Readout technologies for directional WIMP Dark Matter detection

J. B.R. Battat; I. G. Irastorza; A. Aleksandrov; T. Asada; E. Baracchini; J. Billard; G. Bosson; O. Bourrion; J. Bouvier; A. Buonaura; K. Burdge; S. Cebrián; P. Colas; L. Consiglio; T. Dafni; N. D'Ambrosio; C. Deaconu; G. De Lellis; T. Descombes; A. Di Crescenzo; N. Di Marco; G. Druitt; R. Eggleston; E. Ferrer-Ribas; T. Fusayasu; J. Galán; G. Galati; J. A. García; J. G. Garza; V. Gentile; M. Garcia-Sciveres; Y. Giomataris; N. Guerrero; O. Guillaudin; A. M. Guler; J. Harton; T. Hashimoto; M. T. Hedges; F. J. Iguaz; T. Ikeda; I. Jaegle; J. A. Kadyk; T. Katsuragawa; S. Komura; H. Kubo; K. Kuge; J. Lamblin; A. Lauria; E. R. Lee; P. Lewis; M. Leyton; D. Loomba; J. P. Lopez; G. Luzón; F. Mayet; H. Mirallas; K. Miuchi; T. Mizumoto; Y. Mizumura; P. Monacelli; J. Monroe; M. C. Montesi; T. Naka; K. Nakamura; H. Nishimura; A. Ochi; T. Papevangelou; J. D. Parker; N. S. Phan; F. Pupilli; J. P. Richer; Q. Riffard; G. Rosa; D. Santos; T. Sawano; H. Sekiya; I. S. Seong; D. P. Snowden-Ifft; N. J.C. Spooner; A. Sugiyama; R. Taishaku; A. Takada; A. Takeda; M. Tanaka; T. Tanimori; T. N. Thorpe; V. Tioukov; H. Tomita; A. Umemoto; S. E. Vahsen; Y. Yamaguchi; M. Yoshimoto; E. Zayas

doi:10.1016/j.physrep.2016.10.001

Readout technologies for directional WIMP Dark Matter detection

J. B.R. Battat, I. G. Irastorza, A. Aleksandrov, T. Asada, E. Baracchini, J. Billard, G. Bosson, O. Bourrion, J. Bouvier, A. Buonaura, K. Burdge, S. Cebrián, P. Colas, L. Consiglio, T. Dafni, N. D'Ambrosio, C. Deaconu, G. De Lellis, T. Descombes, A. Di CrescenzoN. Di Marco, G. Druitt, R. Eggleston, E. Ferrer-Ribas, T. Fusayasu, J. Galán, G. Galati, J. A. García, J. G. Garza, V. Gentile, M. Garcia-Sciveres, Y. Giomataris, N. Guerrero, O. Guillaudin, A. M. Guler, J. Harton, T. Hashimoto, M. T. Hedges, F. J. Iguaz, T. Ikeda, I. Jaegle, J. A. Kadyk, T. Katsuragawa, S. Komura, H. Kubo, K. Kuge, J. Lamblin, A. Lauria, E. R. Lee, P. Lewis, M. Leyton, D. Loomba, J. P. Lopez, G. Luzón, F. Mayet, H. Mirallas, K. Miuchi, T. Mizumoto, Y. Mizumura, P. Monacelli, J. Monroe, M. C. Montesi, T. Naka, K. Nakamura, H. Nishimura, A. Ochi, T. Papevangelou, J. D. Parker, N. S. Phan, F. Pupilli, J. P. Richer, Q. Riffard, G. Rosa, D. Santos, T. Sawano, H. Sekiya, I. S. Seong, D. P. Snowden-Ifft, N. J.C. Spooner, A. Sugiyama, R. Taishaku, A. Takada, A. Takeda, M. Tanaka, T. Tanimori, T. N. Thorpe, V. Tioukov, H. Tomita, A. Umemoto, S. E. Vahsen, Y. Yamaguchi, M. Yoshimoto, E. Zayas

研究成果: Review article › 査読

64 被引用数 (Scopus)

抄録

The measurement of the direction of WIMP-induced nuclear recoils is a compelling but technologically challenging strategy to provide an unambiguous signature of the detection of Galactic dark matter. Most directional detectors aim to reconstruct the dark-matter-induced nuclear recoil tracks, either in gas or solid targets. The main challenge with directional detection is the need for high spatial resolution over large volumes, which puts strong requirements on the readout technologies. In this paper we review the various detector readout technologies used by directional detectors. In particular, we summarize the challenges, advantages and drawbacks of each approach, and discuss future prospects for these technologies.

