nLab
Myers-Steenrod theorem

Contents

Idea

Recall that an isometry between two Riemannian manifolds (M,g),(N,h) is a diffeomorphism ϕ:MN such that ϕ *h=g. In other words, ϕ respects the Riemannian structure as well as the differentiable structure.

It follows that if d,d are the metrics on M,N induced by the Riemannian metrics g,h, then d(ϕ(x),ϕ(y))=d(x,y) for x,yM—that is, ϕ is distance-preserving. Interestingly, a version of the converse is true, according to the Myers–Steenrod theorem:

Theorem (Myers–Steenrod)

If ϕ:MN is distance-preserving and surjective, then it is an isometry (in particular, it is smooth).

For notational simplicity, assume N=M.

ϕ is evidently a homeomorphism. Now pick pM and a neighborhood D r(p) such that for any qD r(p), there is a unique geodesic in that neighborhood connecting p,q. Call it γ. I claim that ϕγ is a geodesic in N.

The geodesic γ can be assumed to be parametrized by unit length. We have for all t,

(1)d(p,q)=d(γ(t),p)+d(γ(t),q).d(p,q) = d(\gamma(t),p) + d(\gamma(t), q).

Thus

(2)d(ϕ(p),ϕ(q))=d(ϕ(γ(t)),ϕ(p))+d(ϕ(γ(t)),ϕ(q)).d(\phi(p),\phi(q)) = d(\phi(\gamma(t)),\phi(p)) + d(\phi(\gamma(t)), \phi(q)) .

In other words, we have strict equality in the triangle inequality.

Geodesic preservation

In a Riemannian manifold M, if q,r lie in a small neighborhood of p and

(3)d(q,r)+d(r,p)=d(q,p),d(q,r) + d(r,p) = d(q,p) ,

then r lies on a geodesic betwen p,q.
Indeed, draw a geodesic α from q to r and a geodesic β from r to p that travel at unit speed and minimze the distances; we can do this locally even without the assumption of completeness. The catenation αβ minimizes the length from q to p, so it is an unbroken geodesic. Thus r lies on the geodesic.

So, returning to the discussion above, we see that by (2) ϕ sends geodesics to geodesics.

Exponential coordinates

Now fix open UT p(M),VT q(N) containing the origin such that exp p takes U diffeomorphically to a neighborhood D r(p), and exp q takes V diffeomorphically to D r(q). There is an expression for ϕ as a map ϕ˜:UV in these exponential coordinates.
It is obtained as follows: if vU, take a geodesic γ v with γ v(0)=v and consider (ϕγ v)(0). In fact this induces more generally a map

(4)ϕ˜:T p(M)T q(M).\tilde{\phi}: T_p(M) \to T_q(M).

Since γ v moves at constant speed v and ϕγ v moves at the same speed, it follows that ϕ˜ is norm-preserving. Also ϕ˜(0)=0. If we can show that ϕ˜ is linear, then we’ll get smoothness in this exponential coordinate system—hence smoothness in general.

ϕ˜ is an isometry

It can be checked that

(5)lim A,B0T p(M)d(exp p(A),exp p(B))AB=1.\boxed{\lim_{A,B \to 0 \in T_p(M)} \frac{d(\exp_p(A),\exp_p(B)) }{|A-B|} } = 1.

We will postpone this for now.

This is what we will use to show that ϕ˜:T p(M)T q(M) is an isometry, where each tangent space is given the norm from the Riemannian metric. Pick A,BT p(M) and consider the geodesics γ A,γ B at p and γ A,γ B where A=ϕ˜(A),B=ϕ˜(B). Then d(γ A(t),γ B(t))=d(γ A(t),γ B(t)). So

(6)1=lim t0d(exp p(tA),exp p(tB))tAB=lim t0d(exp q(tA),exp q(tB))tAB=ABAB.1= \lim_{t \to 0} \frac{d(\exp_p(t A),\exp_p(t B)) }{t|A-B|} = \lim_{t \to 0} \frac{d(\exp_q(t A'),\exp_q(t B')) }{t|A-B|} = \frac{|A'-B'|}{|A-B|}.

To show that ϕ˜ is linear, we appeal to a general fact:

Let X,Y be normed linear spaces and T:XY a map such that TxTx=xx for x,xX. Then T is linear if T(0)=0.

Conclusion of the proof

Now we have seen that ϕ is smooth, and that for vT p(M), v p=ϕ *(v) ϕ(p), i.e. ϕ preserves lengths on tangent vectors. By the polarization identity, ϕ preserves the inner product, and is thus an isometry.

A lemma

We never proved a fact about the exponential map—the equality

(7)lim A,B0T p(M)d(exp p(A),exp p(B))AB=1.\lim_{A,B \to 0 \in T_p(M)} \frac{d(\exp_p(A),\exp_p(B)) }{|A-B|} = 1.

We will briefly sketch the idea here. AB is the length of the linear path from A to B in T p(M), so it will be sufficient to show:

Lemma

If c:(0,1)T p(M) is a path in T p(M), then as c((0,1))0 with the derivative c staying bounded,

(8)l(exp p(c))l(c)=1.\frac{ l(\exp_p(c))}{l(c)} = 1.

We are abusing notation quite a bit here, but it should not cause confusion.

The reason is that

(9)l(c)=cl(c) = \int |c'|

while

(10)l(exp p(c))=(exp p) *c(t)c(t) exp p(c(t))l(\exp_p(c)) = \int | (\exp_p)_{*c(t)} c'(t) |_{\exp_p(c(t))}

where in the second equation we are referring to the norms induced by the metric on the various tangent spaces of M. The difference between these two is o(l(c)), because exp p has derivative the identity at 0T p(M), and the metric on T exp p(c(t))(M) is very close (say by a factor of 1±ϵ) to that of T p(M) if we work in local coordinates and agree to identify the tangent spaces.

Revised on December 15, 2009 19:37:35 by Toby Bartels (173.60.119.197)