1. Introduction and main results
We consider the stochastic differential equation (SDE)
where the function
$b: \mathbb{R}^d \rightarrow \mathbb{R}^d$
satisfies Assumption 1 below,
$A \in \mathbb{R}^{d \times d}$
is a positive-definite matrix,
$(Z_t)_{t\geqslant 0}$
is a d-dimensional rotationally invariant
$\alpha$
-stable Lévy process with
$\alpha \in (1,2)$
and
$x\in\mathbb{R}^{d}$
.
Under Assumption 1, the SDE (1.1) admits a unique invariant measure
$\nu$
(see e.g. [Reference Liang and Wang27, Corollary 1.4]). In order to approximate the invariant measure
$\nu$
, we consider the following Euler–Maruyama (EM) scheme: let
$Y_{0}=x$
and
where
$t_{0}=0$
,
$t_{n}=\sum_{i=1}^n \gamma_{i}$
,
$\{\gamma_{n}\}_{n\in \mathbb{N}}$
is a decreasing sequence of positive numbers satisfying
$\sum_{i=1}^{\infty}\gamma_{i}=\infty$
, and
$\{\zeta_n\}_{n \in \mathbb N}$
are independent and identically distributed (i.i.d.) d-dimensional rotationally invariant
$\alpha$
-stable random vectors. It is easy to see that the random variables
$\{Y_{t_n}\}_{n \geqslant 1}$
obtained by
have the same distribution as those obtained by (1.2).
Owing to the complexity of sampling multi-dimensional stable distributions (see the detailed discussions in [Reference Chambers, Mallows and Stuck9] and [Reference Nolan33, Section 1.9]), we also use the Pareto distribution for the innovations in the EM scheme (1.5) below. Let
$\tilde{Z}_1,\tilde{Z}_2, \ldots $
be a sequence of i.i.d. d-dimensional Pareto random vectors, that is,
Then we are able to approximate the SDE (1.1) by the iterative scheme
\begin{equation}\tilde{Y}_{t_{n+1}} = \tilde{Y}_{t_n} + \gamma_{n+1} b(\tilde{Y}_{t_n}) + \frac{\gamma_{n+1}^{\frac{1}{\alpha}}}{\beta} A\tilde{Z}_{n+1},\end{equation}
where
$\beta=(\frac{\alpha}{\sigma_{d-1}d_{\alpha}})^{\frac{1}{\alpha}}$
with
$\sigma_{d-1}=\frac{2\pi^{\frac{d}{2}}}{\Gamma(\frac{d}{2})}$
and
$d_{\alpha} = \frac{\alpha 2^{\alpha-1}\pi^{-\frac{d}{2}}\Gamma(\frac{d+\alpha}{2})}{\Gamma(1-\frac{\alpha}{2})}$
.
1.1. Motivation and related work
There has been extensive research on the EM scheme for SDEs; see, for example, [Reference Bally and Talay3, Reference Bao, Huang and Yuan4, Reference Dareiotis and Gerencs12, Reference Jacod19, Reference Janicki, Michna and Weron20, Reference Li, Mao, Song, Wu and Yin24, Reference Li, Ma, Yang and Yuan25, Reference Marion, Mao and Renshaw29, Reference Sanz-Serna and Zygalakis41, Reference Shao42, Reference Tarami and Avaji44, Reference Yuan and Mao47] and the references therein for more details. Over the past decade, EM schemes for SDEs such as (1.1) have been intensively studied by many authors, including [Reference Butkovsky, Dareiotis and Gerencsér5, Reference Hashimoto17, Reference Huang and Liao18, Reference Kühn and Schilling21, Reference Li and Zhao23, Reference Mimica, Sandrić and Schilling30, Reference Pamen and Taguchi35–Reference Protter and Talay37]. Most of these works focus on the case where the step size of the EM scheme is constant, demonstrating the convergence rate over a finite time interval [0,T] for some constant
$T>0$
. However, as
$T \rightarrow \infty$
, this rate usually blows up. To the best of our knowledge, [Reference Chen, Deng, Schilling and Xu6] is the first paper that has studied the long-term behaviour of the EM scheme of an SDE driven by an
$\alpha$
-stable process, but the step size therein is constant. However, in most real applications, the step sizes (or learning rates) tend to decrease as the iterations progress. What is more, [Reference Chen, Deng, Schilling and Xu6] assumes a strong condition on the drift function b in the first EM scheme. A primary motivation for our research is to improve upon the results presented in [Reference Chen, Deng, Schilling and Xu6].
Another motivation for this paper stems from the recent paper [Reference Pagès and Panloup34] by Pagès and Panloup, who considered the convergence rate of an unadjusted Langevin algorithm with decreasing step sizes. Our EM schemes have a similar form to the unadjusted Langevin algorithm with additive innovation in [Reference Pagès and Panloup34], only replacing the standard normal random variables therein with Pareto random vectors or
$\alpha$
-stable random vectors. A remarkable result of [Reference Pagès and Panloup34] is that the unadjusted Langevin algorithm converges to the targeted measure at a rate depending only on the step sizes
$\gamma_n$
at the terminal iterate n. We prove in this paper that the EM scheme (1.5) exhibits the same phenomenon in the Wasserstein–1 distance setting.
Because of the significance of high-dimensional sampling problems arising in machine learning, there has recently been a surge in studies of the convergence rates of EM schemes to their corresponding SDEs as time tends to infinity. When
$\alpha=2$
, Fang et al. [Reference Fang, Shao and Xu15] used the EM scheme to approximate the invariant measure for an SDE driven by Brownian motion with the help of the Malliavin calculus and Stein’s method; Pagès et al. [Reference Pagès and Panloup34] used the Bismut–Elworthy–Li formula to approximate the invariant measure under the EM scheme and obtain the order-1 optimal convergence rate. For more details about the Brownian motion case, we refer to [Reference Angeli, Crisan and Ottobre1, Reference Li, Wang and Xu22, Reference Li, Ma, Yang and Yuan25, Reference Sanz-Serna and Zygalakis41] and the references therein. Furthermore, besides the developments in convergence analysis of unadjusted Langevin algorithms [Reference Dalalyan10, Reference Durmus and Moulines13, Reference Durmus and Moulines14], heavy-tailed stochastic algorithms have recently attracted a lot of attention; see, for instance, [Reference Lim28, Reference Neu, Dziugaite, Haghifam and Roy31, Reference Nguyen, Simsekli, Gurbuzbalaban and Richard32]. In particular, by using the convergence result in [Reference Chen, Deng, Schilling and Xu6], heavy-tailed stochastic gradient descent algorithms are delicately analysed in [Reference Raj, Barsbey, Gurbuzbalaban, Zhu and Simsekli38, Reference Raj, Barsbey, Gürbüzbalaban, Zhu and Simsekli39]. We expect that the more general results in the present paper will be useful for studying heavy-tailed stochastic algorithms.
1.2. Notation
We denote by
$|\cdot|$
the Euclidean norm of
$\mathbb R^d$
, i.e. for
$x \in \mathbb R^d$
,
$|x|=\sqrt{x^2_1+\ldots +x^2_d}$
. Given any two probability measures
$\nu_1$
and
$\nu_2$
on
$\mathbb{R}^d$
, their
$L^p$
-Wasserstein distance
$W_p$
with
$p\geqslant 1$
is defined as
where
$\mathcal{C}(\nu_1,\nu_2)$
is the set of probability distributions on
$\mathbb{R}^d \times \mathbb{R}^d$
with marginal measures
$\nu_1$
and
$\nu_2$
. By using the Kantorovich duality (see [Reference Villani43, Theorem 5.10]), the Wasserstein-1 distance can also be defined as
where
${\rm Lip}(1)$
is the set of Lipschitz functions with Lipschitz constant 1, that is,
${\rm Lip}(1)= \{ f: \frac{|f(x)-f(y)|}{|x-y|} \leqslant 1\ \ \forall x, y \in \mathbb{R}^d \}.$
For matrices
$A=(A_{ij})_{d\times d}$
and
$B=(B_{ij})_{d\times d}$
, define
$ \langle A,B\rangle_{\rm HS}=\sum_{i,j=1}^d A_{ij} B_{ij}$
; then the Hilbert–Schmidt norm is
$\| A\|_{\rm HS}=\sqrt{ \langle A,A\rangle_{\rm HS} }$
.
For
$k \in \mathbb{N}_0\,:\!=\,\mathbb{N} \cup\{0\}$
, denote by
$\mathcal C^k\left(\mathbb{R}^d, \mathbb{R}\right)$
the set of functions which have kth-order continuous derivatives. In particular,
$\mathcal C^0\left(\mathbb{R}^d, \mathbb{R}\right)= \mathcal C\left(\mathbb{R}^d, \mathbb{R}\right)$
denotes the set of continuous functions. For
$f \in \mathcal C^2\left(\mathbb{R}^d, \mathbb{R}\right)$
and
$v_1, v_2, x \in \mathbb{R}^d$
, the directional derivatives
${\nabla}_{v_1} f(x)$
and
$\nabla_{v_2} \nabla_{v_1} f(x)$
are defined by
The operator norm of
$\nabla^2 f(x) \in \mathbb{R}^{d \times d}$
is defined by
Let
$\| f \|_{\infty} = \text{supp}_{x\in \mathbb{R}^d}|f(x)|$
for a bounded continuous function f. For any
$f\in \mathcal{C}^2(\mathbb{R}^d,\mathbb{R})$
, let
$\nabla f$
and
$\nabla^2 f $
be the gradient and Hessian matrix of f, respectively, and write
$\| \nabla f \|_{\infty} = \text{supp}_{x\in \mathbb{R}^d} |\nabla f(x)|$
and
$\| \nabla^2 f \|_{{\rm HS},\infty}= \text{supp}_{x\in \mathbb{R}^d} \| \nabla^2 f(x) \|_{{\rm HS}}$
if they both exist.
For
$k \in \mathbb{N}_0$
, further denote by
$\mathcal C^k_{\rm lin}(\mathbb{R}^d,\mathbb{R})$
the set of functions in
$\mathcal C^k\left(\mathbb{R}^d, \mathbb{R}\right)$
that have linear growth, i.e.
When
$k=0$
, we write this set as
$\mathcal C_{\rm lin}(\mathbb{R}^d,\mathbb{R})$
.
For any random variable X, denote its law by
$\mathcal{L}(X)$
, and for any
$r_{1},r_{2}\in\mathbb{R}$
, let
$r_{1}\vee r_{2}=\max\{r_{1},r_{2}\}$
.
1.3. Assumptions and the main results
We impose the following assumptions on the drift b.
Assumption 1. The drift b is a Lipschitz function, i.e. there exists a constant
$L>0$
such that
Moreover, there exist constants
$\theta_1>0$
and
$K\geqslant 0$
such that
It is well known that under Assumption 1, the process
$(X_t)_{t \geqslant 0}$
admits at least one invariant measure by the classical Krylov–Bogoliubov theorem; see, for instance, [Reference Da Prato and Zabczyk11, Section 3.1]. Under this assumption, we further show that
$(X_t)_{t \geqslant 0}$
satisfies a certain contraction property in the Wasserstein-1 distance, which, together with the existence of invariant measures, immediately implies the ergodicity in the Wasserstein-1 distance. More details are given in Lemma 6.
Many functions b satisfy the above assumption; here we give a one-dimensional example.
Example 1. For any
$x\in\mathbb{R}$
, let
\begin{equation*}b(x)= \left\{\begin{aligned}x^2-x & {\rm \ \ if \ \ } |x|\leqslant 1, \\-x+1 & {\rm \ \ if \ \ } |x|>1.\end{aligned}\right.\end{equation*}
Then
$\text{supp}_{x\in \mathbb{R}} \{ |\nabla b(x)| \}=3$
. In addition, if
$|x|\leqslant 1$
and
$|y|\leqslant 1$
, then
When
$|x|\leqslant 1$
and
$|y|>1$
, one has
\begin{eqnarray*}(x-y)(b(x)-b(y)) & \,=\, & (x-y)(x^2-x+y-1)\ = \ -(x-y)^2+(x-y)(x^2-1) \\& \leqslant & -\frac{1}{2}(x-y)^2+\frac{(x^2-1)^2}{2}\ \leqslant \ -\frac{1}{2}(x-y)^2+\frac{1}{2}.\end{eqnarray*}
The result is similar for the case where
$|x|>1$
and
$|y|\leqslant 1$
. Finally, if
$|x|>1$
and
$|y|>1$
, then
It follows from the above straightforward calculations that Assumption 1 holds with
$L=3, \theta_{1}=\frac{1}{2}$
and
$K=2$
.
For the sequence
$(\gamma_{n})_{n\in \mathbb{N}}$
of step sizes, we make the following assumption.
Assumption 2.
-
(i) The step sizes
$(\gamma_n)_{n\in \mathbb{N}}$
form a decreasing sequence such that
$\lim\limits_{n\to \infty} \gamma_n=0$
and
$\sum_{n=1}^{\infty}\gamma_{n}=\infty$
. -
(ii) The step sizes
$(\gamma_n)_{n\in \mathbb{N}}$
satisfy the inequality (1.10)for some
\begin{eqnarray}\omega \,:\!=\, \limsup_{k\to \infty} \frac{\gamma_k^{\theta}-\gamma_{k+1}^{\theta}}{\gamma_{k+1}^{1+\theta}} <+\infty\end{eqnarray}
$\theta\in(0,1]$
.
Throughout the paper, we use C to denote a constant that may depend on parameters such as
$L,\theta,K,\omega$
and
$\kappa\in[1,\alpha)$
, and its value may vary from line to line.
Now we are in a position to state our main theorems. We first give an error bound between the processes
$(X_t)_{t\geqslant 0}$
and
$(Y_{t_n})_{n\in \mathbb{N}_0}$
. In the following,
$\mathcal{L}(X_{t}^x)$
denotes the law of
$X_t$
starting from x at time
$t = 0$
, and
$\mathcal{L}(Y_{t_n}^x)$
is similarly defined. In addition, we set
which is a constant that arises from the exponential ergodicity of the process
$X_{t}$
(see Lemma 6 below) and will play an important role in the subsequent statements.
Theorem 1. Let
$(X_t)_{t\geqslant 0}$
and
$(Y_{t_n})_{n\in \mathbb{N}_0}$
be governed by (1.1) and (1.3), respectively. Under Assumption 1, suppose that Assumption 2 holds with
$\theta=\frac{1}{\alpha}$
and
$\omega<\rho$
. Then there exists a positive constant C independent of d and n such that for all
$x \in \mathbb{R}^d$
and
$t_n>1$
,
Here and in what follows,
$\nu$
denotes the invariant measure of
$(X_t)_{t\geqslant 0}$
.
