Latest results of dark matter detection with the DarkSide experiment

E. Picciau; P. Agnes; I. F.M. Albuquerque; 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; Frank 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; 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; 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:10.1393/ncc/i2020-20026-3

Latest results of dark matter detection with the DarkSide experiment

E. Picciau, P. Agnes, I. F.M. Albuquerque, 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, Frank 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, 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, 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

Abstract

In this contribution the latest results of dark matter direct detection obtained by the DarkSide Collaboration are discussed. New limits on the scattering cross-section between dark matter particles and baryonic matter have been set. The results have been reached using the DarkSide-50 detector, a double-phase Time Projection Chamber (TPC) filled with ⁴⁰Ar and installed at Laboratori Nazionali del Gran Sasso (LNGS). In 2018, the DarkSide Collaboration has performed three different types of analysis. The so-called high-mass analysis into the range between ∼ 10 GeV and ∼ 1000 GeV is discussed under the hypothesis of scattering between dark matter and Ar nuclei. The low-mass analysis, performed using the same hypothesis, extends the limit down to ∼1.8 GeV. Through a different hypothesis, that predicts dark matter scattering off the electrons inside of the Ar atom, it has been possible to set limits for sub-GeV dark matter masses.

Original language	English (US)
Article number	26
Journal	Nuovo Cimento della Societa Italiana di Fisica C
Volume	43
Issue number	2-3
DOIs	https://doi.org/10.1393/ncc/i2020-20026-3
State	Published - Jun 2020

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Physics and Astronomy (miscellaneous)

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10.1393/ncc/i2020-20026-3

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Picciau, E., Agnes, P., Albuquerque, I. F. M., 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). Latest results of dark matter detection with the DarkSide experiment. Nuovo Cimento della Societa Italiana di Fisica C, 43(2-3), [26]. https://doi.org/10.1393/ncc/i2020-20026-3

@article{08c546b2bad04abb9b10d18b0cdf0226,

title = "Latest results of dark matter detection with the DarkSide experiment",

abstract = "In this contribution the latest results of dark matter direct detection obtained by the DarkSide Collaboration are discussed. New limits on the scattering cross-section between dark matter particles and baryonic matter have been set. The results have been reached using the DarkSide-50 detector, a double-phase Time Projection Chamber (TPC) filled with 40Ar and installed at Laboratori Nazionali del Gran Sasso (LNGS). In 2018, the DarkSide Collaboration has performed three different types of analysis. The so-called high-mass analysis into the range between ∼ 10 GeV and ∼ 1000 GeV is discussed under the hypothesis of scattering between dark matter and Ar nuclei. The low-mass analysis, performed using the same hypothesis, extends the limit down to ∼1.8 GeV. Through a different hypothesis, that predicts dark matter scattering off the electrons inside of the Ar atom, it has been possible to set limits for sub-GeV dark matter masses.",

author = "E. Picciau and P. Agnes and Albuquerque, {I. F.M.} 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 Frank 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 {Navrer Agasson}, A. 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 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 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",

year = "2020",

month = jun,

doi = "10.1393/ncc/i2020-20026-3",

language = "English (US)",

volume = "43",

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

issn = "1124-1896",

publisher = "Societa Italiana di Fisica",

number = "2-3",

}

Picciau, E, Agnes, P, Albuquerque, IFM, 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, Navrer Agasson, A, Nozdrina, AO, Oleinik, A, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pandola, L, Pantic, E, Paoloni, E, Pelczar, K, Pelliccia, N, 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, 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, 'Latest results of dark matter detection with the DarkSide experiment', Nuovo Cimento della Societa Italiana di Fisica C, vol. 43, no. 2-3, 26. https://doi.org/10.1393/ncc/i2020-20026-3

TY - JOUR

T1 - Latest results of dark matter detection with the DarkSide experiment

AU - Picciau, E.

AU - Agnes, P.

AU - Albuquerque, I. F.M.

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, Frank

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 - Navrer Agasson, A.

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 - 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 - 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.

PY - 2020/6

Y1 - 2020/6

N2 - In this contribution the latest results of dark matter direct detection obtained by the DarkSide Collaboration are discussed. New limits on the scattering cross-section between dark matter particles and baryonic matter have been set. The results have been reached using the DarkSide-50 detector, a double-phase Time Projection Chamber (TPC) filled with 40Ar and installed at Laboratori Nazionali del Gran Sasso (LNGS). In 2018, the DarkSide Collaboration has performed three different types of analysis. The so-called high-mass analysis into the range between ∼ 10 GeV and ∼ 1000 GeV is discussed under the hypothesis of scattering between dark matter and Ar nuclei. The low-mass analysis, performed using the same hypothesis, extends the limit down to ∼1.8 GeV. Through a different hypothesis, that predicts dark matter scattering off the electrons inside of the Ar atom, it has been possible to set limits for sub-GeV dark matter masses.

AB - In this contribution the latest results of dark matter direct detection obtained by the DarkSide Collaboration are discussed. New limits on the scattering cross-section between dark matter particles and baryonic matter have been set. The results have been reached using the DarkSide-50 detector, a double-phase Time Projection Chamber (TPC) filled with 40Ar and installed at Laboratori Nazionali del Gran Sasso (LNGS). In 2018, the DarkSide Collaboration has performed three different types of analysis. The so-called high-mass analysis into the range between ∼ 10 GeV and ∼ 1000 GeV is discussed under the hypothesis of scattering between dark matter and Ar nuclei. The low-mass analysis, performed using the same hypothesis, extends the limit down to ∼1.8 GeV. Through a different hypothesis, that predicts dark matter scattering off the electrons inside of the Ar atom, it has been possible to set limits for sub-GeV dark matter masses.

UR - http://www.scopus.com/inward/record.url?scp=85091665810&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85091665810&partnerID=8YFLogxK

U2 - 10.1393/ncc/i2020-20026-3

DO - 10.1393/ncc/i2020-20026-3

M3 - Article

AN - SCOPUS:85091665810

SN - 1124-1896

VL - 43

JO - Nuovo Cimento della Societa Italiana di Fisica C

JF - Nuovo Cimento della Societa Italiana di Fisica C

IS - 2-3

M1 - 26

ER -

Latest results of dark matter detection with the DarkSide experiment

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