Track Reconstruction and Performance of DRIFT Directional Dark Matter Detectors using Alpha Particles
First results are presented from an analysis of data from the DRIFT-IIa and DRIFT-IIb directional dark matter detectors at Boulby Mine in which alpha particle tracks were reconstructed and used to characterise detector performance--an important step towards optimising directional technology. The dri...
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creator | Burgos, S bes, J Ghag, C Gold, M Kudryavtsev, V A Lawson, T B Loomba, D Majewski, P McMillan, J E Muna, D Murphy, A StJ Nicklin, G G Paling, S M Petkov, A Plank, S J S Robinson, M Sanghi, N Smith, N J T Snowden-Ifft, D P Spooner, N J C Sumner, T J Turk, J Tziaferi, T |
description | First results are presented from an analysis of data from the DRIFT-IIa and DRIFT-IIb directional dark matter detectors at Boulby Mine in which alpha particle tracks were reconstructed and used to characterise detector performance--an important step towards optimising directional technology. The drift velocity in DRIFT-IIa was [59.3 +/- 0.2 (stat) +/- 7.5 (sys)] m/s based on an analysis of naturally-occurring alpha-emitting background. The drift velocity in DRIFT-IIb was [57 +/- 1 (stat) +/- 3 (sys)] m/s determined by the analysis of alpha particle tracks from a Po-210 source. 3D range reconstruction and energy spectra were used to identify alpha particles from the decay of Rn-222, Po-218, Rn-220 and Po-216. This study found that (22 +/- 2)% of Po-218 progeny (from Rn-222 decay) are produced with no net charge in 40 Torr CS2. For Po-216 progeny (from Rn-220 decay) the uncharged fraction is (100 +0 -35)%. |
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The drift velocity in DRIFT-IIa was [59.3 +/- 0.2 (stat) +/- 7.5 (sys)] m/s based on an analysis of naturally-occurring alpha-emitting background. The drift velocity in DRIFT-IIb was [57 +/- 1 (stat) +/- 3 (sys)] m/s determined by the analysis of alpha particle tracks from a Po-210 source. 3D range reconstruction and energy spectra were used to identify alpha particles from the decay of Rn-222, Po-218, Rn-220 and Po-216. This study found that (22 +/- 2)% of Po-218 progeny (from Rn-222 decay) are produced with no net charge in 40 Torr CS2. For Po-216 progeny (from Rn-220 decay) the uncharged fraction is (100 +0 -35)%.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.0707.1758</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Alpha decay ; Alpha particles ; Alpha rays ; Dark matter ; Detectors ; Drift ; Energy spectra ; Particle decay ; Particle tracking ; Physics - Instrumentation and Detectors ; Progeny ; Radon isotopes ; Reconstruction</subject><ispartof>arXiv.org, 2007-07</ispartof><rights>Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the associated terms available at http://arxiv.org/abs/0707.1758.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,782,786,887,27932</link.rule.ids><backlink>$$Uhttps://doi.org/10.1016/j.nima.2007.10.013$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.0707.1758$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Burgos, S</creatorcontrib><creatorcontrib>bes, J</creatorcontrib><creatorcontrib>Ghag, C</creatorcontrib><creatorcontrib>Gold, M</creatorcontrib><creatorcontrib>Kudryavtsev, V A</creatorcontrib><creatorcontrib>Lawson, T B</creatorcontrib><creatorcontrib>Loomba, D</creatorcontrib><creatorcontrib>Majewski, P</creatorcontrib><creatorcontrib>McMillan, J E</creatorcontrib><creatorcontrib>Muna, D</creatorcontrib><creatorcontrib>Murphy, A StJ</creatorcontrib><creatorcontrib>Nicklin, G G</creatorcontrib><creatorcontrib>Paling, S M</creatorcontrib><creatorcontrib>Petkov, A</creatorcontrib><creatorcontrib>Plank, S J S</creatorcontrib><creatorcontrib>Robinson, M</creatorcontrib><creatorcontrib>Sanghi, N</creatorcontrib><creatorcontrib>Smith, N J T</creatorcontrib><creatorcontrib>Snowden-Ifft, D