3.1. Normal coordinates for an embedded submanifold
We start our discussion by introducing the basic notions of the normal exponential map and normal coordinates with respect to an embedded submanifold.
This part seems to be standard in Riemannian geometry. For the consistence of the notations and the completeness of the paper, here we include detailed
discussions and proofs.
Let be an oriented Riemannian manifold of dimension and let be a closed embedded oriented submanifold of codimension in .
In our later applications, we only need the case .
Denote by the normal bundle of in , equipped with the induced fiberwise Riemannian inner products. For any , denotes the fiber of in .
The normal exponential map of in is defined as
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where is the standard exponential map at .
By standard implicit function theorem, it is straightforward that is a diffeomorphism from some neighborhood of the zero section of to some tubular neighborhood of in .
Now we define the normal coordinates.
Fix . First we choose local coordinates in a small neighborhood of such that
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at . We also assume that is compatible with the orientation on .
Next, we pick local orthonormal sections of the normal bundle
such that
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on . Again we assume that is compatible with the orientation on , i.e. is compatible with the orientation on . Then we can find such that restricts to a diffeomorphism from
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to a neighborhood of . In particular, .
Definition 3.1 (Normal coordinates).
For any with , the local normal coordinates are defined as follows
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By definition for each fixed point in , the curve
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is a normal geodesic which is orthogonal to .
Let
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be the induced coordinate vector fields. Then when both are viewed as sections of over .
For
and , we denote
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By definition, we have
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for all .
The second fundamental form of the embedding can be written as , where
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Denote by the mean curvature vector, then
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In the above coordinates,
we define the normal distance function
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A straightforward extension of the usual Gauss Lemma gives the following and we omit the proof.
Lemma 3.2 (Generalized Gauss Lemma).
For any , there is some sufficiently small neighborhood of and a tubular neighborhood with such that the function defined by (3.12) satisfies the following properties:
- (1)
holds in . In particular, is the normal distance function
in , i.e., for all .
- (2)
is orthogonal to ’s in , and hence
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For the convenience of later discussion, we introduce several notations concerning the normal regularity order near the submanifold . It will be frequently used throughout the paper.
Definition 3.3 (Normal regularity order).
Let be a tensor locally defined in which is on , then for a non-negative integer we say as
- (1)
if for each
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for all multi-indices and .
In particular, if , then for all .
- (2)
if .
- (3)
if and
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In other words, is smooth in
and has vanishing normal derivatives along up to order .
Notice that the defining condition does not depend on the choice of the local coordinates, since if we have another coordinate system , then we have
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and . Similarly, we can also use any local coordinate system such that along for .
Lemma 3.4.
In the above normal coordinates, we have the following expansions of the metric tensor of along the normal directions,
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where denotes the restriction of the metric to , denotes the Riemann curvature tensor of .
Proof.
The above expansions can be proved using the Jacobi fields. Fix a point , we we choose a unit vector with . Let be the following radial geodesic in ,
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such that . In the normal coordinates, the geodesic can represented as
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For each and , we define the geodesic variations
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Then variation fields of and give
the following Jacobi fields along the radial geodesic respectively:
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By definition,
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Taking first derivatives at ,
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Then applying the Jacobi equation along the geodesic ,
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where denotes the Riemann curvature tensor of , so it follows that
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Therefore,
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Let , then we obtain the desired expansions.
∎
As a digression we briefly discuss the intrinsic meaning of the above expansion. The point is that locally the Riemannian metric is approximated by a Riemannian metric on the normal bundle up to the first order. Notice we have the natural projection and is a Riemannian vector bundle together with an induced “normal” connection, given by the normal component of the Levi-Civita connection of . The latter hence gives rise to a distribution of horizontal subspaces at each point of , which in our coordinates is spanned by , where
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is a smooth function on .
We define so that at each point of , the vertical and horizontal subspaces are orthogonal and on the vertical part is given by the bundle metric on , and on the horizontal part is given by the perturbation of the base metric using the second fundamental form. In this way we get a coordinate free description of the above expansion up to the first order.
We also define
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Then the curvature of the normal connection is given by
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