Synthesis of new neutron-rich heavy nuclei: An experimentalist's view

I attempt to experimentally evaluate the prospects of synthesizing new neutron- rich superheavy nuclei. I consider three possible synthetic paths to neutron- rich superheavy nuclei: (a) the use of neutron-rich radioactive beams. (b) the use of damped collisions and (c) the use of multi-nucleon transfer reactions. I consider the prospects of synthesizing new n-rich isotopes of Rf-Bh using light n-rich radioactive beams and targeted beams from ReA3, FRIB and SPIRAL2. For the damped collision path, I present the results of a study of a surrogate reaction, 160Gd + 186W. These data indicate the formation of Au (trans-target) fragments and the depletion of yields of target-like fragments by fission and fragment emission. The data are compared to predictions of Zagrebaev and Greiner. For the multi-nucleon transfer reactions, the results of a study of the 136Xe + 208Pb reaction are discussed. I consider the possibility of multi-nucleon transfer reactions with radioactive beams

An experimentalist's view of the uncertainties in understanding heavy element synthesis

The overall uncertainties in predicting heavy element synthesis cross sections are examined in terms of the uncertainties associated with the calculations of capture cross sections, fusion probabilities and survival probabilities. Attention is focussed on hot fusion reactions. The predicted heavy element formation cross sections are uncertain to at least one order of magnitude

Going Some : March Two Step

https://digitalcommons.library.umaine.edu/mmb-ps/1797/thumbnail.jp

The Red Ribbon : Waltzes

https://digitalcommons.library.umaine.edu/mmb-ps/2531/thumbnail.jp

Ferns and Flowers : Waltzes

https://digitalcommons.library.umaine.edu/mmb-ps/2514/thumbnail.jp

Relativistic effects for the reaction Ubq + 6 CO = Ubq (CO)6 or Ubq (OC)6:Prediction of the existence, atomization energy, and isomerization energy of the isomers Ubq (CO)6 and Ubq (OC)6 of element Ubq ( Z=124, eka-uranium)

Our ab initio all-electron relativistic Dirac*Fock (DF) calculations for the octahedral (Oh) Ubq(CO)6 and Ubq(OC)6 predict atomization energies (Ae) of 50.25 (47.93) and 43.43 (44.88 ) eV, respectively where the corresponding non-relativistic calculated Ae's are given in parenthesis. Our calculated DF and NR isomerization energies (E iso) for Ubq (CO) 6 = Ubq (OC) 6 are 6.83 and 3.05 eV, respectively. Our calculated DF (NR) energy for the reaction Ubq + 6CO = Ubq (CO)6 is -4.31 (-4.30) eV, while the energy of the isomeric reaction Ubq + 6CO = Ubq(OC)6 is 2.52 ( -1.25 ) eV, respectively. The relativistic effects increase the Eiso of Ubq (CO)6 by ~3.78 eV , decrease the Ubq-C bond distance by 0.12 angstroms and have a negligible effect on the C-O bond distance as expected. These are the first results of relativistic effects for isomerztion energy and atomization energy of the superheavy Ubq (CO)6 and Ubq(OC)6. The bond distances Ubq-C and Ubq-O optimized at the DF level of theory for Ubq(CO)6 and Ubq(OC)6 are 2.572 and 2.559 angstroms, while the corresponding optimized bond distances Ubq-C and Ubq-O at the NR level of theory are 2.691 and 3.616 angstroms, respectively. Both our DF and NR calculations clearly predict the formation of both the isomers Ubq(CO)6 and Ubq(OC), and the former is predicted to be more stable at the DF level of theory by ~7 eV than the latter.No such calculations have been reported before for systems of such superheavy elements.Comment: The present calculations do not include electron correlation effects which are very significant but their accurate calculation would require an order of magnitude computational expense as compared to the present relativistic calculation

Heavy Residue Formation in 20 MeV/nucleon 197Au + 90Zr collisions

The yields and velocity distributions of heavy residues and fission fragments from the reaction of 20 MeV/nucleon 197Au + 90Zr have been measured using the MSU A1200 fragment separator. A bimodal distribution of residues is observed, with one group, resulting from peripheral collisions, having fragment mass numbers A=160-200, while the other group, resulting from ``hard'' collisions, has A=120-160. This latter group of residues can be distinguished from fission fragments by their lower velocities. A model combining deep-inelastic transfer and incomplete fusion for the primary interaction stage and a statistical evaporation code for the deexcitation stage has been used to describe the properties of the product distributions.Comment: 19 pages, 6 figures, preprint submitted to Nucl. Phys.