The darkside multiton detector for the direct dark matter search

C. E. Aalseth; P. Agnes; A. Alton; K. Arisaka; D. M. Asner; H. O. Back; B. Baldin; K. Biery; G. Bonfini; M. Bossa; A. Brigatti; J. Brodsky; F. Budano; L. Cadonati; M. Cadoni; F. Calaprice; N. Canci; A. Candela; H. Cao; M. Cariello; P. Cavalcante; A. Chepurnov; A. G. Cocco; C. Condon; L. Crippa; D. D'Angelo; M. D'Incecco; S. Davini; M. De Deo; A. Derbin; A. Devoto; F. Di Eusanio; E. Edkins; A. Empl; A. Fan; G. Fiorillo; K. Fomenko; G. Forster; M. Foxe; D. Franco; F. Gabriele; C. Galbiati; A. Goretti; L. Grandi; M. Gromov; M. Y. Guan; Y. Guardincerri; B. Hackett; K. Herner; A. Hime; P. Humble; E. Hungerford; Al Ianni; An Ianni; D. E. Jaffe; C. Jollet; K. Keeter; C. Kendziora; S. Kidner; V. Kobychev; G. Koh; D. Korablev; G. Korga; A. Kurlej; P. X. Li; M. Lissia; P. Lombardi; L. Ludhova; S. Luitz; G. Lukyachenko; Y. Q. Ma; I. Machulin; A. Mandarano; S. M. Mari; J. Maricic; L. Marini; D. Markov; J. Martoff; A. Meregaglia; E. Meroni; P. D. Meyers; T. Miletic; R. Milincic; M. Montuschi; M. E. Monzani; P. Mosteiro; B. Mount; V. Muratova; P. Musico; D. Montanari; A. Nelson; S. Odrowski; A. Odrzywolek; J. L. Orrell; M. Orsini; F. Ortica; L. Pagani; M. Pallavicini; E. Pantic; S. Parmeggiano; B. Parsells; K. Pelczar; N. Pelliccia; S. Perasso; L. Perasso; A. Pocar; S. Pordes; D. Pugachev; H. Qian; K. Randle; G. Ranucci; A. Razeto; K. Recine; B. Reinhold; A. Renshaw; A. Romani; N. Rossi; B. Rossi; S. D. Rountree; D. Sablone; P. Saggese; R. Saldanha; W. Sands; S. Sangiorgio; E. Segreto; D. Semenov; E. Shields; M. Skorokhvatov; M. Smallcomb; O. Smirnov; A. Sotnikov; Y. Suvurov; R. Tartaglia; J. Tatarowicz; G. Testera; A. Tonazzo; E. Unzhakov; R. B. Vogelaar; M. Wada; S. E. Walker; H. Wang; Y. Wang; A. W. Watson; S. Westerdale; R. Williams; M. Wojcik; J. Xu; C. G. Yang; J. Yoo; B. Yu; S. Zavatarelli; W. L. Zhong; G. Zuzel

doi:10.1155/2015/541362

The darkside multiton detector for the direct dark matter search

C. E. Aalseth, P. Agnes, A. Alton, K. Arisaka, D. M. Asner, H. O. Back, B. Baldin, K. Biery, G. Bonfini, M. Bossa, A. Brigatti, J. Brodsky, F. Budano, L. Cadonati, M. Cadoni, F. Calaprice, N. Canci, A. Candela, H. Cao, M. CarielloP. Cavalcante, A. Chepurnov, A. G. Cocco, C. Condon, L. Crippa, D. D'Angelo, M. D'Incecco, S. Davini, M. De Deo, A. Derbin, A. Devoto, F. Di Eusanio, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, G. Forster, M. Foxe, D. Franco, F. Gabriele, C. Galbiati, A. Goretti, L. Grandi, M. Gromov, M. Y. Guan, Y. Guardincerri, B. Hackett, K. Herner, A. Hime, P. Humble, E. Hungerford, Al Ianni, An Ianni, D. E. Jaffe, C. Jollet, K. Keeter, C. Kendziora, S. Kidner, V. Kobychev, G. Koh, D. Korablev, G. Korga, A. Kurlej, P. X. Li, M. Lissia, P. Lombardi, L. Ludhova, S. Luitz, G. Lukyachenko, Y. Q. Ma, I. Machulin, A. Mandarano, S. M. Mari, J. Maricic, L. Marini, D. Markov, J. Martoff, A. Meregaglia, E. Meroni, P. D. Meyers, T. Miletic, R. Milincic, M. Montuschi, M. E. Monzani, P. Mosteiro, B. Mount, V. Muratova, P. Musico, D. Montanari, A. Nelson, S. Odrowski, A. Odrzywolek, J. L. Orrell, M. Orsini, F. Ortica, L. Pagani, M. Pallavicini, E. Pantic, S. Parmeggiano, B. Parsells, K. Pelczar, N. Pelliccia, S. Perasso, L. Perasso, A. Pocar, S. Pordes, D. Pugachev, H. Qian, K. Randle, G. Ranucci, A. Razeto, K. Recine, B. Reinhold, A. Renshaw, A. Romani, N. Rossi, B. Rossi, S. D. Rountree, D. Sablone, P. Saggese, R. Saldanha, W. Sands, S. Sangiorgio, E. Segreto, D. Semenov, E. Shields, M. Skorokhvatov, M. Smallcomb, O. Smirnov, A. Sotnikov, Y. Suvurov, R. Tartaglia, J. Tatarowicz, G. Testera, A. Tonazzo, E. Unzhakov, R. B. Vogelaar, M. Wada, S. E. Walker, H. Wang, Y. Wang, A. W. Watson, S. Westerdale, R. Williams, M. Wojcik, J. Xu, C. G. Yang, J. Yoo, B. Yu, S. Zavatarelli, W. L. Zhong, G. Zuzel

