Discussion Overview
The discussion centers around the comparison of two formulas from MTW (Misner, Thorne, and Wheeler) related to the proper time experienced by a radially free falling observer in a Schwarzschild solution. Participants explore the implications of these formulas, particularly in the context of observers starting at rest versus those starting at escape velocity, and the behavior of these formulas as the radial coordinate approaches infinity.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- One participant notes a constant ratio of 3/4 Pi between the two formulas but expresses confusion about their convergence as r approaches infinity.
- Another participant mentions that the escape velocity is a critical point and compares the infall times for different velocities, suggesting that the ratio of infall times remains infinite at escape velocity.
- There is a discussion about the derivation of the second formula (25.38) and its relation to the energy and angular momentum of a test particle falling from infinity.
- Some participants express confusion regarding the interpretation of escape velocity and its implications for the proper time to reach the singularity.
- Concerns are raised about the differences in energy at infinity between a free falling observer and a stationary observer, with one participant emphasizing that the former has an energy of 1 while the latter has less than 1.
- Participants discuss the implications of increasing values of r on the proper time differential between the two observers, with some suggesting that the proper time difference increases without bound while the ratio remains constant.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the implications of the formulas or the nature of the differences between free falling and stationary observers at infinity. Multiple competing views remain regarding the interpretation of the results and the behavior of the proper time as r increases.
Contextual Notes
Participants express uncertainty about specific derivations and the implications of the formulas, particularly regarding the limits as r approaches infinity and the physical interpretations of escape velocity. There are also references to potential discrepancies in different editions of MTW.