Discussion Overview
The discussion revolves around the contribution of gravitational redshift to the total redshift observed in quasars and its implications for Hubble's law. Participants explore the nature of redshift in quasars, particularly in relation to their distance and the effects of gravitational fields near supermassive black holes.
Discussion Character
- Debate/contested
- Technical explanation
- Conceptual clarification
Main Points Raised
- One participant questions the percentage of total redshift in quasars attributed to gravitational redshift, suggesting it may affect calculations of distance based on redshift.
- Another participant argues that the gravitational redshift component in quasar spectra is effectively negligible, as the light originates from regions far from the supermassive black hole.
- A different viewpoint emphasizes that radiation emitted near a black hole would be overshadowed by emissions from more distant matter, complicating the detection of gravitational redshift.
- Concerns are raised about the lack of observed time dilation in quasars compared to Type Ia supernovae, prompting questions about fundamental differences in their behavior.
- Some participants note that while the majority of redshift is cosmological, evidence of gravitational redshift can be seen in the shape of emission lines in quasar spectra, indicating a complex interplay of factors.
- There is a discussion on the terminology surrounding quasars, QSO's, and AGNs, with participants expressing confusion about the distinctions and their implications for the observed phenomena.
Areas of Agreement / Disagreement
Participants express differing views on the significance of gravitational redshift in quasars, with some asserting its negligible impact while others suggest it may have observable effects. The discussion remains unresolved regarding the implications of these differing perspectives on Hubble's law and the nature of time dilation in quasars.
Contextual Notes
Participants highlight the complexity of quasar emissions, including contributions from various physical regimes and the evolutionary changes quasars undergo over time, which may affect observations and interpretations.