利用脉冲星计时阵列研究超大质量黑洞的人口统计与环境
星系天体物理
2019-03-21 v1 广义相对论与量子宇宙学
摘要
对大型（>50）毫秒脉冲星阵列的精密计时将在未来约 3–7 年内探测到来自超大质量双黑洞的纳赫兹引力波辐射。我们综述了这些探测的科学机遇、成功所需条件，以及与 2020 年代电磁仪器的协同作用。
引用
@article{arxiv.1903.08183,
title = {Supermassive Black-hole Demographics & Environments With Pulsar Timing Arrays},
author = {Stephen R. Taylor and Sarah Burke-Spolaor and Paul T. Baker and Maria Charisi and Kristina Islo and Luke Z. Kelley and Dustin R. Madison and Joseph Simon and Sarah Vigeland},
journal= {arXiv preprint arXiv:1903.08183},
year = {2019}
}
备注
Submitted to the Astro2020 Decadal Survey. One of 5 core white-papers authored by members of the NANOGrav Collaboration. 9 pages, 2 figures