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Dimension estimates for $C^1$ iterated function systems and repellers. Part II

Published online by Cambridge University Press:  08 September 2021

DE-JUN FENG*
Affiliation:
Department of Mathematics, The Chinese University of Hong Kong, Sha Tin, Hong Kong
KÁROLY SIMON
Affiliation:
Department of Stochastics, Institute of Mathematics and MTA-BME Stochastics Research Group, Budapest University of Technology and Economics, 1521 Budapest, PO Box 91, Hungary (e-mail: simonk@math.bme.hu)
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Abstract

This is the second part of our study on the dimension theory of $C^1$ iterated function systems (IFSs) and repellers on $\mathbb {R}^d$ . In the first part [D.-J. Feng and K. Simon. Dimension estimates for $C^1$ iterated function systems and repellers. Part I. Preprint, 2020, arXiv:2007.15320], we proved that the upper box-counting dimension of the attractor of every $C^1$ IFS on ${\Bbb R}^d$ is bounded above by its singularity dimension, and the upper packing dimension of every ergodic invariant measure associated with this IFS is bounded above by its Lyapunov dimension. Here we introduce a generalized transversality condition (GTC) for parameterized families of $C^1$ IFSs, and show that if the GTC is satisfied, then the dimensions of the IFS attractor and of the ergodic invariant measures are given by these upper bounds for almost every (in an appropriate sense) parameter. Moreover, we verify the GTC for some parameterized families of $C^1$ IFSs on ${\Bbb R}^d$ .

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1 Introduction

The present paper is a continuation of our work in [Reference Feng and Simon24] for studying the dimension theory of $C^1$ iterated function systems (IFSs) and repellers.

One of the fundamental problems in fractal geometry and dynamical systems is to compute various fractal dimensions of attractors of IFSs and associated invariant measures. The corresponding problem has been well understood when the underlying IFSs consist of similitudes or conformal maps satisfying certain separation conditions (see e.g. [Reference Bowen7, Reference Gatzouras and Peres25, Reference Hochman26, Reference Hutchinson30, Reference Patzschke39, Reference Przytycki and Urbański41, Reference Ruelle44]). The problem becomes substantially more difficult when the underlying IFSs are non-conformal. In the last three decades, much significant progress has been achieved for affine IFSs, see e.g. [Reference Bárány, Hochman and Rapaport2, Reference Bedford5, Reference Das and Simmons11, Reference Falconer13, Reference Falconer and Kempton19, Reference Feng and Shmerkin23, Reference Hochman and Rapaport27, Reference Jordan, Pollicott and Simon32, Reference Käenmäki34, Reference McMullen37], the references in the survey papers [Reference Chen and Pesin10, Reference Falconer17] and an upcoming book [Reference Bárány, Simon and Solomyak3].

In contrast to the extensive studies on affine IFSs, there have been relatively few results on those IFSs which are neither conformal nor affine. In 1994, Falconer [Reference Falconer15] introduced a quantity (known as the singularity dimension) in terms of sub-additive topological pressure, and showed that it is an upper bound for the upper box-counting dimension of repellers of $C^2$ expanding maps satisfying a ‘bunching’ condition. Later, in 1997, Zhang [Reference Zhang50] proved that this upper bound holds for the Hausdorff dimension of repellers of arbitrary $C^1$ expanding maps. We remark that the results of Falconer and Zhang extend directly to the IFS setting. Recently, Cao, Pesin and Zhao [Reference Cao, Pesin and Zhao9] also gave an upper bound for the upper box-counting dimension of repellers of $C^{1+\alpha }$ expanding maps satisfying a certain dominated splitting property. However that upper bound depends on the splitting involved and is usually strictly larger than the singularity dimension. In [Reference Feng and Simon24], the authors proved that the singularity dimension is an upper bound of the upper box-counting dimension of the attractor of every $C^1$ IFS or the repeller of every $C^1$ expanding map, which improved the aforementioned results in [Reference Cao, Pesin and Zhao9, Reference Falconer15, Reference Zhang50]. The authors also established a measure analogue of this result, that is, the upper packing dimension of every ergodic invariant measure associated with a $C^1$ IFS or repeller is bounded above by its Lyapunov dimension, which improved an earlier result of Jordan and Pollicott [Reference Jordan and Pollicott31] for the upper Hausdorff dimension of measures. The reader is referred to §2.2 for the definitions of singularity dimension and Lyapunov dimension.

In [Reference Hu29], Hu computed the box-counting dimension of repellers of $C^2$ maps on ${\Bbb R}^2$ which have an invariant strong unstable foliation along which they expand more strongly than in the complementary directions. Very recently, Falconer, Fraser and Lee [Reference Falconer, Fraser and Lee18] computed the $L^q$ -spectra of Bernoulli measures associated with a class of planar IFSs consisting of $C^{1+\alpha }$ maps for which the Jacobian is a lower triangular matrix subject to a domination condition and satisfying the rectangular open set condition. As a corollary, they obtained a formula for the box-counting dimension of the attractors of such planar IFSs. In another recent paper [Reference Jurga and Lee33], Jurga and Lee proved that, under slightly stronger assumptions, these Bernoulli measures (and more generally, quasiBernoulli measures) on the attractors are exact dimensional with dimension given by a Ledrappier–Young-type formula. In earlier related works, Bedford and Urbański [Reference Bedford and Urbański6] calculated the box-counting and Hausdorff dimensions of the attractors of a very special class of planar nonlinear triangular $C^{1+\alpha }$ IFSs (of which the attractors are curves), Manning and Simon [Reference Manning and Simon36] and Bárány [Reference Bárány1] studied the sub-additive pressure associated with nonlinear $C^{1+\alpha }$ IFSs whose maps have triangular Jacobians.

In this paper, we introduce a generalized transversality condition (GTC) for parameterized families of $C^1$ IFSs on ${\Bbb R}^d$ , and show that if the GTC is satisfied, then for almost every (a.e.) (in an appropriate sense) parameter, the Hausdorff and box-counting dimensions of the IFS attractor are indeed given by the singularity dimension, and the dimension of ergodic invariant measures on the attractor is given by its Lyapunov dimension. Moreover, we will verify the GTC for several classes of translational families of $C^1$ IFSs.

Before formulating our results precisely, we first recall some basic notation and definitions. By a $C^1$ IFS on a compact set $Z\subset {\Bbb R}^d$ , we mean a finite collection $\mathcal F=\{f_i\}_{i=1}^{\ell }$ of self-maps on Z, such that there exists an open set $U\supset Z$ so that each $f_i$ extends to a $C^1$ -diffeomorphism $f_i: U\to f_i(U)\subset U$ with

$$ \begin{align*} \rho_i:=\sup_{x\in U}\|D_xf_i\|<1, \end{align*} $$

where $D_xf$ stands for the differential of f at x and $\|\cdot \|$ is the standard matrix norm (that is, $\|A\|$ is the largest singular value of A).

Let K be the attractor of the IFS $\mathcal F$ , that is, K is the unique non-empty compact subset of Z such that

(1.1) $$ \begin{align} K=\bigcup_{i=1}^{\ell} f_i(K) \end{align} $$

(cf. [Reference Hutchinson30]).

Let $(\Sigma ,\sigma )$ be the one-sided full shift over the alphabet $\{1,\ldots , \ell \}$ . Let $\Pi : \Sigma \to K$ denote the corresponding coding map associated with the IFS $\mathcal F$ , that is,

(1.2) $$ \begin{align} \Pi(\mathbf{i})=\lim_{n\to \infty}f_{i_1}\circ \cdots\circ f_{i_n}(0), \quad \mathbf{i}=(i_n)_{n=1}^{\infty}. \end{align} $$

It is well known that $\Pi $ is continuous and surjective [Reference Hutchinson30]. For a $\sigma $ -invariant Borel probability measure $\mu $ on $\Sigma $ , let $\Pi _*\mu $ denote the push-forward of $\mu $ by $\Pi $ , that is, $\Pi _*\mu (E)=\mu (\Pi ^{-1}(E))$ for each Borel subset E of ${\Bbb R}^d$ .

For a Borel probability measure $\xi $ on ${\Bbb R}^d$ , we call

$$ \begin{align*} \underline{d}_{\xi}(x)=\liminf_{r\to 0}\frac{\log \xi(B(x,r))}{\log r}\quad \text{and}\quad \overline{d}_{\xi}(x)=\limsup_{r\to 0}\frac{\log \xi(B(x,r))}{\log r} \end{align*} $$

the lower and upper local dimensions of $\xi $ at x, where $B(x,r)$ stands for the closed ball centered at x of radius r. Moreover, we call

$$ \begin{align*} \underline{\dim}_H\xi=\mathrm{ess}\!\! \inf_{x\in \mathrm{spt}(\xi)}\underline{d}_{\xi}(x) \quad \text{and}\quad \overline{\dim}_P\xi=\mathrm{ess}\!\! \sup\limits_{x\in \mathrm{spt}(\xi)}\overline{d}_{\xi}(x) \end{align*} $$

the lower Hausdorff dimension and upper packing dimension of $\xi $ , respectively. If $\underline {\dim }_H\xi =\overline {\dim }_P\xi $ , we say that $\xi $ is exact dimensional and write $\dim \xi $ or $\dim _H \xi $ for this common value.

To introduce the notion of GTC, let $\ell \geq 2$ and let ${\mathcal F}^t=\{f_1^t,\ldots , f_{\ell }^t\}$ , $t\in {\Omega }$ , be a parameterized family of $C^1$ IFSs defined on a common compact subset Z of ${\Bbb R}^d$ , where $({\Omega }, \rho )$ is a separable metric space, such that the following two conditions hold.

  • (C1) The maps $f_i^t$ have a common Lipschitz constant $\theta \in (0,1)$ , that is,

    (1.3) $$ \begin{align} |f^t_i(x)-f^t_i(y)| \leq \theta |x-y| \end{align} $$
    for all $1\leq i\leq \ell $ , $t\in {\Omega }$ and $x,y\in Z$ .
  • (C2) The mapping $t\mapsto f^t_i(x)$ is continuous over ${\Omega }$ for every given $x\in Z$ and $1\leq i\leq \ell $ .

For each $t\in {\Omega }$ , let $K^t$ denote the attractor of $\mathcal F^t$ , and let $\Pi ^t:\; \Sigma \to {\Bbb R}^d$ denote the coding map associated with the IFS ${\mathcal F}^t$ . Due to the conditions (C1) and (C2), the mapping $(t,\mathbf {i})\mapsto \Pi ^t(\mathbf {i})$ is continuous over the product space ${\Omega }\times \Sigma $ .

For $t\in {\Omega }$ , $r>0$ and ${\textbf {i}}\in \Sigma _*:=\bigcup _{n=0}^{\infty } \{1,\ldots , \ell \}^n$ , set

(1.4) $$ \begin{align} Z_{\textbf{i}}^t(r)= \inf_{x\in \Sigma} \min\bigg \{ \frac{r^k}{ \phi^k (D_{\Pi^t x}f^t_{{\textbf{i}}} ) }:\; k=0, 1,\ldots, d\bigg\} , \end{align} $$

where $f^t_{{\textbf {i}}}:=f^t_{i_1}\circ \cdots \circ f^t_{i_n}$ for ${\textbf { i}}=i_1\ldots i_n$ , $f^t_{\varepsilon }$ denotes the identity map on ${\Bbb R}^d$ and $\phi ^s(\cdot )$ stands for the singular value function (see (2.5) for the definition).

Definition 1.1. Let $\eta $ be a locally finite Borel measure on ${\Omega }$ . We say that the family ${\mathcal F}^t$ , $t\in {\Omega }$ , satisfies a GTC with respect to $\eta $ if there exist $\delta _0>0$ and a function $\psi : (0,\delta _0)\to [0,\infty )$ with $\lim _{\delta \to 0}\psi (\delta )=0$ such that the following statement holds: for every $t_0\in {\Omega }$ and every $0<\delta <\delta _0$ , there exists a constant $C=C(t_0, \delta )>0$ such that for all distinct ${\textbf {i}}, {\textbf {j}}\in \Sigma $ and $r>0$ ,

(1.5) $$ \begin{align} \eta\{t\in B(t_0, \delta): \; |\Pi^t({\textbf{i}})-\Pi^t({\textbf{j}}) |< r\}\leq C e^{|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)} Z^{t_0}_{{\textbf{i}}\wedge {\textbf{ j}}}(r) , \end{align} $$

where $B(t_0,\delta )$ denotes the closed ball in ${\Omega }$ of radius $\delta $ centered at t, $\mathbf {i}\wedge \mathbf {j}$ denotes the common initial segment of $\mathbf {i}$ and $\mathbf {j}$ , and $|\mathbf {i}\wedge \mathbf {j}|$ is the length of the word $\mathbf {i}\wedge \mathbf {j}$ .

The introduction of the GTC is inspired by the work of Jordan, Pollicott and Simon [Reference Jordan, Pollicott and Simon32], who defined the self-affine transversality condition for certain translational families of affine IFSs. The new feature here is that the upper bound term on the right-hand side of (1.5) depends upon $t_0$ , $\delta $ and $|{\textbf {i}}\wedge {\textbf {j}}|$ , while in the setting of [Reference Jordan, Pollicott and Simon32], the corresponding upper bound term is independent of these parameters and is determined by the linear parts of one pre-given affine IFS.

For $t\in {\Omega }$ and a $\sigma $ -invariant measure $\mu $ on $\Sigma $ , we write

(1.6) $$ \begin{align} d(t):=\dim_S(\mathcal F^t),\quad d_{\mu}(t):=\dim_{L,\mathcal F^t}\mu \end{align} $$

for the singularity dimension of $\mathcal F^t$ and the Lyapunov dimension of $\mu $ with respect to $\mathcal F^t$ , respectively; see Definitions 2.32.4. For $E\subset {\Bbb R}^d$ , let $\dim _HE$ denote the Hausdorff dimension of E, and let $\overline {\dim }_BE, \;\underline {\dim }_BE$ denote the upper and lower box-counting dimensions of E, respectively (cf. [Reference Falconer16]). When $\overline {\dim }_BE=\underline {\dim }_BE$ , the common value is said to be the box-counting dimension of E and is denoted by $\dim _BE$ .

The first result of the present paper is the following.

Theorem 1.2. Let ${\mathcal F}^t=\{f_1^t,\ldots , f_{\ell }^t\}$ , $t\in {\Omega }$ , be a parameterized family of $C^1$ IFSs defined on a common compact subset Z of ${\Bbb R}^d$ , such that the conditions (C1)–(C2) hold. Let $\eta $ be a locally finite Borel measure on ${\Omega }$ . Assume that $({\mathcal F}^t)_{t\in {\Omega }}$ satisfies the GTC with respect to $\eta $ . Then the following properties hold.

  1. (i) Let $\mu $ be a $\sigma $ -invariant ergodic measure on $\Sigma $ . For $\eta $ -a.e. $t\in {\Omega }$ , $\Pi ^t_*\mu $ is exact dimensional and

    $$ \begin{align*}\dim_H \Pi^t_*\mu=\min\{d, d_{\mu}(t)\}. \end{align*} $$
    Moreover, $\Pi ^t_*\mu \ll {\mathcal L}_d$ for $\eta $ -a.e. $t\in \{t'\in {\Omega }: d_{\mu }(t')>d\}$ , where ${\mathcal L}_d$ denotes the Lebesgue measure on ${\Bbb R}^d$ .
  2. (ii) For $\eta $ -a.e. $t\in {\Omega }$ ,

    $$ \begin{align*}\dim_H K^t=\dim_BK^t=\min\{d, d(t)\}. \end{align*} $$
    Moreover, ${\mathcal L}_d(K^t)>0$ for $\eta $ -a.e. $t\in \{t'\in {\Omega }: \; d(t')>d\}$ .

The above theorem is a nonlinear analogue of the results of Jordan, Pollicott and Simon [Reference Jordan, Pollicott and Simon32, Theorems 4.2 and 4.3] for affine IFSs. We emphasize that in the nonlinear case, the singularity and Lyapunov dimensions depend on the parameter t, while in the affine case, the corresponding quantities are constant. This is a key difference between the affine case and the nonlinear case. We remark that Theorem 1.2 also extends and generalizes the corresponding results of Simon, Solomyak and Urbański ([Reference Simon, Solomyak and Urbański45, Theorem 3.1], [Reference Simon, Solomyak and Urbański46, Theorem 2.3]) for $C^{1+\alpha }$ conformal IFSs on ${\Bbb R}$ .

Now a natural question arises of how to verify the GTC for a parameterized family of $C^1$ IFSs. In what follows, we investigate this question for certain translational families of $C^1$ IFSs.

First we introduce some definitions.

Definition 1.3. Let $\mathcal F=\{f_i\}_{i=1}^{\ell }$ be a $C^1$ IFS on a compact set $Z\subset {\Bbb R}^d$ such that $f_i(Z)\subset \mathrm {int}(Z)$ for each i. Set

(1.7) $$ \begin{align} f_i^{\boldsymbol{\mathfrak{t}}}:=f_i+\mathbf{t}_i, \quad i=1,\ldots, \ell, \end{align} $$

where $\boldsymbol {\mathfrak {t}}=(\mathbf {t}_1,\ldots , \mathbf {t}_{\ell })\in {\Bbb R}^{\ell d}$ with ${\textbf {t}}_i\in {\Bbb R}^d$ . By continuity, there is a small $r_0>0$ such that $f_i^{\boldsymbol {\mathfrak {t}}}(Z)\subset \mathrm {int}(Z)$ for every $\boldsymbol {\mathfrak {t}}$ with $|\boldsymbol {\mathfrak {t}}|<r_0$ and every i, where $|\cdot |$ is the Euclidean norm. Set $\mathcal F^{\boldsymbol {\mathfrak {t}}}=\{f_i^{\boldsymbol {\mathfrak {t}}}\}_{i=1}^{\ell }$ for each $\boldsymbol {\mathfrak {t}}$ with $|\boldsymbol {\mathfrak {t}}|<r_0$ . We call $(\mathcal F^{\boldsymbol {\mathfrak {t}}})_{\boldsymbol {\mathfrak {t}}\in \Delta }$ , where $\Delta :=\{\boldsymbol {\mathfrak {s}}\in {\Bbb R}^{\ell d}:\; |\boldsymbol {\mathfrak {s}}|<r_0\}$ , a translational family of IFSs generated by $\mathcal F$ .

Definition 1.4. Let $\mathcal F=\{f_i\}_{i=1}^{\ell }$ be a $C^1$ IFS on a compact set $Z\subset {\Bbb R}^d$ . We say that $\mathcal F$ is dominated lower triangular, if for each $z\in Z$ and $i\in \{1,\ldots , \ell \}$ , the Jacobian $D_zf_i$ of $f_i$ at z is a lower triangular matrix such that

$$ \begin{align*}|(D_zf_i)_{11}|\geq |(D_zf_i)_{22}|\geq \cdots\geq |(D_zf_i)_{dd}|. \end{align*} $$

We remark that in the above definition, the condition for an IFS to be dominated lower triangular is slightly weaker than that required in [Reference Falconer, Fraser and Lee18, Reference Jurga and Lee33].

