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The Existence and Averaging Principle for Caputo Fractional Stochastic Delay Differential Systems with Poisson Jumps

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24 November 2023

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27 November 2023

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Abstract
In this paper, we obtain the existence and uniqueness theorem for solutions of Caputo type fractional stochastic delay differential systems (FSDDSs) with Poisson jumps by utilizing delayed perturbation of Mittag-Leffler function. Moreover, by using Burkholder-Davis-Gundy's inequality, Doob's martingale inequality and Holder inequality, we prove that the solution of the averaged FSDDSs converges to that of the standard FSDDSs in the sense of Lp. Some known results in the literature are extended.
Keywords: 
Subject: Computer Science and Mathematics  -   Analysis

1. Introduction

Fractional stochastic delay differential systems (FSDDs) are mathematical models that involve fractional derivatives, stochastic noise, and time delays. The fractional derivatives represent the memory effects and long-range dependence in the system, while the stochastic noise and delays account for the random fluctuations and time delays, respectively. FSDDs find applications in many fields, including physics, biology, finance, and engineering. They can be used to model systems with memory and randomness, such as anomalous diffusion processes, fractional-order control systems with stochastic disturbances, and biological systems with fractional-order kinetics and stochastic effects. They provide a powerful framework for understanding and predicting the behavior of complex systems with memory, randomness, and time delays. See for examples [1-6], and the references cited therein.
The averaging principle is a mathematical tool used to simplify the analysis of dynamical systems with fast and slow time scales. It provides an approximate description of the system’s behavior. In 1968, Khasminskii [7] first used the average principle to prove that the solution of the average equation can converge to the solution of the complex system. In [8], the authors presented an averaging method for stochastic differential equations with non-Gaussian L e ´ vy noise. With the development of fractional calculus, many works have emerged that apply the averaging principle to fractional stochastic differential equations (FSDEs). In [9], Xu, et.al. presents an averaging principle for Caputo FSDEs driven by Brown motion. In [10], Luo, et.al. established an averaging principle for the solution of the a class of FSDEs with time-delays. In [11], Ahmed and Zhu investigated the averaging principle for the Hilfer fractional stochastic delay differential equation with Poisson jumps in the sense of mean square. The periodic averaging method for impulsive conformable fractional stochastic differential equations with Poisson jumps are discussed in [12] by Ahmed. In [13], Wang and Lin extended the averaging principle of the following FSDEs
  C D 0 α [ x ( t ) h ( t , x ( t ) ] = f ( t , x ( t ) ) + g ( t , x ( t ) ) d B t d t , t J = [ 0 , T ] , x ( 0 ) = x 0 ,
in the sense of mean square ( L 2 convergence) to L p convergence ( p 2 ), which generated some works on the averaging principle for FSDES [9,10,14]. In [15], Yang, et.al. studied the averaging principle for a class of ψ -Capuo fractional stochastic delay differential equations with Poisson jumps.
Recently, Li and Wang in [16] studied the following Caputo type FSDDEs:
( C D 0 α Y ) ( t ) = A Y ( t ) + B Y ( t h ) + f ( t , Y ( t ) ) + σ ( t , Y ( t ) ) d W ( t ) d t , t J , Y ( t ) = Φ ( t ) , h t 0 , h > 0 ,
the existence, uniqueness and the averaging principle for (1.2) are established.
In the present paper, motivated by [11,13,16], we study the following Caputo FSDDEs with Poisson jumps
( C D 0 α x ) ( t ) = A x ( t ) + B x ( t τ ) + f ( t , x ( t ) , x ( t τ ) ) + σ ( t , x ( t ) , x ( t τ ) ) d W ( t ) d t , + V g ( t , x ( t ) , x ( t τ ) , v ) N ¯ ( d t , d v ) , t J , x ( t ) = ϕ ( t ) , τ t 0 ,
where   C D 0 α is the left Caputo fractional derivative with 1 2 < α < 1 , J = [ 0 , T ] , A , B R n × n are two constant matrices, the state vector x R n is a stochastic process, f : J × R n × R n R n , σ : J × R n × R n R n × m and g : J × R n × R n × V R n are measurable continuous functions. Let ( Ω , F , P ) be a complete probability space equipped with some filtration ( F t ) t 0 satisfying the usual condition, W ( t ) is an m-dimensional Brownian motion on the probability space ( Ω , F , P ) adapted to the filtration ( F t ) t 0 . Let ( V , Φ , λ ( d v ) ) be a σ -finite measurable space. Given stationary Poisson point process ( p t ) t 0 , which is defined on ( Ω , F , P ) with values in V and with characteristic measure λ . We denote by N ( t , d v ) the counting measure of p t such that N ¯ ( t , Θ ) : = E ( N ( t , Θ ) ) = t λ ( Θ ) for Θ Φ . Define N ¯ ( t , d v ) : = N ( t , d v ) t λ ( d v ) , and the Poisson martingale measure generated by p t .
