First results from the LUX dark matter experiment at the Sanford Underground Research Facility
| Autor(a) principal: | |
|---|---|
| Data de Publicação: | 2014 |
| Outros Autores: | , , , , , |
| Tipo de documento: | Artigo |
| Idioma: | eng |
| Título da fonte: | Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) |
| Texto Completo: | http://dx.doi.org/10.1103/PhysRevLett.112.091303 http://hdl.handle.net/10400.26/26493 |
Resumo: | The Large Underground Xenon (LUX) experiment, a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), was cooled and filled in February 2013. We report results of the first WIMP search dataset, taken during the period April to August 2013, presenting the analysis of 85.3 live-days of data with a fiducial volume of 118 kg. A profile-likelihood analysis technique shows our data to be consistent with the background-only hypothesis, allowing 90% confidence limits to be set on spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of $7.6 \times 10^{-46}$ cm$^{2}$ at a WIMP mass of 33 GeV/c$^2$. We find that the LUX data are in strong disagreement with low-mass WIMP signal interpretations of the results from several recent direct detection experiments. |
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First results from the LUX dark matter experiment at the Sanford Underground Research FacilityThe Large Underground Xenon (LUX) experiment, a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), was cooled and filled in February 2013. We report results of the first WIMP search dataset, taken during the period April to August 2013, presenting the analysis of 85.3 live-days of data with a fiducial volume of 118 kg. A profile-likelihood analysis technique shows our data to be consistent with the background-only hypothesis, allowing 90% confidence limits to be set on spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of $7.6 \times 10^{-46}$ cm$^{2}$ at a WIMP mass of 33 GeV/c$^2$. We find that the LUX data are in strong disagreement with low-mass WIMP signal interpretations of the results from several recent direct detection experiments.Repositório ComumLUX collaboration (102 authors)de Viveiros, L.Lindote, A.Lopes, M.I.Neves, F.Silva, C.Solovov, V.N.2019-02-03T23:39:09Z2014-03-042019-02-03T23:39:09Z2014-03-04T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1103/PhysRevLett.112.091303http://hdl.handle.net/10400.26/26493enginfo: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:RCAAP2025-05-14T13:12:14Zoai:comum.rcaap.pt:10400.26/26493Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-29T07:20:30.059106Repositórios 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 |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility |
| title |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility |
| spellingShingle |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility LUX collaboration (102 authors) |
| title_short |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility |
| title_full |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility |
| title_fullStr |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility |
| title_full_unstemmed |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility |
| title_sort |
First results from the LUX dark matter experiment at the Sanford Underground Research Facility |
| author |
LUX collaboration (102 authors) |
| author_facet |
LUX collaboration (102 authors) de Viveiros, L. Lindote, A. Lopes, M.I. Neves, F. Silva, C. Solovov, V.N. |
| author_role |
author |
| author2 |
de Viveiros, L. 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 (102 authors) de Viveiros, L. Lindote, A. Lopes, M.I. Neves, F. Silva, C. Solovov, V.N. |
| description |
The Large Underground Xenon (LUX) experiment, a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), was cooled and filled in February 2013. We report results of the first WIMP search dataset, taken during the period April to August 2013, presenting the analysis of 85.3 live-days of data with a fiducial volume of 118 kg. A profile-likelihood analysis technique shows our data to be consistent with the background-only hypothesis, allowing 90% confidence limits to be set on spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of $7.6 \times 10^{-46}$ cm$^{2}$ at a WIMP mass of 33 GeV/c$^2$. We find that the LUX data are in strong disagreement with low-mass WIMP signal interpretations of the results from several recent direct detection experiments. |
| publishDate |
2014 |
| dc.date.none.fl_str_mv |
2014-03-04 2014-03-04T00:00:00Z 2019-02-03T23:39:09Z 2019-02-03T23:39:09Z |
| dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
| dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
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publishedVersion |
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http://dx.doi.org/10.1103/PhysRevLett.112.091303 http://hdl.handle.net/10400.26/26493 |
| url |
http://dx.doi.org/10.1103/PhysRevLett.112.091303 http://hdl.handle.net/10400.26/26493 |
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eng |
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eng |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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