The LUX-ZEPLIN (LZ) Experiment
We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe s...
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| creator | Akerib, D S Akerlof, C W Araújo, H M Armstrong, J E Bauer, D Baxter, A Benson, T Biekert, A Boulton, E M Brás, P Breidenbach, M Busenitz, J K Carlsmith, D L Carmona-Benitez, M C Chan, C Chiller, A A Chiller, C Colling, D Conley, R A Coughlen, R Cutter, J E de Viveiros, L Edwards, B N Faham, C H Fayer, S Francis, V B Froborg, F Gantos, N J Geffre, A Gehman, V M Gelfand, R Genovesi, J Gokhale, S Gwilliam, C B Hanzel, K Harrison, A Hasselkus, C Heise, J Hitchcock, O Hjemfelt, C W Ji Johnson, P Jones, W G Kaboth, A C Kamaha, A Kazkaz, K Khaitan, D Khaleeq, M Kravitz, S W Kreczko, L Kudryavtsev, V A Lambert, A R A Laundrie Leason, E A Lee, H S Lee, C Lenardo, B G Liao, J F -T Liao Linehan, R Liu, R Luitz, S Makkinje, J Malling, D C MarrLaundrie, P McConnell, C T McLaughlin, J Miller, E H Minaker, Z J Mizrachi, E Naylor, A Nedlik, C Nilima, A O'Neill, F G Oliver-Mallory, K C Pagenkopf, D Palmaccio, V M Pangilinan, M Pierson, S Rodrigues, J P Rutherford, G Saba, J S Sabarots, L Sarychev, M Shutt, T A Solovov, V N Sorensen, P Sosnovtsev, V V Sutcliffe, P Tan, M Taylor, W C Taylor, D J Temples, D Tennyson, B P Thomas, K J Uvarov, S W -Z Wei While, M Wisniewski, W J Witherell, M S |
| description | We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe skin veto detector and by a liquid scintillator Outer Detector loaded with gadolinium for efficient neutron capture and tagging. LZ is located in the Davis Cavern at the 4850' level of the Sanford Underground Research Facility in Lead, South Dakota, USA. We describe the major subsystems of the experiment and its key design features and requirements. |
| doi_str_mv | 10.48550/arxiv.1910.09124 |
| format | Article |
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The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe skin veto detector and by a liquid scintillator Outer Detector loaded with gadolinium for efficient neutron capture and tagging. LZ is located in the Davis Cavern at the 4850' level of the Sanford Underground Research Facility in Lead, South Dakota, USA. We describe the major subsystems of the experiment and its key design features and requirements.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1910.09124</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Dark matter ; Experiments ; Gadolinium ; Nuclear capture ; Physics - High Energy Physics - Experiment ; Physics - Instrumentation and Detectors ; Physics - Instrumentation and Methods for Astrophysics ; Radiation counters ; Scintillation counters ; Subsystems ; Underground caverns ; Xenon</subject><ispartof>arXiv.org, 2019-11</ispartof><rights>2019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.1016/j.nima.2019.163047$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.1910.09124$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Akerib, D S</creatorcontrib><creatorcontrib>Akerlof, C W</creatorcontrib><creatorcontrib>Araújo, H M</creatorcontrib><creatorcontrib>Armstrong, J E</creatorcontrib><creatorcontrib>Bauer, 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L</creatorcontrib><creatorcontrib>Kudryavtsev, V A</creatorcontrib><creatorcontrib>Lambert, A R</creatorcontrib><creatorcontrib>A Laundrie</creatorcontrib><creatorcontrib>Leason, E A</creatorcontrib><creatorcontrib>Lee, H S</creatorcontrib><creatorcontrib>Lee, C</creatorcontrib><creatorcontrib>Lenardo, B G</creatorcontrib><creatorcontrib>Liao, J</creatorcontrib><creatorcontrib>F -T