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The hot and dense core formed in the collapse of a massive star is a powerful source of hypothetical feebly-interacting particles such as sterile neutrinos, dark photons, axion-like particles (ALPs), and others.
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F. S. Kitaura, H. T. Janka and W. Hillebrandt, Explosions of O-Ne-Mg cores, the Crab supernova, and subluminous type II-P supernovae , Astron. Astrophys. 450
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G. G. Raffelt, Astrophysical axion bounds , Lect. Notes Phys. 741
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M. J. Dolan, T. Ferber, C. Hearty, F. Kahlhoefer and K. Schmidt-Hoberg, Revised constraints and belle ii sensitivity for visible and invisible axion-like particles , Journal of High Energy Physics 2017
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in: P. A. Zyla et al., Review of Particle Physics
D. E. Groom and S. R. Klein, Passage of particles through matter , · 2020
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