\begin{document}$ g_{9/2} $\end{document} and neutron orbit \begin{document}$ g_{7/2} $\end{document} are studied as the new monopole correction that perfectly reproduces the first 1+ level in 130In. The energy interval of proton (neutron) core excitations in 130In lies in the range of 4.5−6.5 (2.0−4.1) MeV, and the high energy yrast states are predicted as neutron core excitations. The \begin{document}$ \beta $\end{document} decays are calculated among the A=130 nuclei of 130In, 130Sn and 130Cd."> Monopole effects, core excitations, and <inline-formula><tex-math id="M14">\begin{document}${\beta}$\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/fe3794ee-36ac-484c-9616-b39409892ad4/CPC-2018-0447_M14.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/fe3794ee-36ac-484c-9616-b39409892ad4/CPC-2018-0447_M14.png"/></alternatives></inline-formula> decay in the <i>A </i>= 130 hole nuclei near <sup>132</sup>Sn -
  • [1]

    K. L. Kratz, H. Gabelmann, W. Hillebrandt et al, Z. Phys. A,325: 489 (1986)

  • [2]

    A. Jungclaus, H. Grawe, S. Nishimura et al, Phys. Rev. C,94: 024303 (2016)

  • [3]

    I. Dillmann, K. L. Kratz, A. Wohr et al, Phys. Rev. Lett.,91: 162503 (2003)

  • [4]

    G. Martínez-Pinedo and K. Langanke, Phys. Rev. Lett.,83: 4502 (1999)

  • [5]

    J. J. Cuenca-García, G. Martínez-Pinedo, K. Langanke et al, Eur. Phys. J. A,34: 99 (2007)

  • [6]

    T. Otsuka, T. Suzuki, R. Fujimoto et al, Phys. Rev. Lett.,95: 232502 (2005)

  • [7]

    H. K. Wang, Y. Sun, Hua Jin et al, Phys. Rev. C,88: 054310 (2013)

  • [8]

    M. Górska, L. Cáceres, H. Grawe et al, Phys. Lett. B,672: 313 (2009)

  • [9]

    F. Minato and C. L. Bai, Phys. Rev. Lett.,110: 122501 (2013)

  • [10]

    Y. F. Niu, Z. M. Niu, G. Colò et al, Phys. Rev. Lett.,114: 142501 (2015)

  • [11]

    Y. F. Niu, Z. M. Niu, G. Colò et al, Phys. Lett. B,780: 325 (2018)

  • [12]

    P. Bhattacharyya, P. J. Daly, C. T. Zhang et al, Phys. Rev. Lett.,87: 062502 (2001)

  • [13]

    K. L. Jones, A. S. Adekola, D. W. Bardayan et al, Nature (London),465: 454 (2010)

  • [14]

    K. L. Jones, F. M. Nunes, A. S. Adekola et al, Phys. Rev. C,84: 034601 (2011)

  • [15]

    H. Watanabe, G. Lorusso, S. Nishimura et al, Phys. Rev. Lett.,111: 152501 (2013)

  • [16]

    H. K. Wang, K. Kaneko, and Y. Sun, Phys. Rev. C,89: 064311 (2014)

  • [17]

    M. Hasegawa, K. Kaneko, and S. Tazaki, Nucl. Phys. A,688: 765 (2001)

  • [18]

    K. Kaneko, M. Hasegawa, and T. Mizusaki, Phys. Rev. C,66: 051306(R) (2002)

  • [19]

    K. Kaneko, Y. Sun, M. Hasegawa et al, Phys. Rev. C,78: 064312 (2008)

  • [20]

    K. Kaneko, Y. Sun, T. Mizusaki et al, Phys. Rev. C,83: 014320 (2011)

  • [21]

    Han-Kui Wang, Kazunari Kaneko, Yang Sun et al, Phys. Rev. C,91: 021303(R) (2015)

  • [22]

    H. K. Wang, K. Kaneko, Y. Sun et al, Phys. Rev. C,95: 011304(R) (2017)

  • [23]

    B. A. Brown and W. D. M. Rae, Nucl. Data Sheets,120: 115 (2014)

  • [24]

    H. K. Wang, S. K. Ghorui, K. Kaneko et al, Phys. Rev. C,96: 054313 (2017)

  • [25]

    Q. Zhi, E. Caurier, J. J. Cuenca-García et al, Phys. Rev. C,87: 025803 (2013)

  • [26]

    Z. M. Niu, Y. F. Niu, H. Z. Liang et al, Phys. Lett. B,723: 172 (2013)

  • [27]

    P. Möller, M. R. Mumpower, T. Kawano et al, Atomic Data and Nuclear Data Tables 125(2019)1-92

Baidu
map