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January 2007
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5 Reads
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2 Citations
We discuss the possibility of producing superheavy elements in the astrophysical r-process. Thus, we consider a detailed calculation of fission-barrier heights and neutron separation energies for heavy neutron-rich nuclei. The dependence of the neutron-induced fission cutoff of the r-process on the uncertainty in the nuclear models is discussed in some detail.
... The structure of neutron fission contours is, of course, similar to these spontaneous fission con tours (see W. M. Howard [7,8])" This is a major new and encourj-ging result w!;uh tells us that previous experiments did not fa'l in prcrluc >rg clernr -t: "*^th £ r ' ICO ijtic^u:'-.: firsinr. too*-: vc: .__ a -""" f. ...
January 2007
