| Issue |
EPJ Web Conf.
Volume 297, 2024
International Symposium on Nuclear Astrophysics (ISNA23)
|
|
|---|---|---|
| Article Number | 02001 | |
| Number of page(s) | 4 | |
| Section | Contribution by Young Researchers | |
| DOI | https://doi.org/10.1051/epjconf/202429702001 | |
| Published online | 07 June 2024 | |
https://doi.org/10.1051/epjconf/202429702001
Exploring Enhanced 12C Production in Astrophysical Environments through Inverse Maxwellian Averaged Reaction Rate
1 Nuclear Physics Division, Bhabha Atomic Research Centre, Mumbai 400085, India
2 Homi Bhabha National Institute, Anushaktinagar, Mumbai 400094, India
* e-mail: abaishya@barc.gov.in
** e-mail: ssantra@barc.gov.in
Published online: 7 June 2024
A significant increase in stable 12C production can result from lightparticle- induced deexcitation from resonances above the 3α breakup threshold. The enhancement in 12C production has been calculated in the temperature range of T9 = 0.1 to 10 using the inverse Maxwellian Averaged Reaction Rate (MARR) generated directly by the TALYS code, a unique new approach. Calculated proton-induced enhancements are nearly identical to the conventional approach, but the neutron-induced enhancements are strikingly different at low temperatures. An attempt has been made to analyze the differences between the two approaches.
© 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.