Remark 1. Note that the Wasserstein-1 distance is well-defined only for distributions with a finite first moment; therefore, our method is not applicable to the case of
$\alpha \in (0,1]$
, as in this range
$\mathbb{E}|Z_{t}|=\infty$
and
$\mathbb{E}|X_{t}|=\infty$
, resulting in undefined first moments.
Remark 2. As an example of decreasing step sizes
$(\gamma_n)_{n\in \mathbb{N}}$
, we take
where
$c>1$
is a constant. Let
$\theta=\frac{1}{\alpha}$
in (1.10); then a straightforward calculation yields
\[\omega = \limsup_{k\to \infty} \frac{\gamma_{k}^{\frac{1}{\alpha}}-\gamma_{k+1}^{\frac{1}{\alpha}}}{\gamma_{k+1}^{1+\frac{1}{\alpha}}}= \frac{\rho}{\alpha c} < \rho.\]
In this case, the constant
$\frac{C}{\rho-\omega}\exp(\frac{\rho-\omega}{2}\gamma_{1})\exp(d^{4-2\alpha} 2^{d})d^{5}$
in Theorem 1 reduces to
$C\exp(d^{4-2\alpha}2^{d+1})d^{5}$
.
We also consider an additional smoothness condition for the coefficient b, as follows.
Assumption 3. The coefficient
$b\in\mathcal{C}^{2}(\mathbb{R}^{d})$
, and there exists a constant
$\theta_{2}>0$
independent of the dimension d such that
An interesting example which satisfies Assumption 3 is
$b(x)=-x$
, and we will analyse this example carefully in Appendix A.
Remark 3. It is easy to verify from Assumption 1 that
Inequality (1.8) and Assumption 3 further imply that
Theorem 2. Let
$(X_t)_{t\geqslant 0}$
and
$(Y_{t_n})_{n\in \mathbb{N}_0}$
be governed by (1.1) and (1.3), respectively. Suppose that Assumptions 1 and 3 hold and also that Assumption 2 holds with
$\theta=1+\frac{1}{\alpha}-\frac{1}{\kappa}$
and
$\omega<\rho$
, where
$\kappa \in[1,\alpha)$
. Then there exists a constant
$C>0$
independent of d and n such that for all
$x \in \mathbb{R}^d$
and
$t_n>1$
,
\begin{align}& W_1(\mathcal{L}(X_{t_n}^x), \mathcal{L}(Y_{t_n}^x)) \nonumber \\& \quad \leqslant \frac{C}{\rho-\omega}\exp\!\left(\frac{\rho-\omega}{2}\gamma_1\right) \exp(d^{4-2\alpha} 2^{d}) d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2} )}\gamma_{n}^{1+\frac{1}{\alpha}-\frac{1}{\kappa}}(1+|x|^{\kappa}),\end{align}
\begin{align}& W_1(\nu,\mathcal{L}(Y_{t_n}^x)) \nonumber \\& \quad \leqslant \frac{C}{\rho-\omega}\exp\!\left(\frac{\rho-\omega}{2}\gamma_1\right) \exp(d^{4-2\alpha} 2^{d})d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}\,\gamma_{n}^{1+\frac{1}{\alpha}-\frac{1}{\kappa}} (1+|x|^{\kappa}). \end{align}
Remark 4. We conjecture that the optimal convergence rate for the first scheme Y is
$\gamma_n$
, rather than
$\gamma_n^{1-\varepsilon}$
for any
$\varepsilon \in (0,1)$
. However, due to the limitations of our current techniques, we are only able to establish a rate of
$\gamma_n^{1-\varepsilon}$
. Eliminating this arbitrarily small
$\varepsilon>0$
will require the development of new techniques.
For the EM scheme with Pareto-distributed noise, we have the following convergence theorem.
Theorem 3. Let
$(X_t)_{t\geqslant 0}$
and
$(\tilde{Y}_{t_n})_{n\in \mathbb{N}_0}$
be governed by (1.1) and (1.5) respectively. Suppose that Assumptions 1 and 3 hold and also that Assumption 2 holds with
$\theta=\frac{1}{\alpha}$
and
$\omega<\rho$
. Then there exists a positive constant C independent of d and n such that for all
$x \in \mathbb{R}^d$
and
$t_n>1$
,
Remark 5.
-
(i) For any
$0<\theta\leqslant \delta\leqslant 1$
, by the fact that it follows that the condition on the step-size sequence in Theorem 2 is slightly more restrictive than that in Theorems 1 and 3.
\begin{eqnarray*}\frac{\gamma_{n}^{\theta}-\gamma_{n+1}^{\theta}}{\gamma_{n+1}^{1+\theta}}\leqslant\frac{\gamma_{n}^{\delta}-\gamma_{n+1}^{\delta}}{\gamma_{n+1}^{1+\delta}},\end{eqnarray*}
-
(ii) In Theorem 3, in order to ensure the convergence of the series in the proof, we require Assumption 2 with
$\theta=\frac{1}{\alpha}$
, which is slightly stricter than the condition
$\theta=\frac{2-\alpha}{\alpha}$
. -
(iii) The rate
$\gamma_{n}^{\frac{2}{\alpha}-1}$
in Theorem 3 is optimal for the one-dimensional stable Ornstein–Uhlenbeck (OU) process; see Lemma 10 in Appendix A.
The rest of this paper is organized as follows. We provide detailed proofs of our main results, Theorems 1, 2 and 3, in Section 2. Section 3 is dedicated to proving the crucial lemmas stated in Section 2. Finally, in Appendix A, we demonstrate that the optimal convergence rate
$\gamma_{n}^{\frac{2}{\alpha}-1}$
for the EM scheme with the Pareto distribution is achieved in the case of the stable Ornstein–Uhlenbeck process on
$\mathbb{R}$
.
2. Proofs of Theorems 1, 2 and 3
For any
$t_j>t_i \geqslant 0$
and
$f \in \mathcal C_{\rm lin}(\mathbb{R}^d,\mathbb{R})$
, define
\begin{align*}P_{t_i,t_j} f(x)&=\mathbb{E}[f(X_{t_j})|X_{t_i}=x]\quad \forall x \in \mathbb{R}^d, \\Q_{t_i,t_j} f(x)&=\mathbb{E}[f(Y_{t_j})|Y_{t_i}=x]\quad \forall x \in \mathbb{R}^d\end{align*}
and
Then, using the discrete version of Duhamel’s principle and the Markov property of the process
$(X_{t})_{t\geqslant 0}$
, we split
$P_{0,t_n} h(x) - Q_{0,t_n} h(x)$
as follows:
\begin{eqnarray}P_{0,t_n} h(x) - Q_{0,t_n} h(x)&\,=\,& \sum_{i=1}^{n} Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_{i},t_n} h(x) \\&\,=\,& \sum_{i=1}^{n^*} Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_{i},t_n} h(x) \nonumber \\&&+ \sum_{i=n^*+1}^{n-1} Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_{i},t_n} h(x) \nonumber \\&&+ \: Q_{0,t_{n-1}} \circ ( P_{t_{n-1},t_{n}} - Q_{t_{n-1},t_{n}} ) h(x), \nonumber\end{eqnarray}
where
$n^*=\max\{i:t_n-t_i>1\}$
.
For proving Theorems 1, 2 and 3, the exponential contraction property and the regularity of
$P_{t_i, t_n}$
play a crucial role. These properties are formulated and presented as lemmas in the next subsection.
2.1. Auxiliary lemmas
Similar to Proposition A.1 and Lemmas 3.3 and 3.4 in [Reference Pagès and Panloup34], we first give the moment estimates for
$(X_t)_{t\geqslant 0}$
,
$(Y_{t_n})_{n\in \mathbb{N}_0}$
and
$(\tilde{Y}_{t_n})_{n\in \mathbb{N}_0}$
, which will be proved in Section 3. For simplicity, for any
$i\leqslant j$
, we denote by
$X_{t_{i},t_{j}}^{x}$
the value of the process at time
$t_j$
while starting from x at time
$t_{i}$
. If
$t_i=0$
, then we denote it by
$X_{t_j}^x$
. The quantities
$Y_{t_{i},t_{j}}^{x}$
and
$\tilde{Y}_{t_{i},t_{j}}^x$
are similarly defined.
Lemma 1. Let
$(X_{t})_{t\geqslant0}$
,
$(Y_{t_n})_{n\in \mathbb{N}_0}$
and
$(\tilde{Y}_{t_n})_{n\in \mathbb{N}_0}$
be the processes defined by (1.1), (1.3) and (1.5), respectively. Suppose that Assumption 1 holds. Then for any
$1\leqslant\kappa <\alpha$
, there exists a constant
$C>0$
independent of d such that for all
$x \in \mathbb{R}^d$
,
Lemma 2. Let
$(X_{t})_{t\geqslant 0}$
be the solution to the SDE (1.1), and let
$(Y_{t_{n}})_{n\in\mathbb{N}_{0}}$
be the Markov chains defined by (1.3). Suppose that Assumption 1 holds. Then for any
$1\leqslant\kappa <\alpha$
, there exists a positive constant C independent of d such that for all
$n\in\mathbb{N}$
and
$x\in\mathbb{R}^{d}$
,
Based on the above lemmas, according to [Reference Chen, Nourdin, Xu and Yang7, Lemma 18], we can derive the following bound on the difference between
$P_{t_{n-1},t_{n}}f$
and
$Q_{t_{n-1},t_{n}}f$
, the proof of which is postponed to Section 3.
Lemma 3. Under Assumptions 1 and 3, let
$f\in \mathcal{C}^2(\mathbb{R}^d,\mathbb{R})$
satisfy
$\| \nabla f \|_{\infty} < \infty$
and
$\| \nabla^2 f \|_{{\rm HS}, \infty} < \infty$
. Then for
$\kappa \in[1,\alpha)$
, there exists a constant
$C>0$
independent of d such that for all
$k\in \mathbb{N}$
and
$x\in\mathbb{R}^{d}$
,
In the second EM scheme, the difference between
$P_{t_{n-1},t_{n}}f$
and
$\tilde{Q}_{t_{n-1},t_{n}}f$
is estimated in the following lemma.
Lemma 4 Under Assumption 1, let
$f\in \mathcal{C}^2(\mathbb{R}^d,\mathbb{R})$
satisfy
$\| \nabla f \|_{\infty} < \infty$
and
$\| \nabla^2 f \|_{{\rm HS}, \infty} $
$ < \infty$
. Then there exists a constant
$C>0$
independent of d such that for all
$k\in \mathbb{N}$
and
$x\in\mathbb{R}^{d}$
,
The above two lemmas work similarly to [Reference Pagès and Panloup34, Proposition 3.5]. Furthermore, corresponding to [Reference Pagès and Panloup34, Proposition 3.2], we also need the following regularities for
$P_{t_i,t_j}h(x)$
with
$h\in {\rm Lip}(1)$
and
$j\geqslant i$
, which can be proved in a similar way to Lemma 2.1 in [Reference Chen, Deng, Schilling and Xu6].
Lemma 5. Let
$h\in {\rm Lip}(1)$
and suppose that Assumptions 1 and 3 hold. Then there exists a constant
$C>0$
independent of d such that for all
$0 < t_j-t_i \leqslant 1$
and
$u_1,u_2 \in \mathbb{R}^d$
,
\begin{align*}\| \nabla_{u_1} P_{t_i,t_j} h \|_{\infty} &\leqslant C|u_1|, \\\| \nabla_{u_2} \nabla_{u_1} P_{t_i,t_j} h \|_{{\rm HS},\infty} &\leqslant C(t_j-t_i)^{-\frac{1}{\alpha}} |u_1| |u_2|.\end{align*}
Remark 6 Lemma 2.1 in [Reference Chen, Deng, Schilling and Xu6] is established by using the Bismut formula and a time-change argument as developed in [Reference Zhang48], under the condition that the constant matrix A is positive definite. However, this time-change approach fails in the case of multiplicative noise, where A is replaced by a general matrix function. Specifically, the convergence
$X_{t}^{l^{\epsilon}}\rightarrow X_{t}^{l}$
is no longer valid, as detailed in [Reference Wang, Xu and Zhang45, p. 3198]. Consequently, we focus on the case of additive noise and maintain the assumption that A is a positive-definite constant matrix.
Pagès et al. [Reference Pagès and Panloup34] investigated the convergence rate in the total variation distance with the help of the Domino–Malliavin method for non-smooth functions. It seems hard to obtain a similar result in our setting due to the limitation of the Malliavin calculus for SDEs driven by
$\alpha$
-stable noise.
The exponential ergodicity of the solution
$(X_t)_{t\geqslant 0}$
of the SDE (1.1) under Assumption 1 can be obtained using the same argument as in the proof of Theorem 1.3 in [Reference Liang and Wang27]; the proof is postponed to Section 3.5. The following lemma, together with [Reference Pagès and Panloup34, Corollary 2.4], is crucial for establishing the exponential ergodicity for the process
$(X_t)_{t\geqslant 0}$
.
Lemma 6. Under Assumption 1, there exists a constant
$C>0$
independent of d such that for all
$x,y\in\mathbb{R}^{d}$
and
$t>0$
,
In addition, the process
$(X_t)_{t\geqslant 0}$
in (1.1) is exponentially ergodic.
In addition, similar to Lemma A.3 in [Reference Pagès and Panloup34], the following lemma about the decreasing steps also plays an important role in proving the main theorems. This lemma will be proved in Section 3.
Lemma 7. For some
$\theta\in(0,1]$
, let
$(\gamma_{n})_{n\in \mathbb{N}}$
be a decreasing positive sequence such that
\begin{eqnarray*}\omega \,:\!=\, \limsup_{k\to \infty} \frac{\gamma_k^{\theta}-\gamma_{k+1}^{\theta}}{\gamma_{k+1}^{1+\theta}} <+\infty.\end{eqnarray*}
Let
$\omega<\rho= d^{2\alpha-4}2^{-d}\exp(-2^{d} d^{4-2\alpha})$
and let
$(v_{n})_{n\in \mathbb{N}}$
be the sequence defined by
$v_{0}=0$
and, for every
$n\geqslant1$
,
Then
Assume that n is large enough that
$t_{n}>1$
and let
$n^*=\max\{ i: t_n - t_i >1 \}$
. We further have
\begin{eqnarray}\sum_{i=n^*+1}^{n-1}(t_n-t_i)^{-\frac{1}{\alpha}} \gamma_i^{1+\theta}\leqslant C {\mathrm{e}}^{\rho(1+\gamma_{1})} \gamma_{n}^{\theta}\end{eqnarray}
for some constant
$C>0$
independent of d.
