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Julia Sets of Hyperbolic Rational Maps have Positive Fourier Dimension

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Abstract

Let \(f:\widehat{{\mathbb {C}}}\rightarrow \widehat{{\mathbb {C}}}\) be a hyperbolic rational map of degree \(d \ge 2\), and let \(J \subset {\mathbb {C}}\) be its Julia set. We prove that J always has positive Fourier dimension. The case where J is included in a circle follows from a recent work of Sahlsten and Stevens (Fourier transform and expanding maps on Cantor sets preprint. arXiv:2009.01703, 2020). In the case where J is not included in a circle, we prove that a large family of probability measures supported on J exhibit polynomial Fourier decay: our result applies in particular to the measure of maximal entropy and to the conformal measure.

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Acknowledgements

The author would like to thank his PhD supervisor, Frederic Naud, for numerous helpful conversations and for pointing out various helping references. The author would also like to thank Jialun Li for introducing him to the method of Dolgopyat. The author would like to thank the referee for useful remarks concerning the historical overview and for spotting a few missing arguments in the text. This work is part of the author’s PhD and is funded by the Ecole Normale Superieure de Rennes. The author have no relevant financial or non-financial interests to disclose.

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Correspondence to Gaétan Leclerc.

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Appendices

Appendix A Large Deviations

The goal of this section is to prove the large deviation Theorem 2.8, by using properties of the pressure.

The link between the spectral radius of \({\mathcal {L}}_\varphi \) and the pressure given by the Perron-Frobenius-Ruelle theorem allows us to get the following useful formula. We extract the first one from [Ru78], Theorem 7.20 and remark 7.28, and the second one from [Ru89], lemma 4.5.

Proposition A.1

 

$$\begin{aligned} P(\varphi )= & {} \lim _{n \rightarrow \infty } \frac{1}{n} \log \sum _{f^n(x)=x} e^{S_n \varphi (x)}\\ P(\varphi )= & {} \lim _{n \rightarrow \infty } \frac{1}{n} \max _{b \in {\mathcal {A}}} \sup _{x \in P_b} \log \underset{{\mathbf {a}} \rightsquigarrow b}{\sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} } e^{S_n \varphi ( g_{{{\textbf {a}}}}(x) )} \end{aligned}$$

We begin by proving another avatar of those spectral radius formulas (which is nothing new).

Lemma A.2

Choose any \(x_{{{\textbf {a}}}}\) in each of the \(P_{{{\textbf {a}}}}\), \({{\textbf {a}}} \in {\mathcal {W}}_{n}\), \(\forall n\). Then

$$\begin{aligned} P(\varphi ) = \lim _n \frac{1}{n} \log \sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} e^{S_n \varphi (x_{{\textbf {a}}})} . \end{aligned}$$

Proof

Since \(P_{{{\textbf {a}}}}\) is compact, and by continuity, for every n there exists \(b^{(n)} \in {\mathcal {A}}\) and \(y_{b^{(n)}}^{(n)} \in P_{b^{(n)}}\) such that

$$\begin{aligned} \max _{b \in {\mathcal {A}}} \sup _{x \in P_b} \log \underset{{\mathbf {a}} \rightsquigarrow b}{\sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} } e^{S_n \varphi ( g_{{{\textbf {a}}}}(x) )} = \log \underset{{\mathbf {a}} \rightsquigarrow b^{(n)}}{\sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} } e^{S_n \varphi ( g_{{{\textbf {a}}}}(y_{b^{(n)}}^{(n)}) )}. \end{aligned}$$

Define \(y_{{{\textbf {a}}}} := g_{{{\textbf {a}}}}(y_{b^{(n)}}^{(n)}) \in P_{{{\textbf {a}}}}\) for clarity. The dependence on n is not lost since it is contained in the length of the word. First of all, since \(\varphi \) has exponentially vanishing variations, there exists a constant \(C_1>0\) such that

$$\begin{aligned} \forall x,y \in P_{{{\textbf {a}}}}, \ | S_n \varphi (x) - S_n \varphi (y) |\le C_1 . \end{aligned}$$

Now we want to relate the sums with the \(x_{\mathbf {a}}\)’s and the \(y_{{\mathbf {a}}}\)’s, but the indices are different. To do it properly, we are going to use the fact that f is topologically mixing: there exists some \(N \in {\mathbb {N}}\) such that the matrix \(M^N\) has all its entries positive. In particular, it means that

$$\begin{aligned} \forall b \in {\mathcal {A}}, \ \forall {{\textbf {a}}} \in {\mathcal {W}}_{n+1}, \ \exists {{\textbf {c}}} \in {\mathcal {W}}_{N}, \ {\textbf {ac}}b \in {\mathcal {W}}_{n+N+1} . \end{aligned}$$

The point is that we are sure that the word is admissible.

