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Publications du CSNSM | |
| HAL: in2p3-00683038, version 1 |
| ADS Bibliographic id: 2012JPhCS.337a2037C |
| DOI: 10.1088/1742-6596/337/1/012037 |
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| 5th Biannual Conference on Nuclear Physics in Astrophysics (NPA)/24th Nuclear Physics Divisional Conference of the European-Physical-Society (EPS), Eliat : Israël (2011) |
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| Variation of fundamental constants and the triple-alpha reaction in Population III stars and BBN |
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| The effect of variations of the fundamental constants on the thermonuclear rate of the triple alpha reaction, 4He(αα, γ)12C, that bridges the gap between 4He and 12C is investigated. We have followed the evolution of 15 and 60 Mbigodot zero metallicity stellar models, up to the end of core helium burning. The calculated oxygen and carbon abundances resulting from helium burning can then be used to constrain the variation of the fundamental constants. To investigate the effect of an enhanced triple alpha reaction rate in Big-Bang Nucleosynthesis, we first evaluated Standard Big-Bang Nucleosynthesis CNO production with a network of more than 400 reactions using the TALYS code to calculate missing rates. |
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| 1: | CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse |
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| Subject(s) | : | Physics/Astrophysics/Solar and Stellar Astrophysics Sciences of the Universe/Astrophysics/Solar and Stellar Astrophysics |
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| THERMONUCLEAR REACTION-RATES – NUCLEAR-REACTION RATES – COMPILATION – EVOLUTION |
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| in2p3-00683038, version 1 | |
| http://hal.in2p3.fr/in2p3-00683038 | |
| oai:hal.in2p3.fr:in2p3-00683038 | |
| From: Christine Hadrossek | |
| Submitted on: Wednesday, 28 March 2012 09:50:39 | |
| Updated on: Friday, 30 November 2012 15:56:31 | |