2.2. Proof of Theorem 1
It follows from (1.7) and (2.1) that
\begin{eqnarray}W_1(\mathcal{L}(X_{t_n}^x), \mathcal{L}(Y_{t_n}^x))&\,=\,& \text{supp}_{h\in {\rm Lip}(1)} \{ P_{0,t_n} h(x) - Q_{0,t_n} h(x) \}\nonumber\\&\leqslant& \sum_{i=1}^{n}\text{supp}_{h\in{\rm Lip}(1)}\left|Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_{i},t_n} h(x)\right|\nonumber\\&\,=\,& \sum_{i=1}^{n-1}\text{supp}_{h\in{\rm Lip}(1)}\left| Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}}-Q_{t_{i-1},t_{i}}) \circ P_{t_{i},t_n} h(x)\right|\nonumber\\&&+\: \text{supp}_{h\in{\rm Lip}(1)}\left| Q_{0,t_{n-1}} \circ (P_{t_{n-1},t_{n}}- Q_{t_{n-1},t_{n}})h(x)\right|.\end{eqnarray}
We first bound the last term in (2.11). Since
$h\in {\rm Lip}(1)$
, one can derive from the Markov property, (2.7) and (2.3) with
$\kappa=1$
that
\begin{align*}& \text{supp}_{h\in {\rm Lip}(1)} \left|Q_{0,t_{n-1}} \circ (P_{t_{n-1},t_{n}} -Q_{t_{n-1},t_{n}})h(x)\right|\nonumber\\&\quad = \text{supp}_{h\in {\rm Lip}(1)}\left|\mathbb{E}[h(X_{t_{n-1},t_{n}}^{Y_{t_{n-1}}^{x}})]-\mathbb{E}[h(Y_{t_{n-1},t_{n}}^{Y_{t_{n-1}}^{x}})]\right|\nonumber\\\end{align*}\begin{align} &\quad \leqslant\mathbb{E}\left|X_{t_{n-1},t_{n}}^{Y_{t_{n-1}}^{x}}-Y_{t_{n-1},t_{n}}^{Y_{t_{n-1}}^{x}}\right|\ \leqslant \ C d^{\frac{5}{2} } (1+\mathbb{E}|Y_{t_{n-1}}^{x}|)\gamma_{n}^{1+\frac{1}{\alpha}} \nonumber \\&\quad \leqslant Cd^{5}(1+|x|)\gamma_{n}^{1+\frac{1}{\alpha}}.\end{align}
For the first sum in (2.11), we use Lemma 6 and the Markov property to show that there exists a constant
$C>0$
independent of d such that for any
$x,y\in \mathbb{R}^d$
,
It follows from this, the Markov property, (2.7) and (2.3) that
\begin{align*}& \text{supp}_{h\in {\rm Lip}(1)} \left| Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) \right| \\&\quad = \text{supp}_{h\in {\rm Lip}(1)} \left|\mathbb{E}\left[P_{t_{i},t_{n}}h\left(X_{t_{i-1},t_{i}}^{Y_{t_{i-1}}^{x}}\right)\right]-\mathbb{E}\left[P_{t_{i},t_{n}}h\left(Y_{t_{i-1},t_{i}}^{Y_{t_{i-1}^{x}}}\right)\right]\right| \nonumber \\&\quad \leqslant C{\mathrm{e}}^{ d^{4-2\alpha} 2^{d}} \exp(-d^{2\alpha-4}2^{-d}{\mathrm{e}}^{-2^{d} d^{4-2\alpha}}(t_{n}-t_{i})) \mathbb{E}\left|X_{t_{i-1},t_{i}}^{Y_{t_{i-1}}^{x}}-Y_{t_{i-1},t_{i}}^{Y_{t_{i-1}^{x}}}\right|\\&\quad \leqslant C{\mathrm{e}}^{ d^{4-2\alpha} 2^{d}} \exp(-d^{2\alpha-4}2^{-d}{\mathrm{e}}^{-2^{d} d^{4-2\alpha}}(t_{n}-t_{i}))d^{\frac{5}{2}}\left(1+\mathbb{E}\left|Y_{t_{i-1}}^{x}\right|\right)\gamma_{i}^{1+\frac{1}{\alpha}}\\&\quad \leqslant C{\mathrm{e}}^{ d^{4-2\alpha} 2^{d}} \exp(-d^{2\alpha-4}2^{-d}{\mathrm{e}}^{-2^{d} d^{4-2\alpha}}(t_{n}-t_{i}))d^{5}\left(1+\left|x\right|\right)\gamma_{i}^{1+\frac{1}{\alpha}}.\end{align*}
Recall that
$\rho= d^{2\alpha-4}2^{-d} {\mathrm{e}}^{-2^{d} d^{4-2\alpha}}$
. We have
\begin{align*}&\sum_{i=1}^{n-1}\text{supp}_{h\in{\rm Lip}(1)}\left|Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_{i},t_n} h(x)\right|\\& \quad \leqslant C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5}(1+|x|)\sum_{i=1}^{n-1}{\mathrm{e}}^{-\rho(t_{n}-t_{i})}\gamma_{i}^{1+\frac{1}{\alpha}}\leqslant\frac{C}{\rho-\omega}{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_{1}}{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5} (1+|x|)\gamma_{n}^{\frac{1}{\alpha}},\end{align*}
where the last inequality follows from (2.8).
Combining all of the above, we deduce that there exists a constant
$C>0$
independent of d and n such that
This proves (1.11).
Now we prove (1.12). Notice that
\begin{eqnarray}W_{1}(\nu,\mathcal{L}(X_{t_n}^x))&\leqslant& \int_{\mathbb{R}^{d}}W_{1}(\mathcal{L}(X_{t_n}^x), \mathcal{L}(X_{t_n}^y))\nu(\mathrm{d} y)\nonumber\\&\leqslant& C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}{\mathrm{e}}^{-\rho t_{n}} \int_{\mathbb{R}^{d}}|x-y|\nu(\mathrm{d} y) \nonumber \\&\leqslant& C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}} d(1+|x|){\mathrm{e}}^{-\rho t_{n}},\end{eqnarray}
where the first inequality in (2.14) is from Lemma 6. Then, by (1.11) and (2.9),
\begin{align*}W_{1}(\nu, \mathcal{L}(Y_{t_n}^x)) &\leqslant W_{1}(\nu,\mathcal{L}(X_{t_n}^x))+W_{1}(\mathcal{L}(X_{t_n}^x), \mathcal{L}(Y_{t_n}^x))\\&\leqslant\frac{C}{\rho-\omega}{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1} {\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5}({\mathrm{e}}^{-\rho t_{n}}+\gamma_{n}^{\frac{1}{\alpha}}) (1+|x|) \\&\leqslant\frac{C}{\rho-\omega}{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1} {\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5}\gamma_{n}^{\frac{1}{\alpha}} (1+|x|).\end{align*}
The proof is complete.
2.3. Proof of Theorem 2
According to (2.11), we have
\begin{eqnarray}W_1(\mathcal{L}(X_{t_n}^x), \mathcal{L}(Y_{t_n}^x))&\leqslant& \sum_{i=1}^{n-1}\text{supp}_{h\in{\rm Lip}(1)}\left|Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_{i},t_n} h(x)\right| \nonumber \\&&+ \:\text{supp}_{h\in{\rm Lip}(1)}\left| Q_{0,t_{n-1}} \circ ( P_{t_{n-1},t_{n}} - Q_{t_{n-1},t_{n}} )h(x)\right|.\end{eqnarray}
For the first sum on the right-hand side of (2.15), we bound it as follows:
\begin{align} & \sum_{i=1}^{n-1} \text{supp}_{h\in{\rm Lip}(1)} \left| Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}}- Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) \right| \nonumber \\&\quad\leqslant \sum_{i=1}^{n^*} \text{supp}_{h\in{\rm Lip}(1)} \left| Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) \right| \nonumber \\&\qquad + \sum_{i=n^*+1}^{n-1} \text{supp}_{h\in{\rm Lip}(1)} \left| Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) \right| \nonumber \\&\quad=: \mathcal{R}_1 + \mathcal{R}_2,\end{align}
recalling that
$n^*=\max\{ i: t_n - t_i >1 \}$
.
Let us first give the estimate for
$\mathcal{R}_1$
, in which
$t_n-t_i>1$
. Recall that
$\rho= d^{2\alpha-4}2^{-d} {\mathrm{e}}^{-2^{d} d^{4-2\alpha}}$
; then one can derive from (2.13) that
\begin{align*}& \text{supp}_{h\in {\rm Lip}(1)} | Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) | \\&= \text{supp}_{h\in {\rm Lip}(1)} | Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_{i}+1} \circ P_{t_{i}+1,t_n} h(x) | \nonumber \\&= \text{supp}_{\{g=P_{t_{i}+1,t_n} h: h\in {\rm Lip}(1)\}} | Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_{i}+1} g(x) | \nonumber \\&\leqslant \text{supp}_{g\in {\rm Lip}(\ell)} | Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_{i}+1} g(x) | \nonumber \\&\leqslant C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}{\mathrm{e}}^{-\rho(t_{n}-t_{i}-1)} \text{supp}_{ g\in {\rm Lip}(1) } | Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_i+1} g(x)|,\end{align*}
where
$\ell=C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}{\mathrm{e}}^{-\rho(t_{n}-t_{i}-1)}$
and the first inequality follows from (2.13). Then, it follows from Lemmas 1, 3 and 5 that
\begin{align*}& \text{supp}_{h\in {\rm Lip}(1)} | Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) | \\&\quad\leqslant C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}{\mathrm{e}}^{-\rho(t_{n}-t_{i}-1)} d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}\\ &\qquad\times (1+|x|^{\kappa}) \text{supp}_{g\in {\rm Lip}(\ell)} (\| \nabla P_{t_i,t_i+1}g\|_{\infty} + \| \nabla^2 P_{t_i,t_i+1}g\|_{{\rm HS},\infty}) \gamma_i^{2+\frac{1}{\alpha}-\frac{1}{\kappa}}\nonumber \\&\quad\leqslant C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}{\mathrm{e}}^{-\rho(t_{n}-t_{i}-1)}d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}(1+|x|^{\kappa})\gamma_i^{2+\frac{1}{\alpha}-\frac{1}{\kappa}} ,\end{align*}
which implies that there exists a positive constant C independent of d and n such that
\begin{eqnarray}\mathcal{R}_1&\,=\,&\sum_{i=1}^{n^*}\text{supp}_{h\in{\rm Lip}(1)} \left|Q_{0,t_{i-1}} \circ (P_{t_{i-1},t_{i}}-Q_{t_{i-1},t_{i}}) \circ P_{t_i,t_n} h(x) \right| \nonumber \\&\leqslant& C{\mathrm{e}}^{d^{4-2\alpha} 2^{d}} d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}(1+|x|^{\kappa})\sum_{i=1}^{n^*} {\mathrm{e}}^{-\rho (t_{n}-t_{i}-1) } \gamma_i^{2+\frac{1}{\alpha}-\frac{1}{\kappa}} \nonumber \\&\leqslant&\frac{ C{\mathrm{e}}^{\rho}}{\rho-\omega}{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1} {\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}(1+|x|^{\kappa}) \gamma_{n}^{1+\frac{1}{\alpha}-\frac{1}{\kappa}},\end{eqnarray}
where the last inequality holds by (2.8).
For
$\mathcal{R}_2$
, it follows from Lemmas 1, 3, and 5 that
\begin{eqnarray}\mathcal{R}_2&\,=\,&\sum_{i=n^*+1}^{n-1} \text{supp}_{h\in{\rm Lip}(1)}\left| Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) \right| \nonumber \\&\leqslant& C {\mathrm{e}}^{\rho(1+\gamma_{1})} d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})} (1+|x|^{\kappa})\sum_{i=n^*+1}^{n-1}(t_n-t_i)^{-\frac{1}{\alpha}} \gamma_i^{2+\frac{1}{\alpha}-\frac{1}{\kappa}}\nonumber\\&\leqslant& C {\mathrm{e}}^{\rho(1+\gamma_{1})} d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}(1+|x|^{\kappa})\gamma_{n}^{1+\frac{1}{\alpha}-\frac{1}{\kappa}},\end{eqnarray}
where the constant C is independent of d and the last inequality is from (2.10). Hence, (2.16), (2.17) and (2.18) imply that
\begin{align}& \sum_{i=1}^{n-1} \text{supp}_{h\in{\rm Lip}(1)}\left| Q_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - Q_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) \right|\nonumber\\&\quad\leqslant\frac{C}{\rho-\omega}\,{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1} {\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}(1+|x|^{\kappa}) \gamma_{n}^{1+\frac{1}{\alpha}-\frac{1}{\kappa}}.\end{align}
In addition, the second term in (2.15) is directly obtained from (2.12); that is,
Therefore, there exists a positive constant C independent of d such that
This proves (1.15).
Now we prove (1.16). By (2.14), (1.15) and (2.9), we have
\begin{eqnarray*}W_{1}(\nu, \mathcal{L}(Y_{t_n}^x))&\leqslant& W_{1}(\nu,\mathcal{L}(X_{t_n}^x))+W_{1}(\mathcal{L}(X_{t_n}^x), \mathcal{L}(Y_{t_n}^x))\\&\leqslant&\frac{C}{\rho-\omega}\,{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1}{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})}({\mathrm{e}}^{-\rho t_{n}}+\gamma_{n}^{1+\frac{1}{\alpha}-\frac{1}{\kappa}}) (1+|x|^{\kappa}) \\&\leqslant&\frac{C}{\rho-\omega}\,{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1}{\mathrm{e}}^{d^{4-2\alpha} 2^{d}} d^{5\vee(3\kappa)\vee(4+\frac{3}{2\kappa}) \vee (\frac{3}{2}+\frac{3}{2\kappa}+\frac{3\kappa}{2})} \gamma_{n}^{1+\frac{1}{\alpha}-\frac{1}{\kappa}} (1+|x|^{\kappa}).\end{eqnarray*}
The proof is complete.
