Two dimensional anti de Sitter space without cosmological constant?

In summary, the conversation revolves around the calculation of the Einstein tensor for a spacetime which is possibly AdS_2. The result of zero for the Einstein tensor causes confusion and prompts further investigation using different software packages. Eventually, it is discovered that the Einstein tensor vanishes in 2D gravity due to its definition, which is counterintuitive but confirmed by references from books. In the end, it is acknowledged that there is always something new to learn in the field of theoretical and mathematical physics.
  • #1
implicitnone
19
0
I have a spacetime which is (I think) AdS_2. The metric is,

whiixw.png


I'm trying to find the Einstein tensor, defined as,

c774f25c5cd752b2805b84a67ce9ac98.png


and the result is zero! I thought that, for the AdS spacetimes I needed to have a nonzero Einstein tensor which is caused by the cosmological constant.

What is wrong with my calculation? Or can you assure me that my result is correct and this metric is not AdS?

I'm using GRTensorII to do the calculations.
 
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  • #2
hey check your calculations...I tried calculating it manually and I got a non-zero Einstein tensor. I got it as a diagonal matrix.
 
  • #3
aashay said:
hey check your calculations...I tried calculating it manually and I got a non-zero Einstein tensor. I got it as a diagonal matrix.

Thank you for your efforts. I will do so. It will be the first time that grtensor confused me.
 
  • #4
You are welcome..By the way, what is 'grtensor'?Is it some kind of software?
 
  • #5
aashay said:
You are welcome..By the way, what is 'grtensor'?Is it some kind of software?

GRTensorII is a Maple package for tensor and GR calculations:

http://grtensor.org/
 
  • #6
Very weird but I also tried with two other ways with computer. The internal packages of Maple and EinsteinTensor package of Mathematica library. They both gave zero Enstein tensor again!
 
  • #7
I checked using Maxima and ctensor, and I verified that the Einstein tensor was zero:
Code:
load(ctensor);
dim:2;
ct_coords:[t,x];
lg:matrix([-(1+x^2),0],
          [0,1/(1+x^2)]);
cmetric();
einstein(true);
Maxima and ctensor are free and open-source, so anyone who wants to check this and play around with it can do so. E.g., if aashay has calculated the Riemann tensor, he/she could change the code so that it would output that, and we could compare and see if they're the same.

I would assume that spacetime curvature has a very simple characterization in 1+1 dimensions, e.g., there can only be one nonvanishing element in the Riemann tensor.
 
  • #8
Thank you very much bcrowell!

Learning never ends :) It was my first deal with 1+1 gravity and now I checked with some books and saw that the Einstein tensor identically vanishes in 2D gravity because of the definition.

(See for example: "Lower dimensional gravity" by John David Brown or "Diverse topics in theoretical and mathematical physics" by Roman Jackiw. They are both available as Google books.)
 
  • #9
implicitnone said:
Learning never ends :) It was my first deal with 1+1 gravity and now I checked with some books and saw that the Einstein tensor identically vanishes in 2D gravity because of the definition.

Ah, that's interesting. Kind of counterintuitive, since you *can* have intrinsic curvature in two spatial dimensions.
 
  • #10
bcrowell said:
Ah, that's interesting. Kind of counterintuitive, since you *can* have intrinsic curvature in two spatial dimensions.

It really is! Knowing that I can still count on GRTensorII feels good :)
 

FAQ: Two dimensional anti de Sitter space without cosmological constant?

What is two dimensional anti de Sitter space without cosmological constant?

Two dimensional anti de Sitter space without cosmological constant is a mathematical concept in theoretical physics that describes a two-dimensional space with a negative curvature. It is a simplified version of the full anti de Sitter space, a solution to Einstein's field equations in general relativity.

How does two dimensional anti de Sitter space without cosmological constant differ from the full anti de Sitter space?

The main difference between the two is the absence of a cosmological constant in the two-dimensional version. This means that the space has no intrinsic curvature and is locally flat, while the full anti de Sitter space has a negative cosmological constant and thus has a negative curvature.

What are the applications of two dimensional anti de Sitter space without cosmological constant?

Two dimensional anti de Sitter space without cosmological constant is mainly used as a theoretical tool to study the properties of anti de Sitter space and its relation to other areas of physics, such as string theory and holography. It also has applications in quantum gravity and black hole physics.

How is two dimensional anti de Sitter space without cosmological constant related to holography?

Two dimensional anti de Sitter space without cosmological constant is closely related to the holographic principle, which states that the information of a system can be fully described by a theory living on the boundary of that system. In the case of two-dimensional anti de Sitter space, the theory on the boundary can be described by a conformal field theory, providing a powerful tool for studying the properties of anti de Sitter space.

What are some open questions or challenges regarding two dimensional anti de Sitter space without cosmological constant?

Some open questions include the precise relationship between two-dimensional anti de Sitter space and other areas of physics, such as string theory and holography. Additionally, there are ongoing efforts to better understand the properties and dynamics of black holes in this space, as well as further exploring its implications for quantum gravity.

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