Discussion Overview
The discussion centers on the implications of Hubble's velocity law regarding time dilation for distant receding objects in the context of cosmology and special relativity. Participants explore whether proper time measured by observers near these objects is dilated and the consequences of superluminal recession rates.
Discussion Character
- Debate/contested
- Conceptual clarification
- Exploratory
Main Points Raised
- Some participants assert that according to Hubble's law, the velocity of distant objects is given by v = H_0 * r, where H_0 is the Hubble constant and r is the distance.
- One participant questions whether proper time for an observer near a receding object is dilated by a gamma factor of 1/sqrt(1-v^2/c^2) when measured in our time coordinates.
- Another participant disagrees, stating that for many galaxies, the velocities exceed the speed of light, leading to a gamma factor involving the square root of a negative number, which would not make sense as a time dilation factor.
- There is a discussion about the implications of galaxies receding faster than light, including the idea that photons from such galaxies may never reach us due to the expansion of space.
- A thought experiment is proposed regarding a long rigid platform in space and whether objects moving with the Hubble flow would exceed the speed of light relative to an observer at one end of the platform.
- Another participant suggests that even a hypothetical super-rigid platform could not allow for any part of it to exceed the speed of light, raising questions about the nature of observable objects in such a scenario.
Areas of Agreement / Disagreement
Participants express differing views on the application of special relativity to receding galaxies and the implications of superluminal velocities. The discussion remains unresolved, with competing perspectives on the nature of time dilation and the behavior of light from distant galaxies.
Contextual Notes
Participants highlight limitations in applying special relativity to cosmological scenarios, particularly regarding the frames of reference of receding galaxies and the implications of superluminal recession rates.