionali del Gran Sasso (LNGS) is a dark matter direct search experiment based on the detection of rare nuclear recoils possibly induced by hypothetical dark matter particles, which are supposed to be neutral, massive (> 10 GeV) and weakly interacting (WIMP). DarkSide aims to perform background-free WIMP searches using a series of dual-phase liquid argon time projection chambers filled with ultra-pure liquid argon. The detector currently operating at LNGS is DarkSide-50, a detector which holds 46 kg of active liquid argon and is now filled with argon extracted from underground and taking data in its final configuration. Combining the underground argon data with the preceding search made with atmospheric argon, a 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section of 2.0 x 10∼⁴⁴ cm² is set. The next phase of the experiment foresees the construction of a new detector with an active mass of ∼ 20 and equipped with silicon photomultipliers, called DarkSide-20k.

Original language	English (US)
Article number	087
Journal	Proceedings of Science
State	Published - 2016
Event	9th Neutrino Oscillation Workshop, NOW 2016 - Otranto, Lecce, Italy Duration: Sep 4 2016 → Sep 11 2016

All Science Journal Classification (ASJC) codes

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@article{b370911958a544da9ce43634ea80ab9b,

title = "DarkSide",

abstract = "The DarkSide project at Laboratori Nazionali del Gran Sasso (LNGS) is a dark matter direct search experiment based on the detection of rare nuclear recoils possibly induced by hypothetical dark matter particles, which are supposed to be neutral, massive (> 10 GeV) and weakly interacting (WIMP). DarkSide aims to perform background-free WIMP searches using a series of dual-phase liquid argon time projection chambers filled with ultra-pure liquid argon. The detector currently operating at LNGS is DarkSide-50, a detector which holds 46 kg of active liquid argon and is now filled with argon extracted from underground and taking data in its final configuration. Combining the underground argon data with the preceding search made with atmospheric argon, a 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section of 2.0 x 10∼44 cm2 is set. The next phase of the experiment foresees the construction of a new detector with an active mass of ∼ 20 and equipped with silicon photomultipliers, called DarkSide-20k.",

author = "Bianca Bottino and M. Bossa and A. Mandarano and C. Savarese and A. Razeto and G. Bonfini and A. Candela and M. Carlini and P. Cavalcante and {De Deo}, M. and M. D'Incecco and F. Gabriele and Goretti, {A. M.} and A. Ianni and M. Orsini and N. Rossi and D. Sablone and R. Tartaglia and M. Pallavicini and G. Testera and M. Cariello and L. Marini and P. Musico and L. Pagani and S. Davini and Mari, {S. M.} and F. Budano and S. Bussino and {De Vincenzi}, M. and I. James and G. Fiorillo and S. Catalanotti and Cocco, {A. G.} and G. Covone and F. Granato and B. Rossi and P. Trinchese and S. Walker and A. Devoto and M. Cadeddu and M. Cadoni and M. Lissia and G. Ranucci and A. Brigatti and D. D'Angelo and P. Lombardi and S. Parmeggiano and P. Saggese and D. Franco and P. Agnes and A. Tonazzo and {De Cecco}, S. and C. Giganti and C. Galbiati and Meyers, {P. D.} and Albuquerque, {I. F.M.} and J. Brodsky and H. Cao and F. Calaprice and G. Koh and X. Li and H. Qian and W. Sands and E. Shields and C. Stanford and M. Wada and S. Westerdale and X. Xiang and J. Xu and C. Zhu and S. Pordes and K. Biery and G. Forster and K. Herner and Y. Guardincerri and Kendziora, {C. L.} and J. Yoo and H. Wang and A. Fan and Y. Suvorov and A. Pocar and A. Monte and K. Randle and J. Maricic and E. Edkins and Hackett, {B. R.} and R. Milincic and B. Reinhold and Hungerford, {E. V.} and Renshaw, {A. L.} and N. Canci and A. Empl and G. Korga and Singh, {P. N.} and Martoff, {C. J.} and J. Napolitano and T. Miletic and Watson, {A. W.} and E. Pantic and T. Johnson and A. Chepurnov and M. Gromov and O. Smirnov and K. Fomenko and D. Korablev and A. Sotnikov and A. Wishneva and Wojcik, {M. M.} and K. Pelczar and G. Zuzel and A. Derbin and Muratova, {V. N.} and Semenov, {D. A.} and Unzhakov, {E. V.}",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).; 9th Neutrino Oscillation Workshop, NOW 2016 ; Conference date: 04-09-2016 Through 11-09-2016",

