The DarkSide direct dark matter search with liquid argon
The DarkSide-50 direct dark matter detector is a liquid argon time projection chamber (TPC) surrounded by a liquid scintillator neutron veto (LSV) and a water Cerenkov muon veto (WCV). Located under 3800 m.w.e. at the Laboratori Nazionali del Gran Sasso, Italy, it is the only direct dark matter expe...
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| creator | Edkins, E. Agnes, P. Alton, A. Arisaka, K. Baldin, B. Biery, K. Bossa, M. Brigatti, A. Budano, F. Calaprice, F. Canci, N. Candela, A. Cao, H. Cariello, M. Cavalcante, P. Chavarria, A. Chepurnov, A. Cocco, A. G. Crippa, L. D’Angelo, D. D’Incecco, M. Davini, S. De Deo, M. Derbin, A. Devoto, A. Di Eusanio, F. Di Pietro, G. Franco, D. Gabriele, F. Gromov, M. Hackett, B. Humble, P. Hungerford, E. V. Ianni, Al Ianni, An Jollet, C. Keeter, K. Kendziora, C. Korablev, D. Kurlej, A. Li, P. X. Loer, B. Love, C. Luitz, S. Mandarano, A. Marini, L. Martoff, C. J. Meregaglia, A. Meroni, E. Meyers, P. D. Milincic, R. Monzani, M. E. Musico, P. Nelson, A. Odrowski, S. Orsini, M. Ortica, F. Pagani, L. Pantic, E. Papp, L. Parmeggiano, S. Parsells, R. Pelczar, K. Pelliccia, N. Perasso, S. Pocar, A. Pordes, S. Pugachev, D. Qian, H. Randle, K. Ranucci, G. Razeto, A. Reinhold, B. Renshaw, A. Romani, A. Rountree, S. D. Sablone, D. Saggese, P. Segreto, E. Shields, E. Skorokhvatov, M. Smirnov, O. Sotnikov, A. Stanford, C. Suvorov, Y. Tartaglia, R. Tatarowicz, J. Testera, G. Unzhakov, E. Vogelaar, R. B. Walker, S. Wang, H. Wang, Y. Watson, A. Westerdale, S. Wojcik, M. Wright, A. Xiang, X. Yoo, J. Zavatarelli, S. |
| description | The DarkSide-50 direct dark matter detector is a liquid argon time projection chamber (TPC) surrounded by a liquid scintillator neutron veto (LSV) and a water Cerenkov muon veto (WCV). Located under 3800 m.w.e. at the Laboratori Nazionali del Gran Sasso, Italy, it is the only direct dark matter experiment currently operating background free. The atmospheric argon target was replaced with argon from underground sources in April, 2015. The level of 39Ar, a β emitter present in atmospheric argon (AAr), has been shown to have been reduced by a factor of (1.4 ± 0.2) x 103. The combined spin-independent WIMP exclusion limit of 2.0 x 10−44 cm2 (mχ
= 100 GeV/c
2) is currently the best limit on a liquid argon target. |
| doi_str_mv | 10.1063/1.5010122 |
| format | Conference Proceeding |
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= 100 GeV/c
2) is currently the best limit on a liquid argon target.</description><identifier>ISSN: 0094-243X</identifier><identifier>EISSN: 1551-7616</identifier><identifier>DOI: 10.1063/1.5010122</identifier><identifier>CODEN: APCPCS</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Argon ; Astrophysics ; Dark matter ; Emitters ; Instrumentation and Detectors ; Physics ; Radiation counters ; Scintillation counters</subject><ispartof>AIP Conf.Proc, 2017, Vol.1900 (1)</ispartof><rights>Author(s)</rights><rights>2017 Author(s). Published by AIP Publishing.