EPJ Web Conf.
Volume 227, 202010th European Summer School on Experimental Nuclear Astrophysics
|Number of page(s)||4|
|Section||Session 2: Contribution by Young Researchers|
|Published online||14 January 2020|
Transfer reactions as an Indirect Method in Nuclear Astrophysics
1 National Institute of Physics and Nuclear Engineering (IFIN-HH), Bucharest-Magurele, R0-077125, Romania
2 Cyclotron Institute, Texas A & M University, College Station, TX, 77843-3366
Published online: 14 January 2020
In my presentation, I will discuss the use of transfer reactions as an indirect method of determining information important for nuclear astrophysics. Specifically, I will focus on peripheral reactions and their analysis with the Asymptotic Normalization Coefficients (ANC) method. I will present results from related experiments that have been conducted at the Cyclotron Institute, Texas A&M University with focus on the 0ptical Model Parameters obtained and the need for reliable calculations. Additionally, I will describe the im- provements in the measured data that we obtained after upgrading the detection system used.
© The Authors, published by EDP Sciences, 2020
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.
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.