Possibilities of direct production of superheavy nuclei with Z=112--118 in different evaporation channels
J. Hong, G. G. Adamian, N. V. Antonenko, P. Jachimowicz, M. Kowal

TL;DR
This paper predicts the production cross sections of superheavy nuclei with Z=112--118 in various evaporation channels using a comprehensive nuclear data approach, aiding future experimental synthesis of new isotopes.
Contribution
It introduces a unified method to estimate superheavy nuclei production in different channels, incorporating detailed nuclear data and advanced modeling techniques.
Findings
Predicted cross sections align well with existing experimental data.
Proposed new channels for synthesizing superheavy isotopes with proton and alpha emission.
Identified promising reactions with measurable cross sections for future experiments.
Abstract
The production cross sections of heaviest isotopes of superheavy nuclei with charge numbers 112--118 are predicted in the --, --, and --evaporation channels of the Ca-induced complete fusion reactions for future experiments. The estimates of synthesis capabilities are based on a uniform and consistent set of input nuclear data. Nuclear masses, deformations, shell corrections, fission barriers, and decay energies are calculated within the 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 via minimization 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 well with experimentally known cross-sections,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNuclear physics research studies · Astronomical and nuclear sciences · Nuclear Physics and Applications
