Analyzing direct dark matter detection data with unrejected background events by the AMIDAS website

Details Analyzing direct dark matter detection data with unrejected background events by the AMIDAS website Analyzing direct dark matter detection data with unrejected background events by the AMIDAS website

2011-11-28

arxiv.org/abs/1111.6346v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

9 pages, 10 eps figures, 1 table, to appear in the proceedings of the Seventh International Workshop on the Dark Side of the U

Scientific paper

In this talk I have presented the data analysis results of extracting properties of halo WIMPs: the mass and the (ratios between the) spin-independent and spin-dependent couplings/cross sections on nucleons by the AMIDAS website by taking into account possible unrejected background events in the analyzed data sets. Although non-standard astronomical setup has been used to generate pseudodata sets for our analyses, it has been found that, without prior information/assumption about the local density and velocity distribution of halo Dark Matter, these WIMP properties have been reconstructed with ~ 2% to <~ 30% deviations from the input values.

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