2004•Chinese Physics LettersOpen access

Identification of Oblate Band in Odd–Odd 184 Au

Zhang Yu-Hu, Hualei Wang, G. de Angelis, Nicolae M. Mărginean, Andrés Gadea, Daniel Ricardo Napoli, Michael Axiotis, Catalin Rusu, T. Martínez, Zhou Xiao-Hong, Wentao Guo, Minliang Liu, Lei Xiang-Guo, Guo Ying-Xiang, F. R. Xu

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Abstract

High-spin states in 184 Au have been populated via the 149 Sm( 29 Si, 4 n γ) 184 Au reaction at a beam energy of 140 MeV. Three- or higher-fold γ-ray coincidences have been measured using the multidetector array of GASP. A rotational band built on the 11 − oblate π h 11/2 −1 ⊗ν i 13/2 −1 structure has been newly observed, similar to those reported in 186−194 Au. This result extends the knowledge of shape coexistence to the currently lightest odd–odd Au isotope.

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High-spin states in 184 Au have been populated via the 149 Sm( 29 Si, 4 n γ) 184 Au reaction at a beam energy of 140 MeV. Three- or higher-fold γ-ray coincidences have been measured using the multidetector array of GASP. A rotational band built on the 11 − oblate π h 11/2 −1 ⊗ν i 13/2 −1 structure has been newly observed, similar to those reported in 186−194 Au. This result extends the knowledge of shape coexistence to the currently lightest odd–odd Au isotope.

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Available abstract

High-spin states in 184 Au have been populated via the 149 Sm( 29 Si, 4 n γ) 184 Au reaction at a beam energy of 140 MeV. Three- or higher-fold γ-ray coincidences have been measured using the multidetector array of GASP. A rotational band built on the 11 − oblate π h 11/2 −1 ⊗ν i 13/2 −1 structure has been newly observed, similar to those reported in 186−194 Au. This result extends the knowledge of shape coexistence to the currently lightest odd–odd Au isotope.

Key concepts: Oblate spheroid, Physics, Beam energy, Isotope, Atomic physics, Spin (aerodynamics), Beam (structure), Nuclear physics

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