暗能量的距离探针
宇宙学与河外天体物理
2016-03-02 v2
摘要
本文档介绍了宇宙前沿社区规划研究（Snowmass 2013）距离子组的结果。我们总结了该领域的当前状态以及未来的前景和挑战。除了已建立的利用Ia型超新星和重子声学振荡的探针外，我们还考虑了基于星系团、活动星系核、引力波警报和强透镜时间延迟的潜在方法。
引用
@article{arxiv.1309.5382,
title = {Distance Probes of Dark Energy},
author = {A. Kim and N. Padmanabhan and G. Aldering and S. Allen and C. Baltay and R. Cahn and C. D'Andrea and N. Dalal and K. Dawson and K. Denney and D. Eisenstein and D. Finley and W. Freedman and S. Ho and D. Holz and A. Kent and D. Kasen and R. Kessler and S. Kuhlmann and E. Linder and P. Martini and P. Nugent and S. Perlmutter and B. Peterson and A. Riess and D. Rubin and M. Sako and N. Suntzeff and N. Suzuki and R. Thomas and W. M. Wood-Vasey and S. Woosley},
journal= {arXiv preprint arXiv:1309.5382},
year = {2016}
}
备注
Report from the "Dark Energy and CMB" working group for the American Physical Society's Division of Particles and Fields long-term planning exercise ("Snowmass"). Accepted for publication in Astroparticle Physics