Bulletin of the American Physical Society
6th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Sunday–Friday, November 26–December 1 2023; Hawaii, the Big Island
Session DB03: CEU Poster Session & Physical Review Reception (2:00 P.M. - 4:00 P.M. HST)
2:00 PM,
Wednesday, November 29, 2023
Hilton Waikoloa Village
Room: Lagoon Lanai
Chair: Shelly Lesher, University of Wisconsin La Crosse
Abstract: DB03.00015 : Radioactive Stacked Foil Analysis for Nuclear Cross-sections*
Presenter:
Leonith Rodriguez
(University of Texas at El Paso)
Authors:
Leonith Rodriguez
(University of Texas at El Paso)
Laura A McCann
(Texas A&M University)
Jerome Gauthier
(Texas A&M University)
sherry J yennello
(TAMU)
Collaboration:
SJY group
This project aims to discover what other isotopes were created during the production of terbium-149 which consisted of a beam of lithium-6 on a natural samarium target at different energies. Some predictions can be made by looking at the chart of nuclides and focusing on the isotopes’ half-lives, stabilities, and properties. After a single night of beam, the foils were counted a day after irradiation, using three high-purity germanium (HPGe) detectors. Background, natural samarium foils (with thicknesses of 100 and 250 micrometers), europium-152 source, and gold foils (with a thickness of 5 micrometers) data was collected on the HPGes. To analyze these spectra, the python toolkit called Curie was used to simplify the identification and fitting of the peaks. After calibrating the spectra using the europium-152 source in Curie, the resulting isotopes can be identified. With this data we can conclude that the isotope production of terbium-149 via this method may be possible, but more measurements will need to be performed to confirm the optimal production pathway.
The project focus on one single night of data collected. Three detectors were used. The data was gathered a day after the reaction occurred. Each detector holds data files of background (when no beam or target are involved), natural Samarium with a thickness of 100 and 250 micrometers (Which may include different stable isotopes), Europium-152 (Used as calibration energy source), and Gold with a thickness of 5 micrometers (used as target). Giving us an approximate total of 700 runs.
*Departmenf Of Energy grant number DE-FG02-93ER40773TREND funded by Department of Energy grant nuber DE-SC0022469
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