In this paper, we first prove the existence and uniqueness of solutions of Caputo type FSDDEs (1.3) by using delayed perturbation of Mittag-Leffler function and Banach fixed point theorem; Secondly, we prove the averaging principle for Caputo FSDDEs (1.3) in the sense of L p (pth moment) with inequality techniques. The main contributions and advantages of this paper are as follows:
(1) The solution of the averaged FSDDEs converges to that of the standard FSDDEs in the sense of L p , which is a generalization of the existing result ( p = 2 ) of the averaging principle for FSDDEs,
(2) The fractional calculus, stochastic inequality and H o ¨ lder inequality are effectively used to establish our result.
(3) our work in this paper is novel and more technical. Our result extends the main results of [17].
This paper will be organized as follows. In Section 2, we will briefly recall some definitions and preliminaries. In Section 3, we prove the existence and uniqueness of solutions for Caputo FSDDEs (1.3) with Poisson jumps. In Section 4, we prove that the solution of the FSDDEs (1.3) converges to that of the standard one in L p sense. In Section 5, an example is presented to illustrate our theoretical results. Finally, the paper is concluded in Section 6.

2. Preliminaries

In this section, we recall some basic definitions and lemmas which are used in the sequel.
Let Υ = L p ( Ω , F , P ) denote the space of all F ( t ) measurable, p squqre integrable functions x : Ω R n with x ( t ) p s : = i = 1 n E ( | x i ( t ) | p ) 1 / p , and x = i = 1 n | x i | and A = max 1 i n i = 1 n | a i j | be the vector norm and matrix norm, respectively. A process x : [ τ , T ] L p ( Ω , F , P ) is said to be F ( t ) -adapted if x ( t ) Υ .
Definition 2.1 [17]. Let α > 0 , and f be an integrable function defined on [ a , b ] . The left Riemann-Liouville fractional integral operator of order α of a function f is defined by
  a I t α f ( t ) = 1 Γ ( α ) a t ( t s ) α 1 f ( s ) d s , t > a .
Definition 2.2 [17]. Let n 1 < α < n , and f C n ( [ a , b ] ) . The left Caputo fractional derivative of order α of a function f is defined by
  a C D t α f ( t ) = ( a I t n α f ( n ) ) ( t ) = 1 Γ ( n α ) a t ( t s ) n α 1 f ( n ) ( s ) d s , t > a ,
where n = [ α ] + 1 .
Definition 2.3 [18]. The coefficient matrices Q k ( s ) , k = 0 , 1 , 2 , . . . , satisfy the following multivariate determining matrix equation
Q 0 ( s ) = Q k ( τ ) = Θ , Q 1 ( 0 ) = I , k = 0 , 1 , 2 , , s = 0 , τ , 2 τ , ,
Q k + 1 ( s ) = A Q k ( s ) + B Q k ( s τ ) , k = 0 , 1 , 2 , , s = 0 , τ , 2 τ , ,
where I is an identity matrix and Θ is a zero matrix.
Definition 2.4 [18]. Delayed perturbation of two parameter Mittag-Leffler type matrix function X τ , α , β A , B generated by A , B is defined by
X τ , α , β A , B ( t ) : = Θ , t [ τ , 0 ) , I , t = 0 , i = 0 Q i + 1 ( 0 ) t i α + β 1 Γ ( i α + β ) + i = 1 Q i + 1 ( τ ) ( t τ ) i α + β 1 Γ ( i α + β ) + + i = 0 Q i + 1 ( p τ ) ( t p τ ) i α + β 1 Γ ( i α + β ) , p τ < t ( p + 1 ) τ .
From [17], we can easily obtain the following definition.
