A recent experiment with the JUROGAM III - MARA spectrometer at JYFL (University of Jyväskylä Institute of Physics) allowed for the first time the production of 29S via 3-neutron evaporation starting from the 20Ne+12C fusion-evaporation reaction. This experiment extends the possibility of testing the Shell Model predictions to the A=29 T=3/2 isobaric multiplet. In the present work we aim to investigate the populated reaction channels and to reconstruct the level scheme of 29S, one of the main contaminants. Moreover, the estimation of the production cross-section of 29S from fusion-evaporation of 20Ne+12C will be obtained as a function of the excitation energy.

A recent experiment with the JUROGAM III - MARA spectrometer at JYFL (University of Jyväskylä Institute of Physics) allowed for the first time the production of 29S via 3-neutron evaporation starting from the 20Ne+12C fusion-evaporation reaction. This experiment extends the possibility of testing the Shell Model predictions to the A=29 T=3/2 isobaric multiplet. In the present work we aim to investigate the populated reaction channels and to reconstruct the level scheme of 29S, one of the main contaminants. Moreover, the estimation of the production cross-section of 29S from fusion-evaporation of 20Ne+12C will be obtained as a function of the excitation energy.

First production of the isospin T=3/2 nucleus 29S using the 3-neutron evaporation channel of the 20Ne+12C fusion reaction

LAZZARETTO, DENISE
2023/2024

Abstract

A recent experiment with the JUROGAM III - MARA spectrometer at JYFL (University of Jyväskylä Institute of Physics) allowed for the first time the production of 29S via 3-neutron evaporation starting from the 20Ne+12C fusion-evaporation reaction. This experiment extends the possibility of testing the Shell Model predictions to the A=29 T=3/2 isobaric multiplet. In the present work we aim to investigate the populated reaction channels and to reconstruct the level scheme of 29S, one of the main contaminants. Moreover, the estimation of the production cross-section of 29S from fusion-evaporation of 20Ne+12C will be obtained as a function of the excitation energy.
2023
First production of the isospin T=3/2 nucleus 29S using the 3-neutron evaporation channel of the 20Ne+12C fusion reaction
A recent experiment with the JUROGAM III - MARA spectrometer at JYFL (University of Jyväskylä Institute of Physics) allowed for the first time the production of 29S via 3-neutron evaporation starting from the 20Ne+12C fusion-evaporation reaction. This experiment extends the possibility of testing the Shell Model predictions to the A=29 T=3/2 isobaric multiplet. In the present work we aim to investigate the populated reaction channels and to reconstruct the level scheme of 29S, one of the main contaminants. Moreover, the estimation of the production cross-section of 29S from fusion-evaporation of 20Ne+12C will be obtained as a function of the excitation energy.
Nuclear physics
Gamma spectroscopy
Fusion-evaporation
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.12608/70111