Abstract
In this paper, we investigate the partial practical exponential stability of neutral stochastic functional differential equations with Markovian switching. The main tool used to prove the results is the Lyapunov method. We analyze an illustrative example to show the applicability and interest of the main results.
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1 Introduction
Neutral stochastic differential equations with Markovian switching have attracted much attention over the last decades within the scopes and main problems from the applied sciences and which are modeled by stochastic differential equations (see [1, 4, 8, 9]). Neutral stochastic differential equations with Markovian switching are useful to model physical, biological and economical dynamical phenomena. In the literature, many authors have studied the existence and uniqueness of solution to neutral stochastic differential equations with a Markovian switching (see [10, 11]). Stability is the most important concept in modern control theory, and switching systems can be used to model a wide type of physical and engineering systems in practice; hence, stability of neutral stochastic differential equations with a Markovian switching has received an increasing attention (see [6, 7, 10]). However, in many physical systems, such stability is sometimes too strong to be satisfied. Therefore, the notion of stability with respect to part of the variables (i.e. partial stability) (see [5, 6, 12, 13]) has been used, and the Lyapunov method, as an indispensable tool, has been used to investigated the partial stability and stabilizability in various practically important problems. However, when the origin is not necessarily an equilibrium point, it is still possible to study the asymptotic stability of solutions with respect to a small neighborhood of the origin, which yields to the concept of practical stability (see [2, 3]).
The structure of the paper is as follows. In Sect. 2, we introduce some basic notions and assumptions. Section 3 is devoted to prove some sufficient conditions ensuring practical partial pth moment exponential stability of solutions to neutral stochastic functional differential equations with Markovian switching. We prove a sufficient condition ensuring the convergence of the solution (with respect to part of the variables) to a ball with radius \(r>0\) in pth moment, even in the case that zero is not an equilibrium point. In Sect. 4, we prove a sufficient condition ensuring practical exponential instability in the qth moment. Finally, we analyze an example to illustrate our results in Section 5.
2 Preliminaries and Definitions
Let \(\left( \Omega ,{\mathcal {F}}, \left\{ {\mathcal {F}}_t\right\} _{t\ge 0},{\mathbb {P}}\right) \) be a complete probability space with a filtration satisfying the usual conditions, i.e., the filtration is right continuous and increasing and \({\mathcal {F}}_0\) contains all \({\mathbb {P}}\)-null sets. W(t) is an m-dimensional Brownian motion defined on the probability space. For a given \(\tau >0\), let \(C([-\tau , 0];{\mathbb {R}}^n)\) be the family of functions \(\varphi \) from \([-\tau , 0]\) to \({\mathbb {R}}^n\) that are right-continuous and have limits on the left. \(C([-\tau , 0];{\mathbb {R}}^n)\) is equipped with the norm \(\Vert \varphi \Vert = \sup _{-\tau \le s\le 0}|\varphi (s)|\) and \(|x|=\sqrt{x^Tx}\) for any \(x \in {\mathbb {R}}^n\). If A is a matrix, its trace norm is denoted by \(|A| =\sqrt{trace(A^TA)}\), while its operator norm is denoted by \(\Vert A\Vert = \sup \{|Ax| : |x| = 1\}\). Denote by \(C^b_{{\mathcal {F}}_0}([-\tau , 0];{\mathbb {R}}^n)\) the family of all \({\mathcal {F}}_0\)-measurable bounded \(C([-\tau , 0];{\mathbb {R}}^n)\)-valued random variables \(\xi = \{\xi (\theta ) : -\tau \le \theta \le 0\}\). Let \(p > 0\), \(t\ge 0\), \(L^p_{{\mathcal {F}}_t}([-\tau , 0];{\mathbb {R}}^n)\) denote the family of all \({\mathcal {F}}_t\)-measurable, \(C([-\tau , 0];{\mathbb {R}}^n)\)-valued random variables \(\varphi = \{\varphi (\theta ) : -\tau \le \theta \le 0\}\) such that \(\sup _{-\tau \le \theta \le 0}{\mathbb {E}}|\varphi (\theta )|^p<\infty \).
