A short walk through the physics of neutron stars

TL;DR

This paper provides a concise overview of neutron star physics, covering their history, observational methods, and theoretical aspects like structure, composition, and emission processes.

Contribution

It offers a summarized review integrating historical context, observational techniques, and theoretical models of neutron stars in a single accessible overview.

Findings

Different types of telescopes used for observation

Various astrophysical manifestations of neutron stars

Key theoretical issues like composition and cooling mechanisms

Abstract

In this work we shortly review several aspects of the physics of neutron stars. After the introduction we present a brief historical overview of the idea of neutron stars as well as of the theoretical and observational developments that followed it from the mid 1930s to the present. Then, we review few aspects of their observation discussing, in particular, the different types of telescopes that are used, the many astrophysical manifestations of these objects, and several observables such as masses, radii or gravitational waves. Finally, we briefly summarize some of theoretical issues like their composition, structure equations, equation of state, and neutrino emission and cooling.