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0001-7309-3023 ; 0000-0001-9611-2004 ; 0000-0001-9888-9175 ; 0000-0002-7790-1224 ; 0000-0002-2934-9148 ; 0000-0001-7117-1251 ; 0000-0001-8824-6205 ; 0000-0003-2913-8057 ; 0000-0002-6916-6776</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/acp/article-lookup/doi/10.1063/1.5010122$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>309,310,314,776,780,785,786,790,881,4498,23909,23910,25118,27901,27902,76126</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01645658$$DView record in HAL$$Hfree_for_read</backlink></links><search><contributor>Raby, Stuart</contributor><contributor>Sandick, Pearl</contributor><contributor>Kumar, Jason</contributor><contributor>Babu, Kaladi</contributor><contributor>Balantekin, Baha</contributor><contributor>Strigari, Louis</contributor><contributor>Szczerbinska, Barbara</contributor><contributor>Mishra, Sanjib</contributor><creatorcontrib>Edkins, E.</creatorcontrib><creatorcontrib>Agnes, P.</creatorcontrib><creatorcontrib>Alton, A.</creatorcontrib><creatorcontrib>Arisaka, K.</creatorcontrib><creatorcontrib>Baldin, B.</creatorcontrib><creatorcontrib>Biery, K.</creatorcontrib><creatorcontrib>Bossa, M.</creatorcontrib><creatorcontrib>Brigatti, A.</creatorcontrib><creatorcontrib>Budano, F.</creatorcontrib><creatorcontrib>Calaprice, F.</creatorcontrib><creatorcontrib>Canci, N.</creatorcontrib><creatorcontrib>Candela, A.</creatorcontrib><creatorcontrib>Cao, H.</creatorcontrib><creatorcontrib>Cariello, M.</creatorcontrib><creatorcontrib>Cavalcante, P.</creatorcontrib><creatorcontrib>Chavarria, A.</creatorcontrib><creatorcontrib>Chepurnov, A.</creatorcontrib><creatorcontrib>Cocco, A. 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V.</creatorcontrib><creatorcontrib>Ianni, Al</creatorcontrib><creatorcontrib>Ianni, An</creatorcontrib><creatorcontrib>Jollet, C.</creatorcontrib><creatorcontrib>Keeter, K.</creatorcontrib><creatorcontrib>Kendziora, C.</creatorcontrib><creatorcontrib>Korablev, D.</creatorcontrib><creatorcontrib>Kurlej, A.</creatorcontrib><creatorcontrib>Li, P. X.</creatorcontrib><creatorcontrib>Loer, B.</creatorcontrib><creatorcontrib>Love, C.</creatorcontrib><creatorcontrib>Luitz, S.</creatorcontrib><creatorcontrib>Mandarano, A.</creatorcontrib><creatorcontrib>Marini, L.</creatorcontrib><creatorcontrib>Martoff, C. J.</creatorcontrib><creatorcontrib>Meregaglia, A.</creatorcontrib><creatorcontrib>Meroni, E.</creatorcontrib><creatorcontrib>Meyers, P. D.</creatorcontrib><creatorcontrib>Milincic, R.</creatorcontrib><creatorcontrib>Monzani, M. E.</creatorcontrib><creatorcontrib>Musico, P.</creatorcontrib><creatorcontrib>Nelson, A.</creatorcontrib><creatorcontrib>Odrowski, S.</creatorcontrib><creatorcontrib>Orsini, M.</creatorcontrib><creatorcontrib>Ortica, F.</creatorcontrib><creatorcontrib>Pagani, L.</creatorcontrib><creatorcontrib>Pantic, E.</creatorcontrib><creatorcontrib>Papp, L.</creatorcontrib><creatorcontrib>Parmeggiano, S.</creatorcontrib><creatorcontrib>Parsells, R.</creatorcontrib><creatorcontrib>Pelczar, K.</creatorcontrib><creatorcontrib>Pelliccia, N.</creatorcontrib><creatorcontrib>Perasso, S.</creatorcontrib><creatorcontrib>Pocar, A.</creatorcontrib><creatorcontrib>Pordes, S.</creatorcontrib><creatorcontrib>Pugachev, D.</creatorcontrib><creatorcontrib>Qian, H.</creatorcontrib><creatorcontrib>Randle, K.</creatorcontrib><creatorcontrib>Ranucci, G.</creatorcontrib><creatorcontrib>Razeto, A.</creatorcontrib><creatorcontrib>Reinhold, B.</creatorcontrib><creatorcontrib>Renshaw, A.</creatorcontrib><creatorcontrib>Romani, A.</creatorcontrib><creatorcontrib>Rountree, S. D.</creatorcontrib><creatorcontrib>Sablone, D.</creatorcontrib><creatorcontrib>Saggese, P.</creatorcontrib><creatorcontrib>Segreto, E.