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On sub-Riemannian geodesic curvature in dimension three

  • Davide Barilari ORCID logo EMAIL logo and Mathieu Kohli
Published/Copyright: April 24, 2021

Abstract

We introduce a notion of geodesic curvature k ζ for a smooth horizontal curve 𝜁 in a three-dimensional contact sub-Riemannian manifold, measuring how much a horizontal curve is far from being a geodesic. We show that the geodesic curvature appears as the first corrective term in the Taylor expansion of the sub-Riemannian distance between two points on a unit speed horizontal curve

d SR 2 ( ζ ( t ) , ζ ( t + ε ) ) = ε 2 - k ζ 2 ( t ) 720 ε 6 + o ( ε 6 ) .

The sub-Riemannian distance is not smooth on the diagonal; hence the result contains the existence of such an asymptotics. This can be seen as a higher-order differentiability property of the sub-Riemannian distance along smooth horizontal curves. It generalizes the previously known results on the Heisenberg group.

MSC 2010: 53C17; 53C22; 53C23

Award Identifier / Grant number: ANR-15-CE40-0018

Funding statement: This work was supported by the Grant ANR-15-CE40-0018 “Sub-Riemannian Geometry and Interactions” of the French ANR.

A Jacobi fields and asymptotics of the Lie brackets

In what follows, we discuss asymptotics of sub-Riemannian Jacobi fields. In this appendix, we give a self-contained presentation to prove Proposition 29, but we refer to [4] (see also [9] for a survey) for more general results, which contain in particular Lemma 40 presented below.

We denote S p * M := H - 1 ( 1 / 2 ) T p * M , and we set

S := S p * M { d q δ q Σ p } ,

where we recall d q δ denotes the differential of 𝛿 at 𝑞. We can interpret 𝔖 as the union of the integral lines of the Hamiltonian flow that are the lifts to T * M of geodesics leaving from 𝑝 that are parametrized by arc length and that have not yet reached their cut time.

Proposition 37

Let Φ H t denote the flow of H . The map

F : S F ( S ) S p * M × R , F ( λ ) = ( Φ - H δ ( π ( λ ) ) ( λ ) , δ ( π ( λ ) ) ) ,

is a diffeomorphism whose inverse is F - 1 : F ( S ) S , F - 1 ( ξ , δ ¯ ) = Φ H δ ¯ ( ξ ) .

We can see ( ξ , δ ¯ ) as coordinates on the set 𝔖. The function 𝛿 is thereby transported from its initial domain Σ p to 𝔖 since δ ¯ = δ π . In the coordinates ( ξ , δ ¯ ) ,

(A.1) δ ¯ = H , π * H = Γ π ,

where π * denotes the differential of π : T M M .

Remark 38

As a consequence of definitions (4.3) and (4.4), for every orthonormal frame of the distribution { X 1 , X 2 } and i , j , k = 0 , 1 , 2 , we have [ X ¯ i , X ¯ j ] = [ X i , X j ] ¯ , which in turn implies

c X ¯ i , X ¯ j X ¯ k = c ¯ X i , X j X k , [ h X i , X ¯ j ] = [ h X i , h X j ] = 0 .

We can now introduce Jacobi fields.[2]

Definition 39

A vector field 𝒥 defined along an integral line γ ¯ : I T * M of the Hamiltonian field is said to be a Jacobi field if the Lie derivative L H J = 0 along γ ¯ .

We need the following result.

Lemma 40

Let us consider { X 1 , X 2 } an orthonormal frame of the distribution. There exist two smooth vector fields J : S T S and J 0 : S T S ,

(A.2) J i = α i X ¯ 1 + β i X ¯ 2 + σ i X ¯ 0 + j 1 i h X 1 + j 2 i h X 2 + j 0 i h X 0 , i { , 0 } ,

that satisfy for i { , 0 } the following conditions:

  1. J i is a Jacobi field, i.e., [ J i , H ] = 0 ;

  2. for every ξ S p * M , we have π * ( J i ( ξ ) ) = 0 ( J i is vertical at zero) and

    σ F - 1 ( ξ , δ ¯ ) δ ¯ 2 2 and σ 0 F - 1 ( ξ , δ ¯ ) - δ ¯ 3 6 .

