Dark Matter Physics from the CMB-S4 Experiment

Cora Dvorkin, Renée Hlozek, Rui An, Kimberly K. Boddy, Francis-Yan Cyr-Racine, Gerrit S. Farren, Vera Gluscevic, Daniel Grin, David J. E. Marsh, Joel Meyers, Keir K. Rogers, Katelin Schutz, Weishuang Linda Xu

Read on arXiv

arXiv

2203.07064

Date

2022-03-14

Frontier

Cosmic Frontier (CF)

Topical groups

Submitted by

Cora Dvorkin

Abstract

The nature of dark matter is one of the major puzzles of fundamental physics, integral to the understanding of our universe across almost every epoch. The search for dark matter takes place at different energy scales, and use data ranging from particle colliders to astrophysical surveys. We focus here on CMB-S4, a future ground-based Cosmic Microwave Background (CMB) experiment, which is expected to provide exquisite measurements of the CMB temperature and polarization anisotropies. These measurements (on their own and in combination with other surveys) will allow for new means to shed light on the nature of dark matter.