Let \(\{r(t), t\in {\mathbb {R}}^+ = [0,+\infty [ \}\) be a right-continuous Markov chain on the probability space \(\{\Omega ,{\mathcal {F}}, \left\{ {\mathcal {F}}_t\right\} _{t\ge 0},{\mathbb {P}}\}\) taking values in a finite state space \(S = \{1,2, \dots ,N\}\) with a generator \(\Gamma =\left( \gamma _{ij}\right) _{{\mathbb {N}}\times {\mathbb {N}}}\) given by
where \(\Delta >0\). Here \(\gamma _{ij}\ge 0\) is the transition rate from i to j, if \(i \ne j\), while
We assume that the Markov chain r(t) is independent of the Brownian motion W(t). It is known that almost every sample path of r(t) is a right-continuous step function with a finite number of simple jumps in any finite sub-interval of \({\mathbb {R}}^+\).
Consider the following neutral stochastic functional differential equation with Markovian switching:
with the initial condition \(x_0 = \xi = (\xi _1,\xi _2)^T \in C^b_{{\mathcal {F}}_0}([-\tau , 0];{\mathbb {R}}^n)\) where \(\xi _1\in {\mathbb {R}}^k\) and \(\xi _2\in {\mathbb {R}}^p\), \(k + p = n\), which is independent of \(W(\cdot )\), \(x(t)=(x_1(t),x_2(t))\in {\mathbb {R}}^k\times {\mathbb {R}}^p\) and \(x_t = \{x(t + \theta ) : -\tau \le \theta \le 0\}\). Let \(\widetilde{x(t)} = x(t)-G(x_t)\). Here, we, furthermore, assume that
Denote by \(C^{1,2}\left( [-\tau ,+\infty [\times {\mathbb {R}}^n\times S;{\mathbb {R}}^+\right) \) the family of all non-negative functions V(t, x, i) on \([-\tau ,+\infty [\times {\mathbb {R}}^n\times S\), which are twice continuously differentiable with respect to x and once continuously differentiable with respect to t.
For any \((t, x, i)\in [-\tau ,+\infty [\times {\mathbb {R}}^n\times S\), \(x_t=\varphi \in C([-\tau ,0];{\mathbb {R}}^n)\) and \({\widetilde{\varphi }}(\theta )=\varphi (\theta )-G(\varphi )\), define an operator \(LV:{\mathbb {R}}^+\times C([-\tau ,0];{\mathbb {R}}^n)\times S\rightarrow {\mathbb {R}}\) by (see [11])
where
For our purpose, we will state some assumptions which can ensure the existence and uniqueness of a solution, denoted by \(x(t)=(x_1(t),x_2(t))\) on \(t >0 \), for Eq. (2.1).
\({\mathcal {A}}_1\): (A local Lipschitz condition): For each \(p=1,2,\dots \), there is an \(l_p>0\) such that
for all \(t\ge 0\), \(i\in S\) and \(\varphi _1\), \(\varphi _2\in C([-\tau ,0];{\mathbb {R}}^n)\) with \(||\varphi _1||\vee ||\varphi _2||\le p\).
\({\mathcal {A}}_2\): There exist three functions \(V\in C^{1,2}\left( [-\tau ,\infty )\times {\mathbb {R}}^n\times S;{\mathbb {R}}^+\right) \), \(U_1\), \(U_2\in C\left( [-\tau ,\infty )\times {\mathbb {R}}^n;{\mathbb {R}}^+\right) \) and a probability measure m on \([-\tau ,0]\) satisfying
\(\int _{-\tau }^{0}\mathrm{d}m(\theta )=1\), and nonnegative constants \(c_1'\), \(c_2'\), \(c_3'\) with \(c_2'>c_3'\), such that
and for all \((t,x,i)\in {\mathbb {R}}_+\times C([-\tau ,0];{\mathbb {R}}^n)\times S\), we have
for all \(i\in S\) and \(x_t=\varphi \in C([-\tau ,0];{\mathbb {R}}^n)\), \(t\ge 0\) and where \({\widetilde{\varphi }}(\theta )=\varphi (\theta )-G(\varphi )\).
\({\mathcal {A}}_3\): There exists a constant \(k\in [0, 1)\) such that
for all \(\varphi _1\), \(\varphi _2\in C([-\tau ,0];{\mathbb {R}}^n)\).
