QLIMR Module
Welcome to the documentation for the QLIMR module, a computational tool designed to obtain gravitational observables of slowly rotating neutron stars. The acronym “QLIMR” stands for Quadrupole moment (Q), tidal Love number (L), Moment of inertia (I), Mass (M), and Radius (R) of the star. This module provides a comprehensive framework for studying the gravitational properties of neutron stars using a barotropic Equation of State (EoS) provided by the user. In the following sections, you will find all the relevant information needed to effectively harness the capabilities of the QLIMR module.