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Cocycle Stability of Linear Automorphisms and their Jointly Integrable Perturbations

Ignacio Correa
Abstract

We show cocycle stability for linear maps with a weak irreducibility condition and their jointly integrable perturbations.

1 Introduction

For a dynamical system ff we are interested in solving for which φ:𝕋d𝕋d\varphi:\mathbb{T}^{d}\rightarrow\mathbb{T}^{d} the cohomological equation

φ(x)=u(fx)u(x)+const.\varphi(x)=u(fx)-u(x)+\mathrm{const.} (\star)

has a solution uu (in other words, we want to see when φ\varphi is cohomologus to a constant).

The classic result for this question is Livsic, which for hyperbolic systems states that having trivial periodic data is a sufficient and necessary condition. For linear ergodic automorphisms Veech showed that this is also the case [Vee86].

One can also show, using Fourier series, that for Diophantine translation of the torus there is no restriction at all (other than perhaps some extra regularity) as for which φ\varphi accept solutions.

For partially hyperbolic systems (which a priori might not have periodic points) Katok and Kononenko came up with a natural necessary condition: to have trivial periodic cycle functionals, that is φ\varphi should have trivial holonomies along cycles made out of stable and unstable segments (see § 2.3 or [KK96] for details).

We will show that, in some cases, this is restriction is sufficient, which immediately implies cocycle stability in the sense of [KK96, Definition 1]. That is, the set of coboundaries is closed, which would be the case since then we would have

{φ:φ=ufu}={φ=0}γ su-cycle{PCFγφ=0}.\biggl{\{}\varphi:\varphi=u\circ f-u\biggr{\}}=\biggl{\{}\int\varphi=0\biggr{\}}\cup\bigcup_{\gamma\text{ $su$-cycle}}\biggl{\{}PCF_{\gamma}\varphi=0\biggr{\}}.

More specifically we will show that the CRC^{R} functions are CrC^{r}-sable.

Results in this direction are known when ff has some accessibility condition [Wil13, KK96]. So instead in these notes we will work with the spiritual opposite of this case: the jointly integrable case (by this we mean that the susu-distribution EsEuE^{s}\oplus E^{u} is integrable, see definition 2.2).

While some other minor results can be established with the “naive” idea of our technique (see § A.2), our most interesting application would be to linear maps and their (jointly integrable) perturbations.

Theorem A.

Given a chosen regularity rr (and a central dimension cc) there is a minimum regularity RR so that for any partially hyperbolic FSL(d,)F\in SL(d,\mathbb{Z}) Katznelson irreducible and strongly RR-bunched automorphism of the torus, if a jointly integrable diffeomorphism f:𝕋d𝕋df:\mathbb{T}^{d}\to\mathbb{T}^{d} is CRC^{R}-close enough to FF then it is cocycle stable with the following regularities:

If φ\varphi is CRC^{R} with PCFγφ=0\operatorname{PCF}_{\gamma}\varphi=0 for any susu-cycle γ\gamma, then the cohomological equation

φ(x)=u(fx)u(x)+const.\varphi(x)=u(fx)-u(x)+\mathrm{const.} (\star1)

has a CrC^{r} solution uu.

Katznelson irreducible is the (very weak) irreducibility condition needed to apply Katznelson’s lemma [Kat71, Lemma 3] and is explicitly defined in definition 3.4. There we show that this condition is actually necessary for solving (\star1).

For the purposes of potential applications, in § A.1, we also give explicit values for RR.

Our main tool would a d\mathbb{Z}^{d}-action on a central leaf called central translations, introduced by F. Rodriguez-Hertz in [Rod05] and defined here in § 2.2. Following that paper the objective would be to show that these enjoy a Diophantine property (§ 3.2) in the linear case and then, using Moser’s techniques [Mos90], we show that they can be linearized in the non-linear case (§ 3.3).

In here we are able to show this Diophantine property in more generality, and since [Rod05, § 6.3] doesn’t use any of their other hypotheses we have the following result:

Corollary B.

If a partially hyperbolic automorphism FSL(d,)F\in SL(d,\mathbb{Z}) is Katznelson irreducible and (9c+4)(9c+4)-bunched, then any C9c+4C^{9c+4} jointly integrable diffeomorphism ff which is C6c+1C^{6c+1}-close to FF is ergodic and topologically conjugated to FF.

In here cc is the dimension of the center distribution for the partial hyperbolic splitting.

In [Rod05, Theorem 5.1] it is shown that, in the pseudo-Anosov case (which is stronger than Katznelson irreducibility) with center dimension 22, there is a dichotomy on the accessibility classes: either EsEuE^{s}\oplus E^{u} is integrable or ff is accessible111Their hypothesis of having eigenvalues of modulus one is not necessary for this result.. In the general accessible case Wilkinson [Wil13] showed the cocycle stability. So we get that these automorphisms are “stably cocycle stable”:

Corollary C.

If FSL(d,)F\in SL(d,\mathbb{Z}) is pseudo-Anosov, partially hyperbolic with splitting SCUS\oplus C\oplus U with dimC=2\dim C=2, and strongly RR-bunched, then any ff which is CRC^{R}-close to FF (with RR big enough) is cocycle stable.

The RR in this theorem as well as the regularity of the solution of (\star1) are as established in § A.1.

The idea of the proof is that we can solve (\star1) along a central leaf using the Diophantine property of the central translations (§ 4.1). Then using the holonomy functionals defined in § 2.3 we can extend this solution to the whole torus (§ 4.2).

In § A.2, which can be read independently of the rest of this notes, we illustrate this idea of using Diophantine dynamics to solve (\star1) along the center and then extend using holonomy functionals in a simpler case.

2 Preliminaries

2.1 Partial Hyperbolicity

Definition 2.1.

We say that a diffeomorphism f:MMf:M\to M is partially hyperbolic if there is an invariant splitting TM=EsEcEuTM=E^{s}\oplus E^{c}\oplus E^{u} so that (for some metric)

Dxsf\displaystyle\lVert D^{s}_{x}f\rVert <1,\displaystyle<1, m(Dxuf)\displaystyle m(D^{u}_{x}f) >1,\displaystyle>1,
Dxsf\displaystyle\lVert D^{s}_{x}f\rVert <m(Dxcf),\displaystyle<m(D^{c}_{x}f), m(Dxuf)\displaystyle m(D^{u}_{x}f) >Dxcf,\displaystyle>\lVert D^{c}_{x}f\rVert,

where m(A)m(A) is the conorm of AA and Dσf=Df|EσD^{\sigma}f=Df|_{{E^{\sigma}}}.

For general partially hyperbolic systems EsE^{s} and EuE^{u} are integrable into invariant foliations 𝒲ss\mathcal{W}^{ss} and 𝒲uu\mathcal{W}^{uu}. In our case, where ff is a perturbation of a linear map, also EcE^{c}, EsEcE^{s}\oplus E^{c}, and EcEuE^{c}\oplus E^{u} are integrable into invariant foliations 𝒲c\mathcal{W}^{c}, 𝒲cs\mathcal{W}^{cs}, and 𝒲cu\mathcal{W}^{cu} [HPS70].

Definition 2.2.

We say that a partially hyperbolic diffeomorphism ff is jointly integrable if there is an invariant foliation 𝒲su\mathcal{W}^{su} tangent to EsEuE^{s}\oplus E^{u}. We call the leaves of 𝒲su\mathcal{W}^{su} of susu-leaves.

Remark 2.3.

This foliation 𝒲su\mathcal{W}^{su}, when it exist, has CrC^{r} leaves. Indeed, locally we can express the leaves as graphs and we can use Journé’s lemma [Jou88] on the functions giving these graphs to prove this regularity. Furthermore, 𝒲su(x)\mathcal{W}^{su}(x) only needs to be a set saturated by stable and unstable leaves and transversal to the center leaves. But we won’t use this fact in any relevant way, the only important thing is that the projection along stable leaves and along unstable leaves commute.

Of course linear maps FSL(d,)F\in SL(d,\mathbb{Z}) (thought as maps of the torus 𝕋d\mathbb{T}^{d}) are jointly integrable as the invariant splitting should be a splitting d=SCU\mathbb{R}^{d}=S\oplus C\oplus U into vector subspaces.

