Superfluidity and Superconductivity in Neutron Stars

By compressing matter to densities up to several times the density of atomic nuclei, the catastrophic gravitational collapse of the core of stars with a mass <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow>...

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Bibliographic Details
Main Author: Nicolas Chamel
Format: Article
Language:English
Published: MDPI AG 2024-02-01
Series:Universe
Subjects:
n/a
Online Access:https://www.mdpi.com/2218-1997/10/3/104