P</creatorcontrib><creatorcontrib>Spooner, N J C</creatorcontrib><creatorcontrib>Sumner, T J</creatorcontrib><creatorcontrib>Turk, J</creatorcontrib><creatorcontrib>Tziaferi, T</creatorcontrib><title>Track Reconstruction and Performance of DRIFT Directional Dark Matter Detectors using Alpha Particles</title><title>arXiv.org</title><description>First results are presented from an analysis of data from the DRIFT-IIa and DRIFT-IIb directional dark matter detectors at Boulby Mine in which alpha particle tracks were reconstructed and used to characterise detector performance--an important step towards optimising directional technology. 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For Po-216 progeny (from Rn-220 decay) the uncharged fraction is (100 +0 -35)%.</description><subject>Alpha decay</subject><subject>Alpha particles</subject><subject>Alpha rays</subject><subject>Dark matter</subject><subject>Detectors</subject><subject>Drift</subject><subject>Energy spectra</subject><subject>Particle decay</subject><subject>Particle tracking</subject><subject>Physics - Instrumentation and Detectors</subject><subject>Progeny</subject><subject>Radon isotopes</subject><subject>Reconstruction</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</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>eNotkN9LwzAUhYMgOObefZKAz5350bTJ41idDiaO0fdymyXarWtmkor-9-s2nw738HHhfAg9UDJNpRDkGfxv8zMlOcmnNBfyBo0Y5zSRKWN3aBLCjhDCspwJwUfIlB70Hm-Mdl2IvtexcR2GbovXxlvnD9Bpg53FxWa5KHHReHNBoMUF-D1-hxiNx4WJQ-98wH1ouk88a49fgNfgY6NbE-7RrYU2mMl_jlG5eCnnb8nq43U5n60SEJQmkCkFxGwtsXZra6EYtZLVpNaEZ1xbnSqqas2MZiloSYcrT0HqYWUmMlXzMXq8vr0oqI6-OYD_q84qqrOKAXi6AkfvvnsTYrVzvR_GhIoRRZgkgyl-Aqd2Yc8</recordid><startdate>20070712</startdate><enddate>20070712</enddate><creator>Burgos, S</creator><creator>bes, J</creator><creator>Ghag, C</creator><creator>Gold, M</creator><creator>Kudryavtsev, V A</creator><creator>Lawson, T B</creator><creator>Loomba, D</creator><creator>Majewski, P</creator><creator>McMillan, J E</creator><creator>Muna, D</creator><creator>Murphy, A StJ</creator><creator>Nicklin, G G</creator><creator>Paling, S M</creator><creator>Petkov, A</creator><creator>Plank, S J S</creator><creator>Robinson, M</creator><creator>Sanghi, N</creator><creator>Smith, N J T</creator><creator>Snowden-Ifft, D P</creator><creator>Spooner, N J C</creator><creator>Sumner, T J</creator><creator>Turk, J</creator><creator>Tziaferi, T</creator><general>Cornell University Library, 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>20070712</creationdate><title>Track Reconstruction and Performance of DRIFT Directional Dark Matter Detectors using Alpha Particles</title><author>Burgos, S ; 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The drift velocity in DRIFT-IIa was [59.3 +/- 0.2 (stat) +/- 7.5 (sys)] m/s based on an analysis of naturally-occurring alpha-emitting background. The drift velocity in DRIFT-IIb was [57 +/- 1 (stat) +/- 3 (sys)] m/s determined by the analysis of alpha particle tracks from a Po-210 source. 3D range reconstruction and energy spectra were used to identify alpha particles from the decay of Rn-222, Po-218, Rn-220 and Po-216. This study found that (22 +/- 2)% of Po-218 progeny (from Rn-222 decay) are produced with no net charge in 40 Torr CS2. For Po-216 progeny (from Rn-220 decay) the uncharged fraction is (100 +0 -35)%.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0707.1758</doi><oa>free_for_read</oa></addata></record> |
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subjects | Alpha decay Alpha particles Alpha rays Dark matter Detectors Drift Energy spectra Particle decay Particle tracking Physics - Instrumentation and Detectors Progeny Radon isotopes Reconstruction |
title | Track Reconstruction and Performance of DRIFT Directional Dark Matter Detectors using Alpha Particles |
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