Compact Star Properties from an Extended Linear Sigma Model
The equation of state provided by effective models of strongly interacting matter should comply with the restrictions imposed by current astrophysical observations of compact stars. Using the equation of state given by the (axial-)vector meson extended linear sigma model, we determine the mass&#...
Main Authors: | , , , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2019-07-01
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Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/5/7/174 |