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Axion dark matter: What is it and why now?

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-pari...

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Autores principales: Chadha-Day, Francesca, Ellis, John, Marsh, David J. E.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8865781/
https://www.ncbi.nlm.nih.gov/pubmed/35196098
http://dx.doi.org/10.1126/sciadv.abj3618
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author Chadha-Day, Francesca
Ellis, John
Marsh, David J. E.
author_facet Chadha-Day, Francesca
Ellis, John
Marsh, David J. E.
author_sort Chadha-Day, Francesca
collection PubMed
description 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.
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spelling pubmed-88657812022-03-10 Axion dark matter: What is it and why now? Chadha-Day, Francesca Ellis, John Marsh, David J. E. Sci Adv Physical and Materials Sciences 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. American Association for the Advancement of Science 2022-02-23 /pmc/articles/PMC8865781/ /pubmed/35196098 http://dx.doi.org/10.1126/sciadv.abj3618 Text en 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 (https://creativecommons.org/licenses/by-nc/4.0/) , 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.
spellingShingle Physical and Materials Sciences
Chadha-Day, Francesca
Ellis, John
Marsh, David J. E.
Axion dark matter: What is it and why now?
title Axion dark matter: What is it and why now?
title_full Axion dark matter: What is it and why now?
title_fullStr Axion dark matter: What is it and why now?
title_full_unstemmed Axion dark matter: What is it and why now?
title_short Axion dark matter: What is it and why now?
title_sort axion dark matter: what is it and why now?
topic Physical and Materials Sciences
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8865781/
https://www.ncbi.nlm.nih.gov/pubmed/35196098
http://dx.doi.org/10.1126/sciadv.abj3618
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