Analysis of the fusion mechanism in the synthesis of superheavy element 119 via the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Cr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>54</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mspace width="4pt"/><mml:mmultiscripts><mml:mi>Am</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>243</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math> reaction
Bakhodir KayumovInstitute of Nuclear Physics, Uzbekistan Academy of Sciences, 100214 Tashkent, UzbekistanO.K. GanievFaculty of Physics, National University of Uzbekistan, 100174 Tashkent, UzbekistanA. K. NasirovJoint Institute for Nuclear Research, 141980 Dubna, RussiaG. A. YuldashevaInstitute of Nuclear Physics, Uzbekistan Academy of Sciences, 100214 Tashkent, Uzbekistan
ABI
Annotatsiya
The combined dinuclear system (DNS) model and statistical model incorporated in kewpie2 have been used to study the prospects for the synthesis of a superheavy element (SHE) with $Z=119$ in the $^{54}\mathrm{Cr}+^{243}\mathrm{Am}$ fusion reaction. The method of calculation has been verified by description of the evaporation residue cross sections measured for the $^{48}\mathrm{Ca}+^{243}\mathrm{Am}$ reaction. The calculated results of the partial and total cross sections for the complete fusion, quasifission, fast fission, and evaporation residues formation for both reactions are discussed.
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