Abstract
The nucleus 12C has a rather significant role in modern nuclear physics, but whose influence can be traced to the work of Hoyle in the 1950s, when it was concluded that there should be a state close to 7.68 MeV responsible for the synthesis of carbon in stellar nucleosynthesis. Although a state at 7.65 MeV was subsequently discovered, its properties have remained something of a mystery until rather recently. This paper explores our current understanding of the structure of 12C, in particular the nature of the Hoyle state.
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Acknowledgements
The author would like to thank his collaborators, particularly colleagues at Birmingham and iThemba Laboratories whose contributions have been crucial in developing the present understanding of the structure of 12C.
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FREER, M. The structure of 12C. Pramana - J Phys 83, 643–650 (2014). https://doi.org/10.1007/s12043-014-0859-6
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DOI: https://doi.org/10.1007/s12043-014-0859-6