On the relativistic and electrodynamical stability of massive nuclear density cores
Vladimir Popov, Michael Rotondo, Remo Ruffini, She-Sheng Xue

TL;DR
This paper develops a unified relativistic model for nuclear density cores, extending classic atomic results to massive cores with up to 10^57 nucleons, revealing stability conditions and electric field properties.
Contribution
It introduces a novel treatment of massive nuclear cores using relativistic Thomas-Fermi equations, generalizing atomic models to astrophysical scales and identifying a new stability island.
Findings
Discovery of a new stability island for A > A_R
Balance of Coulomb repulsion and gravity in massive cores
Presence of overcritical electric fields near the surface
Abstract
We present a unified treatment of nuclear density cores recovering the classic results for neutral atoms with heavy nuclei having a mass number and extrapolating these results to massive nuclear density cores with . The treatment consists of solving the relativistic Thomas-Fermi equation describing a system of neutrons, protons and electrons in beta decay equilibrium. The protons are distributed at a constant density within a spherical core of radius . A new island of stability is found for . The Coulomb repulsion, screened by relativistic electrons, is balanced by the gravitational self-interaction of the core. In analogy to heavy nuclei they present, near their surface, an overcritical electric field. The relation between and is…
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Taxonomy
TopicsNuclear physics research studies · Atomic and Subatomic Physics Research · Quantum, superfluid, helium dynamics
