Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich region

We present experimental evidence for the one- and two-phonon γ vibrational bands in the isotopes 103−108Mo by analyzing high-statistics γ-γ-γ and γ-γ-γ-γ coincidence data from the spontaneous fission of 252Cf. The consistency of the one- and two-phonon γ bands in both odd- and even-mass isotopes wit...

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Main Authors: Wang E.H., Abushawish M., Hamilton J.H., Dudouet J., Navin A., Bhattacharyya S., Stezowski O., Bhat G., Sheikh J.A., Jehangir S., Rejmund M., Lemasson A., Clément E., Sun S., Zhang H., Xu W.Z., Wang S.Y., Qi B., Jiao C.F., Luo Y.X., Rasmussen J.O., Zhu S.J.
Format: Article
Language:English
Published: EDP Sciences 2025-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2025/09/epjconf_nsd2024_00022.pdf
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author Wang E.H.
Abushawish M.
Hamilton J.H.
Dudouet J.
Navin A.
Bhattacharyya S.
Stezowski O.
Bhat G.
Sheikh J.A.
Jehangir S.
Rejmund M.
Lemasson A.
Clément E.
Sun S.
Zhang H.
Xu W.Z.
Wang S.Y.
Qi B.
Jiao C.F.
Luo Y.X.
Rasmussen J.O.
Zhu S.J.
author_facet Wang E.H.
Abushawish M.
Hamilton J.H.
Dudouet J.
Navin A.
Bhattacharyya S.
Stezowski O.
Bhat G.
Sheikh J.A.
Jehangir S.
Rejmund M.
Lemasson A.
Clément E.
Sun S.
Zhang H.
Xu W.Z.
Wang S.Y.
Qi B.
Jiao C.F.
Luo Y.X.
Rasmussen J.O.
Zhu S.J.
author_sort Wang E.H.
collection DOAJ
description We present experimental evidence for the one- and two-phonon γ vibrational bands in the isotopes 103−108Mo by analyzing high-statistics γ-γ-γ and γ-γ-γ-γ coincidence data from the spontaneous fission of 252Cf. The consistency of the one- and two-phonon γ bands in both odd- and even-mass isotopes within this range provides a robust test for microscopic theories. Additionally, we have identified evidence for one-, two-, and possibly three-phonon γ bands in 103,105Nb. Triaxial projected shell model calculations successfully reproduce the level structures and align well with the excitation energies of the observed one- and two-phonon γ bands. The potential existence of three-phonon γ bands in 103,105Nb is further supported by recent particle-vibration coupling model calculations. Furthermore, chiral vibrational bands have been observed in 104,106Mo.
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institution Kabale University
issn 2100-014X
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publishDate 2025-01-01
publisher EDP Sciences
record_format Article
series EPJ Web of Conferences
spelling doaj-art-14fcb64d9268490a8e3bbb84e27f16a12025-08-20T03:54:07ZengEDP SciencesEPJ Web of Conferences2100-014X2025-01-013240002210.1051/epjconf/202532400022epjconf_nsd2024_00022Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich regionWang E.H.0Abushawish M.1Hamilton J.H.2Dudouet J.3Navin A.4Bhattacharyya S.5Stezowski O.6Bhat G.7Sheikh J.A.8Jehangir S.9Rejmund M.10Lemasson A.11Clément E.12Sun S.13Zhang H.14Xu W.Z.15Wang S.Y.16Qi B.17Jiao C.F.18Luo Y.X.19Rasmussen J.O.20Zhu S.J.21School of Energy and Power Engineering, Shandong UniversityUniversité de Lyon 1, CNRS/IN2P3, UMR5822, IP2IDepartment of Physics and Astronomy, Vanderbilt UniversityUniversité de Lyon 1, CNRS/IN2P3, UMR5822, IP2IGANIL, CEA/DRF-CNRS/IN2P3, BP 55027Variable Energy Cyclotron Centre, 1/AF BidhannagarUniversité de Lyon 1, CNRS/IN2P3, UMR5822, IP2IDepartment of Physics, Government Degree College ShopianDepartment of Physics, Islamic University of Science and TechnologyDepartment of Physics, Islamic University of Science and TechnologyGANIL, CEA/DRF-CNRS/IN2P3, BP 55027GANIL, CEA/DRF-CNRS/IN2P3, BP 55027GANIL, CEA/DRF-CNRS/IN2P3, BP 55027School of Space Science and Technology, Institute of Space Sciences, Shandong UniversitySchool of Space Science and Technology, Institute of Space Sciences, Shandong UniversitySchool of Space Science and Technology, Institute of Space Sciences, Shandong UniversitySchool of Energy and Power Engineering, Shandong UniversitySchool of Space Science and Technology, Institute of Space Sciences, Shandong UniversitySchool of Physics and Astronomy, Sun Yat-sen UniversityLawrence Berkeley National LaboratoryLawrence Berkeley National LaboratoryDepartment of Physics, Tsinghua UniversityWe present experimental evidence for the one- and two-phonon γ vibrational bands in the isotopes 103−108Mo by analyzing high-statistics γ-γ-γ and γ-γ-γ-γ coincidence data from the spontaneous fission of 252Cf. The consistency of the one- and two-phonon γ bands in both odd- and even-mass isotopes within this range provides a robust test for microscopic theories. Additionally, we have identified evidence for one-, two-, and possibly three-phonon γ bands in 103,105Nb. Triaxial projected shell model calculations successfully reproduce the level structures and align well with the excitation energies of the observed one- and two-phonon γ bands. The potential existence of three-phonon γ bands in 103,105Nb is further supported by recent particle-vibration coupling model calculations. Furthermore, chiral vibrational bands have been observed in 104,106Mo.https://www.epj-conferences.org/articles/epjconf/pdf/2025/09/epjconf_nsd2024_00022.pdf
spellingShingle Wang E.H.
Abushawish M.
Hamilton J.H.
Dudouet J.
Navin A.
Bhattacharyya S.
Stezowski O.
Bhat G.
Sheikh J.A.
Jehangir S.
Rejmund M.
Lemasson A.
Clément E.
Sun S.
Zhang H.
Xu W.Z.
Wang S.Y.
Qi B.
Jiao C.F.
Luo Y.X.
Rasmussen J.O.
Zhu S.J.
Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich region
EPJ Web of Conferences
title Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich region
title_full Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich region
title_fullStr Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich region
title_full_unstemmed Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich region
title_short Multi-phonon γ vibrational bands and chiral vibrations in the A∼100 neutron-rich region
title_sort multi phonon γ vibrational bands and chiral vibrations in the a∼100 neutron rich region
url https://www.epj-conferences.org/articles/epjconf/pdf/2025/09/epjconf_nsd2024_00022.pdf
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