Abstract
In this paper, we apply the max metric \(d_{n, q}\) and the mean metric \({\overline{d}}_{n, q}\) to the definitions of measure-theoretic pressure and topological pressure. In fact, we generalize Katok’s entropy formula to measure-theoretic pressure by the mean metric.
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1 Introductions
Entropy is one of the measurements of the complexity of dynamical systems. Measure-theoretic entropy and topological entropy are important determinants of complexity in dynamical system. The relationship between these two quantities is the well-known variational principle. In 1958, Kolmogorov firstly introduced the measure-theoretic entropy of a measure-preserving dynamical system as an isomorphic invariant [11, 12]. Later Adler et al. introduced the topological entropy of a topological dynamical system by open covers as a conjugate invariant [1]. Equivalent definitions based on separated and spanning set were independently given by Bowen [2] and Dinaburg [5].
Topological pressure is a generalization of topological entropy. The theories of topological pressure, varitional principle and equilibrium states play a prominent role in statistical mechanics, ergodic theory and dynamical systems [10, 14]. Since the works of Bowen [3] and Ruelle [16], the topological pressure turned into a basic tool of the dimension theory in dynamical systems.
In the investigation of the Sarnak’s conjecture, Huang, Wang and Ye [7] introduced the measure complexity of an invariant measure \(\mu \) similar to the one introduced by Katok [13], by using the mean metric instead of the Bowen metric (for discussion and results related to mean metric, see also [18]). In 2015, by using separated sets, Gröger and Jäger [9] gave a definition of topological entropy of the whole system in mean metrics, and proved that the topological entropy defined by mean metrics is equivalent to the classical topological entropy. Huang et al. [7] introduced the notion of measure complexity for a topological dynamical system. Then, they [8] established Katok’s entropy formula for ergodic measures in the case of mean metrics. In fact, this formula [8] showed that one can replace the Bowen metrics with the mean metrics when studying the measure complexity for a topological dynamical system. In this paper, inspired by Huang et al. [8], we apply two metrics: the max metric \(d_{n, q}\) and the mean metric \({\overline{d}}_{n, q}\) to the definitions of measure-theoretic pressure and topological pressure. In fact, we generalize Katok’s entropy formula to measure-theoretic pressure by the mean metric.
2 Preliminaries and Main Results
Throughout this paper, by a topological dynamical system (t.d.s. for short) we mean a pair (X, T), where X is a compact metric space with a metric d and T is a homeomorphism from X to itself. Let \(C(X, {\mathbb {R}})\) denote the set of all continuous functions of X. Given a t.d.s. (X, T), let M(X) denote the collection of all Borel probability measures on measurable space \(\left( X, {\mathcal {B}}_X\right) \), where \({\mathcal {B}}_X\) denote the Borel \(\sigma \)-algebra on X. The set of all T-invariant Borel probability measures in M(X) will be denoted by M(X, T). The set of all T-invariant ergodic measures in M(X, T) will be denoted by \(M^e(X, T)\). It is noted that each \(\mu \in M(X, T)\) induces a measure preserving system (m.p.s. for short) \(\left( X, {\mathcal {B}}_X, \mu , T\right) \).
Let (X, T) be a t.d.s. with a metric d. For \(q, n \in {\mathbb {N}}\), we consider the max metric
for any \(x, y \in X\). For \(\varphi \in C(X,{\mathbb {R}})\),\(\mu \in M(X, T)\) and \(\varepsilon >0\), set
and
Let
where
for any \(x \in X\). We define
When \(q=1\), [9] establish measure-theoretic pressure version of Katok’s entropy formula as follows:
Theorem 2.1
[9] Let (X, T) be a t.d.s. If \(\mu \in M(X, T)\) is ergodic, then
For \(\mu \in M(X, T)\) and \(q, n \in {\mathbb {N}}\), we consider the mean metric
for any \(x, y \in X\). For \(\varepsilon >0\) and \(\varphi \in C(X,{\mathbb {R}})\), let
where
for any \(x \in X\). We define
When \(q=1\), [6] established measure-theoretic pressure version of Katok’s entropy formula in mean metrics as follows:
Theorem 2.2
[6] Let (X, T) be a t.d.s. If \(\mu \in M(X, T)\) is ergodic, then
Next, we need to define the topological pressure:
Let (X, T) be a t.d.s., for \(q, n \in {\mathbb {N}}\) and \(\varphi \in C(X,{\mathbb {R}})\), we consider
For \(\varepsilon > 0\) and \(\varphi \in C(X,{\mathbb {R}})\),put
When \(\varepsilon \rightarrow 0\), we can get
Also, the variation principle [19] reveals the basic relationship between topological pressure and measure-theoretic pressure: let (X, T) is a TDS and \(\varphi \in C(X,{\mathbb {R}})\), then
We give the computation formula of the measure-theoretic pressure of an ergodic measure preserving system (resp., the topological pressure of a topological dynamical system) by the two metrics \(d_{n, q}\) and \({\overline{d}}_{n, q}\).