For a given \({{\textbf {a}}} \in {\mathcal {W}}_{n+1}\), there exists a \({{\textbf {c}}} \in {\mathcal {W}}_{N}\) such that \( {\textbf {ac}}b^{(n+N+1)} \in {\mathcal {W}}_{n+N+1}\), and so, using the fact that \(e^{S_n \varphi } \ge 0\), we get:

$$\begin{aligned} e^{S_n \varphi (x_{{{\textbf {a}}}})} \le \underset{ {\textbf {ac}}b^{(n+N+1)} \in {\mathcal {W}}_{n+N+1}}{\sum _{{{\textbf {c}}} \in {\mathcal {W}}_{N} }} e^{C_1} e^{S_n \varphi (y_{{\textbf {ac}}b^{(n+N+1)}})} . \end{aligned}$$

Then, since \(S_{n}(\varphi ) \le S_{n+N}(\varphi ) +N \Vert \varphi \Vert _{\infty ,J}\), we have:

$$\begin{aligned} e^{S_n \varphi (x_{{{\textbf {a}}}})} \le \underset{ {\textbf {ac}}b^{(n+N+1)} \in {\mathcal {W}}_{n+N+1}}{\sum _{{{\textbf {c}}} \in {\mathcal {W}}_{N} }} e^{C_2} e^{S_{n+N}(\varphi )(y_{{\textbf {ac}}b^{(n+N+1)}})} . \end{aligned}$$

Hence

$$\begin{aligned} \log \left( {\sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} } e^{S_n \varphi ( x_{{{\textbf {a}}}} )} \right)\le & {} \log \left( \sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} \underset{ {\textbf {ac}}b^{(n+N+1)} \in {\mathcal {W}}_{n+N+1}}{\sum _{{{\textbf {c}}} \in {\mathcal {W}}_{N} }} e^{C_2} e^{S_{n+N} \varphi (y_{{\textbf {ac}}b^{(n+N+1)}})} \right) \\= & {} C_2 + \log \left( \underset{{\mathbf {d}} \rightsquigarrow b^{(n+N+1)}}{\sum _{{{\textbf {d}}} \in {\mathcal {W}}_{n+N+1} }} e^{S_n \varphi (y_{{{\textbf {d}}}})} \right) , \end{aligned}$$

and so

$$\begin{aligned} \limsup _{n \rightarrow \infty } \frac{1}{n} \log \left( {\sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} } e^{S_n \varphi ( x_{{{\textbf {a}}}} )} \right) \le P(\varphi ) . \end{aligned}$$

The other inequality is easier, we have

$$\begin{aligned} \log \left( \underset{ {\mathbf {a}} \rightsquigarrow b^{(n)}}{\sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} } e^{S_n \varphi ( y_{{{\textbf {a}}}} )} \right) \le C_1 + \log \left( \sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} e^{S_n \varphi (x_{{{\textbf {a}}}})} \right) , \end{aligned}$$

which gives us

$$\begin{aligned} P(\varphi ) \le \liminf \frac{1}{n} \log \left( \sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} e^{S_n \varphi (x_{{{\textbf {a}}}})} \right) . \end{aligned}$$

\(\square \)

Another useful formula is the computation of the differential of the pressure.

Theorem A.3

The map \(P : C^1(U,{\mathbb {R}}) \rightarrow {\mathbb {R}} \) is differentiable. If \(\varphi \in C^1(U,{\mathbb {R}})\) is a normalized potential, then we have:

$$\begin{aligned} \forall \psi \in C^1(U,{\mathbb {R}}), \ (dP)_{\varphi }(\psi ) = \int _J \psi d\mu _{\varphi } . \end{aligned}$$

Proof

This is the corollary 5.2 in [Ru89]. Loosely, the argument goes as follows.

