Discussion Overview
The discussion revolves around the implications of cosmic rays being overwhelmingly positively charged and whether this leads to the expectation of highly charged Reissner-Nordstrom black holes, potentially near extremality. Participants explore theoretical aspects, estimations of charge density, and the distribution of charges in the universe.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- Some participants propose that the emission of positively charged cosmic rays implies a buildup of negative charge, potentially leading to highly charged black holes.
- Others argue against the assumption that an enormous negative charge must accumulate, suggesting that cosmic rays do not necessarily correlate with significant charge buildup.
- One participant estimates the cosmic ray density and calculates total charge in a galaxy, concluding that the charge could exceed the extremality threshold for black holes, but questions the validity of the assumptions made.
- Another participant points out that the estimated charge density leads to an implausible charge per gram of mass in galaxies, raising concerns about the electrostatic forces involved.
- Some participants discuss the distribution of negative charges, questioning why they are not observed alongside the positive cosmic rays and suggesting they may be attached to matter rather than freely distributed.
- One participant speculates that negatively charged regions might attract positive charges, preventing significant accumulation of negative charge in the interstellar medium.
- A later reply suggests that electrons are more easily scattered than protons, which could explain the observed lack of negative charge in cosmic rays.
Areas of Agreement / Disagreement
Participants express differing views on the relationship between cosmic rays and charge buildup, with no consensus on whether significant negative charge accumulates or how it is distributed. The discussion remains unresolved regarding the implications for black holes and the nature of charge in the universe.
Contextual Notes
Limitations include assumptions about cosmic ray density and the overall charge neutrality of the universe, as well as the dependence on specific definitions of charge distribution. The calculations presented rely on various approximations that may not hold under scrutiny.