Book contents
- Frontmatter
- Contents
- Preface
- PART I INTRODUCTIONS
- PART II THE CONTINUUM LIMIT: N → ∞
- 5 Paradoxical Thermodynamics
- 6 Statistical Mechanics
- 7 Motion in a Central Potential
- 8 Some Equilibrium Models
- 9 Methods
- PART III MEAN FIELD DYNAMICS: N = 106
- PART IV MICROPHYSICS: N = 2
- PART V GRAVOTHERMODYNAMICS: N = 106
- PART VI GRAVITATIONAL SCATTERING: N = 3
- PART VII PRIMORDIAL BINARIES: N = 4
- PART VIII POST-COLLAPSE EVOLUTION: N = 106
- PART IX STAR CLUSTER ECOLOGY
- Appendix A A Simple N-Body Integrator
- Appendix B Hints to Solution of Problems
- References
- Index
7 - Motion in a Central Potential
Published online by Cambridge University Press: 05 June 2012
- Frontmatter
- Contents
- Preface
- PART I INTRODUCTIONS
- PART II THE CONTINUUM LIMIT: N → ∞
- 5 Paradoxical Thermodynamics
- 6 Statistical Mechanics
- 7 Motion in a Central Potential
- 8 Some Equilibrium Models
- 9 Methods
- PART III MEAN FIELD DYNAMICS: N = 106
- PART IV MICROPHYSICS: N = 2
- PART V GRAVOTHERMODYNAMICS: N = 106
- PART VI GRAVITATIONAL SCATTERING: N = 3
- PART VII PRIMORDIAL BINARIES: N = 4
- PART VIII POST-COLLAPSE EVOLUTION: N = 106
- PART IX STAR CLUSTER ECOLOGY
- Appendix A A Simple N-Body Integrator
- Appendix B Hints to Solution of Problems
- References
- Index
Summary
- Type
- Chapter
- Information
- The Gravitational Million–Body ProblemA Multidisciplinary Approach to Star Cluster Dynamics, pp. 58 - 67Publisher: Cambridge University PressPrint publication year: 2003