Effects of the entrance channel and fission barrier in synthesis of superheavy element $Z$=120
A. K. Nasirov (1,2), G. Mandaglio (3), G. Giardina (3), A. Sobiczewski, (4), A. I. Muminov (2) ((1) Joint Institute for Nuclear Research, Dubna,, Russia, (2) Institute of Nuclear Physics, Tashkent, Uzbekistan, (3), Dipartimento di Fisica dell' Universit\`a di Messina

TL;DR
This study compares fusion and evaporation residue cross sections for two reactions aimed at synthesizing superheavy element Z=120, highlighting the influence of entrance channel properties and nuclear mass models on production probabilities.
Contribution
It provides a comparative analysis of two reaction pathways for superheavy element synthesis using combined models and different nuclear mass calculations, identifying the more favorable reaction.
Findings
$^{50}$Ti+$^{249}$Cf has higher fusion excitation function than $^{54}$Cr+$^{248}$Cm.
Evaporation residue cross sections are larger for the more asymmetric $^{50}$Ti+$^{249}$Cf reaction.
Using different nuclear mass models significantly affects the predicted cross sections.
Abstract
The fusion and evaporation residue cross sections for the Ti+Cf and Cr+Cm reactions calculated by the combined dinuclear system and advanced statistical models are compared. These reactions are considered to be used to synthesize the heaviest superheavy element. The Ti+Cf reaction is more mass asymmetric than Cr+Cm and the fusion excitation function for the former reaction is higher than the one for the latter reaction. The evaporation residue excitation functions for the mass asymmetric reaction is higher in comparison with the one of the Cr+Cm reaction. The use of the mass values of superheavy nuclei calculated in the framework of the macroscopic-microscopic model by the Warsaw group leads to smaller evaporation residue cross section for both the reactions in comparison with the case of using the masses…
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