SUMMARY
The discussion centers on the feasibility of a proper time measuring clock existing in a changing Friedman metric, particularly regarding its ability to occupy spatial locations between events as space expands. The proper time is defined by the integral equation involving the metric tensor \( g_{\mu \nu} \) and the world line parameter \( \lambda \). Participants clarify that while real clocks are influenced by geodesic deviation due to tidal gravity, it is possible to construct sufficiently small clocks that minimize these effects. The conversation also touches on the transition from the spacetime interval equation in flat spacetime to the integral expression for proper time in a non-flat Friedman universe.
PREREQUISITES
- Understanding of Friedman metric in cosmology
- Familiarity with proper time and spacetime intervals
- Knowledge of geodesic deviation and tidal gravity
- Basic grasp of differential geometry and metric tensors
NEXT STEPS
- Study the implications of geodesic deviation in general relativity
- Explore the derivation of proper time in non-flat spacetimes
- Investigate the properties of the metric tensor \( g_{\mu \nu} \) in cosmological models
- Review textbooks such as "Gravitation" by Misner, Thorne, and Wheeler (MTW) for deeper insights
USEFUL FOR
Researchers, physicists, and students in the fields of general relativity and cosmology, particularly those interested in the behavior of time measurement in expanding universes.