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

20 Scopus citations

Abstract

Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (<100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide-50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.

Original language	English (US)
Article number	541362
Journal	Advances in High Energy Physics
Volume	2015
DOIs	https://doi.org/10.1155/2015/541362
State	Published - Jan 20 2015

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

Access to Document

10.1155/2015/541362

Cite this

Aalseth, C. E., Agnes, P., Alton, A., Arisaka, K., Asner, D. M., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., ... Zuzel, G. (2015). The darkside multiton detector for the direct dark matter search. Advances in High Energy Physics, 2015, Article 541362. https://doi.org/10.1155/2015/541362

@article{2e575ccf00ba47368e542617d67dd52e,

title = "The darkside multiton detector for the direct dark matter search",

abstract = "Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (<100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide-50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.",

author = "Aalseth, {C. E.} and P. Agnes and A. Alton and K. Arisaka and Asner, {D. M.} and Back, {H. O.} and B. Baldin and K. Biery and G. Bonfini and M. Bossa and A. Brigatti and J. Brodsky and F. Budano and L. Cadonati and M. Cadoni and F. Calaprice and N. Canci and A. Candela and H. Cao and M. Cariello and P. Cavalcante and A. Chepurnov and Cocco, {A. G.} and C. Condon and L. Crippa and D. D'Angelo and M. D'Incecco and S. Davini and {De Deo}, M. and A. Derbin and A. Devoto and {Di Eusanio}, F. and E. Edkins and A. Empl and A. Fan and G. Fiorillo and K. Fomenko and G. Forster and M. Foxe and D. Franco and F. Gabriele and C. Galbiati and A. Goretti and L. Grandi and M. Gromov and Guan, {M. Y.} and Y. Guardincerri and B. Hackett and K. Herner and A. Hime and P. Humble and E. Hungerford and Al Ianni and An Ianni and Jaffe, {D. E.} and C. Jollet and K. Keeter and C. Kendziora and S. Kidner and V. Kobychev and G. Koh and D. Korablev and G. Korga and A. Kurlej and Li, {P. X.} and M. Lissia and P. Lombardi and L. Ludhova and S. Luitz and G. Lukyachenko and Ma, {Y. Q.} and I. Machulin and A. Mandarano and Mari, {S. M.} and J. Maricic and L. Marini and D. Markov and J. Martoff and A. Meregaglia and E. Meroni and Meyers, {P. D.} and T. Miletic and R. Milincic and M. Montuschi and Monzani, {M. E.} and P. Mosteiro and B. Mount and V. Muratova and P. Musico and D. Montanari and A. Nelson and S. Odrowski and A. Odrzywolek and Orrell, {J. L.} and M. Orsini and F. Ortica and L. Pagani and M. Pallavicini and E. Pantic and S. Parmeggiano and B. Parsells and K. Pelczar and N. Pelliccia and S. Perasso and L. Perasso and A. Pocar and S. Pordes and D. Pugachev and H. Qian and K. Randle and G. Ranucci and A. Razeto and K. Recine and B. Reinhold and A. Renshaw and A. Romani and N. Rossi and B. Rossi and Rountree, {S. D.} and D. Sablone and P. Saggese and R. Saldanha and W. Sands and S. Sangiorgio and E. Segreto and D. Semenov and E. Shields and M. Skorokhvatov and M. Smallcomb and O. Smirnov and A. Sotnikov and Y. Suvurov and R. Tartaglia and J. Tatarowicz and G. Testera and A. Tonazzo and E. Unzhakov and Vogelaar, {R. B.} and M. Wada and Walker, {S. E.} and H. Wang and Y. Wang and Watson, {A. W.} and S. Westerdale and R. Williams and M. Wojcik and J. Xu and Yang, {C. G.} and J. Yoo and B. Yu and S. Zavatarelli and Zhong, {W. L.} and G. Zuzel",

