Effective field theory interactions for liquid argon target in DarkSide-50 experiment

P. Agnes; I. F.M. Albuquerque; T. Alexander; A. K. Alton; M. Ave; H. O. Back; G. Batignani; K. Biery; V. Bocci; G. Bonfini; W. M. Bonivento; B. Bottino; S. Bussino; M. Cadeddu; M. Cadoni; F. Calaprice; A. Caminata; N. Canci; A. Candela; M. Caravati; M. Cariello; M. Carlini; M. Carpinelli; S. Catalanotti; V. Cataudella; P. Cavalcante; S. Cavuoti; A. Chepurnov; C. Cicalò; A. G. Cocco; G. Covone; D. D'Angelo; S. Davini; A. De Candia; S. De Cecco; M. De Deo; G. De Filippis; G. De Rosa; A. V. Derbin; A. Devoto; F. Di Eusanio; M. D'Incecco; G. Di Pietro; C. Dionisi; M. Downing; D. D'Urso; E. Edkins; A. Empl; G. Fiorillo; K. Fomenko; D. Franco; F. Gabriele; C. Galbiati; C. Ghiano; S. Giagu; C. Giganti; G. K. Giovanetti; O. Gorchakov; A. M. Goretti; F. Granato; A. Grobov; M. Gromov; M. Guan; Y. Guardincerri; M. Gulino; B. R. Hackett; K. Herner; B. Hosseini; D. Hughes; P. Humble; E. V. Hungerford; Al Ianni; An Ianni; V. Ippolito; T. N. Johnson; K. Keeter; C. L. Kendziora; I. Kochanek; G. Koh; D. Korablev; G. Korga; A. Kubankin; M. Kuss; M. La Commara; M. Lai; X. Li; M. Lissia; G. Longo; A. A. Machado; I. N. Machulin; A. Mandarano; L. Mapelli; S. M. Mari; J. Maricic; C. J. Martoff; A. Messina; P. D. Meyers; R. Milincic; A. Monte; M. Morrocchi; V. N. Muratova; P. Musico; A. Navrer Agasson; A. O. Nozdrina; A. Oleinik; M. Orsini; F. Ortica; L. Pagani; M. Pallavicini; L. Pandola; E. Pantic; E. Paoloni; K. Pelczar; N. Pelliccia; E. Picciau; A. Pocar; S. Pordes; S. S. Poudel; H. Qian; F. Ragusa; M. Razeti; A. Razeto; A. L. Renshaw; M. Rescigno; Q. Riffard; A. Romani; B. Rossi; N. Rossi; D. Sablone; O. Samoylov; W. Sands; S. Sanfilippo; C. Savarese; B. Schlitzer; E. Segreto; D. A. Semenov; A. Shchagin; A. Sheshukov; P. N. Singh; M. D. Skorokhvatov; O. Smirnov; A. Sotnikov; C. Stanford; S. Stracka; Y. Suvorov; R. Tartaglia; G. Testera; A. Tonazzo; P. Trinchese; E. V. Unzhakov; M. Verducci; A. Vishneva; R. B. Vogelaar; M. Wada; T. J. Waldrop; H. Wang; Y. Wang; A. W. Watson; S. Westerdale; M. M. Wojcik; X. Xiang; X. Xiao; C. Yang; Z. Ye; C. Zhu; G. Zuzel

doi:10.1103/PhysRevD.101.062002

Effective field theory interactions for liquid argon target in DarkSide-50 experiment

