The synthesis of ultramagnetized heavy atomic nuclei during type II supernova explosions and neutron star mergers is considered. For a magnetic field of 0.1–10 ТТ the Zeeman effect leads to a linear nuclear magnetic response, which can be described in terms of magnetic susceptibility. Under the influence of magnetic fields, the path of the r-process changes with an increase in the proportion of nuclei with masses less than magic, as well as an enhancement of the volume of nuclides of smaller masses at the r-process peaks.
V. N. Kondratyev (Wed,) studied this question.
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