Our main results are as follows:
Theorem 2.3
Let (X, T) be a t.d.s.. Then for any \(\mu \in M^e(X, T)\) and \(\varphi \in C(X,{\mathbb {R}})\), we have
and
Let (X, T) be a t.d.s. with a metric d. For \(q, n \in {\mathbb {N}}\) and \(\varepsilon >0\),
We define
Similarly, we can define \(S_{d_{n, q}}(\varphi ,\varepsilon ), S_n^*(\varphi ,\varepsilon )\) by changing \({\overline{d}}_{n, q}\) into \(d_{n, q}\).
Theorem 2.4
Let (X, T) be a t.d.s and \(\varphi \in C(X,{\mathbb {R}})\). Then
and
3 Proof of Theorem 2.3
Before the proof of Theorem 2.3, we need a lemma which similar to Lemma 3.1 in [6] as follows. In order to prove the Lemma 3.1, we need the relationship between the \({\overline{d}}_{n,q}\)-ball \(B_{{\overline{d}}_{n,q}}(x, \varepsilon )\) where the mistake function \(g: {\mathbb {N}} \times (0,1] \rightarrow {\mathbb {R}}\) by \(g(n, \varepsilon ):=n \varepsilon \) for any \(\varepsilon \in (0,1], n \in {\mathbb {N}}\). The function g is called a mistake function. Note that g is a special mistake function and the definition of the function g is different from the definition of the mistake function in [17] or [20].
Definition 3.1
Let \(0<\varepsilon \le 1\) and \(n \ge 1\). The mistake dynamical ball \(B_{d_{n,q}}(g; x, \varepsilon )\) centered at x with radius \(\varepsilon \) and length n associated to function g is defined as follows:
Lemma 3.1
For any \(x \in X, n \in {\mathbb {N}}\) and \(\varepsilon >0\), we have
where \(g=n\sqrt{\varepsilon }.\)
Proof
For any \(q \in {\mathbb {N}}\), Set
Noting that
If \(y \in B_{{\overline{d}}_{n,q}}(x, \varepsilon )\), i.e., \({\overline{d}}_{n,q}(x, y)<\varepsilon \), we have
Thus, we obtain
Then \(y \in B_{d_{n,q} }(g; x, \sqrt{\varepsilon })\),
Therefore, we have \(B_{{\overline{d}}_{n,q}}(x, \varepsilon ) \subset B_{d_{n,q} }(g; x, \sqrt{\varepsilon })\). \(\square \)
Next, we prove the Theorem 2.3.
Proof
Let (X, T) be a t.d.s. First we show that for any \(\mu \in M^e(X, T)\)
Fix \(\varepsilon >0\) and \(\mu \in M^e(X, T)\). Recall that \(d_{n,1}(x, y)=\max \limits _{0 \le i \le n-1} d\left( T^i x, T^i y\right) \). It is obvious that \({\overline{d}}_{n, 1}(x, y) \le d_{n,1}(x, y)\) and \( B_{d_{n,1}}(x, \varepsilon ) \subset B_{{\overline{d}}_{n, 1}}(x, \varepsilon )\). For any \(\tau > 0 \) and n large enough, by Theorem 2.1 there exists a finite subset \(F_n\) of X such that
and an open subset \(K_n\) of X with \(\mu \left( K_n\right) >1-\varepsilon \) such that for any \(x \in K_n\) there is \(y \in F_n\) with \(d_{n,1}(x, y)<\varepsilon \), which implies \({\overline{d}}_{n, 1}(x, y) \le d_{n,1}(x, y)<\varepsilon \). This implies that
and hence we have
Let \(\tau \rightarrow 0\), we finish this proof.
