Calculating Riemann Tensor for S^2 with Pull-Back Metric from Euclidean Space

In summary, the Riemann tensor of the 2-sphere of radius r can be found by rewriting the metric in spherical coordinates and identifying the g_{\mu \nu} components. Then, using the definition of the Riemann tensor in terms of the Christoffel symbols, it can be calculated by hand. This may take some time, but it is not a difficult task.
  • #1
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Find the Riemann tensor of the 2-sphere of radius r

S[tex]^{2}_{r}[/tex]={(x,y,z) [tex]\in[/tex][tex]\Re^{3}[/tex]|x[tex]^{2}[/tex] + y[tex]^{2}[/tex] + z[tex]^{2}[/tex] = r[tex]^{2}[/tex]}

with metric g obtained as the pull-back of the Euclidean metric gR3 by the inclusion
map S[tex]^{2}[/tex] [tex]\hookrightarrow[/tex][tex]\Re^{3}[/tex].


Any help would be appreciated. Thanks
 
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  • #2
This seems to be a pretty straight forward problem. Rewrite your metric in spherical coordinates. Identify your [itex] g_{\mu \nu} [/itex]. Go to a book on General Relativity and find the definition of the Riemann tensor in terms of the Christoffel symbols and calculate it out. It will take a little time, but it's not hard.
 

1. What is a Riemann metric?

A Riemann metric, also known as a Riemannian metric, is a mathematical concept used in differential geometry to measure distances and angles on a smooth, curved surface.

2. How is a Riemann metric different from a Euclidean metric?

A Riemann metric takes into account the curvature of a surface, while a Euclidean metric assumes a flat, straight surface. This means that the measurements and calculations using a Riemann metric will differ from those using a Euclidean metric on a curved surface.

3. What is the importance of the Riemann metric in physics?

The Riemann metric is essential in the field of general relativity, where it is used to describe the curvature of spacetime and the gravitational force. It also plays a role in other areas of physics, such as electromagnetism and quantum mechanics.

4. How is the Riemann metric calculated?

The Riemann metric is calculated using a mathematical formula that takes into account the local properties of a surface, such as its curvature and orientation. It involves the use of tensors, which are mathematical objects that represent the properties of a surface at a specific point.

5. Can the Riemann metric be generalized to higher dimensions?

Yes, the concept of a Riemann metric can be extended to higher dimensions, such as four-dimensional spacetime in general relativity. This allows for the measurement of distances and angles on more complex surfaces, such as those with multiple curves and folds.

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