Abstract
We review the current status of astrophysical bounds on QCD axions, primarily based on the observational effects of nonstandard energy losses on stars, including black-hole superradiance. Over the past few years, many of the traditional arguments have been reexamined both theoretically and using modern data and new ideas have been put forth. This compact review updates similar Lecture Notes written by one of us in 2006.
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CITATION STYLE
APA
Caputo, A., & Raffelt, G. (2024). Astrophysical Axion Bounds: The 2024 Edition. In Proceedings of Science (Vol. 454). Sissa Medialab Srl. https://doi.org/10.22323/1.454.0041
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