P. Agnes, I. F.M. Albuquerque, T. Alexander, A. K. Alton, M. Ave, H. O. Back, G. Batignani, K. Biery, V. Bocci, G. Bonfini, W. M. Bonivento, B. Bottino, S. Bussino, M. Cadeddu, M. Cadoni, F. Calaprice, A. Caminata, N. Canci, A. Candela, M. CaravatiM. Cariello, M. Carlini, M. Carpinelli, S. Catalanotti, V. Cataudella, P. Cavalcante, S. Cavuoti, A. Chepurnov, C. Cicalò, A. G. Cocco, G. Covone, D. D'Angelo, S. Davini, A. De Candia, S. De Cecco, M. De Deo, G. De Filippis, G. De Rosa, A. V. Derbin, A. Devoto, F. Di Eusanio, M. D'Incecco, G. Di Pietro, C. Dionisi, M. Downing, D. D'Urso, E. Edkins, A. Empl, G. Fiorillo, K. Fomenko, D. Franco, F. Gabriele, C. Galbiati, C. Ghiano, S. Giagu, C. Giganti, G. K. Giovanetti, O. Gorchakov, A. M. Goretti, F. Granato, A. Grobov, M. Gromov, M. Guan, Y. Guardincerri, M. Gulino, B. R. Hackett, K. Herner, B. Hosseini, D. Hughes, P. Humble, E. V. Hungerford, Al Ianni, An Ianni, V. Ippolito, T. N. Johnson, K. Keeter, C. L. Kendziora, I. Kochanek, G. Koh, D. Korablev, G. Korga, A. Kubankin, M. Kuss, M. La Commara, M. Lai, X. Li, M. Lissia, G. Longo, A. A. Machado, I. N. Machulin, A. Mandarano, L. Mapelli, S. M. Mari, J. Maricic, C. J. Martoff, A. Messina, P. D. Meyers, R. Milincic, A. Monte, M. Morrocchi, V. N. Muratova, P. Musico, A. Navrer Agasson, A. O. Nozdrina, A. Oleinik, M. Orsini, F. Ortica, L. Pagani, M. Pallavicini, L. Pandola, E. Pantic, E. Paoloni, K. Pelczar, N. Pelliccia, E. Picciau, A. Pocar, S. Pordes, S. S. Poudel, H. Qian, F. Ragusa, M. Razeti, A. Razeto, A. L. Renshaw, M. Rescigno, Q. Riffard, A. Romani, B. Rossi, N. Rossi, D. Sablone, O. Samoylov, W. Sands, S. Sanfilippo, C. Savarese, B. Schlitzer, E. Segreto, D. A. Semenov, A. Shchagin, A. Sheshukov, P. N. Singh, M. D. Skorokhvatov, O. Smirnov, A. Sotnikov, C. Stanford, S. Stracka, Y. Suvorov, R. Tartaglia, G. Testera, A. Tonazzo, P. Trinchese, E. V. Unzhakov, M. Verducci, A. Vishneva, R. B. Vogelaar, M. Wada, T. J. Waldrop, H. Wang, Y. Wang, A. W. Watson, S. Westerdale, M. M. Wojcik, X. Xiang, X. Xiao, C. Yang, Z. Ye, C. Zhu, G. Zuzel

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

3 Scopus citations

Abstract

We reanalyze data collected with the DarkSide-50 experiment and recently used to set limits on the spinindependent interaction rate of weakly interacting massive particles (WIMPs) on argon nuclei with an effective field theory framework. The dataset corresponds to a total (16660 ± 270) kg d exposure using a target of low-radioactivity argon extracted from underground sources. We obtain upper limits on the effective couplings of the 12 leading operators in the nonrelativistic systematic expansion. For each effective coupling we set constraints on WIMP-nucleon cross sections, setting upper limits between 2.4 × 10^-45 cm² and 2.3 × 10^-42 cm² (8.9 × 10^-45 cm² and 6.0 × 10^-42 cm²) for WIMPs of mass of 100 GeV=c2 (1000 GeV=c²) at 90% confidence level.

Original language	English (US)
Article number	062002
Journal	Physical Review D
Volume	101
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevD.101.062002
State	Published - Mar 15 2020
Externally published	Yes

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

Access to Document

10.1103/PhysRevD.101.062002

Cite this

Agnes, P., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Ave, M., Back, H. O., Batignani, G., Biery, K., Bocci, V., Bonfini, G., Bonivento, W. M., Bottino, B., Bussino, S., Cadeddu, M., Cadoni, M., Calaprice, F., Caminata, A., Canci, N., Candela, A., ... Zuzel, G. (2020). Effective field theory interactions for liquid argon target in DarkSide-50 experiment. Physical Review D, 101(6), [062002]. https://doi.org/10.1103/PhysRevD.101.062002

