Discussion Overview
The discussion revolves around the contributions of gravitational bending and Newtonian refraction of light as it passes near a star, particularly focusing on the implications of these effects in the context of General Relativity (GR) and observational data. Participants explore theoretical models, historical experiments, and the validity of certain papers related to this topic.
Discussion Character
- Debate/contested
- Technical explanation
- Historical
Main Points Raised
- Some participants suggest that Newtonian refraction must play a role in the bending of light near the sun, questioning how to separate its contributions from those of GR.
- Others propose that a model of the solar atmosphere's composition and density could be used to calculate the refractive index and its effect on light paths, potentially using Maxwell's equations or Huygens' Principle.
- One participant recalls that during the 1919 eclipse, Eddington's measurements of stellar light deflection aligned closely with GR predictions, with no mention of refraction effects.
- Another participant notes that the solar corona is unstable, suggesting that any refractive effects would be variable and difficult to reconcile with consistent GR predictions.
- Concerns are raised about the credibility of a referenced paper, including its lack of peer review and citations, and the unusual redefinition of black holes presented in it.
- Some participants express skepticism about the paper's validity, questioning its presence on arXiv and the standards of publication at the time it was posted.
- A later comment mentions that the Gaia telescope observes deflection of starlight by the Sun, indicating that this effect is measurable and significant, independent of stellar atmospheres.
Areas of Agreement / Disagreement
Participants express a range of views on the contributions of gravitational bending versus refraction, with no consensus reached. Some agree on the potential role of refraction, while others emphasize the historical context and results of GR tests, leading to an ongoing debate.
Contextual Notes
Participants note limitations in the discussion, including the need for clarity on the assumptions made regarding the solar atmosphere and the historical context of Eddington's measurements. The credibility of the referenced paper is also questioned, highlighting the lack of peer review and its unconventional claims.