\begin{document}$82\leqslant Z\leqslant 92$\end{document}. The NST case and HF formalism based on the Skyrme-SLy4 effective interaction reveal different isospin asymmetries for selected alpha emitters. Furthermore, the obtained results reveal an increase in the α-decay widths of about 30% for the NST case in comparison with the equivalent values obtained by HF formalism. The standard deviations for calculated half-lives within the NST case and HF formalism are about 0.438 and 0.391, respectively."> Determination of isospin asymmetry effects on <i>α</i>-decay -
  • [1]

    G. Z. Gamow, Phys.,51: 204 (1928)

  • [2]

    R. W. Gurney and E. U. Condon, Nature,122: 439 (1928)

  • [3]

    K. Varga, R. Lovas, and R. Liotta, Phys. Rev. Lett.,69: 37 (1992)

  • [4]

    B. A. Brown, Phys. Rev. C,46: 811 (1992)

  • [5]

    B. Buck et al, At. Data Nucl. Data Tables,54: 53 (1993)

  • [6]

    C. Xu and Z. Ren, Phys. Rev. C,74: 014304 (2006)

  • [7]

    G. Royer and H. F. Zhang, Phys. Rev. C,77: 037602 (2008)

  • [8]

    H. F. Zhang, Y. Gao, N. Wang et al, Phys. Rev. C,85: 14325 (2012)

  • [9]

    Y. Ren and Z.Ren, Phys. Rev. C,85: 044608 (2012)

  • [10]

    Y. Qian and Z. Ren, Phys. lett. B,738: 87 (2014)

  • [11]

    M. Ismail and A. Adel, J. Phys. G: Nucl. Phys.,44: 125106 (2017)

  • [12]

    D. Ni and Z. Ren, Phys. Rev. C,80: 014314 (2009)

  • [13]

    D. Ni and Z. Ren, Nucl. Phys. A,825: 145 (2009)

  • [14]

    E. Shin, Y. Lim, C. H. Hyun et al, Phys. Rev. C,94: 024320 (2016)

  • [15]

    Y. Qian and Z. Ren, J. Phys. G: Nucl. Phys.,43: 065102 (2016)

  • [16]

    D. T. Akrawy, H. Hassanabadi, S. S. Hosseini et al, Nucl. Phys. A,975: 19 (2018)

  • [17]

    W. M. Seif and A. Abdurrahman, Chinese Phys. C,42: 014106 (2018)

  • [18]

    D. Ni and Z. Ren, Phys. Rev. C,92: 054322 (2015)

  • [19]

    S. Typel, Phys. Rev. C,89: 064321 (2014)

  • [20]

    G. R. Satchler and W. G. Love, Phys. Rep.,55: 183 (1979)

  • [21]

    D. Ni and Z. Ren, Phys. Rev. C,93: 054318 (2016)

  • [22]

    W. M. Seif, M. Shalaby, and M. F. Alrakshy, Phys. Rev. C,84: 064608 (2011)

  • [23]

    M. Ismail and A. Adel, Phys. Rev. C,86: 014616 (2012)

  • [24]

    J. C. Pei, F. R. Xu, Z. J. Lin et al, Phys. Rev. C,76: 044326 (2007)

  • [25]

    C. Xu and Z. Z. Ren, Nucl. Phys. A,753: 174 (2005)

  • [26]

    M. Ismail, A. Y. Ellithi, M. M. Botros et al, Phys. Rev. C,81: 024602 (2010)

  • [27]

    Y. Qian and Z. Ren, Phys. lett. B,777: 298 (2018)

  • [28]

    D. T. Khoa, G. R. Satchler, and W. von Oertzen, Phys. Rev. C,56: 954 (1997)

  • [29]

    D. N. Basu et al, J. Phys. G: Nucl. Part. Phys.,29: 2079-2085 (2003)

  • [30]

    B. Buck, A. C. Merchant, and S. M. Perez, Phys. Rev. C,45: 2247 (1992)

  • [31]

    K. Wildermuth and Y. C. Tang, A Unified Theory of the Nucleus(Academic Press, New York, 1977)

  • [32]

    S. A. Gurvitz and G. \begin{document}${\small{\rm{\ddot K}}}$\end{document} albermann, Phys. Rev. Lett.,59: 262 (1987)

  • [33]

    D. Ni, Z. Ren, T. Dong, and Y. Qian, Phys. Rev. C,87: 024310 (2013)

  • [34]

    P. Möller, A. J. Sierk, T. Ichikawa et al, At. Data Nucl. Data Tables,109-110: 1 (2016)

  • [35]

    D. E. Ward, B. G. Carlsson, and S.Åberg, Phys. Rev. C,88: 064316 (2013)

  • [36]

    W. M. Seif, Phys. Rev. C,91: 014322 (2015)

  • [37]

    S. Goriely, M. Samyn, M. Bender et al, Phys. Rev. C,68: 054325 (2003)

  • [38]

    A. Trzcińska, J. Jastrzȩbski, P. Lubiński et al, Phys. Rev. Lett.,87: 082501 (2001)

  • [39]

    I. Angeli, At. Data Nucl. Data Tables,87: 185 (2004)

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