2004
DOI: 10.1103/physrevc.70.014006
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3α-cluster structure of the0+states inC12

Abstract: The 0 + states of 12 C are considered within the framework of the microscopic three-α-cluster model. The main attention is paid to accurate calculation of the width of the extremely narrow near-threshold 0 + 2 state which plays a key role in stellar nucleosynthesis. It is shown that the

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Cited by 31 publications
(53 citation statements)
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“…The low-lying resonance states of 12 C have been studied over many years both theoretically and experimentally, motivated partly by their astrophysical importance [1][2][3][4][5][6][7][8][9][10]. Surprisingly, many issues are still not really understood, e.g., the energies, angular momenta, structure, and decay properties of the resonances.…”
Section: Introductionmentioning
confidence: 99%
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“…The low-lying resonance states of 12 C have been studied over many years both theoretically and experimentally, motivated partly by their astrophysical importance [1][2][3][4][5][6][7][8][9][10]. Surprisingly, many issues are still not really understood, e.g., the energies, angular momenta, structure, and decay properties of the resonances.…”
Section: Introductionmentioning
confidence: 99%
“…Decay through 8 Be(2 + ) is possible in both cases but this state is rather broad and the result would be hard to distinguish from direct decay. We see no indication of population of this channel in the numerical results.…”
Section: Computed Distributionsmentioning
confidence: 99%
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