First candidates for γ vibrational bands built on the [505]11/2− neutron orbital in odd-A Dy isotopes

Majola, S. N. T.; Sithole, M. A.; Mdletshe, L.; Hartley, D.; Timár, J.; Nyakó, B. M.; Allmond, J. M.; Bark, R. A.; Beausang, C.; Bianco, L.; Bucher, T. D.; Bvumbi, S. P.; Carpenter, M. P.; Chiara, C. J.; Cooper, N.; Cullen, D. M.; Curien, D.; Dinoko, T. S.; Gall, B. J. P.; Garrett, P. E.; Greenlees, P. T.; Hirvonen, J.; Jakobsson, U.; Jones, P. M.; Julin, R.; Juutinen, S.; Ketelhut, S.; Kheswa, B. V.; Kondev, F. G.; Korichi, A.; Kulp, W. D.; Lauritsen, T.; Lawrie, E. A.; Makhathini, L.; Masiteng, P. L.; Maqabuka, B.; McCutchan, E. A.; Miller, D.; Miller, S.; Minkova, A.; Msebi, L.; Mthembu, S. H.; Ndayishimye, J.; Nieminen, P.; Ngcobo, P. Z.; Ntshangase, S. S.; Orce, J. N.; Peura, P.; Rahkila, P.; Redon, N.; Riedinger, L. L.; Riley, M. A.; Roux, D. G.; Ruotsalainen, P.; Piot, J.; Saren, J.; Sharpey-Schafer, J. F.; Scholey, C.; Shirinda, O.; Simpson, J.; Sorri, J.; Stefanescu, I.; Stolze, S.; Uusitalo, J.; Wang, X.; Werner, V.; Wood, J. L.; Yu, C.-H.; Zhu, S.; Zimba, G.

doi:10.1103/PhysRevC.101.044312

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Katso/Avaa

816.5 Kb

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Majola, S. N. T., Sithole, M. A., Mdletshe, L., Hartley, D., Timár, J., Nyakó, B. M., Allmond, J. M., Bark, R. A., Beausang, C., Bianco, L., Bucher, T. D., Bvumbi, S. P., Carpenter, M. P., Chiara, C. J., Cooper, N., Cullen, D. M., Curien, D., Dinoko, T. S., Gall, B. J. P., . . . Zimba, G. (2020). First candidates for γ vibrational bands built on the [505]11/2− neutron orbital in odd-A Dy isotopes. Physical Review C, 101(4), Article 044312. https://doi.org/10.1103/PhysRevC.101.044312

Julkaistu sarjassa

Physical Review C

Tekijät

Majola, S. N. T. |

Sithole, M. A. |

Mdletshe, L. |

Hartley, D. |

Timár, J. |

Nyakó, B. M. |

Allmond, J. M. |

Bark, R. A. |

Beausang, C. |

Bianco, L. |

Bucher, T. D. |

Bvumbi, S. P. |

Carpenter, M. P. |

Chiara, C. J. |

Cooper, N. |

Cullen, D. M. |

Curien, D. |

Dinoko, T. S. |

Gall, B. J. P. |

Garrett, P. E. |

Greenlees, P. T. |

Hirvonen, J. |

Jakobsson, U. |

Jones, P. M. |

Julin, R. |

Juutinen, S. |

Ketelhut, S. |

Kheswa, B. V. |

Kondev, F. G. |

Korichi, A. |

Kulp, W. D. |

Lauritsen, T. |

Lawrie, E. A. |

Makhathini, L. |

Masiteng, P. L. |

Maqabuka, B. |

McCutchan, E. A. |

Miller, D. |

Miller, S. |

Minkova, A. |

Msebi, L. |

Mthembu, S. H. |

Ndayishimye, J. |

Nieminen, P. |

Ngcobo, P. Z. |

Ntshangase, S. S. |

Orce, J. N. |

Peura, P. |

Rahkila, P. |

Redon, N. |

Riedinger, L. L. |

Riley, M. A. |

Roux, D. G. |

Ruotsalainen, P. |

Piot, J. |

Saren, J. |

Sharpey-Schafer, J. F. |

Scholey, C. |

Shirinda, O. |

Simpson, J. |

Sorri, J. |

Stefanescu, I. |

Stolze, S. |

Uusitalo, J. |

Wang, X. |

Werner, V. |

Wood, J. L. |

Yu, C.-H. |

Zhu, S. |

Zimba, G.

Päivämäärä

2020

Oppiaine

Kiihdytinlaboratorio Accelerator Laboratory

Tekijänoikeudet

Rotational structures have been measured using the Jurogam II and GAMMASPHERE arrays at low spin following the 155Gd(α,2n)157Dy and 148Nd(12C,5n)155Dy reactions at 25 and 65 MeV, respectively. We report high-K bands, which are conjectured to be the first candidates of a Kπ=2+γ vibrational band, built on the [505]11/2− neutron orbital, in both odd-A155,157Dy isotopes. The coupling of the first excited K=0+ states or the so-called β vibrational bands at 661 and 676 keV in 154Dy and 156Dy to the [505]11/2− orbital, to produce a Kπ=11/2− band, was not observed in both 155Dy and 157Dy, respectively. The implication of these findings on the interpretation of the first excited 0+ states in the core nuclei 154Dy and 156Dy are also discussed.

Julkaisija

American Physical Society

ISSN Hae Julkaisufoorumista

2469-9985

Lisätietoja rahoituksesta

This work is supported by the South African National Research Foundation under Grants No. 96829, No. 109711, and No. 106012). Support for L.B. and P.E.G. was provided by the Natural Sciences and Engineering Research Council of Canada. V.W. wishes to acknowledge support provided by the German Federal Ministry for education and Research under Grant No. 05P19RDFN1. Support was also provided by the U ... showmore

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