In our theorems we ask for hypothesis on FF with respect to an implicitly given partial hyperbolic splitting. Whenever we ask for ff to be jointly integrable, we mean with respect to the splitting that comes from perturbing the given splitting.

Asking for stronger conditions (called bunching conditions) in the domination of center it is known [Wil13] that relevant holonomy maps have certain amount of regularity.

Definition 2.4.

We say that ff partially hyperbolic is RR-bunched if (for some metric) for every xx

Dxsf\displaystyle\lVert D^{s}_{x}f\rVert <m(Dxcf)R,\displaystyle<m(D^{c}_{x}f)^{R}, m(Dxuf)\displaystyle m(D^{u}_{x}f) >DxcfR,\displaystyle>\lVert D^{c}_{x}f\rVert^{R},
Dxsf\displaystyle\lVert D^{s}_{x}f\rVert <m(Dxcf)DxcfR,\displaystyle<m(D^{c}_{x}f)\lVert D^{c}_{x}f\rVert^{-R}, m(Dxuf)\displaystyle m(D^{u}_{x}f) >Dxcfm(Dxcf)R.\displaystyle>\lVert D^{c}_{x}f\rVert m(D^{c}_{x}f)^{-R}.

If further

max{Dxsf,m(Dxuf)1}<min{m(Dxcf)R,DxcfR}\max\{\lVert D^{s}_{x}f\rVert,m(D^{u}_{x}f)^{-1}\}<\min\{m(D^{c}_{x}f)^{R},\lVert D^{c}_{x}f\rVert^{-R}\}

we say that ff is strongly RR-bunched.

Note that the bounds for partial hyperbolicity and for bunching are all open in the C1C^{1} topology, so if ff is close enough to a linear map FF satisfying this conditions so will ff.

On the other hand, for a linear map FF is easy to show that the partial hyperbolicity condition and the bunching conditions are equivalent to analogous conditions when replacing norms and conorms with the biggest and smallest (absolute value of) eigenvalue of the respective subspace. In this case if F|CF|_{C} only has eigenvalues of modulus one then it is RR-bunched and strongly RR-bunched for any RR.

In this notes partial hyperbolicity and jointly integrability are always assumed.

2.2 Central Translations

Solving (\star1) without any hypothesis on φ\varphi usually requires a certain Diophantine property. In our case this property is hidden behind an auxiliary construction called the central translations.

Is easy to see that in our case (jointly integrable perturbations of linear maps) every pair of susu-leaf and central leaf intersect exactly once in the universal cover. Fix a “favorite” central leaf 𝒞=𝒲c(0)\mathcal{C}=\mathcal{W}^{c}(0) of a fix point 0.

We define an action Tn:𝒞𝒞T_{n}:\mathcal{C}\to\mathcal{C} of d\mathbb{Z}^{d} in 𝒞\mathcal{C} by

{Tnx}=𝒞𝒲su(x+n)\{T_{n}x\}=\mathcal{C}\bigcap\mathcal{W}^{su}(x+n)

where, by abuse of notation, we are thinking of 𝒞,𝒲su(x+n)d\mathcal{C},\mathcal{W}^{su}(x+n)\subset\mathbb{R}^{d} as living in the universal cover.

We refer to these as central translations. In § 3.2 we will show that these are, in a certain sense, Diophantine and so the perturbations can be linearized (§ 3.3) and we will be able to use this Diophantine property to solve the cohomological equation along the center in § 4.1.

Since the intention is to linearize these translations we start here by projecting them to a vector space

T~n=ΠTnΠ1:CC\tilde{T}_{n}=\Pi\circ T_{n}\circ\Pi^{-1}:C\to C

where CdC\subset\mathbb{R}^{d} is the central subspace for the nearby linear map FF and Π:𝒞C\Pi:\mathcal{C}\to C is the projection to this subspace along the susu-leaves of ff. See [Rod05, Proposition B.1] to see that Π\Pi is indeed well defined and invertible.

This Π\Pi shouldn’t be confused with πc:d𝒞\pi^{c}:\mathbb{R}^{d}\to\mathcal{C} the projection to our favorite central leaf for ff

{πcx}=𝒞𝒲su(x).\{\pi^{c}x\}=\mathcal{C}\bigcap\mathcal{W}^{su}(x).

Notice that πc\pi^{c} and Π\Pi are both “reasonable” holonomy maps, and that Tn(x)=πc(x+n)T_{n}(x)=\pi^{c}(x+n). So according to [PSW97] we have

Lemma 2.5.

If ff is RR-bunched and CRC^{R} then TnT_{n} and T~n\tilde{T}_{n} are uniformly CRC^{R}, and πc\pi^{c} is uniformly CRC^{R} along the leaves of 𝒲c\mathcal{W}^{c}.

We describe what uniformly CRC^{R} means right after lemma 2.7.

2.3 Holonomy Functionals

Let us define the holonomy functionals. Consider xx a point and x+𝒲ss(x)x^{+}\in\mathcal{W}^{ss}(x), and x𝒲uu(x)x^{-}\in\mathcal{W}^{uu}(x). In each case we define the functional Hol\operatorname{Hol} in the following ways

Holxx+φ=n=0φ(fnx)φ(fnx+),\displaystyle\operatorname{Hol}_{x}^{x^{+}}\varphi=\sum_{n=0}^{\infty}\varphi(f^{n}x)-\varphi(f^{n}x^{+}),
Holxxφ=n=1φ(fnx)φ(fnx)\displaystyle\operatorname{Hol}_{x}^{x^{-}}\varphi=-\sum_{n=1}^{\infty}\varphi(f^{-n}x)-\varphi(f^{-n}x^{-})

and if γ=(x0,x1,,xk)\gamma=(x_{0},x_{1},\dots,x_{k}) is a susu-sequence, by that we mean xj𝒲ss(xj1)x_{j}\in\mathcal{W}^{ss}(x_{j-1}) or xj𝒲uu(xj1)x_{j}\in\mathcal{W}^{uu}(x_{j-1}), we extend the functional

Holγφ=j=1kHolxj1xjφ.\operatorname{Hol}_{\gamma}\varphi=\sum_{j=1}^{k}\operatorname{Hol}_{x_{j-1}}^{x_{j}}\varphi.

In the case where γ\gamma is periodic, that is x0=xkx_{0}=x_{k}, this is the periodic cycle functional PCFγφ=HolγφPCF_{\gamma}\varphi=\operatorname{Hol}_{\gamma}\varphi.

The condition PCFγφ=0PCF_{\gamma}\varphi=0 for all susu-sequence γ\gamma is a natural necessary condition for solving the cohomological equation (\star1). In such case we say that φ\varphi has trivial periodic cycle functionals, and in this notes we will always assume that φ\varphi satisfies this condition.

So, under this hypothesis, if y𝒲su(x)y\in\mathcal{W}^{su}(x) (recall that in this notes we consider ff being jointly integrable) we write

Holxyφ=Holγφ\operatorname{Hol}_{x}^{y}\varphi=\operatorname{Hol}_{\gamma}\varphi

where γ=(x0=x,x1,,xk=y)\gamma=(x_{0}=x,x_{1},\dots,x_{k}=y) is a susu-sequence going from xx to yy (the trivial periodic cycle hypothesis makes this well defined, regardless of the choice of γ\gamma).

Formally φ(fnx)-\sum\varphi(f^{n}x) and φ(fnx)\sum\varphi(f^{-n}x) solve (\star1), so, naively, we can think of “Holxyφ=u(y)u(x)\operatorname{Hol}_{x}^{y}\varphi=u(y)-u(x)”. This, in a sense, shows that this functional solves the equation along 𝒲su\mathcal{W}^{su}.

Below we establish some trivial properties of these functionals to reference in the future (one of which formalizes the idea of the previous paragraph).

Lemma 2.6.