Now we are to prove that for any \(\mu \in M^e(X, T)\)
Given a Borel partition \(\eta =\left\{ A_1, \ldots , A_k\right\} \) of X and \(0<\delta <1\), it is sufficient to show
where \(a=\lim \limits _{\varepsilon \rightarrow 0} \liminf \limits _{n \rightarrow \infty } \frac{1}{n} \log {\overline{S}}_n^*(\varphi ,\mu , \varepsilon )\). Take \(0<\tau <\frac{1}{2}\) with
By [19], Lemma 4.15 and Corollary 4.12.1], it is easy to see that there is a Borel partition \(\xi =\left\{ B_1, \ldots , B_k, B_{k+1}\right\} \) of X associated with \(\eta \) such that \(B_i \subset A_i\) is closed for \(1 \le i \le k\) and \(B_{k+1}=X \backslash K\) with \(K=\bigcup _{i=1}^k B_i, \mu \left( B_{k+1}\right) <\tau ^2\) and
It is clear that \(B_i \cap B_j=\emptyset , 1 \le i<j \le k\) and \(\mu (K)>1-\tau ^2\). Let \(b=\min \limits _{1 \le i<j \le k} d\left( B_i, B_j\right) \). Then \(b>0\).
Given \(\gamma >0,0<\varepsilon <\min \left\{ 1-2 \tau , \frac{1}{2} b(1-2 \tau )\right\} \). For \(q, n \in {\mathbb {N}}\) and \(\gamma \ge 0 \), by the definition of \(S_{{\overline{d}}_{n, q}}(\varphi ,\mu , \varepsilon )\) there are \(x_1, \ldots , x_{m(n, q)} \in X\) such that \(\mu \left( \bigcup _{i=1}^{m(n, q)} B_{{\overline{d}}_{n, q}}\left( x_i, \varepsilon \right) \right) >1-\varepsilon \), where
Let \(F_{n, q}=\bigcup _{i=1}^{m(n, q)} B_{{\overline{d}}_{n, q}}\left( x_i, \varepsilon \right) .\) Then \(\mu \left( F_{n, q}\right) >1-\varepsilon \). For \(x \in X\), let \(K_q(x)=\left\{ i \in {\mathbb {Z}}_{+}: T^{q i} x \in K\right\} \) and
\(E_{n, q}=\left\{ x \in X: \frac{\left| K_q(x) \cap [0, n-1]\right| }{n} \le 1-\tau \right\} \). Note that
We have
which implies that \(\mu \left( E_{n, q}\right) <\tau \). Put \(W_{n, q}=\left( K \cap F_{n, q}\right) \backslash E_{n, q}\). Then
and for \(z \in W_{n, q}\)
For a given \(1 \le i \le m(n, q)\), let
We claim
where \(c(\varepsilon )=2 \frac{\varepsilon }{b}+2 \tau \) and \([n c(\varepsilon )]\) is the integer part of \(n c(\varepsilon )\). To see this, let \(U_1, U_2 \in \xi _{n, q}(i)\). Take \(x \in U_1 \cap B_{{\overline{d}}_{n, q}}\left( x_i, \varepsilon \right) \cap W_{n, q}\) and \(y \in U_2 \cap B_{{\overline{d}}_{n, q}}\left( x_i, \varepsilon \right) \cap W_{n, q}\). Then \({\overline{d}}_{n, q}(x, y)<2 \varepsilon \) and \(\left| K_q(x) \cap K_q(y) \cap [0, n-1]\right| >(1-2 \tau ) n\). This implies that
Hence (3.3) holds. It remains to show \(h_\mu (T, \xi )+\int \varphi \textrm{d}\mu \le a+\delta \). If \(C \in \xi \vee T^{-q} \xi \vee \cdots \vee T^{-q(n-1)} \xi \cap W_{n,q}\),We define
For each \(C \in \xi \vee T^{-q} \xi \vee \cdots \vee T^{-q(n-1)} \xi \cap W_{n,q}\), we can choose some \(x_C \in \bar{C}\), so that \(S_{n,q}\varphi (x_C)=\alpha (C)\). For \(q, n \in {\mathbb {N}}\), we know that
For any \(C \in \xi \vee T^{-q} \xi \vee \cdots \vee T^{-q(n-1)} \xi \cap W_{n, q}\), then \(C \subset \bigcup _{i=1}^{m(n, q)} B_{{\overline{d}}_{n, q}}\left( x_i, \varepsilon \right) \), there exists \(1 \le i \le m(n, q)\) such that \({\overline{d}}_{n, q}\left( x_C, x_i\right) \le \varepsilon <2 \varepsilon \). Hence, by Lemma 3.1, \(x_C \in B_{d_{n, q}}\left( g; x_i, \sqrt{2 \varepsilon }\right) \) with \(g=n \sqrt{2 \varepsilon }\) and
Then
Combining this with 3.3, we have
Hence,
Since q is arbitrary, we have
Combing with the Stirling’s formula which implies that
one has
By taking \(\varepsilon \rightarrow 0\), we can have
Hence by (3.1), \(h_\mu (T, \eta )+\int \varphi \mathrm {~d} \mu <a+2 \delta \). This finishes the proof of the first formula of Theorem 2.3.
