Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors
Weakly interacting massive particles (WIMPs) are possible components of the Universe's dark matter (DM). The detection of WIMPs is signaled by the recoil of the atomic nuclei which form a detector. CoGeNT at the Soudan Underground Laboratory (SUL) and DAMA at the Laboratori Nazionali del Gran S...
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ftconicet:oai:ri.conicet.gov.ar:11336/55203 2023-10-09T21:45:57+02:00 Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors Civitarese, Enrique Osvaldo Fushimi, Keiko Juliana Mosquera, Mercedes Elisa application/pdf http://hdl.handle.net/11336/55203 eng eng IOP Publishing info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0954-3899/43/12/125201/meta info:eu-repo/semantics/altIdentifier/doi/10.1088/0954-3899/43/12/125201 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1611.00802 http://hdl.handle.net/11336/55203 Civitarese, Enrique Osvaldo; Fushimi, Keiko Juliana; Mosquera, Mercedes Elisa; Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors; IOP Publishing; Journal Of Physics G-nuclear And Particle Physics; 43; 12; 11-2016; 1-17; 125201 0954-3899 CONICET Digital CONICET info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ ANDES LABORATORY DARK MATTER WIMP https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion ftconicet https://doi.org/10.1088/0954-3899/43/12/125201 2023-09-24T19:50:11Z Weakly interacting massive particles (WIMPs) are possible components of the Universe's dark matter (DM). The detection of WIMPs is signaled by the recoil of the atomic nuclei which form a detector. CoGeNT at the Soudan Underground Laboratory (SUL) and DAMA at the Laboratori Nazionali del Gran Sasso (LNGS) have reported data on annual modulation of signals attributed to WIMPs. Both experiments are located in laboratories in the Northern Hemisphere. DM detectors are planned to operate (or already operate) in laboratories in the Southern Hemisphere, including SABRE at Stawell Underground Physics Laboratory (SUPL) in Australia, and DM-ICE in Antarctica. In this work we have analyzed the dependence of diurnal and annual modulation of signals, pertaining to the detection of WIMP, on the coordinates of the laboratory, for experiments which may be performed in the planned new Agua Negra Deep Experimental Site (ANDES) underground facility, to be built in San Juan, Argentina. We made predictions for NaI and Ge-type detectors placed in ANDES, to compare with DAMA, CoGeNT, SABRE and DM-ICE arrays, and found that the diurnal modulation of the signals, at the ANDES site, is amplified at its maximum value, both for NaI (Ge)-type detectors, while the annual modulation remains unaffected by the change in coordinates from north to south. Fil: Civitarese, Enrique Osvaldo. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Fushimi, Keiko Juliana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Article in Journal/Newspaper Antarc* Antarctica CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas) San Juan Argentina Journal of Physics G: Nuclear and Particle Physics 43 12 125201 |
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CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas) |
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English |
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ANDES LABORATORY DARK MATTER WIMP https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
spellingShingle |
ANDES LABORATORY DARK MATTER WIMP https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 Civitarese, Enrique Osvaldo Fushimi, Keiko Juliana Mosquera, Mercedes Elisa Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors |
topic_facet |
ANDES LABORATORY DARK MATTER WIMP https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
description |
Weakly interacting massive particles (WIMPs) are possible components of the Universe's dark matter (DM). The detection of WIMPs is signaled by the recoil of the atomic nuclei which form a detector. CoGeNT at the Soudan Underground Laboratory (SUL) and DAMA at the Laboratori Nazionali del Gran Sasso (LNGS) have reported data on annual modulation of signals attributed to WIMPs. Both experiments are located in laboratories in the Northern Hemisphere. DM detectors are planned to operate (or already operate) in laboratories in the Southern Hemisphere, including SABRE at Stawell Underground Physics Laboratory (SUPL) in Australia, and DM-ICE in Antarctica. In this work we have analyzed the dependence of diurnal and annual modulation of signals, pertaining to the detection of WIMP, on the coordinates of the laboratory, for experiments which may be performed in the planned new Agua Negra Deep Experimental Site (ANDES) underground facility, to be built in San Juan, Argentina. We made predictions for NaI and Ge-type detectors placed in ANDES, to compare with DAMA, CoGeNT, SABRE and DM-ICE arrays, and found that the diurnal modulation of the signals, at the ANDES site, is amplified at its maximum value, both for NaI (Ge)-type detectors, while the annual modulation remains unaffected by the change in coordinates from north to south. Fil: Civitarese, Enrique Osvaldo. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Fushimi, Keiko Juliana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina |
format |
Article in Journal/Newspaper |
author |
Civitarese, Enrique Osvaldo Fushimi, Keiko Juliana Mosquera, Mercedes Elisa |
author_facet |
Civitarese, Enrique Osvaldo Fushimi, Keiko Juliana Mosquera, Mercedes Elisa |
author_sort |
Civitarese, Enrique Osvaldo |
title |
Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors |
title_short |
Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors |
title_full |
Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors |
title_fullStr |
Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors |
title_full_unstemmed |
Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors |
title_sort |
calculated wimp signals at the andes laboratory: comparison with northern and southern located dark matter detectors |
publisher |
IOP Publishing |
url |
http://hdl.handle.net/11336/55203 |
geographic |
San Juan Argentina |
geographic_facet |
San Juan Argentina |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0954-3899/43/12/125201/meta info:eu-repo/semantics/altIdentifier/doi/10.1088/0954-3899/43/12/125201 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1611.00802 http://hdl.handle.net/11336/55203 Civitarese, Enrique Osvaldo; Fushimi, Keiko Juliana; Mosquera, Mercedes Elisa; Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors; IOP Publishing; Journal Of Physics G-nuclear And Particle Physics; 43; 12; 11-2016; 1-17; 125201 0954-3899 CONICET Digital CONICET |
op_rights |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
op_doi |
https://doi.org/10.1088/0954-3899/43/12/125201 |
container_title |
Journal of Physics G: Nuclear and Particle Physics |
container_volume |
43 |
container_issue |
12 |
container_start_page |
125201 |
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1779321611433803776 |