本文言語	English
ページ（範囲）	1-46
ページ数	46
ジャーナル	Physics Reports
巻	662
DOI	https://doi.org/10.1016/j.physrep.2016.10.001
出版ステータス	Published - 2016 11月 29
外部発表	はい

ASJC Scopus subject areas

物理学および天文学（全般）

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10.1016/j.physrep.2016.10.001

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Battat, J. B. R., Irastorza, I. G., Aleksandrov, A., Asada, T., Baracchini, E., Billard, J., Bosson, G., Bourrion, O., Bouvier, J., Buonaura, A., Burdge, K., Cebrián, S., Colas, P., Consiglio, L., Dafni, T., D'Ambrosio, N., Deaconu, C., De Lellis, G., Descombes, T., ... Zayas, E. (2016). Readout technologies for directional WIMP Dark Matter detection. Physics Reports, 662, 1-46. https://doi.org/10.1016/j.physrep.2016.10.001

Battat, JBR, Irastorza, IG, Aleksandrov, A, Asada, T, Baracchini, E, Billard, J, Bosson, G, Bourrion, O, Bouvier, J, Buonaura, A, Burdge, K, Cebrián, S, Colas, P, Consiglio, L, Dafni, T, D'Ambrosio, N, Deaconu, C, De Lellis, G, Descombes, T, Di Crescenzo, A, Di Marco, N, Druitt, G, Eggleston, R, Ferrer-Ribas, E, Fusayasu, T, Galán, J, Galati, G, García, JA, Garza, JG, Gentile, V, Garcia-Sciveres, M, Giomataris, Y, Guerrero, N, Guillaudin, O, Guler, AM, Harton, J, Hashimoto, T, Hedges, MT, Iguaz, FJ, Ikeda, T, Jaegle, I, Kadyk, JA, Katsuragawa, T, Komura, S, Kubo, H, Kuge, K, Lamblin, J, Lauria, A, Lee, ER, Lewis, P, Leyton, M, Loomba, D, Lopez, JP, Luzón, G, Mayet, F, Mirallas, H, Miuchi, K, Mizumoto, T, Mizumura, Y, Monacelli, P, Monroe, J, Montesi, MC, Naka, T, Nakamura, K, Nishimura, H, Ochi, A, Papevangelou, T, Parker, JD, Phan, NS, Pupilli, F, Richer, JP, Riffard, Q, Rosa, G, Santos, D, Sawano, T, Sekiya, H, Seong, IS, Snowden-Ifft, DP, Spooner, NJC, Sugiyama, A, Taishaku, R, Takada, A, Takeda, A, Tanaka, M, Tanimori, T, Thorpe, TN, Tioukov, V, Tomita, H, Umemoto, A, Vahsen, SE, Yamaguchi, Y, Yoshimoto, M & Zayas, E 2016, 'Readout technologies for directional WIMP Dark Matter detection', Physics Reports, vol. 662, pp. 1-46. https://doi.org/10.1016/j.physrep.2016.10.001

@article{db241f86dc7040b193de4cad5c5542f6,

title = "Readout technologies for directional WIMP Dark Matter detection",

abstract = "The measurement of the direction of WIMP-induced nuclear recoils is a compelling but technologically challenging strategy to provide an unambiguous signature of the detection of Galactic dark matter. Most directional detectors aim to reconstruct the dark-matter-induced nuclear recoil tracks, either in gas or solid targets. The main challenge with directional detection is the need for high spatial resolution over large volumes, which puts strong requirements on the readout technologies. In this paper we review the various detector readout technologies used by directional detectors. In particular, we summarize the challenges, advantages and drawbacks of each approach, and discuss future prospects for these technologies.",