If y,z𝒲su(x)y,z\in\mathcal{W}^{su}(x) then Hol\operatorname{Hol} satisfies the following properties

Fundamental theorem of dynamics
Holxy(ufu)=u(y)u(x)\operatorname{Hol}_{x}^{y}(u\circ f-u)=u(y)-u(x) (FT)

or, equivalently,

(HolfxfyHolxy)φ=φ(y)φ(x)\left(\operatorname{Hol}_{fx}^{fy}-\operatorname{Hol}_{x}^{y}\right)\varphi=\varphi(y)-\varphi(x) (FT)
Additivity
Holxzφ=Holxyφ+Holyzφ.\operatorname{Hol}_{x}^{z}\varphi=\operatorname{Hol}_{x}^{y}\varphi+\operatorname{Hol}_{y}^{z}\varphi. (Add.)

We establish too the regularity that we will need for these functionals.

Lemma 2.7.

If ff and φ\varphi are CRC^{R} then

Holx0xφ:𝒲su(x0)\operatorname{Hol}^{x}_{x_{0}}\varphi:\mathcal{W}^{su}(x_{0})\to\mathbb{R}

is uniformly CRC^{R}.

If further ff is strongly RR-bunched then

Holxπcxφ:𝒲c(x0)\operatorname{Hol}^{\pi^{c}x}_{x}\varphi:\mathcal{W}^{c}(x_{0})\to\mathbb{R}

is uniformly CRC^{R}.

By uniformly CRC^{R} we mean that all partial derivatives (and the Hölder constants for the highest order derivatives if RR is not an integer) are bounded both along 𝒲σ(x0)\mathcal{W}^{\sigma}(x_{0}) and as we vary x0𝕋dx_{0}\in\mathbb{T}^{d}.

Proof.

For first part, if we restrict our attention to 𝒲ss(x)\mathcal{W}^{ss}(x) and 𝒲uu(x)\mathcal{W}^{uu}(x) then it is just a simple calculation. Then using Journé [Jou88] we have the result.

For the second part strongly RR-bunched implies that the CRC^{R} cocycle dynamics f~:M×M×\tilde{f}:M\times\mathbb{R}\to M\times\mathbb{R}

f~(x,t)=(fx,t+φ(x))\tilde{f}(x,t)=(fx,t+\varphi(x))

is partially hyperbolic RR-bunched (see [Wil13]).

If y𝒲ss(x)y\in\mathcal{W}^{ss}(x) we can show that d(f~n(x,0),f~n(x,Holxyφ))d(\tilde{f}^{n}(x,0),\tilde{f}^{n}(x,\operatorname{Hol}_{x}^{y}\varphi)) goes to 0 exponentially fast with and easy computation. We have an analogous result for y𝒲uu(x)y\in\mathcal{W}^{uu}(x), so

𝒲f~su(x,t)={(y,Holxyφ+t):x𝒲fsu(x)}.\mathcal{W}^{su}_{\tilde{f}}(x,t)=\left\{(y,\operatorname{Hol}_{x}^{y}\varphi+t):x\in\mathcal{W}^{su}_{f}(x)\right\}.

So, since the CRC^{R} holonomy map from 𝒲fc(x0)×\mathcal{W}^{c}_{f}(x_{0})\times\mathbb{R} to 𝒲fc(πcx0)×\mathcal{W}^{c}_{f}(\pi^{c}x_{0})\times\mathbb{R} is

(x,t)(πcx,Holxπcxφ+t),(x,t)\mapsto\left(\pi^{c}x,\operatorname{Hol}_{x}^{\pi^{c}x}\varphi+t\right),

we get that Holxπcxφ\operatorname{Hol}_{x}^{\pi^{c}x}\varphi is CRC^{R} as a map from 𝒲fc(x0)\mathcal{W}^{c}_{f}(x_{0}) to \mathbb{R}. ∎

3 Central Translations are Diophantine

For most of this section we will restrict our attention to the case where f=FSL(d,)f=F\in SL(d,\mathbb{Z}) is a linear automorphism. To emphasize the difference within the linear and not linear case (as both cases will eventually coexist) we will call the splitting for the linear map FF of SCUS\oplus C\oplus U and use aa to refer to the points of 𝕋d\mathbb{T}^{d} or d\mathbb{R}^{d} when FF is the map acting there.

3.1 Katznelson Irreducibility

Definition 3.1.

We say that FSL(d,)F\in SL(d,\mathbb{Z}) partially hyperbolic with splitting SCUS\oplus C\oplus U is Katznelson irreducible if Cd={0}C\cap\mathbb{Z}^{d}=\{0\}.

We remark that this definition depends on the choice of the splitting, and in many situations the optimal splitting would be when CC is the generalized eigenspace of eigenvalues of modulus 11. In the latter case Katznelson irreducibility is just ergodicity (see below).

Notice that by partial hyperbolicity F|CF|_{C} and FSUF_{S\oplus U} have no common eigenvalues, so this condition is enough to apply Katznelson’s lemma [Kat71, Lemma 3].

To compare with more algebraic definition of irreducibility we give the following equivalence:

Lemma 3.2.

A partial hyperbolic automorphism FSL(d,)F\in SL(d,\mathbb{Z}) is Katznelson irreducible if and only there is no rational factor η(x)[x]\eta(x)\in\mathbb{Q}[x] of its characteristic polynomial having only eigenvalues of F|CF|_{C} as roots.

Proof.

Indeed if 𝒑Cd{0}\bm{p}\in C\cap\mathbb{Z}^{d}\setminus\{0\} then Q=span{Fi𝒑}iCQ=\operatorname{span}\{F^{i}\bm{p}\}_{i\in\mathbb{Z}}\subset C is a rational subspace and the characteristic polynomial of F|QF|_{Q} has only eigenvalues of F|CF|_{C} as roots.

On the other direction kerη(F)C\ker\eta(F)\subset C is a rational subspace and so it has integer vectors. ∎

From this lemma the following implications are obvious for FSL(d,)F\in SL(d,\mathbb{R})

IrreducibilityKatznelson IrreducibilityErgodicity.\text{Irreducibility}\implies\text{Katznelson Irreducibility}\implies\text{Ergodicity}.

and none of the reverse implications are true, except in the case where F|CF|_{C} has only eigenvalues of modulus 11, in which case

Katznelson IrreducibilityErgodicity\text{Katznelson Irreducibility}\iff\text{Ergodicity}

since a rational polynomial can have only roots of modulus 11 if those roots are roots of unity.

We show now that this condition is actually necessary to solve the cohomological equation under our hypotheses.

Theorem 3.3.

If for FSL(d,)F\in SL(d,\mathbb{Z}) the equation (\star1) can be solved for any φ\varphi with trivial periodic cycle functionals, then it is Katznelson irreducible.

Proof.

If FF is not Katznelson irreducible, then take η(x)[x]\eta(x)\in\mathbb{Q}[x] the factor of the characteristic polynomial χF(x)\chi_{F}(x) with only eigenvalues of F|CF|_{C} as roots.

Then V=kerη(F)CV=\ker\eta(F)\subset C and W=kerχFη(F)SUW=\ker\frac{\chi_{F}}{\eta}(F)\supset S\oplus U are invariant sub-tori. By taking the quotient V~=𝕋d/W\tilde{V}=\mathbb{T}^{d}/W we get a torus finitely covered by VV.

By taking a power of FF we can assume that there are two different fixed points in VV that project to different points in V~\tilde{V}. By defining any function in V~\tilde{V} that gives different values to such projections, we can extend that function to 𝕋d\mathbb{T}^{d} by making it constant along WW.

Such function clearly has trivial periodic cycle functional while it cannot be cohomologus to a constant since it gives different values to two different fixed points. ∎

3.2 Using Katznelson to Show a Diophantine Property

For vd=SCUv\in\mathbb{R}^{d}=S\oplus C\oplus U we call vcCv^{c}\in C its projection along SUS\oplus U. If dimC=c\dim C=c we have, after perhaps rearranging the basis, that e1c,,ecce_{1}^{c},\dots,e^{c}_{c} is a basis of CC.

