TL;DR
This review summarizes recent advances in modeling neutron star crusts across multiple physics disciplines and discusses how these models compare with observational data.
Contribution
It provides a comprehensive overview of recent progress in microscopic and macroscopic modeling of neutron star crusts and their observational implications.
Findings
Progress in microscopic and macroscopic models of neutron star crusts
Comparison of theoretical models with observational data
Interdisciplinary approaches integrating nuclear physics, condensed matter, and relativity
Abstract
The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity. This review summarizes the progress, which has been achieved over the last few years, in modeling neutron star crusts, both at the microscopic and macroscopic levels. The confrontation of these theoretical models with observations is also briefly discussed.
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