Dr Francesca Chadha-Day francesca.chadha-day@durham.ac.uk
Associate Professor
Dr Francesca Chadha-Day francesca.chadha-day@durham.ac.uk
Associate Professor
John Ellis
David J.E. Marsh
The axion has emerged in recent years as a leading particle candidate to provide the mysterious dark matter in the cosmos, as we review here for a general scientific audience. We describe first the historical roots of the axion in the Standard Model of particle physics and the problem of charge-parity invariance of the strong nuclear force. We then discuss how the axion emerges as a dark matter candidate and how it is produced in the early universe. The symmetry properties of the axion dictate the form of its interactions with ordinary matter. Astrophysical considerations restrict the particle mass and interaction strengths to a limited range, which facilitates the planning of experiments to detect the axion. A companion review discusses the exciting prospect that the axion could be detected in the near term in the laboratory.
Chadha-Day, F., Ellis, J., & Marsh, D. J. (2022). Axion dark matter: What is it and why now?. Science Advances, 8(8), https://doi.org/10.1126/sciadv.abj3618
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 14, 2022 |
Online Publication Date | Feb 23, 2022 |
Publication Date | Feb 25, 2022 |
Deposit Date | Mar 9, 2022 |
Publicly Available Date | Mar 9, 2022 |
Journal | Science Advances |
Electronic ISSN | 2375-2548 |
Publisher | American Association for the Advancement of Science |
Peer Reviewed | Peer Reviewed |
Volume | 8 |
Issue | 8 |
DOI | https://doi.org/10.1126/sciadv.abj3618 |
Public URL | https://durham-repository.worktribe.com/output/1211999 |
Published Journal Article
(720 Kb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by-nc/4.0/
Copyright Statement
Copyright © 2022 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC).
https://creativecommons.org/licenses/by-nc/4.0/
This is an open-access article distributed under the terms of the Creative Commons Attribution-NonCommercial license, which permits use, distribution, and reproduction in any medium, so long as the resultant use is not for commercial advantage and provided the original work is properly cited.
Updated bounds on axion-like particles from X-ray observations
(2022)
Journal Article
Axion quasiparticles for axion dark matter detection
(2021)
Journal Article
Superradiance in stars: non-equilibrium approach to damping of fields in stellar media
(2022)
Journal Article
Axion-like particle oscillations
(2022)
Journal Article
ALP anarchy
(2024)
Journal Article
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
Apache License Version 2.0 (http://www.apache.org/licenses/)
Apache License Version 2.0 (http://www.apache.org/licenses/)
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search