EPJ Web of Conferences
Volume 117, 201612th International Conference on Nucleus-Nucleus Collisions 2015
|Number of page(s)||8|
|Section||IX. Nuclear Astrophysics|
|Published online||11 May 2016|
Indirect techniques for astrophysical reaction rates determinations
1 IPN, IN2P3-CNRS, Université Paris sud 11, 91406 Orsay, France
2 LPT, Université A. Mira, 06000 Béjaia, Algérie
3 LPCQ, Université Mouloud Mammeri, Tizi-Ouzou, Algérie
4 CSNSM, IN2P3-CNRS, Université Paris Sud 11, 91405 Orsay, France
5 Department of Physics, University of York, York, UK
Published online: 11 May 2016
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.
© Owned by the authors, published by EDP Sciences - SIF, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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