Performance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays

WA105 collaboration

doi:10.1088/1748-0221/16/08/P08063

dc.contributor.author	WA105 collaboration
dc.date.accessioned	2021-10-19T06:31:01Z
dc.date.available	2021-10-19T06:31:01Z
dc.date.issued	2021
dc.identifier.citation	WA105 collaboration. (2021). Performance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays. <i>Journal of Instrumentation</i>, <i>16</i>(8), Article P08063. <a href="https://doi.org/10.1088/1748-0221/16/08/P08063" target="_blank">https://doi.org/10.1088/1748-0221/16/08/P08063</a>
dc.identifier.other	CONVID_101505046
dc.identifier.uri	https://jyx.jyu.fi/handle/123456789/78252
dc.description.abstract	We report the results of the analyses of the cosmic ray data collected with a 4 tonne (3×1×1 m3) active mass (volume) Liquid Argon Time-Projection Chamber (TPC) operated in a dual-phase mode. We present a detailed study of the TPC's response, its main detector parameters and performance. The results are important for the understanding and further developments of the dual-phase technology, thanks to the verification of key aspects, such as the extraction of electrons from liquid to gas and their amplification through the entire one square metre readout plain, gain stability, purity and charge sharing between readout views.	en
dc.format.mimetype	application/pdf
dc.language.iso	eng
dc.publisher	IOP Publishing
dc.relation.ispartofseries	Journal of Instrumentation
dc.rights	CC BY 4.0
dc.subject.other	large detector systems for particle and astroparticle physics
dc.subject.other	neutrino detectors
dc.subject.other	particle tracking detectors
dc.subject.other	time projection chambers
dc.title	Performance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays
dc.type	article
dc.identifier.urn	URN:NBN:fi:jyu-202110195281
dc.contributor.laitos	Fysiikan laitos	fi
dc.contributor.laitos	Department of Physics	en
dc.type.uri	http://purl.org/eprint/type/JournalArticle
dc.type.coar	http://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatus	peerReviewed
dc.relation.issn	1748-0221
dc.relation.numberinseries	8
dc.relation.volume	16
dc.type.version	publishedVersion
dc.rights.copyright	© 2021 CERN. Published by IOP Publishing Ltd on behalf of Sissa Medialab
dc.rights.accesslevel	openAccess	fi
dc.subject.yso	kosminen säteily
dc.subject.yso	neutriinot
dc.subject.yso	hiukkasfysiikka
dc.subject.yso	tutkimuslaitteet
dc.subject.yso	ilmaisimet
dc.format.content	fulltext
jyx.subject.uri	http://www.yso.fi/onto/yso/p14258
jyx.subject.uri	http://www.yso.fi/onto/yso/p5219
jyx.subject.uri	http://www.yso.fi/onto/yso/p15576
jyx.subject.uri	http://www.yso.fi/onto/yso/p2440
jyx.subject.uri	http://www.yso.fi/onto/yso/p4220
dc.rights.url	https://creativecommons.org/licenses/by/4.0/
dc.relation.doi	10.1088/1748-0221/16/08/P08063
jyx.fundinginformation	This work would not have been possible without the support of the Swiss National Science Foundation, Switzerland; CEA and CNRS/IN2P3, France; KEK and the JSPS program, Japan; Ministerio de Ciencia e Innovación in Spain under grants FPA2016-77347-C2, SEV-2016-0588 and MdM-2015-0509, Comunidad de Madrid, the CERCA program of the Generalitat de Catalunya and the fellowship (LCF/BQ/DI18/11660043) from “La Caixa” Foundation (ID 100010434); the Programme PNCDI III, CERN-RO, under Contract 2/2020, Romania; the U.S. Department of Energy under Grant No. DE-SC0011686. This project has received funding from the European Union’s Horizon 2020 Research and Innovation program under Grant Agreement no. 654168. The authors are also grateful to the French government operated by the National Research Agency (ANR) for the LABEX Enigmass, LABEX Lyon Institute of Origins (ANR-10-LABX-0066) of the Université de Lyon for its financial support within the program “Investissements d’Avenir” (ANR-11-IDEX-0007).
dc.type.okm	A1

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