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