Fine structure in the α decay of 179Hg and 177Au
- NázevTitle
- Fine structure in the α decay of 179Hg and 177AuFine structure in the α decay of 179Hg and 177Au
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- A. Spacek, A. Herzan, M. Sedlak, M. Venhart, M. Veselský
- DOIDOI
- 10.1140/epja/s10050-025-01513-9
- Časopis / citaceJournal / citation
- European Physical Journal A, Hadrons and Nuclei. 2025, 61(3), 1-9. ISSN 1434-6001.
- RokYear
- 2025
- JazykLanguage
- eng
- WoSWoS
- 001439401900001
- ScopusScopus
- 2-s2.0-86000770638
- RIVRIV
- RIV/68407700:21670/25:00389265!RIV26-MSM-21670___
- ProjektProject
- Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
AbstraktAbstract
The alpha-decay fine structure of 179Hg and 177Au was studied by means of decay spectroscopy. Two experiments were performed at the Accelerator Laboratory of the University of Jyv & auml;skyl & auml; (JYFL), Finland, utilizing the recoil separator RITU and a digital data acquisition system. The heavy-ion induced fusion-evaporation reactions 3682Kr + 44100Ru and 3888Kr + 4292Mo were used to produce the 179Hg and 177Au nuclei, respectively. Studying the evaporation residues (ER, recoils)-alpha 1-alpha 2 correlations and alpha-gamma coincidences, a new alpha decay with E alpha = 6156(10) keV was observed from 179Hg. This decay populates the (9/2-) excited state at an excitation energy of 131.3(5) keV in 175Pt. The internal conversion coefficient for the 131.3(5) keV transition de-exciting this state was measured for the first time. Regarding the 177Au nucleus, a new alpha decay with E alpha = 5998(9) keV was observed to populate the 156.1(6) keV excited state in 173Ir. Two de-excitation paths were observed from this excited state. Moreover, a new 215.7(13) keV transition was observed to depopulate the 424.4(13) keV excited state in 173Ir. Properties of the 179Hg and 177Au alpha decays were examined in a framework of reduced widths and hindrance factors. For clarity and simplicity, the spin and parity assignments (e.g. J pi) are presented without brackets throughout the text.
The alpha-decay fine structure of 179Hg and 177Au was studied by means of decay spectroscopy. Two experiments were performed at the Accelerator Laboratory of the University of Jyv & auml;skyl & auml; (JYFL), Finland, utilizing the recoil separator RITU and a digital data acquisition system. The heavy-ion induced fusion-evaporation reactions 3682Kr + 44100Ru and 3888Kr + 4292Mo were used to produce the 179Hg and 177Au nuclei, respectively. Studying the evaporation residues (ER, recoils)-alpha 1-alpha 2 correlations and alpha-gamma coincidences, a new alpha decay with E alpha = 6156(10) keV was observed from 179Hg. This decay populates the (9/2-) excited state at an excitation energy of 131.3(5) keV in 175Pt. The internal conversion coefficient for the 131.3(5) keV transition de-exciting this state was measured for the first time. Regarding the 177Au nucleus, a new alpha decay with E alpha = 5998(9) keV was observed to populate the 156.1(6) keV excited state in 173Ir. Two de-excitation paths were observed from this excited state. Moreover, a new 215.7(13) keV transition was observed to depopulate the 424.4(13) keV excited state in 173Ir. Properties of the 179Hg and 177Au alpha decays were examined in a framework of reduced widths and hindrance factors. For clarity and simplicity, the spin and parity assignments (e.g. J pi) are presented without brackets throughout the text.