$^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search

Bibliographic Details
Main Author: LUX collaboration (93 authors)
Publication Date: 2017
Other Authors: Brás, P., Lindote, A., Lopes, M.I., Neves, F., Silva, C., Solovov, V.N.
Format: Article
Language: eng
Source: Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)
Download full: http://dx.doi.org/10.1103/PhysRevD.96.112009
http://hdl.handle.net/10400.26/27750
Summary: LUX was the first dark matter experiment to use a Kr83m calibration source. In this paper, we describe the source preparation and injection. We also present several Kr83m calibration applications in the context of the 2013 LUX exposure, including the measurement of temporal and spatial variation in scintillation and charge signal amplitudes, and several methods to understand the electric field within the time projection chamber.
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spelling $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter searchLUX was the first dark matter experiment to use a Kr83m calibration source. In this paper, we describe the source preparation and injection. We also present several Kr83m calibration applications in the context of the 2013 LUX exposure, including the measurement of temporal and spatial variation in scintillation and charge signal amplitudes, and several methods to understand the electric field within the time projection chamber.Repositório ComumLUX collaboration (93 authors)Brás, P.Lindote, A.Lopes, M.I.Neves, F.Silva, C.Solovov, V.N.2019-02-05T17:21:18Z2017-12-262019-02-05T17:21:18Z2017-12-26T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1103/PhysRevD.96.112009http://hdl.handle.net/10400.26/27750enginfo:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2025-05-14T13:14:50Zoai:comum.rcaap.pt:10400.26/27750Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-29T07:21:11.802834Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse
dc.title.none.fl_str_mv $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
title $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
spellingShingle $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
LUX collaboration (93 authors)
title_short $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
title_full $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
title_fullStr $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
title_full_unstemmed $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
title_sort $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search
author LUX collaboration (93 authors)
author_facet LUX collaboration (93 authors)
Brás, P.
Lindote, A.
Lopes, M.I.
Neves, F.
Silva, C.
Solovov, V.N.
author_role author
author2 Brás, P.
Lindote, A.
Lopes, M.I.
Neves, F.
Silva, C.
Solovov, V.N.
author2_role author
author
author
author
author
author
dc.contributor.none.fl_str_mv Repositório Comum
dc.contributor.author.fl_str_mv LUX collaboration (93 authors)
Brás, P.
Lindote, A.
Lopes, M.I.
Neves, F.
Silva, C.
Solovov, V.N.
description LUX was the first dark matter experiment to use a Kr83m calibration source. In this paper, we describe the source preparation and injection. We also present several Kr83m calibration applications in the context of the 2013 LUX exposure, including the measurement of temporal and spatial variation in scintillation and charge signal amplitudes, and several methods to understand the electric field within the time projection chamber.
publishDate 2017
dc.date.none.fl_str_mv 2017-12-26
2017-12-26T00:00:00Z
2019-02-05T17:21:18Z
2019-02-05T17:21:18Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.96.112009
http://hdl.handle.net/10400.26/27750
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http://hdl.handle.net/10400.26/27750
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