@article{81453159292c48f19ad398d00120d5c5,

title = "Effective field theory interactions for liquid argon target in DarkSide-50 experiment",

abstract = "We reanalyze data collected with the DarkSide-50 experiment and recently used to set limits on the spinindependent interaction rate of weakly interacting massive particles (WIMPs) on argon nuclei with an effective field theory framework. The dataset corresponds to a total (16660 ± 270) kg d exposure using a target of low-radioactivity argon extracted from underground sources. We obtain upper limits on the effective couplings of the 12 leading operators in the nonrelativistic systematic expansion. For each effective coupling we set constraints on WIMP-nucleon cross sections, setting upper limits between 2.4 × 10-45 cm2 and 2.3 × 10-42 cm2 (8.9 × 10-45 cm2 and 6.0 × 10-42 cm2) for WIMPs of mass of 100 GeV=c2 (1000 GeV=c2) at 90% confidence level.",

author = "P. Agnes and Albuquerque, {I. F.M.} and T. Alexander and Alton, {A. K.} and M. Ave and Back, {H. O.} and G. Batignani and K. Biery and V. Bocci and G. Bonfini and Bonivento, {W. M.} and B. Bottino and S. Bussino and M. Cadeddu and M. Cadoni and F. Calaprice and A. Caminata and N. Canci and A. Candela and M. Caravati and M. Cariello and M. Carlini and M. Carpinelli and S. Catalanotti and V. Cataudella and P. Cavalcante and S. Cavuoti and A. Chepurnov and C. Cical{\`o} and Cocco, {A. G.} and G. Covone and D. D'Angelo and S. Davini and {De Candia}, A. and {De Cecco}, S. and {De Deo}, M. and {De Filippis}, G. and {De Rosa}, G. and Derbin, {A. V.} and A. Devoto and {Di Eusanio}, F. and M. D'Incecco and {Di Pietro}, G. and C. Dionisi and M. Downing and D. D'Urso and E. Edkins and A. Empl and G. Fiorillo and K. Fomenko and D. Franco and F. Gabriele and C. Galbiati and C. Ghiano and S. Giagu and C. Giganti and Giovanetti, {G. K.} and O. Gorchakov and Goretti, {A. M.} and F. Granato and A. Grobov and M. Gromov and M. Guan and Y. Guardincerri and M. Gulino and Hackett, {B. R.} and K. Herner and B. Hosseini and D. Hughes and P. Humble and Hungerford, {E. V.} and Al Ianni and An Ianni and V. Ippolito and Johnson, {T. N.} and K. Keeter and Kendziora, {C. L.} and I. Kochanek and G. Koh and D. Korablev and G. Korga and A. Kubankin and M. Kuss and {La Commara}, M. and M. Lai and X. Li and M. Lissia and G. Longo and Machado, {A. A.} and Machulin, {I. N.} and A. Mandarano and L. Mapelli and Mari, {S. M.} and J. Maricic and Martoff, {C. J.} and A. Messina and Meyers, {P. D.} and R. Milincic and A. Monte and M. Morrocchi and Muratova, {V. N.} and P. Musico and Agasson, {A. Navrer} and Nozdrina, {A. O.} and A. Oleinik and M. Orsini and F. Ortica and L. Pagani and M. Pallavicini and L. Pandola and E. Pantic and E. Paoloni and K. Pelczar and N. Pelliccia and E. Picciau and A. Pocar and S. Pordes and Poudel, {S. S.} and H. Qian and F. Ragusa and M. Razeti and A. Razeto and Renshaw, {A. L.} and M. Rescigno and Q. Riffard and A. Romani and B. Rossi and N. Rossi and D. Sablone and O. Samoylov and W. Sands and S. Sanfilippo and C. Savarese and B. Schlitzer and E. Segreto and Semenov, {D. A.} and A. Shchagin and A. Sheshukov and Singh, {P. N.