2.4. Proof of Theorem 3
By (2.15), we can write
\begin{eqnarray*}W_1(\mathcal{L}(X_{t_n}^x), \mathcal{L}(\tilde{Y}_{t_n}^x))&\leqslant&\sum_{i=1}^{n-1}\text{supp}_{h\in{\rm Lip}(1)}\left|\tilde{Q}_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - \tilde{Q}_{t_{i-1},t_{i}} ) \circ P_{t_{i},t_n} h(x)\right|\\&&+\:\text{supp}_{h\in{\rm Lip}(1)}\left|\tilde{Q}_{0,t_{n-1}} \circ ( P_{t_{n-1},t_{n}} - \tilde{Q}_{t_{n-1},t_{n}} )h(x)\right|,\end{eqnarray*}
and by the same argument as in the proof of (2.19) but with Lemma 3 replaced by Lemma 4, we have
\begin{align*}&\sum_{i=1}^{n-1} \text{supp}_{h\in{\rm Lip}(1)} \left|\tilde{Q}_{0,t_{i-1}} \circ ( P_{t_{i-1},t_{i}} - \tilde{Q}_{t_{i-1},t_{i}} ) \circ P_{t_i,t_n} h(x) \right|\\&\quad\leqslant\frac{C}{\rho-\omega}\,{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1}{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{\frac{5(1+\kappa)}{2\kappa}\vee(\frac{11-\alpha}{2})}(1+|x|) \gamma_{n}^{\frac{2-\alpha}{\alpha}}.\end{align*}
In addition, (2.4) and (2.6) give
\begin{align*}& \text{supp}_{h\in{\rm Lip}(1)}\left|\tilde{Q}_{0,t_{n-1}} \circ ( P_{t_{n-1},t_{n}} - \tilde{Q}_{t_{n-1},t_{n}} )h(x)\right|\\&\quad\leqslant \text{supp}_{h\in{\rm Lip}(1)}\left|\mathbb{E}\left[h\left(X_{t_{n-1},t_{n}}^{\tilde{Y}_{t_{n-1}}^{x}}\right)-h\left(\tilde{Y}_{t_{n-1}}^{x}\right)\right]\right|+ \text{supp}_{h\in{\rm Lip}(1)} \left|\mathbb{E}\left[h\left(\tilde{Y}_{t_{n-1},t_{n}}^{\tilde{Y}_{t_{n-1}}^{x}}\right)-h\left(\tilde{Y}_{t_{n-1}}^{x}\right)\right]\right|\\&\quad\leqslant \mathbb{E}\left|X_{t_{n-1},t_{n}}^{\tilde{Y}_{t_{n-1}}^{x}}-\tilde{Y}_{t_{n-1}}^{x}\right|+\mathbb{E}\left|\gamma_{n}b(\tilde{Y}_{t_{n-1}})+\frac{\gamma_{n}^{\frac{1}{\alpha}}}{\beta}A\tilde{Z}_{n}\right|\\&\quad\leqslant Cd^{\frac{5}{2}} \left(1+\mathbb{E}|\tilde{Y}_{t_{n-1}}^{x}|\right)\gamma_{n}^{\frac{1}{\alpha}}\ \leqslant \ Cd^{5} (1+|x|)\gamma_{n}^{\frac{1}{\alpha}}.\end{align*}
Combining the above, we obtain
This proves (1.17).
Next, we prove (1.18). By (2.14), (1.17) and (2.9), we have
\begin{eqnarray*}W_{1}(\nu, \mathcal{L}(\tilde{Y}_{t_n}^x))&\leqslant& W_{1}(\nu,\mathcal{L}(X_{t_n}^x))+W_{1}(\mathcal{L}(X_{t_n}^x), \mathcal{L}(\tilde{Y}_{t_n}^x))\\&\leqslant&\frac{C}{\rho-\omega}\,{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1}{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5}({\mathrm{e}}^{-\rho t_{n}}+\gamma_{n}^{\frac{2-\alpha}{\alpha}}) (1+|x|)\\&\leqslant&\frac{C}{\rho-\omega}\,{\mathrm{e}}^{\frac{\rho-\omega}{2}\gamma_1}{\mathrm{e}}^{d^{4-2\alpha} 2^{d}}d^{5}\gamma_{n}^{\frac{2-\alpha}{\alpha}} (1+|x|).\end{eqnarray*}
The proof is complete.
3. Proof of the auxiliary lemmas in Section 2
3.1. Proof of Lemma 1
For any
$\kappa \in [1,\alpha)$
, define
then
$|x|^{\kappa}\leqslant V_{\kappa}(x)\leqslant1+|x|^{\kappa}$
.
We first prove (2.2). Recall that the infinitesimal generator
$\mathcal{A}$
of the process
$(X_{t})_{t\geqslant 0}$
is
where
By Itô’s formula, (1.9) and the same argument as in the proof of (A.3) in [Reference Chen, Deng, Schilling and Xu6], we have
\begin{eqnarray*}\frac{\mathrm{d} \mathbb{E}\left[V_{\kappa}(X_{t}^{x})\right]}{\mathrm{d} t}&\,=\,&\mathbb{E}\left[\left\langle b\!\left(X_{t}^{x}\right),\nabla V_{\kappa}(X_{t}^{x})\right\rangle\right]+\mathbb{E}\left[\Delta^{\frac{\alpha}{2},A}V_{\kappa}(X_{t}^{x})\right]\\&\leqslant&-\frac{\theta_{1}}{2}\mathbb{E}\left[V_{\kappa}(X_{t}^{x})\right]+C_{1},\end{eqnarray*}
where
\begin{align*}C_{1}&=\theta_{1}\kappa+\kappa K+\theta_{1}^{1-\kappa}|b(0)|^{\kappa}\\&\quad+\frac{d_{\alpha}\kappa(3-\kappa)\sqrt{d}\sigma_{d-1}}{2(2-\alpha)}\|A\|_{{\rm op}}^{2}+\frac{d_{\alpha}\kappa\sigma_{d-1}}{\alpha-\kappa}\|A\|_{{\rm op}}^{\kappa}+\left(\frac{\theta_{1}}{4}\right)^{1-\kappa}\left(\frac{d_{\alpha}\sigma_{d-1}}{\alpha-1}\|A\|_{{\rm op}}\right)^{\kappa}.\end{align*}
This inequality, together with
$X_{0}=x$
, implies
Hence, the desired result follows from the fact that
for some constant
$C>0$
, which is independent of d.
For the remaining two inequalities, we only give the proof of (2.3). Inequality (2.4) can be proved in the same way.
By Assumption 1 and the same argument as in the proof of Lemma 1.8 in [Reference Chen, Deng, Schilling and Xu6], we have
where
\begin{align*}C_{2}&=\frac{\theta_{1}\kappa}{2} \left(\frac{2\gamma_{n+1}|b(0)|^{2}}{\theta_{1}}+2\gamma_{n+1}^{2}|b(0)|^{2}+1+2\gamma_{n+1} K\right)+ \frac{\kappa |b(0)|^{2}}{\theta_{1}}+2\kappa \gamma_{n+1} |b(0)|^{2}\\&\quad+\kappa K+d_{\alpha}\kappa\sigma_{d-1}\left(\frac{(3-\kappa)\sqrt{d}}{2(2-\alpha)}\|A\|_{{\rm op}}^{2}+\frac{1}{\alpha-\kappa}\|A\|_{{\rm op}}^{\kappa}+\frac{|b(0)|^{\kappa-1}}{\alpha-1}\|A\|_{{\rm op}}\right)\\&\quad+d_{\alpha}\kappa\sigma_{d-1}\frac{\mathbb{E}|Z_{1}|^{\kappa-1}}{\alpha-1}\|A\|_{{\rm op}}+\left(\frac{d_{\alpha}\sigma_{d-1}(1+ L^{\kappa-1})}{\alpha-1}\|A\|_{{\rm op}}\right)^{\kappa}\left(\frac{2}{\theta_{1}}\right)^{\kappa-1}.\end{align*}
By induction, we further have
\begin{align*}\mathbb{E}\left[V_{\kappa}(Y_{t_{n+1}}^{x})\right]&\leqslant\prod_{i=1}^{n+1}\left(1-\frac{\theta_{1}}{2}\gamma_{i}\right)V_{\kappa}(x)+C_{2}\sum_{i=1}^{n+1}\prod_{j=i+1}^{n+1}\left(1-\frac{\theta_{1}}{2}\gamma_{j}\right)\gamma_{i}\\&\leqslant V_{\kappa}(x)+C_{2}\sum_{i=1}^{n+1}\prod_{j=i+1}^{n+1}\left(1-\frac{\theta_{1}}{2}\gamma_{j}\right)\gamma_{i},\end{align*}
where we have used the convention that
$\prod_{j=n+2}^{n+1}\left(1-\frac{\theta_{1}}{2}\gamma_{j}\right)=1$
. In addition,
\begin{align*}\frac{\theta_{1}}{2}\sum_{i=1}^{n+1}\prod_{j=i+1}^{n+1}\left(1-\frac{\theta_{1}}{2}\gamma_{j}\right)\gamma_{i}=1-\prod_{j=1}^{n+1}\left(1-\frac{\theta_{1}}{2}\gamma_{j}\right)\leqslant 1,\end{align*}
which implies
Since
$V_{\kappa}(x)\leqslant1+|x|^{\kappa}$
, the desired result follows from the fact that
for some constant
$C>0$
, which is independent of d.
3.2. Proof of Lemma 2
The first inequality follows immediately from
\begin{align*}\mathbb{E} |Y_{t_{n-1},t_{n}}^{x}-x|^{\kappa}&= \mathbb{E}\left|\gamma_{n} b(x) + A\left(Z_{t_{n}}-Z_{t_{n-1}}\right)\right|^{\kappa}\\&\leqslant 2\left[\gamma_{n}^{\kappa}|b(x)|^{\kappa}+\|A\|_{{\rm op}}^{\kappa} \mathbb{E}|Z_{\gamma_{n}}|^{\kappa}\right]\leqslant Cd^{\kappa}(1+|x|^{\kappa})\gamma_{n}^{\frac{\kappa}{\alpha}}.\end{align*}
By Hölder’s inequality and (2.2), we obtain
\begin{eqnarray*}\mathbb{E}|X_{s,t}^{x}-x|^{\kappa}&\,=\,&\mathbb{E}\left|\int_{s}^{t}b\!\left(X_{s,r}^{x}\right)\mathrm{d} r+A\left(Z_{t}-Z_{s}\right)\right|^{\kappa}\\&\leqslant& 2\mathbb{E}\left|\int_{s}^{t}b\!\left(X_{s,r}^{x}\right)\mathrm{d} r\right|^{\kappa}+2\|A\|_{{\rm op}}^{\kappa}|Z_{t-s}|^{\kappa}\\&\leqslant & 2(t-s)^{\kappa-1}\int_{s}^{t}\mathbb{E}\left|b\!\left(X_{s,r}^{x}\right)\right|^{\kappa}\,\mathrm{d} r+2d^{\frac{\kappa}{2}}\mathbb{E}|Z_{1}|^{\kappa}(t-s)^{\frac{\kappa}{\alpha}}\\&\leqslant & Cd^{\frac{5\vee(3\kappa)}{2}}(1+|x|^{\kappa})(t-s)^{\frac{\kappa}{\alpha}},\end{eqnarray*}
which implies the second inequality.
For the last inequality, notice that
$\gamma_{n}=t_{n}-t_{n-1}$
, Hölder’s inequality, (1.13) and (2.6) imply
\begin{eqnarray*}\mathbb{E} |X_{t_{n-1},t_{n}}^{x}-Y_{t_{n-1},t_{n}}^{x}|^{\kappa}&\,=\,&\mathbb{E} \left|\int_{t_{n-1}}^{t_{n}}\left[b\!\left(X_{t_{n-1},s}^{x}\right)-b(x)\right]\mathrm{d} s\right|^{\kappa}\\&\leqslant& \gamma_{n}^{\kappa-1}\int_{t_{n-1}}^{t_{n}}\mathbb{E}\left|b\!\left(X_{t_{n-1},s}^{x}\right)-b(x)\right|^{\kappa}\,\mathrm{d} s\\&\leqslant& L\gamma_{n}^{\kappa-1}\int_{t_{n-1}}^{t_{n}}\mathbb{E}\left|X_{t_{n-1},s}^{x}-x\right|^{\kappa}\,\mathrm{d} s\\&\leqslant & Cd^{\frac{5\vee(3\kappa)}{2}}(1+|x|^{\kappa})\gamma_{n}^{\kappa-1}\int_{t_{n-1}}^{t_{n}}(s-t_{n-1})^{\frac{\kappa}{\alpha}}\,\mathrm{d} s\\&\,=\,& Cd^{\frac{5\vee(3\kappa)}{2}}(1+|x|^{\kappa})\gamma_{n}^{\kappa+\frac{\kappa}{\alpha}}.\end{eqnarray*}
The proof is complete.
