Discussion Overview
The discussion centers around the longevity of electromagnetic waves, particularly in the context of the cosmic microwave background (CMB) radiation from the big bang and how it compares to the behavior of radio waves from AM and FM antennas. Participants explore the mechanisms behind wave propagation and the implications of photon decay.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant questions how electromagnetic waves from the big bang can still be detected after 14 billion years, contrasting this with the behavior of AM and FM radio waves which weaken over distance.
- Another participant clarifies that while AM and FM waves weaken with distance, they do not completely die out, suggesting that they become too weak for detection rather than disappearing entirely.
- A further contribution discusses the Inverse Square Law (ISL) and its implications for signal strength over large distances, noting that it affects both nearby and distant astronomical objects similarly.
- One participant points out that the ISL does not apply to the CMB since it emanates from all directions rather than a single point source.
- Another participant introduces the concept of photon decay, arguing that if photons were to decay, they would need to have mass. They reference experimental limits on photon mass and suggest that a photon's lifetime could be extraordinarily long, potentially exceeding the age of the universe.
- This participant proposes that unless a photon is absorbed or interacts with something else, it could theoretically exist indefinitely.
Areas of Agreement / Disagreement
Participants express differing views on the application of the Inverse Square Law to the CMB and the concept of photon decay. There is no consensus on the implications of these points, and the discussion remains unresolved regarding the longevity of electromagnetic waves.
Contextual Notes
The discussion involves assumptions about wave propagation, the nature of photons, and the conditions under which electromagnetic waves may be detected or decay. These factors are not fully resolved and depend on specific definitions and experimental limitations.