Carbon-12 - Wikipedia, the free encyclopedia:
"The Hoyle state is an excited state of carbon-12 with precisely the properties necessary to allow just the right amount of carbon to be created in a stellar environment. The existence of the Hoyle state is essential for the nucleosynthesis of carbon in helium-burning red giant stars. The resonant state was predicted by Fred Hoyle in the 1950s based on the observed abundances of heavy elements in the universe. The resonant state allows carbon to be produced via the triple-alpha process. The existence of the Hoyle state has been confirmed experimentally, but its precise properties are still being investigated.[2] In 2011, an ab initio calculation of the low-lying states of carbon-12 found (in addition to the ground and excited spin-2 state) a resonance with all of the properties of the Hoyle state.[3][4]"
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