The differentiability is essentially a consequence of the fact that \(e^{P(\psi )}\) is an isolated eigenvalue of \({\mathcal {L}}_\psi \). To compute the differential, consider \(v_t \in C^1\) the normalized eigenfunction for \({\mathcal {L}}_{\varphi + t \psi }\) such that \(v_0=1\). We have, for small t:

$$\begin{aligned} {\mathcal {L}}_{\varphi + t \psi } v_t = e^{P(\varphi + t \psi )} v_t \end{aligned}$$

Hence,

$$\begin{aligned} {\mathcal {L}}_{\varphi + t \psi } (\psi v_t ) + {\mathcal {L}}_{\varphi + t \psi } (\partial _t v_t) = v_t e^{P(\varphi + t \psi )} \frac{d}{dt} P(\varphi + t \psi ) + e^{P(\varphi + t \psi )} \partial _t v_t \end{aligned}$$

Taking \(t=0\) and integrating against \(\mu _\varphi \) gives

$$\begin{aligned} (d P)_{\varphi }(\psi ) = \int _J {\mathcal {L}}_{\varphi }(\psi ) d\mu _\varphi = \int _J \psi d\mu _\varphi . \end{aligned}$$

\(\square \)

Now, we are ready to prove Theorem 2.8. The proof is adapted from [JS16], subsection 4.

Proof

Let \(\varphi \) be a normalized potential, and let \(\psi \) be another \(C^1\) potential. Let \(\varepsilon > 0\). Let \(j(t) := P\left( (\psi - \int \psi d\mu _\varphi - \varepsilon )t + \varphi \right) \). We know by Theorem A.3 that \(j'(0) = -\varepsilon < 0\). Hence, there exists \(t_0> 0\) such that \(P( (\psi - \int \psi d\mu _\varphi - \varepsilon )t_0 + \varphi ) < 0\).

Define \(2 \delta _0 := -P\left( (\psi - \int \psi d\mu _\varphi - \varepsilon )t_0 + \varphi \right) \). We then have

$$\begin{aligned} \mu _\varphi \left( \left\{ x \in J \ , \ \frac{1}{n} S_n \psi (x) - \int _J \psi d\mu _{\varphi } \ge \varepsilon \right\} \right) \le \sum _{{{\textbf {a}}} \in C_{n+1}} \mu _\varphi (P_{\mathbf {a}}) , \end{aligned}$$

where \(C_{n+1} := \{ {\mathbf {a}} \in {\mathcal {W}}_{n+1} \ | \ \exists x \in P_{{\mathbf {a}}} , \ S_n \psi (x)/n - \int \psi d\mu _{\varphi } \ge \varepsilon \} \). For each \({\mathbf {a}}\) in some \(C_{n+1}\), choose \(x_{{\mathbf {a}} } \in P_{{\mathbf {a}} }\) such that \(S_n \psi (x_{{\mathbf {a}} })/n - \int \psi d\mu _{\varphi } \ge \varepsilon \). For the other \({\mathbf {a}}\), choose \(x_{{\mathbf {a}}} \in P_{{{\textbf {a}}}}\) randomly.

Now, since \(\mu _\varphi \) is a Gibbs measure, there exists \(C_0>0\) such that:

$$\begin{aligned} \sum _{{{\textbf {a}}} \in C_{n+1}} \mu _\varphi (P_{\mathbf {a}})\le & {} C_0 \sum _{{{\textbf {a}}} \in C_{n+1}} \exp (S_n \varphi (x_{{\textbf {a}}})) \\\le & {} C_0 \sum _{{{\textbf {a}}} \in C_{n+1}} \exp \left( {S_n\left( \left( \psi -\int \psi d\mu _\varphi - \varepsilon \right) t_0 + \varphi \right) (x_{{\textbf {a}}} )} \right) \\\le & {} C_0 \sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} \exp \left( {S_n\left( \left( \psi -\int \psi d\mu _\varphi - \varepsilon \right) t_0 + \varphi \right) (x_{{\textbf {a}}} )} \right) . \end{aligned}$$

Then, by the lemma A.2, we can write for \(n \ge n_0\) large enough:

$$\begin{aligned}&C_0 \sum _{{{\textbf {a}}} \in {\mathcal {W}}_{n+1}} \exp \left( {S_n\left( \left( \psi -\int \psi d\mu _\varphi - \varepsilon \right) t_0 + \varphi \right) (x_{{\textbf {a}}} )} \right) \\&\quad \le C e^{n \delta _0} e^{n P( (\psi - \int \psi d\mu _\varphi - \varepsilon )t_0 + \varphi )} \le C e^{- \delta _0 n} , \end{aligned}$$

and so

$$\begin{aligned} \mu _\varphi \left( \left\{ x \in J \ , \ \frac{1}{n} S_n \psi (x) - \int _X \psi d\mu _{\varphi } \ge \varepsilon \right\} \right) \le Ce^{- n \delta _0} . \end{aligned}$$

The symmetric case is done by replacing \(\psi \) by \(-\psi \), and combining the two gives us the desired bound. \(\square \)

Appendix B Uniform Spectral Estimate for a Family of Twisted Transfer Operator

Here, we will show how to prove Theorem 6.4. It is a generalization of Theorem 2.5 in [OW17]: we will explain what we need to change in the original paper for the theorem to hold more generally.

