Analyzing Direct Dark Matter Detection Data by the AMIDAS Website
High Energy Physics - Phenomenology
2015-05-30 v1 High Energy Astrophysical Phenomena
High Energy Physics - Experiment
Abstract
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. 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 ~5% to < ~40% deviations from the input values.
Keywords
Cite
@article{arxiv.1109.0125,
title = {Analyzing Direct Dark Matter Detection Data by the AMIDAS Website},
author = {Chung-Lin Shan},
journal= {arXiv preprint arXiv:1109.0125},
year = {2015}
}
Comments
12 pages, 8 eps figures, 1 table, to appear in the proceedings of the 3rd Workshop on Directional Detection of Dark Matter (CYGNUS 2011), June 7-10, 2011, Aussois, France