} and Skorokhvatov, {M. D.} and O. Smirnov and A. Sotnikov and C. Stanford and S. Stracka 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 Vogelaar, {R. B.} and M. Wada and Waldrop, {T. J.} and H. Wang and Y. Wang and Watson, {A. W.} and S. Westerdale 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: The DarkSide Collaboration offers its profound gratitude to the LNGS and its staff for their invaluable technical and logistical support. We also thank the Fermilab Particle Physics, Scientific, and Core Computing Divisions. Construction and operation of the DarkSide-50 detector was supported by the U.S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004072, No. PHY-1004054, No. PHY-1242585, No. PHY-1314483, No. PHY-1314501, No. PHY-1314507, No. PHY-1352795, No. PHY-1622415, and associated collaborative grants No. PHY-1211308 and No. PHY-1455351), the Italian Istituto Nazionale di Fisica Nucleare, the U.S. Department of Energy (Contracts No. DE-FG02-91ER40671, No. DEAC02-07CH11359, and No. DE-AC05-76RL01830), the Russian Science Foundation (Grant No. 18-72-00211), the Polish NCN (Grant No. UMO-2014/15/B/ST2/02561) and the Foundation for Polish Science (Grant No. Team2016-2/ 17). We also acknowledge financial support from the French Institut National de Physique Nucl{\'e}aire et de Physique des Particules (IN2P3), the UnivEarthS Labex program of Sorbonne Paris Cit{\'e} (Grants No. ANR-10-LABX-0023 and No. ANR-11-IDEX-0005-02), and from the S{\~a}o Paulo Research Foundation (FAPESP) (Grant No. 2016/09084-0). Isotopes used in this research were supplied by the United States Department of Energy Office of Science by the Isotope Program in the Office of Nuclear Physics. Funding Information: The DarkSide Collaboration offers its profound gratitude to the LNGS and its staff for their invaluable technical and logistical support. We also thank the Fermilab Particle Physics, Scientific, and Core Computing Divisions. Construction and operation of the DarkSide-50 detector was supported by the U.S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004072, No. PHY-1004054, No. PHY-1242585, No. PHY- 1314483, No. PHY-1314501, No. PHY-1314507, No. PHY-1352795, No. PHY-1622415, and associated collaborative grants No. PHY-1211308 and No. PHY- 1455351), the Italian Istituto Nazionale di Fisica Nucleare, the U.S. Department of Energy (Contracts No. DE-FG02-91ER40671, No. DEAC02-07CH11359, and No. DE-AC05-76RL01830), the Russian Science Foundation (Grant No. 18-72-00211), the Polish NCN (Grant No. UMO-2014/15/B/ST2/02561) and the Foundation for Polish Science (Grant No. Team2016-2/ 17). We also acknowledge financial support from the French Institut National de Physique Nucl?aire et de Physique des Particules (IN2P3), the UnivEarthS Labex program of Sorbonne Paris Cit? (Grants No. ANR-10- LABX-0023 and No. ANR-11-IDEX-0005-02), and from the S?o Paulo Research Foundation (FAPESP) (Grant No. 2016/09084-0). Isotopes used in this research were supplied by the United States Department of Energy Office of Science by the Isotope Program in the Office of Nuclear Physics.*%blankline%* Publisher Copyright: {\textcopyright} 2020 American Physical Society.",

