Consistent Description of the $${^{12}{\rm C}(0_2^+)}$$ State
| Autor: | S. I. Fedotov, A. V. Malykh, O. I. Kartavtsev |
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| Rok vydání: | 2009 |
| Předmět: | |
| Zdroj: | Few-Body Systems. 45:153-155 |
| ISSN: | 1432-5411 0177-7963 |
| Popis: | The excited $${0_2^+}$$ state of 12C is of key importance for description of the triple-α reaction, which is the only way for helium burning in stars. Authors’ efforts to calculate the lowest 0+ states within the framework of the α-cluster model are summarized and discussed. In particular, the recently calculated $${0_2^+}$$ state’s width and $${0_2^+ \to 0_1^+ }$$ transition density are in good agreement with the experimental data. |
| Databáze: | OpenAIRE |
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