Moreover, the functions σ i are smooth and are independent of the choice of { X 1 , X 2 } .

Proof

By combining the expression of H given by (4.5) and that of J i , we can reformulate the condition [ J i , H ] = 0 by decomposing it on the frame

( X ¯ 0 , X ¯ 1 , X ¯ 2 , h X 0 , h X 1 , h X 2 ) .

The corresponding system of differential equation is given by

(A.3) { H σ i = h X 2 α i - h X 1 β i , H α i = ( h X 2 α i - h X 1 β i ) c ¯ 1 , 2 1 + h X 1 σ i η ( X 1 ) + h X 2 σ i c ¯ 0 , 2 1 + j 1 i , H β i = ( h X 2 α i - h X 1 β i ) c ¯ 1 , 2 2 + h X 2 σ i η ( X 2 ) + h X 1 σ i c ¯ 0 , 1 2 + j 2 i , H j 1 i = - k ( h X 2 h X k ( α i X 1 + β i X 2 + σ i X 0 ) c ¯ 1 , 2 k + c ¯ 1 , 2 k ( j 2 i h X k + h X 2 j k i ) ) , H j 2 i = - k ( h X 1 h X k ( α i X 1 + β i X 2 + σ i X 0 ) c ¯ 2 , 1 k + c ¯ 2 , 1 k ( j 1 i h X k + h X 1 j k i ) ) , H j 0 i = k , 0 ( h X h X k ( α i X 1 + β i X 2 + σ i X 0 ) c ¯ 0 , k + c ¯ 0 , j k ( j i h X k + h X j k i ) ) .

In order to define the vector fields J and J 0 , it is then sufficient to define their values on S p * M , the values on the whole space F ( S ) then following from the differential equation (A.3). We define, on S p * M ,

J | S p * M = h X 2 h X 1 - h X 1 h X 2 , J 0 | S p * M = h X 0 .

We now use (A.3) to establish the asymptotics of σ 0 and σ by computing the derivatives and evaluating at zero. We find out that, for any 𝜉 in S p * M ,

σ i ( ξ ) = 0 ,
H ( σ i ) ( ξ ) = h X 2 ( ξ ) α i ( ξ ) - h X 1 ( ξ ) β i ( ξ ) = 0 ,
H 2 ( σ i ) ( ξ ) = h X 2 ( ξ ) H ( α i ) ( ξ ) - h X 1 ( ξ ) H ( β i ) ( ξ ) = h X 2 ( ξ ) j 1 i ( ξ ) - h X 1 ( ξ ) j 2 i ( ξ ) ,
where we used α i ( ξ ) = β i ( ξ ) = σ i ( ξ ) = 0 at S p * M . Using ξ H - 1 ( 1 / 2 ) , we have

H 2 ( σ ) ( ξ ) = h X 2 2 ( ξ ) + h X 1 2 ( ξ ) = 1 , H 2 ( σ 0 ) ( ξ ) = 0 .

Furthermore, using again ξ H - 1 ( 1 / 2 ) ,

H 3 ( σ 0 ) ( ξ ) = h X 2 ( ξ ) H ( j 1 i ) ( ξ ) - h X 1 ( ξ ) H ( j 2 i ) ( ξ ) = - h X 2 2 ( ξ ) - h X 1 2 ( ξ ) = - 1 .

Now, thanks to the first identity in (A.1),

H n ( σ i ) ( ξ ) = n δ ¯ n | δ ¯ = 0 σ i F - 1 ( ξ , δ ¯ ) ,

which proves the asymptotics in (ii). The fact that the functions σ i are smooth and independent of the choice of ( X 1 , X 2 ) is due to the identity σ i = ω d π ( J i ) . ∎

Lemma 41

We have S S p * M h Γ - 1 ( 1 ) h J Γ - 1 ( 0 ) .