Definition 2.5. A R n -value stochastic process { x ( t ) : τ t T } is called a solution of (1.3) if x ( t ) satisfies the integral equation of the following form:
x ( t ) = X τ , α , 1 A , B ( t + τ ) ϕ ( τ ) + τ 0 X τ , α , α A , B ( t s ) [ C D τ + α ϕ ) ( s ) A ϕ ( s ) ] d s + 0 t X τ , α , α A , B ( t s ) f ( s , x ( s ) , x ( s τ ) ) d s + 0 t X τ , α , α A , B ( t s ) σ ( s , x ( s ) , x ( s τ ) ) d W ( s ) + 0 t X τ , α , α A , B ( t s ) V g ( s , x ( s ) , x ( s τ ) , v ) N ¯ ( d s , d v ) , t J , ϕ ( t ) , t [ τ , 0 ] ,
where x ( t ) is F ( t ) -adapted and E ( τ T x ( t ) p d t ) < .
Lemma 2.1 ([19]). For any t 0 , 0 < α < 1 , 0 < β 1 and α + β 1 , we have
X τ , α , β A , B ( t ) t β 1 E α , β ( ( A + B ) t α ) ,
where E α , β ( z ) = k = 0 z k Γ ( k α + β ) , z R is the Mittag-Leffler function.
Lemma 2.2For any p 2 , α 1 1 p , 1 and γ > 0 , one has
0 t ( t s ) p α p E p α p + 1 , 1 ( γ s p α p + 1 ) d s Γ ( p α p + 1 ) γ E p α p + 1 , 1 ( γ t p α p + 1 ) ,
where Γ ( α ) : = 0 + s α 1 e s d s is the Gamma function.
Proof. Let γ > 0 be arbitrary. Consifer the corresponding linear Caputo fractional differential equation of the following form
  C D 0 + p α p + 1 x ( t ) = γ x ( t ) .
From [20], it is easy to know that the Mittag-Leffler function E p α p + 1 , 1 ( γ t p α p + 1 ) is a solution of (2.7). So, the following equality holds:
E p α p + 1 , 1 ( γ t p α p + 1 ) = 1 + γ Γ ( p α p + 1 ) 0 t ( t s ) p α p E p α p + 1 , 1 ( γ s p α p + 1 ) d s ,
which completes the proof.
Lemma 2.3 ([21, 22]). Let ϕ : R + × V R n and assume that
0 t V | ϕ ( s , v ) | p λ ( d v ) d s < , p 2 .
Then there exists D p > 0 such that
E sup 0 t u 0 t V ϕ ( s , v ) N ¯ ( d s , d v ) p D p E 0 u V | ϕ ( s , v ) | 2 λ ( d v ) d s p 2 + E 0 u V | ϕ ( s , v ) | p λ ( d v ) d s .
Lemma 2.4 ([23]). Let u , v be two integrable functions and g be continuous defined on domain [ a , b ] . Moreover, assume that
(1) u and v are nonnegative, and v is nondecreasing;
(2) g is nonnegative and nondecreasing.
If
u ( t ) v ( t ) + g ( t ) a t ( t τ ) α 1 u ( τ ) d τ ,
then
u ( t ) v ( t ) E α ( g ( t ) Γ ( α ) ( t a ) α ) , t [ a , b ] ,
where E α ( · ) is the Mittag-Leffler function.
To study the qualitative properties of solution for (1.3), we impose the following conditions on data of the problem.
(H1) For any x 1 , x 2 , y 1 , y 2 R n and t J , there exist two constants C 1 , C 2 > 0 such that
f ( t , x 1 , y 1 ) f ( t , x 2 , y 2 ) p σ ( t , x 1 , y 1 ) σ ( t , x 2 , y 2 ) p
V g ( t , x 1 , y 1 , v ) g ( t , x 2 , y 2 , v ) p λ ( d v ) C 1 p ( x 1 x 2 p + y 1 y 2 p ) ,
where · is the norm of R n , x y = m a x { x , y } .
(H2) Let σ ( · , 0 , 0 ) and g ( · , 0 , 0 ) are essentially bounded, i.e.
σ ( · , 0 , 0 ) : = e s s sup t [ 0 , ) σ ( t , 0 , 0 ) < + , g ( · , 0 , 0 ) : = e s s sup t [ 0 , ) g ( t , 0 , 0 ) < + ,
and f ( · , 0 , 0 ) is L p integrable, i.e.
f L p = 0 T f ( t , 0 , 0 ) p d t < + .

