Discussion Overview
The discussion centers on the concept of charged black holes, particularly examining whether the notion of a charged black hole is coherent within the frameworks of general relativity (GR) and quantum electrodynamics (QED). Participants explore the implications of charge invariance, gravitational effects on charge, and the behavior of charged matter near the event horizon (EH).
Discussion Character
- Debate/contested
- Technical explanation
- Conceptual clarification
Main Points Raised
- Some participants argue that the established view holds that the net charge of a black hole is invariant regardless of whether infalling charged matter is outside, at, or inside the event horizon, as determined by Gauss's law.
- One participant questions the implications of lowering charged matter towards the EH, suggesting that as coordinate mass reduces due to gravitational effects, so too might the coordinate charge, leading to a potential asymptotic vanishing of observed charge as the EH is approached.
- Another participant challenges the idea that charge divided by energy is globally invariant, arguing that local invariance does not necessarily imply global invariance.
- Some participants reference the Reissner-Nordström solution as a framework for understanding charged black holes, noting that black holes can be characterized by their total charge, mass, and angular momentum.
- Concerns are raised about the lack of literature addressing the specific objections regarding charge invariance and gravitational redshift of charge, with requests for references to support claims made in the discussion.
Areas of Agreement / Disagreement
Participants express differing views on the implications of charge invariance and the behavior of charged matter near black holes. There is no consensus on the validity of the established view or the implications of gravitational effects on charge.
Contextual Notes
Some participants note the need for references to support claims regarding established views and the relationship between gravitational redshift and charge invariance. The discussion highlights the complexity and nuances involved in understanding charged black holes.