Proof

Let us consider any covector in S S p * M . It can be written as d δ q for a certain 𝑞 in Σ p by definition of 𝔖. Now, if we choose ( Γ , J Γ ) as a frame of the distribution, by using (4.1), we can write, thanks to Lemma 22,

h Γ ( d δ q ) = d δ q ( Γ ) = 1 , h J Γ ( d δ q ) = d δ q ( J Γ ) = 0 .

We are now able to compute the asymptotics of the Lie brackets of the elements of the frame ( Γ , J Γ , X 0 ) .

Proposition 42

The quantities δ ¯ c Γ , J Γ J Γ and δ ¯ 2 c Γ , X 0 J Γ (a priori defined on S S p * M ) can be smoothly extended to 𝔖 and are respectively equal to −4 and −6 over S p * M .

Proof

Let us write the vector fields J 0 and J introduced in Lemma 40 over S T p * M with respect to the orthonormal frame Γ , J Γ ,

J i = α i Γ ¯ + β i J Γ ¯ + σ i X ¯ 0 + j 1 i h Γ + j 2 i h J Γ + j 0 i h X 0 .

Since S T p * M is contained in h Γ - 1 ( 1 ) h J Γ - 1 ( 0 ) (by Lemma 41), we have j 1 i = j 2 i = 0 , and the first and the third equation of (A.3) can be combined as 0 = H 2 σ i + c ¯ Γ , J Γ J Γ H σ i + c ¯ X 0 , Γ J Γ σ i . Since this last equation is satisfied by σ 0 and σ , we find out that

(A.4) ( - H 2 σ - H 2 σ 0 δ ¯ ) = ( H σ δ ¯ σ δ ¯ 2 H σ 0 δ ¯ 2 σ 0 δ ¯ 3 ) ( δ ¯ c ¯ Γ , J Γ J Γ δ ¯ 2 c ¯ X 0 , Γ J Γ ) .

The matrix of this system as well as its left-hand side are smooth over 𝔖 when δ ¯ goes to zero by applying Lemma 26 to the asymptotics given in Lemma 40 (we use the first identity in (A.1)), and

( - H 2 σ - H 2 σ 0 δ ¯ ) ( - 1 1 ) , ( H σ δ ¯ σ δ ¯ 2 H σ 0 δ ¯ 2 σ 0 δ ¯ 3 ) ( 1 1 2 - 1 2 - 1 6 ) .

Inverting (A.4), we obtain that the functions δ ¯ c ¯ Γ , J Γ J Γ and δ ¯ 2 c ¯ X 0 , Γ J Γ that were a priori defined on S S p * M can in fact be smoothly extended to the domain 𝔖. Taking then the limit as δ ¯ goes to zero, we find the values of δ ¯ c ¯ Γ , J Γ J Γ and δ ¯ 2 c ¯ X 0 , Γ J Γ on the set δ ¯ - 1 ( 0 ) = S p * M . ∎

We obtain similar results for δ ¯ 2 H c ¯ Γ , J Γ J Γ and δ ¯ 2 J Γ ¯ c ¯ Γ , J Γ J Γ .

Proposition 43

The function δ ¯ 2 H c ¯ Γ , J Γ J Γ , a priori defined on S S p * M , can be extended to a smooth function on 𝔖, and its evaluation is equal to 4 on S p * M .

Proof

We know from Proposition 42 that δ ¯ c ¯ Γ , J Γ J Γ can be extended to a smooth function on 𝔖 that is equal to −4 on δ ¯ - 1 ( 0 ) . Since H is also smooth, we can write

δ ¯ H ( δ ¯ c ¯ Γ , J Γ J Γ ) = δ ( H δ ¯ ) c ¯ Γ , J Γ J Γ + δ ¯ 2 ( H c ¯ Γ , J Γ J Γ ) .

So, recalling that H δ ¯ , we have that

δ ¯ 2 ( H c ¯ Γ , J Γ J Γ ) = δ ¯ H ( δ ¯ c ¯ Γ , J Γ J Γ ) - δ ¯ c ¯ Γ , J Γ J Γ

has a smooth extension on 𝔖 that is equal to 4 on δ ¯ - 1 ( 0 ) = S p * M . ∎

Proposition 44

The function δ ¯ 2 J Γ ¯ c ¯ Γ , J Γ J Γ that is a priori defined on S S p * M can be extended to a smooth function on the domain 𝔖.