</creatorcontrib><creatorcontrib>Shields, E.</creatorcontrib><creatorcontrib>Skorokhvatov, M.</creatorcontrib><creatorcontrib>Smirnov, O.</creatorcontrib><creatorcontrib>Sotnikov, A.</creatorcontrib><creatorcontrib>Stanford, C.</creatorcontrib><creatorcontrib>Suvorov, Y.</creatorcontrib><creatorcontrib>Tartaglia, R.</creatorcontrib><creatorcontrib>Tatarowicz, J.</creatorcontrib><creatorcontrib>Testera, G.</creatorcontrib><creatorcontrib>Unzhakov, E.</creatorcontrib><creatorcontrib>Vogelaar, R. B.</creatorcontrib><creatorcontrib>Walker, S.</creatorcontrib><creatorcontrib>Wang, H.</creatorcontrib><creatorcontrib>Wang, Y.</creatorcontrib><creatorcontrib>Watson, A.</creatorcontrib><creatorcontrib>Westerdale, S.</creatorcontrib><creatorcontrib>Wojcik, M.</creatorcontrib><creatorcontrib>Wright, A.</creatorcontrib><creatorcontrib>Xiang, X.</creatorcontrib><creatorcontrib>Yoo, J.</creatorcontrib><creatorcontrib>Zavatarelli, S.</creatorcontrib><title>The DarkSide direct dark matter search with liquid argon</title><title>AIP Conf.Proc</title><description>The DarkSide-50 direct dark matter detector is a liquid argon time projection chamber (TPC) surrounded by a liquid scintillator neutron veto (LSV) and a water Cerenkov muon veto (WCV). Located under 3800 m.w.e. at the Laboratori Nazionali del Gran Sasso, Italy, it is the only direct dark matter experiment currently operating background free. The atmospheric argon target was replaced with argon from underground sources in April, 2015. The level of 39Ar, a β emitter present in atmospheric argon (AAr), has been shown to have been reduced by a factor of (1.4 ± 0.2) x 103. The combined spin-independent WIMP exclusion limit of 2.0 x 10−44 cm2 (mχ
= 100 GeV/c
2) is currently the best limit on a liquid argon target.</description><subject>Argon</subject><subject>Astrophysics</subject><subject>Dark matter</subject><subject>Emitters</subject><subject>Instrumentation and Detectors</subject><subject>Physics</subject><subject>Radiation counters</subject><subject>Scintillation counters</subject><issn>0094-243X</issn><issn>1551-7616</issn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2017</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNp9kE9LAzEQxYMoWKsHv0HAk8LWmWQ32RyL_yoUPFjBW0g3iZvadttsWvHbu6VFb56GN_zmveERcokwQBD8FgcFICBjR6SHRYGZFCiOSQ9A5RnL-fspOWvbGQBTUpY9Uk5qR-9N_HwN1lEboqsStZ2mC5OSi7R1JlY1_QqppvOw3gRLTfxolufkxJt56y4Os0_eHh8md6Ns_PL0fDccZzUrZcq6FMOEzC0DA2BdaWEqnBJT4UEJVTrPuJfSc26VFWgKyznzkPvKiKn1yPvkeu9bm7lexbAw8Vs3JujRcKx3O0CRF6Iotzv2as-uYrPeuDbpWbOJy-49zRAFQJ6XqqNu9lRbhWRSaJa_vtsmatSHBvXK-v9gBL2r_O-A_wBpmnBH</recordid><startdate>20171103</startdate><enddate>20171103</enddate><creator>Edkins, E.</creator><creator>Agnes, P.</creator><creator>Alton, A.</creator><creator>Arisaka, K.</creator><creator>Baldin, B.</creator><creator>Biery, K.</creator><creator>Bossa, M.</creator><creator>Brigatti, A.</creator><creator>Budano, F.</creator><creator>Calaprice, F.</creator><creator>Canci, N.</creator><creator>Candela, A.</creator><creator>Cao, H.</creator><creator>Cariello, M.</creator><creator>Cavalcante, P.</creator><creator>Chavarria, A.</creator><creator>Chepurnov, A.</creator><creator>Cocco, A. 