Neutron Stars and the High Density Equation of State
T.Klahn, C.D.Roberts, D.B.Blaschke, F.Sandin
TL;DR
This paper reviews recent developments in understanding the high-density equation of state of neutron stars, emphasizing the role of quark matter phase structure and its implications for astrophysics.
Contribution
It offers a perspective on the challenges and opportunities in modeling neutron star cores using the high-density equation of state and quark matter phases.
Findings
Insights into the phase structure of quark matter in neutron star cores
Discussion of challenges in modeling high-density matter
Potential observational signatures of quark matter in neutron stars
Abstract
One of the key ingredients to understand the properties of neutrons stars is the equation of state at finite densities far beyond nuclear saturation. Investigating the phase structure of quark matter that might be realized in the core of NS inspires theory and observation. We discuss recent results of our work to point out our view on challenges and possibilities in this evolving field by means of a few examples.
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