Status and perspective of the DarkSide experiment at LNGS

P. Agnes; L. Agostino; I. F.M. Albuquerque; T. Alexander; A. K. 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; 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. V. Derbin; A. Devoto; F. Di Eusanio; G. Di Pietro; C. Dionisi; E. Edkins; A. Empl; A. Fan; G. Fiorillo; K. Fomenko; D. Franco; F. Gabriele; C. Galbiati; S. Giagu; C. Giganti; G. K. Giovanetti; A. M. Goretti; F. Granato; M. Gromov; M. Guan; Y. Guardincerri; B. R. Hackett; K. Herner; D. Hughes; P. Humble; E. V. Hungerford; Al Ianni; An Ianni; I. James; T. N. Johnson; C. Jollet; K. Keeter; C. L. Kendziora; G. Koh; D. Korablev; G. Korga; A. Kubankin; X. Li; M. Lissia; B. Loer; P. Lombardi; G. Longo; Y. Ma; A. A. Machado; I. N. Machulin; A. Mandarano; S. M. Mari; J. Maricic; L. Marini; C. J. Martoff; A. Meregaglia; P. D. Meyers; R. Milincic; J. D. Miller; A. Monte; B. J. Mount; V. N. Muratova; P. Musico; J. Napolitano; A. Navrer Agasson; A. Oleinik; 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. L. Renshaw; M. Rescigno; Q. Riffard; A. Romani; B. Rossi; N. Rossi; D. Sablone; P. Saggese; W. Sands; C. Savarese; B. Schlitzer; E. Segreto; D. A. Semenov; P. N. Singh; M. D. Skorokhvatov; O. Smirnov; A. Sotnikov; C. Stanford; Y. Suvorov; R. Tartaglia; G. Testera; A. Tonazzo; P. Trinchese; E. V. Unzhakov; M. Verducci; A. Vishneva; B. Vogelaar; M. Wada; S. Walker; H. Wang; Y. Wang; A. W. Watson; S. Westerdale; J. Wilhelmi; M. M. Wojcik; X. Xiang; X. Xiao; J. Xu; C. Yang; Z. Ye; W. Zhong; C. Zhu; G. Zuzel

doi:10.1393/ncc/i2017-17164-8

Status and perspective of the DarkSide experiment at LNGS

P. Agnes, L. Agostino, I. F.M. Albuquerque, T. Alexander, A. K. 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, M. CadoniF. 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. V. Derbin, A. Devoto, F. Di Eusanio, G. Di Pietro, C. Dionisi, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, D. Franco, F. Gabriele, C. Galbiati, S. Giagu, C. Giganti, G. K. Giovanetti, A. M. Goretti, F. Granato, M. Gromov, M. Guan, Y. Guardincerri, B. R. Hackett, K. Herner, D. Hughes, P. Humble, E. V. Hungerford, Al Ianni, An Ianni, I. James, T. N. Johnson, C. Jollet, K. Keeter, C. L. Kendziora, G. Koh, D. Korablev, G. Korga, A. Kubankin, X. Li, M. Lissia, B. Loer, P. Lombardi, G. Longo, Y. Ma, A. A. Machado, I. N. Machulin, A. Mandarano, S. M. Mari, J. Maricic, L. Marini, C. J. Martoff, A. Meregaglia, P. D. Meyers, R. Milincic, J. D. Miller, A. Monte, B. J. Mount, V. N. Muratova, P. Musico, J. Napolitano, A. Navrer Agasson, A. Oleinik, 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. L. Renshaw, M. Rescigno, Q. Riffard, A. Romani, B. Rossi, N. Rossi, D. Sablone, P. Saggese, W. Sands, C. Savarese, B. Schlitzer, E. Segreto, D. A. Semenov, P. N. Singh, M. D. Skorokhvatov, O. Smirnov, A. Sotnikov, C. Stanford, Y. Suvorov, R. Tartaglia, G. Testera, A. Tonazzo, P. Trinchese, E. V. Unzhakov, M. Verducci, A. Vishneva, B. Vogelaar, M. Wada, S. Walker, H. Wang, Y. Wang, A. W. Watson, S. Westerdale, J. Wilhelmi, M. M. Wojcik, X. Xiang, X. Xiao, J. Xu, C. Yang, Z. Ye, W. Zhong, C. Zhu, G. Zuzel

