Discussion Overview
The discussion revolves around the expansion speed of the universe at the time of the Cosmic Microwave Background (CMB), specifically 370,000 years after the Big Bang. Participants explore the distinction between historical expansion speeds and the current Hubble parameter.
Discussion Character
Main Points Raised
- One participant seeks to understand the specific speed at which points in space were moving apart at 370,000 years after the Big Bang, rather than the current Hubble parameter.
- Another participant questions the focus on the specific time frame of 370,000 years post-Big Bang instead of the current Hubble parameter.
- Some participants argue that the concept of a single speed at which points in space are moving apart is problematic, as it depends on the distance between those points.
- It is noted that Hubble's law indicates that recession speed is proportional to distance, suggesting that only the Hubble parameter or specific recession speeds at given distances can be provided, rather than a singular recession velocity.
Areas of Agreement / Disagreement
Participants express disagreement regarding the notion of a singular expansion speed, with some emphasizing the dependence on distance and others focusing on the Hubble parameter. The discussion remains unresolved regarding the specific speed at the time of the CMB.
Contextual Notes
The discussion highlights limitations in defining expansion speed without specifying distances, as well as the dependence on the Hubble parameter for meaningful interpretation of recession velocities.