Proving that a complex transfer operator is eventually contracting is linked to analytic extensions results for dynamical zeta functions, and is often referred to as a spectral gap. Such results are of great interest to study, for example, periodic orbit distribution in hyperbolic dynamical systems (see for example the chapter 5 and 6 in [PP90]), or asymptotics for dynamically defined quantities (as in [OW17] or [PU17]). One of the first result of this kind can be found in a work of Dolgopyat [Do98], in which he used a method that has been broadly extended since. We can find various versions of Dolgopyat’s method in papers of Naud [Na05], Stoyanov [St11], Petkov [PS16], Oh-Winter [OW17], Li [Li18b], and Sharp-Stylianou [ShSt20], to only name a few.

In this annex, we will outline the argument of Dolgopyat’s method as explained in [OW17] adapted to our general setting. We need three ingredients to make the method work: the NLI (non local integrability), the NCP (another non concentration property), and a doubling property.

Definition B.1

Define \(\tau (x) := \log |f'(x)| \in {\mathbb {R}}\) and \(\theta (x) := \arg f'(x) \in {\mathbb {R}}/2 \pi {\mathbb {Z}}.\) The transfer operator in Theorem 6.4 acts on \(C^1_b({\mathfrak {U}},{\mathbb {C}})\) and may be rewritten in the form

$$\begin{aligned} {\mathcal {L}}_{\varphi ,it,l} = {\mathcal {L}}_{\varphi - i t \mathcal {\tau } - i l \mathcal {\theta }}. \end{aligned}$$

For some normalized \(\varphi \in C^1(U,{\mathbb {R}})\), \(l \in {\mathbb {Z}}\) and \(t \in {\mathbb {R}}\).

With those notations, Theorem 6.4 can be rewritten as follows.

Theorem B.1

Suppose that J is not included in a circle. For any \(\varepsilon >0\), there exists \(C>0\), \(\rho <1\) such that for any \(n \ge 1\) and any \(t\in {\mathbb {R}}\), \(l \in {\mathbb {Z}}\) such that \(|t|+|l| > 1\),

$$\begin{aligned} \Vert {\mathcal {L}}_{\varphi - i(t \tau + l \theta )}^n \Vert _{C^1_b({\mathfrak {U}},{\mathbb {C}})} \le C (|l|+|t|)^{1+\varepsilon } \rho ^n \end{aligned}$$

Now we may recall the three main technical ingredients.

Theorem B.2

(NLI, [OW17] section 3). The function \(\tau \) satisfies the NLI property if there exists \(a_0 \in {\mathcal {A}}\), \(x_1 \in P_{a_0}\) , \(N \in {\mathbb {N}}\), admissible words \({\mathbf {a}}, {\mathbf {b}} \in {\mathcal {W}}_{N+1}\) with \(a_0\rightsquigarrow {\mathbf {a}},{\mathbf {b}}\), and an open neighborhood \(U_0\) of \(x_1\) such that for any \(n \ge N\), the map

$$\begin{aligned} ({\tilde{\tau }}, {\tilde{\theta }}) := (S_n \tau \circ g_{\mathbf {a}} - S_n \tau \circ g_{\mathbf {b}}, S_n\theta \circ g_{\mathbf {a}} - S_n\theta \circ g_{\mathbf {b}}) : U_0 \rightarrow {\mathbb {R}} \times {\mathbb {R}}/2 \pi {\mathbb {Z}} \end{aligned}$$

is a local diffeomorphism.

Remark B.1

Remark 4.7 in [SS20] and Proposition 3.8 in [OW17] points out the fact that the NLI is a consequence of our non-linear setting, which itself comes from the fact that we supposed that our Julia set is different from a circle.

