暗物质相互作用的宇宙学探针：未来十年
宇宙学与河外天体物理
2019-03-14 v1
摘要
宇宙学观测为探测暗物质粒子的基本性质提供了独特而稳健的途径——它们广泛检验一系列引人注目的理论情景，往往超越或补充地面及其他实验的覆盖范围。我们讨论了将在未来十年实现强有力的暗物质身份宇宙学搜寻计划中扮演关键角色的观测与理论进展。具体而言，我们聚焦于宇宙微波背景各向异性与谱畸变的测量，以及结构示踪体（如 Lyman- 森林、星系和宇宙学 21-cm 信号）。
引用
@article{arxiv.1903.05140,
title = {Cosmological Probes of Dark Matter Interactions: The Next Decade},
author = {Vera Gluscevic and Yacine Ali-Haimoud and Keith Bechtol and Kimberly K. Boddy and Celine Boehm and Jens Chluba and Francis-Yan Cyr-Racine and Cora Dvorkin and Daniel Grin and Julien Lesgourgues and Mathew S. Madhavacheril and Samuel D. McDermott and Julian B. Munoz and Ethan O. Nadler and Vivian Poulin and Sarah Shandera and Katelin Schutz and Tracy R. Slatyer and Benjamin Wallisch},
journal= {arXiv preprint arXiv:1903.05140},
year = {2019}
}
备注
Astro2020 Decadal Survey science white paper; list of endorsers available at https://github.com/veragluscevic/Astro2020-DM-Cosmology-Endorsers