Discussion Overview
The discussion revolves around the concept of "apparent superluminal velocity of galaxies," particularly in the context of general relativity (GR) and the implications of cosmic expansion. Participants explore the theoretical underpinnings, misconceptions, and various interpretations related to galaxies appearing to move faster than light due to the expansion of the universe.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants discuss the lack of a general, coordinate-independent notion of relative velocity in GR, emphasizing that velocities are context-dependent.
- There are claims that while objects cannot exceed the speed of light, the expansion of space can result in galaxies receding from us at apparent superluminal speeds, particularly for redshifts greater than approximately 1.7.
- One participant mentions that naive applications of the Doppler formula can lead to misconceptions about galaxies receding faster than light, suggesting that the recession should not be taken literally.
- Another participant notes that the metric of spacetime changes due to cosmic expansion, affecting the wavelength of light and contributing to the apparent superluminal velocities.
- Some participants express interest in ongoing research and papers being written on the topic, indicating a continued exploration of these ideas.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the interpretations of apparent superluminal velocities, with multiple competing views and ongoing debates about the implications of general relativity and cosmic expansion.
Contextual Notes
Participants highlight the complexities of discussing velocities in the context of GR, including the dependence on definitions of distance and the coordinate systems used. There are references to various papers and FAQs that address these complexities, but no definitive resolution is presented.
Who May Find This Useful
This discussion may be of interest to those studying general relativity, cosmology, or the physics of galaxies, as well as individuals exploring the implications of cosmic expansion on observed velocities.