Research output: Contribution to journal › Article › peer-review

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Abstract

The DarkSide experiment aims to perform a background-free direct search for dark matter with a dual-phase argon TPC. The current phase of the experiment, DarkSide-50, is acquiring data at Laboratori Nazionali del Gran Sasso and produced the most sensitive limit on the WIMP-nucleon cross section ever obtained with a liquid argon target (2.0 × 10^-44 cm² for a WIMP mass of 100 GeV/c²). The future phase of the experiment will be a 20 t fiducial mass detector, designed to reach a sensitivity of ∼ 1 × 10^-47 cm² (at 1 TeV/c² WIMP mass) with a background-free exposure of 100 ty. This work contains a discussion of the current status of the DarkSide-50 WIMP search and of the results which are more relevant for the construction of the future detector.

Original language	English (US)
Article number	164
Journal	Nuovo Cimento della Societa Italiana di Fisica C
Volume	40
Issue number	5
DOIs	https://doi.org/10.1393/ncc/i2017-17164-8
State	Published - Sep 1 2017

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Physics and Astronomy (miscellaneous)

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10.1393/ncc/i2017-17164-8

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Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Asner, D. M., Back, H. O., Baldin, B., Biery, K., Bocci, V., Bonfini, G., Bonivento, W., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., ... Zuzel, G. (2017). Status and perspective of the DarkSide experiment at LNGS. Nuovo Cimento della Societa Italiana di Fisica C, 40(5), Article 164. https://doi.org/10.1393/ncc/i2017-17164-8

@article{fa7dba2a559d4c74a471d5284160e318,

title = "Status and perspective of the DarkSide experiment at LNGS",

abstract = "The DarkSide experiment aims to perform a background-free direct search for dark matter with a dual-phase argon TPC. The current phase of the experiment, DarkSide-50, is acquiring data at Laboratori Nazionali del Gran Sasso and produced the most sensitive limit on the WIMP-nucleon cross section ever obtained with a liquid argon target (2.0 × 10-44 cm2 for a WIMP mass of 100 GeV/c2). The future phase of the experiment will be a 20 t fiducial mass detector, designed to reach a sensitivity of ∼ 1 × 10-47 cm2 (at 1 TeV/c2 WIMP mass) with a background-free exposure of 100 ty. This work contains a discussion of the current status of the DarkSide-50 WIMP search and of the results which are more relevant for the construction of the future detector.",

