Distance Probes of Dark Energy
Cosmology and Nongalactic Astrophysics
2016-03-02 v2
Abstract
This document presents the results from the Distances subgroup of the Cosmic Frontier Community Planning Study (Snowmass 2013). We summarize the current state of the field as well as future prospects and challenges. In addition to the established probes using Type IA supernovae and baryon acoustic oscillations, we also consider prospective methods based on clusters, active galactic nuclei, gravitational wave sirens and strong lensing time delays.
Keywords
Cite
@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}
}
Comments
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