Liao</creatorcontrib><creatorcontrib>Linehan, R</creatorcontrib><creatorcontrib>Liu, R</creatorcontrib><creatorcontrib>Luitz, S</creatorcontrib><creatorcontrib>Makkinje, J</creatorcontrib><creatorcontrib>Malling, D C</creatorcontrib><creatorcontrib>MarrLaundrie, P</creatorcontrib><creatorcontrib>McConnell, C T</creatorcontrib><creatorcontrib>McLaughlin, J</creatorcontrib><creatorcontrib>Miller, E H</creatorcontrib><creatorcontrib>Minaker, Z J</creatorcontrib><creatorcontrib>Mizrachi, E</creatorcontrib><creatorcontrib>Naylor, A</creatorcontrib><creatorcontrib>Nedlik, C</creatorcontrib><creatorcontrib>Nilima, A</creatorcontrib><creatorcontrib>O'Neill, F G</creatorcontrib><creatorcontrib>Oliver-Mallory, K C</creatorcontrib><creatorcontrib>Pagenkopf, D</creatorcontrib><creatorcontrib>Palmaccio, V M</creatorcontrib><creatorcontrib>Pangilinan, M</creatorcontrib><creatorcontrib>Pierson, S</creatorcontrib><creatorcontrib>Rodrigues, J P</creatorcontrib><creatorcontrib>Rutherford, G</creatorcontrib><creatorcontrib>Saba, J S</creatorcontrib><creatorcontrib>Sabarots, L</creatorcontrib><creatorcontrib>Sarychev, M</creatorcontrib><creatorcontrib>Shutt, T A</creatorcontrib><creatorcontrib>Solovov, V N</creatorcontrib><creatorcontrib>Sorensen, P</creatorcontrib><creatorcontrib>Sosnovtsev, V V</creatorcontrib><creatorcontrib>Sutcliffe, P</creatorcontrib><creatorcontrib>Tan, M</creatorcontrib><creatorcontrib>Taylor, W C</creatorcontrib><creatorcontrib>Taylor, D J</creatorcontrib><creatorcontrib>Temples, D</creatorcontrib><creatorcontrib>Tennyson, B P</creatorcontrib><creatorcontrib>Thomas, K J</creatorcontrib><creatorcontrib>Uvarov, S</creatorcontrib><creatorcontrib>W -Z Wei</creatorcontrib><creatorcontrib>While, M</creatorcontrib><creatorcontrib>Wisniewski, W J</creatorcontrib><creatorcontrib>Witherell, M S</creatorcontrib><title>The LUX-ZEPLIN (LZ) Experiment</title><title>arXiv.org</title><description>We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe skin veto detector and by a liquid scintillator Outer Detector loaded with gadolinium for efficient neutron capture and tagging. LZ is located in the Davis Cavern at the 4850' level of the Sanford Underground Research Facility in Lead, South Dakota, USA. We describe the major subsystems of the experiment and its key design features and requirements.</description><subject>Dark matter</subject><subject>Experiments</subject><subject>Gadolinium</subject><subject>Nuclear capture</subject><subject>Physics - High Energy Physics - Experiment</subject><subject>Physics - Instrumentation and Detectors</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Radiation counters</subject><subject>Scintillation counters</subject><subject>Subsystems</subject><subject>Underground caverns</subject><subject>Xenon</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotj0FLw0AUhBdBsNT-AC8a8KKHtC_v7cvbHKVELYTqIYL0EtbNBlu0jZtW6r83tp4GhmHmG6UuEhhrwwwTG_bL73GS9QZkCeoTNUCiJDYa8UyNum4FAJgKMtNAXZbvPipeXuNF_lzM5tFNsbiN8n3rw_LTr7fn6rSxH50f_etQlfd5OX2Mi6eH2fSuiC0jx7Ul8NqABmmkNpnX2mEDpOs3MJacAxLTSCYpIoll8eBS1yBaIucToaG6OtYe4Ku2H7fhp_o7UR1O9InrY6INm6-d77bVarML656pQgJhZiGmX7NGRak</recordid><startdate>20191104</startdate><enddate>20191104</enddate><creator>Akerib, D S</creator><creator>Akerlof, C W</creator><creator>Araújo, H M</creator><creator>Armstrong, J E</creator><creator>Bauer, D</creator><creator>Baxter, A</creator><creator>Benson, T</creator><creator>Biekert, A</creator><creator>Boulton, E M</creator><creator>Brás, P</creator><creator>Breidenbach, M</creator><creator>Busenitz, J K</creator><creator>Carlsmith, D L</creator><creator>Carmona-Benitez, M C</creator><creator>Chan, C</creator><creator>Chiller, A