On possible lower bounds for the direct detection rate of SUSY Dark Matter
High Energy Physics - Phenomenology
2009-11-07 v1
Abstract
One can expect accessible lower bounds for dark matter detection rate due to restrictions on masses of the SUSY-partners. To explore this correlation one needs a new-generation large-mass detector. The absolute lower bound for detection rate can naturally be due to spin-dependent interaction. Aimed at detecting dark matter with sensitivity higher than event/day/kg an experiment should have a non-zero-spin target. Perhaps, the best is to create a GENIUS-like detector with both Ge-73 (high spin) and Ge-76 nuclei.
Cite
@article{arxiv.hep-ph/0201046,
title = {On possible lower bounds for the direct detection rate of SUSY Dark Matter},
author = {V. A. Bednyakov},
journal= {arXiv preprint arXiv:hep-ph/0201046},
year = {2009}
}
Comments
latex, 5 pages, 3 figures. Talk given at the III International Conference on Non-accelerator New Physics (NANP'01), Dubna, 19--23 June, 2001