Definition 1.5. Let $\ell \in {\Bbb N}$ with $\ell \geq 2$ . Assume for $j=1,\ldots , n$ , $\mathcal F_j=\{f_{i,j}\}_{i=1}^{\ell }$ is an IFS on $Z_j\subset {\Bbb R}^{q_j}$ . Let $\mathcal F=\{f_i\}_{i=1}^{\ell }$ be an IFS on $Z_1\times \cdots \times Z_n\subset {\Bbb R}^{q_1}\times \cdots \times {\Bbb R}^{q_n}$ given by

$$ \begin{align*}f_i(x_1,\ldots, x_n)=(f_{i,1}(x_1),\ldots, f_{i,n}(x_n)), \quad i=1,\ldots, \ell, \; x_k\in Z_k \text{ for } 1\leq k\leq n. \end{align*} $$

We say that $\mathcal F$ is the direct product of $\mathcal F_1,\ldots , \mathcal F_n$ , and write $\mathcal F=\mathcal F_1\times \cdots \times \mathcal F_n$ .

Now we are ready to state the second main result of the paper.

Theorem 1.6. Let $\mathcal F=\{f_i\}_{i=1}^{\ell }$ be a $C^1$ IFS on a compact set $Z\subset {\Bbb R}^d$ such that $f_i(Z)\subset \mathrm {int} (Z)$ for each i. Suppose either one of the following three conditions holds.

  1. (i) $\mathcal F$ is dominated lower triangular on Z satisfying

    (1.8) $$ \begin{align} \max_{i\neq j}\Big(\sup_{y,z\in Z} \|D_yf_i\|+\|D_zf_j\|\Big)<1, \end{align} $$
    and Z is convex.
  2. (ii) $\mathcal F$ is a $C^1$ conformal IFS on Z satisfying (1.8), and Z is connected.

  3. (iii) $\mathcal F=\mathcal F_1\times \cdots \times \mathcal F_n$ , where for each $k\in \{1,\ldots , n\}$ , $\mathcal F_k$ is a $C^1$ IFS on a compact $Z_k\subset {\Bbb R}^{d_k}$ satisfying either (i) or (ii), in which $\mathcal F$ and Z are replaced by $\mathcal F_k$ and $Z_k$ , respectively.

Then there is a small $r_0>0$ such that the translational family

$$ \begin{align*}\mathcal F^{\boldsymbol{\mathfrak{t}}}=\{f_i+\mathbf{t}_i\}_{i=1}^{\ell},\quad \boldsymbol{\mathfrak{t}}=(\mathbf{t}_1,\ldots, \mathbf{t}_{\ell})\in \Delta:=\{\boldsymbol{\mathfrak{s}}\in {\Bbb R}^{\ell d}:\; |\boldsymbol{\mathfrak{s}}|<r_0\},\end{align*} $$

satisfies the GTC with respect to the Lebesgue measure $\mathcal L_{\ell d}$ on $\Delta $ . As a consequence, the conclusions of Theorem 1.2 hold for the family $(\mathcal F^{\boldsymbol {\mathfrak {t}}})_{\boldsymbol {\mathfrak {t}}\in \Delta }$ .

The above theorem is a (partial) nonlinear extension of the corresponding results in [Reference Falconer13, Reference Jordan, Pollicott and Simon32, Reference Solomyak47] for affine IFSs. Recall that in the case when $\mathcal F=\{f_i(x)=A_ix+a_i\}_{i=1}^{\ell }$ is an affine IFS on ${\Bbb R}^d$ , under the assumption that

(1.9) $$ \begin{align} \max_{1\leq i\leq \ell}\|A_i\|<1/3, \end{align} $$

Falconer [Reference Falconer13] proved that the dimension of the attractor of $\mathcal F^{\boldsymbol {\mathfrak {t}}}=\{f_i+{\textbf {t}}_i\}_{i=1}^{\ell }$ is equal to its affinity dimension for ${\mathcal L}_{\ell d}$ -a.e. $\boldsymbol {\mathfrak {t}}=({\textbf {t}}_1,\ldots , {\textbf {t}}_{\ell })\in {\Bbb R}^{\ell d}$ . Later, Solomyak [Reference Solomyak47] pointed out that the bound $1/3$ in (1.9) can be replaced by $1/2$ . By an observation of Edgar [Reference Edgar12], $1/2$ is optimal. Under the same assumption that

(1.10) $$ \begin{align} \max_{1\leq i\leq \ell}\|A_i\|<1/2, \end{align} $$

Jordan, Pollicott and Simon [Reference Jordan, Pollicott and Simon32] showed that the translational family $(\mathcal F^{\boldsymbol {\mathfrak {t}}})_{\boldsymbol {\mathfrak {t}}\in {\Bbb R}^{\ell d}}$ satisfies the self-affine transversality condition. It was pointed out in [Reference Bárány, Simon and Solomyak3, Theorem 9.1.2] that the assumption (1.10) can by further replaced by a slightly more general condition $\max _{i\neq j}(\|A_i\|+\|A_j\|)<1$ .

We remark that Theorem 1.6 also extends the results of Simon, Solomyak and Urbański ([Reference Simon, Solomyak and Urbański45, Proposition 7.1], [Reference Simon, Solomyak and Urbański46, Corollary 7.3]) for translational families of $C^{1+\alpha }$ conformal IFSs on ${\Bbb R}$ . It is worth pointing out that for every $C^1$ conformal IFS satisfying the open set condition (or $C^1$ conformal expanding map), the dimension of its attractor (or repeller) satisfies the Bowen–Ruelle formula, and is equal to the singularity dimension; meanwhile, the dimension of ergodic invariant measures on the attractor (repeller) is given by the Lyapunov dimension (see [Reference Bowen7, Reference Gatzouras and Peres25, Reference Patzschke39, Reference Ruelle44]).

The paper is organized as follows. In §2, we give some preliminaries, including the variational principle for sub-additive topological pressure, and the definitions and properties of singularity dimension and Lyapunov dimension. In §3, we prove Theorem 1.2. The proof of Theorem 1.6 is rather long and will be given in §§47, where we divide the whole proof into three different parts, by considering the conditions (i)–(iii) in Theorem 1.6 separately.

2 Preliminaries

2.1 Variational principle for sub-additive pressure

In order to define the singularity and Lyapunov dimensions, we require some elements from the sub-additive thermodynamic formalism.

Let $(\Sigma ,\sigma )$ be the one-sided full shift over the alphabet $\{1,\ldots , \ell \}$ . That is, $\Sigma =\{1,\ldots , \ell \}^{\Bbb N}$ , which is endowed with the product topology, and $\sigma :\Sigma \to \Sigma $ is the left shift defined by $(x_i)_{i=1}^{\infty }\mapsto (x_{i+1})_{i=1}^{\infty }$ . Write $\Sigma _n=\{1,\ldots , \ell \}^n$ for $n\geq 0$ , with the convention $\Sigma _0=\{\varepsilon \}$ , where $\varepsilon $ stands for the empty word. Set $\Sigma _*=\bigcup _{n=0}^{\infty } \Sigma _n$ . For $x=(x_i)_{i=1}^{\infty }\in \Sigma $ and $n\in {\Bbb N}$ , write $x|n=x_1\ldots x_n$ .

Let $C(\Sigma )$ denote the set of real-valued continuous functions on $\Sigma $ . Let $\mathcal {G}=\{g_n\}_{n=1}^{\infty }$ be a sub-additive potential on $\Sigma $ , that is, $g_n\in C(\Sigma )$ for all $n\geq 1$ such that

(2.1) $$ \begin{align} g_{m+n}(x) \leq g_{n}(x)+g_{m}(\sigma^nx) \quad\text{for all } x\in \Sigma \text{ and }n,m\in {\Bbb N}. \end{align} $$

The topological pressure of $\mathcal G$ is defined by

(2.2) $$ \begin{align} P(\Sigma,\sigma, \mathcal G)= \lim_{n\to\infty} \frac{1}{n}\log\bigg( \sum_{I\in\, \Sigma_n} \sup_{x\in [I]} \exp(g_n(x)) \bigg), \end{align} $$

where $[I]:=\{x\in \Sigma :\; x|n=I\}$ for $I\in \Sigma _n$ . The limit can be seen to exist by using a standard sub-additivity argument.

If the potential $\mathcal G$ is additive, that is, $g_n=\sum _{k=0}^{n-1}g\circ \sigma ^k$ for some $g\in C(\Sigma )$ , then $P(\Sigma , \sigma , \mathcal G)$ recovers the classical topological pressure $P(\Sigma , \sigma , g)$ of g (see e.g. [Reference Walters49]).

Let $\mathcal {M}(\Sigma ,\sigma )$ denote the set of $\sigma $ -invariant Borel probability measures on $\Sigma $ . For $\mu \in \mathcal {M}(\Sigma ,\sigma )$ , let $h_{\mu }(\sigma )$ denote the measure-theoretic entropy of $\mu $ (cf. [Reference Walters49]). Moreover, for $\mu \in \mathcal M(\Sigma , \sigma )$ , by sub-additivity,

(2.3) $$ \begin{align} \mathcal{G}_*(\mu):=\lim_{n\to\infty} \frac{1}{n} \int\!\! g_n\, d\mu=\inf_n \frac{1}{n} \int\!\! g_n\, d\mu\in [-\infty,\infty). \end{align} $$

See e.g. [Reference Walters49, Theorem 10.1]. We call $\mathcal {G}_*(\mu )$ the Lyapunov exponent of $\mathcal {G}$ with respect to $\mu $ .

The following variational principle for the topological pressure of sub-additive potentials generalizes the classical variational principle for additive potentials [Reference Ruelle43, Reference Walters48].

Theorem 2.1. [Reference Cao, Feng and Huang8]

Let $\mathcal {G}=\{g_n\}_{n=1}^{\infty }$ be a sub-additive potential on $(\Sigma ,\sigma )$ . Then

(2.4) $$ \begin{align} P(\Sigma, \sigma,\mathcal{G})= \sup\{h_{\mu}(\sigma)+\mathcal{G}_*(\mu):\; \mu\in\mathcal{M}(\Sigma,\sigma) \}. \end{align} $$

Although in [Reference Cao, Feng and Huang8] this is proved for sub-additive potentials on an arbitrary continuous dynamical system on a compact space, we state it only for shift spaces. Particular cases of the above result, under stronger assumptions on the potentials, were previously obtained by many authors, see for example [Reference Barreira4, Reference Falconer14, Reference Feng20, Reference Feng and Lau22, Reference Käenmäki34, Reference Mummert38] and references therein.

Measures that achieve the supremum in (2.4) are called equilibrium measures for the potential ${\mathcal G}$ . There exists at least one ergodic equilibrium measure; see e.g. [Reference Feng21, Proposition 3.5] and the remark there.

2.2 Singularity dimension and Lyapunov dimension with respect to $C^1$ IFSs

In this subsection, we define the singularity and Lyapunov dimensions with respect to $C^1$ IFSs.

Let $\mathcal F=\{f_i\}_{i=1}^{\ell }$ be a $C^1$ IFS on a compact set $Z\subset {\Bbb R}^d$ and let K denote the attractor of $\mathcal F$ (cf. §1). Let $(\Sigma ,\sigma )$ be the one-sided full shift over the alphabet $\{1,\ldots , \ell \}$ and let $\Pi : \Sigma \to K$ be the coding map defined as in (1.2).

Let ${\Bbb R}^{d\times d}$ denote the collection of $d\times d$ real matrices. For $T\in {\Bbb R}^{d\times d}$ , let

$$ \begin{align*}\alpha_1(T)\geq\cdots\geq \alpha_d(T)\end{align*} $$

denote the singular values of T. Following [Reference Falconer13], for $s\geq 0$ , we define the singular value function $\phi ^s:\; {\Bbb R}^{d \times d}\to [0,\infty )$ as

(2.5) $$ \begin{align} \phi^s(T)=\left\{ \begin{array}{@{}ll} \alpha_1(T)\cdots \alpha_k(T) \alpha_{k+1}^{s-k}(T) & \text{if }0\leq s< d,\\ \det(T)^{s/d} & \text{if } s\geq d, \end{array} \right. \end{align} $$

where $k=[s]$ is the integral part of s. Here we make the convention that $0^0=1$ . The following result on $\phi ^s$ is well known; see e.g. [Reference Falconer13].

Lemma 2.2.

  1. (i) $\phi ^s(ST)\leq \phi ^s(S)\phi ^s(T)$ for all $S, T\in {\Bbb R}^{d\times d}$ and $s\geq 0$ .

  2. (ii) $\phi ^{s+t}(T)\leq \phi ^s(T)\|T\|^t$ for all $T\in {\Bbb R}^{d\times d}$ , $s,t\geq 0$ .

For a differentiable mapping $f:\; U\subset {\Bbb R}^d\to {\Bbb R}^d$ , let $D_zf$ denote the differential of f at $z\in U$ . Sometimes we also write $f'(z)$ for $D_zf$ , and also call $D_zf$ the Jacobian matrix of f at z. Below we introduce the concepts of singularity and Lyapunov dimensions.

Definition 2.3. The singularity dimension of $\mathcal F=\{f_i\}_{i=1}^{\ell }$ , written as $\dim _S\mathcal F$ , is the unique non-negative value s for which

$$ \begin{align*}P(\Sigma,\sigma, \mathcal G^s)=0, \end{align*} $$

where $\mathcal G^s=\{g_n^s\}_{n=1}^{\infty }$ is the sub-additive potential on $\Sigma $ defined by

(2.6) $$ \begin{align} g_n^s(x)=\log \phi^s(D_{\Pi\sigma^n x}f_{x|n}), \quad x\in \Sigma, \end{align} $$

with $f_{x|n}:=f_{x_1}\circ \cdots \circ f_{x_n}$ for $x=(x_n)_{n=1}^{\infty }$ .

Definition 2.4. Let $\mu $ be a $\sigma $ -invariant Borel probability measure on $\Sigma $ . The Lyapunov dimension of $\mu $ with respect to $\mathcal F=\{f_i\}_{i=1}^{\ell }$ , written as $\dim _{\mathrm {L}, {\mathcal F}} \mu $ , is the unique non-negative value s for which

$$ \begin{align*}h_{\mu}(\sigma)+ \mathcal G^s_*(\mu)=0, \end{align*} $$

where $\mathcal G^s=\{g^s_n\}_{n=1}^{\infty }$ is defined as in (2.6) and $\mathcal G^s_*(\mu ):=\lim _{n\to \infty } ({1}/{n})\int g^s_n\; d\mu $ .

Remark 2.5.

  1. (i) It is not hard to show that there exist $a<b<0$ such that

    $$ \begin{align*}nsa\leq g_n^s(x)\leq ns b,\quad g_n^{s+t}(x)\leq g_n^s(x)+ntb \end{align*} $$
    for all $x\in \Sigma $ , $n\in {\Bbb N}$ and $s,t\geq 0$ , where $g_n^s(x)$ is defined as in (2.6). The existence and uniqueness of s in Definitions 2.32.4 just follow from this fact.
  2. (ii) The concept of singularity dimension was first introduced by Falconer [Reference Falconer13, Reference Falconer15]; see also [Reference Käenmäki and Vilppolainen35]. It is also called affinity dimension in the case when the IFS $\{f_i\}_{i=1}^{\ell }$ is affine, that is, each map $f_i$ is affine.

  3. (iii) The definition of Lyapunov dimension of invariant measures with respect to an IFS presented above was adopted from [Reference Jordan and Pollicott31]. It is a generalization of that given in [Reference Jordan, Pollicott and Simon32] for affine IFSs.

The following result describes the relation between the singularity dimension and the Lyapunov dimension.

Lemma 2.6. Let $\mathcal F=\{f_i\}_{i=1}^{\ell }$ be a $C^1$ IFS on a compact subset Z of ${\Bbb R}^d$ . Suppose $\theta \in (0,1)$ is a common Lipschitz constant for $f_1,\ldots , f_{\ell }$ . That is,

$$ \begin{align*}|f_i(x)-f_i(y)|\leq \theta|x-y| \quad \text{for all }1\leq i\leq \ell,\; x,y\in Z. \end{align*} $$

Then the following properties hold.

  1. (i) $\dim _S\mathcal F=\sup \{\dim _{L,\mathcal F}\mu :\; \mu \in \mathcal M(\Sigma ,\sigma )\}$ . The supremum is attained by at least one ergodic measure.

  2. (ii) $\dim _S\mathcal F\leq ({\log \ell }/{\log (1/\theta )})$ .

Proof Since $\theta $ is a common Lipschitz constant for $f_1,\ldots , f_{\ell }$ , $\|D_zf_i\|\leq \theta $ for each $1\leq i\leq \ell $ and $z\in Z$ . It follows from Lemma 2.2(ii) that for $s_2>s_1\geq 0$ ,

$$ \begin{align*}\phi^{s_2}(D_{\Pi\sigma^n x} f_{x|n})\leq \phi^{s_1}(D_{\Pi\sigma^n x} f_{x|n}) \theta^{n(s_2-s_1)} \quad\text{for all }x\in \Sigma,\; n\in {\Bbb N}, \end{align*} $$

from which we see that

$$ \begin{align*}P(\Sigma,\sigma,\mathcal G^{s_2})\leq P(\Sigma,\sigma,\mathcal G^{s_1})-(s_2-s_1)\log (1/\theta). \end{align*} $$

Hence $P(\Sigma , \sigma , \mathcal G^s)$ is strictly decreasing in s.

Now let $\mu \in \mathcal M(\Sigma ,\sigma )$ . Write $s=\dim _{L,\mathcal F}\mu $ . Then $h_{\mu }(\sigma )+\mathcal G^s_*(\mu )=0$ . Applying Theorem 2.1 to the sub-additive potential $\mathcal G^s$ yields that $P(\Sigma , \sigma , \mathcal G^s)\geq 0$ . Hence $\dim _S\mathcal F\geq s=\dim _{L,\mathcal F}\mu $ . It follows that

$$ \begin{align*}\dim_S\mathcal F\geq \sup\{\dim_{L,\mathcal F}\mu:\; \mu\in \mathcal M(\Sigma,\sigma)\}.\end{align*} $$

To show that equality holds, write $s'=\dim _S\mathcal F$ . Let $\nu $ be an ergodic equilibrium measure for the potential $\mathcal G^{s'}$ . Then

$$ \begin{align*}0=P(\Sigma, \sigma, \mathcal G^{s'}\!)=h_{\nu}(\sigma)+\mathcal G^{s'}_*(\nu),\end{align*} $$

which implies that $\dim _{L, \mathcal F}\nu =s'$ . That is, $\dim _{L, \mathcal F}\nu =\dim _S\mathcal F$ . This completes the proof of (i).

