| Issue |
EPJ Web Conf.
Volume 260, 2022
The 16th International Symposium on Nuclei in the Cosmos (NIC-XVI)
|
|
|---|---|---|
| Article Number | 01001 | |
| Number of page(s) | 7 | |
| Section | Nuclear Reaction Rates and Stellar Abundances | |
| DOI | https://doi.org/10.1051/epjconf/202226001001 | |
| Published online | 24 February 2022 | |
https://doi.org/10.1051/epjconf/202226001001
An indirect technique in nuclear astrophysics: alpha-cluster transfer reaction
China Institute of Atomic Energy, P.O. Box 275 (10), Beijing 102413, China
* e-mail: fermi09@foxmail.com
Published online: 24 February 2022
Helium(4He, or α)is the second most abundant element in the observable Universe. The α-particle induced reactions such as(α, γ), (α, n) and (α, p) play a crucial role in nuclear astrophysics, especially for understanding stellar heliumburning. Because of the strong Coulomb repulsion, it is greatly hindered to directly measure the cross sections for these α-capture reactions at stellar energies. Alpha-cluster transfer reaction is a powerful tool for investigation of astrophysical(α, γ), (α, n)and(α, p)reactions since it can preferentially populate the natural-parity states with an α-cluster structure which dominantly contribute to these astrophysical α-capture reactions during stellar heliumburning. In this paper, we reviewthe theoretical scheme, theexperimental technique, astrophysical applications and the future perspectives of such approach based on α-cluster transfer reactions.
© The Authors, published by EDP Sciences, 2022
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