Denote \(x = (x_1,x_2)^T \in {\mathbb {R}}^n\), where \(x_1\in {\mathbb {R}}^k\) and \(x_2 \in {\mathbb {R}}^p\), \(k + p = n\), and the definitions of \({\widetilde{x}}=\left( \widetilde{x_1},\widetilde{x_2}\right) ^T\in {\mathbb {R}}^n\) and \(G(x_t) = \left( G_1(x_t),G_2(x_t)\right) ^T \in {\mathbb {R}}^n\) are similar to \(x = (x_1,x_2)^T\). The domain \(B_K = \left\{ x \in {\mathbb {R}}^n : |x_1| < K\right\} \), and the stopping time \(\tau _K=\inf \left\{ t\ge t_0;x(t)\notin B_K\right\} \). Let \(K\rightarrow \infty \), then \(\tau _K\rightarrow \infty \). Denote the set of functions
We will study the partial stability of the neutral stochastic functional differential equation with Markovian switching when 0 is not an equilibrium point, but in a small neighborhood of the origin in terms of convergence of solution in probability to a small ball \(B_{r}:=\{x\in {\mathbb {R}}^{d}:||x_1||\le r\}\), \(r>0\).
Definition 2.1
The solution \(x(t)=(x_1(t),x_2(t))\) of Eq. (2.1) is said to be practically exponentially \(x_1^p\)-stable \((p>0)\), if there exist positive constants \(\alpha \), c, r such that, for any \((x_1,x_0)\in {\mathbb {R}}^k\times C^b_{{\mathcal {F}}_0}([-\tau , 0];{\mathbb {R}}^n)\),
When \(p=1\) (respectively, \(p=2\)), the solution x(t) of stochastic system (2.1) is called exponential \(x_1\)-stable in the mean (respectively in the mean-square).
Remark 2.2
Note that, as the origin \(x=0\) may not be an equilibrium point of system (2.1), then we can no longer study the stability of the origin as an equilibrium point nor should we expect the pth moment of the solution (with respect to part of the variables) of the system to approach the origin almost surely as \(t\rightarrow +\infty \). Inequality (2.6) implies that \({\mathbb {E}}\left( |x_1|^p\right) \) will be ultimately bounded by a small bound \(r>0\), that is, \({\mathbb {E}}\left( |x_1|^p\right) \) will be small for sufficiently large t. This can be viewed as a robustness property of convergence almost surely to the origin provided that f and g satisfy \(f(t,0,r(t))=0\) and \(g(t,0,r(t))=0\), \(\forall t\ge 0\). In this case the origin becomes an equilibrium point.
3 Main Results
Now we can state and prove our main results.
Theorem 3.1
Under assumptions \({\mathcal {A}}_1\)-\({\mathcal {A}}_3\), for any given initial condition \(\xi \in C^b_{{\mathcal {F}}_0}([-\tau , 0];{\mathbb {R}}^n)\) and \(i_0\in S\), there exists a unique global solution x(t), \(t\ge -\tau \) of Eq. (2.1).
Proof
See [10] and [11]. \(\square \)
Lemma 3.2
-
(i)
Let \(0<p\le 1\) and a, \(b\in {\mathbb {R}}_+\). Then
$$\begin{aligned} (a+b)^p\le a^p+b^p. \end{aligned}$$ -
(ii)
Let \(p>1\), \(\varepsilon >0\) and a, \(b\in {\mathbb {R}}_+\). Then
$$\begin{aligned} (a+b)^p\le \left( 1+\varepsilon ^{\frac{1}{p-1}}\right) ^{p-1}\left[ a^p+\frac{b^p}{\varepsilon }\right] . \end{aligned}$$
Proof
See [9]. \(\square \)
Let us rewrite now assumption \({\mathcal {A}}_3\) in a new way:
\({\mathcal {A}}^{\prime }_3\): There exist constants \(k\in [0, 1)\), \(p,\delta >0\) such that
for all \(\varphi _1\), \(\varphi _2\in C([-\tau ,0];{\mathbb {R}}^n)\).
