Discussion Overview
The discussion revolves around the fate of high-energy background photons in the context of the expanding Universe, particularly focusing on the Cosmic Microwave Background (CMB) and the implications of energy conservation in General Relativity (GR). Participants explore theoretical aspects, implications of redshift, and the nature of energy in an expanding universe.
Discussion Character
- Exploratory
- Debate/contested
- Technical explanation
Main Points Raised
- Some participants propose that high-energy background photons have been redshifted, resulting in their observation as a lower energy spectrum consistent with a temperature of 2.7K.
- Others argue that energy cannot be created or destroyed, raising questions about where the energy of these photons has gone.
- One participant suggests that the energy may convert to gravitational energy, questioning how the curvature of spacetime changes with the Universe's expansion.
- Another participant states that energy is not conserved in an expanding universe and that global energy conservation may not be definable in GR.
- Some contributions challenge the idea that photons did not lose energy, emphasizing the frame-dependent nature of energy in cosmological contexts.
- There are discussions about the implications of redshift and whether it can be viewed as an apparent loss of energy due to changing coordinate systems.
- One participant expresses a belief in the logical consistency of the universe, suggesting that underlying theories may be simpler than they appear.
Areas of Agreement / Disagreement
Participants express multiple competing views regarding the fate of high-energy photons and the nature of energy conservation in an expanding universe. There is no consensus on these issues, and the discussion remains unresolved.
Contextual Notes
Participants highlight limitations in defining energy conservation in GR and the dependence of energy definitions on the chosen coordinate system. The discussion also touches on the complexities of observational phenomena in curved spacetime.