Discussion Overview
The discussion revolves around the concept of co-moving density in cosmology, particularly in relation to the effects of cosmic expansion on mass and energy density. Participants explore the implications of defining density in co-moving versus proper regions of space, considering factors such as the behavior of light and relativistic particles in an expanding universe.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Conceptual clarification
Main Points Raised
- Some participants propose that in a proper region of space, mass/energy density changes due to expansion and work done by pressure, while in a co-moving region, density should remain constant due to the absence of expansion.
- Others argue that when including light, the co-moving density is not constant because the wavelengths of photons increase with expansion, leading to a decrease in energy.
- A participant suggests that "cold" particles can be treated as stationary in an expanding volume, thus their mass/energy does not change, while relativistic particles experience energy loss due to expansion.
- There is a discussion about the implications of co-moving coordinates on the measurement of the Cosmic Microwave Background (CMB) and how it relates to temperature and energy content.
- One participant raises a question about the effect of expansion on high-velocity particles moving towards distant galaxies, suggesting that their speeds may be reduced due to cosmic expansion.
- Another participant introduces the idea that dark matter (DM) particles may lose kinetic energy through expansion, which could play a role in structure formation in the universe.
- There is a query about whether two observers can be jointly at rest relative to the CMB, to which a participant confirms that it is possible under certain conditions.
Areas of Agreement / Disagreement
The discussion contains multiple competing views regarding the behavior of co-moving density and the effects of cosmic expansion on different types of particles. Participants do not reach a consensus on these points, and various interpretations of the implications of co-moving and proper density remain unresolved.
Contextual Notes
Participants express uncertainty regarding the definitions of density and the conditions under which different types of particles behave in an expanding universe. The discussion highlights the complexity of measuring energy and momentum in co-moving versus proper frames of reference.