To see (ii), notice that $\phi ^{s'}(D_{\Pi \sigma ^n x} f_{x|n})\leq \theta ^{ns'}$ for all $x\in \Sigma $ and $n\in {\Bbb N}$ . It follows from the definition of $P(\Sigma , \sigma , \mathcal G^{s'})$ that

$$ \begin{align*}0=P(\Sigma, \sigma, \mathcal G^{s'})\leq \lim_{n\to \infty} \frac{1}{n} \log (\ell^n \theta^{ns'})=\log \ell +s'\log \theta, \end{align*} $$

from which we obtain $s'\leq ({\log \ell }/{\log (1/\theta )})$ . This completes the proof of (ii).

For a $\sigma $ -invariant ergodic measure $\mu $ on $\Sigma $ , let $\Pi _*\mu $ denote the push-forward of $\mu $ by $\Pi $ . In the following, we present the main result obtained in the first part [Reference Feng and Simon24] of our study on the dimension of $C^1$ IFSs: the upper box-counting dimension of the attractor of $\mathcal F$ is bounded above by the singularity dimension of $\mathcal F$ , whilst the upper packing dimension of $\Pi _*\mu $ is bounded above by the Lyapunov dimension of $\mu $ .

Theorem 2.7. [Reference Feng and Simon24]

Let $\mathcal F=\{f_i\}_{i=1}^{\ell }$ be a $C^1$ IFS with attractor K, and let $\mu $ be a $\sigma $ -invariant ergodic measure on $\Sigma $ . Then the following properties hold.

  1. (i) $\overline {\dim }_B K\leq \dim _S \mathcal F$ .

  2. (ii) $\overline {\dim }_P \Pi _*\mu \leq \dim _{L,\mathcal F}(\mu )$ .

3 The proof of Theorem 1.2

In this section, we prove Theorem 1.2. A key part of the proof is the following proposition.

Proposition 3.1. Assume that $\mathcal F^t$ , $t\in {\Omega }$ , satisfies the GTC with respect to a locally finite Borel measure $\eta $ on ${\Omega }$ . Let $\mu $ be a $\sigma $ -invariant ergodic measure on $\Sigma $ . Let $t_0\in {\Omega }$ and $0<\delta <\delta _0$ , where $\delta _0$ is given as in Definition 1.1, Then the following properties hold.

  1. (i) For $\eta $ -a.e. $t\in B(t_0,\delta )$ ,

    (3.1) $$ \begin{align} \underline{\dim}_H\Pi^t_*\mu\geq \min\{d, d_{\mu}(t_0)\}-\frac{\psi(\delta)}{\log (1/\theta)}, \end{align} $$
    where $\psi (\cdot )$ is given as in Definition 1.1, and $\theta $ is given as in (1.3).
  2. (ii) If $d_{\mu }(t_0)>d+({\psi (\delta )}/{\log (1/\theta )})$ , then $\Pi ^t_*\mu \ll \mathcal L_d$ for $\eta $ -a.e. $t\in B(t_0,\delta )$ .

The proof of the above proposition is adapted from an argument used in [Reference Jordan, Pollicott and Simon32, Propositions 4.3 and 4.4]. For the reader’s convenience, we include a full proof. We begin with the following.

Lemma 3.2. Assume that $(\mathcal F^t)_{t\in {\Omega }}$ satisfies the GTC with respect to a locally finite Borel measure $\eta $ on ${\Omega }$ . Let s be non-integral with $0<s<d$ . Let $t_0\in {\Omega }$ and $0<\delta <\delta _0$ , where $\delta _0$ is given as in Definition 1.1. Then there exists a number $c>0$ , dependent on s and $\delta $ , such that for all distinct $\mathbf {i},\mathbf {j}\in \Sigma $ ,

(3.2) $$ \begin{align} \int_{B(t_0,\delta)} |\Pi^t({\textbf{i}})-\Pi^t(\mathbf{j}) |^{-s} \;d\eta(t)\leq c e^{|\mathbf{i}\wedge \mathbf{j}|\psi(\delta)} \Big( \max_{x\in \Sigma} \phi^s (D_{\Pi^{t_0} x} f^{t_0}_{\mathbf{i}\wedge \mathbf{j}})\Big)^{-1}, \end{align} $$

where $\psi (\cdot )$ is given as in Definition 1.1.

Proof Take $y\in \Sigma $ so that $ \phi ^s (D_{\Pi ^{t_0} y} f^{t_0}_{\mathbf {i}\wedge \mathbf {j}})= \max _{x\in \Sigma } \phi ^s (D_{\Pi ^{t_0} x} f^t_{\mathbf {i}\wedge \mathbf {j}}). $ Let k be the unique integer such that $s\in (k, k+1)$ . Clearly $k\in \{0,1,\ldots , d-1\}$ . For convenience, write

$$ \begin{align*}a:=\phi^k (D_{\Pi^{t_0} y} f^{t_0}_{\mathbf{i}\wedge \mathbf{j}}),\quad b:=\phi^{k+1}(D_{\Pi^{t_0} y} f^{t_0}_{\mathbf{i}\wedge \mathbf{j}}), \end{align*} $$

where $\phi ^s(\cdot )$ stands for the singular value function (see (2.5) for the definition). A direct check shows that

(3.3) $$ \begin{align} \phi^s (D_{\Pi^{t_0} y} f^t_{\mathbf{i}\wedge \mathbf{j}})=a^{k+1-s}b^{s-k}. \end{align} $$

Observe that

$$ \begin{align*} \int_{B(t_0,\delta)} & |\Pi^t({\textbf{i}})-\Pi^t(\mathbf{j}) |^{-s} \;d\eta(t)\\ &=s\int_0^{\infty} r^{-s-1} \eta \{t\in B(t_0,\delta):\; |\Pi^t({\textbf{ i}})-\Pi^t({\textbf{j}}) |< r\}\; dr\\ &\leq sCe^{|\mathbf{i}\wedge \mathbf{j}|\psi(\delta)} \int_0^{\infty} r^{-s-1} Z^{t_0}_{\mathbf{i}\wedge \mathbf{j}}(r) \; dr \quad (\text{by (1.5)})\\ &\leq sCe^{|\mathbf{i}\wedge \mathbf{j}|\psi(\delta)} \int_0^{\infty} r^{-s-1} \min\bigg\{ \frac{r^k}{a}, \frac{r^{k+1}}{b} \bigg\} \; dr \quad (\text{by (1.4)})\\ &\leq sCe^{|\mathbf{i}\wedge \mathbf{j}|\psi(\delta)} \int_0^{b/a} \frac{r^{k-s}}{b} \;dr+ \int_{b/a}^{\infty} \frac{r^{k-s-1}}{a}\; dr\\ &=sCe^{|\mathbf{i}\wedge \mathbf{j}|\psi(\delta)} \bigg(\frac{1}{k+1-s}+\frac{1}{s-k}\bigg)a^{s-k-1}b^{k-s}\\ &=sC\bigg(\frac{1}{k+1-s}+\frac{1}{s-k}\bigg)e^{|\mathbf{i}\wedge \mathbf{j}|\psi(\delta)} (\phi^s (D_{\Pi^{t_0} y}f^{t_0}_{\mathbf{i}\wedge \mathbf{ j}}))^{-1}\quad (\text{by (3.3))}. \end{align*} $$

This proves (3.2) by setting $c=sC(({1}/({k+1-s}))+({1}/({s-k})))$ .

Proof of Proposition 3.1 Fix $t_0\in {\Omega }$ and $\delta \in (0,\delta _0)$ . We first prove part (i). Let $\epsilon>0$ and let s be non-integral so that

(3.4) $$ \begin{align} 0<s<\min\{d, d_{\mu}(t)\}-\frac{\psi(\delta)}{\log (1/\theta)}-2\epsilon. \end{align} $$

To show that (3.1) holds for $\eta $ -a.e. $t\in B(t_0,\delta )$ , it suffices to show that

(3.5) $$ \begin{align} \underline{\dim}_H\Pi^t_*\mu\geq s \quad \text{for } \eta\text{-a.e.~}t\in B(t_0,\delta). \end{align} $$

For this purpose, we write

(3.6) $$ \begin{align} \varphi^s(I)=\max_{x\in \Sigma} \phi^s(D_{\Pi^{t_0}_x} f_I^{t_0}),\quad I\in \Sigma_*. \end{align} $$

We first prove that

(3.7) $$ \begin{align} \lim_{n\to \infty}\frac{\mu([\mathbf{i}|n])}{\varphi^s(\mathbf{i}|n) \exp(-n \psi(\delta))\theta^{n\epsilon}}=0\quad \text{for } \mu\text{-a.e.~}\mathbf{ i}\in \Sigma. \end{align} $$

To see this, according to the definition of $d_{\mu }(t_0)$ (cf. (1.6) and Definition 2.4),

(3.8) $$ \begin{align} h_{\mu}(\sigma)+\lim_{n\to \infty}\frac{1}{n}\int \log \phi^{d_{\mu}(t_0)} (D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n})\; d\mu(\mathbf{ i})=0. \end{align} $$

It follows from (3.8), the Shannon–McMillan–Breiman theorem and Kingman’s sub-additive ergodic theorem (see [Reference Walters49, pp. 93 and 231]) that

(3.9) $$ \begin{align} \lim_{n\to \infty}\frac{1}{n}\log \frac{\mu([\mathbf{i}|n])}{\phi^{d_{\mu}(t_0)} (D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n})}=0 \quad \text{for } \mu\text{-a.e.~}\mathbf{i}\in \Sigma. \end{align} $$

Observe that for each $\mathbf {i}\in \Sigma $ and $n\in {\Bbb N}$ ,

$$ \begin{align*} \phi^{d_{\mu}(t_0)} (D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n}) &\leq \phi^{s} (D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n}) \|D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n}\|^{d_{\mu}(t_0)-s} \quad \text{(by Lemma 2.2(ii))}\\ &\leq \varphi^{s} (\mathbf{i}|n) \theta^{n(d_{\mu}(t_0)-s)}\quad\quad \text{(by (3.6) and (1.3))}\\ &\leq \varphi^s(\mathbf{i}|n) \exp(-n \psi(\delta))\theta^{2n\epsilon} \quad \text{(by (3.4))}. \end{align*} $$

Combining the above inequality with (3.9) yields (3.7).

By (3.7), we may find a countable disjoint collection of Borel subsets $E_j$ of $\Sigma $ with $\mu (\Sigma \backslash \bigcup _{j=1}^{\infty } E_j)=0$ and numbers $c_j>0$ such that

(3.10) $$ \begin{align} \mu_j([\mathbf{i}|n])\leq c_j \varphi^s(\mathbf{i}|n) \exp(-n \psi(\delta))\theta^{n\epsilon} \quad \text{for all }\mathbf{i}\in \Sigma,\; n\in {\Bbb N}, \end{align} $$

where $\mu _j$ stands for the restriction of $\mu $ to $E_j$ defined by $\mu _j(A)=\mu (E_j\cap A)$ . Clearly,

(3.11) $$ \begin{align} \mu=\sum_{j=1}^{\infty} \mu_j. \end{align} $$

Hence, to prove (3.5), it suffices to show that for each j,

(3.12) $$ \begin{align} \underline{\dim}_H\Pi^t_*\mu_j\geq s \quad \text{for } \eta\text{-a.e.~}t\in B(t_0,\delta). \end{align} $$

By the potential theoretic characterization of the Hausdorff dimension (see e.g. [Reference Falconer16, Theorem 4.13]), it is enough to show that for each j and $\eta $ -a.e. $t\in B(t_0,\delta )$ , $\Pi ^t_*\mu _j$ has finite s-energy:

$$ \begin{align*}I_s(\Pi^t_*\mu_j):=\iint \frac{ d \Pi^t_*\mu_j (x)d \Pi^t_*\mu_j (y)}{|x-y|^{s}}<\infty. \end{align*} $$

Integrating over $B(t_0,\delta )$ with respect to $\eta $ and using Fubini’s theorem,

$$ \begin{align*} \int_{B(t_0,\delta)}I_s(\Pi^t_*\mu_j)\; d\eta(t)&=\int_{B(t_0,\delta)} \iint \frac{ d \Pi^t_*\mu_j (x)d \Pi^t_*\mu_j (y)}{|x-y|^{s}} d\eta(t)\\ &=\int_{B(t_0,\delta)} \iint \frac{ d\mu_j (\mathbf{i})\,d \mu_j (\mathbf{j})}{|\Pi^t(\mathbf{i})-\Pi^t(\mathbf{j})|^{s}} d\eta(t)\\ &= \iint \int_{B(t_0,\delta)} \frac{d\eta(t)}{|\Pi^t(\mathbf{i})-\Pi^t(\mathbf{j})|^{s}} \ d\mu_j (\mathbf{i})\,d \mu_j (\mathbf{j})\\ &\leq \iint c e^{|\mathbf{i}\wedge \mathbf{j}|\psi(\delta)}(\varphi^s(\mathbf{i}\wedge \mathbf{j}))^{-1} d\mu_j (\mathbf{i})\,d \mu_j (\mathbf{ j})\quad \text{(by (3.2), (3.6))}\\ &\leq c\int \sum_{n=0}^{\infty} e^{n\psi(\delta)} (\varphi^s(\mathbf{j}|n))^{-1} \mu_j([\mathbf{j}|n])d \mu_j (\mathbf{j})\\ &\leq cc_j\int \sum_{n=0}^{\infty} \theta^{n\epsilon} d \mu_j (\mathbf{j})\quad \text{(by (3.10))}\\ &<\infty. \end{align*} $$

It follows that $I_s(\Pi ^t_*\mu _j)<\infty $ for $\eta $ -a.e. $t\in B(t_0,\delta )$ . This completes the proof of part (i).

Next we prove part (ii). Take a small $\epsilon>0$ so that

(3.13) $$ \begin{align} d_{\mu}(t_0)>d+\frac{\psi(\delta)}{\log (1/\theta)}+2\epsilon. \end{align} $$

Then for every $\mathbf {i}\in \Sigma $ and $n\in {\Bbb N}$ ,

$$ \begin{align*} \phi^{d_{\mu}(t_0)} (D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n}) &\leq \phi^{d} (D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n}) \|D_{\Pi^{t_0}\sigma^n\mathbf{i}} f^{t_0}_{\mathbf{i}|n}\|^{d_{\mu}(t_0)-d} \quad \text{(by Lemma 2.2(ii))}\\ &\leq \varphi^{d} (\mathbf{i}|n) \theta^{n(d_{\mu}(t_0)-d)}\quad\quad \text{(by (3.6) and (1.3))}\\ &\leq \varphi^d(\mathbf{i}|n) \exp(-n \psi(\delta))\theta^{2n\epsilon} \quad \text{(by (3.13))}. \end{align*} $$

Combining the above inequality with (3.9) yields that

$$ \begin{align*}\lim_{n\to \infty}\frac{\mu([\mathbf{i}|n])}{\varphi^d(\mathbf{i}|n) \exp(-n \psi(\delta))\theta^{n\epsilon}}=0\quad \text{for } \mu\text{-a.e.~}\mathbf{i}\in \Sigma. \end{align*} $$

Hence, there exist finite positive measures $\nu _j$ and numbers $a_j$ ( $j\geq 1)$ such that $\mu =\sum _{j=1}^{\infty } \nu _j$ and

(3.14) $$ \begin{align} \nu_j([\mathbf{i}|n])\leq a_j \varphi^d(\mathbf{i}|n) \exp(-n \psi(\delta))\theta^{n\epsilon} \quad \text{for all }\mathbf{i}\in \Sigma,\; n\in {\Bbb N}. \end{align} $$

Since $\mu =\sum _{j=1}^{\infty } \nu _j$ , to show that $\Pi ^t_*\mu \ll \mathcal L_d$ for $\eta $ -a.e. $t\in B(t_0,\delta )$ , it suffices to show that for each j,

(3.15) $$ \begin{align} \Pi^t_*\nu_j\ll \mathcal L_d \quad \text{for } \eta\text{-a.e.~}t\in B(t_0,\delta). \end{align} $$

To this end, fix j. We will follow a standard approach (introduced by Peres and Solomyak in [Reference Peres and Solomyak40]). In particular, it suffices to show that

$$ \begin{align*}I:=\int_{B(t_0,\delta)} \int \liminf_{r\to 0} \frac{\Pi^t_*\nu_j(B_{{\Bbb R}^d}(x,r)) }{r^d}\; d\Pi^t_*\nu_j(x)\,d\eta(t) <\infty, \end{align*} $$

where $B_{{\Bbb R}^d}(x,r)$ stands for the closed ball in ${\Bbb R}^d$ centered at x of radius r. Observe that by (1.4) and (3.6),

(3.16) $$ \begin{align} Z^{t_0}_{\boldsymbol{\omega}}(r)\leq \inf_{x\in \Sigma} \frac{r^d}{ \phi^d (D_{\Pi^{t_0} x}f^t_{\boldsymbol{\omega}} ) }=\frac{r^d}{\varphi^d(\boldsymbol{\omega})}\quad \text{for }\boldsymbol{\omega}\in \Sigma_*,\; r>0. \end{align} $$

Applying Fatou’s Lemma and Fubini’s Theorem,

$$ \begin{align*} I&\leq \liminf_{r\to 0}\frac{1}{r^d} \int_{B(t_0,\delta)} \int \Pi^t_*\nu_j(B_{{\Bbb R}^d}(x,r)) \; d\Pi^t_*\nu_j(x)\,d\eta(t)\\ &=\liminf_{r\to 0}\frac{1}{r^d} \int_{B(t_0,\delta)} \iint {\textbf{1}}_{\{ (x,y): \; |x-y|\leq r\}} \; d\Pi^t_*\nu_j(x)\,d\Pi^t_*\nu_j(y)\,d\eta(t)\\ &=\liminf_{r\to 0}\frac{1}{r^d} \int_{B(t_0,\delta)} \iint {\textbf{1}}_{\{(\mathbf{i}, \mathbf{j}):\; |\Pi^t(\mathbf{i})-\Pi^t(\mathbf{j})|\leq r\}} \; d\nu_j(\mathbf{i})\,d\nu_j(\mathbf{j})\,d\eta(t) \\ &=\liminf_{r\to 0}\frac{1}{r^d} \iint \int {\textbf{1}}_{\{ t\in B(t_0,\delta):\; |\Pi^t(\mathbf{i})-\Pi^t(\mathbf{j})|\leq r\}} \; d\eta(t)\,d\nu_j(\mathbf{i})\,d\nu_j(\mathbf{j}) \\ &=\liminf_{r\to 0}\frac{1}{r^d} \iint \eta\{t\in B(t_0,\delta):\; |\Pi^t(\mathbf{i})-\Pi^t(\mathbf{j})|\leq r\} \; d\nu_j(\mathbf{i})\,d\nu_j(\mathbf{j}). \end{align*} $$

By (1.5) and (3.16), we obtain that

$$ \begin{align*} I &\leq \liminf_{r\to 0}\frac{1}{r^d} \iint C e^{|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)} Z_{{\textbf{i}}\wedge {\textbf{j}}}^{t_0}(r) \; d\nu_j(\mathbf{i})\,d\nu_j(\mathbf{j})\\ &\leq \iint \frac{C e^{|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)}}{\varphi^d(\mathbf{i}\wedge \mathbf{j})} \; d\nu_j(\mathbf{i})\,d\nu_j(\mathbf{j})\\ &\leq \int \sum_{n=0}^{\infty} \frac{C e^{n \psi(\delta)}}{\varphi^d( \mathbf{j}|n)}\nu_j ([\mathbf{j} |n])\; d\nu_j(\mathbf{j})\\ &\leq a_jC\int \sum_{n=0}^{\infty} \theta^{n\epsilon}\; d\nu_j(\mathbf{j}) \quad \text{(by ({3.14}))}\\ &<\infty, \end{align*} $$

which completes the proof of part (ii).

