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

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SUMMARY

The discussion focuses on calculating the Riemann tensor for the 2-sphere \( S^{2}_{r} \) of radius \( r \) using the pull-back metric from Euclidean space \( \mathbb{R}^{3} \). The metric \( g \) is derived from the inclusion map \( S^{2} \hookrightarrow \mathbb{R}^{3} \). Participants emphasize rewriting the metric in spherical coordinates and identifying the components \( g_{\mu \nu} \). The calculation of the Riemann tensor involves using the definition based on Christoffel symbols, as found in standard General Relativity texts.

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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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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.
 

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