year = "2020",

month = mar,

day = "15",

doi = "10.1103/PhysRevD.101.062002",

language = "English (US)",

volume = "101",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

number = "6",

}

Agnes, P, Albuquerque, IFM, Alexander, T, Alton, AK, Ave, M, Back, HO, Batignani, G, Biery, K, Bocci, V, Bonfini, G, Bonivento, WM, Bottino, B, Bussino, S, Cadeddu, M, Cadoni, M, Calaprice, F, Caminata, A, Canci, N, Candela, A, Caravati, M, Cariello, M, Carlini, M, Carpinelli, M, Catalanotti, S, Cataudella, V, Cavalcante, P, Cavuoti, S, Chepurnov, A, Cicalò, C, Cocco, AG, Covone, G, D'Angelo, D, Davini, S, De Candia, A, De Cecco, S, De Deo, M, De Filippis, G, De Rosa, G, Derbin, AV, Devoto, A, Di Eusanio, F, D'Incecco, M, Di Pietro, G, Dionisi, C, Downing, M, D'Urso, D, Edkins, E, Empl, A, Fiorillo, G, Fomenko, K, Franco, D, Gabriele, F, Galbiati, C, Ghiano, C, Giagu, S, Giganti, C, Giovanetti, GK, Gorchakov, O, Goretti, AM, Granato, F, Grobov, A, Gromov, M, Guan, M, Guardincerri, Y, Gulino, M, Hackett, BR, Herner, K, Hosseini, B, Hughes, D, Humble, P, Hungerford, EV, Ianni, A, Ianni, A, Ippolito, V, Johnson, TN, Keeter, K, Kendziora, CL, Kochanek, I, Koh, G, Korablev, D, Korga, G, Kubankin, A, Kuss, M, La Commara, M, Lai, M, Li, X, Lissia, M, Longo, G, Machado, AA, Machulin, IN, Mandarano, A, Mapelli, L, Mari, SM, Maricic, J, Martoff, CJ, Messina, A, Meyers, PD, Milincic, R, Monte, A, Morrocchi, M, Muratova, VN, Musico, P, Agasson, AN, Nozdrina, AO, Oleinik, A, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pandola, L, Pantic, E, Paoloni, E, Pelczar, K, Pelliccia, N, Picciau, E, Pocar, A, Pordes, S, Poudel, SS, Qian, H, Ragusa, F, Razeti, M, Razeto, A, Renshaw, AL, Rescigno, M, Riffard, Q, Romani, A, Rossi, B, Rossi, N, Sablone, D, Samoylov, O, Sands, W, Sanfilippo, S, Savarese, C, Schlitzer, B, Segreto, E, Semenov, DA, Shchagin, A, Sheshukov, A, Singh, PN, Skorokhvatov, MD, Smirnov, O, Sotnikov, A, Stanford, C, Stracka, S, Suvorov, Y, Tartaglia, R, Testera, G, Tonazzo, A, Trinchese, P, Unzhakov, EV, Verducci, M, Vishneva, A, Vogelaar, RB, Wada, M, Waldrop, TJ, Wang, H, Wang, Y, Watson, AW, Westerdale, S, Wojcik, MM, Xiang, X, Xiao, X, Yang, C, Ye, Z, Zhu, C & Zuzel, G 2020, 'Effective field theory interactions for liquid argon target in DarkSide-50 experiment', Physical Review D, vol. 101, no. 6, 062002. https://doi.org/10.1103/PhysRevD.101.062002

TY - JOUR

T1 - Effective field theory interactions for liquid argon target in DarkSide-50 experiment

AU - Agnes, P.

AU - Albuquerque, I. F.M.

AU - Alexander, T.

AU - Alton, A. K.

AU - Ave, M.

AU - Back, H. O.

AU - Batignani, G.

AU - Biery, K.

AU - Bocci, V.

AU - Bonfini, G.

AU - Bonivento, W. M.

AU - Bottino, B.

AU - Bussino, S.

AU - Cadeddu, M.

AU - Cadoni, M.

AU - Calaprice, F.

AU - Caminata, A.

AU - Canci, N.

AU - Candela, A.

AU - Caravati, M.

AU - Cariello, M.

AU - Carlini, M.

AU - Carpinelli, M.

AU - Catalanotti, S.

AU - Cataudella, V.

AU - Cavalcante, P.

AU - Cavuoti, S.

AU - Chepurnov, A.

AU - Cicalò, C.

AU - Cocco, A. G.

AU - Covone, G.

AU - D'Angelo, D.

AU - Davini, S.

AU - De Candia, A.

AU - De Cecco, S.

AU - De Deo, M.

AU - De Filippis, G.

AU - De Rosa, G.

AU - Derbin, A. V.

AU - Devoto, A.

AU - Di Eusanio, F.

AU - D'Incecco, M.

AU - Di Pietro, G.