Proof

Let us consider the fields J 0 and J over 𝔖 that we introduced in Lemma 40. We start by proving the following claim: for every 𝜉 in 𝔖, the vector V ( ξ ) defined by (A.5) is colinear to J Γ .

(A.5) V ( ξ ) := d π ( σ ( ξ ) J 0 ( ξ ) - σ 0 ( ξ ) J ( ξ ) ) .

First notice that V ( ξ ) belongs to the distribution since its component along the Reeb vector field X 0 is zero thanks to (A.2). Let us then prove that it is orthogonal to the gradient of 𝛿. Indeed, for i { 0 , } , by definition of Jacobi field, one has 0 = [ H , J i ] δ ¯ = H J i δ ¯ - J i ( H δ ¯ ) = H J i δ ¯ , where we used that H δ ¯ = 1 . So J i δ ¯ is constant on the integral lines of H . But, on S p * M , the function J i δ ¯ is equal to zero. Therefore, J i δ ¯ = 0 on 𝔖. Thus d π ( J i ( ξ ) ) belongs to the kernel of d δ . The vector V ( ξ ) is a linear combination of vectors in the kernel of d δ ; hence it is also in the kernel of d δ . By Lemma 22, this means that V ( ξ ) is colinear to J Γ , and the claim is proved.

Let us define b : S R such that, for any 𝜉 in 𝔖,

(A.6) V ( ξ ) = b ( ξ ) J Γ ( π ( ξ ) )

in such a way that, for all 𝜉 in S T p * M ,

d π ( σ ( ξ ) J 0 ( ξ ) - σ 0 ( ξ ) J ( ξ ) b ( ξ ) ) = J Γ ( π ( ξ ) ) .

Since c ¯ Γ , J Γ J Γ is constant on the fiber of T * M , we can replace J Γ ¯ in the expression with a vector field that projects over J Γ . Then we have

(A.7) δ ¯ 2 J Γ ¯ c ¯ Γ , J Γ J Γ = δ ¯ 2 ( σ J 0 c ¯ Γ , J Γ J Γ - σ 0 J c ¯ Γ , J Γ J Γ b ) .

To prove that the right-hand side of (A.7) is smooth, we write the fields J i over S T p * M as

J i = α i Γ ¯ + β i J Γ ¯ + σ i X ¯ 0 + j 1 i h Γ + j 2 i h J Γ + j 0 i h X 0 .

Combining with (A.5) and (A.6), we obtain that, for any 𝜉 in S T p * M , b ( ξ ) = σ ( ξ ) β 0 ( ξ ) - σ 0 ( ξ ) β ( ξ ) . Now, thanks to Lemma 41, h Γ = 1 and h J Γ = 0 on S T p * M , so the first equation of (A.3) becomes H σ i = - β i . As a consequence, for every 𝜉 in S T p * M , b ( ξ ) = σ 0 ( ξ ) H σ ( ξ ) - σ ( ξ ) H σ 0 ( ξ ) . Hence

δ ¯ 2 J Γ ¯ c ¯ Γ , J Γ J Γ = δ ¯ 2 ( σ J 0 c ¯ Γ , J Γ J Γ - σ 0 J c ¯ Γ , J Γ J Γ b ) = δ ¯ ( σ J 0 ( δ ¯ c ¯ Γ , J Γ J Γ ) - σ 0 J ( δ ¯ c ¯ Γ , J Γ J Γ ) σ 0 H σ - σ H σ 0 ) ,

where we used that J i δ ¯ = 0 for i { 0 , } . By applying Proposition 42, δ ¯ c ¯ Γ , J Γ J Γ can be extended to a smooth function defined on 𝔖, and its value on S p * M is constant. Therefore, the functions J i ( δ ¯ c ¯ Γ , J Γ J Γ ) can be extended to smooth functions on 𝔖 that vanish at every point of S p * M . We combine this with the smoothness and the asymptotics of the functions σ i that come from Lemma 40, and thanks to Lemma 26, the function δ ¯ 2 J Γ ¯ c Γ , J Γ J Γ can be extended to a smooth function on 𝔖. ∎