Now we are ready to prove Theorem 1.2.

Proof of Theorem 1.2(i) Let $\mu $ be a $\sigma $ -invariant ergodic measure on $\Sigma $ . We first show that for $\eta $ -a.e. $t\in {\Omega }$ , $\Pi ^t_*\mu $ is exact dimensional with dimension equal to $\min \{d, d_{\mu }(t)\}$ . Recall that $\overline {\dim }_P\Pi ^t_*\mu \leq \min \{d, d_{\mu }(t)\}$ for each $t\in {\Omega }$ (see Theorem 2.7(ii)). Hence, it is sufficient to show that for $\eta $ -a.e. $t\in {\Omega }$ , $\underline {\dim }_H \Pi ^t_*\mu \geq \min \{d, d_{\mu }(t)\}$ . Suppose on the contrary that this is false. Then there exist $k\in {\Bbb N}$ and $A\subset {\Omega }$ with $\eta (A)>0$ such that

(3.17) $$ \begin{align} \underline{\dim}_H \Pi^t_*\mu< \min\{d, d_{\mu}(t)\}-\frac2k\quad \text{for all } t\in A. \end{align} $$

Take a number $\delta \in (0, \delta _0)$ small enough such that

(3.18) $$ \begin{align} \frac{ \psi(\delta)}{\log (1/\theta)}<\frac1k. \end{align} $$

Since ${\Omega }$ is a separable metric space, it has a countable dense subset

$$ \begin{align*} Y=\{y_n: \; n\in {\Bbb N}\}. \end{align*} $$

Notice that by (1.3) and Lemma 2.6,

$$ \begin{align*}0\leq d_{\mu}(t)\leq d(t)\leq \frac{ \log \ell}{ \log (1/\theta)}\quad \text{for each }t\in {\Omega}. \end{align*} $$

Due to this fact, for each $n\in {\Bbb N}$ , we may pick $y_n^*\in B(y_n,\delta /2)$ so that

(3.19) $$ \begin{align} d_{\mu}(y_n^*)\geq \sup_{t\in B(y_n, \delta/2)}d_{\mu}(t)-\frac{1}{k}. \end{align} $$

Let $Y^*=\{y_{n}^*:\; n\in {\Bbb N}\}$ . Clearly, $Y^*$ is countable. We claim that

(3.20) $$ \begin{align} \sup_{y^*\in B(t, \delta)\cap Y^*} d_{\mu}(y^*)\geq d_{\mu}(t)-\frac1k \quad \text{for all } t\in {\Omega}. \end{align} $$

To see this, let $t\in {\Omega }$ . Since Y is dense in ${\Omega }$ , there exists an integer m such that $\rho (y_m, t)\leq \delta /2$ . Then

(3.21) $$ \begin{align} y_m^*\in B(y_m, \delta/2)\subset B(t,\delta). \end{align} $$

Meanwhile, by (3.19),

$$ \begin{align*}d_{\mu}(y_m^*)\geq \sup_{t'\in B(y_m, \delta/2)}d_{\mu}(t')-\frac{1}{k}\geq d_{\mu}(t)-\frac1k, \end{align*} $$

where in the last inequality, we use the fact that $t\in B(y_m, \delta /2)$ (since $\rho (y_m, t)\leq \delta /2$ ). This proves (3.20), since $y^*_{m}\in B(t,\delta )\cap Y^*$ by (3.21).

Set for $n\in {\Bbb N}$ ,

(3.22) $$ \begin{align} {\Omega}_n=\{t\in B(y_n^*,\delta):\; d_{\mu}(y^*_n)\geq d_{\mu}(t)-1/k\}. \end{align} $$

By (3.20), ${\Omega }=\bigcup _{n=1}^{\infty } {\Omega }_n$ . Define

$$ \begin{align*}E_n=\{t\in B(y_n^*,\delta):\; \underline{\dim}_H \Pi^t_*\mu<\min\{d, d_{\mu}(y_n^*)\}-1/k\},\quad n\in {\Bbb N}. \end{align*} $$

By (3.17), we see that $A\cap {\Omega }_n\subset E_n$ for each $n\in {\Bbb N}$ . However, by Proposition 3.1(i) and (3.18), for each $n\in {\Bbb N}$ and $\eta $ -a.e. $t\in B(y_n^*,\delta )$ ,

$$ \begin{align*}\underline{\dim}_H \Pi^t_*\mu\geq \min\{d, d_{\mu}(y_n^*)\}-\frac{ \psi(\delta)}{\log (1/\theta)}> \min\{d, d_{\mu}(y_n^*)\}-\frac1k. \end{align*} $$

It follows that $\eta (E_n)=0$ for each $n\in {\Bbb N}$ . Hence

$$ \begin{align*}\eta(A)=\eta\bigg(A\cap \bigg( \bigcup_{n=1}^{\infty} {\Omega}_n\bigg)\bigg)\leq \sum_{n=1}^{\infty} \eta(A\cap {\Omega}_n)\leq \sum_{n=1}^{\infty} \eta(E_n)=0, \end{align*} $$

leading to a contradiction. This proves the statement that for $\eta $ -a.e. $t\in {\Omega }$ , $\Pi ^t_*\mu $ is exact dimensional with dimension $\min \{d, d_{\mu }(t)\}$ .

Next we prove that $\Pi ^t_*\mu \ll \mathcal L_d$ for $\eta $ -a.e. $t\in \{t'\in {\Omega }:\; d_{\mu }(t')>d\}$ . Again we use a contradiction. Suppose on the contrary that this result is false. Then there exist $k\in {\Bbb N}$ and $A'\subset {\Omega }$ with $\eta (A')>0$ such that

(3.23) $$ \begin{align} d_{\mu}(t)>d+\frac2k \quad \text{and}\quad \Pi^t_*\mu\not\ll \mathcal L_d\quad \text{for all }t\in A'. \end{align} $$

Set

$$ \begin{align*}F_n=\{t\in B(y_n^*,\delta):\; \Pi^t_*\mu\not \ll \mathcal L_d\}, \quad n\in {\Bbb N}. \end{align*} $$

Clearly, $A'\cap {\Omega }_n\subset F_n$ for each $n\in {\Bbb N}$ . Since ${\Omega }=\bigcup _{n=1}^{\infty } {\Omega }_n$ and $\eta (A')>0$ , there exists $m\in {\Bbb N}$ so that $\eta (A'\cap {\Omega }_m)>0$ . Hence $A'\cap {\Omega }_m\neq \emptyset $ . Pick $t\in A'\cap {\Omega }_m$ . By (3.22), (3.23) and (3.18),

$$ \begin{align*}d_{\mu}(y_m^*)\geq d_{\mu}(t)-\frac{1}{k}>d+\frac{1}{k}>d+\frac{ \psi(\delta)}{\log (1/\theta)}.\end{align*} $$

Hence $\eta (F_m)=0$ by Proposition 3.1(ii). Since $A'\cap {\Omega }_m\subset F_m$ , it follows that $\eta (A'\cap {\Omega }_m)=0$ , leading to a contradiction.

Proof of Theorem 1.2(ii) By Lemma 2.6, for each $t\in {\Omega }$ , we can find a $\sigma $ -invariant ergodic measure $\mu _t$ on $\Sigma $ such that

$$ \begin{align*}d(t)=d_{\mu_t}(t). \end{align*} $$

Moreover, $0\leq d(t)\leq (\log \ell /\log (1/\theta ))$ .

Next we prove that $\dim _H K^t=\dim _BK^t=\min \{d, d(t)\}$ for $\eta $ -a.e. $t\in {\Omega }$ . By Theorem 2.7, $\overline {\dim }_B K^t\leq \min \{d, d(t)\}$ for every $t\in {\Omega }$ . Hence it is sufficient to show that

$$ \begin{align*}\dim_H K^t\geq \min\{d, d(t)\} \quad \text{for } \eta\text{-a.e.~}t\in {\Omega}. \end{align*} $$

Suppose on the contrary that this statement is false. Then there exist $k\in {\Bbb N}$ and $H\subset {\Omega }$ with $\eta (H)>0$ such that

(3.24) $$ \begin{align} \dim_H K^t<\min\{d, d(t)\}-2/k \quad \text{for all } t\in H. \end{align} $$

Take a number $\delta \in (0,\delta _0)$ such that (3.18) holds. Since $d(t)$ is uniformly bounded from above, similar to the construction of $Y^*$ in the proof of part (i), we can construct a countable dense subset $Y'=\{y^{\prime }_n\}_{n=1}^{\infty }$ of ${\Omega }$ such that

(3.25) $$ \begin{align} \sup_{y'\in B(t, \delta)\cap Y'} d(y')\geq d(t)-\frac1k \quad \text{for all } t\in {\Omega}. \end{align} $$

Write

(3.26) $$ \begin{align} {\Omega}_n'=\{t\in B(y^{\prime}_n,\delta):\; d(y^{\prime}_n)\geq d(t)-1/k\}\quad \text{for }n\in {\Bbb N}. \end{align} $$

By (3.25), ${\Omega }=\bigcup _{n=1}^{\infty } {\Omega }_n'$ . Notice that for each $n\in {\Bbb N}$ ,

$$ \begin{align*} {\Omega}_n'\cap H&\subset \{t\in B(y_n', \delta):\; \dim_H K^t<\min\{d, d(y_n')\}-1/k\}\\ &\subset \{t\in B(y_n', \delta):\; \underline{\dim}_H \Pi^t_*(\mu_{y_n'})<\min\{d, d_{\mu_{y_n'}} (y_n')\}-1/k\}\\ &\subset \bigg\{t\in B(y_n', \delta):\; \underline{\dim}_H \Pi^t_*(\mu_{y_n'})<\min\{d, d_{\mu_{y_n'}} (y_n')\}-\frac{ \psi(\delta)}{\log (1/\theta)}\bigg\}, \end{align*} $$

where we have used the facts that $\dim _H K^t\geq \underline {\dim }_H \Pi ^t_*(\mu _{y_n'})$ and $d(y_n')=d_{\mu _{y_n'}} (y_n')$ in the second inclusion, and (3.18) in the last inclusion. Hence $\eta ({\Omega }_n'\cap H)=0$ for each n by applying Proposition 3.1(i). It follows that $\eta (H)\leq \sum _{n=1}^{\infty } \eta ({\Omega }_n'\cap H)=0$ , leading to a contradiction. This completes the proof of the statement that $\dim _H K^t=\min \{d, d(t)\}$ for $\eta $ -a.e. $t\in {\Omega }$ .

Finally, we prove that $\mathcal L_d(K^t)>0$ for $\eta $ -a.e. $t\in \{t'\in {\Omega }:\; d(t')>d\}$ . Suppose on the contrary that this result is false. Then there exist $k\in {\Bbb N}$ and $H'\subset {\Omega }$ with $\eta (H')>0$ such that

(3.27) $$ \begin{align} d(t)>d+\frac2k \quad \text{and}\quad \mathcal L_d(K^t)=0\quad \text{for all }t\in H'. \end{align} $$

Set

$$ \begin{align*}F_n'=\{t\in B(y_n',\delta):\; \mathcal L_d(K^t)=0\}, \quad n\in {\Bbb N}. \end{align*} $$

Clearly, $H'\cap {\Omega }_n'\subset F^{\prime }_n$ for each $n\in {\Bbb N}$ . Since ${\Omega }=\bigcup _{n=1}^{\infty } {\Omega }_n'$ and $\eta (H')>0$ , there exists $m\in {\Bbb N}$ so that $\eta (H'\cap {\Omega }_m')>0$ . Hence $H'\cap {\Omega }_m'\neq \emptyset $ . Taking $t\in H'\cap {\Omega }_m'$ and applying (3.26), (3.27) and (3.18) gives

$$ \begin{align*}d_{\mu_{y_m'}}(y_m')=d(y_m')\geq d(t)-\frac1k>d+\frac{1}{k}>d+\frac{ \psi(\delta)}{\log (1/\theta)}.\end{align*} $$

Now by Proposition 3.1(ii), $\Pi ^t_*(\mu _{y_m'})\ll \mathcal L_d$ for $\eta $ -a.e. $t\in B(y_m', \delta )$ . This implies that $\eta (F_m')=0$ . Since $H'\cap {\Omega }_m'\subset F_m'$ , it follows that $\eta (H'\cap {\Omega }_m')=0$ , leading to a contradiction.

4 Translational family of IFSs generated by a dominated lower triangular $C^1$ IFS

In this section, we show that under mild assumptions, a translational family of $C^1$ IFSs, generated by a dominated lower triangular $C^1$ IFS, satisfies the GTC. To begin with, let S be a compact subset of ${\Bbb R}^d$ with non-empty interior.

Definition 4.1. Let $\ell \in {\Bbb N}$ with $\ell \geq 2$ . We say that $\mathcal F=\{f_i\}_{i=1}^{\ell }$ is a dominated lower triangular $C^1$ IFS on S if the following conditions hold.

  1. (i) $f_i(S)\subset \mathrm {int} (S)$ , $i=1,\ldots , \ell $ .

  2. (ii) There exists a bounded open connected set $U\supset S$ such that each $f_i$ extends to a contracting $C^1$ diffeomorphism $f_i: U\to f_i(U)$ with $\overline {f_i(U)}\subset U$ .

  3. (iii) For each $z\in S$ and $i\in \{1,\ldots , \ell \}$ , the Jacobian matrix $D_zf_i$ of $f_i$ at z is a lower triangular matrix such that

    $$ \begin{align*}|(D_zf_i)_{\mathit{jj}}|\leq |(D_zf_i)_{kk}|\quad \text{for all }1\leq k\leq j\leq d. \end{align*} $$

In the remaining part of this section, we fix a dominated lower triangular $C^1$ IFS $\mathcal F=\{f_i\}_{i=1}^{\ell }$ on S.

By continuity, there exists a small $r_0>0$ such that the following holds. Setting

$$ \begin{align*} f_i^{\boldsymbol{\mathfrak{t}}}:=f_i+\mathbf{t}_i \end{align*} $$

for $1\leq i\leq \ell $ and $\boldsymbol {\mathfrak {t}}=(\mathbf {t}_1,\ldots , \mathbf {t}_{\ell })\in {\Bbb R}^{\ell d}$ with $|\boldsymbol {\mathfrak {t}}|< r_0$ , we have $f_i^{\boldsymbol {\mathfrak {t}}}(S)\subset \mathrm {int}(S)$ for each i.

Write $\Delta :=\{\boldsymbol {\mathfrak {t}}\in {\Bbb R}^{\ell d}:\; |\boldsymbol {\mathfrak {t}}|<r_0\}$ and set

$$ \begin{align*} \mathcal F^{\boldsymbol{\mathfrak{t}}}=\{f_i^{\boldsymbol{\mathfrak{t}}}\}_{i=1}^{\ell},\quad \boldsymbol{\mathfrak{t}}\in \Delta. \end{align*} $$

We call $\mathcal F^{\boldsymbol {\mathfrak {t}}}$ , ${\boldsymbol {\mathfrak {t}}\in \Delta }$ , a translational family of IFSs generated by $\mathcal F$ . For $\mathbf {i}=i_1\ldots i_n\in \Sigma _n$ , we write $f_{\mathbf { i}}^{\boldsymbol {\mathfrak {t}}}=f_{i_1}^{\boldsymbol {\mathfrak {t}}}\circ \cdots \circ f_{i_n}^{\boldsymbol {\mathfrak {t}}}$ .

For a $C^1$ map $g: S\to {\Bbb R}^d$ and $z_1,\ldots , z_d\in S$ , we write

(4.1) $$ \begin{align} D_{z_1,\ldots, z_d}^*g=\left[\begin{array}{c} \nabla^Tg_1(z_1) \\ \vdots \\ \nabla^Tg_d(z_d) \end{array}\right]=\left[ \begin{array}{ccc} \displaystyle\frac{\partial g_1}{\partial x_1}(z_1) & \cdots &\displaystyle\frac{\partial g_1}{\partial x_d}(z_1)\\ \vdots & \ddots & \vdots \\ \displaystyle\frac{\partial g_d}{\partial x_1}(z_d) & \cdots &\displaystyle\frac{\partial g_d}{\partial x_d}(z_d) \end{array} \right], \end{align} $$

where $g_i$ is the ith component of the map g, $i=1,\ldots , d$ . Clearly,

(4.2) $$ \begin{align} (D_{z_1,\ldots, z_d}^*g)_{\mathit{ij}}=(D_{z_i}g)_{\mathit{ij}}\quad \text{for all }1\leq i,j\leq d. \end{align} $$

The main result in this section is the following.

Theorem 4.2. Let $\mathcal F^{\boldsymbol {\mathfrak {t}}}$ , ${\boldsymbol {\mathfrak {t}}\in \Delta }$ , be a translational family of IFSs generated by a dominated lower triangular $C^1$ IFS $\mathcal F$ defined on a compact convex subset S of ${\Bbb R}^d$ . Suppose in addition that

(4.3) $$ \begin{align} \rho:=\max_{1\leq i,j\leq \ell:\; i\neq j} \Big(\sup_{y\in S} \|D_yf_i\|+\sup_{z\in S} \|D_zf_j\|\Big)<1. \end{align} $$

Then $\mathcal F^{\boldsymbol {\mathfrak {t}}}$ , $\boldsymbol {\mathfrak {t}}\in \Delta $ , satisfies the GTC with respect to $\ell d$ -dimensional Lebesgue measure $\mathcal L_{\ell d}$ restricted to $\Delta $ .

The proof of the above theorem is based on the following.

Proposition 4.3. Let $\mathcal F^{\boldsymbol {\mathfrak {t}}}$ , ${\boldsymbol {\mathfrak {t}}\in \Delta }$ , be a translational family of IFSs generated by a dominated lower triangular $C^1$ IFS $\mathcal F$ on a compact subset S of ${\Bbb R}^d$ . Then there exists a function $h: (0, r_0)\to (0,\infty )$ with $\lim _{\delta \to 0} h(\delta )=0$ such that for each $\delta \in (0,r_0)$ , there is $C(\delta )\geq 1$ so that

(4.4) $$ \begin{align} \| D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}}\cdot(D^*_{z_1,\ldots, z_d} f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{t}}})^{-1}\|\leq C(\delta) e^{nh(\delta)} \end{align} $$

for every $n\in {\Bbb N}$ , $\boldsymbol {\omega }\in \Sigma _n$ , $y, z_1,\ldots , z_d\in S$ and $\boldsymbol {\mathfrak {s}},\boldsymbol {\mathfrak {t}}\in \Delta $ with $|\boldsymbol {\mathfrak {s}}-\boldsymbol {\mathfrak {t}}|<\delta $ .

