Relativistic nuclear dissociation in emulsion reveals increasing contributions from 8Be(0+), 9B, and 12C Hoyle state with higher alpha multiplicity, consistent with cluster fusion.
Ajzenberg-Selove, Energy Levels of Light Nuclei, A = 3 – 20, Nucl
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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.