Issue |
EPJ Web Conf.
Volume 297, 2024
International Symposium on Nuclear Astrophysics (ISNA23)
|
|
---|---|---|
Article Number | 01012 | |
Number of page(s) | 5 | |
Section | Lectures | |
DOI | https://doi.org/10.1051/epjconf/202429701012 | |
Published online | 07 June 2024 |
https://doi.org/10.1051/epjconf/202429701012
Theoretical applications to nuclear astrophysics
1 Department of Physics, Punjabi University Patiala, Patiala 147002, Punjab, India.
2 Department of Mathematics, Lyallpur Khalsa College, Jalandhar 144001, Punjab, India.
* e-mail: shubhchintak_phy@pbi.ac.in
Published online: 7 June 2024
Nuclear reaction study is important to understand elemental abundance in the universe and stability of stars. For several reactions due to the paucity of experimental data or diffculties in performing the direct measurements, we depend upon theoretical estimates and therefore one needs reliable theoretical models with minimum inputs. This paper is a short review of our work on nuclear reactions and their applications to astrophysics. In particular, we discuss the nuclear transfer and breakup reaction while focusing on our theoretical modelings and techniques involved.
© The Authors, published by EDP Sciences, 2024
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.