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| Journal Article | PUBDB-2026-01204 |
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2025
IOP
London
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Please use a persistent id in citations: doi:10.1088/1475-7516/2025/07/075 doi:10.3204/PUBDB-2026-01204
Report No.: BARI-TH/778-25; arXiv:2502.19476
Abstract: We investigate the potential of IAXO and its intermediate version, BabyIAXO, to detectaxions produced in core-collapse supernovae (SNe). Our study demonstrates that these experimentshave realistic chances of identifying SN axions, offering crucial insights into both axion physicsand SN dynamics. IAXO's sensitivity to SN axions allows for the exploration of regions of theaxion parameter space inaccessible through solar observations. In addition, in the event of anearby SN, d ∼ 𝒪(100) pc, and sufficiently large axion couplings, gaγ ≳ 10$^{-11}$ GeV$^{-1}$, IAXO could have a chance to significantly advanceour understanding of axion production in nuclear matter and provide valuable information about thephysics of SNe, such as pion abundance, the equation of state, and other nuclear processesoccurring in extreme environments.
Keyword(s): axions ; supernovas
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Preprint
Detecting Supernova Axions with IAXO
[10.3204/PUBDB-2025-00880]
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