Neutron Stars, the Most Exotic Nuclear Lab in the Universe

TL;DR

This paper introduces neutron stars, highlighting their extreme physical conditions, macroscopic properties, and how astronomical observations reveal insights into ultra-dense nuclear matter and fundamental physics.

Contribution

It provides an accessible overview of neutron star physics, connecting observational data with the extreme microscopic conditions inside these compact objects.

Findings

Neutron stars exhibit extreme density and gravitational stability.

Neutronization occurs with increasing density in neutron star interiors.

Observations of neutron stars inform about super-dense, superfluid nuclear matter.

Abstract

In this lecture, we give a first introduction to neutron stars, based on fundamental physical principles. After outlining their amazing macroscopic properties, as obtained from observations, we infer the extreme conditions of matter in their interiors. We then describe two crucial physical phenomena which characterize compact stars, gravitational stability of strongly degenerate matter and neutronization of nuclear matter with increasing density, and explain how the formation and properties of neutron stars are a consequence of the extreme compression of matter under gravity. Finally, we describe how astronomical observations of various external macroscopic features can give invaluable information about the exotic microscopic scenario inside: neutrons stars represent a unique probe to study super-dense, isospin-asymmetric, superfluid, bulk hadronic matter.