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G. ; Crippa, L. ; D’Angelo, D. ; D’Incecco, M. ; Davini, S. ; De Deo, M. ; Derbin, A. ; Devoto, A. ; Di Eusanio, F. ; Di Pietro, G. ; Franco, D. ; Gabriele, F. ; Gromov, M. ; Hackett, B. ; Humble, P. ; Hungerford, E. V. ; Ianni, Al ; Ianni, An ; Jollet, C. ; Keeter, K. ; Kendziora, C. ; Korablev, D. ; Kurlej, A. ; Li, P. X. ; Loer, B. ; Love, C. ; Luitz, S. ; Mandarano, A. ; Marini, L. ; Martoff, C. J. ; Meregaglia, A. ; Meroni, E. ; Meyers, P. D. ; Milincic, R. ; Monzani, M. E. ; Musico, P. ; Nelson, A. ; Odrowski, S. ; Orsini, M. ; Ortica, F. ; Pagani, L. ; Pantic, E. ; Papp, L. ; Parmeggiano, S. ; Parsells, R. ; Pelczar, K. ; Pelliccia, N. ; Perasso, S. ; Pocar, A. ; Pordes, S. ; Pugachev, D. ; Qian, H. ; Randle, K. ; Ranucci, G. ; Razeto, A. ; Reinhold, B. ; Renshaw, A. ; Romani, A. ; Rountree, S. D. ; Sablone, D. ; Saggese, P. ; Segreto, E. ; Shields, E. ; Skorokhvatov, M. ; Smirnov, O. ; Sotnikov, A. ; Stanford, C. ; Suvorov, Y. ; Tartaglia, R. ; Tatarowicz, J. ; Testera, G. ; Unzhakov, E. ; Vogelaar, R. B. ; Walker, S. ; Wang, H. ; Wang, Y. ; Watson, A. ; Westerdale, S. ; Wojcik, M. ; Wright, A. ; Xiang, X. ; Yoo, J. ; Zavatarelli, S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-h287t-977a2674d20a00de8d0b6e96b6f09698ef23f77f33d9d61a5d332f04fca6bdf13</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Argon</topic><topic>Astrophysics</topic><topic>Dark matter</topic><topic>Emitters</topic><topic>Instrumentation and Detectors</topic><topic>Physics</topic><topic>Radiation counters</topic><topic>Scintillation counters</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Edkins, E.</creatorcontrib><creatorcontrib>Agnes, P.</creatorcontrib><creatorcontrib>Alton, A.</creatorcontrib><creatorcontrib>Arisaka, K.</creatorcontrib><creatorcontrib>Baldin, B.</creatorcontrib><creatorcontrib>Biery, K.</creatorcontrib><creatorcontrib>Bossa, M.</creatorcontrib><creatorcontrib>Brigatti, A.</creatorcontrib><creatorcontrib>Budano, F.</creatorcontrib><creatorcontrib>Calaprice, F.</creatorcontrib><creatorcontrib>Canci, N.</creatorcontrib><creatorcontrib>Candela, A.</creatorcontrib><creatorcontrib>Cao, H.</creatorcontrib><creatorcontrib>Cariello, M.</creatorcontrib><creatorcontrib>Cavalcante, P.</creatorcontrib><creatorcontrib>Chavarria, A.</creatorcontrib><creatorcontrib>Chepurnov, A.</creatorcontrib><creatorcontrib>Cocco, A. G.</creatorcontrib><creatorcontrib>Crippa, L.</creatorcontrib><creatorcontrib>D’Angelo, D.</creatorcontrib><creatorcontrib>D’Incecco, M.</creatorcontrib><creatorcontrib>Davini, S.</creatorcontrib><creatorcontrib>De Deo, M.</creatorcontrib><creatorcontrib>Derbin, A.</creatorcontrib><creatorcontrib>Devoto, A.</creatorcontrib><creatorcontrib>Di Eusanio, F.</creatorcontrib><creatorcontrib>Di Pietro, G.</creatorcontrib><creatorcontrib>Franco, D.</creatorcontrib><creatorcontrib>Gabriele, F.</creatorcontrib><creatorcontrib>Gromov, M.</creatorcontrib><creatorcontrib>Hackett, B.</creatorcontrib><creatorcontrib>Humble, P.</creatorcontrib><creatorcontrib>Hungerford, E. V.</creatorcontrib><creatorcontrib>Ianni, Al</creatorcontrib><creatorcontrib>Ianni, An</creatorcontrib><creatorcontrib>Jollet, C.</creatorcontrib><creatorcontrib>Keeter, K.</creatorcontrib><creatorcontrib>Kendziora, C.</creatorcontrib><creatorcontrib>Korablev, D.</creatorcontrib><creatorcontrib>Kurlej, A.</creatorcontrib><creatorcontrib>Li, P. X.</creatorcontrib><creatorcontrib>Loer, B.</creatorcontrib><creatorcontrib>Love, C.</creatorcontrib><creatorcontrib>Luitz, S.</creatorcontrib><creatorcontrib>Mandarano, A.