Discussion Overview
The discussion revolves around the phenomenon of redshift in light due to the expansion of the universe, specifically addressing the implications for energy conservation. Participants explore the theoretical underpinnings of energy loss in redshifted light, the applicability of conservation laws in General Relativity (GR), and the conceptual challenges posed by these ideas.
Discussion Character
- Debate/contested
- Conceptual clarification
- Exploratory
- Technical explanation
Main Points Raised
- Some participants assert that light loses energy when redshifted (E=hf), questioning the conservation of energy in this context.
- Others argue that conservation of energy does not apply at cosmological scales, particularly in GR, where energy is not well-defined.
- A participant references Leonard Susskind's idea of thinking of energy as being "stretched" during redshift, which raises further questions about the nature of energy in an expanding universe.
- Some contributions mention the Cosmic Microwave Background (CMB) light being redshifted by a factor of z=1100, leading to significant energy loss, yet no consensus on where this energy goes is reached.
- One participant speculates that the lost energy might relate to vacuum energy or "dark energy," but acknowledges that no rigorous mathematical connection has been established.
- Questions are raised about the implications of local curvature in GR and whether energy conservation holds in specific scenarios, such as a collapsing system of photons.
- Another participant suggests that the observed redshift could involve photons shedding energy in ways that are difficult to measure, potentially linking this to the expansion of space-time.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the nature of energy conservation in the context of redshift and GR. Multiple competing views are presented regarding the implications of redshift on energy and the definitions of energy in cosmological contexts.
Contextual Notes
The discussion highlights the limitations of applying classical conservation laws in the framework of General Relativity and the unresolved nature of energy definitions in cosmological scenarios.