keywords = "Dark Matter detectors, Gaseous imaging and tracking detectors, Micropattern gaseous detectors, Nuclear emulsions, Time Projection Chambers, Wire chambers",

author = "Battat, {J. B.R.} and Irastorza, {I. G.} and A. Aleksandrov and T. Asada and E. Baracchini and J. Billard and G. Bosson and O. Bourrion and J. Bouvier and A. Buonaura and K. Burdge and S. Cebri{\'a}n and P. Colas and L. Consiglio and T. Dafni and N. D'Ambrosio and C. Deaconu and {De Lellis}, G. and T. Descombes and {Di Crescenzo}, A. and {Di Marco}, N. and G. Druitt and R. Eggleston and E. Ferrer-Ribas and T. Fusayasu and J. Gal{\'a}n and G. Galati and Garc{\'i}a, {J. A.} and Garza, {J. G.} and V. Gentile and M. Garcia-Sciveres and Y. Giomataris and N. Guerrero and O. Guillaudin and Guler, {A. M.} and J. Harton and T. Hashimoto and Hedges, {M. T.} and Iguaz, {F. J.} and T. Ikeda and I. Jaegle and Kadyk, {J. A.} and T. Katsuragawa and S. Komura and H. Kubo and K. Kuge and J. Lamblin and A. Lauria and Lee, {E. R.} and P. Lewis and M. Leyton and D. Loomba and Lopez, {J. P.} and G. Luz{\'o}n and F. Mayet and H. Mirallas and K. Miuchi and T. Mizumoto and Y. Mizumura and P. Monacelli and J. Monroe and Montesi, {M. C.} and T. Naka and K. Nakamura and H. Nishimura and A. Ochi and T. Papevangelou and Parker, {J. D.} and Phan, {N. S.} and F. Pupilli and Richer, {J. P.} and Q. Riffard and G. Rosa and D. Santos and T. Sawano and H. Sekiya and Seong, {I. S.} and Snowden-Ifft, {D. P.} and Spooner, {N. J.C.} and A. Sugiyama and R. Taishaku and A. Takada and A. Takeda and M. Tanaka and T. Tanimori and Thorpe, {T. N.} and V. Tioukov and H. Tomita and A. Umemoto and Vahsen, {S. E.} and Y. Yamaguchi and M. Yoshimoto and E. Zayas",

note = "Funding Information: J.B.R.B. acknowledges the support of the Alfred P. Sloan Foundation ( BR2012-011 ), the National Science Foundation ( PHY-1649966 ), the Research Corporation for Science Advancement (Award #23325 ), the Massachusetts Space Grant Consortium ( NNX16AH49H ), and the Wellesley College Summer Science Research program ( 26179 ). I.G.I. and the Zaragoza group acknowledges support from the European Research Council (ERC) through the ERC-2009-StG-240054 grant (T-REX project) as well as from the Spanish Ministry of Economy and Competitiveness under grants FPA2008-03456 , FPA2011-24058 , and FPA2013-41085-P . This work was partially supported by the European Union{\textquoteright}s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 657751 . This work was supported in part by the Office of High Energy Physics of the U.S. Department of Energy (DoE) under contract DE-AC02-05CH11231 . F.I. acknowledges the support from the Juan de la Cierva program ( JCI-2012-13882 ). D.L. acknowledges support from the National Science Foundation (NSF) under grants 1407773 and 1506329 . This work was partially supported by KAKENHI Grant-in-Aids for Young Scientist(A) ( 16684004 , 19684005 , 23684014 , 15H05446 ) KAKENHI Grant-in-Aid for Scientific Research on Innovative Area ( 26104005 ); KAKENHI Grant-in-Aids for Scientific Research(A) ( 16H02189 ); KAKENHI Grant-in-Aids for Scientific Research(B) ( 21340063 ); KAKENHI Grant-in-Aids for Challenging Exploratory Research ( 23654084 , 15K13485 ); KAKENHI Grant-in-Aids for JSPS Fellows ( 23-812 ); from the Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan. This work was partially supported by Program for Advancing Strategic International Networks to Accelerate the Circulation of Talented Researchers, JSPS, Japan ( R2607 ). The Royal Holloway, University of London group is supported by ERC Starting Grant number ERC StG 279980 and STFC grant ST/N00034X/1 . D.P.S.I. acknowledges support from the NSF under grants 1407754 , 1103511 , 1521027 and 1506237 , and undergraduate student support from Occidental College Undergraduate Research Center summer program . S.V. and the Hawaii group acknowledge support from the U.S. Department of Homeland Security under Award Number 2011-DN-077-ARI050-03 and the DoE under Award Numbers DE-SC0007852 and DE-SC0010504 . Finally, we thank the anonymous referee for their helpful comments. Publisher Copyright: {\textcopyright} 2016 Elsevier B.V.",

