EPJ Web Conf.
Volume 260, 2022The 16th International Symposium on Nuclei in the Cosmos (NIC-XVI)
|Number of page(s)||4|
|Section||Nuclear Properties for Astrophysics|
|Published online||24 February 2022|
Experimental studies on astrophysical reactions at the low-energy RI beam separator CRIB
1 Center for Nuclear Study (CNS), University of Tokyo, Wako, Japan
2 China Institute of Atomic Energy, Beijing, China
3 School of Physics and Astronomy, the University of Edinburgh, Edinburgh, UK and Nuclear Engineering (IFIN-HH), Bucharest-M˘
4 Extreme Light Infrastructure – Nuclear Physics, Horia Hulubei National Institute for R&D in Physics agurele, Romania
5 Istituto Nazionale di Fisica Nucleare -Laboratori Nazionali del Sud, Catania, Italy
6 Department of Physics and Astronomy, University of Catania, Catania, Italy
7 Centro Siciliano di Fisica Nucleare e Struttura della Materia, CSFNSM, Catania, Italy
8 Department of Physics, University of Jyväskylä, Jyväskylä, Finland
9 Department of Physics, Sungkyunkwan University, Suwon, Korea
10 Center for Exotic Nuclear Studies, Institute for Basic Science, Daejeon, Korea
11 The Institute of Physical and Chemical Research (RIKEN), Wako, Japan
12 Faculty of Engineering and Architecture, Kore University of Enna, Enna, Italy
13 Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, China
14 Research Center for Nuclear Physics (RCNP), Osaka University, Osaka, Japan
15 Department of Physics, Tohoku University, Sendai, Japan
16 Department of Physics, Ewha Womans University, Seoul, Korea
17 Korea University, Seoul, Korea
18 Institute for Nuclear Research (Atomki), Debrecen, Hungary
19 Department of Physics, University of Naples Federico II, Naples, Italy
20 Istituto Nazionale di Fisica Nucleare -Section of Naples, Naples, Italy
21 Rare Isotope Science Project, Institute for Basic Science, Daejeon, Korea
22 Istituto Nazionale di Fisica Nucleare -Section of Perugia, Perugia, Italy
23 Department of Physics and Geology, University of Perugia, Perugia, Italy
24 Faculty of Physics, VNU University of Science, Hanoi, Vietnam
25 School of Nuclear Science and Technology, University of Chinese Academy of Sciences, Beijing, China
26 School of Physics and Astronomy, Monash University, Victoria, Australia
27 The Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, MI, USA
28 Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
29 College of Nuclear Science and Technology, Beijing Normal University, Beijing, China
30 Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-Sen University, Zhuhai, China
31 Department of Physics & Astronomy, McMaster University, Ontario, Canada
32 Technische Universität Darmstadt, Darmstadt, Germany
33 Département de Physique, Université Libre de Bruxelles, Bruxelles, Belgium
34 School of Nuclear Science and Technology, Lanzhou University, Lanzhou, China
* e-mail: email@example.com
Published online: 24 February 2022
Experimental studies on astrophysical reactions involving radioactive isotopes (RI) often accompany technical challenges. Studies on such nuclear reactions have been conducted at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study, the University of Tokyo. We discuss two cases of astrophysical reaction studies at CRIB; one is for the 7Be+n reactions which may affect the primordial 7Li abundance in the Big-Bang nucleosynthesis, and the other is for the 22Mg(α, p) reaction relevantin X-raybursts.
© The Authors, published by EDP Sciences, 2022
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.