3. Existence and uniqueness result

Let H p ( [ 0 , T ] ) be the space of all the processes x which are measurable, F ( t ) -adapted, and satisfied that x H p : = sup 0 t T x ( t ) p s < . Obviously, ( H p ( [ 0 , T ] ) , · H p ) is a Banach space. Set μ = A + B . For any t [ τ , T ] and ϕ C ( [ τ , 0 ] , R n ) , we define an operator T : H p ( [ 0 , T ] ) H p ( [ 0 , T ] ) as follows :
( T x ) ( t ) = X τ , α , 1 A , B ( t + τ ) ϕ ( τ ) + τ 0 X τ , α , α A , B ( t s ) [ C D τ + α ϕ ) ( s ) A ϕ ( s ) ] d s + 0 t X τ , α , α A , B ( t s ) f ( s , x ( s ) , x ( s τ ) ) d s + 0 t X τ , α , α A , B ( t s ) σ ( s , x ( s ) , x ( s τ ) ) d W ( s ) + 0 t X τ , α , α A , B ( t s ) V g ( s , x ( s ) , x ( s τ ) , v ) N ¯ ( d s , d v ) .
Lemma 3.1Let 1 1 p < α < 1 . Assume that (H1) and (H2) hold. Then the operator T is well-defined.
Proof. For any x H p ( [ 0 , T ] ) , by (3.1) and the following elementary inequality
i = 1 m a i p m p 1 i = 1 5 a i p , a i R n , i = 1 , 2 , . . . , m .
we have
( T x ) ( t ) p s p 5 p 1 E ( X τ , α , 1 A , B ( t + τ ) ϕ ( τ ) p ) + 5 p 1 E τ 0 X τ , α , α A , B ( t s ) [ ( C D τ + α ϕ ) ( s ) A ϕ ( s ) ] d s p + 5 p 1 E 0 t X τ , α , α A , B ( t s ) f ( s , x ( s ) , x ( s τ ) ) d s p + 5 p 1 E 0 t X τ , α , α A , B ( t s ) σ ( s , x ( s ) , x ( s τ ) ) d W ( s ) p + 5 p 1 E 0 t X τ , α , α A , B ( t s ) V g ( s , x ( s ) , x ( s τ ) , v ) N ¯ ( d s , d v ) p : = I 1 + I 2 + I 3 + I 4 + I 5 .
For I 1 , from Lemma 2.1, one has
I 1 = 5 p 1 E ( X τ , α , 1 A , B ( t + τ ) ϕ ( τ ) p ) 5 p 1 E ( X τ , α , 1 A , B ( t + τ ) p ϕ ( τ ) p ) 5 p 1 ϕ ( τ ) p ( E α , 1 ( μ ( T + τ ) ) α ) ) p .
For I 2 , by Lemma 2.1, H o ¨ lder inequality and α > 1 1 p , we obtain
I 2 = 5 p 1 E τ 0 X τ , α , α A , B ( t s ) [ ( C D τ + α ϕ ) ( s ) A ϕ ( s ) ] d s p 5 p 1 τ 0 X τ , α , α A , B ( t s ) p d s · E τ 0 ( C D τ + α ϕ ) ( s ) A ϕ ( s ) q d s p 1 5 p 1 Ξ ( T + τ ) p α p + 1 p α p + 1 ( E α , α ( μ ( T + τ ) α ) ) ) p ,
where 1 p + 1 q = 1 and Ξ = τ 0 ( C D τ + α ϕ ) ( s ) A ϕ ( s ) q d s p 1 < .
For I 3 , applying (H1), (H2), H o ¨ lder inequality, Lemma 2.1 and Jensen inequality, one has
I 3 = 5 p 1 E 0 t X τ , α , α A , B ( t s ) f ( s , x ( s ) , x ( s τ ) ) d s p 5 p 1 0 t X τ , α , α A , B ( t s ) q d s p q · E 0 t f ( s , x ( s ) , x ( s τ ) ) f ( s , 0 , 0 ) + f ( s , 0 , 0 ) p d s 5 p 1 0 t t q ( α 1 ) E α , α ( μ ( t s ) α ) q d s p q · 2 p 1 E 0 t f ( s , x ( s ) , x ( s τ ) ) f ( s , 0 , 0 ) p d s + 0 t f ( s , 0 , 0 ) p d s 10 p 1 E α , α ( μ T α ) p T q α q + 1 q α q + 1 p q E 0 t C 1 p ( x ( s ) p + x ( s τ ) p ) d s + 0 t f ( s , 0 , 0 ) p d s 10 p 1 E α , α ( μ T α ) p T q α q + 1 q α q + 1 p q T C 1 p ( 2 x H p p + ϕ q ) + f L p ,
since
sup 0 t T E x ( t τ ) q max sup τ t 0 E ϕ ( t ) q , sup 0 t T E x ( t ) q = max ϕ q , x H q q ϕ q + x H q q .
