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Fusion probability for neutron-rich radioactive-Sn-induced reactions

J. F. Liang (梁君健), C. J. Gross, Z. Kohley, D. Shapira, R. L. Varner, J. M. Allmond, A. L. Caraley, K. Lagergren, and P. E. Mueller
Phys. Rev. C 85, 031601(R) – Published 2 March 2012

Abstract

Evaporation residue cross sections for 124,126,127,128Sn+64Ni and 132Sn+58Ni have been measured to study the effects of neutron excess in neutron-rich radioactive nuclei on the fusion probability. A comparison of the reduced evaporation residue cross sections for 126Sn+64Ni and 132Sn+58Ni, which make the same compound nucleus, shows that the fusion probability is indistinguishable for reactions involving the same atomic elements, Sn and Ni, but different isotope combinations. For the reactions with 64Ni, the fusion probability does not decrease with increasing neutron excess in Sn, contrary to the result of the stable beam Sn+Zr measurement.

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  • Received 29 September 2011

DOI:https://doi.org/10.1103/PhysRevC.85.031601

©2012 American Physical Society

Authors & Affiliations

J. F. Liang (梁君健)1, C. J. Gross1, Z. Kohley1, D. Shapira1, R. L. Varner1, J. M. Allmond1, A. L. Caraley2, K. Lagergren3, and P. E. Mueller1

  • 1Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 2Department of Physics, State University of New York at Oswego, Oswego, New York 13126, USA
  • 3Joint Institute for Heavy Ion Research, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA

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Vol. 85, Iss. 3 — March 2012

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