This book, written for a general readership, reviews and explains the three- body problem in historical context reaching to latest developments in computational physics and gravitation theory.
The focus of this book is on statistical and perturbation methods specifically applied to the general three body problem in celestial mechanics. It provides a comprehensive overview of techniques used to analyze the complex interactions between three bodies under gravitational influence, offering insights into their dynamics and stability. The text is aimed at researchers and students interested in advanced mathematical approaches to understanding this classic problem in physics and astronomy.