Constraints on Phase Transitions in Neutron Star Matter

Recent inference results of the sound velocity in the cores of neutron stars are summarized. Implications for the equation of state and the phase structure of highly compressed baryonic matter are discussed. In view of the strong constraints imposed by the heaviest known pulsars, the equation of sta...

Full description

Bibliographic Details
Main Authors: Len Brandes, Wolfram Weise
Format: Article
Language:English
Published: MDPI AG 2024-01-01
Series:Symmetry
Subjects:
Online Access:https://www.mdpi.com/2073-8994/16/1/111