Standard

The DarkSide experiment. / The ATLAS collaboration.

в: Nuovo Cimento della Societa Italiana di Fisica C, Том 40, № 1, 52, 01.01.2017.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

The ATLAS collaboration 2017, 'The DarkSide experiment', Nuovo Cimento della Societa Italiana di Fisica C, Том. 40, № 1, 52. https://doi.org/10.1393/ncc/i2017-17052-3

APA

The ATLAS collaboration (2017). The DarkSide experiment. Nuovo Cimento della Societa Italiana di Fisica C, 40(1), [52]. https://doi.org/10.1393/ncc/i2017-17052-3

Vancouver

The ATLAS collaboration. The DarkSide experiment. Nuovo Cimento della Societa Italiana di Fisica C. 2017 янв. 1;40(1):52. doi: 10.1393/ncc/i2017-17052-3

Author

The ATLAS collaboration. / The DarkSide experiment. в: Nuovo Cimento della Societa Italiana di Fisica C. 2017 ; Том 40, № 1.

BibTeX

@article{968da9dc72364fa9b3969be2031141c1,
title = "The DarkSide experiment",
abstract = "DarkSide is a dark matter direct search experiment at Laboratori Nazionali del Gran Sasso (LNGS). DarkSide is based on the detection of rare nuclear recoils possibly induced by hypothetical dark matter particles, which are supposed to be neutral, massive (m > 10 GeV) and weakly interactive (WIMP). The dark matter detector is a two-phase time projection chamber (TPC) filled with ultra-pure liquid argon. The TPC is placed inside a muon and a neutron active vetoes to suppress the background. Using argon as active target has many advantages, the key features are the strong discriminant power between nuclear and electron recoils, the spatial reconstruction and easy scalability to multi-tons size. At the moment DarkSide-50 is filled with ultra-pure argon, extracted from underground sources, and from April 2015 it is taking data in its final configuration. When combined with the preceding search with an atmospheric argon target, it is possible to set a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 2.0×10 -44 cm2 for a WIMP mass of 100 GeV/c2. The next phase of the experiment, DarkSide-20k, will be the construction of a new detector with an active mass of ∼ 20 tons.",
author = "{The ATLAS collaboration} and B. Bottino and Aalseth, {C. E.} and G. Acconcia and F. Acerbi and P. Agnes and L. Agostino and Albuquerque, {I. F.M.} and T. Alexander and A. Alton and P. Ampudia and R. Ardito and K. Arisaka and Arnquist, {I. J.} and Asner, {D. M.} and Back, {H. O.} and B. Baldin and G. Batignani and K. Biery and Bisogni, {M. G.} and V. Bocci and A. Bondar and G. Bonfini and W. Bonivento and M. Bossa and A. Brigatti and J. Brodsky and F. Budano and R. Bunker and S. Bussino and M. Buttafava and A. Buzulutskov and M. Cadeddu and M. Cadoni and N. Calandri and F. Calaprice and J. Calvo and L. Campajola and N. Canci and A. Candela and C. Cantini and H. Cao and M. Caravati and M. Cariello and M. Carlini and M. Carpinelli and A. Castellani and S. Catalanotti and P. Cavalcante and A. Dolgov and L. Shekhtman",
year = "2017",
month = jan,
day = "1",
doi = "10.1393/ncc/i2017-17052-3",
language = "English",
volume = "40",
journal = "Nuovo Cimento della Societa Italiana di Fisica C",
issn = "1124-1896",
publisher = "Editrice Compositori s.r.l.",
number = "1",

}

RIS

TY - JOUR

T1 - The DarkSide experiment

AU - The ATLAS collaboration

AU - Bottino, B.

AU - Aalseth, C. E.

AU - Acconcia, G.

AU - Acerbi, F.

AU - Agnes, P.

AU - Agostino, L.

AU - Albuquerque, I. F.M.

AU - Alexander, T.

AU - Alton, A.

AU - Ampudia, P.

AU - Ardito, R.

AU - Arisaka, K.

AU - Arnquist, I. J.

AU - Asner, D. M.

AU - Back, H. O.

AU - Baldin, B.

AU - Batignani, G.

AU - Biery, K.

AU - Bisogni, M. G.

AU - Bocci, V.

AU - Bondar, A.

AU - Bonfini, G.

AU - Bonivento, W.

AU - Bossa, M.

AU - Brigatti, A.

AU - Brodsky, J.

AU - Budano, F.

AU - Bunker, R.

AU - Bussino, S.

AU - Buttafava, M.

AU - Buzulutskov, A.

AU - Cadeddu, M.

AU - Cadoni, M.

AU - Calandri, N.

AU - Calaprice, F.

AU - Calvo, J.

AU - Campajola, L.

AU - Canci, N.

AU - Candela, A.

AU - Cantini, C.

AU - Cao, H.

AU - Caravati, M.

AU - Cariello, M.

AU - Carlini, M.

AU - Carpinelli, M.

AU - Castellani, A.

AU - Catalanotti, S.

AU - Cavalcante, P.

AU - Dolgov, A.

AU - Shekhtman, L.

PY - 2017/1/1

Y1 - 2017/1/1

N2 - DarkSide is a dark matter direct search experiment at Laboratori Nazionali del Gran Sasso (LNGS). DarkSide is based on the detection of rare nuclear recoils possibly induced by hypothetical dark matter particles, which are supposed to be neutral, massive (m > 10 GeV) and weakly interactive (WIMP). The dark matter detector is a two-phase time projection chamber (TPC) filled with ultra-pure liquid argon. The TPC is placed inside a muon and a neutron active vetoes to suppress the background. Using argon as active target has many advantages, the key features are the strong discriminant power between nuclear and electron recoils, the spatial reconstruction and easy scalability to multi-tons size. At the moment DarkSide-50 is filled with ultra-pure argon, extracted from underground sources, and from April 2015 it is taking data in its final configuration. When combined with the preceding search with an atmospheric argon target, it is possible to set a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 2.0×10 -44 cm2 for a WIMP mass of 100 GeV/c2. The next phase of the experiment, DarkSide-20k, will be the construction of a new detector with an active mass of ∼ 20 tons.

AB - DarkSide is a dark matter direct search experiment at Laboratori Nazionali del Gran Sasso (LNGS). DarkSide is based on the detection of rare nuclear recoils possibly induced by hypothetical dark matter particles, which are supposed to be neutral, massive (m > 10 GeV) and weakly interactive (WIMP). The dark matter detector is a two-phase time projection chamber (TPC) filled with ultra-pure liquid argon. The TPC is placed inside a muon and a neutron active vetoes to suppress the background. Using argon as active target has many advantages, the key features are the strong discriminant power between nuclear and electron recoils, the spatial reconstruction and easy scalability to multi-tons size. At the moment DarkSide-50 is filled with ultra-pure argon, extracted from underground sources, and from April 2015 it is taking data in its final configuration. When combined with the preceding search with an atmospheric argon target, it is possible to set a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 2.0×10 -44 cm2 for a WIMP mass of 100 GeV/c2. The next phase of the experiment, DarkSide-20k, will be the construction of a new detector with an active mass of ∼ 20 tons.

UR - http://www.scopus.com/inward/record.url?scp=85013760395&partnerID=8YFLogxK

U2 - 10.1393/ncc/i2017-17052-3

DO - 10.1393/ncc/i2017-17052-3

M3 - Article

AN - SCOPUS:85013760395

VL - 40

JO - Nuovo Cimento della Societa Italiana di Fisica C

JF - Nuovo Cimento della Societa Italiana di Fisica C

SN - 1124-1896

IS - 1

M1 - 52

ER -

ID: 10181467