Using this basis to identify CC with c\mathbb{R}^{c} we can write the projection to CC as a linear map P:dcP:\mathbb{R}^{d}\to\mathbb{R}^{c}, with P(ei)=eiP(e_{i})=e_{i} for i=1,,ci=1,\dots,c. With this notations we can write (in the linear case) the central translations defined in § 2.2 as Tna=a+PnT_{n}a=a+Pn, and we can show that they satisfy the following Diophantine condition:

Definition 3.4.

Let a linear map P:dcP:\mathbb{Z}^{d}\to\mathbb{R}^{c} induce a d\mathbb{Z}^{d}-action by translations (na=a+Pnn\cdot a=a+Pn). We say that such PP is Diophantine if, for some constants K>0K>0 and τ>0\tau>0, for any integer vector qc{0}q\in\mathbb{Z}^{c}\setminus\{0\} there is some i=1,,di=1,\dots,d so that for any pp\in\mathbb{Z}

|Peiqp|>K|q|τ.\lvert Pe_{i}\cdot q-p\rvert>\frac{K}{\lvert q\rvert^{\tau}}.

After showing this we will show, using Moser in § 3.3, that the general central translations (of a map ff that is a jointly integrable perturbation of a linear map FF instead of a linear map itself) is conjugated to the Diophantine translations of the nearby linear map.

Theorem 3.5.

For a Katznelson irreducible automorphism FSL(d,)F\in SL(d,\mathbb{Z}), writing its central translations as Tna=a+PnT_{n}a=a+Pn as describe before we have that PP is Diophantine with τ=c\tau=c, the dimension of the central distribution for the partial hyperbolic splitting. That is

|Peiqp|>K|q|c\lvert Pe_{i}\cdot q-p\rvert>\frac{K}{\lvert q\rvert^{c}}

with the existential quantifiers of definition 3.4.

During the proof we will actually use Katznelson’s lemma for FtF^{t}.

Lemma 3.6.

If FSL(d,d)F\in SL(d,\mathbb{Z}^{d}) is Katznelson irreducible then for any integer vector 𝐩d\bm{p}\in\mathbb{Z}^{d}

d(𝒑,(SU))>K^|𝒑|c.d(\bm{p},(S\oplus U)^{\perp})>\frac{\hat{K}}{\lvert\bm{p}\rvert^{c}}.
Proof.

Of course we just need to show that we can apply Katznelson’s lemma. Namely we need to show (SU)d={0}(S\oplus U)^{\perp}\cap\mathbb{Z}^{d}=\{0\} and that Ft|(SU)F^{t}|_{(S\oplus U)^{\perp}} and Ft|CF^{t}|_{C^{\perp}} have no common eigenvalue.

This is clear from the characterization by polynomials in lemma 3.2 and the fact that Ft|(SU)F^{t}|_{(S\oplus U)^{\perp}} and F|CF|_{C}, and Ft|CF^{t}|_{C^{\perp}} and F|SUF|_{S\oplus U} have the same eigenvalues. ∎

Proof of Theorem 3.5.

The Diophantine condition is equivalent to the existence of an ii so that

|eiPtqp|>K|q|τ\lvert e_{i}\cdot P^{t}q-p\rvert>\frac{K}{\lvert q\rvert^{\tau}}

which in turn is equivalent to

Ptq𝒑>K|q|τ\lVert P^{t}q-\bm{p}\rVert>\frac{K}{\lvert q\rvert^{\tau}}

for any 𝒑d\bm{p}\in\mathbb{Z}^{d} (indeed picking each coordinate of 𝒑\bm{p} to be the closest integer to the respective coordinate of PtqP^{t}q is easy to conclude the former inequality).

But (using lemma 3.6 for the last inequality)

Ptq𝒑d(𝒑,ImPt)=d(𝒑,(KerP))=d(𝒑,(SU)))>K^|𝒑|c.\lVert P^{t}q-\bm{p}\rVert\geq d(\bm{p},\operatorname{Im}P^{t})=d(\bm{p},(\operatorname{Ker}P)^{\perp})=d(\bm{p},(S\oplus U)^{\perp}))>\frac{\hat{K}}{\lvert\bm{p}\rvert^{c}}.

In summary

Ptq𝒑>K^|𝒑|c.\lVert P^{t}q-\bm{p}\rVert>\frac{\hat{K}}{\lvert\bm{p}\rvert^{c}}.

Now we need to change the 𝒑\bm{p} for the qq in the right hand expression. If Ptq𝒑>0.5\lVert P^{t}q-\bm{p}\rVert>0.5 we can just adjust the KK to be smaller than 0.50.5 (notice |q|1\lvert q\rvert\geq 1), otherwise we have that the norms of PtqP^{t}q and 𝒑\bm{p} cannot be too far, so |𝒑|<2|Ptq|<2Pt|q|\lvert\bm{p}\rvert<2\lvert P^{t}q\rvert<2\lVert P^{t}\rVert\lvert q\rvert, finally concluding

Ptq𝒑>K^(2Pt)c1|𝒒|c.\lVert P^{t}q-\bm{p}\rVert>\frac{\hat{K}}{\left(2\lVert P^{t}\rVert\right)^{c}}\frac{1}{\lvert\bm{q}\rvert^{c}}.

3.3 Using Moser to Linearize the Central Translations

Theorem 3.7.

For a chosen integer regularity k^\hat{k}\in\mathbb{N}, if fCRf\in C^{R} is C6c+1C^{6c+1}-close to FF and FF is RR-bunched, with R3k^+3c+2R\geq 3\hat{k}+3c+2 and R9c+4R\geq 9c+4, there exist h:𝒞ch:\mathcal{C}\to\mathbb{R}^{c}, which is Ck^C^{\hat{k}}, so that

hTnh1(x)=x+Pnh\circ T_{n}\circ h^{-1}(x)=x+Pn

where P:dcP:\mathbb{Z}^{d}\to\mathbb{R}^{c} is exactly as defined in § 3.2 for the nearby linear map FF.

This is essentially already done in [Rod05], we sketch the construction below and explain the regularities.

Recall than in § 2.2 we projected TnT_{n} to maps T~n:CC\tilde{T}_{n}:C\to C of a vector space. We also make the identification C=cC=\mathbb{R}^{c} exactly like we did in § 3.2.

By means of bump functions we can construct h~:cc\tilde{h}:\mathbb{R}^{c}\rightarrow\mathbb{R}^{c} so that

h~T~h~1=R\tilde{h}\circ\tilde{T}_{\ell}\circ\tilde{h}^{-1}=R_{\ell}

for c×{0}d\ell\in\mathbb{Z}^{c}\times\{0\}\subset\mathbb{Z}^{d}, where Rα=xx+αR_{\alpha}=x\mapsto x+\alpha, and for a general ndn\in\mathbb{Z}^{d}

h~T~nh~1C6c+1RPn\tilde{h}\circ\tilde{T}_{n}\circ\tilde{h}^{-1}\approx_{C^{6c+1}}R_{Pn}

(the proximity to the respective translation for the linear map comes from [Rod05, Corollary 2.4]).

To improve this h~\tilde{h} into a simultaneous linearization we follow Moser [Mos90]. Moser shows how to simultaneously linearize commuting perturbations of rotations of the circle with a Diophantine condition analogous to ours by using some KAM type of arguments.

Essentially all the difficulties of generalizing this to general dimension are already taken care by F. Rodriguez-Hertz (the only minor detail is that in the proof of [Rod05, Lemma B.3] it is used the fact that F|CF|_{C} is an isometry, but actually the argument works just as well with the hypothesis of partial hyperbolicity).

In here we will follow the constants in Moser to see how much they can be optimized. Clearly in our case τ=c\tau=c. In lemma 3.1 from Moser there is a convergence that is over c\mathbb{Z}^{c} in our case, making it so that we need σ>2τ+c=3c\sigma>2\tau+c=3c.

In page 119 we leave, for now, the variables κ\kappa and \ell free, and set Ns=εsξN_{s}=\varepsilon_{s}^{-\xi} with ξ\xi free. The conditions needed to make the rest of the page work would be

ξσ+1>κ,\displaystyle\xi\sigma+1>\kappa,
ξ+22>κ,\displaystyle-\xi+2-\frac{2}{\ell}>\kappa,
ξ1>κ.\displaystyle\ell\xi-1>\kappa.