For I 4 , by using (H1), (H2), Cauchy-Schwarz inequality, Ito’s isometry, Lemma 2.1 and Jensen inequality, we have
I 4 = 5 p 1 E 0 t X τ , α , α A , B ( t s ) σ ( s , x ( s ) , x ( s τ ) ) d W ( s ) 2 p 2 5 p 1 E 0 t X τ , α , α A , B ( t s ) 2 σ ( s , x ( s ) , x ( s τ ) ) 2 d s p 2 5 p 1 E 0 t 1 p p 2 d s p 2 p · 0 t X τ , α , α A , B ( t s ) p σ ( s , x ( s ) , x ( s τ ) ) p d s 2 p p 2 5 p 1 T p 2 1 E 0 t X τ , α , α A , B ( t s ) p σ ( s , x ( s ) , x ( s τ ) ) p d s 5 p 1 T p 2 1 2 p 1 E α , α ( μ T α ) p E 0 t ( t s ) p α p [ C 1 p ( x ( s ) p + x ( s τ ) p ) + σ ( s , 0 , 0 ) p ] d s 10 p 1 T p α p 2 p α p + 1 E α , α ( μ T α ) p ( C 1 p ( 2 x H p p + ϕ p ) + σ ( · , 0 , 0 ) p ) .
For I 5 , by using (H1), (H2), Lemmas 2.1, 2.3 and Jensen inequality, we obtain
I 5 = 5 p 1 E 0 t V X τ , α , α A , B ( t s ) g ( s , x ( s ) , x ( s τ ) , v ) N ¯ ( d s , d v ) p 5 p 1 D p E 0 t V | X τ , α , α A , B ( t s ) | 2 g 2 ( s , x ( s ) , x ( s τ ) , v ) λ ( d v ) d s p 2 + 5 p 1 D p E 0 t V | X τ , α , α A , B ( t s ) | p g p ( s , x ( s ) , x ( s τ ) , v ) λ ( d v ) d s 5 p 1 D p ( T p 2 1 + 1 ) E 0 t | X τ , α , α A , B ( t s ) | p V g p ( s , x ( s ) , x ( s τ ) , v ) λ ( d v ) d s 5 p 1 D p ( T p 2 1 + 1 ) 2 p 1 E α , α ( μ T α ) p · E 0 t ( t s ) p α p [ C 1 p ( x ( s ) p + x ( s τ ) p ) + g ( s , 0 , 0 , 0 ) p ] d s 10 p 1 D p ( T p 2 1 + 1 ) T p α p + 1 p α p + 1 E α , α ( μ T α ) p ( C 1 p ( 2 x H p p + ϕ p ) + g ( · , 0 , 0 , 0 ) p ) .
Submitting (3.4)-(3.8) into (3.3), which implies that T x H p < . Thus, the operator T is well-defined.
Theorem 3.1Let 1 1 p < α < 1 . Assume that ( H 1 ) and ( H 2 ) hold, then (1.3) has a unique solution x H p ( [ 0 , T ] ) .
Proof. For T > 0 , we choosing and fix a constant γ > 0 such that
γ > 2 · 3 p 1 C 1 p E α , α ( μ T α ) p ( T p q + ( D p + 1 ) T p 2 1 + 1 ) Γ ( p α p + 1 ) .
On the space H p ( [ 0 , T ] ) , we define a weighted norm · γ as below
x γ : = sup t [ 0 , T ] E ( x ( t ) p ) E p α p + 1 , 1 ( γ t p α p + 1 ) 1 p , x H p ( [ 0 , T ] ) .