In the next two subsections, we prove Proposition 4.3 and Theorem 4.2, respectively.

4.1 Proof of Proposition 4.3

We first prove several auxiliary lemmas.

Lemma 4.4. Let $c\geq 1$ and $d\in {\Bbb N}$ . Let A be a real $d\times d$ non-singular lower triangular matrix such that

(4.5) $$ \begin{align} |A_{\mathit{ij}}|\leq c|A_{\mathit{jj}}|\quad \text{for all }1\leq i,j\leq d. \end{align} $$

Then

$$ \begin{align*}|(A^{-1})_{\mathit{ij}}|\leq (c\sqrt{d})^{d-1}|(A^{-1})_{\mathit{ii}}|\quad \text{for all }1\leq i,j\leq d. \end{align*} $$

Proof It is well known (see e.g. [Reference Horn and Johnson28]) that $A^{-1}=({1}/{\det (A)}) \text {adj}(A)$ , where $\text {adj}(A)$ is the adjugate matrix of A defined by

$$ \begin{align*}(\text{adj}(A))_{\mathit{ij}}=(-1)^{i+j}\det(A(j,i)),\quad 1\leq i,j\leq d, \end{align*} $$

where $A(j,i)$ is the $(d-1)\times (d-1)$ matrix that results from A by removing the jth row and ith column. By the Hadamard’s inequality (see e.g. [Reference Horn and Johnson28, Corollary 7.8.2]), $|\!\det (A(j,i))|$ is bounded above by the product of the Euclidean norms of the columns of $A(j,i)$ . In particular, this implies that

$$ \begin{align*}|\!\det(A(j,i))|\leq \prod_{1\leq k\leq d:\; k\neq i}|v_k|, \end{align*} $$

where $v_k$ denotes the kth column vector of A. By (4.5),

$$ \begin{align*}|v_k|=\sqrt{\sum_{i=1}^d(A_{ik})^2}\leq c\sqrt{d}|A_{kk}|,\end{align*} $$

so $|\!\det (A(j,i))|\leq (c\sqrt {d})^{d-1} \prod _{1\leq k\leq d:\; k\neq i} |A_{kk}|$ . Hence for given $1\leq i,j\leq d$ ,

$$ \begin{align*}\frac{|(A^{-1})_{\mathit{ij}}|}{|(A^{-1})_{\mathit{ii}}|}=\frac{|\!\det(A(j,i)|}{\det(A)\cdot |(A^{-1})_{\mathit{ii}}|}\leq \frac{(c\sqrt{d})^{d-1} \prod_{1\leq k\leq d:\; k\neq i} |A_{kk}|}{\det(A)\cdot |(A^{-1})_{\mathit{ii}}|}=(c\sqrt{d})^{d-1}.\\[-42pt] \end{align*} $$

For $c\geq 1$ and $d\in {\Bbb N}$ , let $\mathcal T_c(d)$ denote the collection of real $d\times d$ lower triangular matrices $A=(a_{\mathit {ij}})$ satisfying the following two conditions:

  1. (i) $|a_{11}|\geq |a_{22}|\geq \cdots \geq |a_{dd}|>0$ ;

  2. (ii) $|a_{\mathit {ij}}|\leq c|a_{\mathit {jj}}|$ for all $ 1\leq i,j\leq d$ .

Then we have the following estimates.

Lemma 4.5. Let $n\in {\Bbb N}$ and $A_1,\ldots , A_n\in \mathcal T_c(d)$ . Then for $1\leq j\leq i\leq d$ ,

(4.6) $$ \begin{align} |(A_1\cdots A_n)_{\mathit{ij}}|\leq (cn)^{i-j} |(A_1\cdots A_n)_{\mathit{jj}}|. \end{align} $$

Proof We prove by induction on n. Since $A_1\in \mathcal T_c(d)$ , the inequality (4.6) holds when $n=1$ . Now assume that (4.6) holds when $n=k$ . Below we show that it also holds when $n=k+1$ .

Given $A_1,\ldots , A_{k+1}\in \mathcal T_c(d)$ , we write $A=A_1$ and $B=A_2\cdots A_{k+1}$ . Clearly B is lower triangular. By the induction assumption, $|B_{\mathit {ij}}|\leq (ck)^{i-j} |B_{\mathit {jj}}|$ for each pair $(i,j)$ with $1\leq j\leq i\leq d$ .

Now fix a pair $(i,j)$ with $1\leq j\leq i\leq d$ . Observe that

(4.7) $$ \begin{align} \frac{(AB)_{\mathit{ij}}}{(AB)_{\mathit{jj}}}=\sum_{ p=j}^i\frac{A_{\mathit{ip}}}{A_{\mathit{\mathit{jj}}}} \cdot \frac{B_{\mathit{pj}}}{B_{\mathit{jj}}}=\frac{A_{\mathit{ii}}}{A_{\mathit{jj}}} \cdot \frac{B_{\mathit{ij}}}{B_{\mathit{jj}}}+\sum_{p=j}^{i-1} \frac{A_{\mathit{ip}}}{A_{\mathit{jj}}} \cdot \frac{B_{\mathit{pj}}}{B_{\mathit{jj}}}. \end{align} $$

Applying the inequalities $|A_{\mathit {ii}}|\leq |A_{\mathit {jj}}|$ , $|B_{\mathit {ij}}|\leq (ck)^{i-j}|B_{\mathit {jj}}|$ , $|A_{\mathit {ip}}|\leq c|A_{pp}|\leq c|A_{\mathit {jj}}|$ and $|B_{\mathit {pj}}|\leq (ck)^{p-j}|B_{\mathit {jj}}|$ to (4.7) gives

$$ \begin{align*}\bigg|\frac{(AB)_{\mathit{ij}}}{(AB)_{\mathit{jj}}}\bigg|\leq (ck)^{i-j} + c\sum_{p=j}^{i-1}(ck)^{p-j}\leq (c(k+1))^{i-j}. \end{align*} $$

Hence (4.6) holds for $n=k+1$ .

Lemma 4.6. Let $\mathcal F^{\boldsymbol {\mathfrak {t}}}=\{f_i^{\boldsymbol {\mathfrak {t}}}\}_{i=1}^{\ell }$ , ${\boldsymbol {\mathfrak {t}}\in \Delta }$ , be a translational family of IFSs on a compact subset S of ${\Bbb R}^d$ generated by a $C^1$ IFS $\mathcal F=\{f_i\}_{i=1}^{\ell }$ . Let $\theta \in (0,1)$ be a common Lipschitz constant of $f_1,\ldots , f_{\ell }$ on S. That is,

$$ \begin{align*}|f_i(u)-f_i(v)|\leq \theta|u-v| \quad \text{for all }1\leq i\leq \ell\text{ and }u, v\in S. \end{align*} $$

Then for ${\mathfrak {s}}, {\mathfrak {t}}\in \Delta $ , $u,v\in S$ , $n\in {\Bbb N}$ and $\boldsymbol {\tau }\in \Sigma _{n}$ ,

(4.8) $$ \begin{align} | f^{\boldsymbol{\mathfrak{t}} }_{\boldsymbol{\tau}}(u) - f^{\boldsymbol{\mathfrak{s}} }_{\boldsymbol{\tau}}(v) | \leq \frac{|\boldsymbol{\mathfrak{t}} -\boldsymbol{\mathfrak{s}}|}{1-\theta} + \theta^{n} \bigg( |u-v|- \frac{|\boldsymbol{\mathfrak{t}} -\boldsymbol{\mathfrak{s}}|}{1-\theta} \bigg). \end{align} $$

In particular,

(4.9) $$ \begin{align} | f^{\boldsymbol{\mathfrak{t}} }_{\boldsymbol{\tau}}(u) - f^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\tau}}(u) | \leq \frac{|\boldsymbol{\mathfrak{t}} -\boldsymbol{\mathfrak{s}}|}{1-\theta}\quad \text{and} \quad | f^{\boldsymbol{\mathfrak{t}} }_{\boldsymbol{\tau}}(u) - f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\tau}}(v) | \leq \theta^n |u-v|. \end{align} $$

Proof To verify (4.8), we let $i\in \{1,\ldots , \ell \}$ . Then

$$ \begin{align*} | f^{\boldsymbol{\mathfrak{t}} }_i(u)-f^{\boldsymbol{\mathfrak{s}}}_i(v) | &\leq | f^{\boldsymbol{\mathfrak{t}} }_i(u)-f^{\boldsymbol{\mathfrak{s}} }_i(u) | + | f^{\boldsymbol{\mathfrak{s}} }_i(u)-f^{\boldsymbol{\mathfrak{s}} }_i(v) | \\ &= | \mathbf{t}_i-\mathbf{s}_i | + | f_i(u)-f_i(v) | \\ &\leq | \boldsymbol{\mathfrak{t}}-\boldsymbol{\mathfrak{s}} | +\theta|u-v|. \end{align*} $$

Let $\varphi :\;{\Bbb R}\to {\Bbb R}$ be a contracting affine map defined by $\varphi (x)= | \boldsymbol {\mathfrak {t}}-\boldsymbol {\mathfrak {s}} | +\theta x$ for given $\boldsymbol {\mathfrak {s}}$ and $\boldsymbol {\mathfrak {t}}$ . Then for every $1\leq i\leq \ell $ ,

(4.10) $$ \begin{align} | f^{\boldsymbol{\mathfrak{t}} }_i(u)-f^{\boldsymbol{\mathfrak{s}}}_i(v) | \leq \varphi(|u-v|). \end{align} $$

Now we can prove (4.8) by using the above inequality. Indeed, using (4.10) and the fact that $\varphi (\cdot )$ is monotone increasing, we obtain that for $1\leq i,j\leq \ell $ ,

$$ \begin{align*} | f^{\boldsymbol{\mathfrak{t}} }_j( f^{\boldsymbol{\mathfrak{t}} }_i(u) ) - f^{\boldsymbol{\mathfrak{s}} }_j( f^{\boldsymbol{\mathfrak{s}} }_i(v) ) | \leq \varphi( | f^{\boldsymbol{\mathfrak{t}} }_{i}(u) - f^{\boldsymbol{\mathfrak{s}}}_{i}(v) | ) \leq \varphi^2(|u-v|). \end{align*} $$

Successive application of this implies that for every $\boldsymbol {\tau }\in \Sigma _{n}$ and $u,v\in S$ ,

$$ \begin{align*}| f^{\boldsymbol{\mathfrak{t}} }_{\boldsymbol{\tau}}(u) - f^{\boldsymbol{\mathfrak{s}} }_{\boldsymbol{\tau}}(v) | \leq \varphi^{n}(|u-v|)=\frac{|\boldsymbol{\mathfrak{t}} -\boldsymbol{\mathfrak{s}}|}{1-\theta} + \theta^{n} \bigg( |u-v|- \frac{|\boldsymbol{\mathfrak{t}} -\boldsymbol{\mathfrak{s}}|}{1-\theta} \bigg). \end{align*} $$

This proves (4.8). The assertions in (4.9) then follow directly from (4.8).

Now we are ready to prove Proposition 4.3.

Proof of Proposition 4.3 We divide the proof into five small steps.

Step 1. Write

(4.11) $$ \begin{align} C_n:=\sup\bigg\{ \bigg|\frac{(D_yf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}{(D_zf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}\bigg|:\; \boldsymbol{\mathfrak{t}}\in \Delta,\; y,z\in S, \;{\boldsymbol{\omega}}\in \Sigma_n,\; 1\leq i\leq d\bigg\}. \end{align} $$

We claim that

(4.12) $$ \begin{align} \lim_{n\to \infty}\frac{1}{n}\log C_n=0. \end{align} $$

To prove this claim, for each $p\in \{1,\ldots , \ell \}$ and $i\in \{1,\ldots , d\}$ , we define a function $a_{p,i}:\; S\to {\Bbb R}$ by

$$ \begin{align*} a_{p,i}(z)=\log |(D_zf_p)_{\mathit{ii}}|. \end{align*} $$

Clearly, the functions $a_{p,i}$ are continuous on S. Since the matrix $D_zf_p$ is lower triangular for each $z\in S$ and $1\leq p\leq \ell $ , it follows that for $\boldsymbol {\mathfrak {t}}\in \Delta $ , $y,z\in S$ , ${\boldsymbol {\omega }}=\omega _1\cdots \omega _n\in \Sigma _n$ and $1\leq i\leq d$ ,

(4.13) $$ \begin{align} \log |(D_zf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}|=\sum_{k=1}^n a_{\omega_k,i}(f^{\boldsymbol{\mathfrak{t}}}_{\sigma^k{{\boldsymbol{\omega}}}}(z)) \end{align} $$

and

(4.14) $$ \begin{align} \log \bigg|\frac{(D_yf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}{(D_zf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}\bigg|=\sum_{k=1}^n \bigg(a_{\omega_k,i}(f^{\boldsymbol{\mathfrak{t}}}_{\sigma^k{{\boldsymbol{\omega}}}}(y))- a_{\omega_k,i}(f^{\boldsymbol{\mathfrak{t}}}_{\sigma^k{{\boldsymbol{\omega}}}}(z))\bigg), \end{align} $$

where $\sigma ^k{{\boldsymbol {\omega }}}:=\omega _{k+1}\cdots \omega _n$ for $1\leq k\leq n-1$ , $\sigma ^n{{\boldsymbol {\omega }}}:=\varepsilon $ (here $\varepsilon $ stands for the empty word) and $f^{\boldsymbol {\mathfrak {t}}}_{\varepsilon }(y):=y$ . Define $\gamma : (0,\infty )\to (0,\infty )$ by

(4.15) $$ \begin{align} \gamma(u)=\max_{1\leq p\leq \ell,\;1\leq i\leq d}\sup \{|a_{p,i}(y)-a_{p,i}(z)|:\; y,z\in S,\; |y-z|\leq u\}. \end{align} $$

Since S is compact and $a_{p,i}$ are continuous, it follows that $\lim _{u\to 0}\gamma (u)=0$ . To estimate the term in the left-hand side of the equality (4.14), by Lemma 4.6 we obtain that

$$ \begin{align*}|f^{\boldsymbol{\mathfrak{t}}}_{\sigma^k{{\boldsymbol{\omega}}}}(y)-f^{\boldsymbol{\mathfrak{t}}}_{\sigma^k{{\boldsymbol{\omega}}}}(z)|\leq \theta^{n-k}|y-z|\leq \theta^{n-k}\mathrm{diam}(S), \end{align*} $$

where $\theta \in (0,1)$ is a common Lipschitz constant of $f_1,\ldots , f_{\ell }$ on S. Hence by (4.14),

$$ \begin{align*}\frac{1}{n} \log \bigg|\frac{(D_yf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}{(D_zf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}\bigg|\leq \frac{1}{n} \sum_{k=1}^n\gamma(\theta^{n-k}\mathrm{diam}(S))\to 0\quad \text{as }n\to \infty. \end{align*} $$

This proves (4.12).

Step 2. For $\boldsymbol {\mathfrak {s}},\boldsymbol {\mathfrak {t}}\in \Delta $ , $y\in S$ , $n\in {\Bbb N}$ , ${\boldsymbol {\omega }}\in \Sigma _n$ and $1\leq i\leq d$ ,

(4.16) $$ \begin{align} \bigg|\frac{(D_yf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}{(D_yf^{\boldsymbol{\mathfrak{s}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}\bigg|\leq \exp\bigg(n\gamma\bigg(\frac{|\boldsymbol{\mathfrak{t}}-\boldsymbol{\mathfrak{s}}|}{1-\theta}\bigg)\bigg), \end{align} $$

where $\gamma (\cdot )$ is defined as in (4.15) and $\theta \in (0,1)$ is a common Lipschitz constant for $f_1,\ldots , f_{\ell }$ on S.

To prove (4.16), by (4.13) we see that

$$ \begin{align*} \log \bigg|\frac{(D_yf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}{(D_yf^{\boldsymbol{\mathfrak{s}}}_{{\boldsymbol{\omega}}} )_{\mathit{ii}}}\bigg|&=\sum_{k=1}^n (a_{\omega_k,i}(f^{\boldsymbol{\mathfrak{t}}}_{\sigma^k{{\boldsymbol{\omega}}}}(y))- a_{\omega_k,i}(f^{\boldsymbol{\mathfrak{s}}}_{\sigma^k{{\boldsymbol{\omega}}}}(y))\\ &\leq n \gamma \bigg(\frac{|\boldsymbol{\mathfrak{t}}-\boldsymbol{\mathfrak{s}}|}{1-\theta}\bigg), \end{align*} $$

where in the second inequality, we have used the fact that $|f^{\boldsymbol {\mathfrak {t}}}_{\sigma ^k{{\boldsymbol {\omega }}}}(y)-f^{\boldsymbol {\mathfrak {s}}}_{\sigma ^k{{\boldsymbol {\omega }}}}(y)|\leq ({|\boldsymbol {\mathfrak {t}}-\boldsymbol {\mathfrak {s}}|})/({1-\theta })$ (which follows from (4.9)). This proves (4.16).

Step 3. Set

(4.17) $$ \begin{align} c=\sup\bigg\{\bigg|\frac{(D_yf_p)_{\mathit{ij}}}{(D_yf_p)_{\mathit{jj}}}\bigg|:\; y\in S,\; 1\leq p\leq \ell,\; 1\leq i,j\leq d\bigg\}. \end{align} $$

Then

(4.18) $$ \begin{align} \bigg|\frac{(D_yf_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}})_{\mathit{ij}}}{(D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}})_{\mathit{jj}}} \bigg|\leq (cn)^d \quad \text{for all } \boldsymbol{\mathfrak{s}}\in \Delta,\; y\in S,\; \boldsymbol{\omega}\in \Sigma_n,\; 1\leq i,j\leq d. \end{align} $$

To see this, we simply notice that $D_yf_{{\boldsymbol {\omega }}}^{\boldsymbol {\mathfrak {s}}}=\prod _{k=1}^n D_{f^{\boldsymbol {\mathfrak {s}}}_{\sigma ^k {\boldsymbol {\omega }}}(y)}f_{\omega _k}$ and apply Lemma 4.5.

Step 4. Let c and $C_n$ be defined as in (4.17) and (4.11). Then for $\boldsymbol {\mathfrak {t}}\in \Delta $ , $y, z_1,\ldots , z_d\in S$ , $\boldsymbol {\omega }\in \Sigma _n$ and $1\leq k,j\leq d$ ,

(4.19) $$ \begin{align} |((D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})^{-1})_{kj}| \leq (cn)^{d(d-1)}(\sqrt{d})^{d-1}(C_n)^d \frac{1}{|(D_yf^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{kk}|}, \end{align} $$

where $D_{z_1,\ldots , z_d}^*g$ is defined as in (4.1).