For the next page we leave the variable mm free and we need the argument to work for kk up to k^\hat{k}, so the condition for the argument to work would be

ξσ+1r^mr^mξσ+κ1κ1>0.-\xi\sigma+1-\frac{\hat{r}}{m}-\frac{\hat{r}}{m}\frac{\xi\sigma+\kappa-1}{\kappa-1}>0.

For the argument to work we need existence of derivatives up to order +σ\ell+\sigma and m+σm+\sigma and to control derivatives up order \ell. So we need to optimize those numbers.

Taking κ\kappa close enough to 11 and ξ\xi close enough to κ1σ\frac{\kappa-1}{\sigma} the conditions are satisfied for

>2σ,\displaystyle\ell>2\sigma,
m>3k^.\displaystyle m>3\hat{k}.

Since σ\sigma, \ell and mm need to be integers we can solve the problem with σ=3c+1\sigma=3c+1, =6c+3\ell=6c+3 and m=3k^+1m=3\hat{k}+1.

3.4 Using Fourier to Solve Cohomological Equations for the Central Translations

So far we show that, in a sense, the central translations are Diophantine. We now show that Diophantine translations have no restrictions to solve certain cohomological equations.

Theorem 3.8.

Let the linear map P:dcP:\mathbb{Z}^{d}\to\mathbb{R}^{c}, inducing a d\mathbb{Z}^{d}-action by translations, be Diophantine (see definition 3.4). Further assume that P=P\ell=\ell for any c×{0}d\ell\in\mathbb{Z}^{c}\times\{0\}\subset\mathbb{Z}^{d}.

Then any Cr+2c+HölderC^{r+2c+\text{H\"{o}lder}} cocycle Φ:d×c\Phi:\mathbb{Z}^{d}\times\mathbb{R}^{c}\to\mathbb{R} for the induced action is CrC^{r}-cohomologus to a group morphism λ:d\lambda:\mathbb{Z}^{d}\to\mathbb{R}, that is there is uCr(c,)u\in C^{r}(\mathbb{R}^{c},\mathbb{R}) so that

Φ(n,a)=u(a+Pn)u(a)+λ(n).\Phi(n,a)=u(a+Pn)-u(a)+\lambda(n).

Furthermore λ(n)=[0,1]cΦ(n,a)𝑑a\lambda(n)=\int_{[0,1]^{c}}\Phi(n,a)\,da.

We remark that the condition P=P\ell=\ell can be replaced by Φ\Phi being defined on the torus 𝕋c\mathbb{T}^{c}.

Proof.

For this proof we write c=c×{0}d\mathbb{Z}^{c}=\mathbb{Z}^{c}\times\{0\}\subset\mathbb{Z}^{d} so that P=P\ell=\ell for c\ell\in\mathbb{Z}^{c}. Also we will call “KK” to different constants.

We first project to the torus 𝕋c=c/c\mathbb{T}^{c}=\mathbb{R}^{c}/\mathbb{Z}^{c} by constructing v:cv:\mathbb{R}^{c}\to\mathbb{R} so that Φ~(n,a)=Φ(n,a)+v(a+Pn)v(a)\tilde{\Phi}(n,a)=\Phi(n,a)+v(a+Pn)-v(a) satisfies that Φ~(n,a+)=Φ~(n,a)\tilde{\Phi}(n,a+\ell)=\tilde{\Phi}(n,a) for c\ell\in\mathbb{Z}^{c}.

Soon we will define vv for a[0,1)ca\in[0,1)^{c}, after that we will extend it for a+ca+\ell\in\mathbb{R}^{c}, c\ell\in\mathbb{Z}^{c}, by

v(a+)=v(a)Φ(,a)v(a+\ell)=v(a)-\Phi(\ell,a)

This way we get for c\ell\in\mathbb{Z}^{c}

Φ~(n,a+)\displaystyle\tilde{\Phi}(n,a+\ell) =Φ(n,a+)Φ(n+,a)Φ(,a)+v(a++Pn)v(a+Pn)Φ(,a+Pn)v(a+)v(a)+Φ(,a)\displaystyle=\underbrace{\Phi(n,a+\ell)}_{\Phi(n+\ell,a)-\cancel{\Phi(\ell,a)}}+\underbrace{v(a+\ell+Pn)}_{v(a+Pn)-\Phi(\ell,a+Pn)}\underbrace{-v(a+\ell)}_{-v(a)+\cancel{\Phi(\ell,a)}}
=Φ(n+,a)Φ(,a+Pn)Φ(n,a)+v(a+Pn)v(a)\displaystyle=\underbrace{\Phi(n+\ell,a)-\Phi(\ell,a+Pn)}_{\Phi(n,a)}+v(a+Pn)-v(a)
=Φ~(n,a).\displaystyle=\tilde{\Phi}(n,a).

We only need to choose a smooth v:[0,1)cv:[0,1)^{c}\to\mathbb{R} so that its extension to c\mathbb{R}^{c} is smooth at the boundaries of [0,1]c[0,1]^{c}. For this consider b:[0,1][0,1]b:[0,1]\to[0,1] a bump function (CC^{\infty}, constantly 0 around 0 and constantly 11 around 11) and just define

v(a)=b(ai)Φ(ei,aei)v(a)=-\sum b(a_{i})\Phi(e_{i},a-e_{i})

where eice_{i}\in\mathbb{Z}^{c} are the canonical elements and aia_{i} is the ii-th coordinate of aa. With this definition we can check that vv, when some aia_{i} tends to 11, coincides with the definition given by the extension, from there smoothness is clear.

We can consider now that PP induces an action on the torus 𝕋c\mathbb{T}^{c} with cocycle Φ~\tilde{\Phi} cohomologus to the original cocycle in c\mathbb{R}^{c}. So now we have effectively “projected” our problem to the torus, where we can use Fourier:

Φ~(n,a)=cΦ^n,e2πia.\tilde{\Phi}(n,a)=\sum_{\ell\in\mathbb{Z}^{c}}\hat{\Phi}_{n,\ell}e^{2\pi i\ell\cdot a}.

The cocycle condition (Φ~(n+m,a)=Φ~(n,a)+Φ~(m,a+Pn)\tilde{\Phi}(n+m,a)=\tilde{\Phi}(n,a)+\tilde{\Phi}(m,a+Pn)) now becomes

Φ^n+m,=Φ^n,+Φ^m,e2πiPn\hat{\Phi}_{n+m,\ell}=\hat{\Phi}_{n,\ell}+\hat{\Phi}_{m,\ell}e^{2\pi i\ell\cdot Pn}

which implies Φ^n,+Φ^m,e2πiPn=Φ^m,+Φ^n,e2πiPm\hat{\Phi}_{n,\ell}+\hat{\Phi}_{m,\ell}e^{2\pi i\ell\cdot Pn}=\hat{\Phi}_{m,\ell}+\hat{\Phi}_{n,\ell}e^{2\pi i\ell\cdot Pm} because we can commute the roles on nn and mm. From there

Φ^n,e2πiPn1=Φ^m,e2πiPm1.\frac{\hat{\Phi}_{n,\ell}}{e^{2\pi i\ell\cdot Pn}-1}=\frac{\hat{\Phi}_{m,\ell}}{e^{2\pi i\ell\cdot Pm}-1}. (1)

Now we want to solve the original problem in this context: that is finding ww and λ\lambda so that

Φ~(n,a)=w(a+Pn)w(a)+λ(n).\tilde{\Phi}(n,a)=w(a+Pn)-w(a)+\lambda(n).

Of course λ(n)=Φ~(n,a)𝑑a\lambda(n)=\int\tilde{\Phi}(n,a)\,da (the cocycle condition for Φ~\tilde{\Phi} translates into the group morphism condition for λ\lambda). Because translations preserve volume we have Φ~(n,a)𝑑a=[0,1]cΦ(n,a)𝑑a\int\tilde{\Phi}(n,a)\,da=\int_{[0,1]^{c}}\Phi(n,a)\,da.

