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

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Find the Riemann tensor of the 2-sphere of radius r

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

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


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 g_{\mu \nu}. 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.
 
There are two things I don't understand about this problem. First, when finding the nth root of a number, there should in theory be n solutions. However, the formula produces n+1 roots. Here is how. The first root is simply ##\left(r\right)^{\left(\frac{1}{n}\right)}##. Then you multiply this first root by n additional expressions given by the formula, as you go through k=0,1,...n-1. So you end up with n+1 roots, which cannot be correct. Let me illustrate what I mean. For this...
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