A simple formula is introduced which indicates the amount by which projections of dark matter direct detection experiments are expected to be degraded due to backgrounds.
@article{arxiv.0812.0787,
title = {Backgrounds and Projected Limits from Dark Matter Direct Detection Experiments},
author = {Scott Dodelson},
journal= {arXiv preprint arXiv:0812.0787},
year = {2009}
}
Comments
4 pages, 3 figures, code available at http://home.fnal.gov/~dodelson/dm.html