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Sample records for e4-transitions

  1. Description of E4 Transitions in A = 192, 194,196, 198 Platinum Isotopes in a Microscopic sdgIBM- 1

    Institute of Scientific and Technical Information of China (English)

    ZHANG ZhanJun; YANG Jie; WANG Xin; LIU Yong

    2001-01-01

    Influence of the effective fermion hexadecapole force newly incorporated in a microscopic sdgIBM-1 on spectra, reduced E2 and E4 transition matrix elements (T(E2)s and T(E4)s) in the even-even platinum isotopes (A = 192,194,196,198) is investigated in terms of numerical calculations. It is found that the introduced interaction causes only limited modification to the spectrum and T(E2)s, apart from a few exceptions. However, it plays an essential role in describing E4 transitions. Thus in the case that the interaction is incorporated with certain strength, a reasonable description of all the E4 transitions in the platinum isotopes is reached in the microscopic sdgIBM-1 in comparing both to experimental data and the results calculated in phenomenological boson model.``

  2. Electric moments and charge deformation parameters in 152,154Sm, 156Gd, and 166Er

    NARCIS (Netherlands)

    Fischer, H.; Kamke, D.; Kittling, H.J.; Kuhlmann, E.; Plicht, H.; Schormann, R.

    1977-01-01

    Coulomb excitation experiments with α particles were performed on the four rare-earth nuclei 152,154Sm, 156Gd, and 166Er. E2 and E4 transition matrix elements of low-lying levels in the rotational ground-state bands were obtained. Model dependent charge deformation parameters βc2 and βc4 were extrac

  3. Calculation of the Nuclear Transition Charge Density in a Microscopic sdgIBM-1

    Institute of Scientific and Technical Information of China (English)

    ZHANG Zhan-Jun; SANG Jian-ping; LIU Yong

    2000-01-01

    Formulae of proton and neutron boson structure functions (BSF's) are deduced in terms of a microscopic approach of sdgIBM (namely, microscopic sdgIBM). For the nucleus 190Os, the value of BSF's is worked out. Due to the high similarity, the maximum F-spin truncation is made under the full-symmetry approximation. Thereafter, calculations of E2 and E4 transition charge densities (TCD's) are performed in the sdgIBM-1. It is found that the E2 and E4 TCD's can be reproduced quite satisfactorily in the uniform frame of microscopic sdgIBM-1.

  4. Electric moments and charge deformation parameters in /sup 152/ /sup 154/Sm, /sup 156/Gd, and /sup 166/Er

    Energy Technology Data Exchange (ETDEWEB)

    Fischer, H.; Kamke, D.; Kittling, H.J.; Kuhlmann, E.; Plicht, H.; Schormann, R.

    1977-03-01

    Coulomb excitation experiments with ..cap alpha.. particles were performed on the four rare-earth nuclei /sup 152/ /sup 154/Sm, /sup 156/Gd, and /sup 166/Er. E2 and E4 transition matrix elements of low-lying levels in the rotational ground-state bands were obtained. Model dependent charge deformation parameters ..beta../sup c//sub 2/ and ..beta../sup c//sub 4/ were extracted by assuming a deformed Fermi distribution with diffuse surface. The possible difference between charge and nuclear hexadecapole deformation observed in /sup 154/Sm does not show up in the isotone /sup 156/Gd.

  5. Double K-shell-vacancy production in the decay of 114mIn

    Science.gov (United States)

    van Eijk, C. W. E.; Wijnhorst, J.; Popelier, M. A.

    1981-08-01

    The probability PKK of double K-shell-vacancy production per K-shell internal conversion of the 192-keV E4 transition in the decay of 114mIn has been determined by means of a hypersatellite KαH-x-ray-K-x-ray coincidence experiment using an intrinsic Ge and a NaI(Tl) detector, and by means of a direct measurement of the KαH1- and KαH2-x-ray components with a curved-crystal spectrometer. The results are in good agreement: PKK=(10.8+/-0.9)×10-5 and PKK=(9.6+/-0.8)×10-5, respectively. The average value is PKK=(10.2+/-0.6)×10-5. For the intensity ratio of the KαH1- and KαH2-x-ray components we obtained 1.57+/-0.17, and for the energy shifts of the two components we obtained, respectively, 566.8+/-1.4 and 560.2+/-1.3 eV.