\begin{document}$ K^\pi = 5^- $\end{document} configuration in neutron-rich Mo, Ru and Pd isotopes were systematically investigated by the configuration-constrained cranking shell model based on the Skyrme Hartree-Fock method with pairing treated by shell-model diagonalization. The calculations efficiently reproduce the experimental moments of inertia of both the ground-state and side bands. Rotational bands built on two-particle \begin{document}$ K^\pi = 5^- $\end{document} configurations have been the subject of intense study. Possible configurations were assigned to the observed \begin{document}$ 5^- $\end{document} bands in 102-106Mo, 108-112Ru and 112-114Pd. We predict the existence of the \begin{document}$ 5^- $\end{document} bands in 108,110Mo. These results provide deep insights into the structure of neutron-rich nuclei, and provide useful information for future experiments."> <inline-formula><tex-math id="M300">\begin{document}${K^\pi=5^-}$\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/b206f833-c09e-4b8a-87c2-5cfa2ad4968b/CPC-2019-0154_M300.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/b206f833-c09e-4b8a-87c2-5cfa2ad4968b/CPC-2019-0154_M300.png"/></alternatives></inline-formula> rotational bands in neutron-rich Mo, Ru, and Pd nuclei -
  • [1]

    P. Walker and G. Dracoulis., Nature,399: 35-40 (1999)

  • [2]

    G. Audi, O. Bersillon, J. Blachot et al, Nucl. Phys. A,729(1): 3-128 (2003)

  • [3]

    F. R. Xu, P. M. Walker, and R. Wyss, Phys. Rev. C,65: 021303 (2002)

  • [4]

    Y. X. Luo, S. J. Zhu, J. H. Hamilton et al, Phys. Lett. B,670(4): 307-312 (2009)

  • [5]

    Y. X. Luo, J. O. Rasmussen, J. H. Hamilton et al, Nucl. Phys. A,919: 67-98 (2013)

  • [6]

    H. Hua, C. Y. Wu, D. Cline et al, Phys. Rev. C,69: 014317 (2004)

  • [7]

    Data extracted using the NNDC On-Line Data Service

  • [8]

    P. M. Walker and F. R. Xu, Physica Scripta,91(1): 013010 (2015)

  • [9]

    C. Y. Wu, H. Hua, D. Cline et al, Phys. Rev. C,73: 034312 (2006)

  • [10]

    H. Hua, C. Y. Wu, D. Cline et al, Phys. Lett. B,562(3): 201-207 (2003)

  • [11]

    P. Moller, J. R. Nix, W. D. Myers et al, Atomic Data and Nuclear Data Tables,59(2): 185-381 (1995)

  • [12]

    G. A. Lalazissis, S. Raman, and P. Ring, Atomic Data and Nuclear Data Tables,71(1): 1-40 (1999)

  • [13]

    P. H. Regan, T. M. Menezes, C. J. Pearson et al, Phys. Rev. C,55: 2305-2313 (1997)

  • [14]

    J. A. Alcántara-Núñez, J. R. B. Oliveira, E. W. Cybulska et al, Phys. Rev. C,71: 054315 (2005)

  • [15]

    I. Deloncle, A. Bauchet, M. G. Porquet et al, The European Physical Journal A,8(2): 177-185 (2000)

  • [16]

    H. Dejbakhsh and S. Bouttchenko, Phys. Rev. C,52: 1810-1817 (1995)

  • [17]

    A. Guessous, N. Schulz, W. R. Phillips et al, Phys. Rev. Lett.,75: 2280-2283 (1995)

  • [18]

    J. A. Shannon, W. R. Phillips, J. L. Durell et al, Phys. Lett. B,336(2): 136-140 (1994)

  • [19]

    C. L. Zhang, G. H. Bhat, W. Nazarewicz et al, Phys. Rev. C,92: 034307 (2015)

  • [20]

    E. Cheifetz, R. C. Jared, S. G. Thompson et al, Phys. Rev. Lett.,25: 38-43 (1970)

  • [21]

    M. A. C. Hotchkis, J. L. Durell, J. B. Fitzgerald et al, Nucl. Phys. A,530(1): 111-134 (1991)

  • [22]

    L. M. Yang, S. J. Zhu, K. Li et al, Chinese Physics Letters,18(1): 24 (2001)

  • [23]

    R. Q. Xu, S. J. Zhu, J. H. Hamilton et al, Chinese Physics Letters,19(2): 180 (2002)

  • [24]

    J. B. Snyder, W. Reviol, D. G. Sarantites et al, Phys. Lett. B,723(1): 61-65 (2013)

  • [25]

    A. Bhat, A. Bharti, and S. K. Khosa, The European Physical Journal A,48(3): 39 (2012)

  • [26]

    R. Chaudhary, R. Devi, and S. K. Khosa, The European Physical Journal Plus,133(2): 81 (2018)

  • [27]

    W. Y. Liang, C. F. Jiao, Q. Wu et al, Phys. Rev. C,92: 064325 (2015)

  • [28]

    X. M. Fu, F. R. Xu, C. F. Jiao et al, Phys. Rev. C,89: 054301 (2014)

  • [29]

    X. M. Fu, F. R. Xu, J. C. Pei et al, Phys. Rev. C,87: 044319 (2013)

  • [30]

    W. Satu la, J. Dobaczewski, and W. Nazarewicz, Phys. Rev. Lett.,81: 3599-3602 (1998)

  • [31]

    F. R. Xu, R. Wyss, and P. M. Walker, Phys. Rev. C,60: 051301 (1999)

  • [32]

    J. Y. Zeng, T. H. Jin, and Z. J. Zhao, Phys. Rev. C,50: 1388-1397 (1994)

  • [33]

    X. Wu, Z. H. Zhang, J. Y. Zeng et al, Phys. Rev. C,83: 034323 (2011)

  • [34]

    Z. H. Zhang, X. T. He, J. Y. Zeng et al, Phys. Rev. C,85: 014324 (2012)

  • [35]

    Z. H. Zhang, Phys. Rev. C,98: 034304 (2018)

  • [36]

    X. T. He and Y. C. Li, Phys. Rev. C,98: 064314 (2018)

  • [37]

    F. R. Xu, P. M. Walker, J. A. Sheikh et al, Phys. Lett. B,435(3): 257-263 (1998)

  • [38]

    F. R. Xu, E. G. Zhao, R. Wyss et al, Phys. Rev. Lett.,92: 252501 (2004)

  • [39]

    H. L. Liu, F. R. Xu, P. M. Walker et al, Phys. Rev. C,83: 011303 (2011)

  • [40]

    J. Y. Zeng and T. S. Cheng, Nucl. Phys. A,405(1): 1-28 (1983)

  • [41]

    J. Bartel, P. Quentin, M. Brack et al, Nucl. Phys. A,386(1): 79-100 (1982)

  • [42]

    S. J. Zhu, J. H. Hamilton, A. V. Ramayya et al, Eur. Phys. J. A,25: 459-462 (2005)

  • [43]

    I. Stefanescu, A. Gelberg, J. Jolie et al, Nucl. Phys. A,789(1): 125-141 (2007)

  • [44]

    X. L. Che, S. J. Zhu, J. H. Hamilton et al, Chinese Physics Letters,21(10): 1904 (2004)

  • [45]

    Z. Jiang, S. J. Zhu, J. H. Hamilton et al, Chinese Physics Letters,20: 350-353 (2003)

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