Discussion Overview
The discussion revolves around the GZK paradox and its potential explanations in the context of an expanding universe. Participants explore various theoretical models and implications related to cosmic rays, supernovae, and relativistic effects, focusing on both conceptual and mathematical aspects.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- One participant suggests that if the universe were divided into two mass zones that repel each other, this could explain why cosmic rays have not been stopped by the cosmic microwave background (CMBR), despite expectations based on the GZK limit.
- Another participant questions the connection between the acceleration of distant supernovae and the GZK limit, noting that the distances involved are significantly different.
- A participant proposes that if quarks in cosmic ray protons are considered to have a size and undergo relativistic length contraction, this could reduce the probability of collisions with CMBR photons, allowing protons to reach Earth.
- Reference to Stecker's discussion of the GZK effect is made, emphasizing that relativistic effects were considered in calculations regarding photomeson production cross sections.
- One participant shares a calculation indicating that the size of a charge sphere in a quark is much smaller than that of a proton at rest, suggesting that this could affect interaction probabilities with CMBR photons.
- Concerns are raised about how these considerations might also apply to high-energy protons colliding with other particles, potentially leading to different behaviors in air showers than what has been observed.
- Another participant notes that while the size of quarks affects collision probabilities, it does not determine the outcomes of collisions, assuming a similar number of oxygen quarks to CMBR photons encountered by cosmic rays.
Areas of Agreement / Disagreement
Participants express differing views on the relationship between supernovae acceleration and the GZK limit, with some proposing alternative models involving relativistic effects. The discussion remains unresolved with multiple competing perspectives presented.
Contextual Notes
Participants highlight the complexity of the GZK paradox and the need for careful consideration of relativistic effects, collision probabilities, and the implications of different theoretical models. Some assumptions and definitions remain unaddressed, contributing to the ongoing debate.