Event and Cauchy horizons for a charged black hole

In summary, the Reissner-Nordstrom metric describes the geometry of a black hole and includes two parameters, ##r_+## and ##r_-##, which are known as the event horizon and Cauchy horizon respectively. These are important features of a black hole and have specific definitions in terms of the metric. In cases where the charge parameter ##Q## is greater than the mass parameter ##M##, there is no event horizon or Cauchy horizon, resulting in a naked singularity. However, this is not considered to be physically reasonable.
  • #1
Afonso Campos
29
0
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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  • #3
Things don't look like they end well for ##|Q| > M##?
 
  • #4
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.
 
  • #5
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
 
  • #6
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.
 

1. What is an event horizon for a charged black hole?

An event horizon for a charged black hole is a boundary in space-time beyond which no information or light can escape. It is formed when the gravitational pull of the black hole is strong enough to prevent anything from escaping, including light.

2. How is the event horizon of a charged black hole different from a regular black hole?

The event horizon of a charged black hole is different from a regular black hole because it is affected by the electric charge of the black hole. This charge can influence the shape and size of the event horizon, and also affects the behavior of matter and radiation near the black hole.

3. What is a Cauchy horizon for a charged black hole?

A Cauchy horizon for a charged black hole is a boundary in space-time beyond which the future of the black hole cannot be predicted. It is formed when the black hole's electric charge is strong enough to distort the space-time around it, making it impossible to accurately predict what will happen inside the black hole.

4. Can a charged black hole have multiple event or Cauchy horizons?

Yes, a charged black hole can have multiple event and Cauchy horizons depending on its electric charge and other properties. These horizons can also change over time as the black hole evolves.

5. How do event and Cauchy horizons affect the behavior of matter and radiation near a charged black hole?

The event and Cauchy horizons of a charged black hole can influence the behavior of matter and radiation near the black hole by distorting space-time and creating strong gravitational forces. These horizons can also affect the paths of particles and light, making it difficult to observe and study the black hole's properties.

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