Discussion Overview
The discussion revolves around the phenomenon of high redshift quasars appearing in nearby galaxies, exploring potential explanations and interpretations of their redshifts. Participants reference historical opinions, current research, and the implications for cosmological models, including General Relativity and dark energy.
Discussion Character
- Exploratory
- Debate/contested
- Technical explanation
- Conceptual clarification
Main Points Raised
- Some participants reference an article discussing high redshift quasars in nearby galaxies and seek explanations for this phenomenon.
- Geoffrey Burbidge's long-held view that quasar redshifts are not cosmological is noted, with some arguing that the quasar's apparent proximity is misleading due to its actual distance.
- Concerns are raised about the lack of evidence for intervening material in quasar spectra, suggesting that a nearby galaxy should show more signs of gas and dust along the line of sight.
- Morley B Bell's research is mentioned, proposing that if quasars' redshifts are cosmological, the resulting explanations are complex and leave many unsolved puzzles, while an alternative view suggests an intrinsic redshift component that diminishes over time.
- Some participants assert that dark matter and dark energy do not necessitate modifications to General Relativity, while others argue that these concepts arise from gravitational effects not fully explained by GR.
- Questions are raised about specific unsolved puzzles related to quasar redshifts and their implications for cosmological models, including the accelerating expansion of the universe.
- Participants discuss the implications of quasar distribution and characteristics, suggesting that conventional evolutionary models may not adequately explain observed phenomena.
Areas of Agreement / Disagreement
There is no consensus among participants. Multiple competing views exist regarding the interpretation of quasar redshifts, the implications for General Relativity, and the nature of dark energy and dark matter.
Contextual Notes
Participants express uncertainty regarding the assumptions underlying various models and the definitions of terms used in the discussion. The complexity of the explanations and the existence of unresolved questions are acknowledged.