Theorem 3.3
Let \(c_1\), \(c_2\), \(c_3\), \(\delta \) be positive constants such that \(\frac{c_3}{c_2}\le \delta \) and \(p>0\). Assume that there exist \(V(t,x,i)\in C^{1,2}\left( ]-\tau ,+\infty [\times {\mathbb {R}}^n\times S,{\mathbb {R}}^+\right) \) and \(e^{\frac{c_3}{c_2}t}\rho (t)\in {\mathbb {L}}^1([0,+\infty [)\) such that,
-
(i)
\(\displaystyle {c_1|x_1|^p\le V(t,x,i)\le c_2|x_1|^p}\) for \(x_1\in {\mathbb {R}}^k\).
-
(ii)
\(\displaystyle {LV(t,{\widetilde{\varphi }}(0),i)\le -c_3|{\widetilde{\varphi }}_1(0)|^p + \rho (t)},\; \forall (t,\varphi ,i) \in {\mathbb {R}}^+\times C([-\tau ,0];{\mathbb {R}}^n)\times S\) where \(\varphi =(\varphi _1,\varphi _2)\in C([-\tau ,0];{\mathbb {R}}^k)\times C([-\tau ,0];{\mathbb {R}}^s)\), \(k+s=n\) and \({\widetilde{\varphi }}(0)=\varphi (0)-G(\varphi )\).
Let assumptions \({\mathcal {A}}_1\), \({\mathcal {A}}_2\) and \({\mathcal {A}}^{'}_3\) hold. Then the solution \(x(t)=(x_1(t),x_2(t))\) of Eq. (2.1) is practically exponentially \(x_1^p\)-stable if \(0<p\le 1\). If \(p>1\), the same stability holds true if in addition there exists \(\varepsilon >0\) such that \(k^p<\varepsilon \left( 1+\varepsilon ^{\frac{1}{p-1}}\right) ^{1-p}\).
Proof
According to the stopping time \(\tau _K=\inf \left\{ t\ge t_0;x(t)\notin B_K\right\} \), writing \(x_t=\varphi =(\varphi _1,\varphi _2)\), \(x_1(t)=\varphi _1(0)\), \({\widetilde{\varphi }}(0)=x(t)-G(x_t)\) and \({\widetilde{\varphi }}_1(0)=x_1(t)-G_{1}(x_{t})\) for \(t\ge t_0\), and applying Itô’s formula (see [11]), we can derive for \(t\ge -\tau \)
Hence,
Therefore, by inequality (i), we have
Obviously \(\tau _K\rightarrow \infty \) as \(K\rightarrow \infty \). Then
First case: For \(0<p\le 1\), by Lemma 3.2 and Assumption \({\mathcal {A}}^\prime _3\), we have
For any \(T>0\), we have
Then
where \(C_1(k)=\frac{1}{1-k^{p}}\left( \frac{c_2}{c_1}\left( 1+k^{p}\right) +k^{p}\right) \) and \(C_2(k)=\frac{1}{c_1(1-k^{p})}\).
Letting \(T\rightarrow +\infty \), we have
Therefore, we obtain for all \(t\ge t_0\)
Second case: For \(p>1\), by Lemma 3.2 and Assumption \({\mathcal {A}}_3^\prime \), for \(\varepsilon >0\) such that \(\frac{k^p}{\varepsilon }\left( 1+\varepsilon ^{\frac{1}{p-1}}\right) ^{p-1}<1\) and for \(\lambda >0\), we have
Hence, for any \(T>0\), we have
where
Thus,
where
and
Letting \(T\rightarrow +\infty \), we obtain
Then we have for all \(t\ge t_0\)
We see that for all \(t\ge t_0\),
Setting
we conclude that the solution of system (2.1) is practically exponentially \(x_1^p\)-stable. The proof is, therefore, complete. \(\square \)
In the following corollary, we will study the partial stability in mean square of system (2.1) in the domain \(D=\{(t,x)\in {\mathbb {R}}^+\times {\mathbb {R}}^n;|x|<\infty \}\).
We will consider the new assumption:
\({\mathcal {A}}^{''}_3\): There exists a constant \(k\in [0, 1)\) such that
for all \(\varphi _1\), \(\varphi _2\in C([-\tau ,0];{\mathbb {R}}^n)\) and \(\delta >0\).
