Discussion Overview
The discussion revolves around the implications of the universe's expansion on the conservation of energy, particularly in relation to the redshift of light and gravitational theory. Participants explore whether the elongation of light wavelengths due to cosmic expansion constitutes a violation of energy conservation, examining both general relativity and Newtonian perspectives.
Discussion Character
- Debate/contested
- Technical explanation
- Conceptual clarification
Main Points Raised
- Some participants assert that the expansion of the universe causes the wavelengths of light to increase, leading to a decrease in energy, particularly referencing cosmic background radiation.
- There is uncertainty about whether this decrease in energy constitutes a violation of conservation laws, with some suggesting it is a subtle question within gravitational theory.
- One perspective argues that there is no global conservation of energy in the universe due to the lack of a timelike Killing vector in the Friedmann-Robertson-Walker (FRW) metric.
- Another viewpoint states that general relativity enforces a form of energy conservation through the energy-momentum tensor, as dictated by the Bianchi identity and Einstein's field equations.
- A Newtonian perspective is introduced, suggesting that the redshift of light is compensated by a change in volume, implying that work done during expansion compensates for the redshift.
- Some participants express support for the Newtonian approach, while others question the applicability of this reasoning in the absence of an external atmosphere to push against during expansion.
- There is a suggestion to liken the "pressure" in the Newtonian perspective to dark energy, raising further questions about the nature of work done during the universe's expansion.
- One participant questions whether the work performed during expansion is against gravitational potential energy due to increased distances between galaxies.
Areas of Agreement / Disagreement
Participants do not reach a consensus on whether the expansion of the universe violates conservation of energy. Multiple competing views are presented, particularly between general relativity and Newtonian interpretations.
Contextual Notes
The discussion highlights limitations in understanding energy conservation in cosmological contexts, particularly regarding the assumptions made in different theoretical frameworks and the implications of gravitational effects.