3.3. Proof of Lemma 3
By the Taylor expansion formula, we have
\begin{align*}& \mathbb{E} f\!\left(X_{t_{k-1},t_{k}}^{x}\right)-\mathbb{E} f\!\left(Y_{t_{k-1},t_{k}}^{x}\right)\\&\quad=\mathbb{E}\left\langle\nabla f\!\left(Y_{t_{k-1},t_{k}}^{x}\right),X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right\rangle\\&\qquad+\mathbb{E}\int_{0}^{1}\!\!\left\langle\nabla f\!\left(Y_{t_{k-1},t_{k}}^{x}+r\left(X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right)\right)\!-\!\nabla f\!\left(Y_{t_{k-1},t_{k}}^{x}\right),X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right\rangle\,\mathrm{d} r\\&\quad=:\mathcal{I}+\mathcal{II}+\mathcal{III},\end{align*}
where
\begin{align*}\mathcal{I}&=\mathbb{E}\left\langle\nabla f\!\left(x+\gamma_{k}b(x)+A(Z_{t_{k}}-Z_{t_{k-1}})\right)-\nabla f\!\left(x+\gamma_{k}b(x)\right),X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right\rangle, \\\mathcal{II}&=\mathbb{E}\left\langle\nabla f\!\left(x+\gamma_{k}b(x)\right),X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right\rangle, \\\mathcal{III}&=\mathbb{E}\int_{0}^{1}\left\langle\nabla f\!\left(Y_{t_{k-1},t_{k}}^{x}+r\left(X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right)\right)-\nabla f\!\left(Y_{t_{k-1},t_{k}}^{x}\right),X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right\rangle\mathrm{d} r.\end{align*}
We divide the first term,
$\mathcal{I}$
, into two parts as follows:
\begin{align*} \mathcal{I} &=\mathbb{E}\left[\left\langle\nabla f\!\left(x+\gamma_{k}b(x)+A(Z_{t_{k}}-Z_{t_{k-1}})\right)-\nabla f\!\left(x+\gamma_{k}b(x)\right),X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right\rangle\right.\\ &\left.\qquad\qquad\qquad\qquad\times\left({\bf 1}_{(0,1]}(|Z_{t_{k}}-Z_{t_{k-1}}|)+{\bf 1}_{(1,\infty)}(|Z_{t_{k}}-Z_{t_{k-1}}|)\right)\right]\\ & =:\mathcal{I}_{1}+\mathcal{I}_{2}.\end{align*}
According to [Reference Chen, Nourdin, Xu and Yang7, Lemma 18], it is straightforward to derive the following estimates:
\begin{align*}\mathbb{P}\!\left(|Z_{\gamma_{k}}| > 1\right) &\leqslant C\pi^{-\frac{d}{2}}\Gamma\!\left(\frac{d+\alpha}{2}\right)\int_{|z|\geqslant\gamma_{k}^{-\frac{1}{\alpha}}}\frac{1}{|z|^{\alpha+d}}\,\mathrm{d} z\\&\leqslant C\pi^{-\frac{d}{2}}\Gamma\!\left(\frac{d+\alpha}{2}\right)\sigma_{d-1}\int_{\gamma_{k}^{-\frac{1}{\alpha}}}^{\infty}\frac{1}{r^{\alpha+1}}\,\mathrm{d} r\leqslant C\frac{\Gamma\!\left(\frac{d+\alpha}{2}\right)}{\Gamma\!\left(\frac{d}{2}\right)}\gamma_{k}\leqslant Cd\gamma_{k}\end{align*}
and, for any
$\lambda>\alpha$
,
\begin{align*}\mathbb{E}\left[|Z_{\gamma_{k}}|^\lambda \textbf{1}_{(0,1]}(|Z_{\gamma_{k}}|)\right]&\leqslant C\pi^{-\frac{d}{2}}\Gamma\!\left(\frac{d+\alpha}{2}\right)\gamma_{k}^{\frac{\lambda}{\alpha}}\int_{|z|\leqslant\gamma_{k}^{-\frac{1}{\alpha}}}\frac{|z|^{\lambda}}{|z|^{\alpha+d}}\,\mathrm{d} z\\&\leqslant C\pi^{-\frac{d}{2}}\Gamma\!\left(\frac{d+\alpha}{2}\right)\sigma_{d-1}\gamma_{k}^{\frac{\lambda}{\alpha}}\int_{0}^{\gamma_{k}^{-\frac{1}{\alpha}}}\frac{r^{\lambda}}{r^{\alpha+1}}\,\mathrm{d} r\\&\leqslant C\frac{\Gamma\!\left(\frac{d+\alpha}{2}\right)}{\Gamma\!\left(\frac{d}{2}\right)}\gamma_{k}\leqslant Cd\gamma_{k}.\end{align*}
Since
$\frac{\kappa}{\kappa-1} > \alpha$
, we can use Hölder’s inequality and (2.7) to get
\begin{align*} |\mathcal{I}_{1}| &\leqslant \|\nabla^{2}f\|_{\mathrm{HS},\infty}\|A\|_{{\rm op}}\mathbb{E}\left[|Z_{t_{k}}-Z_{t_{k-1}}|{\bf 1}_{(0,1]}(|Z_{t_{k}}-Z_{t_{k-1}}|)\left|X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right|\right]\\ &\leqslant\|\nabla^{2}f\|_{\mathrm{HS},\infty}\sqrt{d} \left(\mathbb{E}\left[|Z_{\gamma_{k}}|^{\frac{\kappa}{\kappa-1}}{\bf 1}_{(0,1]}(|Z_{\gamma_{k}}|)\right]\right)^{\frac{\kappa-1}{\kappa}} \left(\mathbb{E}\left|X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right|^{\kappa}\right)^{\frac{1}{\kappa}}\\ &\leqslant C (1+|x|)\|\nabla^{2}f\|_{\mathrm{HS},\infty} d^{(\frac{3}{2}+\frac{3}{2\kappa})\vee (3-\frac{1}{\kappa})} \gamma_{k}^{2+\frac{1}{\alpha}-\frac{1}{\kappa}},\end{align*}
and Hölder’s inequality gives
\begin{align*} |\mathcal{I}_{2}| &\leqslant2\|\nabla f\|_{\infty} \mathbb{E}\left[{\bf 1}_{(1,\infty)}(|Z_{t_{k}}-Z_{t_{k-1}}|)\left|X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right|\right]\\ &\leqslant2\|\nabla f\|_{\infty} \left(\mathbb{E}{\bf 1}_{(1,\infty)}(|Z_{\gamma_{k}}|)\right)^{\frac{\kappa-1}{\kappa}} \left(\mathbb{E}\left|X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right|^{\kappa}\right)^{\frac{1}{\kappa}}\\ &\leqslant C (1+|x|) \|\nabla f\|_{\infty}d^{(1+\frac{3}{2\kappa})\vee (\frac{5}{2}-\frac{1}{\kappa})}\gamma_{k}^{\frac{\kappa-1}{\kappa}}\gamma_{k}^{1+\frac{1}{\alpha}}.\end{align*}
Hence, we have
For
$\mathcal{II}$
, one can deduce from (1.1), (1.3), Itô’s formula and (3.2) that
\begin{align*} |\mathcal{II}| &=\left|\mathbb{E}\left\langle\nabla f\!\left(x+\gamma_{k} b(x)\right),\int_{t_{k-1}}^{t_{k}}\left[b(X_{t_{k-1},s}^{x})-b(x)\right] \mathrm{d} s\right\rangle\right|\\ &=\left|\left\langle\nabla f\!\left(x+\gamma_{k} b(x)\right),\int_{t_{k-1}}^{t_{k}}\mathbb{E}\left[b(X_{t_{k-1},s}^{x})-b(x)\right] \mathrm{d} s\right\rangle\right|\\ &=\left|\left\langle\nabla f\!\left(x+\gamma_{k} b(x)\right),\int_{t_{k-1}}^{t_{k}}\int_{t_{k-1}}^{s}\mathbb{E}\left[\mathcal{L}b(X_{t_{k-1},r}^{x})\right] \mathrm{d} r\,\mathrm{d} s\right\rangle\right|\\ &\leqslant C\|\nabla f\|_{\infty} (1+|x|)d^{\frac{5\vee(3\kappa)}{2}} \int_{t_{k-1}}^{t_{k}}(s-t_{k-1})\,\mathrm{d} s \nonumber \\ &\leqslant C\|\nabla f\|_{\infty} (1+|x|)d^{\frac{5\vee(3\kappa)}{2}}\gamma_{k}^{2},\end{align*}
where the second-to-last inequality is from (1.13), the moment estimate (2.2) and the inequality
\begin{eqnarray*}\left|\mathbb{E}\left[\mathcal{L}b(X_{t_{k-1},r}^{x})\right]\right|&\leqslant&\mathbb{E}\left[\left|\nabla b(X_{t_{k-1},r}^{x})\right|\left|b(X_{t_{k-1},r}^{x})\right|\right]+\mathbb{E}\left|\Delta^{\frac{\alpha}{2},A}b(X_{t_{k-1},r}^{x})\right|\\&\leqslant&C\left[1+\mathbb{E}\left|X_{t_{k-1},r}^{x}\right|+d_{\alpha}\sigma_{d-1}(\sqrt{d}\|A\|_{{\rm op}}^{2}+\|A\|_{{\rm op}})\right]\\&\leqslant& C(1+|x|)d^{\frac{5\vee(3\kappa)}{2}},\end{eqnarray*}
which is proved by the same argument as in the proof of (A.2) in [Reference Chen, Deng, Schilling and Xu6].
Finally, by [Reference Chen, Deng, Schilling and Xu6, Lemma 2.6] and (2.7), we have
\begin{align*} \mathcal{III} &\leqslant C\left(\|\nabla f\|_{\infty}+\|\nabla^{2}f\|_{\mathrm{HS},\infty}\right)\mathbb{E}\left|X_{t_{k-1},t_{k}}^{x}-Y_{t_{k-1},t_{k}}^{x}\right|^{\kappa}\\ &\leqslant C (1+|x|^{\kappa}) \left(\|\nabla f\|_{\infty}+\|\nabla^{2}f\|_{\mathrm{HS},\infty}\right) d^{\frac{5\vee(3\kappa)}{2}} \gamma_{k}^{\kappa+\frac{\kappa}{\alpha}}.\end{align*}
This finishes the proof.
3.4. Proof of Lemma 4
Before proving Lemma 4, we first present the following lemma.
Lemma 8 Let
$\alpha\in(1,2)$
and let
$\Delta^{\frac{\alpha}{2},A}$
be defined by (3.3). Then, for any
$f:\mathbb{R}^{d}\to \mathbb{R}$
satisfying
$\|\nabla f\|_{\infty}<\infty$
and
$\|\nabla^{2}f\|_{\mathrm{HS},\infty}<\infty$
, we have
Proof. According to (3.3) and the symmetry of the Lebesgue measure, for any
$R>0$
we have
\begin{align*}\Delta^{\frac{\alpha}{2},A}f(x)& =d_{\alpha}\int_{\mathbb{S}^{d-1}}\int_{0}^{\infty}\frac{f(x+Ar\theta)-f(x)-Ar\left\langle\theta,\nabla f(x)\right\rangle{\bf 1}_{(0,R)}(r)}{r^{\alpha+1}}\,\mathrm{d} r\,\mathrm{d}\theta\\&= d_{\alpha}\int_{\mathbb{S}^{d-1}} \int_{0}^{R}\int_{0}^{r}\frac{\left\langle A\theta,\nabla f(x+A\theta s)-\nabla f(x)\right\rangle}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d} \theta\\ &\quad\mbox{}+d_{\alpha}\int_{\mathbb{S}^{d-1}} \int_{R}^{\infty}\int_{0}^{r}\frac{\left\langle A\theta,\nabla f(x+A\theta s)\right\rangle}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d} \theta.\end{align*}
Then, for all
$x,y\in\mathbb{R}^{d}$
,
\begin{align}& \big|\Delta^{\frac{\alpha}{2},A}f(x) -\Delta^{\frac{\alpha}{2},A}f(y)\big| \nonumber\\&\quad\leqslant d_{\alpha}\|A\|_{{\rm op}}\int_{\mathbb{S}^{d-1}} \int_{0}^{R}\int_{0}^{r}\frac{\left|\nabla f(x+A\theta s)-\nabla f(x)-\nabla f(y+A\theta s)+\nabla f(y)\right|}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d} \theta \nonumber\\&\qquad+d_{\alpha}\|A\|_{{\rm op}}\int_{\mathbb{S}^{d-1}} \int_{R}^{\infty}\int_{0}^{r}\frac{\left|\nabla f(x+A\theta s)-\nabla f(y+A\theta s)\right|}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d} \theta.\end{align}
For the first integral in (3.6), we have
\begin{align*}& \int_{\mathbb{S}^{d-1}} \int_{0}^{R}\int_{0}^{r}\frac{\left|\nabla f(x+A\theta s)-\nabla f(x)-\nabla f(y+A\theta s)+\nabla f(y)\right|}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d} \theta\\&\quad\leqslant \int_{\mathbb{S}^{d-1}} \int_{0}^{R}\int_{0}^{r}\frac{\left|\nabla f(x+A\theta s)-\nabla f(x)\right|+\left|\nabla f(y+A\theta s)-\nabla f(y)\right|}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d} \theta\\&\quad\leqslant 2\|\nabla^{2}f\|_{\mathrm{HS},\infty}\|A\|_{{\rm op}}\int_{\mathbb{S}^{d-1}} \int_0^R \int_{0}^{r}\frac{s}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d}\theta\ = \ \frac{\|\nabla^{2}f\|_{\mathrm{HS},\infty}\|A\|_{{\rm op}}\sigma_{d-1}}{2-\alpha}\,R^{2-\alpha}.\end{align*}
For the second integral in (3.6), we have
\begin{align*}&\int_{\mathbb{S}^{d-1}} \int_{R}^{\infty}\int_{0}^{r}\frac{\left|\nabla f(x+A\theta s)-\nabla f(y+A\theta s)\right|}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d} \theta\\&\quad\leqslant \|\nabla^{2}f\|_{\mathrm{HS},\infty}\|A\|_{{\rm op}}\int_{\mathbb{S}^{d-1}}\int_{R}^{\infty}\int_{0}^{r}\frac{|x-y|}{r^{\alpha+1}}\,\mathrm{d} s\,\mathrm{d} r\,\mathrm{d}\theta\\&\quad= \frac{\|\nabla^{2}f\|_{\mathrm{HS},\infty}\|A\|_{{\rm op}}\sigma_{d-1}}{\alpha-1}\,|x-y|R^{1-\alpha}.\end{align*}
Hence, the assertion follows upon taking
$R=|x-y|$
.
Now, we proceed to prove Lemma 4.