note = "Publisher Copyright: {\textcopyright} 2015 C. E. Aalseth et al.",

year = "2015",

month = jan,

day = "20",

doi = "10.1155/2015/541362",

language = "English (US)",

volume = "2015",

journal = "Advances in High Energy Physics",

issn = "1687-7357",

publisher = "John Wiley and Sons Ltd",

}

Aalseth, CE, Agnes, P, Alton, A, Arisaka, K, Asner, DM, Back, HO, Baldin, B, Biery, K, Bonfini, G, Bossa, M, Brigatti, A, Brodsky, J, Budano, F, Cadonati, L, Cadoni, M, Calaprice, F, Canci, N, Candela, A, Cao, H, Cariello, M, Cavalcante, P, Chepurnov, A, Cocco, AG, Condon, C, Crippa, L, D'Angelo, D, D'Incecco, M, Davini, S, De Deo, M, Derbin, A, Devoto, A, Di Eusanio, F, Edkins, E, Empl, A, Fan, A, Fiorillo, G, Fomenko, K, Forster, G, Foxe, M, Franco, D, Gabriele, F, Galbiati, C, Goretti, A, Grandi, L, Gromov, M, Guan, MY, Guardincerri, Y, Hackett, B, Herner, K, Hime, A, Humble, P, Hungerford, E, Ianni, A, Ianni, A, Jaffe, DE, Jollet, C, Keeter, K, Kendziora, C, Kidner, S, Kobychev, V, Koh, G, Korablev, D, Korga, G, Kurlej, A, Li, PX, Lissia, M, Lombardi, P, Ludhova, L, Luitz, S, Lukyachenko, G, Ma, YQ, Machulin, I, Mandarano, A, Mari, SM, Maricic, J, Marini, L, Markov, D, Martoff, J, Meregaglia, A, Meroni, E, Meyers, PD, Miletic, T, Milincic, R, Montuschi, M, Monzani, ME, Mosteiro, P, Mount, B, Muratova, V, Musico, P, Montanari, D, Nelson, A, Odrowski, S, Odrzywolek, A, Orrell, JL, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pantic, E, Parmeggiano, S, Parsells, B, Pelczar, K, Pelliccia, N, Perasso, S, Perasso, L, Pocar, A, Pordes, S, Pugachev, D, Qian, H, Randle, K, Ranucci, G, Razeto, A, Recine, K, Reinhold, B, Renshaw, A, Romani, A, Rossi, N, Rossi, B, Rountree, SD, Sablone, D, Saggese, P, Saldanha, R, Sands, W, Sangiorgio, S, Segreto, E, Semenov, D, Shields, E, Skorokhvatov, M, Smallcomb, M, Smirnov, O, Sotnikov, A, Suvurov, Y, Tartaglia, R, Tatarowicz, J, Testera, G, Tonazzo, A, Unzhakov, E, Vogelaar, RB, Wada, M, Walker, SE, Wang, H, Wang, Y, Watson, AW, Westerdale, S, Williams, R, Wojcik, M, Xu, J, Yang, CG, Yoo, J, Yu, B, Zavatarelli, S, Zhong, WL & Zuzel, G 2015, 'The darkside multiton detector for the direct dark matter search', Advances in High Energy Physics, vol. 2015, 541362. https://doi.org/10.1155/2015/541362

TY - JOUR

T1 - The darkside multiton detector for the direct dark matter search

AU - Aalseth, C. E.

AU - Agnes, P.

AU - Alton, A.

AU - Arisaka, K.

AU - Asner, D. M.

AU - Back, H. O.

AU - Baldin, B.

AU - Biery, K.

AU - Bonfini, G.

AU - Bossa, M.

AU - Brigatti, A.

AU - Brodsky, J.

AU - Budano, F.

AU - Cadonati, L.

AU - Cadoni, M.

AU - Calaprice, F.

AU - Canci, N.

AU - Candela, A.

