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Part I. Introductions: 1. Astrophysics introduction; 2. Theoretical physics introduction; 3. Computational physics introduction; 4. Mathematical introduction; Part II. The Continuum Limit: 5. Paradoxical thermodynamics; 6. Statistical mechanics; 7. Motion in a central potential; 8. Some famous models; 9. Methods; Part III. Mean Field Dynamics: 10. Violent relaxation; 11. Internal mass loss; 12. External influences; Part IV. Microphysics: 13. Exponential orbit instability; 14. Two-body relaxation; 15. From Kepler to Kustaanheimo; Part V. Gravothermodynamics: 16. Escape and mass segregation; 17. Gravothermal instability; 18. Core collapse rate for star clusters; Part VI. Gravitational Scattering: 19. Thought experiments; 20. Mathematical three-body scattering; 21. Analytical approximations; 22. Laboratory experiments; 23. Gravitational burning and transmutation; Part VII. Primordial Binaries: 24. Binaries in star clusters; 25. Triple formation and evolution; 26. A non-renewable energy source; Part VIII. Post-Collapse Evolution: 27. Surviving core collapse; 28. Gravothermal oscillations; 29. Dissolution; Part IX. Star Cluster Ecology: 30. Stellar and dynamical evolution; 31. Collisions and capture; 32. Binary star evolution and blue stragglers; 33. Star cluster evolution; Appendices.

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