Black Hole Radiation: Questions Clarified

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Discussion Overview

The discussion revolves around the nature of black hole radiation, specifically focusing on the mechanics of gravitational pull near the event horizon and the concept of virtual pair production leading to Hawking radiation. Participants seek clarification on how these phenomena interact and the implications for energy and mass in black holes.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants propose that objects outside the event horizon feel an increasing gravitational pull as they approach it, but the effects may not be significant until crossing the horizon.
  • There is a discussion about virtual pair production occurring at or near the event horizon, with some participants questioning how this process leads to a loss of energy for the black hole.
  • One participant suggests that the escaping particle from a virtual pair has positive energy while the one falling into the black hole has negative energy, thus reducing the black hole's overall mass/energy.
  • Another participant expresses skepticism about the heuristic explanations provided, advocating for more intuitive or simplified explanations that do not rely heavily on complex mathematics.
  • There are mentions of the behavior of black holes when they consume matter and the implications of their gravitational fields on nearby objects, including the potential for particles to escape at high velocities.
  • One participant explores the idea of a black hole's interior potentially resembling environments outside of it, raising questions about the nature of gravity and mass within such extreme conditions.

Areas of Agreement / Disagreement

Participants express differing views on the mechanics of black hole radiation and the implications of virtual pair production. There is no consensus on the explanations provided, and the discussion remains unresolved with multiple competing perspectives.

Contextual Notes

Some participants highlight the limitations of heuristic explanations and the challenges in conveying complex concepts without advanced mathematics. The discussion reflects ongoing uncertainties regarding the nature of energy loss in black holes and the behavior of particles near the event horizon.

  • #31
Outhouse said:
I use that line all the time, but in this case, not sure why many/we even define a black hole as containing a singularity.
We don't, strictly speaking. We say that GR models a black hole as containing a singularity, but we have reason to believe that this means that GR goes wrong somewhere along the way.
 
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  • #32
Outhouse said:
I use that line all the time, but in this case, not sure why many/we even define a black hole as containing a singularity.
Our mathematical description of a black hole has a feature which we term a "singularity". To say that this means that a black hole "contains" a singularity is, perhaps, an abuse of terminology, but it is a common abuse.
 
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  • #33
timmdeeg said:
How strong does the latter weaken the consistency argument

It is true that having a single self-consistent theory that accounts for all known experimental data carries weight; having one theory that has GR and our current quantum field theory as special cases--approximations valid under particular conditions--would be better, by some criteria, than just having the two separate theories, even if there were no experimental data that could not be accounted for by one of the two separate theories. But I don't know how you would quantify this.

timmdeeg said:
are there cases known in the past that a physical problem seemed to be solved from a mathematical point of view which however has turned out later to be wrong?

Sure. Newtonian mechanics. It accounted for all the known experimental data when it was formulated, and for at least a century afterwards, and it unified at least two domains--falling bodies on Earth and motions of the Sun, planets, and Moon--that were previously covered by separate theories (roughly speaking, the mechanics implied by Galileo's experiments with inclined planes, and Kepler's model of the solar system), without any new experimental data that could not be accounted for by one of those two theories. But Newton's model was a clear unification of all that was known at that time about mechanics--yet, as we now know, it is not correct, it's just an approximation valid in a particular regime.
 
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  • #34
PeterDonis said:
It is true that having a single self-consistent theory that accounts for all known experimental data carries weight; having one theory that has GR and our current quantum field theory as special cases--approximations valid under particular conditions--would be better, by some criteria, than just having the two separate theories, even if there were no experimental data that could not be accounted for by one of the two separate theories. But I don't know how you would quantify this.
Perhaps it depends on how the singularity problem can be solved. Perhaps it might be even more convincing if it could be shown that gravity is an emergent phenomenon which reproduces General Relativity. Or do you think that it is quite compelling that QFT should be a special case?
PeterDonis said:
Sure. Newtonian mechanics.
Ah yes. Whereby fortunately in this case the range of validity could investigated experimentally.

Thank you for your comments!

EDIT I'm realizing "perhaps" is just speculation, so please ignore it.
 
Last edited:
  • #35
PeterDonis said:
Where? Please give a reference.
Sorry, can't remember or find it again. It was years before.
 

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