</creatorcontrib><creatorcontrib>Marini, L.</creatorcontrib><creatorcontrib>Martoff, C. J.</creatorcontrib><creatorcontrib>Meregaglia, A.</creatorcontrib><creatorcontrib>Meroni, E.</creatorcontrib><creatorcontrib>Meyers, P. D.</creatorcontrib><creatorcontrib>Milincic, R.</creatorcontrib><creatorcontrib>Monzani, M. E.</creatorcontrib><creatorcontrib>Musico, P.</creatorcontrib><creatorcontrib>Nelson, A.</creatorcontrib><creatorcontrib>Odrowski, S.</creatorcontrib><creatorcontrib>Orsini, M.</creatorcontrib><creatorcontrib>Ortica, F.</creatorcontrib><creatorcontrib>Pagani, L.</creatorcontrib><creatorcontrib>Pantic, E.</creatorcontrib><creatorcontrib>Papp, L.</creatorcontrib><creatorcontrib>Parmeggiano, S.</creatorcontrib><creatorcontrib>Parsells, R.</creatorcontrib><creatorcontrib>Pelczar, K.</creatorcontrib><creatorcontrib>Pelliccia, N.</creatorcontrib><creatorcontrib>Perasso, S.</creatorcontrib><creatorcontrib>Pocar, A.</creatorcontrib><creatorcontrib>Pordes, S.</creatorcontrib><creatorcontrib>Pugachev, D.</creatorcontrib><creatorcontrib>Qian, H.</creatorcontrib><creatorcontrib>Randle, K.</creatorcontrib><creatorcontrib>Ranucci, G.</creatorcontrib><creatorcontrib>Razeto, A.</creatorcontrib><creatorcontrib>Reinhold, B.</creatorcontrib><creatorcontrib>Renshaw, A.</creatorcontrib><creatorcontrib>Romani, A.</creatorcontrib><creatorcontrib>Rountree, S. D.</creatorcontrib><creatorcontrib>Sablone, D.</creatorcontrib><creatorcontrib>Saggese, P.</creatorcontrib><creatorcontrib>Segreto, E.</creatorcontrib><creatorcontrib>Shields, E.</creatorcontrib><creatorcontrib>Skorokhvatov, M.</creatorcontrib><creatorcontrib>Smirnov, O.</creatorcontrib><creatorcontrib>Sotnikov, A.</creatorcontrib><creatorcontrib>Stanford, C.</creatorcontrib><creatorcontrib>Suvorov, Y.</creatorcontrib><creatorcontrib>Tartaglia, R.</creatorcontrib><creatorcontrib>Tatarowicz, J.</creatorcontrib><creatorcontrib>Testera, G.</creatorcontrib><creatorcontrib>Unzhakov, E.</creatorcontrib><creatorcontrib>Vogelaar, R. B.</creatorcontrib><creatorcontrib>Walker, S.</creatorcontrib><creatorcontrib>Wang, H.</creatorcontrib><creatorcontrib>Wang, Y.</creatorcontrib><creatorcontrib>Watson, A.</creatorcontrib><creatorcontrib>Westerdale, S.</creatorcontrib><creatorcontrib>Wojcik, M.</creatorcontrib><creatorcontrib>Wright, A.</creatorcontrib><creatorcontrib>Xiang, X.</creatorcontrib><creatorcontrib>Yoo, J.</creatorcontrib><creatorcontrib>Zavatarelli, S.</creatorcontrib><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Edkins, E.</au><au>Agnes, P.</au><au>Alton, A.</au><au>Arisaka, K.</au><au>Baldin, B.</au><au>Biery, K.</au><au>Bossa, M.</au><au>Brigatti, A.</au><au>Budano, F.</au><au>Calaprice, F.</au><au>Canci, N.</au><au>Candela, A.</au><au>Cao, H.</au><au>Cariello, M.</au><au>Cavalcante, P.</au><au>Chavarria, A.</au><au>Chepurnov, A.</au><au>Cocco, A. G.</au><au>Crippa, L.</au><au>D’Angelo, D.</au><au>D’Incecco, M.</au><au>Davini, S.</au><au>De Deo, M.</au><au>Derbin, A.</au><au>Devoto, A.</au><au>Di Eusanio, F.</au><au>Di Pietro, G.</au><au>Franco, D.</au><au>Gabriele, F.</au><au>Gromov, M.</au><au>Hackett, B.</au><au>Humble, P.</au><au>Hungerford, E. V.</au><au>Ianni, Al</au><au>Ianni, An</au><au>Jollet, C.</au><au>Keeter, K.</au><au>Kendziora, C.</au><au>Korablev, D.</au><au>Kurlej, A.</au><au>Li, P. X.</au><au>Loer, B.</au><au>Love, C.</au><au>Luitz, S.</au><au>Mandarano, A.</au><au>Marini, L.