Discussion Overview
The discussion revolves around the implications of cosmological redshift on photon energy and the principles of energy conservation in the context of general relativity. Participants explore the relationship between redshift, energy conservation, and the nature of spacetime, touching on both theoretical and conceptual aspects.
Discussion Character
- Debate/contested
- Conceptual clarification
- Technical explanation
Main Points Raised
- Some participants question what happens to photon energy lost due to cosmological redshift.
- One participant states that there is no global conservation of energy principle in general relativity applicable to all spacetimes.
- Another argues that redshifted photons are time dilated and that their energy is conserved over time, challenging the validity of this claim.
- A comparison is made to the Pound-Rebka experiment to illustrate energy conservation in specific contexts, noting that cosmological spacetimes lack conserved scalar measures of mass-energy.
- Participants discuss the analogy of throwing a ball from a moving train to explain energy conservation in different reference frames, suggesting that energy is frame-dependent.
- One participant introduces the idea that the energy lost by redshifted photons may contribute to the momentum of the emitter, though this is contested as being a small effect.
- There is a suggestion that the redshift experienced by photons does not occur at the moment of emission, raising questions about its implications for energy conservation.
- Another participant emphasizes that discussing global energy conservation is meaningless because energy cannot be universally defined across different inertial frames.
- Concerns are raised about the relevance and credibility of external quotes and sources used in the discussion.
- Some participants assert that energy conservation is agreed upon in flat spacetime, while questioning the existence of energy in such contexts.
Areas of Agreement / Disagreement
Participants express disagreement on the nature of energy conservation in cosmological contexts, with some asserting that energy conservation holds in flat spacetime while others challenge the applicability of this principle in curved spacetimes. The discussion remains unresolved regarding the implications of redshift on energy conservation.
Contextual Notes
Participants note that the discussion involves complex concepts of spacetime geometry, energy definitions, and the implications of redshift, which may not be accessible to all participants. There are references to specific experiments and theoretical frameworks that may require further clarification.