year = "2016",

language = "English (US)",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Bottino, B, Bossa, M, Mandarano, A, Savarese, C, Razeto, A, Bonfini, G, Candela, A, Carlini, M, Cavalcante, P, De Deo, M, D'Incecco, M, Gabriele, F, Goretti, AM, Ianni, A, Orsini, M, Rossi, N, Sablone, D, Tartaglia, R, Pallavicini, M, Testera, G, Cariello, M, Marini, L, Musico, P, Pagani, L, Davini, S, Mari, SM, Budano, F, Bussino, S, De Vincenzi, M, James, I, Fiorillo, G, Catalanotti, S, Cocco, AG, Covone, G, Granato, F, Rossi, B, Trinchese, P, Walker, S, Devoto, A, Cadeddu, M, Cadoni, M, Lissia, M, Ranucci, G, Brigatti, A, D'Angelo, D, Lombardi, P, Parmeggiano, S, Saggese, P, Franco, D, Agnes, P, Tonazzo, A, De Cecco, S, Giganti, C, Galbiati, C, Meyers, PD, Albuquerque, IFM, Brodsky, J, Cao, H, Calaprice, F, Koh, G, Li, X, Qian, H, Sands, W, Shields, E, Stanford, C, Wada, M, Westerdale, S, Xiang, X, Xu, J, Zhu, C, Pordes, S, Biery, K, Forster, G, Herner, K, Guardincerri, Y, Kendziora, CL, Yoo, J, Wang, H, Fan, A, Suvorov, Y, Pocar, A, Monte, A, Randle, K, Maricic, J, Edkins, E, Hackett, BR, Milincic, R, Reinhold, B, Hungerford, EV, Renshaw, AL, Canci, N, Empl, A, Korga, G, Singh, PN, Martoff, CJ, Napolitano, J, Miletic, T, Watson, AW, Pantic, E, Johnson, T, Chepurnov, A, Gromov, M, Smirnov, O, Fomenko, K, Korablev, D, Sotnikov, A, Wishneva, A, Wojcik, MM, Pelczar, K, Zuzel, G, Derbin, A, Muratova, VN, Semenov, DA & Unzhakov, EV 2016, 'DarkSide', Proceedings of Science.

TY - JOUR

T1 - DarkSide

AU - Bottino, Bianca

AU - Bossa, M.

AU - Mandarano, A.

AU - Savarese, C.

AU - Razeto, A.

AU - Bonfini, G.

AU - Candela, A.

AU - Carlini, M.

AU - Cavalcante, P.

AU - De Deo, M.

AU - D'Incecco, M.

AU - Gabriele, F.

AU - Goretti, A. M.

AU - Ianni, A.

AU - Orsini, M.

AU - Rossi, N.

AU - Sablone, D.

AU - Tartaglia, R.

AU - Pallavicini, M.

AU - Testera, G.

AU - Cariello, M.

AU - Marini, L.

AU - Musico, P.

AU - Pagani, L.

AU - Davini, S.

AU - Mari, S. M.

AU - Budano, F.

AU - Bussino, S.

AU - De Vincenzi, M.

AU - James, I.

AU - Fiorillo, G.

AU - Catalanotti, S.

AU - Cocco, A. G.

AU - Covone, G.

AU - Granato, F.

AU - Rossi, B.

AU - Trinchese, P.

AU - Walker, S.

AU - Devoto, A.

AU - Cadeddu, M.

AU - Cadoni, M.

AU - Lissia, M.

AU - Ranucci, G.

AU - Brigatti, A.

AU - D'Angelo, D.

