Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors

• Main Authors: Civitarese, O., Fushimi, K. J., Mosquera, M. E.
• Format: Text
• Language: unknown
• Published: arXiv 2016
• Subjects: Cosmology and Nongalactic Astrophysics astro-ph.CO; FOS Physical sciences; San Juan; Argentina; South Pole; South pole
• Online Access: https://dx.doi.org/10.48550/arxiv.1611.00802; https://arxiv.org/abs/1611.00802

Weakly Interacting Massive Particles (WIMP) are possible components of the Universe's Dark Matter. The detection of WIMP is signalled 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 WIMP. Both experiments are located in laboratories of the northern hemisphere. Dark matter detectors are planned to operate (or already operate) in laboratories of the southern hemisphere, like SABRE at Stawell Underground Physics Laboratory (SUPL) in Australia, and DM-ICE in the South Pole. In this work we have analysed 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 underground facility ANDES (Agua Negra Deep Experimental Site), 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 site of ANDES, 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. : 16 pages, 12 figures. Accepted for publication into Journal of physics G