Simulation of argon response and light detection in the DarkSide-50 dual phase TPC

P. Agnes; I. F.M. Albuquerque; T. Alexander; A. K. Alton; D. M. Asner; H. O. Back; K. Biery; V. Bocci; G. Bonfini; W. Bonivento; M. Bossa; B. Bottino; F. Budano; S. Bussino; M. Cadeddu; M. Cadoni; F. Calaprice; N. Canci; A. Candela; M. Caravati; M. Cariello; M. Carlini; S. Catalanotti; V. Cataudella; P. Cavalcante; A. Chepurnov; C. Cicalò; A. G. Cocco; G. Covone; D. D'Angelo; M. D'Incecco; S. Davini; A. De Candia; S. De Cecco; M. De Deo; G. De Filippis; M. De Vincenzi; A. V. Derbin; G. De Rosa; 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; An Ianni; I. James; T. N. Johnson; K. Keeter; C. L. Kendziora; G. Koh; D. Korablev; G. Korga; A. Kubankin; X. Li; M. Lissia; B. Loer; G. Longo; Y. Ma; A. A. Machado; I. N. Machulin; A. Mandarano; S. M. Mari; J. Maricic; C. J. Martoff; P. D. Meyers; R. Milincic; 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; K. Pelczar; N. Pelliccia; A. Pocar; S. Pordes; D. A. Pugachev; H. Qian; K. Randle; M. Razeti; A. Razeto; B. Reinhold; A. L. Renshaw; M. Rescigno; Q. Riffard; A. Romani; B. Rossi; N. Rossi; D. Sablone; W. Sands; S. Sanfilippo; 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; C. Yang; Z. Ye; C. Zhu; G. Zuzel

doi:10.1088/1748-0221/12/10/P10015

Simulation of argon response and light detection in the DarkSide-50 dual phase TPC

P. Agnes, I. F.M. Albuquerque, T. Alexander, A. K. Alton, D. M. Asner, H. O. Back, K. Biery, V. Bocci, G. Bonfini, W. Bonivento, M. Bossa, B. Bottino, F. Budano, S. Bussino, M. Cadeddu, M. Cadoni, F. Calaprice, N. Canci, A. Candela, M. CaravatiM. Cariello, M. Carlini, S. Catalanotti, V. Cataudella, P. Cavalcante, A. Chepurnov, C. Cicalò, A. G. Cocco, G. Covone, D. D'Angelo, M. D'Incecco, S. Davini, A. De Candia, S. De Cecco, M. De Deo, G. De Filippis, M. De Vincenzi, A. V. Derbin, G. De Rosa, 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, An Ianni, I. James, T. N. Johnson, K. Keeter, C. L. Kendziora, G. Koh, D. Korablev, G. Korga, A. Kubankin, X. Li, M. Lissia, B. Loer, G. Longo, Y. Ma, A. A. Machado, I. N. Machulin, A. Mandarano, S. M. Mari, J. Maricic, C. J. Martoff, P. D. Meyers, R. Milincic, 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, K. Pelczar, N. Pelliccia, A. Pocar, S. Pordes, D. A. Pugachev, H. Qian, K. Randle, M. Razeti, A. Razeto, B. Reinhold, A. L. Renshaw, M. Rescigno, Q. Riffard, A. Romani, B. Rossi, N. Rossi, D. Sablone, W. Sands, S. Sanfilippo, 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, C. Yang, Z. Ye, C. Zhu, G. Zuzel

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

30 Scopus citations

Abstract

A Geant4-based Monte Carlo package named G4DS has been developed to simulate the response of DarkSide-50, an experiment operating since 2013 at LNGS, designed to detect WIMP interactions in liquid argon. In the process of WIMP searches, DarkSide-50 has achieved two fundamental milestones: the rejection of electron recoil background with a power of ∼10⁷, using the pulse shape discrimination technique, and the measurement of the residual ³⁹Ar contamination in underground argon, ∼3 orders of magnitude lower with respect to atmospheric argon. These results rely on the accurate simulation of the detector response to the liquid argon scintillation, its ionization, and electron-ion recombination processes. This work provides a complete overview of the DarkSide Monte Carlo and of its performance, with a particular focus on PARIS, the custom-made liquid argon response model.

Original language	English (US)
Article number	P10015
Journal	Journal of Instrumentation
Volume	12
Issue number	10
DOIs	https://doi.org/10.1088/1748-0221/12/10/P10015
State	Published - Oct 23 2017

All Science Journal Classification (ASJC) codes

Instrumentation
Mathematical Physics

Keywords

Dark Matter detectors (WIMPs, axions, etc.)
Detector modelling and simulations I (interaction of radiation with matter, interaction of photons with matter, interaction of hadrons with matter, etc)
Ionization and excitation processes
Noble liquid detectors (scintillation, ionization, double-phase)

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10.1088/1748-0221/12/10/P10015