A</creator><creator>Chiller, C</creator><creator>Colling, D</creator><creator>Conley, R A</creator><creator>Coughlen, R</creator><creator>Cutter, J E</creator><creator>de Viveiros, L</creator><creator>Edwards, B N</creator><creator>Faham, C H</creator><creator>Fayer, S</creator><creator>Francis, V B</creator><creator>Froborg, F</creator><creator>Gantos, N J</creator><creator>Geffre, A</creator><creator>Gehman, V M</creator><creator>Gelfand, R</creator><creator>Genovesi, J</creator><creator>Gokhale, S</creator><creator>Gwilliam, C B</creator><creator>Hanzel, K</creator><creator>Harrison, A</creator><creator>Hasselkus, C</creator><creator>Heise, J</creator><creator>Hitchcock, O</creator><creator>Hjemfelt, C</creator><creator>W Ji</creator><creator>Johnson, 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20191104</creationdate><title>The LUX-ZEPLIN (LZ) Experiment</title><author>Akerib, D S ; Akerlof, C W ; Araújo, H M ; Armstrong, J E ; Bauer, D ; Baxter, A ; Benson, T ; Biekert, A ; Boulton, E M ; Brás, P ; Breidenbach, M ; Busenitz, J K ; Carlsmith, D L ; Carmona-Benitez, M C ; Chan, C ; Chiller, A A ; Chiller, C ; Colling, D ; Conley, R A ; Coughlen, R ; Cutter, J E ; de Viveiros, L ; Edwards, B N ; Faham, C H ; Fayer, S ; Francis, V B ; Froborg, F ; Gantos, N J ; Geffre, A ; Gehman, V M ; Gelfand, R ; Genovesi, J ; Gokhale, S ; Gwilliam, C B ; Hanzel, K ; Harrison, A ; Hasselkus, C ; Heise, J ; Hitchcock, O ; Hjemfelt, C ; W Ji ; Johnson, P ; Jones, W G ; Kaboth, A C ; Kamaha, A ; Kazkaz, K ; Khaitan, D ; Khaleeq, M ; Kravitz, S W ; Kreczko, L ; Kudryavtsev, V A ; Lambert, A R ; A Laundrie ; Leason, E A ; Lee, H S ; Lee, C ; Lenardo, B G ; Liao, J ; F -T Liao ; Linehan, R ; Liu, R ; Luitz, S ; Makkinje, J ; Malling, D C ; MarrLaundrie, P ; McConnell, C T ; McLaughlin, J ; Miller, E H ; Minaker, Z J ; Mizrachi, E ; Naylor, A ; Nedlik, C ; Nilima, A ; O'Neill, F G ; Oliver-Mallory, K C ; Pagenkopf, D ; Palmaccio, V M ; Pangilinan, M ; Pierson, S ; Rodrigues, J P ; Rutherford, G ; Saba, J S ; Sabarots, L ; Sarychev, M ; Shutt, T A ; Solovov, V N ; Sorensen, P ; Sosnovtsev, V V ; Sutcliffe, P ; Tan, M ; Taylor, W C ; Taylor, D J ; Temples, D ; Tennyson, B P ; Thomas, K J ; Uvarov, S ; W -Z Wei ; While, M ; Wisniewski, W J ; Witherell, M S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a525-da30e480407f7d89e44c2f034db08a3cc0378f79762237a57e0c6cf22a33ce173</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Dark matter</topic><topic>Experiments</topic><topic>Gadolinium</topic><topic>Nuclear capture</topic><topic>Physics - High Energy Physics - Experiment</topic><topic>Physics - Instrumentation and Detectors</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Radiation counters</topic><topic>Scintillation counters</topic><topic>Subsystems</topic><topic>Underground caverns</topic><topic>Xenon</topic><toplevel>online_resources</toplevel><creatorcontrib>Akerib, D S</creatorcontrib><creatorcontrib>Akerlof, C W</creatorcontrib><creatorcontrib>Araújo, H M</creatorcontrib><creatorcontrib>Armstrong, J E</creatorcontrib><creatorcontrib>Bauer, D</creatorcontrib><creatorcontrib>Baxter, A</creatorcontrib><creatorcontrib>Benson, T</creatorcontrib><creatorcontrib>Biekert, A</creatorcontrib><creatorcontrib>Boulton, E M</creatorcontrib><creatorcontrib>Brás, P</creatorcontrib><creatorcontrib>Breidenbach, M</creatorcontrib><creatorcontrib>Busenitz, J K</creatorcontrib><creatorcontrib>Carlsmith, D L</creatorcontrib><creatorcontrib>Carmona-Benitez, M C</creatorcontrib><creatorcontrib>Chan, C</creatorcontrib><creatorcontrib>Chiller, A A</creatorcontrib><creatorcontrib>Chiller, C</creatorcontrib><creatorcontrib>Colling, D</creatorcontrib><creatorcontrib>Conley, R