To prove (4.19), notice that for all $1\leq k,j\leq d$ ,

$$ \begin{align*} |(D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{kj}|&= |(D_{z_k}f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{kj}| \quad \text{(by (4.2))}\\ &\leq (cn)^d |(D_{z_k}f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{\mathit{jj}}| \quad \text{(by (4.18))}\\ &\leq (cn)^d C_n |(D_{z_j}f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{\mathit{jj}}| \quad \text{(by (4.11))}\\ &= (cn)^d C_n |(D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{\mathit{jj}}|\quad \text{(by (4.2))}. \end{align*} $$

Applying Lemma 4.4 (in which we replace c by $(cn)^dC_n$ and take $A=D_{z_1,\ldots , z_d}^*f^{\boldsymbol {\mathfrak {t}}}_{{\boldsymbol {\omega }}}$ ), we obtain

$$ \begin{align*} \begin{split} |((D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})^{-1})_{kj}|&\leq (cn)^dC_n\sqrt{d})^{d-1}|((D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})^{-1})_{kk}|\\ & =((cn)^dC_n\sqrt{d})^{d-1}|((D_{z_k}f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})^{-1})_{kk}|\\ & =((cn)^dC_n\sqrt{d})^{d-1}\frac{1}{|(D_{z_k}f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{kk}|}\\ &\leq ((cn)^dC_n\sqrt{d})^{d-1}C_n\frac{1}{|(D_{y}f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}})_{kk}|}, \end{split} \end{align*} $$

from which (4.19) follows.

Step 5. Now we are ready to prove (4.4). Let $\delta \in (0,r_0)$ . Write

$$ \begin{align*} u_n:=(cn)^{d(d-1)}(\sqrt{d})^{d-1}(C_n)^d,\quad n\in {\Bbb N}. \end{align*} $$

Then, for $\boldsymbol {\mathfrak {s}},\boldsymbol {\mathfrak {t}}\in \Delta $ with $|\boldsymbol {\mathfrak {t}}-\boldsymbol {\mathfrak {s}}|\leq \delta $ and $1\leq i,j\leq d$ ,

$$ \begin{align*} | (D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}}\cdot(D^*_{z_1,\ldots, z_d} f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{t}}})^{-1})_{\mathit{ij}}| &\leq \sum_{k=1}^d| (D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}})_{ik}|\cdot | (D^*_{z_1,\ldots, z_d} f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{t}}})^{-1})_{kj} |\\ &\leq (cn)^du_n\sum_{k=1}^d\bigg| \frac{(D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}})_{kk}}{(D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{t}}})_{kk}}\bigg|\quad \text{(by (4.18), (4.19))}\\ &\leq d(cn)^du_n\exp\bigg(n \gamma \bigg(\frac{|\boldsymbol{\mathfrak{t}}-\boldsymbol{\mathfrak{s}}|}{1-\theta}\bigg)\bigg)\quad \text{(by (4.16))}\\ &\leq d(cn)^du_n\exp\bigg(n \gamma \bigg(\frac{\delta}{1-\theta}\bigg)\bigg). \end{align*} $$

This implies that

(4.20) $$ \begin{align} \| D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}}\cdot(D^*_{z_1,\ldots, z_d} f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{t}}})^{-1}\|\leq d^2(cn)^du_n\exp\bigg(n \gamma \bigg(\frac{\delta}{1-\theta}\bigg)\bigg), \end{align} $$

where we have used an easily checked fact that

$$ \begin{align*}\|A\|\leq d\max_{1\leq i,j\leq d}|A_{\mathit{ij}}| \end{align*} $$

for $A=(A_{\mathit {ij}})\in {\Bbb R}^{d\times d}$ .

Set $h:(0,r_0)\to (0,\infty )$ by $h(x)=x+ \gamma ({x}/({1-\theta }))$ . Since

$$ \begin{align*}\lim_{n\to \infty}\frac{1}{n}\log (d^2(cn)^du_n)=0, \end{align*} $$

there exists $C(\delta )>0$ such that $d^2(cn)^du_ne^{-n\delta }\leq C(\delta )$ for all $n\geq 1$ . According to this fact and (4.20), we obtain the desired inequality

$$ \begin{align*}\| D_y f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}}\cdot(D^*_{z_1,\ldots, z_d} f_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{t}}})^{-1}\|\leq C(\delta) \exp(nh(\delta));\end{align*} $$

for later convenience, we may assume that $C(\delta )\geq 1$ .

4.2 Proof of Theorem 4.2

The following result plays a key part in our proof.

Lemma 4.7. Let $\{\mathcal F^{\boldsymbol {\mathfrak {t}}}\}_{\boldsymbol {\mathfrak {t}}\in \Delta }$ be a translational family of IFSs on a compact set $S\subset {\Bbb R}^d$ generated by a $C^1$ IFS $\mathcal F=\{f_i\}_{i=1}^{\ell }$ . Suppose that (4.3) holds. Let $\delta>0$ . Then there exists $\widetilde {C}>0$ , which depends on $\mathcal F$ and $\delta $ such that the following holds. Let $\mathbf {a}=(a_n)_{n=1}^{\infty },\mathbf {b}=(b_n)_{n=1}^{\infty }\in \Sigma $ with $a_1\neq b_1$ , and let A be a real invertible $d\times d$ matrix. Then for $\boldsymbol {\mathfrak {s}}\in \Delta $ and $r>0$ ,

(4.21) $$ \begin{align} \mathcal L_{\ell d}&\{\boldsymbol{\mathfrak{t}}\in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}}, \delta)\cap \Delta:\; \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in A^{-1}B_{{\Bbb R}^d}(0,r)\} \nonumber\\ &\leq \widetilde{C}\min\bigg\{\frac{r^k}{\phi^k(A)}:\; k=0,1,\ldots,d\bigg\}, \end{align} $$

where $B_{{\Bbb R}^{\ell d}}(\cdot ,\cdot )$ and $B_{{\Bbb R}^d}(\cdot ,\cdot )$ stand for closed balls in ${\Bbb R}^{\ell d}$ and ${\Bbb R}^{d}$ , respectively.

Since the proof of the above lemma is a little long, we will postpone it until we have finished the proof of Theorem 4.2.

Proof of Theorem 4.2 by assuming Lemma 4.7 Fix $\boldsymbol {\mathfrak {s}}\in \Delta $ and $\delta \in (0,r_0)$ . Let $\mathbf {i},\mathbf {j}\in \Sigma $ with $\mathbf {i}\neq \mathbf {j}$ . Set

$$ \begin{align*} \boldsymbol{\omega}=\mathbf{i}\wedge \mathbf{j}\quad \text{and}\quad n=|\boldsymbol{\omega}|. \end{align*} $$

Write $\mathbf {a}=\sigma ^n \mathbf {i}$ and $\mathbf {b}=\sigma ^n \mathbf {j}$ . Clearly $a_1\neq b_1$ .

Fix $y\in S$ . We claim that for $r>0$ ,

(4.22) $$ \begin{align} &\{\boldsymbol{\mathfrak{t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{j})|< r\}\nonumber\\ &\text{}\; \subset \{\boldsymbol{\mathfrak{t}}\in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in (D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})^{-1} B_{{\Bbb R}^d}(0,C(\delta)e^{nh(\delta)}r) \}, \end{align} $$

where $C(\delta )$ and $h(\delta )$ are given as in Proposition 4.3.

To show (4.22), let $\boldsymbol {\mathfrak {t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol {\mathfrak {s}},\delta )\cap \Delta $ so that $|\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {i})-\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {j})|<r$ . Notice that

$$ \begin{align*} \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ j})=f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}}(\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ a}))-f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}}(\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})). \end{align*} $$

Since S is convex, by the mean value theorem, there exist $z_1,\ldots , z_d\in S$ such that

$$ \begin{align*}\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{j})=(D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}})(\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})). \end{align*} $$

Hence

$$ \begin{align*} \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})&=(D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}})^{-1}(\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ j}))\\ &\in (D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}})^{-1}B_{{\Bbb R}^d}(0,r)\\ &= (D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})^{-1} D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}} (D_{z_1,\ldots, z_d}^*f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}})^{-1}B_{{\Bbb R}^d}(0,r)\\ &\subset (D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})^{-1} B_{{\Bbb R}^d}(0,C(\delta)e^{nh(\delta)}r)\quad \text{(by Proposition~4.3).} \end{align*} $$

This proves (4.22).

By (4.22) and Lemma 4.7, we see that

$$ \begin{align*} \begin{split} \mathcal L_{\ell d}&\{\boldsymbol{\mathfrak{t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{j})|< r\}\\ &\leq \mathcal L_{\ell d} \{\boldsymbol{\mathfrak{t}}\in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in (D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})^{-1} B_{{\Bbb R}^d}(0,C(\delta)e^{nh(\delta)}r) \}\\ &\leq \widetilde{C}\cdot\min\bigg\{\frac{C(\delta)^ke^{nkh(\delta)}r^k}{\phi^k(D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})}:\; k=0,1,\ldots,d\bigg\}\\ &\leq \widetilde{C}C(\delta)^de^{ndh(\delta)}\min\bigg\{\frac{r^k}{\phi^k(D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})}:\; k=0,1,\ldots,d\bigg\}. \end{split} \end{align*} $$

Since $y\in S$ is arbitrary and $\Pi ^{\boldsymbol {\mathfrak {s}}}(\Sigma )\subset S$ , recalling

$$ \begin{align*} Z_{{\boldsymbol{\omega}}}^{\boldsymbol{\mathfrak{s}}}(r)= \inf_{x\in \Sigma} \min\bigg \{ \frac{r^k}{ \phi^k (D_{\Pi^{\boldsymbol{\mathfrak{s}}} x}f^{\boldsymbol{\mathfrak{s}}}_{{\boldsymbol{\omega}}} ) }:\; k=0, 1,\ldots, d\bigg\}, \end{align*} $$

it follows that

$$ \begin{align*}\mathcal L_{\ell d}\{\boldsymbol{\mathfrak{t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{j})|< r\} \leq \widetilde{C}C(\delta)^de^{ndh(\delta)}Z_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}}(r). \end{align*} $$

This completes the proof of the theorem by letting $c_{\delta }=\widetilde {C}C(\delta )^d$ and $\psi (\delta )=dh(\delta )$ .

In what follows we prove Lemma 4.7. To this end, we first prove an elementary geometric lemma.

Lemma 4.8. Let A be a real invertible $d\times d$ matrix. Then for $r_1,r_2>0$ ,

$$ \begin{align*}\mathcal L_{d}((A^{-1}B_{{\Bbb R}^d}(0,r_1))\cap B_{{\Bbb R}^d}(0,r_2))\leq 2^d \min\bigg\{ \frac{r_1^kr_2^{d-k}}{\phi^k(A)}:\; k=0,1,\ldots, d\bigg\}, \end{align*} $$

where $\phi ^s(\cdot )$ is the singular value function defined as in (2.5).

Proof Let $\alpha _1\geq \cdots \geq \alpha _d$ be the singular values of A. Clearly the set

$$ \begin{align*} (A^{-1}B_{{\Bbb R}^d}(0,r_1))\cap B_{{\Bbb R}^d}(0,r_2) \end{align*} $$

is contained in a rectangular parallelepiped with sides $2\min \{r_1/\alpha _i, r_2\}$ , $i=1,\ldots , d$ . It follows that

$$ \begin{align*} \mathcal L_d((A^{-1}B_{{\Bbb R}^d}(0,r_1))\cap B_{{\Bbb R}^d}(0,r_2))&\leq 2^d\prod_{i=1}^d\min\bigg\{\frac{r_1}{\alpha_i},\; r_2\bigg\}\\ &= 2^d \min\bigg\{\frac{r_1^kr_2^{d-k}}{\alpha_1\ldots \alpha_k}:\; k=0,1,\ldots, d\bigg\}\\ &= 2^d \min\bigg\{\frac{r_1^kr_2^{d-k}}{\phi^k(A)}:\; k=0,1,\ldots, d\bigg\}. \\[-42pt] \end{align*} $$

Proof of Lemma 4.7 Let $\mathbf {a}=(a_n)_{n=1}^{\infty },\mathbf {b}=(b_n)_{n=1}^{\infty }\in \Sigma $ with $a_1\neq b_1$ . Without loss of generality, we assume that

(4.23) $$ \begin{align} a_1=1 \quad \text{and} \quad b_1=2. \end{align} $$

Define $g:\Delta \to {\Bbb R}^d$ by

$$ \begin{align*}g(\boldsymbol{\mathfrak{t}})=\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b}). \end{align*} $$

Recall that we have used the notation $ \boldsymbol {\mathfrak {t}} =(\mathbf {t}_1 , \ldots , \mathbf {t}_{\ell } )\in \Delta \subset \mathbb {R}^{\ell d }$ with

$$ \begin{align*}\mathbf{t}_k=(t_{k,1},\ldots, t_{k,d})\in\mathbb{R}^d \quad \text{for all } 1\leq k\leq \ell. \end{align*} $$

For $\boldsymbol {\mathfrak {t}} =(\mathbf {t}_1, \ldots , \mathbf {t}_{\ell } )\in \Delta $ and $k\in \{1,\ldots , \ell \}$ , let $({\partial g}/{\partial \mathbf {t} _k})(\boldsymbol {\mathfrak {t}} )$ denote the Jacobian matrix of the following map from ${\Bbb R}^d$ to ${\Bbb R}^d$ :

$$ \begin{align*} (t_{k,1},\ldots, t_{k, d})\mapsto g(\mathbf{t}_1,\ldots,\mathbf{t}_{k-1}, t_{k,1}, \ldots, t_{k,d}, \mathbf{t}_{k+1}, \ldots,\mathbf{t}_{\ell }). \end{align*} $$

Write $\mathbf {I}=\mathbf {I}_{d}:=\mathrm {diag}(\underbrace {1,\ldots ,1}_{d})$ . First observe that for every $n\in {\Bbb N}$ and ${\mathbf {i}=(i_k)_{k=1}^{\infty }\in \Sigma }$ ,

(4.24) $$ \begin{align} \Pi^{\boldsymbol{\mathfrak{t}} }(\mathbf{i})= \mathbf{t}_{i_1}+f_{i_1} (\mathbf{t}_{i_2}+f_{i_2} ( \mathbf{t}_{i_3}+f_{i_3} ( \ldots f_{i_{n-1}}(\mathbf{t}_{i_n}+f_{i_n}(\Pi^{\boldsymbol{\mathfrak{t}} }\sigma^n\mathbf{i})\ldots )))). \end{align} $$

It follows that for $k\in \{1,\ldots , \ell \}$ ,

(4.25) $$ \begin{align} \frac{\partial\Pi^{\boldsymbol{\mathfrak{t}}} (\mathbf{a})}{\partial\mathbf{t}_{k}} &= \delta_{k, a_1} \cdot \mathbf{I}+(D_{\Pi^{\boldsymbol{\mathfrak{t}}}(\sigma\mathbf{a})}f_{a_1}^{\boldsymbol{\mathfrak{t}}}) \times [\mathbf{I}\cdot\delta_{k, a_2}\nonumber\\ &\quad+(D_{\Pi^{\boldsymbol{\mathfrak{t}}} (\sigma^2\mathbf{a})} f_{a_2}^{\boldsymbol{\mathfrak{t}}})[\mathbf{I}\cdot\delta_{k, a_3}+ (D_{\Pi^{\boldsymbol{\mathfrak{t}}}(\sigma^3\mathbf{a})}f_{a_3}^{\boldsymbol{\mathfrak{t}}}) [\mathbf{I}\cdot\delta_{k, a_4}+\cdots] ]] \nonumber\\ &= \delta_{k, a_1} \cdot \mathbf{I}+ \sum\limits_{n \geq 1 \atop a_{n+1}=k}\ \prod_{k=1}^{n}D_{\Pi^{\boldsymbol{\mathfrak{t}} }(\sigma^k\mathbf{a})}f_{a_k}, \end{align} $$

where $\delta _{i,j}=1$ if $i=j$ and $0$ otherwise.

By (4.25) and the assumption (4.23), we see that for $k\in \{1,\ldots , \ell \}$ ,

(4.26) $$ \begin{align} \frac{\partial g}{{\partial\mathbf{t}_{k}}}(\boldsymbol{\mathfrak{t}} )\!&=\! \frac{\partial \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})}{\partial\boldsymbol{\mathfrak{t}} _{k}} - \frac{\partial \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})}{\partial\boldsymbol{\mathfrak{t}} _{k}}= \delta_{k, 1} \cdot \mathbf{I}-\delta_{k, 2} \cdot \mathbf{I} + E_{k}(\boldsymbol{\mathfrak{t}} ) , \end{align} $$

where

(4.27) $$ \begin{align} E_{k}(\boldsymbol{\mathfrak{t}} ) = \sum\limits_{n \geq 1 \atop a_{n+1}=k}\ \prod_{i=1}^{n}D_{\Pi^{\boldsymbol{\mathfrak{t}} }(\sigma^i\mathbf{a})}f_{a_i} - \sum\limits_{n \geq 1 \atop b_{n+1}=k}\ \prod_{i=1}^{n}D_{\Pi^{\boldsymbol{\mathfrak{t}} }(\sigma^i\mathbf{b})}f_{b_i}. \end{align} $$

Recall that $\rho =\max \nolimits _{i\neq j}(\rho _i+\rho _j)<1$ with $\rho _i:=\max \nolimits _{z\in S}\|D_zf_i\|$ .

Lemma 4.9. There exists $k^*=k^*(\mathbf {a},\mathbf {b})\in \{1,2\}$ such that $\|E_{k^*}(\boldsymbol {\mathfrak {t}} )\| < \rho $ for all $\boldsymbol {\mathfrak {t}} \in \Delta $ .

Proof Our argument is based on an idea of Boris Solomyak, which was used to prove a corresponding statement for self-affine IFSs [Reference Bárány, Simon and Solomyak3, Theorem 9.1.2].

By (4.27), for each $k\in \{1,2\}$ and $\boldsymbol {\mathfrak {t}} \in \Delta $ ,

(4.28)

Clearly, $\unicode{x3bb} _k$ ( $k=1,2$ ) only depend on $\mathbf {a}$ and $\mathbf {b}$ .

Notice that

(4.29)

This implies that one of $\unicode{x3bb} _1,\unicode{x3bb} _2$ is smaller than $\rho $ ; otherwise, since $\rho _1+\rho _2\leq \rho <1$ , it follows that

which contradicts (4.29). Now set

Then $\unicode{x3bb} _{k^*}<\rho $ . Since $\unicode{x3bb} _1, \unicode{x3bb} _2$ only depend on $\mathbf {a}$ and $\mathbf {b}$ , so does $k^*$ . By (4.28),

for all $\boldsymbol {\mathfrak {t}}\in \Delta $ .

In what follows, we always let $k^*=k^*(\mathbf {a}, \mathbf {b})\in \{1,2\}$ be given as in Lemma 4.9.

Lemma 4.10. For all $\boldsymbol {\mathfrak {t}} \in \Delta $ ,

(4.30) $$ \begin{align} \bigg\|\bigg( \frac{\partial g}{{\partial\mathbf{t}_{k^* }}}(\boldsymbol{\mathfrak{t}} )\bigg)^{-1} \bigg\| < \frac{1}{1-\rho}. \end{align} $$

Proof Without loss of generality, we assume that $k^*=1$ . The proof is similar in the case when $k^*=2$ .