Next we are going to prove the second formula
Fix \(\varepsilon >0\) and \(\mu \in M^e(X, T)\). Recall that for any \(x, y\in X, {\overline{d}}_{n, q}(x, y) \le d_{n, q}(x, y) \) and then
Hence, \( S_{{\overline{d}}_{n, q}}(\varphi ,\mu , \varepsilon ) \le S_{d_{n, q}}(\varphi ,\mu , \varepsilon ). \) Thus \({\overline{S}}_n^*(\varphi ,\mu , \varepsilon ) \le S_n^*(\varphi ,\mu , \varepsilon )\). Furthermore, we have
Now we proceed to prove the inverse inequality: for any \(\mu \in M^e(X, T)\),
Fix \(\varepsilon >0\) and \(\mu \in M^e(X, T)\). Recall that \(d_{n, 1}(x, y)=d_n(x, y)\). Hence by Theorem 2.1 we have
So we are done. \(\square \)
4 Proof of Theorem 2.4
Proof
Let (X, T) be a t.d.s. with a metric d. First we show that \(\lim \limits _{\varepsilon \rightarrow 0} \limsup \limits _{n \rightarrow \infty } \frac{1}{n} \log {\overline{S}}_n^*(\varphi ,\varepsilon ) \le P_{\textrm{top}}(T,\varphi )\). For anty \(\tau >0.\) we can choose \(\varepsilon \) small enough and n large enough, By the definition of Topological pressure, there exists a finite subset \(F_n\) of X with \(\bigcup _{x_i\in F_n} B_{d_{n,1}}\left( x_i, \varepsilon \right) =X\) such that
Fix the above \(\varepsilon >0\). For any \(x, y\in X\), it is clear that
Recall that for \(n \in {\mathbb {N}}\),
Since for any \(x \in X\) there is \(y \in F_n\) with \({\overline{d}}_{n, 1}(x, y) \le d_n(x, y)<\varepsilon \). Connecting with (4.1), one has
Hence by taking \(\varepsilon \rightarrow 0\) we have
Let \(\tau \rightarrow 0\), we finish this prove.
Now we are going to prove that
By the varitional principle [19] it is sufficient to show that for any \(\mu \in M^e(X, T)\)
It is easy to see that for \(\varepsilon >0\) and \(n \in {\mathbb {N}}\),
Then by Theorem 2.3,
This finishes the proof of the first formula of Theorem 2.4.
Finally we are going to prove the second formula:
To show \(P_{\textrm{top}}(T,\varphi ) \le \lim \limits _{\varepsilon \rightarrow 0} \liminf \limits _{n \rightarrow \infty } \frac{1}{n} \log S_n^*(\varphi ,\varepsilon )\), by the variation principle it is sufficient to show that for any \(\mu \in M^e(X, T)\)
Note that for \(\varepsilon >0\) and \(n \in {\mathbb {N}}\), \(S_n^*(\varphi ,\mu , \varepsilon ) \le S_n^*(\varphi ,\varepsilon ).\) Then by Theorem 2.3,
Now we proceed to the proof of the inverse inequality:
It is not hard to see that
This finishes the proof of Theorem 2.4. \(\square \)
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Acknowledgements
We would like to thank the referee for careful reading and useful comments that resulted in substantial improvements to this paper. The work was supported by the National Natural Science Foundation of China (No.11901419).
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Zhang, J., Zhao, C. & Liu, L. A Note on the Measure-Theoretic Pressure in Mean Metric. Bull. Malays. Math. Sci. Soc. 46, 78 (2023). https://doi.org/10.1007/s40840-023-01473-7
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DOI: https://doi.org/10.1007/s40840-023-01473-7