As for the rest of the Fourier coefficients, they should satisfy

w^=Φ^m,e2πiPm1\hat{w}_{\ell}=\frac{\hat{\Phi}_{m,\ell}}{e^{2\pi i\ell\cdot Pm}-1}

which is well defined in light of (1). Furthermore, picking the correct ii for the Diophantine condition 3.4, so that |e2πiPm1|Kd(Pm,)>K||c\lvert e^{2\pi i\ell\cdot Pm-1}\rvert\geq Kd(\ell\cdot Pm,\mathbb{Z})>K\lvert\ell\rvert^{-c}, and using |Φ^ei,|KΦ^ei||r2cε\lvert\hat{\Phi}_{e_{i},\ell}\rvert\leq K\lVert\hat{\Phi}_{e_{i}}\rVert\lvert\ell\rvert^{-r-2c-\varepsilon} we have

|w^|K|Φ^ei,|||cKΦ^ei||r2cε||cK||rcε\left|\hat{w}_{\ell}\right|\leq K\left|\hat{\Phi}_{e_{i},\ell}\right|\left|\ell\right|^{c}\leq K\lVert\hat{\Phi}_{e_{i}}\rVert\lvert\ell\rvert^{-r-2c-\varepsilon}\lvert\ell\rvert^{c}\leq K\lvert\ell\rvert^{-r-c-\varepsilon}

so the Fourier series of w^\hat{w} converges to a Cr+HölderC^{r+\text{H\"{o}lder}} function.

We now think of this ww as defined in c\mathbb{R}^{c} and set u=v+wu=v+w. ∎

3.5 Minimality of the Central Translations

Here is a small lemma that we will need later:

Lemma 3.9.

Any orbit for the central translations Tn:𝒞𝒞T_{n}:\mathcal{C}\to\mathcal{C} (as nn varies along d\mathbb{Z}^{d}) is dense.

Proof.

In virtue of lemma 3.7 we only need to prove this in the linear case where Tn:ccT_{n}:\mathbb{R}^{c}\to\mathbb{R}^{c} is of the form Tna=a+PnT_{n}a=a+Pn, where PP satisfies the Diophantine condition of definition 3.4 and P=P\ell=\ell for c×{0}d\ell\in\mathbb{Z}^{c}\times\{0\}\subset\mathbb{Z}^{d}.

Because of the P=P\ell=\ell condition we can think of TnT_{n} as acting on the torus 𝕋c\mathbb{T}^{c} and we just need to show that the set {Pn}nd𝕋c\{Pn\}_{n\in\mathbb{Z}^{d}}\subset\mathbb{T}^{c} is dense.

Because of classification of closed Lie groups is easy to see that, for some sub-torus V𝕋cV\subset\mathbb{T}^{c} and finite subgroup Q𝕋cQ\subset\mathbb{T}^{c},

{Pn}¯=V+Q.\overline{\{Pn\}}=V+Q.

If V𝕋dV\subsetneq\mathbb{T}^{d} then we can get an integer vector pcp\in\mathbb{Z}^{c} perpendicular to VV and (by multiplying for example by the least common multiple of the denominators of all the coordinates of all elements of QQ) so that pqp\cdot q\in\mathbb{Z} for every qQq\in Q.

So now for every ndn\in\mathbb{Z}^{d} we have Pn=v+qPn=v+q for some vVv\in V and qQq\in Q, but then Pnp=qpPn\cdot p=q\cdot p\in\mathbb{Z}, but this contradict the Diophantine condition and so V=𝕋dV=\mathbb{T}^{d} and the orbit of 0 (and hence any orbit) is dense. ∎

4 Proof of Theorem A

4.1 Solving the Cohomological Equation Along a Central Leaf

4.1.1 Constructing the Solution

With our work so far we can solve cohomological equations for the central translations TnT_{n}. This begs to question: how is this relevant to the original dynamic ff?

The idea now is to capture the information of the holonomy functional into a cocycle for the central translations:

Hol(n,x)=Holx+nTnxφ.\operatorname{Hol}(n,x)=\operatorname{Hol}_{x+n}^{T_{n}x}\varphi.

Indeed this is a cocycle for TnT_{n} (in what follows we use that the susu-foliation and φ\varphi are d\mathbb{Z}^{d}-invariant, and (Add.)):

Hol(n+m,x)\displaystyle\operatorname{Hol}(n+m,x) =Holx+n+mTn+mxφ\displaystyle=\operatorname{Hol}_{x+n+m}^{T_{n+m}x}\varphi
=(Holx+n+mTmx+n+HolTmx+nTn+mx)φ\displaystyle=\left(\operatorname{Hol}_{x+n+m}^{T_{m}x+n}+\operatorname{Hol}_{T_{m}x+n}^{T_{n+m}x}\right)\varphi
=(Holx+mTmx+Hol(Tmx)+nTn(Tmx))φ\displaystyle=\left(\operatorname{Hol}_{x+m}^{T_{m}x}+\operatorname{Hol}_{(T_{m}x)+n}^{T_{n}(T_{m}x)}\right)\varphi
=Hol(m,x)+Hol(n,Tmx).\displaystyle=\operatorname{Hol}(m,x)+\operatorname{Hol}(n,T_{m}x).

Using theorem 3.7 we have hh such that h(Tnx)=h(x)+Pnh(T_{n}x)=h(x)+Pn, with PP Diophantine in the sense of definition 3.4. So

Hol^(n,a)=Hol(n,h1(a))\widehat{\operatorname{Hol}}(n,a)=\operatorname{Hol}\left(n,h^{-1}(a)\right)

is a cocycle for the action of PP by translations. So we can apply theorem 3.8 getting:

Hol^(n,a)=u^(a+Pn)u^(a)+λ(n)\widehat{\operatorname{Hol}}(n,a)=\hat{u}(a+Pn)-\hat{u}(a)+\lambda(n)

which in turn gives us an analogous result for the TnT_{n}-cocycle:

Hol(n,x)=u(Tnx)u(x)+λ(n)\operatorname{Hol}(n,x)=u(T_{n}x)-u(x)+\lambda(n) (2)

where u=u^hu=\hat{u}\circ h.

As far as regularities go, this uu comes from theorem 3.8, so it would be Ck+HölderC^{k+\text{H\"{o}lder}} if Hol^\widehat{\operatorname{Hol}} and hh are Ck+2c+HölderC^{k+2c+\text{H\"{o}lder}}. From lemma 2.7 we need FF to be (k+2c+ε)(k+2c+\varepsilon)-strongly bunched for Holx+nTnxφ=Holx+nπc(x+n)φ\operatorname{Hol}_{x+n}^{T_{n}x}\varphi=\operatorname{Hol}_{x+n}^{\pi^{c}(x+n)}\varphi to be this regular (on top of φ\varphi itself being this regular).

On the other hand hh comes from theorem 3.7, so we need ff to be C6c+1C^{6c+1}-close to FF and FF to be both (3k+9c+3)(3k+9c+3) and (9c+4)(9c+4)-bunched.

4.1.2 Properties of The Solution

Several of the obvious computations needed in the rest of this notes would have a “troublesome” λ\lambda, so we get it out of the way already by proving that it is 0.

Lemma 4.1.

In equation (2) we have λ=0\lambda=0.

Proof.

We know that λ(n)=Hol^[0,1]c(n,a)𝑑a\lambda(n)=\int\widehat{\operatorname{Hol}}_{[0,1]^{c}}(n,a)\,da from lemma 3.8. So our strategy is to show that Holx+nTnx\operatorname{Hol}_{x+n}^{T_{n}x} grows sub-linearly on nn (uniformly so in xx), implying that in order for λ\lambda to be linear it has no other choice than to be 0.

We call Snx=𝒲s(x+n)𝒲u(Tnx)S_{n}x=\mathcal{W}^{s}(x+n)\cap\mathcal{W}^{u}(T_{n}x), that is the point so that

Holx+nTnxφ=\displaystyle\operatorname{Hol}_{x+n}^{T_{n}x}\varphi= (0φ(fi(x+n))φ(fiSnx))\displaystyle\left(\sum\limits_{0}^{\infty}\varphi(f^{i}(x+n))-\varphi(f^{i}S_{n}x)\right)
(1φ(fi(Snx))φ(fiTnx)).\displaystyle-\left(\sum\limits_{1}^{\infty}\varphi(f^{-i}(S_{n}x))-\varphi(f^{-i}T_{n}x)\right).

