SUMMARY
The discussion focuses on solving general geodesics in the Friedmann-Lemaître-Robertson-Walker (FLRW) metric when transitioning from comoving to conformal coordinates. Participants clarify that the presence of a Killing vector field does not simplify the geodesic equations due to the dependence of metric coefficients on the conformal coordinate, denoted as eta (##\eta##). The conversation highlights two primary methods for computing geodesics: the brute force approach and the geodesic Lagrangian method. Additionally, it is noted that the shape of orbits in FLRW spacetimes is independent of the choice of scale factor, as referenced in the paper by D. Garfinkle.
PREREQUISITES
- Understanding of the Friedmann-Lemaître-Robertson-Walker (FLRW) metric
- Familiarity with geodesic equations in general relativity
- Knowledge of Killing vector fields and their significance
- Proficiency in differential geometry and tensor calculus
NEXT STEPS
- Study the geodesic Lagrangian method for solving geodesic equations
- Review the paper "The shape of the orbit in FLRW spacetimes" by D. Garfinkle
- Explore the implications of different scale factors on geodesic paths in FLRW metrics
- Investigate the role of Killing vectors in simplifying geodesic calculations
USEFUL FOR
Researchers, physicists, and students in cosmology and general relativity, particularly those interested in the dynamics of geodesics in FLRW spacetimes.