Proof of Lemma 4. From (1.1) and (1.5), we see that
\begin{align*}&\mathbb{E} [f(X_{t_{k-1},t_{k}}^{x})-f(\tilde{Y}_{t_{k-1},t_{k}}^{x})]\\&\quad=\mathbb{E} \left[f\!\left(x+\int_{t_{k-1}}^{t_{k}}b(X_{t_{k-1},r}^{x})\,\mathrm{d} r +A(Z_{t_{k}}-Z_{t_{k-1}})\right)- f\!\left(x+\gamma_{k}b(x) +\frac{\gamma_{k}^{\frac{1}{\alpha}}}{\beta}A\tilde{Z}\right)\right]\\&\quad=\mathcal{J}_{1}+\mathcal{J}_{2},\end{align*}
where
and
\begin{align*}\mathcal{J}_{2}&\,:\!=\, \mathbb{E} \left[f\!\left(x+\gamma_{k}b(x)+AZ_{\gamma_{k}}\right)-f\!\left(x+\gamma_{k} b(x)\right)\right]\\&\quad -\mathbb{E} \left[f\!\left(x+\gamma_{k} b(x)+\frac{\gamma_{k}^{\frac{1}{\alpha}}}{\beta} A\tilde{Z}\right)-f\!\left(x+\gamma_{k} b(x)\right)\right].\end{align*}
We can bound
$\mathcal{J}_{1}$
by using (2.6) with
$\kappa=1$
:
\begin{align*}|\mathcal{J}_{1}|&\leqslant\|\nabla f\|_{\infty}\mathbb{E} \left|\int_{t_{k-1}}^{t_{k}}b(X_{t_{k-1},r}^{x})\,\mathrm{d} r-\gamma_{k} b(x)\right|\\&\leqslant\|\nabla f\|_{\infty}\int_{t_{k-1}}^{t_{k}}\mathbb{E} |b(X_{t_{k-1},r}^{x})-b(x)|\,\mathrm{d} r\\&\leqslant L\|\nabla f\|_{\infty}\int_{t_{k-1}}^{t_{k}}\mathbb{E} |X_{t_{k-1},r}^{x}-x|\,\mathrm{d} r\\&\leqslant C(1+|x|)\|\nabla f\|_{\infty}d^{\frac{5}{2\kappa} \vee \frac{3}{2}} \int_{t_{k-1}}^{t_{k}}(r-t_{k-1})^{\frac{1}{\alpha}}\,\mathrm{d} r \\&\leqslant C(1+|x|)\| \, \nabla f\|_{\infty}d^{\frac{5}{2\kappa} \vee \frac{3}{2}} \gamma_{k}^{1+\frac{1}{\alpha}}.\end{align*}
For the first term of
$\mathcal{J}_{2}$
, we use Dynkin’s formula (see e.g. [Reference Chen and Xu8]) to get
For the second part of
$\mathcal{J}_{2}$
, observing that
$d_{\alpha}= \alpha \sigma_{d-1}^{-1} \beta^{-\alpha}$
, Taylor’s formula implies that
\begin{align*}& \mathbb{E}\left[f\!\left(x+\gamma_{k} b(x)+\frac{\gamma_{k}^{\frac{1}{\alpha}}}{\beta}A\tilde{Z}\right)-f\big(x+\gamma_{k} b(x)\big)\right]\\&\quad= \frac{\gamma_{k}^{\frac{1}{\alpha}}}{\beta}\mathbb{E}\left[\int_{0}^{1}\left\langle\nabla f\!\left(x+\gamma_{k} b(x)+\frac{\gamma_{k}^{\frac{1}{\alpha}}}{\beta}tA\tilde{Z}\right),\: A\tilde{Z}\right\rangle \mathrm{d} t\right]\\&\quad= \frac{\gamma_{k}^{\frac{1}{\alpha}}}{\beta} \int_{|z|\geqslant1} \int_{0}^{1} \alpha \left\langle\nabla f\big(x+\gamma_{k} b(x)+\frac{\gamma_{k}^{\frac{1}{\alpha}}} {\beta}tAz\big),\: Az\right\rangle \frac{\mathrm{d} t\,\mathrm{d} z}{\sigma_{d-1} |z|^{\alpha+d}}\\&\quad= \frac{\alpha\gamma_{k}}{\sigma_{d-1} \beta^{\alpha}}\int_{|z|\geqslant\beta^{-1}\gamma_{k}^{\frac{1}{\alpha}}}\int_{0}^{1}\left\langle\nabla f\big(x+\gamma_{k} b(x)+tAz\big),\:Az\right\rangle \frac{\mathrm{d} t\,\mathrm{d} z}{|z|^{\alpha+d}}\\&\quad= \gamma_{k}\Delta^{\frac{\alpha}{2},A}f(x+\gamma_{k} b(x))-\mathcal{R},\end{align*}
where
Together, the above estimates yield
Further, we have
\begin{eqnarray*}|\mathcal{R}|&\,=\,& \gamma_{k}d_{\alpha} \left|\int_{|z|<\beta^{-1}\gamma_{k}^{\frac{1}{\alpha}}}\int_{0}^{1} \left\langle\nabla f\big(x+\gamma_{k} b(x)+tAz\big)-\nabla f\big(x+\gamma_{k} b(x)\big),\: Az\right\rangle \frac{\mathrm{d} t\,\mathrm{d} z}{|z|^{\alpha+d}} \right|\\&\leqslant& d_{\alpha} \|A\|_{{\rm op}}\gamma_{k}\int_{|z|<\beta^{-1}\gamma_{k}^{\frac{1}{\alpha}}}\int_{0}^{1} \left|\nabla f\big(x+\gamma_{k} b(x)+tAz\big)-\nabla f\big(x+\gamma_{k} b(x)\big)\right| \frac{\mathrm{d} t\,\mathrm{d} z}{|z|^{\alpha+d-1}}\\&\leqslant& C\|\nabla^{2}f\|_{\mathrm{HS},\infty} d_{\alpha} \|A\|_{{\rm op}}^{2}\gamma_{k}\int_{|z|<\beta^{-1}\gamma_k^{\frac{1}{\alpha}}} \frac{\mathrm{d} z}{|z|^{\alpha+d-2}}\\&\leqslant& C\|\nabla^{2}f\|_{\mathrm{HS},\infty} d_{\alpha}\sigma_{d-1} \|A\|_{{\rm op}}^{2}\gamma_{k}^{\frac{2}{\alpha}}\leqslant C\|\nabla^{2}f\|_{\mathrm{HS},\infty}d^{2}\gamma_{k}^{\frac{2}{\alpha}}.\end{eqnarray*}
By Lemma 8, we also have
\begin{align*}&\left|\int_{0}^{\gamma_{k}}\mathbb{E}\left[\Delta^{\frac{\alpha}{2},A}f\big(x+\gamma_{k} b(x)+Z_{r}\big)\right] \mathrm{d} r- \gamma_{k}\Delta^{\frac{\alpha}{2},A}f(x+\gamma_{k} b(x))\right|\\&\quad\leqslant \int_{0}^{\gamma_{k}}\mathbb{E}\left|\Delta^{\frac{\alpha}{2},A}f\big(x+\gamma_{k} b(x)+Z_{r}\big)\big] -\Delta^{\frac{\alpha}{2},A}f(x+\gamma_{k} b(x))\right| \mathrm{d} r\\&\quad\leqslant C\|\nabla^{2}f\|_{\mathrm{HS},\infty}d^{2}\int_{0}^{\gamma_{k}}\mathbb{E}\left[|Z_{r}|^{2-\alpha}\right] \mathrm{d} r\\&\quad= C\|\nabla^{2}f\|_{\mathrm{HS},\infty}d^{2}\int_{0}^{\gamma_{k}}\mathbb{E}\left[|Z_{1}|^{2-\alpha}\right] r^{\frac{2}{\alpha}-1}\,\mathrm{d} r \leqslant C \|\nabla^{2}f\|_{\mathrm{HS},\infty}d^{3-\frac{\alpha}{2}} \,\gamma_{k}^{\frac{2}{\alpha}}.\end{align*}
Combining all the estimates finishes the proof.
3.5. Proof of Lemma 6
In this section, we prove Lemma 6 under a more general condition. Consider
where the drift coefficient b is assumed to satisfy the following condition: there exist positive constants
$K_1,\,K_2$
and
$L_0$
, all independent of the dimension d, such that
It is easy to verify that Assumption 1 satisfies this condition. The corresponding generator
$\mathcal{L}$
for process
$(X_t)_{t\geqslant 0}$
is defined as
where
$\alpha\in(1,2)$
. In addition, there exists a positive constant
$\Lambda \asymp d^{\frac{1}{2}}$
with
$\Lambda \geqslant 1$
such that
We shall use [Reference Liang and Wang27] to prove the contraction property in the lemma under the condition (3.8). Let us first recall some notation from [Reference Liang and Wang27]. For some sufficiently small constant
$\tau \leqslant \frac{1}{32 \Lambda^5} \wedge L_0$
with
$L_0$
and
$\Lambda$
as above, for any
$x,y \in \mathbb{R}^d$
define
and for any
$z\in \mathbb{R}^d$
let
$\Psi: \mathbb{R}^d \to \mathbb{R}^d$
be a continuous and bijective mapping defined by
then the inverse function
$\Psi^{-1}$
is given by
Let the measure
$\pi_0(\mathrm{d} z)$
be related to the Lévy measure
$\pi(\mathrm{d} z)$
and satisfy
$0\leqslant \pi_0(\mathrm{d} z) \leqslant \pi(\mathrm{d} z)$
and
$\int_{\mathbb{R}^d} |z|^2 \pi_0(\mathrm{d} z)<\infty.$
For any integers
$n\geqslant 1$
, define
where
$\pi_{0,n}(B)=\int_{B\cap \{|z|>\frac{1}{n}\} }\pi_0(\mathrm{d} z)$
and
$(\pi_{0,n}\Psi)(B)=\pi_{0,n}(\Psi(B))$
for all Borel-measurable sets
$B\in \mathcal{B}(\mathbb{R}^d)$
.
For the solution
$(X_t)_{t\geqslant 0}$
of the SDE (3.7) and its operator
$\mathcal{L}$
, it follows from [Reference Liang and Wang27, Theorem 2.3 and Proposition 2.6] that there exist the coupling process for
$(X_t)_{t\geqslant 0}$
and the coupling operator
$\widetilde{\mathcal{L}}$
defined as follows: for any
$h\in \mathcal{C}_b^2(\mathbb{R}^d \times \mathbb{R}^d)$
and
$x,y\in \mathbb{R}^d$
,
\begin{eqnarray*}\widetilde{\mathcal{L}} h(x,y)&\,=\,& \langle \nabla_x h(x,y),b(x) \rangle+\langle \nabla_y h(x,y),b(y) \rangle \\&& +\:\frac{1}{2} \int_{ \mathbb{R}^d \setminus \{ 0 \} } ( h(x+ Az,y+A \Psi(z))-h(x,y)-\langle \nabla_x h(x,y),A z \rangle 1_{\{ |z|\leqslant 1 \} } \\&& \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ -\:\langle \nabla_y h(x,y), A \Psi(z) \rangle 1_{ \{ |\Psi(z)| \leqslant 1 \} } ) \mu_{\pi_0,\Psi}(\mathrm{d} z) \\&& +\:\frac{1}{2} \int_{ \mathbb{R}^d \setminus \{ 0 \} } ( h(x+A z,y+A \Psi^{-1}(z))-h(x,y)-\langle \nabla_x h(x,y),A z \rangle 1_{\{ |z|\leqslant 1 \} } \\&& \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ -\:\langle \nabla_y h(x,y), A \Psi^{-1}(z) \rangle 1_{ \{ |\Psi^{-1}(z)| \leqslant 1 \} } ) \mu_{\pi_0,\Psi^{-1}}(\mathrm{d} z) \\&&+ \:\int_{ \mathbb{R}^d \setminus \{ 0 \} } ( h(x+A z,y+A z)-h(x,y)-\langle \nabla_x h(x,y),A z \rangle 1_{\{ |z|\leqslant 1 \} } \\&& \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ -\:\langle \nabla_y h(x,y), A z \rangle 1_{ \{ |z| \leqslant 1 \} } ) \left[ \pi- \frac{1}{2}\mu_{\pi_0,\Psi} -\frac{1}{2}\mu_{\pi_0,\Psi^{-1}} \right](\mathrm{d} z),\end{eqnarray*}
where
$\nabla_x$
and
$\nabla_y$
denote the gradients with respect to variables x and y, respectively.
Let
$\pi_0(\mathrm{d} z) = q(z) \,\mathrm{d} z$
and
$(\pi_0 \Psi^{-1})(\mathrm{d} z) = q_{\Psi}(z)\, \mathrm{d} z$
, and for
$r\geqslant 0$
let
For
$r\in (0,2L_0]$
and constants
$K_1$
and
$K_2$
as in (3.8), define
and
\begin{eqnarray*}g(r) = \left(1+\frac{2K_1}{(2K_2) \wedge g_1^{-1}(2L_0)} \right)g_1(r).\end{eqnarray*}
The proof of exponential ergodicity is standard; for more details see [Reference Liang, Schilling and Wang26, Reference Liang and Wang27, Reference Wang46] and references therein. By applying Theorem 4.4 of [Reference Liang and Wang27], we prove the following exponential ergodicity for the process
$(X_t)_{t\geqslant 0}$
under the Wasserstein-1 distance. Lemma 6 follows from this lemma.
Lemma 9. Let the process
$(X_t)_{t\geqslant 0}$
be as in (3.7). Under condition (3.8), there exist positive constants
$c_{1}$
and
$c_{2}$
independent of d such that for any
$x,y\in \mathbb{R}^d$
and
$t>0$
,
Proof. Recall that
$\pi(\mathrm{d} z) = \frac{d_{\alpha}}{|z|^{d+\alpha}} \,\mathrm{d} z$
. We choose
where
$z_1$
is the first element of vector z, that is,
$z=(z_1,z_2,\ldots,z_d)$
. Thus, we know that
\begin{align*}q(z) &= 1_{\{-\frac{1}{8} < z_1 < \frac{1}{8}, |z|\leqslant 1 \}} \frac{d_{\alpha}}{|z|^{d+\alpha}}, \\q_{\Psi}(z) &= 1_{\{-\frac{1}{8} < (\Psi^{-1}(z))_1 < \frac{1}{8}, |\Psi^{-1}(z)|\leqslant 1 \}} \frac{d_{\alpha}}{|\Psi^{-1}(z)|^{d+\alpha}}\end{align*}
satisfy
We give the estimate for the function J(r) first. For
$x,y\in \mathbb{R}^d$
with
$|\tilde{x}-\tilde{y}| \leqslant \tau$
, we consider the following two cases.
-
(i) If
$(A^{-1}(\tilde{x}-\tilde{y}))_1 \leqslant 0$
, then after some calculations we get that is,
\begin{eqnarray*}q(z) \wedge q_{\Psi}(z) \geqslant \frac{d_{\alpha}}{2^{d+\alpha}} 1_{\{z_1>0, \Lambda|\tilde{x}-\tilde{y}|\leqslant |z| \leqslant \frac{1}{16\Lambda^2} \} } \frac{1}{|z|^{d+\alpha}},\end{eqnarray*}
where the last inequality holds provided
\begin{eqnarray*}\int_{\mathbb{R}^d} [q(z) \wedge q_{\Psi}(z)] \,\mathrm{d} z&\,\geqslant& \frac{d_{\alpha} \sigma_{d-1}}{\alpha 2^{d+\alpha+1}} \left[ \frac{1}{(\Lambda|\tilde{x}-\tilde{y}|)^{\alpha}} - \frac{1}{(\frac{1}{16\Lambda^2})^{\alpha}}\right] \\&\,\geqslant& \frac{d_{\alpha} \sigma_{d-1}}{\alpha 2^{d+\alpha+1}}\left(\frac{1}{\Lambda^{\alpha}}-\frac{1}{2^{\alpha}\Lambda^{3\alpha}}\right) |\tilde{x}-\tilde{y}|^{-\alpha},\end{eqnarray*}
$|\tilde{x}-\tilde{y}| \leqslant \tau \leqslant \frac{1}{32 \Lambda^5}$
.
-
(ii) If
$(A^{-1}(\tilde{x}-\tilde{y}))_1>0$
, then that is,
\begin{eqnarray*}q(z) \wedge q_{\Psi}(z) \geqslant \frac{d_{\alpha}}{2^{d+\alpha}} 1_{\{ (\Psi^{-1}(z))_1>0, \Lambda|\tilde{x}-\tilde{y}|\leqslant |\Psi^{-1}(z)|\leqslant \frac{1}{16\Lambda^2} \} } \frac{1}{|\Psi^{-1}(z)|^{d+\alpha}},\end{eqnarray*}
where the last inequality holds provided
\begin{eqnarray*}\int_{\mathbb{R}^d} [q(z) \wedge q_{\Psi}(z)] \,\mathrm{d} z&\,\geqslant& \frac{d_{\alpha} \sigma_{d-1}}{\alpha 2^{d+\alpha+1}} \left[ \frac{1}{(\Lambda|\tilde{x}-\tilde{y}|)^{\alpha}} - \frac{1}{(\frac{1}{16\Lambda^2})^{\alpha}}\right] \\&\,\geqslant& \frac{d_{\alpha} \sigma_{d-1}}{\alpha 2^{d+\alpha+1}} \left(\frac{1}{\Lambda^{\alpha}}-\frac{1}{2^{\alpha}\Lambda^{3\alpha}}\right) |\tilde{x}-\tilde{y}|^{-\alpha},\end{eqnarray*}
$|\tilde{x}-\tilde{y}| \leqslant \tau \leqslant \frac{1}{32\Lambda^5}$
.
