A Primer on Dark Matter
Abstract
Dark matter is a fundamental constituent of the universe, which is needed to explain a wide variety of astrophysical and cosmological observations. Although the existence of dark matter was first postulated nearly a century ago and its abundance is precisely measured, approximately five times larger than that of ordinary matter, its underlying identity remains a mystery. A leading hypothesis is that it is composed of new elementary particles, which are predicted to exist in many extensions of the Standard Model of particle physics. In this article we review the basic evidence for dark matter and the role it plays in cosmology and astrophysics, and discuss experimental searches and potential candidates. Rather than targeting researchers in the field, we aim to provide an accessible and concise summary of the most important ideas and results, which can serve as a first entry point for advanced undergraduate students of physics or astronomy.
Cite
@article{arxiv.2411.05062,
title = {A Primer on Dark Matter},
author = {Csaba Balazs and Torsten Bringmann and Felix Kahlhoefer and Martin White},
journal= {arXiv preprint arXiv:2411.05062},
year = {2025}
}
Comments
15 pages, 5 figures. Preprint of a chapter for the 'Encyclopedia of Astrophysics' (Editor-in-Chief Ilya Mandel, Section Editor Cullan Howlett) to be published by Elsevier as a Reference Module