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Exact Solutions and Scalar Fields in Gravity - Instituto Avanzado de ...

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On maximally symmetric <strong>and</strong> totally geo<strong>de</strong>sic spaces 29<br />

4. REPRESENTATION OF MAXIMALLY<br />

SYMMETRIC SPACES<br />

In general, one may pose the question if there exists a system of<br />

coord<strong>in</strong>ates <strong>in</strong> a space of constant curvature such that the metric is of<br />

the form<br />

where C is a diagonal matrix with non–zero diagonal elements<br />

for <strong>de</strong>pend<strong>in</strong>g upon the signature.<br />

The substitution <strong>in</strong> the Riemann tensor yields<br />

<strong>in</strong> the right h<strong>and</strong> si<strong>de</strong> there is no summation neither <strong>in</strong> nor <strong>in</strong><br />

From the first equations one arrives at<br />

where <strong>de</strong>pend only on their arguments. Substitut<strong>in</strong>g <strong>in</strong> the<br />

second equations one obta<strong>in</strong>s<br />

where is no summation <strong>in</strong> The constants <strong>and</strong> are arbitrary,<br />

<strong>and</strong> the constant curvature K occurs to be related with them through<br />

Hence, one can give various alternative representations of the metric<br />

of the studied space. In particular, the Riemman form arises when<br />

is different from zero; accomplish<strong>in</strong>g first a shift<strong>in</strong>g of the<br />

followed by scal<strong>in</strong>g transformations<br />

one arrives at the Riemann form<br />

Representation as embedd<strong>in</strong>g <strong>in</strong> a<br />

Let us consi<strong>de</strong>r the metric (26) given as

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