Discussion Overview
The discussion revolves around the phenomenon of redshift observed in light from receding galaxies due to the expanding universe. Participants explore the implications of redshift on energy loss in photons, the conservation of energy in curved spacetime, and the relationship between redshift and distance in different spacetime models.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants note that redshift indicates a loss of energy in light from receding galaxies, questioning where this lost energy goes.
- Others argue that in curved spacetime, energy is not globally conserved, suggesting that the lost energy does not violate any laws of physics.
- One participant explains that redshift can be understood through special relativity, involving both classical Doppler effects and time dilation, which contribute to perceived energy loss.
- A participant raises a question about the implications of redshift on energy measurements using spectrometers and photometers, seeking clarification on how energy relates to frequency and wavelength at the time of emission.
- Another participant emphasizes that the relationship between redshift and distance differs in the context of special relativity compared to the expanding universe modeled by Friedmann-Robertson-Walker (FRW) spacetime.
- Some participants express confusion regarding the interpretation of energy loss and the conditions under which it occurs, particularly in relation to Einstein's work on the energy of light rays.
- References to previous discussions and literature are made to support claims about the relativistic Doppler effect and its relation to classical Doppler shifts.
Areas of Agreement / Disagreement
Participants generally agree that redshift involves energy loss, but there is no consensus on the implications of this loss or the mechanisms behind it. Multiple competing views remain regarding the conservation of energy in cosmological contexts and the interpretation of redshift in different spacetime models.
Contextual Notes
Participants highlight limitations in understanding energy conservation on cosmological scales and the complexities introduced by different models of spacetime. There are unresolved questions about the relationship between redshift, energy, and the conditions of light emission.