Stellar Evolution Bounds on the ALP-Photon Coupling: new Results and Perspectives
Maurizio Giannotti

TL;DR
This paper reviews stellar evolution constraints on the axion-like particle (ALP) photon coupling, presenting new bounds from horizontal branch stars that improve existing limits across a broad mass range.
Contribution
It offers a comprehensive review and a novel analysis of bounds from helium burning stars, establishing the strongest constraints on g_{a extgamma} to date.
Findings
New bounds from horizontal branch stars are the most stringent to date.
The analysis covers a wide ALP mass range.
Stellar evolution provides critical limits on ALP-photon interactions.
Abstract
Stellar evolution considerations are of fundamental importance in our understanding of the axion/ALP-photon coupling, g_{a\gamma}. Helium burning stars are the best laboratories to study this coupling. Here, we will review the bounds from massive and low mass helium burning stars, and present a new analysis of the bound from the horizontal branch stars. The analysis provides the strongest bound to date on g_{a\gamma} in a wide mass range.
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae
