Synthesis of super-heavy elements in the outer crust of a magnetar
arxiv(2024)
摘要
A theoretical understanding of a possible mechanism for synthesizing
super-heavy elements in the outer crust of magnetars is presented. We
demonstrate that such a mechanism can be present whenever the baryon density in
the outer crust of a neutron star reaches values around 10^-2 fm^-3.
This scenario could be realized in magnetars with hypothetical large magnetic
fields, B ≥ 10^18 G. Under such conditions, the Coulomb lattice, formed
by ionized nuclei, enables a mechanism that synthesizes super-heavy elements.
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