Expected production of new exotic<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>α</mml:mi></mml:math>emitters<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Xe</mml:mi><mml:mprescripts/><mml:none/><mml:mn>108</mml:mn></mml:mmultiscripts></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Ba</mml:mi><mml:mprescripts/><mml:none/><mml:mn>112</mml:mn></mml:mmultiscripts></mml:math>in complete fusion reactions
Sh. A. KalandarovInstitute of Nuclear Physics, 702132 Tashkent, UzbekistanG. G. AdamianJoint Institute for Nuclear Research, 141980 Dubna, RussiaN. V. AntonenkoJoint Institute for Nuclear Research, 141980 Dubna, RussiaJ. P. WieleczkoGANIL, CEA et IN2P3-CNRS, B.P. 55027, F-14076, Caen Cedex, France
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The production cross sections of neutron-deficient isotopes $^{108--110}\mathrm{Xe}$ and $^{112--114}\mathrm{Ba}$ in the complete fusion reactions $^{58,56}\mathrm{Ni}+^{54}\mathrm{Fe}$ and $^{58,56}\mathrm{Ni}+^{58}\mathrm{Ni}$ with stable and radioactive beams are studied with the dinuclear system model. The calculated results are compared with the available experimental data. The optimal beam energies and corresponding maximum production cross sections of new isotopes $^{108}\mathrm{Xe}$ and $^{112}\mathrm{Ba}$ are predicted.
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