Hard General Relativity question, help ?

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Homework Help Overview

The discussion revolves around computing the Kretschmann curvature scalar for various solutions of Einstein's equations in the context of General Relativity. The original poster presents two questions: the first involves calculating the Kretschmann scalar for the Schwarzschild exterior and interior solutions, as well as the Friedman-LeMaitre-Robertson-Walker solution; the second asks about the conditions and nature of singularities in these cases.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the necessity of defining the Kretschmann scalar and suggest starting with its definition. There is mention of using computational tools like Maple and GRTensorII to assist in the calculations, while also emphasizing the importance of understanding the manual computation process.

Discussion Status

The conversation is ongoing, with participants providing guidance on computational tools and stressing the importance of manual calculations. There is no explicit consensus on a specific approach, but several lines of reasoning and methods are being explored.

Contextual Notes

Participants note the forum policy requiring evidence of attempts before receiving assistance, which influences the nature of the discussion. There is also mention of the potential for singularities in the solutions discussed, though specifics are not yet detailed.

hamjam9
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Hard General Relativity question, help :(!?

I cannot come up with a solution to the following, can some one please help me? I would greatly apprecieate it! Thank you!

Question 1

The Kretschmann curvature scalar is defined to be K = R_abcdR^abcd where Rabcd is the Riemann tensor. Compute the Kretschmann scalar for each of the following solutions of Einstein’s equtions:
(a) Schwarzschild exterior (vacuum) solution
(b) Schwarzschild interior (constant density) solution
(c) Friedman-LeMaitre-Robertson-Walker solution

In each case, express the Kretschmann scalar both in terms of the quantities occurring in the metric tensor, and in terms of the physical quantities that occur in the energy-momentum tensor, where possible.

Question 2

Describe the conditions under which a singularity exists, and the nature of the singularity for each of the solutions that you considered in problem 1 for the Kretschmann scalar. Ensure that you describe the appropriate physics in each case. Where possible, relate your conclusions to conclusions reached by other lines of argument for these metrics.
 
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What have you tried? You must show some attempt n order to get assistance here; it is forum policy.

A good place to start would be to use the definition of 'Kretschmann scalar'.
 


Gabba is right. It seems like it should be a straight forward matter of defining the K-scalar, and plugging everything in. I'm not saying that it won't take many hours to do this, and you'll probably make a few index errors along the way, but it is straight-forward. If you have Maple, you can download and install the GRTensorII package for free. Take a couple hours to learn to use GRTensorII. Then you'll be able to do this question in about five minutes. Also, the rest of your course will be much easier once you know GRTensorII because these sort of "turn the crank" questions are handled in milliseconds by GRTensorII. And IT doesn't make mistakes (I love computers and hate 'em at the same time).
Of course, it is best that you convince yourself that you COULD do the computation by hand if you had to before you put your faith in a computer program.
 


Pacopag said:
Of course, it is best that you convince yourself that you COULD do the computation by hand if you had to before you put your faith in a computer program.

Exactly: what's he going to do in an exam when Maple isn't there?
 


Ya. That's what I meant. I never use maple for anything that I'm not sure that I COULD do by hand if I had to. Or better yet, DO it by hand, then use maple to check your answer.
 


PS: There will be a new general relativity package in upcoming versions of Maple. It will be located in the Differential Geometry package. Keep your eyes open for it...

and incidentally, you don't have to download anything new, just go to the DG package in Maple. You can compute curvature tensors, Einstein tensors, etc. right there. Just my suggestion.
 

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