Indirect techniques for astrophysical reaction rates determinations
| Autor: | Alison Laird, N. de Séréville, N. Oulebsir, P. Roussel, S. Benamara, I. Stefan, Fairouz Hammache, A. Coc |
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| Přispěvatelé: | Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11) |
| Jazyk: | angličtina |
| Rok vydání: | 2016 |
| Předmět: |
Nuclear reaction
Physics 010308 nuclear & particles physics QC1-999 Context (language use) Inelastic scattering 01 natural sciences 7. Clean energy Reaction rate Nuclear physics Stars 13. Climate action 0103 physical sciences 010306 general physics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Nuclear Experiment |
| Zdroj: | EPJ Web of Conferences, Vol 117, p 09003 (2016) EPJ Web Conf. 12th International Conference on Nucleus-Nucleus Collisions 12th International Conference on Nucleus-Nucleus Collisions, Jun 2015, Catania, Italy. pp.09003, ⟨10.1051/epjconf/201611709003⟩ |
| Popis: | International audience; Direct measurements of nuclear reactions of astrophysical interest can be challenging. Alternative experimental techniques such as transfer reactions and inelastic scattering reactions offer the possibility to study these reactions by using stable beams. In this context, I will present recent results that were obtained in Orsay using indirect techniques. The examples will concern various astrophysical sites, from the Big-Bang nucleo synthesis to the production of radioisotopes in massive stars. |
| Databáze: | OpenAIRE |
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