SUMMARY
The discussion centers on the search for an interior space-time metric for spherically symmetric rotating stars, specifically seeking a solution analogous to the interior Schwarzschild solution for rotating stars. Participants highlight that existing metrics primarily describe the exterior, such as the Kerr Metric and its associated frame-dragging effects. Key references provided include works by Michael Bradley, Gyula Fodor, and Ron Wiltshire, which explore slowly rotating non-stationary fluid solutions and their relationship to Kerr empty space-time.
PREREQUISITES
- Understanding of general relativity and Einstein's equations
- Familiarity with the Schwarzschild and Kerr metrics
- Knowledge of fluid dynamics in relativistic contexts
- Ability to interpret academic papers in theoretical physics
NEXT STEPS
- Research the interior Schwarzschild solution and its implications
- Study the slowly rotating non-stationary fluid solutions of Einstein's equations
- Examine the Wahlquist metric and its limitations in describing isolated rotating bodies
- Explore the concept of trapped null geodesics in rotating interior metrics
USEFUL FOR
The discussion is beneficial for theoretical physicists, astrophysicists, and researchers focused on general relativity, particularly those investigating the interior metrics of rotating stars and their implications in astrophysical models.