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RESEARCH PRODUCT
Observation of mass-asymmetric fission of mercury nuclei in heavy ion fusion
Elizabeth WilliamsAditya WakhleD. C. RaffertyK. RamachandranBettina LommelCedric SimenelS. D. McneilIan CarterBirgit KindlerD. Y. JeungE.v. PrasadC. S. PalshetkarKaitlin CookDuc Huy LuongMahananda DasguptaCh. E. DüllmannJadambaa KhuyagbaatarDavid Hindesubject
PhysicsNuclear and High Energy Physicseducation.field_of_studyIsotopeSpectrometerFissionNuclear TheoryPopulationMass ratioSaddle pointNeutronAtomic physicsNuclear ExperimenteducationExcitationdescription
Background: Mass-asymmetric fission has been observed in low energy fission of $^{180}\mathrm{Hg}$. Calculations predicted the persistence of asymmetric fission in this region even at excitation energies of 30--40 MeV.Purpose: To investigate fission mass distributions by populating different isotopes of Hg using heavy ion fusion reactions.Methods: Fission fragment mass-angle distributions have been measured for two reactions, $^{40}\mathrm{Ca}+^{142}\mathrm{Nd}$ and $^{13}\mathrm{C}+^{182}\mathrm{W}$, populating $^{182}\mathrm{Hg}$ and $^{195}\mathrm{Hg}$, respectively, using the Heavy Ion Accelerator Facility and CUBE spectrometer at the Australian National University. Measurements were made at beam energies around the capture barrier for the two reactions and mass ratio distributions were obtained using the kinematic reconstruction method.Results: Asymmetric fission has been observed following the population of $^{182}\mathrm{Hg}$ at an excitation energy of 22.8 MeV above the saddle point. A symmetric peaked mass ratio distribution was observed for $^{195}\mathrm{Hg}$ nuclei at a similar excitation energy above the saddle point.Conclusions: Mass-asymmetric fission has been observed in neutron deficient Hg nuclei populated via heavy ion fusion for the first time. The results are consistent with observations from beta-delayed fission measurements and provide a proof-of-principle for expanding experimental studies of the influence of shell effects on the fission processes.
year | journal | country | edition | language |
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2015-06-08 | Physical Review C |