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

year = "2017",

month = sep,

day = "1",

doi = "10.1393/ncc/i2017-17164-8",

language = "English (US)",

volume = "40",

journal = "Nuovo Cimento della Societa Italiana di Fisica C",

issn = "2037-4909",

publisher = "Societa Italiana di Fisica",

number = "5",

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Agnes, P, Agostino, L, Albuquerque, IFM, Alexander, T, Alton, AK, Asner, DM, Back, HO, Baldin, B, Biery, K, Bocci, V, Bonfini, G, Bonivento, W, Bossa, M, Bottino, B, Brigatti, A, Brodsky, J, Budano, F, Bussino, S, Cadeddu, M, Cadoni, M, Calaprice, F, Canci, N, Candela, A, Caravati, M, Cariello, M, Carlini, M, Catalanotti, S, Cavalcante, P, Chepurnov, A, Cicalò, C, Cocco, AG, Covone, G, D'Angelo, D, D'Incecco, M, Davini, S, De Cecco, S, De Deo, M, De Vincenzi, M, Derbin, AV, Devoto, A, Di Eusanio, F, Di Pietro, G, Dionisi, C, Edkins, E, Empl, A, Fan, A, Fiorillo, G, Fomenko, K, Franco, D, Gabriele, F, Galbiati, C, Giagu, S, Giganti, C, Giovanetti, GK, Goretti, AM, Granato, F, Gromov, M, Guan, M, Guardincerri, Y, Hackett, BR, Herner, K, Hughes, D, Humble, P, Hungerford, EV, Ianni, A, Ianni, A, James, I, Johnson, TN, Jollet, C, Keeter, K, Kendziora, CL, Koh, G, Korablev, D, Korga, G, Kubankin, A, Li, X, Lissia, M, Loer, B, Lombardi, P, Longo, G, Ma, Y, Machado, AA, Machulin, IN, Mandarano, A, Mari, SM, Maricic, J, Marini, L, Martoff, CJ, Meregaglia, A, Meyers, PD, Milincic, R, Miller, JD, Monte, A, Mount, BJ, Muratova, VN, Musico, P, Napolitano, J, Navrer Agasson, A, Oleinik, A, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pantic, E, Parmeggiano, S, Pelczar, K, Pelliccia, N, Pocar, A, Pordes, S, Pugachev, DA, Qian, H, Randle, K, Ranucci, G, Razeti, M, Razeto, A, Reinhold, B, Renshaw, AL, Rescigno, M, Riffard, Q, Romani, A, Rossi, B, Rossi, N, Sablone, D, Saggese, P, Sands, W, Savarese, C, Schlitzer, B, Segreto, E, Semenov, DA, Singh, PN, Skorokhvatov, MD, Smirnov, O, Sotnikov, A, Stanford, C, Suvorov, Y, Tartaglia, R, Testera, G, Tonazzo, A, Trinchese, P, Unzhakov, EV, Verducci, M, Vishneva, A, Vogelaar, B, Wada, M, Walker, S, Wang, H, Wang, Y, Watson, AW, Westerdale, S, Wilhelmi, J, Wojcik, MM, Xiang, X, Xiao, X, Xu, J, Yang, C, Ye, Z, Zhong, W, Zhu, C & Zuzel, G 2017, 'Status and perspective of the DarkSide experiment at LNGS', Nuovo Cimento della Societa Italiana di Fisica C, vol. 40, no. 5, 164. https://doi.org/10.1393/ncc/i2017-17164-8

TY - JOUR

T1 - Status and perspective of the DarkSide experiment at LNGS

AU - Agnes, P.

AU - Agostino, L.

AU - Albuquerque, I. F.M.

AU - Alexander, T.

AU - Alton, A. K.

AU - Asner, D. M.

AU - Back, H. O.

AU - Baldin, B.

AU - Biery, K.

AU - Bocci, V.

AU - Bonfini, G.

AU - Bonivento, W.

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 - Caravati, M.

AU - Cariello, M.

AU - Carlini, M.

AU - Catalanotti, S.

AU - Cavalcante, P.

AU - Chepurnov, A.

AU - Cicalò, C.

AU - Cocco, A. G.

AU - Covone, G.

AU - D'Angelo, D.

AU - D'Incecco, M.

AU - Davini, S.

AU - De Cecco, S.

AU - De Deo, M.

AU - De Vincenzi, M.

AU - Derbin, A. V.

AU - Devoto, A.

AU - Di Eusanio, F.

AU - Di Pietro, G.

AU - Dionisi, C.

AU - Edkins, E.

AU - Empl, A.

AU - Fan, A.

AU - Fiorillo, G.

AU - Fomenko, K.

AU - Franco, D.

AU - Gabriele, F.

AU - Galbiati, C.

AU - Giagu, S.

AU - Giganti, C.

AU - Giovanetti, G. K.

AU - Goretti, A. M.

AU - Granato, F.

AU - Gromov, M.

AU - Guan, M.

AU - Guardincerri, Y.

AU - Hackett, B. R.

AU - Herner, K.

AU - Hughes, D.

AU - Humble, P.

AU - Hungerford, E. V.

AU - Ianni, Al

AU - Ianni, An

AU - James, I.

