The same telescoping procedure can be obtained for “coordinate-wise Hölder” functions,

f ∈ LipE Z , R, via the control 3 on ∆ i , together with Burkholder’s inequality [5, Theorem 3.1, p. 87], which relates the moments of f − E f with powers of the sum of squares of ∆ i . The non-uniformity as a function of the realization of X i −∞ of the decay of the matrix elements as a function of j which we encountered e.g. in the low-temperature Ising model [7] will be typical as soon as the state space E is unbounded. Indeed, if starting points in the coupling are further away, then it takes more time to get the copies close in the coupling . R EMARK

3.1. The same telescoping procedure can be obtained for “coordinate-wise Hölder” functions,

i.e., functions such that for some 0 α 1 δ α i f := sup f x − f y d α x i , y i : x j = y j , ∀ j 6= i, x i 6= y i . is finite for all i. In 4, we then have to replace d by d α . 4 The Markov case We now consider X n n ∈Z to be a stationary and ergodic Markov chain. We denote by px, d y := P X 1 ∈ d y X = x the transition kernel. We let ν be the unique stationary measure of the Markov chain. We denote by P ν the path space measure of the stationary process X n n ∈Z . By P x we denote the distribution of X ∞ 1 , for the Markov process conditioned on X = x. We further suppose that the coupling ˆ P of Section 2.2 is Markovian, and denote by ˆ P x, y the coupling started from x, y, and corresponding expectation by ˆ E x, y . More precisely, by the Markov property of the coupling we then have that ˆ P x i −∞ , y i −∞ = ˆ P x i , y i is a Markovian coupling ˆ X 1 n , ˆ X 2 n n ∈N of the Markov chains X n n ≥0 starting from X = x i , resp. Y = y i . In this case the expression 4 of the coupling matrix simplifies to Ψ X i −1 ,X i j := D X i −1 ,X i i,i+ j = Z pX i −1 , d y Z d ˆ P X i , y u ∞ , v ∞ du j , v j 5 With this notation, 3 reads |∆ i X i −1 , X i | ≤ X j ≥0 Ψ X i −1 ,X i jδ i+ j f . 6 We define the “generalized coupling time” τ u ∞ , v ∞ := ∞ X j=0 du j , v j . 7 In the case E is a discrete finite or countable alphabet, the “classical” coupling time is defined as usual T u ∞ , v ∞ := inf{k ≥ 0 : ∀ j ≥ k : u j = v j }. If we use the trivial distance dx, y = 1 if x 6= y and dx, y = 0 if x = y, for x, y ∈ E, then we have du j , v j ≤ 1l{T u ∞ , v ∞ ≥ j} 8 1166 and hence τ u ∞ , v ∞ ≤ T u ∞ , v ∞ . Of course, the same inequality remains true if E is a bounded metric space with dx, y ≤ 1 for x, y ∈ E. However a “successful coupling” i.e., a coupling with T ∞ is not expected to exist in general in the case of a non-discrete state space. It can however exist, see e.g. [13] for a successful coupling in the context of Zhang’s model of self-organized criticality. Let us also mention that the “generalized coupling time unavoidably appears in the context of dynamical systems [8]. In the discrete case, using 6 and 8, we obtain the following inequality: Ψ x, y j ≤ X z px, zˆ E z, y € 1l {T u ∞ , v ∞ ≥ j} Š 9 whereas in the general not necessarily discrete case we have, by 7, and monotone convergence, X j ≥0 Ψ x, y j = Z px, dzˆ E y,z τ ≤ Z px, dzˆ E y,z T . 10 R EMARK

4.1. So far, we made a telescoping of f − E f using an increasing family of sigma-fields. One

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