Experimentally Constrained Nuclear Level Density for Doubly Magic 56Ni in the rp-Process
Abstract
Constraining the nuclear level density of doubly magic 56Ni is important for modeling its role in the Ni-Cu cycle, which affects the final elemental abundances produced from the astrophysical rp-process.
Status
Graduate
Department
Physics & Astronomy
College
College of Arts and Sciences
Campus
Athens
Faculty Mentor
Richard, Andrea
Creative Commons License
This work is licensed under a Creative Commons Attribution-NonCommercial-No Derivative Works 4.0 International License.
Experimentally Constrained Nuclear Level Density for Doubly Magic 56Ni in the rp-Process
Constraining the nuclear level density of doubly magic 56Ni is important for modeling its role in the Ni-Cu cycle, which affects the final elemental abundances produced from the astrophysical rp-process.