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Lecture Notes for 120 - UCLA Department of Mathematics

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8.2. RIEMANNIAN GEOMETRY 171<br />

This expression shows how certain third order partials might not commute since<br />

we have<br />

2 3<br />

@ 3 q<br />

@u i @u j @u k<br />

@ 3 q<br />

@u j @u i @u k = ⇥<br />

@q<br />

@u 1 ···<br />

@q<br />

@u n<br />

⇤ 6<br />

4<br />

But recall that since second order partials do commute we have<br />

@ 3 q<br />

@u i @u j @u k = @ 3 q<br />

@u i @u k @u j<br />

So we see that third order partials commute if and only if the Riemann curvature<br />

vanishes. This can be used to establish the difficult existence part <strong>of</strong> the next result.<br />

R 1 ijk<br />

.<br />

R n ijk<br />

Theorem 8.2.1. [Riemann] The Riemann curvature vanishes if and only if<br />

there are Cartesian coordinates around any point.<br />

Pro<strong>of</strong>. The easy direction is to assume that Cartesian coordinates exist. Certainly<br />

this shows that the curvatures vanish when we use Cartesian coordinates, but<br />

this does not guarantee that they also vanish in some arbitrary coordinate system.<br />

For that we need to figure out how the curvature terms change when we change<br />

coordinates. A long tedious calculation shows that if the new coordinates are called<br />

v i and the curvature in these coordinates ˜R l ijk , then<br />

˜R ijk l = @u↵ @u @u @v l<br />

@v i @v j @v k @u R ↵ .<br />

Thus we see that if the all curvatures vanish in one coordinate system, then they<br />

vanish in all coordinate systems.<br />

Conversely, to find Cartesian coordinates set up a system <strong>of</strong> differential equations<br />

@q<br />

@u i = U i<br />

@ ⇥ ⇤<br />

U1 ··· U<br />

@u i n = ⇥ ⇤<br />

U 1 ··· U n [ i]<br />

whose integrability conditions are a consequence <strong>of</strong> having vanishing curvature. ⇤<br />

7<br />

5

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