Bulletin of the American Physical Society
2024 Annual Meeting of the APS Four Corners Section
Friday–Saturday, October 11–12, 2024; Northern Arizona University, Flagstaff, Arizona
Session K01: Poster Session (4:00pm - 6:00pm)
4:00 PM,
Friday, October 11, 2024
Northern Arizona University
Room: Ballroom
Abstract: K01.00033 : Prediction of Neutron Flux Distribution inside a Pure Carbon Moderator
Presenter:
Olivia R Cantrell
(New Mexico Institute of Mining and Technology)
Authors:
Olivia R Cantrell
(New Mexico Institute of Mining and Technology)
Rene Reifarth
(Los Alamos National Laboratory)
Aaron J Couture
(Los Alamos National Laboratory (LANL))
Andrew L Cooper
(Los Alamos National Laboratory)
Collaboration:
Los Alamos National Laboratory
Neutron captures on unstable isotopes are important for a plethora of applications including neutron-induced nucleosynthesis. Nucleosynthesis is the process that creates new atoms from pre-existing nucleons that are more complex than the Hydrogen atom. What we can learn from nucleosyththesis calculations is the space-time distribution of matter in the universe as well as information on stellar evolution. A new experimental method to determine neutron capture cross sections are based on the moderation of high-energy neutrons in carbon moderators. To confirm Monte-Carlo simulations that predict neutron flux distribution, multiple gold wires were activated with different neutron spectra within a cubical moderator made of pure carbon. The activation of the gold wire was measured with high-purity Germanium detectors. This experiment was conducted in conjunction with the University of Notre Dame, where the experimental equipment for this project were utilized. Upon conducting the experiment, the Monte-Carlo simulations were optimized to better fit the experimental results.
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