Extended Extreme Multiple Reissner Nordstrom Black holes

In summary, the conversation is about a question regarding equation 10.21 in "Exact Space-times in Einstein's General Relativity" by Griffiths and Podolski. The equation refers to the standard metric for multiple extreme Reissner Nordstrom black holes and contains the term (1+ sigma(mi/ri)). The person asking the question is wondering about a statement in the book regarding the analytically extended region inside the horizon of the black hole and how it relates to equation 10.21. They are looking for a reference to help them derive this result. Another person suggests looking at equations (10.20) and (9.21) which have a similar form and referencing a paper by Hartle and Hawking from
  • #1
keithdow
29
1
I have a question about equation 10.21 in "Exact Space-times in Einstein's General Relativity" by Griffiths and Podolski. The equation is the well know standard metric for multiple extreme Reissner Nordstrom black holes.
It has the below term:

(1+ sigma(mi/ri))

The point ri = 0 is of course the surface of the hole. My questions is the book states "The analytically extended
region inside this horizon has a metric similar to "10.21" but with a negative sign in the corresponding term in the sum, ... " They don't give a reference. Does anyone know how to I derive the above result?

Thanks.
 
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  • #2
Equations (10.20) and (9.21) have (roughly) the same form. The sentence before the sentence that includes (10.20) states "As shown by Hartle and Hawking (1972)". There is open-access to this paper at

http://projecteuclid.org/euclid.cmp/1103858037

A 1966 paper by Carter might also be useful.
 
  • #3
Thank you sir. You are correct. I am reading it now.
 

Related to Extended Extreme Multiple Reissner Nordstrom Black holes

1. What are Extended Extreme Multiple Reissner Nordstrom Black holes?

Extended Extreme Multiple Reissner Nordstrom Black holes (EEMRN Black holes) are a type of black hole in Einstein-Maxwell theory that has multiple extremal horizons. They are characterized by having multiple electric charges and angular momenta, and are considered to be the most extreme type of black hole in terms of their physical properties.

2. How do EEMRN Black holes differ from regular black holes?

EEMRN Black holes have multiple extremal horizons, whereas regular black holes only have one. This means that the mass, charge, and angular momentum of an EEMRN Black hole are distributed among its multiple horizons, rather than concentrated at a single horizon like in a regular black hole.

3. How do EEMRN Black holes form?

EEMRN Black holes can form when multiple charged particles with opposite charges (such as electrons and positrons) interact and merge together, resulting in a black hole with multiple charges. These charged particles can also have angular momentum, which adds to the angular momentum of the resulting black hole.

4. Can EEMRN Black holes exist in our universe?

While there is currently no evidence of EEMRN Black holes existing in our universe, they are theoretically possible according to Einstein-Maxwell theory. However, they would require very specific conditions to form, which may not occur naturally in our universe.

5. What is the significance of studying EEMRN Black holes?

Studying EEMRN Black holes can provide insights into the fundamental laws of physics and the behavior of extreme objects in the universe. They can also help us understand the properties of black holes in general, which can have implications for astrophysics and cosmology.

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