dc.creatorCivitarese, Enrique Osvaldo
dc.creatorFushimi, Keiko Juliana
dc.creatorMosquera, Mercedes Elisa
dc.date2016-11
dc.date2020-08-19T17:57:16Z
dc.date.accessioned2023-07-14T19:55:56Z
dc.date.available2023-07-14T19:55:56Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/102640
dc.identifierhttps://ri.conicet.gov.ar/11336/55203
dc.identifierhttp://iopscience.iop.org/article/10.1088/0954-3899/43/12/125201/meta
dc.identifierhttps://arxiv.org/abs/1611.00802
dc.identifierissn:0954-3899
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7437246
dc.descriptionWeakly 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.
dc.descriptionFacultad de Ciencias Exactas
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectFísica
dc.subjectAndes laboratory
dc.subjectDark matter
dc.subjectWIMP
dc.titleCalculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors
dc.typeArticulo
dc.typePreprint


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