Science China Physics, Mechanics and Astronomy

, Volume 54, Supplement 1, pp 61–66

Predictions of synthesizing element 119 and 120

Authors

  • ZaiGuo Gan
    • Institute of Modern PhysicsChinese Academy of Sciences
  • XiaoHong Zhou
    • Institute of Modern PhysicsChinese Academy of Sciences
  • MingHui Huang
    • Institute of Modern PhysicsChinese Academy of Sciences
  • ZhaoQing Feng
    • Institute of Modern PhysicsChinese Academy of Sciences
    • Institute of Modern PhysicsChinese Academy of Sciences
    • School of Nuclear Science and TechnologyLanzhou University
Research Paper Radioactive Nuclear Beam Physics and Nuclear Astrophysics

DOI: 10.1007/s11433-011-4436-4

Cite this article as:
Gan, Z., Zhou, X., Huang, M. et al. Sci. China Phys. Mech. Astron. (2011) 54: 61. doi:10.1007/s11433-011-4436-4

Abstract

The evaporation residue cross sections of synthesizing superheavy nuclei Z=119, 120 are calculated by different sets of master equations with different dynamical variables. Two methods basically predicted similar results that the 48Ca induced hot fusion can produce element 119 easier than produce 120, and the evaporation residue cross sections for 119 are detectable by current advanced techniques, while the evaporation residue cross sections are below 0.1 pb for producing element 120.

Keywords

super heavy nucleievaporation residue cross sectionmaster equations

Copyright information

© Science China Press and Springer-Verlag Berlin Heidelberg 2011