\begin{document}$^{76}$\end{document}Ge,\begin{document}$^{82}$\end{document}Se+\begin{document}$^{9}$\end{document}Be) is quantitatively investigated, to further validate the OES universality and OES relations. The OES magnitudes in these experimental data approaching the neutron drip-line generally agree with those evaluated previously, mainly from experimental data near stability. New OES evaluations derived from these experimental data are also recommended for more exotic nuclei near the neutron drip-line, which extends the conclusions of our previous OES studies. In addition, the OES relation calculations are consistent with these experimental data of very neutron-rich nuclides according to their comparisons in this work. Finally, comparisons with additional experimental data (from \begin{document}$^{238}$\end{document}U+\begin{document}$^{9}$\end{document}Be) also support that new OES evaluations and OES relation calculations can be applied for exotic nuclei near the neutron drip-line."> Odd-even staggering for production cross sections ofnuclei near the neutron drip-line -
  • [1]

    O. B. Tarasovet al., Phys. Rev. Lett.102, 142501 (2009)

  • [2]

    O. B. Tarasovet al., Phys. Rev. C80, 034609 (2009)

  • [3]

    O. B. Tarasovet al., Phys. Rev. C87, 054612 (2013)

  • [4]

    O. B. Tarasovet al., Phys. Rev. Lett.121, 022501 (2018)

  • [5]

    J. J. Cowanet al., Rev. Mod. Phys.93, 015002 (2021)

  • [6]

    M. Mockoet al., Phys. Rev. C74, 054612 (2006)

  • [7]

    C. Villagrasa-Cantonet al., Phys. Rev. C75, 044603 (2007)

  • [8]

    P. Napolitaniet al., Phys. Rev. C76, 064609 (2007)

  • [9]

    D. Henzlovaet al., Phys. Rev. C78, 044616 (2008)

  • [10]

    V. Föhret al., Phys. Rev. C84, 054605 (2011)

  • [11]

    J. Alcántara-Núñezet al., Phys. Rev. C92, 024607 (2015)

  • [12]

    H. Suzukiet al., Nucl. Instrum. Methods B317, 756 (2013)

  • [13]

    D. S. Ahnet al., Phys. Rev. Lett.123, 212501 (2019)

  • [14]

    T. Ohnishiet al., J. Phys. Soc. Jpn.77, 083201 (2008)

  • [15]

    T. Ohnishiet al., J. Phys. Soc. Jpn.79, 073201 (2010)

  • [16]

    B. Meiet al., Nucl. Instrum. Methods A624, 109 (2010)

  • [17]

    B. Meiet al., Phys. Rev. C89, 054612 (2014)

  • [18]

    B. Meiet al., Phys. Rev. C94, 044615 (2016)

  • [19]

    R. Silberberg and C. H. Tsao, Phys. Rep.191, 351 (1990)

  • [20]

    W. R. Webber, A. Soutoul, J. C. Kishet al., Astrophys. J. Suppl. Ser.144, 153 (2003)

  • [21]

    D. Schardt, T. Elsässer, and D. Schulz-Ertner, Rev. Mod. Phys.82, 383 (2010)

  • [22]

    C. D. Bowmanet al., Nucl. Instrum. Methods B320, 336 (1992)

  • [23]

    M. V. Ricciardi, A. V. Ignatyuk, A. Kelićet al., Nucl. Phys. A733, 299 (2004)

  • [24]

    B. Mei, X. L. Tu, and M. Wang, Phys. Rev. C97, 044619 (2018)

  • [25]

    B. Mei, Phys. Rev. C100, 054619 (2019)

  • [26]

    J. J. Gaimard and K. H. Schmidt, Nucl. Phys. A531, 709 (1991)

  • [27]

    K. Sümmerer, Phys. Rev. C86, 014601 (2012)

  • [28]

    B. Mei, Phys. Rev. C95, 034608 (2017)

  • [29]

    B. Mei, Phys. Rev. C103, 044610 (2021)

  • [30]

    A. Olmi and S. Piantelli, Eur. Phys. J. A51, 154 (2015)

  • [31]

    T. Sumikamaet al., Phys. Rev. C95, 051601(R) (2017)

Baidu
map