A.1 Proof of Proposition 29

Let us start by proving the first identity. We consider the lift of 𝜁 defined by ζ ¯ : I { 0 } S , where ζ ¯ ( t ) = d δ ζ ( t ) . Recall that δ ¯ = δ π and that c ¯ i , j k = c i , j k π . Therefore,

(A.8) δ ( ζ ( t ) ) c Γ , J Γ J Γ ( ζ ( t ) ) = δ ¯ ( ζ ¯ ( t ) ) c ¯ Γ , J Γ J Γ ( ζ ¯ ( t ) ) .

Recall moreover that ζ ¯ ( t ) = d δ ζ ( t ) is the evaluation at time δ ( ζ ( t ) ) of the integral line of the Hamiltonian flow γ ¯ ζ ( t ) that is a lift of the minimizing geodesic γ ζ ( t ) parametrized by arc length joining 𝑝 to ζ ( t ) . In particular, by Proposition 37,

(A.9) ζ ¯ ( t ) = F - 1 ( γ ¯ ζ ( t ) ( 0 ) , δ ( ζ ( t ) ) ) .

Combining Remark 19 with (6.8) (cf. proof of Proposition 28), one has

(A.10) h X 0 ( γ ¯ ζ ( t ) ( 0 ) ) t 0 h ζ ( 0 ) .

Since γ ζ ( t ) is parametrized by arc length, then γ ¯ ζ ( t ) is contained in H - 1 ( 1 / 2 ) , which implies, for ( X 1 , X 2 ) any choice of orthonormal frame of the distribution,

(A.11) h X 1 2 ( γ ¯ ζ ( t ) ( 0 ) ) + h X 2 2 ( γ ¯ ζ ( t ) ( 0 ) ) = 1 .

By combining (A.9), (A.10), (A.11), we obtain that, for 𝑡 small enough (recall δ ( ζ ( t ) ) 0 ), ζ ¯ ( t ) belongs to a compact subset 𝐾 of 𝔖. Thanks to Proposition 42, the function δ ¯ c ¯ Γ , J Γ J Γ is uniformly continuous on 𝐾. Now, since δ ¯ ( ζ ¯ ( t ) ) = δ ( ζ ( t ) ) 0 for t 0 , and as δ ¯ c ¯ Γ , J Γ J Γ is equal to −4 on δ ¯ - 1 ( 0 ) = S p * M , we deduce, from the uniform continuity,

lim t 0 δ ¯ ( ζ ¯ ( t ) ) c ¯ Γ , J Γ J Γ ( ζ ¯ ( t ) ) = - 4 ,

which proves, thanks to (A.8), the first claim.

The other asymptotics follow from similar arguments, where we use Propositions 43 and 44 instead of Proposition 42 and where we replace (A.8) by the relations

δ 2 ( ζ ( t ) ) c Γ , X 0 J Γ ( ζ ( t ) ) = δ ¯ 2 ( ζ ¯ ( t ) ) c ¯ Γ , X 0 J Γ ( ζ ¯ ( t ) ) ,
δ 2 ( ζ ( t ) ) Γ c Γ , J Γ J Γ ( ζ ( t ) ) = δ ¯ 2 ( ζ ¯ ( t ) ) H c ¯ Γ , J Γ J Γ ( ζ ¯ ( t ) ) ,
δ 2 ( ζ ( t ) ) J Γ c Γ , J Γ J Γ ( ζ ( t ) ) = δ ¯ 2 ( ζ ¯ ( t ) ) J Γ ¯ c ¯ Γ , J Γ J Γ ( ζ ¯ ( t ) ) ,
which are proved as (A.8), using that Γ π = d π H (cf. (A.1)) and J Γ π = d π J Γ ¯ .

Acknowledgements

The authors wish to thank Luca Rizzi for useful discussions.

  1. Communicated by: Zoltan Balogh

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Received: 2020-03-09
Accepted: 2021-03-11
Published Online: 2021-04-24
Published in Print: 2022-07-01

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