The plasma mechanism of stabilization of neutron-excess nuclei in stars
B.V.Vasiliev
TL;DR
This paper explores a plasma-based mechanism that stabilizes neutron-rich nuclei in stars, potentially explaining neutronization processes in both hot stars and dwarfs.
Contribution
It introduces a plasma mechanism that accounts for neutron-excess nuclei stabilization across different stellar environments.
Findings
Proposes a plasma mechanism for neutronization in stars.
Suggests similar processes occur in hot stars and dwarfs.
Abstract
The mechanism of stabilization of neutron-excess nuclei in stars is considered. This mechanism must produce the neutronisation process in hot stars in the same way as it occurs in the dwarfs.
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Taxonomy
TopicsAstro and Planetary Science · Nuclear physics research studies · Quantum, superfluid, helium dynamics