Corollary 3.4
Let \(x= (x_1,x_2)^T\in {\mathbb {R}}^n\), where \(x_1\in {\mathbb {R}}^k\), \(x_2\in {\mathbb {R}}^s\) and \(n=k+s\), be the solution of system (2.1). Suppose that in the domain \(D=\{(t,x)\in {\mathbb {R}}^+\times {\mathbb {R}}^n;|x|<\infty \}\), along with a V-function, it is possible to specify a continuous vector \(\mu (x)\)-function, \(\mu (0)=0\) and \(e^{\frac{c_3}{c_2}t}\rho (t)\in {\mathbb {L}}^1([0,+\infty [)\) such that, for all \((t,\varphi ,i) \in {\mathbb {R}}^+\times C([-\tau ,0];{\mathbb {R}}^n)\times S\) and
we have
-
(i)
$$\begin{aligned} c_1|x_1|^2\le V(t,x,i)\le c_2\left( |x_1|^2+|\mu (x)|^2\right) , \end{aligned}$$
-
(ii)
$$\begin{aligned} LV(t,{\widetilde{\varphi }}(0),i)\le -c_3\left( |\widetilde{\varphi _1}(0)|^2+|\mu ({\widetilde{\varphi }}(0))|^2\right) +\rho (t). \end{aligned}$$(3.5)
Let assumptions \({\mathcal {A}}_1\), \({\mathcal {A}}_2\) and \({\mathcal {A}}^{''}_3\) hold. Assume that there exist \(k\in [0,\frac{\sqrt{2}}{2})\) and \(\delta >0\) such that \(\frac{c_3}{c_2}\le \delta \). Then the solution of system (2.1) is practically exponentially \(x_1\)-stable in mean-square.
Proof
Proceeding as in the previous proof, writing \(x_t=\varphi \), \(x(t)=\varphi (0)\) and \(x_1(t)=\varphi _1(0)\) for \(t\ge t_0\), we have
By inequality (i),
Obviously \(\tau _K\rightarrow \infty \) as \(K\rightarrow \infty \) then
Since \(\mu \) is continuous and \(\mu (0)=0\) then there exist \(\eta >0\) such that \(\displaystyle {|\mu (x_0-G(x_0))|\le \eta |x_0-G(x_0)|}\) for a sufficiently small \(\Vert x_0\Vert \).
Then for \(\displaystyle {x_0=(x_{01},x_{02})\in C([-\tau ,0];{\mathbb {R}}^k)\times C([-\tau ,0];{\mathbb {R}}^s)}\), we have
Therefore,
By Assumption \({\mathcal {A}}_3\) and (ii) in Lemma 3.2 (for \(\varepsilon =1\)), we have for \(k\in [0,\frac{\sqrt{2}}{2})\),
Hence, for any \(T>0\), we have
This implies
Letting \(T\rightarrow +\infty \), we obtain
Therefore, for all \(t\ge t_0\), we have
Setting
and
we prove that the solution of system (2.1) is practically exponentially \(x_1\)-stable in mean square. \(\square \)
4 Practical Exponential Instability in the qth Moment
In this section, we will prove a sufficient condition ensuring practical exponential instability of solutions in the qth moment.
Definition 4.1
The solution \(x(t)=(x_1(t),x_2(t))\) of Eq. (2.1) is said to be practically exponentially unstable in q-th moment \((q>0)\), if there exist positive constants \(\alpha \), c, r such that, for any \(x_0\in C^b_{{\mathcal {F}}_0}([-\tau , 0];{\mathbb {R}}^n)\),
When \(q=2\), the solution x(t) of stochastic system (2.1) is called practically exponentially unstable in mean square.
Remark 4.2
We can take in (4.1) a continuous nonnegative function r(t) instead of r such that \(\lim _{t\rightarrow +\infty }r(t)=0\).
We will consider the new assumption:
\({\mathcal {H}}_3\): There exists a constant \(k\in [0, 1)\) such that
for all \(\varphi _1\), \(\varphi _2\in C([-\tau ,0];{\mathbb {R}}^n)\), \(\delta >0\) and \(q>0\).