year = "2016",

month = nov,

day = "29",

doi = "10.1016/j.physrep.2016.10.001",

language = "English",

volume = "662",

pages = "1--46",

journal = "Physics Reports",

issn = "0370-1573",

publisher = "Elsevier",

}

TY - JOUR

T1 - Readout technologies for directional WIMP Dark Matter detection

AU - Battat, J. B.R.

AU - Irastorza, I. G.

AU - Aleksandrov, A.

AU - Asada, T.

AU - Baracchini, E.

AU - Billard, J.

AU - Bosson, G.

AU - Bourrion, O.

AU - Bouvier, J.

AU - Buonaura, A.

AU - Burdge, K.

AU - Cebrián, S.

AU - Colas, P.

AU - Consiglio, L.

AU - Dafni, T.

AU - D'Ambrosio, N.

AU - Deaconu, C.

AU - De Lellis, G.

AU - Descombes, T.

AU - Di Crescenzo, A.

AU - Di Marco, N.

AU - Druitt, G.

AU - Eggleston, R.

AU - Ferrer-Ribas, E.

AU - Fusayasu, T.

AU - Galán, J.

AU - Galati, G.

AU - García, J. A.

AU - Garza, J. G.

AU - Gentile, V.

AU - Garcia-Sciveres, M.

AU - Giomataris, Y.

AU - Guerrero, N.

AU - Guillaudin, O.

AU - Guler, A. M.

AU - Harton, J.

AU - Hashimoto, T.

AU - Hedges, M. T.

AU - Iguaz, F. J.

AU - Ikeda, T.

AU - Jaegle, I.

AU - Kadyk, J. A.

AU - Katsuragawa, T.

AU - Komura, S.

AU - Kubo, H.

AU - Kuge, K.

AU - Lamblin, J.

AU - Lauria, A.

AU - Lee, E. R.

AU - Lewis, P.

AU - Leyton, M.

AU - Loomba, D.

AU - Lopez, J. P.

AU - Luzón, G.

AU - Mayet, F.

AU - Mirallas, H.

AU - Miuchi, K.

AU - Mizumoto, T.

AU - Mizumura, Y.

AU - Monacelli, P.

AU - Monroe, J.

AU - Montesi, M. C.

AU - Naka, T.

AU - Nakamura, K.

AU - Nishimura, H.

AU - Ochi, A.

AU - Papevangelou, T.

AU - Parker, J. D.

AU - Phan, N. S.

AU - Pupilli, F.

AU - Richer, J. P.

AU - Riffard, Q.

AU - Rosa, G.

AU - Santos, D.

AU - Sawano, T.

AU - Sekiya, H.

AU - Seong, I. S.

AU - Snowden-Ifft, D. P.

AU - Spooner, N. J.C.

AU - Sugiyama, A.

AU - Taishaku, R.

AU - Takada, A.

AU - Takeda, A.

AU - Tanaka, M.

AU - Tanimori, T.

AU - Thorpe, T. N.

AU - Tioukov, V.

AU - Tomita, H.

AU - Umemoto, A.

AU - Vahsen, S. E.

AU - Yamaguchi, Y.

AU - Yoshimoto, M.

AU - Zayas, E.

