TL;DR
This paper discusses the neutron-matter equation of state, focusing on the symmetry energy's empirical constraints and the potential existence of inhomogeneous chiral phases in neutron star cores.
Contribution
It provides new insights into the symmetry energy parameters and explores the possibility of inhomogeneous quark matter phases inside neutron stars.
Findings
Empirical constraints on the symmetry energy slope parameter.
Analysis of inhomogeneous chiral phases in neutron star cores.
Implications for neutron star structure and composition.
Abstract
In this presentation I discuss two aspects of the neutron-matter equation of state. One relates to the symmetry energy of nuclear matter and empirical constraints on its slope parameter at saturation density. The second deals with spatially inhomogeneous chiral phases of deconfined quark matter in the inner core of a neutron star.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Quantum, superfluid, helium dynamics · Atomic and Subatomic Physics Research