Theorem 4.3
Let \(c_1\), \(c_2\), \(c_3\) and q be positive constants such that \(\frac{c_3}{c_1}\ge \delta \). Assume that there exist \(V(t,x,i)\in C^{1,2}\left( ]-\tau ,+\infty [\times {\mathbb {R}}^n\times S,{\mathbb {R}}^+\right) \) and \(\gamma \in C({\mathbb {R}};{\mathbb {R}}_+)\) as well as a nonnegative constant \(\nu \), independent of \(t_0\), such that
-
(i)
\(\displaystyle {c_1|x|^q\le V(t,x,i)\le c_2|x|^q}\) for \(x\in {\mathbb {R}}^n\).
-
(ii)
\(\displaystyle {LV(t,{\widetilde{\varphi }}(0),i)\ge -c_3|{\widetilde{\varphi }}(0)|^q + \gamma (t)},\; \forall (t,\varphi ,i) \in {\mathbb {R}}^+\times C([-\tau ,0];{\mathbb {R}}^n)\times S\) where \(\varphi \in C([-\tau ,0];{\mathbb {R}}^n)\) and \({\widetilde{\varphi }}(0)=\varphi (0)-G(\varphi )\).
-
(iii)
\(\displaystyle {\inf _{t\ge t_{0}}\int _{t_0}^{t}e^{\frac{c_3}{c_1}s}\gamma (s)\mathrm{d}s\ge \nu }\).
Let assumptions \({\mathcal {A}}_1\), \({\mathcal {A}}_2\) and \({\mathcal {H}}_3\) hold. Assume that the constant k in assumption \({\mathcal {H}}_3\) verifies \(k^q<\beta \left( 1+\beta ^{\frac{1}{q-1}}\right) ^{1-q}\) and \(k^q<\alpha \); for \(\alpha \), \(\beta >0\) and \(q>1\). Then, the solution of equation (2.1) is practically qth moment exponentially unstable.
Proof
Define the stopping time \(\displaystyle {\sigma _l=\inf \{t\ge t_{0}; |x(t)|\ge l\}}\). Let \(x_t=\varphi \), \(x(t)=\varphi (0)\) and \({\widetilde{\varphi }}(0)=x(t)-G(x_t)\) for \(t\ge t_0\). By Itô’s formula, we obtain for \(t\ge -\tau \):
Therefore, by inequality (i),
Obviously \(\sigma _l\rightarrow \infty \) as \(l\rightarrow \infty \). Then
First case: For \(0<q\le 1\), by Lemma 3.2 and Assumption \({\mathcal {A}}_3\), we have
On the other hand, by inequality (i), we obtain
Then
This implies
Thus, for any \(T>0\),
Letting \(T\rightarrow +\infty \), we obtain
Therefore, for all \(t\ge t_0\), we have
Setting
the result is proved.
Second case: For \(q>1\), by Lemma 3.2 and Assumption \({\mathcal {A}}_3\), for \(\alpha >0\) and \(\beta >0\) such that
and \(k^q<\alpha \), we have,
By inequality (i),
Then
This implies
Hence, for any \(T>0\), we have
Letting \(T\rightarrow +\infty \), we obtain
Therefore, for all \(t\ge t_0\),
where
and
Finally,
Setting \(\displaystyle {c = \min \Big \{C_1(\alpha ,\beta ,k),C\Big \}}\), \(\displaystyle {\alpha =\frac{c_3}{c_1}}\) and \(\displaystyle {r(t)=\min \Big \{r_1(t),r_2(t)\Big \}}\), we conclude that the solution of system (2.1) is practically exponentially unstable in q-th moment \((q>0)\).