We will prove that 0φ(fi(x+n))φ(fiSnx)\sum_{0}^{\infty}\varphi(f^{i}(x+n))-\varphi(f^{i}S_{n}x) is sub-linear in nn (the other half is analogous). It is clear, since all leaves are close to the linear leaves, that the distance between x+nx+n and SnxS_{n}x is linearly bounded in nn, and since the stable manifold contracts exponentially there is i(n)i(n) (logarithmically in nn) so that fi(n)+j(x+n)f^{i(n)+j}(x+n) and fi(n)+jSnxf^{i(n)+j}S_{n}x are at distance at most μj\mu^{j} for μ<1\mu<1 the contraction rate of the partial hyperbolicity. So

i(n)φ(fi(x+n))φ(fiSnx)<K\sum\limits_{i(n)}^{\infty}\varphi(f^{i}(x+n))-\varphi(f^{i}S_{n}x)<K

and

Holx+nTnxφ<2i(n)maxφ+K.\operatorname{Hol}_{x+n}^{T_{n}x}\varphi<2i(n)\max\varphi+K.

Now we can solve the cohomological equation along the central leaf:

Lemma 4.2.

The uu of equation (2) satisfies

φ(x)=u(fx)u(x)+const.\varphi(x)=u(fx)-u(x)+\mathrm{const.}

for any x𝒞x\in\mathcal{C}.

Proof.

We will call uf=ufuu_{f}=u\circ f-u (so the objective is to prove that ufφu_{f}-\varphi is constant).

Before the computations notice that f(x+n)=fx+Fnf(x+n)=fx+Fn, where FF is the nearby linear map, and fTnx=TFnfxfT_{n}x=T_{Fn}fx (since both lie in 𝒲su(fx+Fn)𝒞\mathcal{W}^{su}(fx+Fn)\cap\mathcal{C}). We will further use equation (FT) in one of the steps.

uf(Tnx)uf(x)\displaystyle u_{f}(T_{n}x)-u_{f}(x) =u(fTnx)u(fx)(u(Tnx)u(x))\displaystyle=u(fT_{n}x)-u(fx)-(u(T_{n}x)-u(x))
=u(TFnfx)u(fx)Holx+nTnxφ\displaystyle=u(T_{Fn}fx)-u(fx)-\operatorname{Hol}_{x+n}^{T_{n}x}\varphi
=Holfx+FnTFnfxφHolx+nTnxφ\displaystyle=\operatorname{Hol}_{fx+Fn}^{T_{Fn}fx}\varphi-\operatorname{Hol}_{x+n}^{T_{n}x}\varphi
=(Holf(x+n)fTnxHolx+nTnx)φ\displaystyle=\left(\operatorname{Hol}_{f(x+n)}^{fT_{n}x}-\operatorname{Hol}_{x+n}^{T_{n}x}\right)\varphi
=φ(Tnx)φ(x+n)\displaystyle=\varphi(T_{n}x)-\varphi(x+n)
=φ(Tnx)φ(x).\displaystyle=\varphi(T_{n}x)-\varphi(x).

So we have concluded

uf(x)φ(x)=uf(Tnx)φ(Tnx),u_{f}(x)-\varphi(x)=u_{f}(T_{n}x)-\varphi(T_{n}x),

so from continuity and minimality of the action of TnT_{n} (lemma 3.9) we conclude that indeed ufφu_{f}-\varphi is constant. ∎

4.2 Extending the Solution

So after § 4.1 we have u:𝒞u:\mathcal{C}\to\mathbb{R} that satisfies the cohomological equation (\star1). We just need to extend it, first to d\mathbb{R}^{d} because of our abuse of notation and then show that it projects to 𝕋d\mathbb{T}^{d} (and that it is indeed a solution). Such extension will be

u(x)=u(πcx)Holxπcxφu(x)=u(\pi^{c}x)-\operatorname{Hol}_{x}^{\pi^{c}x}\varphi

where the right hand side uu is well defined since πcx𝒞\pi^{c}x\in\mathcal{C}.

Lemma 4.3.

This uu satisfies the cohomological equation (\star1).

Proof.

First notice that πcfx=fπcx\pi^{c}fx=f\pi^{c}x since the foliations are ff-invariant. In what follows we will use lemma 4.2 and the “fundamental” theorem (FT).

u(fx)u(x)\displaystyle u(fx)-u(x) =u(fπcx)u(πcx)(HolfxfπcxHolxπcx)φ\displaystyle=u(f\pi^{c}x)-u(\pi^{c}x)-\left(\operatorname{Hol}_{fx}^{f\pi^{c}x}-\operatorname{Hol}_{x}^{\pi^{c}x}\right)\varphi
=φ(πcx)K(φ(πcx)φ(x))\displaystyle=\varphi(\pi^{c}x)-K-(\varphi(\pi^{c}x)-\varphi(x))
=φ(x)K.\displaystyle=\varphi(x)-K.

Lemma 4.4.

This uu is well defined on the torus 𝕋d\mathbb{T}^{d}, that is u(x+n)=u(x)u(x+n)=u(x) for every ndn\in\mathbb{Z}^{d}.

Proof.

First we notice that πc(x+n)=Tnπcx\pi^{c}(x+n)=T_{n}\pi^{c}x since both lie in the intersection 𝒲su(x+n)𝒞\mathcal{W}^{su}(x+n)\cap\mathcal{C}. We will also use the d\mathbb{Z}^{d}-invariance of φ\varphi, the definition of uu along 𝒞\mathcal{C} given in § 4.1 (that is u(Tnx)u(x)=Holx+nTnxφu(T_{n}x)-u(x)=\operatorname{Hol}_{x+n}^{T_{n}x}\varphi), and (Add.).

u(x+n)u(x)\displaystyle u(x+n)-u(x) =u(πc(x+n))u(πcx)(Holx+nπc(x+n)Holxπcx)φ\displaystyle=u(\pi^{c}(x+n))-u(\pi^{c}x)-\left(\operatorname{Hol}_{x+n}^{\pi^{c}(x+n)}-\operatorname{Hol}_{x}^{\pi^{c}x}\right)\varphi
=u(Tnπcx)u(πcx)(Holx+nTnπcxHolx+nπcx+n)φ\displaystyle=u(T_{n}\pi^{c}x)-u(\pi^{c}x)-\left(\operatorname{Hol}_{x+n}^{T_{n}\pi^{c}x}-\operatorname{Hol}_{x+n}^{\pi^{c}x+n}\right)\varphi
=Holπcx+nTnπcxφHolπcx+nTnπcxφ\displaystyle=\operatorname{Hol}_{\pi^{c}x+n}^{T_{n}\pi^{c}x}\varphi-\operatorname{Hol}_{\pi^{c}x+n}^{T_{n}\pi^{c}x}\varphi
=0\displaystyle=0

Let us clarify the regularity of the uu. If we are in conditions for the u:𝒞u:\mathcal{C}\to\mathbb{R} to be Cr+HölderC^{r+\text{H\"{o}lder}} described in § 4.1, and using the second part of lemma 2.7 then the extended uu is uniformly Cr+HölderC^{r+\text{H\"{o}lder}} along 𝒲c\mathcal{W}^{c}.

The only dependence on the direction susu of our uu is the top xx in Holx0xφ\operatorname{Hol}_{x_{0}}^{x}\varphi, so using the first part of lemma 2.7 we have the desired regularity along this direction.

So using Journé’s lemma [Jou88] we have that uu is CrC^{r} if we have enough regularities and bunching.

Appendix A Appendix

A.1 Regularities for Theorem A

When trying to apply our theorem one would need to know how much bunching is needed, so below we clarify exactly the bunching and regularities needed.

Theorem A’.

For this theorem we call cpc_{p} the dimension of the central distribution for the partial hyperbolic splitting and c1c_{1} the dimension of the generalized eigenspace of eigenvalues of modulus 11 for the nearby linear map FF.

