| Issue |
EPJ Web Conf.
Volume 184, 2018
9th European Summer School on Experimental Nuclear Astrophysics
|
|
|---|---|---|
| Article Number | 02001 | |
| Number of page(s) | 4 | |
| Section | Session 2 | |
| DOI | https://doi.org/10.1051/epjconf/201818402001 | |
| Published online | 29 June 2018 | |
https://doi.org/10.1051/epjconf/201818402001
Proton-Induced Reactions of Astrophysical Interest
SUPA, School of Physics and Astronomy, University of Edinburgh,
Edinburgh, UK
* e-mail: Thomas.Chillery@ed.ac.uk
Published online: 29 June 2018
A discrepancy exists between the 6Li abundances predicted from big bang nucleosynthesis models and those measured in pre-main sequence stars. To further constrain the predicted abundances of 6Li in these stars, high accuracy measurements are required of reactions destroying 6Li. Namely 6Li(p,γ)7Be and 6Li(p,α) 3He. These have recently been studied at the Laboratory for Underground Nuclear Astrophysics (LUNA) to measure their low energy cross sections. I present both the campaign’s experimental setup and current status of the data analysis.
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.