Let $\boldsymbol {\mathfrak {t}} \in \Delta $ . By Lemma 4.9, $\|E_1(\boldsymbol {\mathfrak {t}} )\|< \rho <1$ . Thanks to (4.26),

(4.31) $$ \begin{align} \frac{\partial g}{{\partial\mathbf{t}_{1 }}}(\boldsymbol{\mathfrak{t}} ) = \mathbf{I}-(-E_1(\boldsymbol{\mathfrak{t}} )), \end{align} $$

where $\mathbf {I}=\mathrm {diag}(\underbrace {1,\ldots ,1}_d)$ . Since $\|E_1(\boldsymbol {\mathfrak {t}} )\|< \rho <1$ , we see that ${\partial g}/{{\partial \mathbf {t}_{1 }}}(\boldsymbol {\mathfrak {t}} )$ is invertible with

$$ \begin{align*}\bigg(\frac{\partial g}{{\partial\mathbf{t}_{1 }}}(\boldsymbol{\mathfrak{t}})\bigg )^{-1}=\mathbf{I}+ \sum_{n=1}^{\infty} (-E_1(\boldsymbol{\mathfrak{t}} ))^n, \end{align*} $$

from which we obtain that

(4.32) $$ \begin{align} \bigg\|\bigg( \frac{\partial g}{{\partial\mathbf{t}_{1 }}}(\boldsymbol{\mathfrak{t}} )\bigg)^{-1} \bigg\|\leq 1+\sum_{n=1}^{\infty} \|E_1(\boldsymbol{\mathfrak{t}} )\|^n\leq 1+\sum_{n=1}^{\infty} \rho^n=\frac{1}{1-\rho}. \end{align} $$

Next we introduce two mappings $T_1, T_2: \Delta \to \mathbb {R}^{\ell d}$ by

(4.33) $$ \begin{align} T_{1}(\boldsymbol{\mathfrak{t}})= ( g(\boldsymbol{\mathfrak{t}}), \mathbf{t}_{2}, \ldots, \mathbf{t}_{\ell }), \quad T_{2}(\boldsymbol{\mathfrak{t}})= (\mathbf{t}_1, g(\boldsymbol{\mathfrak{t}}), \mathbf{t}_{3}, \ldots, \mathbf{t}_{\ell }), \end{align} $$

where $\boldsymbol {\mathfrak {t}}=(\mathbf {t}_{1},\ldots , \mathbf {t}_{\ell })$ . Recall that $g(\boldsymbol {\mathfrak {t}})=\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {a})-\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {b})$ .

Lemma 4.11. Let $k^*=k^*(\mathbf {a}, \mathbf {b})\in \{1,2\}$ be given as in Lemma 4.9. Then the following properties hold.

  1. (i) The mapping $T_{k^*}:\;\Delta \to {\Bbb R}^{\ell d}$ is injective.

  2. (ii) For each $\boldsymbol {\mathfrak {t}}\in \Delta $ ,

    (4.34) $$ \begin{align} |\!\det(( D_{\boldsymbol{\mathfrak{t}}}T_{k^*})^{-1}) |<\bigg(\frac{1}{1-\rho}\bigg)^d. \end{align} $$

Proof Without loss of generality, we may assume that $k^*=1$ . Then by Lemma 4.9 and (4.33),

(4.35) $$ \begin{align} \|E_1(\boldsymbol{\mathfrak{t}})\|<\rho, \quad T_1(\boldsymbol{\mathfrak{t}})=( g(\boldsymbol{\mathfrak{t}}), \mathbf{t}_{2}, \ldots, \mathbf{t}_{\ell }) \end{align} $$

for $\boldsymbol {\mathfrak {t}}=(\mathbf {t}_{1}, \ldots , \mathbf {t}_{\ell })\in \Delta $ . Hence to prove (i), it suffices to show that for given $\mathbf {t}_{2}, \ldots , \mathbf {t}_{\ell }\in {\Bbb R}^d$ with $\sum _{i=2}^{\ell } |\mathbf {t}_{2}|^2<r_0^2$ , the mapping

$$ \begin{align*}\mathbf{t}_1\mapsto g(\mathbf{t}_{1}, \mathbf{t}_{2}, \ldots, \mathbf{t}_{\ell }) \end{align*} $$

is injective on $\Delta _1:=\{\mathbf {t}_1\in {\Bbb R}^d:\; |\mathbf {t}_1|<\sqrt {r_0^2-\sum _{i=2}^{\ell } |\mathbf {t}_{i}|^2}\}$ . To this end, define $\psi :\; \Delta _1\to {\Bbb R}^d$ by

$$ \begin{align*}\psi(\mathbf{t}_1)=g(\mathbf{t}_{1}, \ldots, \mathbf{t}_{\ell })-\mathbf{t}_1. \end{align*} $$

Then by (4.31) and (4.35),

$$ \begin{align*}\|D_{\mathbf{t}_1}\psi\|=\bigg\|\frac{\partial g}{\partial \mathbf{t}_1}(\mathbf{t}_{1}, \ldots, \mathbf{t}_{\ell })-\mathbf{I}\bigg\|=\|E_1(\mathbf{t}_{1}, \ldots, \mathbf{t}_{\ell })\|<\rho \quad \text{for each } \mathbf{t}_{1}\in \Delta_1. \end{align*} $$

Since $\Delta _1$ is a convex open subset of ${\Bbb R}^d$ , by [Reference Rudin42, Theorem 9.19], the above inequality implies that

$$ \begin{align*}|\psi(\mathbf{t}_1)-\psi(\mathbf{s}_1)|\leq \rho |\mathbf{t}_1-\mathbf{s_1}|<|\mathbf{t}_1-\mathbf{s_1}| \end{align*} $$

for all distinct $\mathbf {t}_1, \mathbf {s_1}\in \Delta _1$ . It follows that for distinct $\mathbf {t}_1, \mathbf {s_1}\in \Delta _1$ ,

$$ \begin{align*} |g(\mathbf{t}_1)-g(\mathbf{s}_1)|&=|\psi(\mathbf{t}_1)+\mathbf{t}_1-\psi(\mathbf{s}_1)-\mathbf{s}_1|\\ &\geq |\mathbf{t}_1-\mathbf{s}_1|-|\psi(\mathbf{t}_1)-\psi(\mathbf{s}_1)|\\ &> 0. \end{align*} $$

This proves (i).

To prove (ii), notice that

$$ \begin{align*} D_{\boldsymbol{\mathfrak{t}}}T_{1}=\left(\begin{array}{c|cccc} \displaystyle\frac{\partial{g}}{\partial{\mathbf{t}_1}}(\boldsymbol{\mathfrak{t}}) & \displaystyle\frac{\partial{g}}{\partial{\mathbf{t}_2}}(\boldsymbol{\mathfrak{t}}) & \displaystyle\frac{\partial{g}}{\partial{\mathbf{t}_3}}(\boldsymbol{\mathfrak{t}}) & \cdots & \displaystyle\frac{\partial{g}}{\partial{\mathbf{t}_{\ell }}}(\boldsymbol{\mathfrak{t}}) \\\hline & & & & \\ \mathbf{0}_{(\ell -1)d,d} & & & \mathbf{I}_{(\ell -1)d} & \\ & & & & \end{array}\right),\end{align*} $$

where $\mathbf {I}_{(\ell -1)d}:=\mathrm {diag}(\underbrace {1, \ldots , 1}_{(\ell -1)d})$ and $\mathbf {0}_{(\ell -1)d,d}$ is the $((\ell -1)d)\times d$ all-zero matrix. That is,

$$ \begin{align*} D_{\boldsymbol{\mathfrak{t}}}T_{1}=\left(\begin{array}{@{}c|c@{}}A(\boldsymbol{\mathfrak{t}})& B(\boldsymbol{\mathfrak{t}})\\ \hline \mathbf{0}_{(\ell-1)d, d}&\mathbf{I}_{(\ell-1)d}\end{array}\right), \end{align*} $$

where $A(\boldsymbol {\mathfrak {t}})$ and $B(\boldsymbol {\mathfrak {t}})$ are given by

$$ \begin{align*} A(\boldsymbol{\mathfrak{t}})= \frac{\partial{g}}{\partial{\mathbf{t}_1}} (\boldsymbol{\mathfrak{t}} ), \quad B(\boldsymbol{\mathfrak{t}})= \bigg(\frac{\partial{g}}{\partial{\mathbf{t}_2}}(\boldsymbol{\mathfrak{t}}), \ldots, \frac{\partial{g}}{\partial{\mathbf{t}_{\ell }}}(\boldsymbol{\mathfrak{t}})\bigg). \end{align*} $$

Hence, by Lemma 4.10, $A^{-1}(\boldsymbol {\mathfrak {t}} )$ exists and

$$ \begin{align*} (D_{\boldsymbol{\mathfrak{t}}}T_{1})^{-1}=\left(\begin{array}{@{}c|c@{}}A^{-1}(\boldsymbol{\mathfrak{t}})&-A^{-1}(\boldsymbol{\mathfrak{t}})\cdot B(\boldsymbol{\mathfrak{t}})\\ \hline \mathbf{0}_{(\ell-1)d,d)} &\mathbf{I}_{(\ell-1)d}\end{array}\right). \end{align*} $$

It follows that

$$ \begin{align*} \det((D_{\boldsymbol{\mathfrak{t}}}T_{1})^{-1})= \det(A^{-1}(\boldsymbol{\mathfrak{t}})) =\det\bigg(\bigg(\frac{\partial g}{\partial\mathbf{t}_1}(\boldsymbol{\mathfrak{t}})\bigg)^{-1}\bigg). \end{align*} $$

By the Hadamard’s inequality (see e.g. [Reference Horn and Johnson28, Corollary 7.8.2]),

$$ \begin{align*} |\!\det((D_{\boldsymbol{\mathfrak{t}}}T_{1})^{-1})|= \bigg|\!\det\bigg( \bigg(\frac{\partial g}{{\partial\mathbf{t}_{1}}}(\boldsymbol{\mathfrak{t}} )\bigg)^{-1}\bigg)\bigg| \leq \bigg\|\bigg(\frac{\partial g}{{\partial\mathbf{t}_{1}}}(\boldsymbol{\mathfrak{t}} )\bigg)^{-1}\bigg\|^{d} \leq \bigg(\frac{1}{1-\rho}\bigg)^{d}, \end{align*} $$

where the last inequality follows from Lemma 4.10. This completes the proof of (ii).

To shorten the notation, from now on we write

(4.36) $$ \begin{align} C_{*}:=\bigg(\frac{1}{1-\rho}\bigg)^{d}. \end{align} $$

Let $\boldsymbol {\mathfrak {s}}=(\mathbf {s}_1,\ldots , \mathbf {s}_{\ell })\in \Delta $ and $\delta , r>0$ . Let A be a given real invertible $d\times d$ matrix.

Write

$$ \begin{align*} E:&=\{\boldsymbol{\mathfrak{t}}\in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}}, \delta)\cap \Delta:\; \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in A^{-1}B_{{\Bbb R}^d}(0,r)\} \\ &= \{\boldsymbol{\mathfrak{t}}\in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}}, \delta)\cap \Delta:\; g(\boldsymbol{\mathfrak{t}})\in A^{-1}B_{{\Bbb R}^d}(0,r)\}. \end{align*} $$

Below, we estimate $\mathcal L_{\ell d}(E)$ .

Notice that $\mathcal L_{\ell d}(E)=\mathcal L_{\ell d}(T_{k^*}^{-1}(T_{k^*}(E)))$ . Recall that by Lemma 4.11, the mapping $T_{k^*}: \Delta \to {\Bbb R}^{\ell d}$ is injective and $\det ((D_{\boldsymbol {\mathfrak {t}}}T_{k^*})^{-1})\leq C_*$ for $\boldsymbol {\mathfrak {t}}\in \Delta $ . So by the substitution rule of multiple integration (see e.g. [Reference Rudin42, Theorem 10.9]),

(4.37) $$ \begin{align} \mathcal L_{\ell d}(E)\leq C_*\mathcal L_{\ell d}(T_{k^*}(E)). \end{align} $$

Next we estimate $\mathcal L_{\ell d}(T_{k^*}(E))$ . Without loss of generality, we may assume that $k^*=1$ . Notice that for each $\boldsymbol {\mathfrak {t}}\in E$ ,

$$ \begin{align*}g(\boldsymbol{\mathfrak{t}})\in A^{-1}B_{{\Bbb R}^d}(0,r);\end{align*} $$

in the meantime, since $\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {a}),\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {b})\in S$ , it follows that

$$ \begin{align*}g(\boldsymbol{\mathfrak{t}})=\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in B_{{\Bbb R}^d}(0, 2\mathrm{diam}(S)).\end{align*} $$

Hence, for each $\boldsymbol {\mathfrak {t}}\in E$ ,

$$ \begin{align*}g(\boldsymbol{\mathfrak{t}})\in (A^{-1}B_{{\Bbb R}^d}(0,r))\cap B_{{\Bbb R}^d}(0, 2\mathrm{diam}(S)). \end{align*} $$

Since $T_1(\boldsymbol {\mathfrak {t}})=(g(\boldsymbol {\mathfrak {t}}), \mathbf {t_2},\ldots , \mathbf {t}_{\ell })$ , it follows that

$$ \begin{align*}T_{1}(E)\subset F_1\times F_2, \end{align*} $$

where

$$ \begin{align*} F_1:=&(A^{-1}B_{{\Bbb R}^d}(0,r))\cap B_{{\Bbb R}^d}(0, 2\mathrm{diam}(S)),\\ F_2:=&\{(\mathbf{t}_2,\ldots, \mathbf{t}_{\ell})\in {\Bbb R}^{(\ell-1)d}:\; |\mathbf{t}_i-\mathbf{s}_i|<\delta\}. \end{align*} $$

Consequently,

$$ \begin{align*} \mathcal L_{\ell d}(T_{1}(E))&\leq \mathcal L_{d}(F_1)\cdot \mathcal L_{(\ell-1)d}(F_2)\\ &\leq 2^d\min\bigg\{ \frac{r^k (2\mathrm{diam}(S))^{d-k}}{\phi^k(A)}:\; k=0,1,\ldots,d \bigg\}\cdot (2\delta)^{(\ell-1)d}\\ &\leq u \min\bigg\{ \frac{r^k }{\phi^k(A)}:\; k=0,1,\ldots,d \bigg\} \end{align*} $$

with $u:=2^{\ell d}\delta ^{(\ell -1)d}\max \{1, 2^d\mathrm {diam}(S)^d\}$ , where we have used Lemma 4.8 in the second inequality. Combining this with (4.37) yields that

$$ \begin{align*}\mathcal L_{\ell d}(E)\leq C_* \mathcal L_{\ell d}(T_1(E))\leq uC_* \min\bigg\{ \frac{r^k }{\phi^k(A)}:\; k=0,1,\ldots,d \bigg\}. \end{align*} $$

This completes the proof of Lemma 4.7.

5 Translational family of IFSs generated by a $C^1$ conformal IFS

In this section, we prove the following result.

Theorem 5.1. Let $\mathcal F=\{f_i:\; S\to S\}_{i=1}^{\ell }$ be an IFS on a compact set $S\subset {\Bbb R}^d$ . Suppose that the following properties hold.

  1. (i) The set S is connected, $S=\overline {\mathrm {int}(S)}$ and $f_i(S)\subset \mathrm {int}(S)$ for all i.

  2. (ii) There is a bounded connected open set $U\supset S$ such that each $f_i$ extends to a $C^1$ conformal diffeomorphism $f_i:\; U\to f_i(U)\subset U$ with

    $$ \begin{align*} \rho_i:=\sup_{x\in U}\|f_i'(x)\|<1. \end{align*} $$
  3. (iii) $\max _{i\neq j} \rho _i+\rho _j<1$ .

Then there is a small $r_0>0$ such that the translational family ${\mathcal F}^{\boldsymbol {\mathfrak {t}}}=\{f_i^{\boldsymbol {\mathfrak {t}}}=f_i+\mathbf {t}_i\}_{i=1}^{\ell }$ , $\boldsymbol {\mathfrak {t}}=(\mathbf {t}_1,\ldots , \mathbf {t}_{\ell })\in \Delta :=\{\boldsymbol {\mathfrak {s}}\in {\Bbb R}^{\ell d}:\; |\boldsymbol {\mathfrak {s}}|<r_0\}$ , satisfies the GTC with respect to the Lebesgue measure $\mathcal L_{\ell d}$ on $\Delta $ .

Proof By the assumptions (i) and (ii), we may pick two open connected sets V and W (for instance, we may let V and W be the $\epsilon $ -neighborhood and $2\epsilon $ -neighborhood of S, respectively, for a sufficiently small $\epsilon>0$ ), such that

$$ \begin{align*} S\subset V\subset \overline{V}\subset W\subset \overline {W}\subset U, \text{ and} \end{align*} $$
$$ \begin{align*} f_i(\overline{V})\subset V \text{ and } f_i(\overline{W})\subset W \quad \text{for all } i. \end{align*} $$

Then by continuity, we can pick a small $r_0$ such that for all $\boldsymbol {\mathfrak {t}}=(\mathbf {t}_1,\ldots , \mathbf {t}_{\ell })\in {\Bbb R}^{\ell d}$ with $|\boldsymbol {\mathfrak {t}}|<r_0$ ,

$$ \begin{align*}f_i^{\boldsymbol{\mathfrak{t}}}(\overline{V})\subset V \text{ and } f_i^{\boldsymbol{\mathfrak{t}}}(\overline{W})\subset W \quad \text{for all } i, \end{align*} $$

where $f_i^{\boldsymbol {\mathfrak {t}}}:=f_i+\mathbf {t}_i$ . Fix this $r_0$ and set $\Delta =\{\boldsymbol {\mathfrak {s}}\in {\Bbb R}^{\ell d}:\; |\boldsymbol {\mathfrak {s}}|<r_0\}$ . In what follows, we prove that the family ${\mathcal F}^{\boldsymbol {\mathfrak {t}}}$ , $\boldsymbol {\mathfrak {t}}\in \Delta $ , satisfies the GTC with respect to $\mathcal L_{\ell d}$ on $\Delta $ .

For $i=1,\ldots , \ell $ , define $g_i: \overline {W}\to {\Bbb R}$ by

$$ \begin{align*}g_i(z)=\log \|f_i'(z)\|.\end{align*} $$

Then $g_i$ is continuous on $\overline {W}$ for each i. Define $\gamma :\; (0,\infty )\to (0,\infty )$ by

$$ \begin{align*}\gamma(u)=\max_{1\leq i\leq \ell} \sup\{|g_i(x)-g_i(y)|:\; x,y\in \overline{W},\; |x-y|\leq u\}. \end{align*} $$

That is, $\gamma $ is a common continuity modulus of $g_1,\ldots , g_{\ell }$ . Clearly $\lim _{u\to 0}\gamma (u)=0$ . Notice that for $\boldsymbol {\mathfrak {t}}\in \Delta $ , $y\in W$ and $\boldsymbol {\omega }\in \Sigma _n$ ,

$$ \begin{align*}\log \|(f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )'(y)\|=\sum_{k=1}^n g_{\omega_k}(f^{\boldsymbol{\mathfrak{t}}}_{\sigma^k{\boldsymbol{\omega}}}(y)). \end{align*} $$

Using similar arguments (with minor changes) as in Step 1 and Step 2 of the proof of Proposition 4.3, we can show that the following two properties hold.

