Complex metric solutions in GR

In summary, the conversation discussed the possibility of interpreting complex solutions in general relativity. The Newman-Penrose formalism was mentioned as a method for obtaining rotating black holes from stationary solutions. The NUT parameter was also brought up as a way to transform mass into NUT and vice versa. It was noted that the Newman-Janis "trick" for going from Schwarzschild to Kerr uses the Newman-Penrose formalism. Finally, a resource on the Newman-Penrose approach to twisting degenerate metrics was shared.
  • #1
haushofer
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A friend of mine had the following funny question:

Imagine I have a metric ansatz with two unknown functions. The Einstein equations give both real and complex solutions for the unknown functions.

Question: Is there a decent interpretation of these complex solutions in GR?

We know about this Newman-Janis formalism in which one uses a complex metric ansatz in order to obtain rotating black holes from stationary solutions, but this is a more general situation.

Any suggestions are appreciated :)
 
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  • #3
I know about complex geometry; I was just wondering if these solutions also can be interpreted in conventional GR :)
 
  • #4
Not the Newman-Janis formalism, it's called the Newman-Penrose formalism. Well if you don't want a complex geometry then you have to get back to a real one somehow. Newman and Penrose use a complex tetrad and complex spin coefficients but wind up taking real and imaginary parts.

The NUT parameter is like an imaginary mass, and you can transform mass into NUT and vice versa by doing the gravitational analog of a duality rotation. This can be applied to more general solutions than just Kerr.
 
  • #5
Bill_K said:
Not the Newman-Janis formalism, it's called the Newman-Penrose formalism.

The Newman-Janis "trick" for going from Schwarzschild to Kerr uses the Newman-Penrose formalism.
 
  • #6
The Newman-Janis "trick" for going from Schwarzschild to Kerr uses the Newman-Penrose formalism.
Indeed it does.
 

1. What is General Relativity (GR)?

General Relativity (GR) is a theory of gravity developed by Albert Einstein in the early 20th century. It describes the physical laws governing the behavior of matter and energy in the presence of massive objects, such as planets, stars, and galaxies. GR is based on the idea that gravity is not a force, but rather a curvature of spacetime caused by the presence of mass and energy.

2. What are complex metric solutions in GR?

In GR, the metric is a mathematical object that describes the curvature of spacetime. A complex metric solution is a solution to the equations of GR that involves complex numbers. This means that spacetime is described by a complex-valued metric, which represents a more general and complex geometry than the real-valued metric solutions usually studied in GR.

3. Why are complex metric solutions important?

Complex metric solutions in GR can provide insights into the behavior of spacetime in extreme situations, such as near black holes or during the early universe. They can also help us understand the role of complex numbers in fundamental physical theories and may have implications for quantum gravity.

4. How are complex metric solutions studied?

Complex metric solutions are typically studied using mathematical techniques, such as numerical simulations and perturbation theory. These methods allow us to analyze the behavior of complex metric solutions and compare them to real-valued solutions to gain a better understanding of the underlying physics.

5. What are some examples of complex metric solutions in GR?

One example of a complex metric solution is the Kerr-Newman metric, which describes the spacetime around a rotating charged black hole. Another example is the G\"odel metric, which represents a rotating universe filled with matter and radiation. Other examples include the Taub-NUT metric, the Schwarzschild metric in complex coordinates, and the complexified Friedmann-Lema\^itre-Robertson-Walker (FLRW) metric.

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