高灵敏度宇宙轴子搜寻的结果
天体物理学
2009-10-30 v1
摘要
我们报告了通过轴子转换为微波光子进行的高灵敏度（10^{-23} 瓦）轻晕轴子搜寻的首批结果。在 90% 置信度下，我们排除了质量为 2.9 x 10^{-6} eV 至 3.3 x 10^{-6} eV 的 KSVZ 轴子作为我们银河系晕中的暗物质。
引用
@article{arxiv.astro-ph/9801286,
title = {Results from a High-Sensitivity Search for Cosmic Axions},
author = {C. Hagmann and D. Kinion and W. Stoeffl and K. van Bibber and E. Daw and H. Peng and Leslie J Rosenberg and J. LaVeigne and P. Sikivie and N. Sullivan and D. Tanner and F. Nezrick and Michael S. Turner and D. Moltz and J. Powell and N. Golubev},
journal= {arXiv preprint arXiv:astro-ph/9801286},
year = {2009}
}
备注
11 text pages, 4 figures (figures 2 and 3 combined), to be published in Physical Review Letters