AU - Johnson, T. N.

AU - Jollet, C.

AU - Keeter, K.

AU - Kendziora, C. L.

AU - Koh, G.

AU - Korablev, D.

AU - Korga, G.

AU - Kubankin, A.

AU - Li, X.

AU - Lissia, M.

AU - Loer, B.

AU - Lombardi, P.

AU - Longo, G.

AU - Ma, Y.

AU - Machado, A. A.

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 - Milincic, R.

AU - Miller, J. D.

AU - Monte, A.

AU - Mount, B. J.

AU - Muratova, V. N.

AU - Musico, P.

AU - Napolitano, J.

AU - Navrer Agasson, A.

AU - Oleinik, A.

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 - Razeti, M.

AU - Razeto, A.

AU - Reinhold, B.

AU - Renshaw, A. L.

AU - Rescigno, M.

AU - Riffard, Q.

AU - Romani, A.

AU - Rossi, B.

AU - Rossi, N.

AU - Sablone, D.

AU - Saggese, P.

AU - Sands, W.

AU - Savarese, C.

AU - Schlitzer, B.

AU - Segreto, E.

AU - Semenov, D. A.

AU - Singh, P. N.

AU - Skorokhvatov, M. D.

AU - Smirnov, O.

AU - Sotnikov, A.

AU - Stanford, C.

AU - Suvorov, Y.

AU - Tartaglia, R.

AU - Testera, G.

AU - Tonazzo, A.

AU - Trinchese, P.

AU - Unzhakov, E. V.

AU - Verducci, M.

AU - Vishneva, A.

AU - Vogelaar, 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 - Xiao, X.

AU - Xu, J.

AU - Yang, C.

AU - Ye, Z.

AU - Zhong, W.

AU - Zhu, C.

AU - Zuzel, G.

PY - 2017/9/1

Y1 - 2017/9/1

N2 - The DarkSide experiment aims to perform a background-free direct search for dark matter with a dual-phase argon TPC. The current phase of the experiment, DarkSide-50, is acquiring data at Laboratori Nazionali del Gran Sasso and produced the most sensitive limit on the WIMP-nucleon cross section ever obtained with a liquid argon target (2.0 × 10-44 cm2 for a WIMP mass of 100 GeV/c2). The future phase of the experiment will be a 20 t fiducial mass detector, designed to reach a sensitivity of ∼ 1 × 10-47 cm2 (at 1 TeV/c2 WIMP mass) with a background-free exposure of 100 ty. This work contains a discussion of the current status of the DarkSide-50 WIMP search and of the results which are more relevant for the construction of the future detector.

AB - The DarkSide experiment aims to perform a background-free direct search for dark matter with a dual-phase argon TPC. The current phase of the experiment, DarkSide-50, is acquiring data at Laboratori Nazionali del Gran Sasso and produced the most sensitive limit on the WIMP-nucleon cross section ever obtained with a liquid argon target (2.0 × 10-44 cm2 for a WIMP mass of 100 GeV/c2). The future phase of the experiment will be a 20 t fiducial mass detector, designed to reach a sensitivity of ∼ 1 × 10-47 cm2 (at 1 TeV/c2 WIMP mass) with a background-free exposure of 100 ty. This work contains a discussion of the current status of the DarkSide-50 WIMP search and of the results which are more relevant for the construction of the future detector.

UR - https://www.scopus.com/pages/publications/85038955421

UR - https://www.scopus.com/inward/citedby.url?scp=85038955421&partnerID=8YFLogxK

U2 - 10.1393/ncc/i2017-17164-8

DO - 10.1393/ncc/i2017-17164-8

M3 - Article

AN - SCOPUS:85038955421

SN - 2037-4909

VL - 40

JO - Nuovo Cimento della Societa Italiana di Fisica C

JF - Nuovo Cimento della Societa Italiana di Fisica C

IS - 5

M1 - 164

ER -

Status and perspective of the DarkSide experiment at LNGS

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