Published August 2010 | Version v1
Journal article

Nuclear orientation in the reaction 34S+238U and synthesis of the new isotope 268Hs

  • 1. Japan Atomic Energy Agency, Tokai, Ibaraki 319-1195 (Japan)
  • 2. Institut fuer Kernphysik, Goethe-Universitaet Frankfurt, D-60438 Frankfurt am Main (Germany)
  • 3. GSI Helmholtzzentrum fuer Schwerionenforschung, D-64291 Darmstadt (Germany)
  • 4. Department of Nuclear Physics and Biophysics, Comenius University, SK-84248 Bratislava (Slovakia)
  • 5. Flerov Laboratory of Nuclear Reactions, 141 980 Dubna (Russian Federation)

Description

The synthesis of isotopes of the element hassium was studied using the reaction 34S+238U→272Hs*. At a kinetic energy of 163.0 MeV in the center-of-mass system we observed one α-decay chain starting at the isotope 267Hs. The cross section was 1.8-1.5+4.2 pb. At 152.0 MeV one decay of the new isotope 268Hs was observed. It decays with a half-life of 0.38-0.17+1.8 s by 9479±16 keV α-particle emission. Spontaneous fission of the daughter nucleus 264Sg was confirmed. The measured cross section was 0.54-0.45+1.3 pb. In-beam measurements of fission-fragment mass distributions were performed to obtain information on the fusion probability at various orientations of the deformed target nucleus. The distributions changed from symmetry to asymmetry when the beam energy was changed from above-barrier to sub-barrier values, indicating orientation effects on fusion and/or quasifission. It was found that the distribution of symmetric mass fragments originates not only from fusion-fission, but has a strong component from quasifission. The result was supported by a calculation based on a dynamical description using the Langevin equation, in which the mass distributions for fusion-fission and quasifission fragments were separately determined.

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. C, Nuclear Physics
Journal Volume
82
Journal Issue
2
Journal Page Range
p. 024611-024611.9
ISSN
0556-2813
CODEN
PRVCAN

Optional Information

Notes
(c) 2010 The American Physical Society