What Makes Charged Black Holes Different from Uncharged Ones?

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SUMMARY

This discussion focuses on the differences between charged black holes (BH) and uncharged black holes, particularly regarding their equations and the implications of electric forces at the event horizon. Participants explore the nature of gravitational forces in relation to electric attraction and the behavior of virtual particles, such as photons and quarks, near the horizon. Key points include the assertion that virtual photons can traverse the horizon and the consideration of color charge in black holes, highlighting the complexities of quantum field theory (QFT) in this context.

PREREQUISITES
  • Understanding of general relativity and black hole physics
  • Familiarity with quantum field theory (QFT)
  • Knowledge of electromagnetic interactions and forces
  • Basic concepts of color charge and quantum chromodynamics (QCD)
NEXT STEPS
  • Research the equations governing charged black holes, specifically the Reissner-Nordström metric
  • Study the role of virtual particles in quantum field theory and their behavior near event horizons
  • Explore the implications of color charge in black holes and its relation to quantum chromodynamics
  • Investigate the concept of exotic charges in string theory and their potential effects on black hole physics
USEFUL FOR

The discussion is beneficial for physicists, astrophysicists, and students interested in advanced topics in black hole research, quantum field theory, and the interplay between gravity and electromagnetic forces.

Dmitry67
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Hi

I have few questions about charged BH.

1 I don't understand why the equations for the charged BH are different from BH without a charge. Why the gravitation, infinitely strong at the horizon, should 'care' about such minor additional forces like the electrical attraction/repulsion. Anyway, horizon is a point of no return as singularity becomes in the future for a free falling observer, no matter if he is charged or not. Additional electric repulsion would not 'save' the falling observer at the horizon.

2 Electron is orbiting a positively charged BH. QFT describes this attraction as exchange of virtual photons. But how can they pass thru the horizon?

3 Can BH have a color charge? Why not? Say green-antigreen u or d virtual quark pairs are torn abart at the horizon. What happens next?

Thank you
 
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Dmitry67 said:
Hi

I have few questions about charged BH.

1 I don't understand why the equations for the charged BH are different from BH without a charge. Why the gravitation, infinitely strong at the horizon, should 'care' about such minor additional forces like the electrical attraction/repulsion. Anyway, horizon is a point of no return as singularity becomes in the future for a free falling observer, no matter if he is charged or not. Additional electric repulsion would not 'save' the falling observer at the horizon.

Sorry, I don't understand this.
Dmitry67 said:
2 Electron is orbiting a positively charged BH. QFT describes this attraction as exchange of virtual photons. But how can they pass thru the horizon?

Roughly, virtual photons don't have to stay on the light-cone. See

http://math.ucr.edu/home/baez/physics/Relativity/BlackHoles/black_gravity.html.
Dmitry67 said:
3 Can BH have a color charge? Why not? Say green-antigreen u or d virtual quark pairs are torn abart at the horizon. What happens next?

Thank you

I thinks it's because, unlike the electromagnetic interaction, the colour force is not long-range, but I don't know the details.

String theorists play with black holes that have "exotic" charges.
 
2 Correct, I forgot about it. Thank you
3 Well, residual strong force is short range, but the fundamental strong interaction is long range, because gluon is massless. It appears to be short range just because of the confinement, so the reason for being short range is very different from the reason why weak interaction is short range.

So I am still thinking about it.
If virtual pair is torn apart by the horizon then both BH and space outside are color-charged...
 

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