New collective structures in 179Au and their implications for the triaxial deformation of the 178Pt core
Balogh, M., Jajčišinová, E., Venhart, M., Herzáň, A., Wood, J. L., Joss, D. T., Ali, F. A., Auranen, K., Bánovská, S., Bírová, M., Carroll, R. J., Cox D., M., Cubiss J., G., Davis, T., Drummond M., C., Greenlees, P. T., Grahn, T., Gredley, A., Henderson, J., . . . Wearing, F. P. (2022). New collective structures in 179Au and their implications for the triaxial deformation of the 178Pt core. Physical Review C, 106(6), Article 064324. https://doi.org/10.1103/PhysRevC.106.064324
Julkaistu sarjassa
Physical Review CTekijät
Päivämäärä
2022Oppiaine
KiihdytinlaboratorioYdin- ja kiihdytinfysiikan huippuyksikköFysiikkaAccelerator LaboratoryCentre of Excellence in Nuclear and Accelerator Based PhysicsPhysicsTekijänoikeudet
©2022 American Physical Society
The extremely neutron-deficient isotope 179Au has been studied by a combination of in-beam γ-ray and isomeric-decay spectroscopy. For in-beam spectroscopy, the recoil-isomer tagging technique was employed, using the known 3/2−, T1/2=328 ns isomer. A new rotational band, associated with the unfavored signature band of the 1h9/2⊕2f7/2 proton-intruder configuration, was revealed. A previously unknown, high-spin isomeric state with an excitation energy of 1743(17) keV and T1/2=2.16(8)µs was discovered. Five decay paths were identified, some of them feeding previously unknown non-yrast excited states, associated with the 1i13/2 proton-intruder configuration. Calculations based on the particle-plus-triaxial-rotor model were performed to interpret the data. On the basis of these calculations, the new 1h9/2⊕2f7/2 rotational band is interpreted as due to triaxial deformation of the underlying configuration with β2≈0.26 and γ≈27∘. Observed non-yrast states of the positive-parity 1i13/2 intruder configuration are interpreted as due to triaxial deformation with β2≈0.26 and γ≈20∘.
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American Physical SocietyISSN Hae Julkaisufoorumista
2469-9985Asiasanat
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https://converis.jyu.fi/converis/portal/detail/Publication/176869008
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The authors express their gratitude to the staff of the Accelerator Laboratory of the University of Jyväskylä for their excellent technical support. This work has been sup ported by the EU-FP7-IA project ENSAR (No. 262010), the Academy of Finland (CoE in Nuclear and Accelerator Based Physics, grant to T.G., Contract No. 131665), the STFC Grant No. ST/P003885/1, the European Research Council through the project SHESTRUCT (Grant Agreement No. 203481), the UK Science and Technology Facilities Council, the Slo vak Research and Development Agency under Contract No. APVV-20-0532, Slovak grant agency VEGA (Contract No. 2/0067/21), and the Research and Development Operational Programme funded by the European Regional Develop ment Fund, Project No. ITMS code 26210120023 (20%). M. Ven. acknowledges funding from the ESET Foundation (Slovakia). ...Lisenssi
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