Event and Cauchy horizons for a charged black hole

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Discussion Overview

The discussion centers on the Reissner-Nordstrom metric for charged black holes, specifically focusing on the definitions and implications of the event horizon (##r_{+}##) and the Cauchy horizon (##r_{-}##). Participants explore the conditions under which these horizons exist and the consequences of exceeding certain parameters, such as the charge-to-mass ratio.

Discussion Character

  • Technical explanation, Debate/contested

Main Points Raised

  • One participant presents the Reissner-Nordstrom metric and defines the event and Cauchy horizons based on the roots of the function ##f(r)##.
  • Another participant questions the definitions of the horizons, suggesting that they are simply accepted terms without deeper explanation.
  • Concerns are raised about the scenario where the charge exceeds the mass (##|Q| > M##), indicating that this leads to the absence of both horizons and results in a naked singularity.
  • Some participants note that the existence of naked singularities is generally viewed as physically unreasonable, while others reference examples that challenge this view.
  • A later reply emphasizes that the term "reasonable" in the context of mathematical models does not imply empirical support for the existence of naked singularities.

Areas of Agreement / Disagreement

Participants express differing views on the physical reasonableness of naked singularities and the implications of the charge-to-mass ratio, indicating that multiple competing perspectives remain unresolved.

Contextual Notes

The discussion includes assumptions about the physical interpretations of mathematical models and the conditions under which horizons exist, which are not fully explored or agreed upon.

Afonso Campos
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Consider the Reissner-Nordstrom metric for a black hole:

$$ds^{2} = - f(r)dt^{2} + \frac{dr^{2}}{f(r)} + r^{2}d\Omega_{2}^{2},$$

where

$$f(r) = 1-\frac{2M}{r}+\frac{Q^{2}}{r^{2}}.$$

We can write

$$f(r) = \frac{1}{r^{2}}(r-r_{+})(r-r_{-}), \qquad r_{\pm} = M \pm \sqrt{M^{2}-Q^{2}}.$$

Then ##r_{+}## is called the event horizon and ##r_{-}## is called the Cauchy horizon.

Why is ##r_{+}## called the event horizon and why is ##r_{-}## called the Cauchy horizon?
 
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Things don't look like they end well for ##|Q| > M##?
 
Paul Colby said:
Things don't look like they end well for |Q|>M|Q| > M?

In that case there is no event horizon or Cauchy horizon, just a naked singularity. Most physicists appear to consider that case as not being physically reasonable.
 
PeterDonis said:
Most physicists appear to consider that case as not being physically reasonable.

There are some reasonable examples of naked singularities though: https://arxiv.org/abs/1006.5960
 
Afonso Campos said:
There are some reasonable examples of naked singularities

"Reasonable" does not mean "I have a mathematical model". "Reasonable" means "I have reason to believe this mathematical model describes something that exists in our actual universe". The paper you cite gives no reason to believe that.
 

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