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

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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