Theorem B.3

(NCP, [OW17] section 4). For each \(n \in {\mathbb {N}}\), for any \({\mathbf {a}} \in {\mathcal {W}}_{n+1}\), there exists \(0< \delta < 1\) such that, for all \(x \in P_{\mathbf {a}}\), all \(w \in {\mathbb {C}}\) of unit length, and all \(\varepsilon \in (0, 1) \),

$$\begin{aligned} B(x,\varepsilon ) \cap \{ y \in P_{\mathbf {a}}, \ |\langle y - x, w \rangle | > \delta \varepsilon \} \ne \emptyset \end{aligned}$$

where \(\langle a + bi, c + di \rangle = ac + bd\) for \(a, b, c, d \in {\mathbb {R}}\).

Remark B.2

The NCP is a consequence of the fractal behavior of our Julia set. This time, if J is included in any smooth set, the NCP fails. But in our case, this is equivalent to being included in a circle, see [ES11]. Notice that this non concentration property has nothing to do with our previous non concentration hypothesis.

Theorem B.4

(Doubling). Let, for \(a \in {\mathcal {A}}\), \(\mu _a\) be the equilibrium measure \(\mu _\varphi \) restricted to \(P_a\). Then each \(\mu _a\) is doubling, that is:

$$\begin{aligned} \exists C>0, \ \forall x \in P_a, \ \forall r<1, \ \mu _a(B(x,2r)) \le C \mu _a(B(x,r)). \end{aligned}$$

Proof

It follows from Theorem A.2 in [PW97] that \(\mu _\varphi \) is doubling: the proof uses the conformality of the dynamics. To prove that \(\mu _a := \mu _{| P_a}\) is still doubling, which is not clear a priori, we follow Proposition 4.5 in [OW17] and prove that there exists \(c>0\) such that for any \(a \in {\mathcal {A}}\), for any \(x \in P_a\), and for any \(r>0\) small enough,

$$\begin{aligned} \frac{\mu _\varphi (B(x,r) \cap P_a)}{\mu _\varphi (B(x,r))} > c . \end{aligned}$$

For this we use a Moran cover \({\mathcal {P}}_r\) associated to our Markov partition, see the proof of Proposition 2.7 for a definition. Recall that any element \(P \in {\mathcal {P}}_r\) have diameter strictly less than r, and recall that there exists a constant \(M>0\) independent of x and r such that we can cover the ball B(xr) with M elements of \({\mathcal {P}}_r\). Moreover, lemma 2.2 in [WW17] allows us to do so using elements \(P\in {\mathcal {P}}_r\) of the form \(P_{\mathbf {a}}\) for \({\mathbf {a}}\) in some \({\mathcal {W}}_n\), \(N_0 \le n \le N_0 + L\) for some \(N_0(x,r)\) and some constant L (independent of x and r). We can then conclude as follows. Let \(P^{(1)} , \dots P^{(M)} \in {\mathcal {P}}_r\) that covers B(xr). There exists i such that \(P^{(i)} \subset P_a\). Hence, by the Gibbs property of \(\mu _\varphi \):

$$\begin{aligned} \frac{\mu _\varphi (B(x,r) \cap P_a)}{\mu _\varphi (B(x,r))} \ge \frac{\mu _\varphi (P^{(i)})}{ {\sum _{j=1}^M} \mu _\varphi (P^{(j)})} \ge M^{-1} C_0^{-2} e^{-(L+2)\Vert \varphi \Vert _\infty }. \end{aligned}$$

\(\square \)

Remark B.3

The doubling property (or Federer property) is a regularity assumption made on the measure that is central for the execution of this version of Dolgopyat’s method. It allows us to control integrals over J by integrals over smaller pieces of J, provided some regularity assumption on the integrand.

Now we will outline the argument of Dolgopyat’s method as used in [OW17]. It can be decomposed into four main steps.

Step 1 We reduce Theorem B.1 to a \(L^2(\mu )\) estimate.

We need to define a modified \(C^1\) norm. Denote by \(\Vert \cdot \Vert _r\) a new norm, defined by

$$\begin{aligned} \Vert h\Vert _r := \left\{ \begin{array}{rcl} \Vert h\Vert _{\infty ,{\mathfrak {U}}} + \frac{\Vert \nabla h\Vert _{\infty ,{\mathfrak {U}}}}{r} \ \text {if} \ r \ge 1 \\ \Vert h\Vert _{\infty ,{\mathfrak {U}}} + \Vert \nabla h \Vert _{\infty ,{\mathfrak {U}}} \ \text {if} \ r < 1 \end{array} \right. \end{aligned}$$

Moreover, we do a slight abuse of notation and write \(\mu \) for \(\sum _{a \in {\mathcal {A}}} \mu _a\), seen as a measure on \({\mathfrak {U}}\). This measure is supported on J, seen as the set \(\bigsqcup _a P_a \subset \bigsqcup _a U_a = {\mathfrak {U}}\). The first step is to show that Theorem B.1 reduces to the following claim.

