SUMMARY
The discussion focuses on constructing the stress-energy tensor for an infinitely long circulating cylinder of light, as described in Mallett's paper. The tensor is given by Tμν = εημην, where ημ = (η0, 0, η2, 0) and ε represents the energy density of the laser light. The participants clarify that the null dust does not exhibit momentum density in the z-direction due to its circular flow in the φ-direction, despite the helical worldlines of its constituents. The discussion also addresses the differences between interior and exterior solutions of the metric tensor in relation to the rotating cylinder.
PREREQUISITES
- Understanding of stress-energy tensors in general relativity
- Familiarity with null dust and its wave 4-vector field
- Knowledge of Einstein's equations and their solutions
- Basic concepts of fluid dynamics in the context of general relativity
NEXT STEPS
- Study Mallett's paper on the stress-energy tensor for circulating light: Mallett (2003)
- Learn about the Van Stockum dust and Gödel metric as examples of circulating dust fields
- Explore the concept of interior and exterior solutions in general relativity
- Review the formalism of null dust fields and their applications in gravitational physics
USEFUL FOR
This discussion is beneficial for physicists, particularly those specializing in general relativity, cosmology, and theoretical physics, as well as graduate students seeking to deepen their understanding of stress-energy tensors and their implications in gravitational models.