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

Evaporation residue cross sections for $^{124,126,127,128}$Sn+$^{64}$Ni and $^{132}$Sn+$^{58}$Ni have been measured to study the effects of neutron excess in neutron-rich radioactive nuclei on fusion. For the reactions with $^{64}$Ni, the fusion probability does not decrease with increasing neutron...

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Bibliographic Details
Published in:Physical review. C, Nuclear physics Vol. 85; no. 3
Main Authors: Liang, J. F., Gross, C. J., Kohley, Z., Shapira, D., Varner, R. L., Allmond, J. M., Caraley, A. L., Lagergren, K., Mueller, P. E.
Format: Journal Article
Language:English
Published: United States 02-03-2012
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Summary:Evaporation residue cross sections for $^{124,126,127,128}$Sn+$^{64}$Ni and $^{132}$Sn+$^{58}$Ni have been measured to study the effects of neutron excess in neutron-rich radioactive nuclei on fusion. For the reactions with $^{64}$Ni, the fusion probability does not decrease with increasing neutron excess in Sn, contrary to the result of the stable beam Sn+Zr measurement. A comparison of the reduced evaporation residue cross sections for $^{126}$Sn+$^{64}$Ni and $^{132}$Sn+$^{58}$Ni, which make the same compound nucleus, shows that the fusion probability is indistinguishable for reactions involving the same atomic elements but different isotope combinations.
Bibliography:DE-AC05-00OR22725
USDOE Office of Science (SC)
ISSN:0556-2813
1089-490X
DOI:10.1103/PhysRevC.85.031601