Theorem B.5

Suppose that the Julia set of f is not contained in a circle. Then there exists \(C>0\) and \( \rho \in (0,1)\) such that for any \(h \in C^1_b({\mathfrak {U}},{\mathbb {C}})\) and any \(n \in {\mathbb {N}}\),

$$\begin{aligned} ||{\mathcal {L}}_{\varphi -i(t \tau + l \theta )}^n h||_{L^2(\mu )} \le C \rho ^n \Vert h \Vert _{|t|+|l|} \end{aligned}$$

for all \(t \in {\mathbb {R}}\) and \(\ell \in {\mathbb {Z}}\) with \(|t| + |l| \ge 1\).

A clear account for this reduction may be found in [Na05], section 5. This step holds in great generality without any major difficulty. Intuitively, Theorem B.1 follows from Theorem B.5 by the Lasota-Yorke inequality, by the quasicompactness of \({\mathcal {L}}_\varphi \), and by the Perron-Frobenius-Ruelle theorem, which implies that \({\mathcal {L}}^N_\varphi h\) is comparable to \(\int h d\mu \) for N large. The difference between the two can be controlled using \(C^1\) bounds.

Step 2 We show that the oscillations in the sum induce enough cancellations.

Loosely, the argument goes as follows. We write, for a well chosen and large N:

$$\begin{aligned} \forall x \in U_b, \ {\mathcal {L}}^N_{\varphi - i (t \tau + l \theta )}h(x) = \underset{{\mathbf {a}} \rightsquigarrow b}{\sum _{{\mathbf {a}} \in {\mathcal {W}}_{N+1}} } e^{ i (t S_N \tau + l S_N \theta )(g_{\mathbf {a}}(x))} h(g_{\mathbf {a}}(x))e^{S_N \varphi (g_{\mathbf {a}}(x) ) } . \end{aligned}$$

If we choose x in a suitable open set \({\widehat{S}} \subset U_0\), the NLI and the NCP tell us that we can extract words \({\mathbf {a}}\) and \({\mathbf {b}}\) from this sum such that some cancellations happen. Indeed, if we isolate the term given by the words from the NLI,

$$\begin{aligned} e^{ i (t S_N \tau + l S_N \theta )(g_{\mathbf {a}}(x))} h(g_{\mathbf {a}}(x))e^{S_N \varphi (g_{\mathbf {a}}(x) ) } + e^{ i (t S_N \tau + l S_N \theta )(g_{\mathbf {b}}(x))} h(g_{\mathbf {b}}(x))e^{S_N \varphi (g_{\mathbf {b}}(x) ) } , \end{aligned}$$

we see that a difference in argument might give us some cancellations. The effect of h in the difference of argument can be carefully controlled by the \(C^1\) norm of h. The interesting part comes from the complex exponential. The difference of arguments of this part is

$$\begin{aligned} t (S_N \tau \circ g_{\mathbf {a}} - S_N \tau \circ g_{\mathbf {b}}) + l (S_N \theta \circ g_{{\mathbf {a}}} - S_N \theta \circ g_{{\mathbf {b}}}) , \end{aligned}$$

which might be rewriten in the form

$$\begin{aligned} \langle (t,l) , ({\tilde{\tau }},{\tilde{\theta }}) \rangle . \end{aligned}$$

Then we proceed as follows. Choose a large number of points \((x_k)\) in \(U_0\). If, for a given \(x_k\), the difference of argument \(\langle (t,l),({\tilde{\tau }},{\tilde{\theta }}) \rangle (x_k)\) is not large enough, we might use the NCP to construct another point \(y_k\) next to \(x_k\) such that \( \langle (t,l),({\tilde{\tau }},{\tilde{\theta }}) \rangle (y_k) \) become larger. The construction goes as follows: the NLI ensures that \(\nabla \langle (t,l) , ({\tilde{\tau }},{\tilde{\theta }}) \rangle (x_k) =: w_k \ne 0 \). Hence, the direction \({\widehat{w}}_k := \frac{w_k}{|w_k|}\) is well defined. The NCP then ensures us the existence of some \(y_k \in J\) which are very close to \(x_k\) and such that \(x_k - y_k\) is a vector pointing in a direction comparable to \({\widehat{w}}_k\). As we are following the gradient of \(\langle (t,l) , ({\tilde{\tau }},{\tilde{\theta }}) \rangle \), we are sure that \(\langle (t,l) , ({\tilde{\tau }},{\tilde{\theta }}) \rangle (y_k)\) will be larger than before.