AU - Lombardi, P.

AU - Parmeggiano, S.

AU - Saggese, P.

AU - Franco, D.

AU - Agnes, P.

AU - Tonazzo, A.

AU - De Cecco, S.

AU - Giganti, C.

AU - Galbiati, C.

AU - Meyers, P. D.

AU - Albuquerque, I. F.M.

AU - Brodsky, J.

AU - Cao, H.

AU - Calaprice, F.

AU - Koh, G.

AU - Li, X.

AU - Qian, H.

AU - Sands, W.

AU - Shields, E.

AU - Stanford, C.

AU - Wada, M.

AU - Westerdale, S.

AU - Xiang, X.

AU - Xu, J.

AU - Zhu, C.

AU - Pordes, S.

AU - Biery, K.

AU - Forster, G.

AU - Herner, K.

AU - Guardincerri, Y.

AU - Kendziora, C. L.

AU - Yoo, J.

AU - Wang, H.

AU - Fan, A.

AU - Suvorov, Y.

AU - Pocar, A.

AU - Monte, A.

AU - Randle, K.

AU - Maricic, J.

AU - Edkins, E.

AU - Hackett, B. R.

AU - Milincic, R.

AU - Reinhold, B.

AU - Hungerford, E. V.

AU - Renshaw, A. L.

AU - Canci, N.

AU - Empl, A.

AU - Korga, G.

AU - Singh, P. N.

AU - Martoff, C. J.

AU - Napolitano, J.

AU - Miletic, T.

AU - Watson, A. W.

AU - Pantic, E.

AU - Johnson, T.

AU - Chepurnov, A.

AU - Gromov, M.

AU - Smirnov, O.

AU - Fomenko, K.

AU - Korablev, D.

AU - Sotnikov, A.

AU - Wishneva, A.

AU - Wojcik, M. M.

AU - Pelczar, K.

AU - Zuzel, G.

AU - Derbin, A.

AU - Muratova, V. N.

AU - Semenov, D. A.

AU - Unzhakov, E. V.

N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).

PY - 2016

Y1 - 2016

N2 - The DarkSide project at Laboratori Nazionali del Gran Sasso (LNGS) is a dark matter direct search experiment based on the detection of rare nuclear recoils possibly induced by hypothetical dark matter particles, which are supposed to be neutral, massive (> 10 GeV) and weakly interacting (WIMP). DarkSide aims to perform background-free WIMP searches using a series of dual-phase liquid argon time projection chambers filled with ultra-pure liquid argon. The detector currently operating at LNGS is DarkSide-50, a detector which holds 46 kg of active liquid argon and is now filled with argon extracted from underground and taking data in its final configuration. Combining the underground argon data with the preceding search made with atmospheric argon, a 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section of 2.0 x 10∼44 cm2 is set. The next phase of the experiment foresees the construction of a new detector with an active mass of ∼ 20 and equipped with silicon photomultipliers, called DarkSide-20k.

AB - The DarkSide project at Laboratori Nazionali del Gran Sasso (LNGS) is a dark matter direct search experiment based on the detection of rare nuclear recoils possibly induced by hypothetical dark matter particles, which are supposed to be neutral, massive (> 10 GeV) and weakly interacting (WIMP). DarkSide aims to perform background-free WIMP searches using a series of dual-phase liquid argon time projection chambers filled with ultra-pure liquid argon. The detector currently operating at LNGS is DarkSide-50, a detector which holds 46 kg of active liquid argon and is now filled with argon extracted from underground and taking data in its final configuration. Combining the underground argon data with the preceding search made with atmospheric argon, a 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section of 2.0 x 10∼44 cm2 is set. The next phase of the experiment foresees the construction of a new detector with an active mass of ∼ 20 and equipped with silicon photomultipliers, called DarkSide-20k.

UR - http://www.scopus.com/inward/record.url?scp=85045527366&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85045527366&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85045527366

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 087

T2 - 9th Neutrino Oscillation Workshop, NOW 2016

Y2 - 4 September 2016 through 11 September 2016

ER -

DarkSide

Abstract

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