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Agnes, P., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Asner, D. M., Back, H. O., Biery, K., Bocci, V., Bonfini, G., Bonivento, W., Bossa, M., Bottino, B., Budano, F., Bussino, S., Cadeddu, M., Cadoni, M., Calaprice, F., Canci, N., Candela, A., ... Zuzel, G. (2017). Simulation of argon response and light detection in the DarkSide-50 dual phase TPC. Journal of Instrumentation, 12(10), Article P10015. https://doi.org/10.1088/1748-0221/12/10/P10015

@article{e578874f1c7e40838880904cf8f10edd,

title = "Simulation of argon response and light detection in the DarkSide-50 dual phase TPC",

abstract = "A Geant4-based Monte Carlo package named G4DS has been developed to simulate the response of DarkSide-50, an experiment operating since 2013 at LNGS, designed to detect WIMP interactions in liquid argon. In the process of WIMP searches, DarkSide-50 has achieved two fundamental milestones: the rejection of electron recoil background with a power of ∼107, using the pulse shape discrimination technique, and the measurement of the residual 39Ar contamination in underground argon, ∼3 orders of magnitude lower with respect to atmospheric argon. These results rely on the accurate simulation of the detector response to the liquid argon scintillation, its ionization, and electron-ion recombination processes. This work provides a complete overview of the DarkSide Monte Carlo and of its performance, with a particular focus on PARIS, the custom-made liquid argon response model.",

keywords = "Dark Matter detectors (WIMPs, axions, etc.), Detector modelling and simulations I (interaction of radiation with matter, interaction of photons with matter, interaction of hadrons with matter, etc), Ionization and excitation processes, Noble liquid detectors (scintillation, ionization, double-phase)",

author = "P. Agnes and Albuquerque, {I. F.M.} and T. Alexander and Alton, {A. K.} and Asner, {D. M.} and Back, {H. O.} and K. Biery and V. Bocci and G. Bonfini and W. Bonivento and M. Bossa and B. Bottino 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 V. Cataudella 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 Candia}, A. and {De Cecco}, S. and {De Deo}, M. and {De Filippis}, G. and {De Vincenzi}, M. and Derbin, {A. V.} and {De Rosa}, G. 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 An Ianni and I. James and Johnson, {T. N.} 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 G. Longo and Y. Ma and Machado, {A. A.} and Machulin, {I. N.} and A. Mandarano and Mari, {S. M.} and J. Maricic and Martoff, {C. J.} and Meyers, {P. D.} and R. Milincic and A. Monte and Mount, {B. J.} and Muratova, {V. N.} and P. Musico and J. Napolitano and Agasson, {A. Navrer} and A. Oleinik and M. Orsini and F. Ortica and L. Pagani and M. Pallavicini and E. Pantic and K. Pelczar and N. Pelliccia and A. Pocar and S. Pordes and Pugachev, {D. A.} and H. Qian and K. Randle 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 W. Sands and S. Sanfilippo 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 C. Yang and Z. Ye and C. Zhu and G. Zuzel",

note = "Funding Information: This work was 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 Russian RSF (Grant No 16-12-10369), and the Polish NCN (Grant UMO-2014/15/B/ST2/02561). 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 Cit{\'e} (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), from S{\~a}o Paulo Research Foundation (FAPESP) grant (2016/09084-0), and from Foundation for Polish Science (grant No. TEAM/2016-2/17). Publisher Copyright: {\textcopyright} 2017 IOP Publishing Ltd and Sissa Medialab.",

year = "2017",

month = oct,

day = "23",

doi = "10.1088/1748-0221/12/10/P10015",

language = "English (US)",

volume = "12",

journal = "Journal of Instrumentation",

issn = "1748-0221",

publisher = "IOP Publishing Ltd.",

number = "10",

}

Agnes, P, Albuquerque, IFM, Alexander, T, Alton, AK, Asner, DM, Back, HO, Biery, K, Bocci, V, Bonfini, G, Bonivento, W, Bossa, M, Bottino, B, Budano, F, Bussino, S, Cadeddu, M, Cadoni, M, Calaprice, F, Canci, N, Candela, A, Caravati, M, Cariello, M, Carlini, M, Catalanotti, S, Cataudella, V, Cavalcante, P, Chepurnov, A, Cicalò, C, Cocco, AG, Covone, G, D'Angelo, D, D'Incecco, M, Davini, S, De Candia, A, De Cecco, S, De Deo, M, De Filippis, G, De Vincenzi, M, Derbin, AV, De Rosa, G, 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, James, I, Johnson, TN, Keeter, K, Kendziora, CL, Koh, G, Korablev, D, Korga, G, Kubankin, A, Li, X, Lissia, M, Loer, B, Longo, G, Ma, Y, Machado, AA, Machulin, IN, Mandarano, A, Mari, SM, Maricic, J, Martoff, CJ, Meyers, PD, Milincic, R, Monte, A, Mount, BJ, Muratova, VN, Musico, P, Napolitano, J, Agasson, AN, Oleinik, A, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pantic, E, Pelczar, K, Pelliccia, N, Pocar, A, Pordes, S, Pugachev, DA, Qian, H, Randle, K, Razeti, M, Razeto, A, Reinhold, B, Renshaw, AL, Rescigno, M, Riffard, Q, Romani, A, Rossi, B, Rossi, N, Sablone, D, Sands, W, Sanfilippo, S, 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, Yang, C, Ye, Z, Zhu, C & Zuzel, G 2017, 'Simulation of argon response and light detection in the DarkSide-50 dual phase TPC', Journal of Instrumentation, vol. 12, no. 10, P10015. https://doi.org/10.1088/1748-0221/12/10/P10015

TY - JOUR

T1 - Simulation of argon response and light detection in the DarkSide-50 dual phase TPC

AU - Agnes, P.