</au><au>Martoff, C. J.</au><au>Meregaglia, A.</au><au>Meroni, E.</au><au>Meyers, P. D.</au><au>Milincic, R.</au><au>Monzani, M. E.</au><au>Musico, P.</au><au>Nelson, A.</au><au>Odrowski, S.</au><au>Orsini, M.</au><au>Ortica, F.</au><au>Pagani, L.</au><au>Pantic, E.</au><au>Papp, L.</au><au>Parmeggiano, S.</au><au>Parsells, R.</au><au>Pelczar, K.</au><au>Pelliccia, N.</au><au>Perasso, S.</au><au>Pocar, A.</au><au>Pordes, S.</au><au>Pugachev, D.</au><au>Qian, H.</au><au>Randle, K.</au><au>Ranucci, G.</au><au>Razeto, A.</au><au>Reinhold, B.</au><au>Renshaw, A.</au><au>Romani, A.</au><au>Rountree, S. D.</au><au>Sablone, D.</au><au>Saggese, P.</au><au>Segreto, E.</au><au>Shields, E.</au><au>Skorokhvatov, M.</au><au>Smirnov, O.</au><au>Sotnikov, A.</au><au>Stanford, C.</au><au>Suvorov, Y.</au><au>Tartaglia, R.</au><au>Tatarowicz, J.</au><au>Testera, G.</au><au>Unzhakov, E.</au><au>Vogelaar, R. B.</au><au>Walker, S.</au><au>Wang, H.</au><au>Wang, Y.</au><au>Watson, A.</au><au>Westerdale, S.</au><au>Wojcik, M.</au><au>Wright, A.</au><au>Xiang, X.</au><au>Yoo, J.</au><au>Zavatarelli, S.</au><au>Raby, Stuart</au><au>Sandick, Pearl</au><au>Kumar, Jason</au><au>Babu, Kaladi</au><au>Balantekin, Baha</au><au>Strigari, Louis</au><au>Szczerbinska, Barbara</au><au>Mishra, Sanjib</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>The DarkSide direct dark matter search with liquid argon</atitle><btitle>AIP Conf.Proc</btitle><date>2017-11-03</date><risdate>2017</risdate><volume>1900</volume><issue>1</issue><issn>0094-243X</issn><eissn>1551-7616</eissn><coden>APCPCS</coden><abstract>The DarkSide-50 direct dark matter detector is a liquid argon time projection chamber (TPC) surrounded by a liquid scintillator neutron veto (LSV) and a water Cerenkov muon veto (WCV). Located under 3800 m.w.e. at the Laboratori Nazionali del Gran Sasso, Italy, it is the only direct dark matter experiment currently operating background free. The atmospheric argon target was replaced with argon from underground sources in April, 2015. The level of 39Ar, a β emitter present in atmospheric argon (AAr), has been shown to have been reduced by a factor of (1.4 ± 0.2) x 103. The combined spin-independent WIMP exclusion limit of 2.0 x 10−44 cm2 (mχ
= 100 GeV/c
2) is currently the best limit on a liquid argon target.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.5010122</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0001-7309-3023</orcidid><orcidid>https://orcid.org/0000-0001-9611-2004</orcidid><orcidid>https://orcid.org/0000-0001-9888-9175</orcidid><orcidid>https://orcid.org/0000-0002-7790-1224</orcidid><orcidid>https://orcid.org/0000-0002-2934-9148</orcidid><orcidid>https://orcid.org/0000-0001-7117-1251</orcidid><orcidid>https://orcid.org/0000-0001-8824-6205</orcidid><orcidid>https://orcid.org/0000-0003-2913-8057</orcidid><orcidid>https://orcid.org/0000-0002-6916-6776</orcidid></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0094-243X |
| ispartof | AIP Conf.Proc, 2017, Vol.1900 (1) |
| issn | 0094-243X 1551-7616 |
| language | eng |
| recordid | cdi_proquest_journals_2116004489 |
| source | AIP Journals Complete |
| subjects | Argon Astrophysics Dark matter Emitters Instrumentation and Detectors Physics Radiation counters Scintillation counters |
| title | The DarkSide direct dark matter search with liquid argon |
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