A</creatorcontrib><creatorcontrib>Coughlen, R</creatorcontrib><creatorcontrib>Cutter, J E</creatorcontrib><creatorcontrib>de Viveiros, L</creatorcontrib><creatorcontrib>Edwards, B N</creatorcontrib><creatorcontrib>Faham, C H</creatorcontrib><creatorcontrib>Fayer, S</creatorcontrib><creatorcontrib>Francis, V B</creatorcontrib><creatorcontrib>Froborg, F</creatorcontrib><creatorcontrib>Gantos, N J</creatorcontrib><creatorcontrib>Geffre, A</creatorcontrib><creatorcontrib>Gehman, V M</creatorcontrib><creatorcontrib>Gelfand, R</creatorcontrib><creatorcontrib>Genovesi, J</creatorcontrib><creatorcontrib>Gokhale, S</creatorcontrib><creatorcontrib>Gwilliam, C B</creatorcontrib><creatorcontrib>Hanzel, K</creatorcontrib><creatorcontrib>Harrison, A</creatorcontrib><creatorcontrib>Hasselkus, C</creatorcontrib><creatorcontrib>Heise, J</creatorcontrib><creatorcontrib>Hitchcock, O</creatorcontrib><creatorcontrib>Hjemfelt, C</creatorcontrib><creatorcontrib>W Ji</creatorcontrib><creatorcontrib>Johnson, P</creatorcontrib><creatorcontrib>Jones, W G</creatorcontrib><creatorcontrib>Kaboth, A C</creatorcontrib><creatorcontrib>Kamaha, A</creatorcontrib><creatorcontrib>Kazkaz, K</creatorcontrib><creatorcontrib>Khaitan, D</creatorcontrib><creatorcontrib>Khaleeq, M</creatorcontrib><creatorcontrib>Kravitz, S W</creatorcontrib><creatorcontrib>Kreczko, L</creatorcontrib><creatorcontrib>Kudryavtsev, V A</creatorcontrib><creatorcontrib>Lambert, A R</creatorcontrib><creatorcontrib>A Laundrie</creatorcontrib><creatorcontrib>Leason, E A</creatorcontrib><creatorcontrib>Lee, H S</creatorcontrib><creatorcontrib>Lee, C</creatorcontrib><creatorcontrib>Lenardo, B G</creatorcontrib><creatorcontrib>Liao, J</creatorcontrib><creatorcontrib>F -T Liao</creatorcontrib><creatorcontrib>Linehan, R</creatorcontrib><creatorcontrib>Liu, R</creatorcontrib><creatorcontrib>Luitz, S</creatorcontrib><creatorcontrib>Makkinje, J</creatorcontrib><creatorcontrib>Malling, D C</creatorcontrib><creatorcontrib>MarrLaundrie, P</creatorcontrib><creatorcontrib>McConnell, C T</creatorcontrib><creatorcontrib>McLaughlin, J</creatorcontrib><creatorcontrib>Miller, E H</creatorcontrib><creatorcontrib>Minaker, Z J</creatorcontrib><creatorcontrib>Mizrachi, E</creatorcontrib><creatorcontrib>Naylor, A</creatorcontrib><creatorcontrib>Nedlik, C</creatorcontrib><creatorcontrib>Nilima, A</creatorcontrib><creatorcontrib>O'Neill, F G</creatorcontrib><creatorcontrib>Oliver-Mallory, K C</creatorcontrib><creatorcontrib>Pagenkopf, D</creatorcontrib><creatorcontrib>Palmaccio, V M</creatorcontrib><creatorcontrib>Pangilinan, M</creatorcontrib><creatorcontrib>Pierson, S</creatorcontrib><creatorcontrib>Rodrigues, J P</creatorcontrib><creatorcontrib>Rutherford, G</creatorcontrib><creatorcontrib>Saba, J S</creatorcontrib><creatorcontrib>Sabarots, L</creatorcontrib><creatorcontrib>Sarychev, M</creatorcontrib><creatorcontrib>Shutt, T A</creatorcontrib><creatorcontrib>Solovov, V N</creatorcontrib><creatorcontrib>Sorensen, P</creatorcontrib><creatorcontrib>Sosnovtsev, V V</creatorcontrib><creatorcontrib>Sutcliffe, P</creatorcontrib><creatorcontrib>Tan, M</creatorcontrib><creatorcontrib>Taylor, W C</creatorcontrib><creatorcontrib>Taylor, D J</creatorcontrib><creatorcontrib>Temples, D</creatorcontrib><creatorcontrib>Tennyson, B P</creatorcontrib><creatorcontrib>Thomas, K J</creatorcontrib><creatorcontrib>Uvarov, S</creatorcontrib><creatorcontrib>W -Z Wei</creatorcontrib><creatorcontrib>While, M</creatorcontrib><creatorcontrib>Wisniewski, W J</creatorcontrib><creatorcontrib>Witherell, M S</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Access