We then let S be the set containing the points where the difference in argument is large enough, so it contains some \(x_k\) and some \(y_k\). This large enough difference in argument that is true in S is also true in a small open neighborhood \({\widehat{S}}\) of S.

We can then write, for \(x \in {\widehat{S}}\), an inequality of the form:

$$\begin{aligned}&\left| e^{ i (t S_N \tau + l S_N \theta )(g_{\mathbf {a}}(x))} h(g_{\mathbf {a}}(x))e^{S_N \varphi (g_{\mathbf {a}}(x) ) } + e^{ i (t S_N \tau + l S_N \theta )(g_{\mathbf {b}}(x))} h(g_{\mathbf {b}}(x))e^{S_N \varphi (g_{\mathbf {b}}(x) ) } \right| \\&\quad \le (1-\eta ) |h(g_{\mathbf {a}}(x))| e^{S_N \varphi (g_{\mathbf {a}}(x))} + |h(g_{\mathbf {b}}(x))| e^{S_N \varphi (g_{\mathbf {b}}(x))} , \end{aligned}$$

where the \((1-\eta )\) comes in front of the part with the smaller modulus. This is, in spirit, lemma 5.2 of [OW17]. We can then summarize the information in the form of a function \(\beta \) that is 1 most of the time, but that is less than \((1-\eta )^{1/2}\) on \({\widehat{S}}\). This allows us to write the following bound:

$$\begin{aligned} {\mathcal {L}}_{\varphi -i(t \tau + l \theta )}^N h \le {\mathcal {L}}_{\varphi }^N \left( |h| \beta \right) . \end{aligned}$$

One of the main difficulty of this part is to make sure that \({\widehat{S}}\) is a set of large enough measure, while still managing not to make the \(C^1\)-norm of \(\beta \) explode. All the hidden technicalities in this part forces us to only get this bound for a well chosen N.

Step 3 These cancellations allow us to compare \({\mathcal {L}}\) to an operator that is contracting on a cone.

We define the following cone, on which the soon-to-be-defined Dolgopyat operator will be well behaved. Define

$$\begin{aligned} K_R({\mathfrak {U}}) := \{ H \in C^1_b({\mathfrak {U}}) \ | \ H \text { is positive, and} \ |\nabla H| \le R H \} , \end{aligned}$$

and then define the Dolgopyat operator by \({\mathcal {M}} H := {\mathcal {L}}_\varphi ^N (H \beta )\). We then show that, if \(H \in K_R({\mathfrak {U}})\) (for a well chosen R):

  1. 1.

    \({\mathcal {M}}(H) \in K_R({\mathfrak {U}}) \)

  2. 2.

    \( \Vert {\mathcal {M}}(H) \Vert _{L^2(\mu )}^2 \le (1-\varepsilon ) \Vert H \Vert _{L^2(\mu )}^2\).

The first point is done using the Lasota-Yorke inequalities, see lemma 5.1 in [OW17]. The second point goes, loosely, as follows.

We write, using Cauchy-Schwartz:

$$\begin{aligned} ({\mathcal {M}}H)^2 = {\mathcal {L}}_\varphi ^N(H \beta )^2 \le {\mathcal {L}}^N_\varphi (H^2){\mathcal {L}}^N_\varphi (\beta ^2) . \end{aligned}$$

On \({\widehat{S}}\), the cancellations represented in the function \(\beta \) spread, thanks to the fact that \(\varphi \) is normalized, as follows:

$$\begin{aligned} {\mathcal {L}}_\varphi ^N (\beta ^2)= & {} \sum _{{\mathbf {a}}} e^{ S_N \varphi \circ g_{{\mathbf {a}}} } \beta ^2 \circ g_{\mathbf {a}} \\= & {} \sum _{{\mathbf {a}} \text { where } \beta =1 } e^{S_N \varphi \circ g_{\mathbf {a}} } \beta ^2 \circ g_{\mathbf {a}} + \sum _{{\mathbf {a}} \text { where } \beta \text { is smaller} } e^{S_N \varphi \circ g_{\mathbf {a}} } \beta ^2 \circ g_{\mathbf {a}} \\\le & {} \sum _{{\mathbf {a}} \text { where } \beta =1 } e^{S_N \varphi \circ g_{\mathbf {a}} } + \sum _{{\mathbf {a}} \text { where } \beta \text { is smaller} } e^{S_N \varphi \circ g_{\mathbf {a}} } (1-\eta ) \\= & {} 1 - \eta e^{-N \Vert \varphi \Vert _\infty }. \end{aligned}$$

