Discussion Overview
The discussion centers on the lack of observed time dilation in the variability of quasars as reported in a study analyzing quasar light curves and their Fourier power spectra. Participants explore the implications of this finding on cosmological theories and the nature of quasars, considering various explanations and challenges to established views.
Discussion Character
- Debate/contested
- Exploratory
- Technical explanation
Main Points Raised
- Some participants express concern over the lack of time dilation in quasar variability, suggesting it poses a serious challenge to modern cosmological theories.
- One viewpoint suggests that time dilation might not be a property of the Universe, implying a non-expanding Universe, though this contradicts strong support for the big bang theory.
- Another perspective proposes that quasars may not be at cosmological distances, a claim that has been historically disputed but has gained support from studies of quasar host galaxies.
- Some argue that observed variations in quasars could be due to intervening processes like gravitational microlensing, while others contend that intrinsic variations from the central accretion disc are more significant.
- A participant references studies that argue against microlensing as the dominant cause of quasar variability, noting evidence of asymmetric light-curve profiles.
- Suggestions are made to investigate potential biases in the data analysis, including selection effects related to redshift and quasar color, as well as the intrinsic nature of quasar variability.
- One participant mentions a related study on gamma-ray bursts that finds evidence of time dilation, suggesting a contrast with quasar findings.
- Concerns are raised about the reliability of the peer review process in validating the findings of the original study.
Areas of Agreement / Disagreement
Participants do not reach a consensus; multiple competing views and uncertainties remain regarding the implications of the findings and the nature of quasar variability.
Contextual Notes
Limitations include potential biases in the selection of quasar samples, the unknown details of quasar variability, and the unresolved nature of the mechanisms behind observed variations.