Combining the above two cases, for any
$0 < r\leqslant \tau$
we know that
with
$\widehat{C}_1=\frac{d_{\alpha} \sigma_{d-1}}{\alpha 2^{d+\alpha+1}} (\frac{1}{\Lambda^{\alpha}}-\frac{1}{2^{\alpha}\Lambda^{3\alpha}})$
. Thus, for any
$0 < r\leqslant \tau$
, we know that
This implies that we can choose the function
$\psi$
as follows:
\begin{eqnarray*}\psi(r)=\left\{\begin{array}{lll}\frac{\widehat{C}_1}{2} r^{1-\alpha} & \text{if } r\in (0,\tau], \\[4pt] \frac{\widehat{C}_1}{2}\tau^{2-\alpha} r^{-1} & \text{if } r\in (\tau,2L_0].\end{array}\right.\end{eqnarray*}
Then we know that
\begin{eqnarray*}g_1(2L_0) &\,=\,& \left(\int_0^{\tau} + \int_{\tau}^{2L_0} \right) \frac{1}{\psi(s)} \,\mathrm{d} s\ \ = \ \ 2\alpha^{-1} \widehat{C}_1^{-1} \tau^{\alpha}+ \tau^{\alpha-2} \widehat{C}_1^{-1} (4L_0^2 - \tau^2), \\g(2L_0) &\,=\,& \left(1+\frac{2K_1}{(2K_2) \wedge g_1^{-1}(2L_0)} \right)g_1(2L_0).\end{eqnarray*}
Using Theorem 4.4 from [Reference Liang and Wang27], we obtain that
where
\begin{eqnarray*}\widehat{C} &\,=\,&\frac{1}{2}\left( 1+\exp\!\left\{ g(2L_0) [ (2K_2) \wedge g_1^{-1}(2L_0) ] \right\} \right) ,\\\lambda &\,=\,& \frac{(2K_2) \wedge g_1^{-1}(2L_0)}{1+\exp\!\left\{ g(2L_0)[ (2K_2) \wedge g_1^{-1}(2L_0) ] \right\} }.\end{eqnarray*}
Recall that
$\widehat{C}_1=\frac{d_{\alpha} \sigma_{d-1}}{\alpha 2^{d+\alpha+1}} (\frac{1}{\Lambda^{\alpha}}-\frac{1}{2^{\alpha}\Lambda^{3\alpha}})$
,
$d_{\alpha}= 2^{\alpha}\Gamma(\frac{d+\alpha}{2})\pi^{-\frac{d}{2}}|\Gamma(-\frac{\alpha}{2})|^{-1}$
and
$\sigma_{d-1}=2\pi^{\frac{d}{2}} \Gamma^{-1}(\frac{d}{2})$
; then there exists a positive constant C independent of d such that
Moreover, there exist positive constants
$c_{1}$
and
$c_{2}$
both independent of d such that
The proof is complete.
Now we are ready to prove Lemma 6.
Proof of Lemma 6. In (3.8), let
$K_{1}= L$
,
$K_{2}=\frac{\theta_{1}}{2}$
and
$L_{0}=\sqrt{\frac{2K}{\theta_{1}}}$
. It follows from (1.8), (1.9) and Lemma 9 that
For a sequence
$\{x_n\}_{n=1}^{\infty} \subseteq \mathbb{R}^d$
and x such that
$\lim_{n\to\infty} x_n=x$
, it follows from (3.9) and the dominated convergence theorem that for any continuous bounded function
$\phi$
,
which implies that the semigroup
$P_{t}$
is Feller.
The existence of an invariant measure will be established below by using the Krylov–Bogolioubov theorem (see e.g. [Reference Hairer16, Theorem 1.10]). Let
$X_0=x$
, and for any measurable set A and
$T>0$
define
Since
$P_{t}$
is Feller, it suffices to show that
$\{ \mu_{T}^{x} \}_{T>0}$
is tight from the Krylov–Bogolioubov theorem. For the function
$V_{\kappa}$
in (3.1), one gets the inequality (3.4); there exists some positive constant c such that
Since
$V_{\kappa}(x)\geqslant 1$
and
$V_{\kappa}(x)\to\infty$
as
$|x|\to \infty$
, for any fixed
$\delta>0$
there exists a compact set
$K_0$
such that
$V_{\kappa}(x)> \frac{c}{\delta}$
for
$x\in K_0^c$
, where
$K_0^c$
is the complement set of
$K_0$
. Then we have
that is,
$\mu_{T}^{x} (K_0^c)<\delta$
, which implies
$\mu_{T}^{x} (K_0)>1-\delta$
. So
$\{\mu_{T}^{x} \}_{T>0}$
is tight. Hence the limit of a convergent subsequence
$\mu_{T}^{x}$
as
$T\to \infty$
provides an invariant measure of
$(P_{t})_{t\geqslant 0}$
.
The inequality (3.9) implies that the invariant measure is unique. Indeed, let
$\mu_1$
and
$\mu_2$
be two invariant measures; for any function
$h\in \mathrm{Lip}(1)$
, we have
\begin{eqnarray*}W_1 (\mu_1,\mu_2)&\,=\,&\text{supp}_{h\in {\rm Lip}(1)} \left\{\mu_1(h)-\mu_2(h)\right\} \\ &\,=\,& \text{supp}_{h\in {\rm Lip}(1)} \left\{\int_{\mathbb{R}^d} \int_{\mathbb{R}^d} \mathbb{E} h( X_t^{x})\mu_1({\mathrm{d}} x) \mu_2({\mathrm{d}} y)-\int_{\mathbb{R}^d} \int_{\mathbb{R}^d} \mathbb{E} h(X_t^{y}) \mu_1({\mathrm{d}} x) \mu_2({\mathrm{d}} y) \right\}\\&\leqslant& \int_{\mathbb{R}^d} \int_{\mathbb{R}^d} \text{supp}_{h\in {\rm Lip}(1)} \{ \mathbb{E} h(X_t^{x})-\mathbb{E} h(X_t^{y}) \} \mu_1({\mathrm{d}} x) \mu_2({\mathrm{d}} y) \\&\,=\,& \int_{\mathbb{R}^d} \int_{\mathbb{R}^d} W_1 (\mathcal{L}(X_t^{x})\mathcal{L}(X_t^{y})) \mu_1({\mathrm{d}} x) \mu_2({\mathrm{d}} y) \ \ \rightarrow \ \ 0\end{eqnarray*}
as
$t \rightarrow \infty$
by (3.9). The proof is complete.
3.6. Proof of Lemma 7
For
$n\geqslant1$
, set
$u_{n}=\frac{v_{n}}{\gamma_{n}^{\theta}}$
. Then
where
$\lambda_n=(\frac{\gamma_{n}}{\gamma_{n+1}})^{\theta}{\mathrm{e}}^{-\rho\gamma_{n+1}}$
. Recall that
$\omega = \limsup\limits_{k\to \infty} \frac{\gamma^{\theta}_k-\gamma^{\theta}_{k+1}}{\gamma_{k+1}^{1+\theta}}< +\infty$
and
$\rho>\omega$
. Then for any constant
$c\in(\omega,\rho)$
, there exists an
$n_{0}\in\mathbb{N}$
such that for all
$n\geqslant n_{0}$
,
\begin{eqnarray}\frac{\gamma^{\theta}_n}{\gamma^{\theta}_{n+1}}\ =\ 1+\frac{\gamma^{\theta}_{n} - \gamma^{\theta}_{n+1}}{\gamma^{1+\theta}_{n+1}} \gamma_{n+1}\ \leqslant \ 1+ c \gamma_{n+1}\ \leqslant \ {\mathrm{e}}^{c \gamma_{n+1}}.\end{eqnarray}
Hence
This and (3.10) imply
Consequently,
where the constant
$M=\text{supp}_{k\geqslant1}{\mathrm{e}}^{(\rho-c)\gamma_{k}}$
. Hence, by induction, we obtain
Consequently,
We take
$c=\frac{\rho+\omega}{2}$
; then
$M={\mathrm{e}}^{(\rho-c)\gamma_1} = {\mathrm{e}}^{\frac{\rho-\omega} 2 \gamma_1}$
. Letting
$n \to \infty$
in (3.12) yields (2.8).
To prove (2.9), we set
$\omega_{n}=\frac{{\mathrm{e}}^{-\rho t_{n}}}{\gamma_{n}^{\theta}}$
. Then, by (3.11), we see that for
$n\geqslant n_{0}$
,
Hence (2.9) follows from (3.13) and the facts that
$\sum_{k=n_{0}}^{\infty}\gamma_{k}=\infty$
and
$c < \rho$
.
Finally, we prove the last inequality, (2.10). By the same argument as in the proof of (3.11), we have
$$\text{supp}_{n\geqslant1}\frac{\gamma_{n}^{\frac{1}{\alpha}}}{\gamma_{n+1}^{\frac{1}{\alpha}}}<1+c\gamma_{1}.$$
This implies that for any
$i\leqslant n-1$
,
\begin{align*}\frac{(t_{n}-t_{i-1})^{\frac{1}{\alpha}}}{(t_{n}-t_{i})^{\frac{1}{\alpha}}}=\frac{(t_{n}-t_{i}+\gamma_{i})^{\frac{1}{\alpha}}}{(t_{n}-t_{i})^{\frac{1}{\alpha}}}\leqslant 2+\frac{2\gamma_{i}^{\frac{1}{\alpha}}}{(t_{n}-t_{i})^{\frac{1}{\alpha}}}\leqslant2+\frac{2\gamma_{i}^{\frac{1}{\alpha}}}{\gamma_{i+1}^{\frac{1}{\alpha}}}\leqslant C.\end{align*}
Hence, we have
\begin{align*}\sum_{i=n^*+1}^{n-1}(t_n-t_i)^{-\frac{1}{\alpha}} \gamma_i^{1+\theta}&\leqslant C\sum_{i=n^*+1}^{n-1}(t_n-t_{i-1})^{-\frac{1}{\alpha}} \gamma_i^{1+\theta}\\&\leqslant C\gamma_{n^{*}}^{\theta}\int^{t_{n-1}}_{t_{n^{*}}}(t_{n}-t)^{-\frac{1}{\alpha}}\,\mathrm{d} t\leqslant C\gamma_{n^{*}}^{\theta}.\end{align*}
In addition, (3.11) implies
\begin{align*}\frac{\gamma_{n^{*}}^{\theta}}{\gamma_{n}^{\theta}}=\prod_{i=n^{*}}^{n-1}\left(\frac{\gamma_{i}}{\gamma_{i+1}}\right)^{\theta}\leqslant {\mathrm{e}}^{c(t_{n}-t_{n^{*}})}\leqslant {\mathrm{e}}^{\rho(1+\gamma_{1})}.\end{align*}
Therefore, we have
\begin{align*}\sum_{i=n^*+1}^{n-1}(t_n-t_i)^{-\frac{1}{\alpha}} \gamma_i^{1+\theta}\leqslant C{\mathrm{e}}^{\rho(1+\gamma_{1})}\gamma_{n}^{\theta}.\end{align*}
This proves (2.10).
Appendix A. Lower bound for the stable OU process
We consider the stable OU process defined by
where
$(Z_t)_{t\geqslant 0}$
is a one-dimensional symmetric
$\alpha$
-stable process with
$\alpha\in(1,2)$
. It is known that the solution to (A.1) is
It follows from [40, Proposition 3.4.1] that the characteristic function for
$X_t$
is
\begin{eqnarray*}\mathbb{E}[\exp({\mathrm{i}} \lambda X_t)]&\,=\,& \exp({\mathrm{i}} \lambda {\mathrm{e}}^{-t}x) \mathbb{E}\left[\exp\!\left({\mathrm{i}} \int_0^t \lambda {\mathrm{e}}^{s-t} \,\mathrm{d} Z_s\right)\right] \\&\,=\,& \exp({\mathrm{i}} \lambda {\mathrm{e}}^{-t}x) \exp\!\left(-\int_0^t |\lambda {\mathrm{e}}^{s-t}|^{\alpha} \,\mathrm{d} s \right) \\&\,=\,& \exp({\mathrm{i}} \lambda {\mathrm{e}}^{-t}x) \exp\!\left(-\frac{1}{\alpha}|\lambda|^{\alpha} [1-{\mathrm{e}}^{-\alpha t}] \right) \\&\to& \exp\!\left(-\frac{1}{\alpha}|\lambda|^{\alpha} \right) \quad\mbox{as } t\to \infty;\end{eqnarray*}
that is, the invariant measure
$\mu$
for the stable OU process
$(X_t)_{t\geqslant 0}$
follows
$\mu \stackrel{\rm d}{=}\mathcal{L}(\alpha^{-\frac{1}{\alpha}} Z_1)$
with
$\mathbb{E}\exp({\mathrm{i}} \lambda Z_1)=\exp(-|\lambda|^{\alpha})$
.
Recall that the EM scheme with the Pareto distribution for
$(X_t)_{t\geqslant 0}$
in (A.1) is given as follows: with
$\tilde{Y}_0=x$
and for any integers
$n\geqslant 1$
,
\begin{eqnarray}\tilde{Y}_{t_{n+1}} = \tilde{Y}_{t_{n}}-\gamma_{n+1}\tilde{Y}_{t_{n}}+\frac{\gamma_{n+1}^{\frac{1}{\alpha}}}{\beta}\,\tilde{Z}_{n+1},\end{eqnarray}
where
$\beta=(\frac{\alpha}{2d_{\alpha}})^{\frac{1}{\alpha}}$
and
$(\tilde{Z}_{n})_{n\geqslant 1}$
is a sequence of i.i.d. random variables with density
Then we have the following lemma.
