Concept: Pulsars and Gravitational Waves Research
Q–Monopole–Ball soliton with unit magnetic charge exists
A new solution binding monopoles through topological and non-topological charges
Frame center acceleration method improved trajectory consistency
Comparing two methods for modeling gravitational effects on spacecraft trajectories
TransFit-CSM models interaction-powered transients with consistent shock diffusion
A new model for predicting how stellar explosions interact with surrounding material
Separability of gravitational wave equations in rotating black hole geometries
Separable wave solutions in rotating black hole spacetimes