Fix a desired integer regularity kk\in\mathbb{N} and define the minimum regularity bounds as

Rb\displaystyle R_{b} {max{3k+9c1+3,9cp+4}if c10,max{k+ε,9cp+4}if c1=0,\displaystyle\geq\begin{cases}\max\{3k+9c_{1}+3,9c_{p}+4\}\quad&\text{if }c_{1}\neq 0,\\ \max\{k+\varepsilon,9c_{p}+4\}\quad&\text{if }c_{1}=0\end{cases},
Rsb\displaystyle R_{sb} >max{k+2c1,2cp}.\displaystyle>\max\{k+2c_{1},2c_{p}\}.

In theorem A if we want uCk+Hölderu\in C^{k+\text{H\"{o}lder}} the exact regularities needed are as follow:

General Case

T

  • FF needs to be RbR_{b}-bunched and ff needs to be CRbC^{R_{b}},

  • FF needs to be strongly RsbR_{sb}-bunched and φ\varphi needs to be CRsbC^{R_{sb}}, and

  • ff needs to be C6cp+1C^{6c_{p}+1}-close to FF.

Linear Case

In the case where f=Ff=F is linear

  • FF needs to be strongly RsbR_{sb}-bunched and φ\varphi needs to be CRsbC^{R_{sb}}.

Or

  • FF needs to be strongly (2cp+ε)(2c_{p}+\varepsilon)-bunched, and

  • φ\varphi needs to be Ck+d+HölderC^{k+d+\text{H\"{o}lder}}.

Low center dimension

If cp=1c_{p}=1 and c1=0c_{1}=0

  • FF needs to be (4+ε)(4+\varepsilon)-bunched and ff needs to be C4+HölderC^{4+\text{H\"{o}lder}}-close to FF, and

  • FF needs to be strongly RsbR_{sb}-bunched and φ\varphi needs to be CRsbC^{R_{sb}}.

If cp=c1=2c_{p}=c_{1}=2 and FF is irreducible with d>4d>4 (or the irreducible factor containing the complex eigenvalues is of degree more than 44)

  • ff needs to be C4k+8+HölderC^{4k+8+\text{H\"{o}lder}}-close to FF, and

  • φ\varphi needs to be Ck+4+HölderC^{k+4+\text{H\"{o}lder}}.

Proof.

Notice that we are always able to bootstrap the regularity of the solution by applying the theorem with k=0k=0 first. After corollary B and remark 2.3 we have jointly integrability for any of the splittings coming from any partial hyperbolic splitting of FF. So, once we know that φ\varphi is a coboundary, we can assume that the center direction is (the perturbation of) the generalized eigenspace of eigenvalues of modulus 11 (or, if the case allows it, apply Livsic or Veech [Vee86]).

In the general case is only a matter of following the regularities along the proof.

For the linear case on one hand we don’t need to use Moser to linearize the central translations. Also in some cases it might be better to bootsrap using Veech.

In the low dimensional cases we can get the Diophantine property with just one translation (see [Rod05, Lemma A.11] for the case c=2c=2), so we can bypass Moser and use a more traditional KAM theory instead (see [Her79, § A.2] and [Rod05, § 6.1]). ∎

We can go even further saying that φ\varphi only needs to be CRsbC^{R_{sb}} along the central direction while in the susu-direction it only needs to be CkC^{k}. Furthermore if we ask uu to be CkC^{k} along the central direction and CC^{\ell} along the susu-direction (with k\ell\leq k) we need φ\varphi to be CRsbC^{R_{sb}} along the central direction and CC^{\ell} along the susu-direction. In here we asking for the regularities to be uniform.

We remark that, after [Vee86, Proposition 1.5], at least some regularity is expected to be lost. We do not claim that our specific regularity loss and bunching are optimal, although probably more refined techniques would be needed to make significant improvements in these numbers.

A.2 A Couple of Toy Examples

For this section we use the holonomy functionals defined in § 2.3.

The simplest example where we can use the idea of solving the equation along susu-leaves and along central leaves independently and then join the solutions would be (x,y)(x+α,Ay)(x,y)\to(x+\alpha,Ay) where α\alpha is Diophantine and AA is Anosov. For the sake of generality we prove something stronger.

Theorem A.1.

Let f:MMf:M\to M be partially hyperbolic so that (\star1) admits a solution for any φ\varphi with trivial periodic cycle functionals, and let f~:M×NM×N\tilde{f}:M\times N\to M\times N and hyperbolic extension

f~(x,y)=(fx,gxy)\tilde{f}(x,y)=(fx,g_{x}y)

so that there is a probability measure μ\mu preserved by gxg_{x} for every xx (and so that the expansion and contraction along NN dominate the center direction of ff).

Then f~\tilde{f} is cocycle stable.

Theorem A.2.

Let f:MMf:M\to M be cocycle stable and consider the suspension space M~=(×M)/f\tilde{M}=(\mathbb{R}\times M)/f where (x,y)(x1,fy)(x,y)\sim(x-1,fy). For α\alpha Diophantine the map f~:M~M~\tilde{f}:\tilde{M}\to\tilde{M}

f~(x,y)=(x+α,y)\tilde{f}(x,y)=(x+\alpha,y)

is cocycle stable

The proof for both theorems is the same (that is the reason for the awkward notation in the second theorem).

Proof.

For the second theorem consider μ\mu an invariant measure for ff.

If φ\varphi has trivial periodic cycle functionals then it easy to see that so does

φμ(x)=Nφ(x,z)𝑑μ(z)\varphi_{\mu}(x)=\int_{N}\varphi(x,z)\,d\mu(z)

and so we can solve

φμ(x)=uμ(fx)uμ(x)+K.\varphi_{\mu}(x)=u_{\mu}(fx)-u_{\mu}(x)+K.

Now define

u(x,y)=uμ(x)+NHol(x,z)(x,y)φdμ(z).u(x,y)=u_{\mu}(x)+\int_{N}\operatorname{Hol}_{(x,z)}^{(x,y)}\varphi\,d\mu(z).

Now, using (FT), we show

u(f~(x,y))u(x,y)\displaystyle u(\tilde{f}(x,y))-u(x,y) =uμ(fx)uμ(x)+N(Holf~(x,z)f~(x,y)Hol(x,z)(x,y))φ𝑑μ(z)\displaystyle=u_{\mu}(fx)-u_{\mu}(x)+\int_{N}\left(\operatorname{Hol}_{\tilde{f}(x,z)}^{\tilde{f}(x,y)}-\operatorname{Hol}_{(x,z)}^{(x,y)}\right)\varphi\,d\mu(z)
=Nφ(x,z)𝑑μ(z)K+N(φ(x,y)φ(x,z))𝑑μ(z)\displaystyle=\int_{N}\varphi(x,z)\,d\mu(z)-K+\int_{N}(\varphi(x,y)-\varphi(x,z))\,d\mu(z)
=φ(x,y)K.\displaystyle=\varphi(x,y)-K.

And interesting example of the first theorem would be and automorphism FF of a nilmanifold NN so that the fibers of the map π:N𝕋a\pi:N\to\mathbb{T}^{a} are hyperbolic and so that the projection of FF to 𝕋a\mathbb{T}^{a} is Katznelson irreducible. These properties are easy to check: if

DF=(A1A20Ak1Ak)DF=\begin{pmatrix}A_{1}&&&&\\ &A_{2}&&\mbox{\huge$\ast$}&\\ &&\ddots&&\\ &\mbox{\huge$0$}&&A_{k-1}\\ &&&&A_{k}\end{pmatrix}

is so that AiA_{i} is hyperbolic for i=1,,k1i=1,\dots,k-1 and AkA_{k} is Katznelson irreducible, with respect to the partial hyperbolic splitting which should have its center direction on the coordinates corresponding to AkA_{k}, then FF is cocycle stable.

This proof actually work for any map that has a cocycle stable factor and whose fibers are hyperbolic (dominating the center of the factor) with “good enough” transversal measures.

“Good enough” might be a smooth volume for instance. We can alway use axiom of choice to create the transversal measures but in this case the solution uu wouldn’t even be measurable.

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