via ProQuest (Open Access)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Akerib, D S</au><au>Akerlof, C W</au><au>Araújo, H M</au><au>Armstrong, J E</au><au>Bauer, D</au><au>Baxter, A</au><au>Benson, T</au><au>Biekert, A</au><au>Boulton, E M</au><au>Brás, P</au><au>Breidenbach, M</au><au>Busenitz, J K</au><au>Carlsmith, D L</au><au>Carmona-Benitez, M C</au><au>Chan, C</au><au>Chiller, A A</au><au>Chiller, C</au><au>Colling, D</au><au>Conley, R A</au><au>Coughlen, R</au><au>Cutter, J E</au><au>de Viveiros, L</au><au>Edwards, B N</au><au>Faham, C H</au><au>Fayer, S</au><au>Francis, V B</au><au>Froborg, F</au><au>Gantos, N J</au><au>Geffre, A</au><au>Gehman, V M</au><au>Gelfand, R</au><au>Genovesi, J</au><au>Gokhale, S</au><au>Gwilliam, C B</au><au>Hanzel, K</au><au>Harrison, A</au><au>Hasselkus, C</au><au>Heise, J</au><au>Hitchcock, O</au><au>Hjemfelt, C</au><au>W Ji</au><au>Johnson, P</au><au>Jones, W G</au><au>Kaboth, A C</au><au>Kamaha, A</au><au>Kazkaz, K</au><au>Khaitan, D</au><au>Khaleeq, M</au><au>Kravitz, S W</au><au>Kreczko, L</au><au>Kudryavtsev, V A</au><au>Lambert, A R</au><au>A Laundrie</au><au>Leason, E A</au><au>Lee, H S</au><au>Lee, C</au><au>Lenardo, B G</au><au>Liao, J</au><au>F -T Liao</au><au>Linehan, R</au><au>Liu, R</au><au>Luitz, S</au><au>Makkinje, J</au><au>Malling, D C</au><au>MarrLaundrie, P</au><au>McConnell, C T</au><au>McLaughlin, J</au><au>Miller, E H</au><au>Minaker, Z J</au><au>Mizrachi, E</au><au>Naylor, A</au><au>Nedlik, C</au><au>Nilima, A</au><au>O'Neill, F G</au><au>Oliver-Mallory, K C</au><au>Pagenkopf, D</au><au>Palmaccio, V M</au><au>Pangilinan, M</au><au>Pierson, S</au><au>Rodrigues, J P</au><au>Rutherford, G</au><au>Saba, J S</au><au>Sabarots, L</au><au>Sarychev, M</au><au>Shutt, T A</au><au>Solovov, V N</au><au>Sorensen, P</au><au>Sosnovtsev, V V</au><au>Sutcliffe, P</au><au>Tan, M</au><au>Taylor, W C</au><au>Taylor, D J</au><au>Temples, D</au><au>Tennyson, B P</au><au>Thomas, K J</au><au>Uvarov, S</au><au>W -Z Wei</au><au>While, M</au><au>Wisniewski, W J</au><au>Witherell, M S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The LUX-ZEPLIN (LZ) Experiment</atitle><jtitle>arXiv.org</jtitle><date>2019-11-04</date><risdate>2019</risdate><eissn>2331-8422</eissn><abstract>We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe skin veto detector and by a liquid scintillator Outer Detector loaded with gadolinium for efficient neutron capture and tagging. LZ is located in the Davis Cavern at the 4850' level of the Sanford Underground Research Facility in Lead, South Dakota, USA. We describe the major subsystems of the experiment and its key design features and requirements.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1910.09124</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2019-11 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_1910_09124 |
| source | arXiv.org; Free E- Journals |
| subjects | Dark matter Experiments Gadolinium Nuclear capture Physics - High Energy Physics - Experiment Physics - Instrumentation and Detectors Physics - Instrumentation and Methods for Astrophysics Radiation counters Scintillation counters Subsystems Underground caverns Xenon |
| title | The LUX-ZEPLIN (LZ) Experiment |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-19T11%3A25%3A25IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20LUX-ZEPLIN%20(LZ)%20Experiment&rft.jtitle=arXiv.org&rft.au=Akerib,%20D%20S&rft.date=2019-11-04&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1910.09124&rft_dat=%3Cproquest_arxiv%3E2307555735%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2307555735&rft_id=info:pmid/&rfr_iscdi=true |