N1 - Funding Information: J.B.R.B. acknowledges the support of the Alfred P. Sloan Foundation ( BR2012-011 ), the National Science Foundation ( PHY-1649966 ), the Research Corporation for Science Advancement (Award #23325 ), the Massachusetts Space Grant Consortium ( NNX16AH49H ), and the Wellesley College Summer Science Research program ( 26179 ). I.G.I. and the Zaragoza group acknowledges support from the European Research Council (ERC) through the ERC-2009-StG-240054 grant (T-REX project) as well as from the Spanish Ministry of Economy and Competitiveness under grants FPA2008-03456 , FPA2011-24058 , and FPA2013-41085-P . This work was partially supported by the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 657751 . This work was supported in part by the Office of High Energy Physics of the U.S. Department of Energy (DoE) under contract DE-AC02-05CH11231 . F.I. acknowledges the support from the Juan de la Cierva program ( JCI-2012-13882 ). D.L. acknowledges support from the National Science Foundation (NSF) under grants 1407773 and 1506329 . This work was partially supported by KAKENHI Grant-in-Aids for Young Scientist(A) ( 16684004 , 19684005 , 23684014 , 15H05446 ) KAKENHI Grant-in-Aid for Scientific Research on Innovative Area ( 26104005 ); KAKENHI Grant-in-Aids for Scientific Research(A) ( 16H02189 ); KAKENHI Grant-in-Aids for Scientific Research(B) ( 21340063 ); KAKENHI Grant-in-Aids for Challenging Exploratory Research ( 23654084 , 15K13485 ); KAKENHI Grant-in-Aids for JSPS Fellows ( 23-812 ); from the Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan. This work was partially supported by Program for Advancing Strategic International Networks to Accelerate the Circulation of Talented Researchers, JSPS, Japan ( R2607 ). The Royal Holloway, University of London group is supported by ERC Starting Grant number ERC StG 279980 and STFC grant ST/N00034X/1 . D.P.S.I. acknowledges support from the NSF under grants 1407754 , 1103511 , 1521027 and 1506237 , and undergraduate student support from Occidental College Undergraduate Research Center summer program . S.V. and the Hawaii group acknowledge support from the U.S. Department of Homeland Security under Award Number 2011-DN-077-ARI050-03 and the DoE under Award Numbers DE-SC0007852 and DE-SC0010504 . Finally, we thank the anonymous referee for their helpful comments. Publisher Copyright: © 2016 Elsevier B.V.

PY - 2016/11/29

Y1 - 2016/11/29

N2 - The measurement of the direction of WIMP-induced nuclear recoils is a compelling but technologically challenging strategy to provide an unambiguous signature of the detection of Galactic dark matter. Most directional detectors aim to reconstruct the dark-matter-induced nuclear recoil tracks, either in gas or solid targets. The main challenge with directional detection is the need for high spatial resolution over large volumes, which puts strong requirements on the readout technologies. In this paper we review the various detector readout technologies used by directional detectors. In particular, we summarize the challenges, advantages and drawbacks of each approach, and discuss future prospects for these technologies.

AB - The measurement of the direction of WIMP-induced nuclear recoils is a compelling but technologically challenging strategy to provide an unambiguous signature of the detection of Galactic dark matter. Most directional detectors aim to reconstruct the dark-matter-induced nuclear recoil tracks, either in gas or solid targets. The main challenge with directional detection is the need for high spatial resolution over large volumes, which puts strong requirements on the readout technologies. In this paper we review the various detector readout technologies used by directional detectors. In particular, we summarize the challenges, advantages and drawbacks of each approach, and discuss future prospects for these technologies.

KW - Dark Matter detectors

KW - Gaseous imaging and tracking detectors

KW - Micropattern gaseous detectors

KW - Nuclear emulsions

KW - Time Projection Chambers

KW - Wire chambers

UR - http://www.scopus.com/inward/record.url?scp=84995761502&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84995761502&partnerID=8YFLogxK

U2 - 10.1016/j.physrep.2016.10.001

DO - 10.1016/j.physrep.2016.10.001

M3 - Review article

AN - SCOPUS:84995761502

VL - 662

SP - 1

EP - 46

JO - Physics Reports

JF - Physics Reports

SN - 0370-1573

ER -

Readout technologies for directional WIMP Dark Matter detection

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