  1. (a) Write for $n\in {\Bbb N}$ ,

    (5.1) $$ \begin{align} C_n:=\sup\bigg\{ \frac{\|(f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )'(y)\|}{\|(f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )'(z)\|}:\; \boldsymbol{\mathfrak{t}}\in \Delta,\; y,z\in W, \;{\boldsymbol{\omega}}\in \Sigma_n\bigg\}. \end{align} $$
    Then $\lim _{n\to \infty }({1}/{n})\log C_n=0$ .
  2. (b) For $y\in W$ , $\boldsymbol {\mathfrak {s}},\boldsymbol {\mathfrak {t}}\in \Delta $ , $n\in {\Bbb N}$ and ${\boldsymbol {\omega }}\in \Sigma _n$ ,

    (5.2) $$ \begin{align} \frac{\|(f^{\boldsymbol{\mathfrak{t}}}_{{\boldsymbol{\omega}}} )'(y)\|}{\|(f^{\boldsymbol{\mathfrak{s}}}_{{\boldsymbol{\omega}}} )'(y)\|}\leq \exp\bigg(n\gamma\bigg(\frac{|\boldsymbol{\mathfrak{t}}-\boldsymbol{\mathfrak{s}}|}{1-\theta}\bigg)\bigg), \end{align} $$
    where $\theta :=\max _{1\leq i\leq \ell }\rho _i<1$ .

Let $\mathcal H$ denote the collection of $C^1$ injective conformal mappings $h: W\to W$ such that $h(\overline {V})\subset V$ . The following fact is known (for a proof, see e.g. part 3 of the proof of [Reference Patzschke39, Lemma 2.2]): there exists a constant $D\in (0,1)$ depending on V and W, such that

(5.3) $$ \begin{align} D\cdot \Big(\inf_{z\in W}\| h'(z)\|\Big) \cdot |x-y|\leq |h(x)-h(y)| \quad \text{for all }h\in \mathcal H,\; x,y\in V. \end{align} $$

Now fix $\boldsymbol {\mathfrak {s}}\in \Delta $ and $\delta \in (0,r_0)$ . Let $\mathbf {i},\mathbf {j}\in \Sigma $ with $\mathbf {i}\neq \mathbf {j}$ . Set

$$ \begin{align*}\boldsymbol{\omega}=\mathbf{i}\wedge \mathbf{j}\quad \text{and}\quad n=|\boldsymbol{\omega}|.\end{align*} $$

Write $\mathbf {a}=\sigma ^n \mathbf {i}$ and $\mathbf {b}=\sigma ^n \mathbf {j}$ . Clearly $a_1\neq b_1$ . Fix $y\in S$ . We claim that for $r>0$ ,

(5.4) $$ \begin{align} &\{\boldsymbol{\mathfrak{t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\! |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{j})|< r\}\nonumber\\ &\text{}\; \subset \{\boldsymbol{\mathfrak{t}}\in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\! \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in (D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})^{-1} B_{{\Bbb R}^d}(0,c(n,\delta)r) \}, \end{align} $$

where

$$ \begin{align*}c(n,\delta):=D^{-1}C_n \exp\bigg(n\gamma\bigg(\frac{\delta}{1-\theta}\bigg)\bigg)>1, \end{align*} $$

in which D is the constant from (5.3).

To show (5.4), let $\boldsymbol {\mathfrak {t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol {\mathfrak {s}},\delta )\cap \Delta $ so that $|\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {i})-\Pi ^{\boldsymbol {\mathfrak {t}}}(\mathbf {j})|<r$ . Notice that

$$ \begin{align*} \begin{split} |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ j})|&=|f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}}(\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ a}))-f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}}(\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b}))|\\ &\geq D\cdot \Big(\inf_{z\in W}\| (f^{\boldsymbol{\mathfrak{t}}}_{\boldsymbol{\omega}})'(z)\|\Big) \cdot |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{ a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})|\quad \text{(by (5.3))}\\ &\geq D(C_n)^{-1} \exp\bigg(-n\gamma\bigg(\frac{\delta}{1-\theta}\bigg)\bigg)\cdot\| (f^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})'(y)\|\cdot |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})|, \end{split} \end{align*} $$

where, in the last inequality, we have used (5.1) and (5.2). It follows that

$$ \begin{align*}|\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})|\leq \| (f^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})'(y)\|^{-1}\cdot D^{-1}C_n \exp\bigg(n\gamma\bigg(\frac{\delta}{1-\theta}\bigg)\bigg)\cdot r. \end{align*} $$

Since $(f^{\boldsymbol {\mathfrak {s}}}_{\boldsymbol {\omega }})'(y)=D_yf^{\boldsymbol {\mathfrak {s}}}_{\boldsymbol {\omega }}$ is a scalar multiple of an orthogonal matrix, the above inequality implies that

$$ \begin{align*}\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in (D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})^{-1} B_{{\Bbb R}^d}(0,c(n,\delta)r). \end{align*} $$

from which (5.4) follows.

By (5.4) and Lemma 4.7 (which is also valid in this context),

$$ \begin{align*} \begin{split} \mathcal L_{\ell d}&\{\boldsymbol{\mathfrak{t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{j})|< r\}\\ &\leq \mathcal L_{\ell d} \{\boldsymbol{\mathfrak{t}}\in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; \Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{a})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{b})\in (D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})^{-1} B_{{\Bbb R}^d}(0,c(n,\delta)r) \}\\ &\leq \widetilde{C}\cdot\min\bigg\{\frac{c(n,\delta)^k r^k}{\phi^k(D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})}:\; k=0,1\ldots,d\bigg\}\\ &\leq \widetilde{C}c(n,\delta)^d\cdot\min\bigg\{\frac{ r^k}{\phi^k(D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})}:\; k=0,1\ldots,d\bigg\}\\ &= \widetilde{C}D^{-d} (C_n)^d \exp\bigg(nd\gamma\bigg(\frac{\delta}{1-\theta}\bigg)\bigg) \min\bigg\{\frac{r^k}{\phi^k(D_yf^{\boldsymbol{\mathfrak{s}}}_{\boldsymbol{\omega}})}:\; k=0,1\ldots,d\bigg\}. \end{split} \end{align*} $$

Since $y\in S$ is arbitrary and $\Pi ^{\boldsymbol {\mathfrak {s}}}(\Sigma )\subset S$ , recalling

$$ \begin{align*} Z_{{\boldsymbol{\omega}}}^{\boldsymbol{\mathfrak{s}}}(r)= \inf_{x\in \Sigma} \min\bigg \{ \frac{r^k}{ \phi^k (D_{\Pi^{\boldsymbol{\mathfrak{s}}} x}f^{\boldsymbol{\mathfrak{s}}}_{{\boldsymbol{\omega}}} ) }:\; k=0, 1,\ldots, d\bigg\}, \end{align*} $$

it follows that

$$ \begin{align*} \mathcal L_{\ell d}& \{\boldsymbol{\mathfrak{t}} \in B_{{\Bbb R}^{\ell d}}(\boldsymbol{\mathfrak{s}},\delta)\cap \Delta:\; |\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{i})-\Pi^{\boldsymbol{\mathfrak{t}}}(\mathbf{j})|< r\} \\ & \leq \widetilde{C}D^{-d} (C_n)^d \exp\bigg(nd\gamma\bigg(\frac{\delta}{1-\theta}\bigg)\bigg)Z_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}}(r)\\ &\leq c_{\delta} e^{n\psi(\delta)}Z_{\boldsymbol{\omega}}^{\boldsymbol{\mathfrak{s}}}(r), \end{align*} $$

where

$$ \begin{align*}c_{\delta}:= \sup_{n\in {\Bbb N}}\widetilde{C}D^{-d} (C_n)^d e^{-n\delta}<\infty,\quad \psi(\delta):=\delta+d\gamma\bigg(\frac{\delta}{1-\theta}\bigg). \end{align*} $$

Since $\lim _{u\to 0}\gamma (u)=0$ , we see that $\lim _{\delta \to 0} \psi (\delta )=0$ . Thus, $({\mathcal F}^{\boldsymbol {\mathfrak {t}}})_{\boldsymbol {\mathfrak {t}}\in \Delta }$ satisfies the GTC.

6 Direct product of parameterized families of $C^1$ IFSs

In this section, we study the direct product of parameterized families of $C^1$ IFSs (cf. Definition 1.5). The main result is the following, stating that the property of the GTC is preserved under the direct product.

Proposition 6.1. Let $\ell \in {\Bbb N}$ with $\ell \geq 2$ . Suppose that for $k=1,\ldots , n$ , $(\mathcal F_k^{t_k})_{t_k\in {\Omega }_k}$ is a parameterized family of $C^1$ IFSs on $Z_j\subset {\Bbb R}^{q_k}$ , satisfying the GTC with respect to a locally finite Borel measure $\eta _k$ on the metric space $({\Omega }_k, d_{{\Omega }_k})$ . Moreover, suppose all the individual IFSs have $\ell $ contractions. Set

$$ \begin{align*}\mathcal F^{(t_1,\ldots, t_n)}=\mathcal F_1^{t_1}\times\cdots\times \mathcal F_n^{t_n},\quad (t_1,\ldots, t_n)\in {\Omega}_1\times\cdots \times {\Omega}_n. \end{align*} $$

Endow ${\Omega }:={\Omega }_1\times \cdots \times {\Omega }_n$ with the product metric $d_{\Omega }$ as follows:

$$ \begin{align*}d_{\Omega}((t_1,\ldots, t_n), (s_1,\ldots, s_n))=\bigg(\sum_{k=1}^n d_{{\Omega}_k}(s_k, t_k)^2\bigg)^{1/2}. \end{align*} $$

Then the family $\mathcal F^{(t_1,\ldots , t_n)}$ , $(t_1,\ldots , t_n)\in {\Omega }_1\times \cdots \times {\Omega }_n$ , satisfies the GTC with respect to $\eta _1\times \cdots \times \eta _n$ .

To prove the above proposition, we need the following.

Lemma 6.2.

  1. (i) Let A be a real non-singular $d\times d$ matrix with singular values $\alpha _1\geq \cdots \geq \alpha _d$ . Then for each $r>0$ ,

    $$ \begin{align*}\min\bigg\{\frac{r^p}{\phi^p(A)}:\; p=0,1,\ldots,d\bigg\}=\prod_{i=1}^d\frac{\min\{ \alpha_i, r\}}{\alpha_i}, \end{align*} $$
    where $\phi ^s(\cdot )$ is the singular value function defined as in (2.5).
  2. (ii) For $j=1,\ldots , n$ , let $A_j$ be a real non-singular $d_j\times d_j$ matrix. Set

    $$ \begin{align*}M=\mathrm{diag}(A_1,\ldots, A_n):=\left[ \begin{array}{cccc} A_1 & {\textbf{0}} & \cdots & {\textbf{0}}\\ {\textbf{0}} & A_2 & \cdots & {\textbf{0}}\\ \vdots & \vdots &\ddots & {\textbf{0}}\\ {\textbf{0}} & {\textbf{0}} & \cdots & A_n \end{array} \right]. \end{align*} $$
    Then
    (6.1) $$ \begin{align} \min&\bigg\{\frac{r^p}{\phi^p(M)}:\! p=0,1,\ldots,d_1+\cdots+d_n\bigg\}\nonumber\\ &=\prod_{i=1}^n \min\bigg\{\frac{r^p}{\phi^p(A_i)}:\! p=0,1,\ldots,d_i\bigg\}. \end{align} $$

Proof The proof of (i) is direct and simple. We leave it to the reader as an exercise. Part (ii) is just a consequence of (i), using the fact that the set of singular values (including the multiplicity) of M are precisely the union of those of $A_i$ , $i=1,\ldots , n$ .

Now we are ready to prove Proposition 6.1.

Proof of Proposition 6.1 Write

$$ \begin{align*}\mathcal F_k^{t_k}=\{f_{i,k}^{t_k}\}_{i=1}^{\ell},\quad t_k\in {\Omega}_k,\; k=1,\ldots,n.\end{align*} $$

For $\boldsymbol {\omega }=\omega _1\ldots \omega _m\in \Sigma _*$ , write $f_{{\boldsymbol {\omega }},k}^{t_k}=f_{\omega _1,k}^{t_k}\circ \cdots \circ f_{\omega _m,k}^{t_k}$ . Let $\Pi ^{t_k}_k$ denote the coding map associated with the IFS $\mathcal F_k^{t_k}$ , and $\Pi ^{(t_1,\ldots , t_n)}$ the coding map associated with the IFS $\mathcal F^{(t_1,\ldots , t_n)}$ . According to the GTC assumption on the families $(\mathcal F_k^{t_k})_{t_k\in {\Omega }_k}$ , $k=1,\ldots , n$ , there exist $\delta _0>0$ and a function $\psi :\; (0, \delta _0)\to [0,\infty )$ with $\lim _{\delta \to 0}\psi (\delta )=0$ such that for every $\delta \kern1.5pt{\in}\kern1.5pt (0, \delta _0)$ and $(s_1,\ldots , s_n)\kern1.5pt{\in}\kern1.5pt {\Omega }_1\times \cdots \times {\Omega }_n$ , there is $C\kern1.5pt{=}\kern1.5pt C(\delta ,s_1,\ldots , s_n)\kern1.5pt{>}\kern1.5pt 0$ satisfying the following: for each $k\in \{1,\ldots , n\}$ , distinct $\mathbf {i},\mathbf { j}\in \Sigma $ and $r>0$ ,

(6.2) $$ \begin{align} \eta_k&\{t_k\in B_{{\Omega}_k}(s_k, \delta):\! |\Pi^{t_k}_k({\textbf{ i}})-\Pi^{t_k}_k({\textbf{j}}) |< r\}\nonumber\\ &\leq C e^{|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)} \inf_{x\in \Sigma} \min\bigg\{ \frac{r^p}{\phi^p(D_{\Pi^{t_k}_kx}f_{\mathbf{i}\wedge \mathbf{j}, k}^{t_k})}:\! p=0,1,\ldots, q_k \bigg\}, \end{align} $$

where $B_{{\Omega }_k}(s_k, \delta )$ stands for the closed ball in ${\Omega }_k$ of radius $\delta $ centered at $s_k$ . Writing $\mathbf {t}=(t_1,\ldots , t_n)$ , $\mathbf {s}=(s_1,\ldots , s_n)$ and using (6.2),

$$ \begin{align*} \eta_1&\times \cdots\times \eta_n\{ \mathbf{t}\in B_{{\Omega}}(\mathbf{s}, \delta): \; |\Pi^{\mathbf{t}}({\textbf{i}})-\Pi^{\mathbf{t}}({\textbf{j}}) |< r\}\\ &\leq \prod_{k=1}^n\eta_k\{t_k\in B_{{\Omega}_k}(s_k, \delta): \; |\Pi^{t_k}_k({\textbf{ i}})-\Pi^{t_k}_k({\textbf{j}}) |< r\}\\ &\leq \prod_{k=1}^n \bigg(C e^{|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)} \inf_{x\in \Sigma} \min\bigg\{ \frac{r^p}{\phi^p(D_{\Pi^{s_k}_kx}f_{\mathbf{i}\wedge \mathbf{j}, k}^{s_k})}:\; p=0,1,\ldots, q_k \bigg\}\bigg)\\ & \leq C^n e^{n|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)}\inf_{x\in \Sigma}\prod_{k=1}^n \min\bigg\{ \frac{r^p}{\phi^p(D_{\Pi^{s_k}_kx}f_{\mathbf{i}\wedge \mathbf{j}, k}^{s_k})}:\; p=0,1,\ldots, q_k \bigg\}\\ & =C^n e^{n|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)}\inf_{x\in \Sigma}\min \bigg\{ \frac{r^p}{\phi^p(D_{\Pi^{\mathbf{t}}x}f_{\mathbf{i}\wedge \mathbf{j}}^{\mathbf{s}})}:\; p=0,1,\ldots, q_1+\cdots+q_n \bigg\}\\ & =C^n e^{n|{\textbf{i}}\wedge {\textbf{j}}| \psi(\delta)}Z_{\mathbf{i}\wedge\mathbf{j}}^{\mathbf{s}}(r), \end{align*} $$

where we have used (6.1) in the second last equality. Hence, the family $\mathcal F^{\mathbf {t}}$ , $\mathbf {t}\in {\Omega }$ , satisfies the GTC with respect to the measure $\eta _1\times \cdots \times \eta _n$ , where the involved constant and the function in the definition of the GTC are $C^n$ and $n\psi (\cdot )$ , respectively.

7 The proof of Theorem 1.6 and final questions

Now we are ready to prove Theorem 1.6.

Proof of Theorem 1.6 This follows directly by combining Theorems 4.2, 5.1 and Proposition 6.1.

Below we list a few ‘folklore’ open questions on the dimension of the attractors of $C^1$ IFSs. One may formulate the corresponding questions on the dimension of push-forwards of ergodic invariant measures on the attractors.

Question 7.1. Is it true that for every $C^1$ IFS $\mathcal F=\{f_i\}_{i=1}^{\ell }$ on ${\Bbb R}^d$ satisfying (1.8), there is a neighborhood $\Delta $ of ${\textbf {0}}$ in ${\Bbb R}^{\ell d}$ such that for $\mathcal L_{\ell d}$ -a.e. $\boldsymbol {\mathfrak {t}}=({\textbf {t}}_1,\ldots , {\textbf {t}}_{\ell })\in \Delta $ ,

$$ \begin{align*}\dim_HK^{\boldsymbol{\mathfrak{t}}}=\dim_BK^{\boldsymbol{\mathfrak{t}}}=\min\{\dim_S \mathcal F^{\boldsymbol{\mathfrak{t}}}, \; d\}, \end{align*} $$

where $K^{\boldsymbol {\mathfrak {t}}}$ is the attractor of the IFS ${\mathcal F}^{\boldsymbol {\mathfrak {t}}}=\{f_i+{\textbf {t}}_{i}\}_{i=1}^{\ell }$ ?

Question 7.2. Do we have

$$ \begin{align*}\dim_HK=\dim_BK=\min\{\dim_S \mathcal F, \; d\} \end{align*} $$

for the attractor K of a ‘generic’ $C^1$ IFS $\mathcal F$ on ${\Bbb R}^d$ (in an appropriate sense)?

Acknowledgements

The authors would like to thank the referee for helpful comments and suggestions. They also thank Zhou Feng for catching some typos. The research of D.-J.F. was partially supported by a HKRGC GRF grant and the Direct Grant for Research in CUHK. The research of K.S. was partially supported by the grant OTKA K104745. A significant part of the research was done during the visit of K.S. to CUHK, which was supported by a HKRGC GRF grant.

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