AU - Dionisi, C.

AU - Downing, M.

AU - D'Urso, D.

AU - Edkins, E.

AU - Empl, A.

AU - Fiorillo, G.

AU - Fomenko, K.

AU - Franco, D.

AU - Gabriele, F.

AU - Galbiati, C.

AU - Ghiano, C.

AU - Giagu, S.

AU - Giganti, C.

AU - Giovanetti, G. K.

AU - Gorchakov, O.

AU - Goretti, A. M.

AU - Granato, F.

AU - Grobov, A.

AU - Gromov, M.

AU - Guan, M.

AU - Guardincerri, Y.

AU - Gulino, M.

AU - Hackett, B. R.

AU - Herner, K.

AU - Hosseini, B.

AU - Hughes, D.

AU - Humble, P.

AU - Hungerford, E. V.

AU - Ianni, Al

AU - Ianni, An

AU - Ippolito, V.

AU - Johnson, T. N.

AU - Keeter, K.

AU - Kendziora, C. L.

AU - Kochanek, I.

AU - Koh, G.

AU - Korablev, D.

AU - Korga, G.

AU - Kubankin, A.

AU - Kuss, M.

AU - La Commara, M.

AU - Lai, M.

AU - Li, X.

AU - Lissia, M.

AU - Longo, G.

AU - Machado, A. A.

AU - Machulin, I. N.

AU - Mandarano, A.

AU - Mapelli, L.

AU - Mari, S. M.

AU - Maricic, J.

AU - Martoff, C. J.

AU - Messina, A.

AU - Meyers, P. D.

AU - Milincic, R.

AU - Monte, A.

AU - Morrocchi, M.

AU - Muratova, V. N.

AU - Musico, P.

AU - Agasson, A. Navrer

AU - Nozdrina, A. O.

AU - Oleinik, A.

AU - Orsini, M.

AU - Ortica, F.

AU - Pagani, L.

AU - Pallavicini, M.

AU - Pandola, L.

AU - Pantic, E.

AU - Paoloni, E.

AU - Pelczar, K.

AU - Pelliccia, N.

AU - Picciau, E.

AU - Pocar, A.

AU - Pordes, S.

AU - Poudel, S. S.

AU - Qian, H.

AU - Ragusa, F.

AU - Razeti, M.

AU - Razeto, A.

AU - Renshaw, A. L.

AU - Rescigno, M.

AU - Riffard, Q.

AU - Romani, A.

AU - Rossi, B.

AU - Rossi, N.

AU - Sablone, D.

AU - Samoylov, O.

AU - Sands, W.

AU - Sanfilippo, S.

AU - Savarese, C.

AU - Schlitzer, B.

AU - Segreto, E.

AU - Semenov, D. A.

AU - Shchagin, A.

AU - Sheshukov, A.

AU - Singh, P. N.

AU - Skorokhvatov, M. D.

AU - Smirnov, O.

AU - Sotnikov, A.

AU - Stanford, C.

AU - Stracka, S.

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, R. B.

AU - Wada, M.

AU - Waldrop, T. J.

AU - Wang, H.

AU - Wang, Y.

AU - Watson, A. W.

AU - Westerdale, S.

