routines for computing neutron star structure and evolution

Fourth Open Gravitational-wave Catalog of Compact Binary Mergers (4-OGC). Using the data from LIGO and Virgo from 2015-2020, a comprehensive catalog including 94 detected mergers (90 BBH, 2 BNS, 2 NSBH) and sub-threshold candidates throughout O1, O2, O3a, and O3b..

Code and results for the disruption of axion miniclusters (AMCs) in the Milky Way, as well as radio signals from encounters between AMCs and neutrons stars.

Analysis pipeline capable of searching for dark compact objects in the Milky Way through astrometric lensing in real or mock Gaia DR4 data.

Constructs neutron star models in the context of regularized 4D Einstein-Gauss-Bonnet gravity, using the KEH/CST numerical scheme.

Python codes for modeling the physics of neutron starts. The coupled differential equations describing the equation of state and the structural model is solved. Comparison between the classical model and the relativistic model (Tolman-Oppenheimer-Volkov equation) is shown.

Collection of codes for general relativistic magnetohydrodynamics simulations. This includes an extension of the IllinoisGRMHD code (to allow the use of finite temperature EOS tables), along with several supporting codes which work within the EinsteinToolkit and Cactus infrastructure. Also included are several examples for running BNS merger sims.

Repository for the Star Log-extended eMulator package, used to solve the Tolman-Oppenheimer-Volkoff equations.

The Event Horizon Siphon is a theoretical framework for a compact, ultra-dense energy engine that harvests relativistic and quantum energy outputs generated in the moments prior to matter crossing a black hole's event horizon. This engine leverages a controlled interaction between a miniature black hole and neutron star matter to extract otherwise

Neutron Star Asteroseismology Solver: A Python-based tool that solves the TOV equations and linear radial pulsation equations to determine the fundamental oscillation frequencies (f-modes) of neutron stars using CompOSE Equation of State data and Monte Carlo sampling

PythiaBNS: Robust BNS Post-Merger Parameter Estimation with Empirical Priors

A toolkit of codes to generate, select and trace Lagrangian ejecta particles in the post-processing of GRMHD simulations. H5 files of the particles' trajectories, animations of their motion and .txt files ready to be inputted into nucleosynthesis networks can be produced with these codes.

Data release for the BBH / BNS search of single-detector LIGO data during O1 and O2.

First measurement of nuclear symmetry energy slope L₀ from vortex oscillations in pulsar glitches. Analysis code and data for RG paper.

Some examples and notes on GWFish from LGWA Workshop

Yuri Levin's website

Supplementary material for the paper "Constraints on wide-band radiative changes after a glitch in PSR J1452-6036".

Supplementary material for the paper "The UTMOST pulsar timing programme I: Overview and first results".

Searches for nontensorial gravitational waves from known pulsars

Semi-analytic Solvers for Two-component General-relativistic Spherically Symmetric Stars