Stability of Spherical Nuclei in the Inner Crust of Neutron Stars

Neutron stars are the densest objects in the Universe. In this paper, we consider the so-called inner crust—the layer where neutron-excess nuclei are immersed in the degenerate gas of electrons and a sea of quasi-free neutrons. It was generally believed that spherical nuclei become unstable with res...

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Bibliographic Details
Main Authors: Nikita A. Zemlyakov, Andrey I. Chugunov
Format: Article
Language:English
Published: MDPI AG 2022-07-01
Series:Particles
Subjects:
Online Access:https://www.mdpi.com/2571-712X/5/3/20