A technique for studying (n,p) reactions of astrophysical interest using radioactive beams with SECAR

A technique for studying (n,p) reactions of astrophysical interest using radioactive beams with SECAR

The formation of nuclei in slightly proton-rich regions of the neutrino-driven wind of core-collapse supernovae could be attributed to the neutrino-p process (νp-process). As it proceeds via a sequence of (p,γ) and (n,p) reactions, it may produce elements in the range of Ni and Sn, considering adequ...

Full description

Bibliographic Details
Main Authors: Tsintari Pelagia, Berg Georg P. A., Blackmon Jeff, Chipps Kelly, Couder Manoel, Deibel Catherine, Dimitrakopoulos Nikolaos, Garg Ruchi, Greife Uwe, Hermansen Kirby, Hood Ashley, Jain Rahul, Maher Cavan, Marshall Caleb, Meisel Zach, Miskovich Sara, Montes Fernando, Perdikakis Georgios, Pereira Jorge, Ruland Thomas, Schatz Hendrik, Setoodehnia Kiana, Smith Michael, Wagner Louis, Zegers Remco G. T.
Format: Article
Language:English
Published: EDP Sciences 2023-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_13005.pdf

Internet

https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_13005.pdf

Similar Items