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: The DarkSide Collaboration offers its profound gratitude to the LNGS and its staff for their invaluable technical and logistical support. We also thank the Fermilab Particle Physics, Scientific, and Core Computing Divisions. Construction and operation of the DarkSide-50 detector was supported by the U.S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004072, No. PHY-1004054, No. PHY-1242585, No. PHY-1314483, No. PHY-1314501, No. PHY-1314507, No. PHY-1352795, No. PHY-1622415, and associated collaborative grants No. PHY-1211308 and No. PHY-1455351), the Italian Istituto Nazionale di Fisica Nucleare, the U.S. Department of Energy (Contracts No. DE-FG02-91ER40671, No. DEAC02-07CH11359, and No. DE-AC05-76RL01830), the Russian Science Foundation (Grant No. 18-72-00211), the Polish NCN (Grant No. UMO-2014/15/B/ST2/02561) and the Foundation for Polish Science (Grant No. Team2016-2/ 17). We also acknowledge financial support from the French Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), the UnivEarthS Labex program of Sorbonne Paris Cité (Grants No. ANR-10-LABX-0023 and No. ANR-11-IDEX-0005-02), and from the São Paulo Research Foundation (FAPESP) (Grant No. 2016/09084-0). Isotopes used in this research were supplied by the United States Department of Energy Office of Science by the Isotope Program in the Office of Nuclear Physics. Funding Information: The DarkSide Collaboration offers its profound gratitude to the LNGS and its staff for their invaluable technical and logistical support. We also thank the Fermilab Particle Physics, Scientific, and Core Computing Divisions. Construction and operation of the DarkSide-50 detector was supported by the U.S. National Science Foundation (NSF) (Grants No. PHY-0919363, No. PHY-1004072, No. PHY-1004054, No. PHY-1242585, No. PHY- 1314483, No. PHY-1314501, No. PHY-1314507, No. PHY-1352795, No. PHY-1622415, and associated collaborative grants No. PHY-1211308 and No. PHY- 1455351), the Italian Istituto Nazionale di Fisica Nucleare, the U.S. Department of Energy (Contracts No. DE-FG02-91ER40671, No. DEAC02-07CH11359, and No. DE-AC05-76RL01830), the Russian Science Foundation (Grant No. 18-72-00211), the Polish NCN (Grant No. UMO-2014/15/B/ST2/02561) and the Foundation for Polish Science (Grant No. Team2016-2/ 17). We also acknowledge financial support from the French Institut National de Physique Nucl?aire et de Physique des Particules (IN2P3), the UnivEarthS Labex program of Sorbonne Paris Cit? (Grants No. ANR-10- LABX-0023 and No. ANR-11-IDEX-0005-02), and from the S?o Paulo Research Foundation (FAPESP) (Grant No. 2016/09084-0). Isotopes used in this research were supplied by the United States Department of Energy Office of Science by the Isotope Program in the Office of Nuclear Physics.*%blankline%* Publisher Copyright: © 2020 American Physical Society.

PY - 2020/3/15

Y1 - 2020/3/15

N2 - We reanalyze data collected with the DarkSide-50 experiment and recently used to set limits on the spinindependent interaction rate of weakly interacting massive particles (WIMPs) on argon nuclei with an effective field theory framework. The dataset corresponds to a total (16660 ± 270) kg d exposure using a target of low-radioactivity argon extracted from underground sources. We obtain upper limits on the effective couplings of the 12 leading operators in the nonrelativistic systematic expansion. For each effective coupling we set constraints on WIMP-nucleon cross sections, setting upper limits between 2.4 × 10-45 cm2 and 2.3 × 10-42 cm2 (8.9 × 10-45 cm2 and 6.0 × 10-42 cm2) for WIMPs of mass of 100 GeV=c2 (1000 GeV=c2) at 90% confidence level.

AB - We reanalyze data collected with the DarkSide-50 experiment and recently used to set limits on the spinindependent interaction rate of weakly interacting massive particles (WIMPs) on argon nuclei with an effective field theory framework. The dataset corresponds to a total (16660 ± 270) kg d exposure using a target of low-radioactivity argon extracted from underground sources. We obtain upper limits on the effective couplings of the 12 leading operators in the nonrelativistic systematic expansion. For each effective coupling we set constraints on WIMP-nucleon cross sections, setting upper limits between 2.4 × 10-45 cm2 and 2.3 × 10-42 cm2 (8.9 × 10-45 cm2 and 6.0 × 10-42 cm2) for WIMPs of mass of 100 GeV=c2 (1000 GeV=c2) at 90% confidence level.

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U2 - 10.1103/PhysRevD.101.062002

DO - 10.1103/PhysRevD.101.062002

M3 - Article

AN - SCOPUS:85083435153

SN - 2470-0010

VL - 101

JO - Physical Review D

JF - Physical Review D

IS - 6

M1 - 062002

ER -

Effective field theory interactions for liquid argon target in DarkSide-50 experiment

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