Relativistic nuclear dissociation in emulsion reveals increasing contributions from 8Be(0+), 9B, and 12C Hoyle state with higher alpha multiplicity, consistent with cluster fusion.
Salpeter, Energy Production in Stars, Annual Review of Nuclear and Particle Science 2 (1953) 41
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The $^{8}$Be nucleus and the Hoyle state in dissociation of relativistic nuclei
Relativistic nuclear dissociation in emulsion reveals increasing contributions from 8Be(0+), 9B, and 12C Hoyle state with higher alpha multiplicity, consistent with cluster fusion.