Lemma 10. Denote the invariant measure of
$(X_{t})_{t\geqslant0}$
defined in (A.1) by
$\nu$
, and let
$(\tilde{Y}_{t_{n}})_{n\in\mathbb{N}_{0}}$
be defined by (A.2). Suppose that Assumption 2 holds with
$\theta=\frac{2-\alpha}{\alpha}$
and
$\omega<\rho\wedge1$
. Then, for any bounded
$x\in\mathbb{R}$
and
$\alpha\in(1,2)$
, we have
\begin{align*}0<\liminf_{n\rightarrow\infty}\frac{W_{1}(\nu,\tilde{Y}_{t_{n}}^{x})}{\gamma_{n}^{\frac{2}{\alpha}-1}}\leqslant\limsup_{n\rightarrow\infty}\frac{W_{1}(\nu,\tilde{Y}_{t_{n}}^{x})}{\gamma_{n}^{\frac{2}{\alpha}-1}}<\infty.\end{align*}
Proof. From (A.2), we can deduce that
\begin{align*}\tilde{Y}_{t_{n}}^{x}&=\prod_{j=1}^{n}(1-\gamma_{j})x+\sum_{j=0}^{n-1}\frac{\gamma_{n-j}^{\frac{1}{\alpha}}\tilde{Z}_{n-j}}{\beta}\prod_{k=n+1-j}^{n}(1-\gamma_{k})\\&=\prod_{j=1}^{n}(1-\gamma_{j})x+\sum_{j=1}^{n}\frac{\gamma_{j}^{\frac{1}{\alpha}}\tilde{Z}_{j}}{\beta}\prod_{k=j+1}^{n}(1-\gamma_{k}).\end{align*}
Write
$\phi(\lambda)=\mathbb{E}\exp({\mathrm{i}} \lambda \tilde{Z}_{1})$
; then we have
\begin{eqnarray*}\mathbb{E}\exp({\mathrm{i}} \lambda\tilde{Y}_{t_{n}}^{x})&\,=\,& \exp\!\left({\mathrm{i}} \lambda\prod_{j=1}^{n}(1-\gamma_{j})x\right)\prod_{j=1}^{n}\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\frac{\gamma_{j}^{\frac{1}{\alpha}}\tilde{Z}_{j}}{\beta}\prod_{k=j+1}^{n}(1-\gamma_{k})\right)\nonumber\\&\,=\,& \exp\!\left({\mathrm{i}} \lambda\prod_{j=1}^{n}(1-\gamma_{j})x\right)\prod_{j=1}^{n}\phi\left(\frac{\gamma_{j}^{\frac{1}{\alpha}}}{\beta}\prod_{k=j+1}^{n}(1-\gamma_{k})\lambda\right).\end{eqnarray*}
By [6, (A.4)], for
$|\lambda|\leqslant 1$
and
$0<\gamma_{1}<1\wedge\beta^{\alpha}$
,
\begin{align*}&\log\phi\left(\frac{\gamma_{j}^{\frac{1}{\alpha}}}{\beta}\prod_{k=j+1}^{n}(1-\gamma_{k})\lambda\right)\\&\quad\geqslant\log\left(1-\gamma_{j}\prod_{k=j+1}^{n}(1-\gamma_{k})^{\alpha}|\lambda|^{\alpha}+\frac{c\alpha}{(2-\alpha)\beta^{2}}\gamma_{j}^{\frac{2}{\alpha}}\prod_{k=j+1}^{n}(1-\gamma_{k})^{2}|\lambda|^{2}\right),\end{align*}
where
$c=\inf_{0 < u\leqslant 1}\frac{1-\cos u}{u^{2}}>0$
. Since
\begin{align*}\lim_{x\downarrow0}\frac{\log\left(1-x+\frac{c\alpha}{(2-\alpha)\beta^{2}}x^{\frac{2}{\alpha}}\right)+x}{x^{\frac{2}{\alpha}}}=\frac{c\alpha}{(2-\alpha)\beta^{2}},\end{align*}
there is a positive constant
$C=C(\alpha)$
such that for small enough
$x>0$
,
These imply that for all
$|\lambda|\leqslant 1$
and large enough n or j, we have
\begin{align*}\log\phi\left(\frac{\gamma_{j}^{\frac{1}{\alpha}}}{\beta}\prod_{k=j+1}^{n}(1-\gamma_{k})\lambda\right)\geqslant-\gamma_{j}\prod_{k=j+1}^{n}(1-\gamma_{k})^{\alpha}|\lambda|^{\alpha}+C\gamma_{j}^{\frac{2}{\alpha}}\prod_{k=j+1}^{n}(1-\gamma_{k})^{2}|\lambda|^{2}.\end{align*}
Hence,
\begin{align}&\log\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\tilde{Y}_{t_{n}}^{x}-x\prod_{j=1}^{n}(1-\gamma_{j})\right)\right)\ = \ \sum_{j=1}^{n}\log\phi\left(\frac{\gamma_{j}^{\frac{1}{\alpha}}}{\beta}\prod_{k=j+1}^{n}(1-\gamma_{k})\lambda\right) \nonumber \\&\quad\geqslant -\sum_{j=1}^{n}\gamma_{j}\prod_{k=j+1}^{n}(1-\gamma_{k})^{\alpha}|\lambda|^{\alpha}+C\sum_{j=1}^{n}\gamma_{j}^{\frac{2}{\alpha}}\prod_{k=j+1}^{n}(1-\gamma_{k})^{2}|\lambda|^{2}.\end{align}
Now, we analyse the last two items in (A.3). For the first term, by the inequality
$1-x \leqslant {\mathrm{e}}^{-x}$
,
\begin{eqnarray} \sum_{j=1}^{n}\gamma_{j}\prod_{k=j+1}^{n}(1-\gamma_{k})^{\alpha}\leqslant \sum_{j=1}^{n}\gamma_{j} {\mathrm{e}}^{-\alpha(t_n-t_j)} \leqslant \frac 1{\alpha}(1-{\mathrm{e}}^{-\alpha t_n}) +O(\gamma_n),\end{eqnarray}
where the last inequality is obtained from
\begin{align*}& \sum_{j=1}^{n}\gamma_{j} {\mathrm{e}}^{-\alpha(t_n-t_j)}- \frac{1}{\alpha}+\frac{1}{\alpha} {\mathrm{e}}^{-\alpha t_n}= {\mathrm{e}}^{-\alpha t_n} \left[ \sum_{j=1}^{n}\gamma_{j} {\mathrm{e}}^{\alpha t_j}- \int_0^{t_n} {\mathrm{e}}^{\alpha s} \,\mathrm{d} s \right] \\&\quad= {\mathrm{e}}^{-\alpha t_n} \sum_{j=1}^{n} \int_{t_{j-1}}^{t_j} ({\mathrm{e}}^{\alpha t_j}- {\mathrm{e}}^{\alpha s}) \,\mathrm{d} s \ \leqslant\ {\mathrm{e}}^{-\alpha t_n} \sum_{j=1}^{n} \int_{t_{j-1}}^{t_j} \alpha {\mathrm{e}}^{\alpha t_j} (t_j-s) \,\mathrm{d} s \\&\quad = \frac{\alpha}{2} {\mathrm{e}}^{-\alpha t_n} \sum_{j=1}^{n} {\mathrm{e}}^{\alpha t_j} \gamma_j^2\ \leqslant\ C \gamma_n,\end{align*}
where the first inequality holds by the mean value theorem and the last inequality holds because of (2.8).
Now we estimate the second term in (A.3). Notice that for some
$x_0>0$
, we have
$1-x\geqslant {\mathrm{e}}^{-\frac{3}{2}x}$
for all
$x \in (0, x_0)$
. Let
$j_0=\inf\{j>0: \gamma_j < x_0\}$
. Then
\begin{eqnarray}\sum_{j=1}^{n} \gamma_{j}^{\frac{2}{\alpha}}\prod_{k=j+1}^{n}(1-\gamma_{k})^{2}\gamma_{n}^{-\frac{2-\alpha}{\alpha}}& \geqslant & \sum_{j=j_0}^{n}\gamma_{j} \prod_{k=j+1}^{n} (1-\gamma_{k})^{2} \left(\frac{\gamma_j}{\gamma_{n}}\right)^{\frac{2-\alpha}{\alpha}} \nonumber \\&\geqslant & \sum_{j=j_0}^{n}\gamma_{j} \prod_{k=j+1}^{n} (1-\gamma_{k})^{2}\ \geqslant \ \sum_{j=j_0}^{n} \gamma_{j} {\mathrm{e}}^{-3(t_n-t_j)} \nonumber \\&\geqslant & \int_{t_{j_0}}^{t_n} {\mathrm{e}}^{-3(t_n-s)} \,\mathrm{d} s= \frac 1 3 \big(1 - {\mathrm{e}}^{-3 (t_n - t_{j_0})}\big).\end{eqnarray}
Combining (A.3), (A.4), (A.5) and the easy fact that
${\mathrm{e}}^{-\alpha t_n}=o(\gamma^{\frac{2-\alpha}{\alpha}}_n)$
, we have
\begin{eqnarray*}\log\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\tilde{Y}_{t_{n}}^{x}-x\prod_{j=1}^{n}(1-\gamma_{j})\right) \right)\geqslant -\frac{1}{\alpha}|\lambda|^{\alpha}+|\lambda|^{\alpha}o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)+|\lambda|^{2}O\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right),\end{eqnarray*}
where
$f(n)=o(g(n))$
as
$n\rightarrow\infty$
means that
$\lim_{n\rightarrow\infty}\frac{f(n)}{g(n)}=0$
, and
$f(n)=O(g(n))$
as
$n\rightarrow\infty$
means that
$\lim_{n\rightarrow\infty}\frac{f(n)}{g(n)}<\infty$
. By the inequality
${\mathrm{e}}^{x}\geqslant1+x$
for any
$x\in\mathbb{R}$
, we further have that
\begin{align*}\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\tilde{Y}_{t_{n}}^{x}-x\prod_{j=1}^{n}(1-\gamma_{j})\right)\right)&\geqslant\exp\!\left[-\frac{1}{\alpha}|\lambda|^{\alpha}+|\lambda|^{\alpha}o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)+|\lambda|^{2}O\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)\right]\\&\geqslant{\mathrm{e}}^{-\frac{|\lambda|^{\alpha}}{\alpha}}\left[1+o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)+|\lambda|^{2-\alpha}O\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)\right].\end{align*}
In addition, since
\begin{align*}\prod_{j=1}^{n}(1-\gamma_{j})=1-\sum_{j=1}^{n}\gamma_{j}\prod_{k=j+1}^{n}(1-\gamma_{k})\end{align*}
and
\begin{align*}\lim_{n\rightarrow\infty}\left(1-\sum_{j=1}^{n}\gamma_{j}\prod_{k=j+1}^{n}(1-\gamma_{k})\right){\mathrm{e}}^{t_{n}}&=\lim_{n\rightarrow\infty}\left(1-\int_{0}^{t_{n}}{\mathrm{e}}^{-(t_{n}-s)}\mathrm{d} s\right){\mathrm{e}}^{t_{n}}\\&=\lim_{n\rightarrow\infty}\left(1-\int_{0}^{t_{n}}{\mathrm{e}}^{-s}\,\mathrm{d} s\right){\mathrm{e}}^{t_{n}}=1,\end{align*}
one can derive from (2.9) that
\begin{align*}\lim_{n\rightarrow\infty}\frac{\prod_{j=1}^{n}(1-\gamma_{j})}{\gamma_{n}^{\frac{2-\alpha}{\gamma_{n}}}}=\lim_{n\rightarrow\infty}\frac{{\mathrm{e}}^{-t_{n}}}{\gamma_{n}^{\frac{2-\alpha}{\alpha}}}=0,\end{align*}
which implies that for large enough n,
\begin{eqnarray}\prod_{j=1}^{n}(1-\gamma_{j})=o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right).\end{eqnarray}
Hence, for large enough n and any bounded x, we have
\begin{align*}& \int_{-1}^{1}\left[\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\alpha^{-\frac{1}{\alpha}}Z_{1}-x\prod_{j=1}^{n}(1-\gamma_{j})\right)\right)-\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\alpha^{-\frac{1}{\alpha}}Z_{1}\right)\right]\mathrm{d} \lambda\\&\quad=\int_{-1}^{1}\mathbb{E}\left[\exp\!\left({\mathrm{i}} \lambda\alpha^{-\frac{1}{\alpha}}Z_{1}\right)\right]\left[\cos\left(\lambda x\prod_{j=1}^{n}(1-\gamma_{j})\right)-1\right]\mathrm{d} \lambda\\&\quad=|x|^2 O\!\left(\prod_{j=1}^{n}(1-\gamma_{j})^2\right)\int_{-1}^{1}\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\alpha^{-\frac{1}{\alpha}}Z_{1}\right)|\lambda|^2 \,\mathrm{d}\lambda\ = \ o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right),\end{align*}
where the second equality holds because
Thus we have
\begin{align}&\int_{-1}^{1}\left[\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\tilde{Y}_{t_{n}}^{x}-x\prod_{j=1}^{n}(1-\gamma_{j})\right)\right)-\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\alpha^{-\frac{1}{\alpha}}Z_{1}-x\prod_{j=1}^{n}(1-\gamma_{j})\right)\right)\right]\mathrm{d} \lambda\nonumber\\&\quad=\int_{-1}^{1}\left[\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\tilde{Y}_{t_{n}}^{x}-x\prod_{j=1}^{n}(1-\gamma_{j})\right)\right)-\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\alpha^{-\frac{1}{\alpha}}Z_{1}\right)\right]\mathrm{d} \lambda\nonumber\\&\qquad+\int_{-1}^{1}\left[\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\left(\alpha^{-\frac{1}{\alpha}}Z_{1}-x\prod_{j=1}^{n}(1-\gamma_{j})\right)\right)-\mathbb{E}\exp\!\left({\mathrm{i}} \lambda\alpha^{-\frac{1}{\alpha}}Z_{1}\right)\right]\mathrm{d} \lambda\nonumber\\&\quad\geqslant\int_{-1}^{1}{\mathrm{e}}^{-\frac{1}{\alpha}|\lambda|^{\alpha}}\left[o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)+|\lambda|^{2-\alpha}O\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)\right]\mathrm{d}\lambda+o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)\nonumber\\&\quad=o\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)+O\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right)=O\!\left(\gamma_{n}^{\frac{2-\alpha}{\alpha}}\right).\end{align}
Then, by the same argument as in the proof of Proposition B.1 in [Reference Chen, Deng, Schilling and Xu6] and taking
\begin{align*}h(y)=\frac{1}{M}\left(\frac{\sin\left(y-x\prod_{j=1}^{n}(1-\gamma_{j})\right)}{y-x\prod_{j=1}^{n}(1-\gamma_{j})}{\bf 1}_{\{y\neq x\prod_{j=1}^{n}(1-\gamma_{j})\}}+{\bf 1}_{\{y=x\prod_{j=1}^{n}(1-\gamma_{j})\}}\right),\quad y\in\mathbb{R},\end{align*}
with
$M=\text{supp}_{z\in\mathbb{R}\backslash\{0\}}|\frac{z\cos z-\sin z}{z^{2}}|\in(0,\infty)$
, the desired result follows.
Acknowledgements
The authors would like to thank the editors and referees for their helpful comments.
Funding information
P. Chen was supported in part by a National Natural Science Foundation of China grant (no. 12301176), a Natural Science Foundation of Jiangsu Province grant (no. BK20220867) and the China Postdoctoral Science Foundation (grant no. 2023M741692). X. Jin was supported by a National Natural Science Foundation of China grant (no. 12401176) and a Fundamental Research Funds for the Central Universities grant (no. JZ2023HGTA0170). Y. Xiao was supported in part by the NSF grant DMS-2153846. L. Xu was supported by an NNSFC grant (no. 12071499) and the University of Macau grant MYRG2018-00133-FST.
Competing interests
There were no competing interests to declare which arose during the preparation or publication process of this article.