AU - Albuquerque, I. F.M.

AU - Alexander, T.

AU - Alton, A. K.

AU - Asner, D. M.

AU - Back, H. O.

AU - Biery, K.

AU - Bocci, V.

AU - Bonfini, G.

AU - Bonivento, W.

AU - Bossa, M.

AU - Bottino, B.

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 - Cataudella, V.

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 Candia, A.

AU - De Cecco, S.

AU - De Deo, M.

AU - De Filippis, G.

AU - De Vincenzi, M.

AU - Derbin, A. V.

AU - De Rosa, G.

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, An

AU - James, I.

AU - Johnson, T. N.

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 - Longo, G.

AU - Ma, Y.

AU - Machado, A. A.

AU - Machulin, I. N.

AU - Mandarano, A.

AU - Mari, S. M.

AU - Maricic, J.

AU - Martoff, C. J.

AU - Meyers, P. D.

AU - Milincic, R.

AU - Monte, A.

AU - Mount, B. J.

AU - Muratova, V. N.

AU - Musico, P.

AU - Napolitano, J.

AU - Agasson, A. Navrer

AU - Oleinik, A.

AU - Orsini, M.

AU - Ortica, F.

AU - Pagani, L.

AU - Pallavicini, M.

AU - Pantic, E.

AU - Pelczar, K.

AU - Pelliccia, N.

AU - Pocar, A.

AU - Pordes, S.

AU - Pugachev, D. A.

AU - Qian, H.

AU - Randle, K.

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 - Sands, W.

AU - Sanfilippo, S.

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 - Yang, C.

AU - Ye, Z.

AU - Zhu, C.

AU - Zuzel, G.

N1 - Funding Information: This work was 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 Russian RSF (Grant No 16-12-10369), and the Polish NCN (Grant UMO-2014/15/B/ST2/02561). 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 Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), from São Paulo Research Foundation (FAPESP) grant (2016/09084-0), and from Foundation for Polish Science (grant No. TEAM/2016-2/17). Publisher Copyright: © 2017 IOP Publishing Ltd and Sissa Medialab.

PY - 2017/10/23

Y1 - 2017/10/23

N2 - A Geant4-based Monte Carlo package named G4DS has been developed to simulate the response of DarkSide-50, an experiment operating since 2013 at LNGS, designed to detect WIMP interactions in liquid argon. In the process of WIMP searches, DarkSide-50 has achieved two fundamental milestones: the rejection of electron recoil background with a power of ∼107, using the pulse shape discrimination technique, and the measurement of the residual 39Ar contamination in underground argon, ∼3 orders of magnitude lower with respect to atmospheric argon. These results rely on the accurate simulation of the detector response to the liquid argon scintillation, its ionization, and electron-ion recombination processes. This work provides a complete overview of the DarkSide Monte Carlo and of its performance, with a particular focus on PARIS, the custom-made liquid argon response model.

AB - A Geant4-based Monte Carlo package named G4DS has been developed to simulate the response of DarkSide-50, an experiment operating since 2013 at LNGS, designed to detect WIMP interactions in liquid argon. In the process of WIMP searches, DarkSide-50 has achieved two fundamental milestones: the rejection of electron recoil background with a power of ∼107, using the pulse shape discrimination technique, and the measurement of the residual 39Ar contamination in underground argon, ∼3 orders of magnitude lower with respect to atmospheric argon. These results rely on the accurate simulation of the detector response to the liquid argon scintillation, its ionization, and electron-ion recombination processes. This work provides a complete overview of the DarkSide Monte Carlo and of its performance, with a particular focus on PARIS, the custom-made liquid argon response model.

KW - Dark Matter detectors (WIMPs, axions, etc.)

KW - Detector modelling and simulations I (interaction of radiation with matter, interaction of photons with matter, interaction of hadrons with matter, etc)

KW - Ionization and excitation processes

KW - Noble liquid detectors (scintillation, ionization, double-phase)

UR - http://www.scopus.com/inward/record.url?scp=85033580371&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85033580371&partnerID=8YFLogxK

U2 - 10.1088/1748-0221/12/10/P10015

DO - 10.1088/1748-0221/12/10/P10015

M3 - Article

AN - SCOPUS:85033580371

SN - 1748-0221

VL - 12

JO - Journal of Instrumentation

JF - Journal of Instrumentation

IS - 10

M1 - P10015

ER -

Simulation of argon response and light detection in the DarkSide-50 dual phase TPC

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