\(\square \)
5 Example
We consider the following neutral stochastic functional differential equation with Markovian switching:
Let \(t_0=0\), the initial data \(x_0=x(\lambda )=\xi =(\xi _1,\xi _2,\xi _3)\in C^b_{{\mathcal {F}}_0}([-1, 0];{\mathbb {R}}^3)\) and \(\{W_i(t)\}_{i\in \{1,2,3\}}\) are one-dimensional Brownian motions. Let
where m is a probability measure defined on \([-1,0]\) satisfying \(\int _{-1}^{0}\mathrm{d}m(\theta )=1\). Let \({\widetilde{\varphi }}(0)=\widetilde{x}(t)=(\widetilde{x}_1(t),\widetilde{x}_2(t),\widetilde{x}_3(t)),\) where \(\widetilde{x}_i(t)=x_i(t)-\frac{1}{2}e^{-\frac{1}{2}}x_i(t-1)\) for \(i\in \{1,2,3\}\). Let \(S=\{1,2,3\}\) and the matrix \(\Gamma =(\gamma _{ij})_{1\le i,j\le 3}\) defined by
where \(1< \gamma <2\).
We will prove that system (5.1) is practically exponentially unstable in mean square with respect to all variables.
Let \(V(t,x,i)=\psi _i(x_1^2+x_2^2+x_3^2)\), for \(i\in S\), where \(\psi _1=\psi _3=1,\) \(\psi _2=\frac{1}{2}\). Then
Let \(U_1(t,x)=\frac{1}{2}\left| x\right| ^2\) and \(U_2(t,x)=\left| x\right| ^2\). By the definition of LV, we have for \(i=1\)
By the Hölder inequality, we have
For \(i=2\), we have
By the Hölder inequality,
For \(i=3\), proceeding as \(i=1\) and \(i=2\), we have
By the Hölder inequality, we have
Then for \(i\in S\),
Thus, assumption \({\mathcal {A}}_2\) is satisfied.
For all \(\varphi _1=y_t\), \(\varphi _2=z_t\in C([-\tau ,0];{\mathbb {R}}^n)\).
then assumption \({\mathcal {A}}_3\) is satisfied with \(k=\frac{1}{2}\).
It is easy to verify assumptions \({\mathcal {A}}_1\). Therefore, by Theorem 3.1, system (5.1) has a unique solution \(x(t)=(x_1(t),x_2(t),x_3(t))\).
Therefore, for \(i\in S\)
Finally,
Hence, by Theorem 4.3, system (5.1) is practically exponentially unstable in mean square.
Now, we define \(V_1\) for \(i\in S\) for \({\widetilde{\varphi }}_{1}(0)=\widetilde{x}_{3}(t)\) by
This implies that
Then for \(i=1\),
Finally, we obtain
In the same way, for \(i=2\),
Therefore,
On the other hand, for \(i=3\),
Therefore,
Then, from inequalities (2.5), (5.5) and (5.6), for any \(i\in S\), we have
Hence,
It is easy to verify that \(V_1\) satisfies assumption \({\mathcal {A}}_2\) with \(U_1(t,x)=\frac{1}{2}x_3^2\), \(U_2(t,x)=x_3^2\), \(c_1'=1\), \(c_2'=\frac{1}{2}\) and \(c_3'=0\).
Thus, assumptions of Theorem 3.3 are satisfied with \(c_1=\frac{1}{2}\), \(c_2=1\), \(c_3=\frac{1}{2}\), \(p=2\), \(\delta =1\), \(\rho (t)=e^{-2t}\), \(k\in [0,\frac{\sqrt{2}}{2})\) and \(\frac{c_3}{c_2}\le \delta \). Then system (5.1) is practically exponentially \(x_3\)-stable in mean square.
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Acknowledgements
The research of T. C. has been partially supported by Ministerio de Ciencia, Innovación y Universidades (Spain), FEDER (European Community) under grant PGC2018-096540-B-I00, and Junta de Andalucía (Spain) under grant US-1254251. Lassad Mchiri and Mohamed Rhaima extend their appreciation to the Deanship of Scientific Research at King Saud University for funding this work through research gourp No. RG-1441-328.
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Caraballo, T., Mchiri, L. & Rhaima, M. Partial Practical Exponential Stability of Neutral Stochastic Functional Differential Equations with Markovian Switching. Mediterr. J. Math. 18, 142 (2021). https://doi.org/10.1007/s00009-021-01786-6
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DOI: https://doi.org/10.1007/s00009-021-01786-6
Keywords
- Neutral stochastic functional differential equations
- Markovian switching
- Lyapunov techniques
- partial exponential stability