AU - Cao, H.

AU - Cariello, M.

AU - Cavalcante, P.

AU - Chepurnov, A.

AU - Cocco, A. G.

AU - Condon, C.

AU - Crippa, L.

AU - D'Angelo, D.

AU - D'Incecco, M.

AU - Davini, S.

AU - De Deo, M.

AU - Derbin, A.

AU - Devoto, A.

AU - Di Eusanio, F.

AU - Edkins, E.

AU - Empl, A.

AU - Fan, A.

AU - Fiorillo, G.

AU - Fomenko, K.

AU - Forster, G.

AU - Foxe, M.

AU - Franco, D.

AU - Gabriele, F.

AU - Galbiati, C.

AU - Goretti, A.

AU - Grandi, L.

AU - Gromov, M.

AU - Guan, M. Y.

AU - Guardincerri, Y.

AU - Hackett, B.

AU - Herner, K.

AU - Hime, A.

AU - Humble, P.

AU - Hungerford, E.

AU - Ianni, Al

AU - Ianni, An

AU - Jaffe, D. E.

AU - Jollet, C.

AU - Keeter, K.

AU - Kendziora, C.

AU - Kidner, S.

AU - Kobychev, V.

AU - Koh, G.

AU - Korablev, D.

AU - Korga, G.

AU - Kurlej, A.

AU - Li, P. X.

AU - Lissia, M.

AU - Lombardi, P.

AU - Ludhova, L.

AU - Luitz, S.

AU - Lukyachenko, G.

AU - Ma, Y. Q.

AU - Machulin, I.

AU - Mandarano, A.

AU - Mari, S. M.

AU - Maricic, J.

AU - Marini, L.

AU - Markov, D.

AU - Martoff, J.

AU - Meregaglia, A.

AU - Meroni, E.

AU - Meyers, P. D.

AU - Miletic, T.

AU - Milincic, R.

AU - Montuschi, M.

AU - Monzani, M. E.

AU - Mosteiro, P.

AU - Mount, B.

AU - Muratova, V.

AU - Musico, P.

AU - Montanari, D.

AU - Nelson, A.

AU - Odrowski, S.

AU - Odrzywolek, A.

AU - Orrell, J. L.

AU - Orsini, M.

AU - Ortica, F.

AU - Pagani, L.

AU - Pallavicini, M.

AU - Pantic, E.

AU - Parmeggiano, S.

AU - Parsells, B.

AU - Pelczar, K.

AU - Pelliccia, N.

AU - Perasso, S.

AU - Perasso, L.

AU - Pocar, A.

AU - Pordes, S.

AU - Pugachev, D.

AU - Qian, H.

AU - Randle, K.

AU - Ranucci, G.

AU - Razeto, A.

AU - Recine, K.

AU - Reinhold, B.

AU - Renshaw, A.

AU - Romani, A.

AU - Rossi, N.

AU - Rossi, B.

AU - Rountree, S. D.

AU - Sablone, D.

AU - Saggese, P.

AU - Saldanha, R.

AU - Sands, W.

AU - Sangiorgio, S.

AU - Segreto, E.

AU - Semenov, D.

AU - Shields, E.

AU - Skorokhvatov, M.

AU - Smallcomb, M.

AU - Smirnov, O.

AU - Sotnikov, A.

AU - Suvurov, Y.

AU - Tartaglia, R.

AU - Tatarowicz, J.

AU - Testera, G.

AU - Tonazzo, A.

AU - Unzhakov, E.

AU - Vogelaar, R. B.

AU - Wada, M.

AU - Walker, S. E.

AU - Wang, H.

AU - Wang, Y.

AU - Watson, A. W.

AU - Westerdale, S.

AU - Williams, R.

AU - Wojcik, M.

AU - Xu, J.

AU - Yang, C. G.

AU - Yoo, J.

AU - Yu, B.

AU - Zavatarelli, S.

AU - Zhong, W. L.

AU - Zuzel, G.

PY - 2015/1/20

Y1 - 2015/1/20

N2 - Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (<100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide-50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.

AB - Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (<100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide-50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.

UR - http://www.scopus.com/inward/record.url?scp=84922384188&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84922384188&partnerID=8YFLogxK

U2 - 10.1155/2015/541362

DO - 10.1155/2015/541362

M3 - Article

AN - SCOPUS:84922384188

SN - 1687-7357

VL - 2015

JO - Advances in High Energy Physics

JF - Advances in High Energy Physics

M1 - 541362

ER -

The darkside multiton detector for the direct dark matter search

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this