Then, we use the doubling property of \(\mu =\sum _a \mu _a\) and the control given by the fact that \(H \in K_R({\mathfrak {U}})\) to bound the integral on all J by the integral on \({\widehat{S}}\):

$$\begin{aligned} \int _J {\mathcal {L}}^N_\varphi (H^2) d\mu \le C_0 \int _{{\widehat{S}}} {\mathcal {L}}^N_\varphi (H^2) d\mu . \end{aligned}$$

Hence, we can write, using the fact that \({\mathcal {L}}_\varphi \) preserves \(\mu \) and the previously mentioned Cauchy-Schwartz inequality:

$$\begin{aligned} \Vert H\Vert _{L^2(\mu )}^2 - \Vert {\mathcal {M}}H\Vert _{L^2(\mu )}^2\ge & {} \int _J \left( {\mathcal {L}}_\varphi ^N(H^2) - {\mathcal {L}}_\varphi ^N(H^2) {\mathcal {L}}_\varphi ^N( \beta ^2) \right) d\mu \\\ge & {} \int _{{\widehat{S}}} \left( {\mathcal {L}}_\varphi ^N(H^2) - {\mathcal {L}}_\varphi ^N(H^2) {\mathcal {L}}_\varphi ^N( \beta ^2) \right) d\mu \\\ge & {} \eta e^{-N \Vert \varphi \Vert _\infty } \int _{{\widehat{S}}}{\mathcal {L}}_\varphi ^N(H^2) d\mu \\\ge & {} \eta C_0^{-1} e^{-N \Vert \varphi \Vert _\infty } \Vert H \Vert _{L^2(\mu )}^2 := \varepsilon \Vert H \Vert _{L^2(\mu )}^2 . \end{aligned}$$

Hence

$$\begin{aligned} \Vert {\mathcal {M}}H\Vert _{L^2(\mu )}^2 \le (1-\varepsilon ) \Vert H\Vert _{L^2(\mu )}^2 . \end{aligned}$$

Step 4 We conclude by an iterative argument.

To conclude, we need to see that we may bound h by some \(H \in K_R({\mathfrak {U}})\), and also that the contraction property is true for all n, not just N.

For any \(n=kN\), we can inductively prove our bound. If \(k=1\), we can choose \(H_0:= \Vert h\Vert _{|t|+|l|}\). Then, \(|h| \le H_0\) and so

$$\begin{aligned} \Vert {\mathcal {L}}_{\varphi - i(t \tau + l \theta ) }^N h \Vert _{L^2(\mu )} \le \Vert {\mathcal {M}} H_0 \Vert _{L^2(\mu )} \le (1-\varepsilon )^{1/2} \Vert h\Vert _{(|t|+|l|)} . \end{aligned}$$

Then, choosing \(H_{k+1} := {\mathcal {M}} H_k \in K_R({\mathfrak {U}})\), we can proceed to the next step of the induction and get

$$\begin{aligned} \Vert {\mathcal {L}}_{\varphi - i(t \tau + l \theta ) }^{kN} h \Vert _{L^2(\mu )} \le \Vert {\mathcal {M}} H_{k-1} \Vert _{L^2(\mu )} \le (1-\varepsilon )^{k/2} \Vert h\Vert _{(|t|+|l|)} . \end{aligned}$$

Finally, if \(n=kN+r\), with \(0 \le j \le N-1\), we write

$$\begin{aligned} \Vert {\mathcal {L}}_{\varphi - i(t \tau + l \theta ) }^{kN+r} h \Vert _{L^2(\mu )} \le (1-\varepsilon )^k \Vert {\mathcal {L}}_\varphi ^r h\Vert _{(|t|+|l|)} \lesssim (1-\varepsilon )^{n/(2N)} \Vert h\Vert _{(|t|+|l|)} , \end{aligned}$$

and the proof is done.

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Leclerc, G. Julia Sets of Hyperbolic Rational Maps have Positive Fourier Dimension. Commun. Math. Phys. 397, 503–546 (2023). https://doi.org/10.1007/s00220-022-04496-6

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