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During a core-collapse supernova (SN), axionlike particles (ALPs) could be produced through the Primakoff process and subsequently convert into $\gamma$ rays in the magnetic field of the Milky Way.
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A. Gal-Yam, P. Nugent, J. Silverman, C. Badenes, T. Matheson, E. Walker et al., PTF weekly SN discovery report, April 15, 2011 , The Astronomer’s Telegram 3288
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Cambridge Astrophysics
S. Woosley, Models for gamma-ray burst progenitors and central engines , p. 191–214 · 2012
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Cambridge Astrophysics
J. Hjorth and J. S. Bloom, The GRB–supernova connection , p. 169–190 · 2012
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M. Im, C. Choi, S.-Y. Lee, G. Lim, S. Hwang, D. Milzaqulov et al., IMSNG: Light curve analysis suggests SN 2017ein as a young SN at the time of the discovery , The Astronomer’s Telegram 10481
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