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The production cross sections of heaviest isotopes of superheavy nuclei withcharge numbers 112--118 are predicted in the $xn$--, $pxn$--, and $\alphaxn$--evaporation channels of the $^{48}$Ca-induced complete fusion reactionsfor future experiments. The estimates of synthesis capabilities are based on auniform and consistent set of input nuclear data. Nuclear masses, deformations,shell corrections, fission barriers, and decay energies are calculated withinthe macroscopic-microscopic approach for even-even, odd-Z, and odd-N nuclei.For odd systems, the blocking procedure is used. To find, the ground states viaminimization and saddle points using Immersion Water flow technique,multidimensional deformation spaces, containing non-axially are used. As shown,current calculations based on a new set of mass and barriers, agree very wellwith experimentally known cross-sections, especially in the $3n$--evaporationchannel. The dependencies of these predictions on the mass/fission barrierstables and fusion models are discussed. A way is shown to produce directlyunknown superheavy isotopes in the $1n$-- or $2n$--evaporation channels. Thesynthesis of new superheavy isotopes unattainable in reactions with emission ofneutrons is proposed in the promising channels with emission of protons($\sigma_{pxn} \simeq 10-200$ fb) and alphas ($\sigma_{\alpha xn} \simeq 5-500$fb).

Possibilities of direct production of superheavy nuclei with Z=112--118 in different evaporation channels