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9.17.3. Theorem.
(The Fundamental Lemma of Riemannian Geometry) A
Riemannian manifold
M
n
possesses a unique symmetric connection that is com-
patible with its metric. This connection is called the
Levi-Civita connection
for the
metric.
Proof.
See [Spiv75] or [MilP77]. The Christoffel symbols defined above are the same
as the Christoffel symbols defined in Section 9.9 for this connection.
Definition.
Let
X
,
Y
,
Z
Œ Vect(
M
). The vector field R(
X
,
Y
)
Z
defined by
(
)
(
)
+—
(
)
+—
[
R
XYZ
,
=-—
Z
Z
Z
]
XY
YX
XY
,
is called the
curvature tensor
of the connection.
The key to Riemannian geometry is an analysis of the curvature tensor. (Tensors
were briefly alluded to in Section 4.9 and are a whole other large topic in differential
geometry and physics.) For example,
9.17.4. Theorem.
If
M
n
is a Riemannian manifold, then the curvature tensor R for
the Levi-Civita connection on
M
n
is 0 if and only if
M
n
is locally isometric to
R
n
with
its usual Riemannian metric.
Proof.
See [Spiv75].
It must be pointed out that Theorem 9.17.4 is a local theorem because there are
manifolds that are
locally
isometric to
R
n
but are not homeomorphic to
R
n
. See
[Spiv75].
Here is another way that one can see the geometry that is embedded in the concept
of the curvature tensor. The latter is really defined by lower-dimensional concepts that
are easier to understand. Let
M
n
be a Riemannian manifold with curvature tensor R.
Let
p
Œ
M
and let
V
be a two-dimensional subspace of the tangent space T
p
(
M
). It turns
out that the geodesics in a neighborhood of
p
that pass through
p
and are tangent
to
V
at
p
actually define a piece of a surface
S
through
p
that is uniquely defined by
V
.
The surface
S
has a Riemannian structure induced by the structure on
M
.
Definition.
The Gauss curvature of
S
at
p
is called the
sectional curvature
of
M
at
p
along
V
and is denoted by K(
p
,
V
).
9.17.5. Theorem.
With the notation and hypotheses leading up to the definition of
sectional curvature, let
X
and
Y
be vectors in T
p
(
M
) that span
V
. Then
(
)
<
R
XYYX
,
,
>
(
)
=
K
pV
,
,
A
where A is the area of the parallelogram spanned by
X
and
Y
.
Proof.
See [Spiv75].