SUMMARY
The discussion centers on calculating proper time in an accelerated frame of reference using Special Relativity (SR) with curved coordinates. It is established that the Lorentz transformation is not applicable in this context, as it pertains only to inertial frames. Instead, the proper time can be calculated using the formula τ = ∫(t1 to t2) √(1 - v(t)²/c²) dt, where v(t) is the velocity of the observer. The integration of this expression provides the necessary proper time without the need for General Relativity (GR) mechanics.
PREREQUISITES
- Understanding of Special Relativity (SR)
- Familiarity with proper time calculations
- Knowledge of curved coordinate systems
- Basic calculus for integration
NEXT STEPS
- Study the derivation of the proper time formula τ = ∫(t1 to t2) √(1 - v(t)²/c²) dt
- Explore the concept of arc length (ds²) in curved coordinates
- Learn about the limitations of Lorentz transformations in non-inertial frames
- Investigate applications of proper time in accelerated reference frames
USEFUL FOR
Physicists, students of relativity, and anyone interested in the mathematical foundations of time calculations in accelerated frames will benefit from this discussion.