1. INTRODUCTION

2. NUMERICAL MODELS

2.1. ‘Observing’ Model Clusters

3. MASS SEGREGATION IN MODELS AND OBSERVED CLUSTERS

3.1. Quantifying Mass Segregation

4. PREDICTING THE NUMBER AND MASS OF RETAINED BLACK HOLES IN OBSERVED GLOBULAR CLUSTERS

5. THE ROLE OF BLACK HOLES IN THE EVOLUTION OF CORE RADIUS

6. COMPARISON WITH PRIOR RESULTS

7. SUMMARY & DISCUSSION

7.1. Summary

7.2. Discussion and Future Work