Similar to the Theorem 1 in [18], It is easy to know that the norms · H p and · γ are equivalent. Hence, ( H p ( [ 0 , T ] ) , · γ ) is a Banach space. We can easily prove that T : H p ( [ 0 , T ] ) H p ( [ 0 , T ] ) defined in (3.1) is uniformly bounded operator by Lemma 3.1. Next, we only check that T is a contraction operator.
Firstly, by using H o ¨ lder inequality, (H1) and Lemma 2.1, we obtain
0 t X τ , α , α A , B ( t s ) ( f ( s , x ( s ) , x ( s τ ) ) f ( s , y ( s ) , y ( s τ ) ) ) d s p 0 t 1 q d s p q · 0 t X τ , α , α A , B ( t s ) p f ( s , x ( s ) , x ( s τ ) ) f ( s , y ( s ) , y ( s τ ) ) p d s t p q 0 t ( t s ) p ( α 1 ) E α , α ( μ ( t s ) α ) p f ( s , x ( s ) , x ( s τ ) ) f ( s , y ( s ) , y ( s τ ) ) p d s T p q E α , α ( μ T α ) p C 1 p 0 t ( t s ) p ( α 1 ) ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ ) p ) d s .
Secondly, similar to the proof of (3.7), one has
0 t X τ , α , α A , B ( t s ) ( σ ( s , x ( s ) , x ( s τ ) ) σ ( s , y ( s ) , y ( s τ ) ) ) d W ( s ) p T p 2 1 0 t X τ , α , α A , B ( t s ) p σ ( s , x ( s ) , x ( s τ ) ) σ ( s , y ( s ) , y ( s τ ) ) p d s T p 2 1 E α , α ( μ T α ) p 0 t ( t s ) p α p [ C 1 p ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ ) p ) d s T p 2 1 C 1 p E α , α ( μ T α ) p 0 t ( t s ) p α p ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ ) p ) d s .
Thirdly, similar to the proof of (3.8), we obtain
0 t X τ , α , α A , B ( t s ) V ( g ( s , x ( s ) , x ( s τ ) , v ) g ( s , y ( s ) , y ( s τ ) , v ) ) N ¯ ( d s , d v )
D p 0 t X τ , α , α A , B ( t s ) 2 V g ( s , x ( s ) , x ( s τ ) , v ) g ( s , y ( s ) , y ( s τ ) , v ) 2 λ ( d v ) d s p 2
+ D p 0 t | X τ , α , α A , B ( t s ) | p V | g ( s , x ( s ) , x ( s τ ) , v ) g ( s , y ( s ) , y ( s τ ) , v ) | p λ ( d v ) d s
D p ( T p 2 1 + 1 ) 0 t X τ , α , α A , B ( T s ) p V g ( s , x ( s ) , x ( s τ ) , v ) g ( s , y ( s ) , y ( s τ ) , v ) p λ ( d v ) d s
D p C 1 p ( T p 2 1 + 1 ) E α , α ( μ T α ) p 0 t ( t s ) p α p ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ p ) d s .
(3.12)
For each x , y H p ( [ 0 , T ] ) , from (3.1), (3.2), and (3.10)-(3.12), we have
E ( T x ( t ) T y ( t ) p )
3 p 1 E 0 t X τ , α , α A , B ( t s ) ( f ( s , x ( s ) , x ( s τ ) ) f ( s , y ( s ) , y ( s τ ) ) ) d s p
+ 3 p 1 E 0 t X τ , α , α A , B ( t s ) ( σ ( s , x ( s ) , x ( s τ ) ) σ ( s , y ( s ) , y ( s τ ) ) ) d W ( s ) p
+ 3 p 1 E 0 t X τ , α , α A , B ( t s ) V ( g ( s , x ( s ) , x ( s τ ) , v ) g ( s , y ( s ) , y ( s τ ) , v ) ) N ¯ ( d s , d v ) p
3 p 1 T p q C 1 p E α , α ( μ T α ) p 0 t ( t s ) p ( α 1 ) E ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ p ) d s
+ 3 p 1 T p 2 1 C 1 p E α , α ( μ T α ) p 0 t ( t s ) p α p E ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ p ) d s
+ 3 p 1 C 1 p D p ( T p 2 1 + 1 ) E α , α ( μ T α ) p 0 t ( t s ) p α p E ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ p ) d s
= ω 0 t ( t s ) p α p E ( x ( s ) y ( s ) p + x ( s τ ) y ( s τ p ) d s ,
(3.13)
where
ω : = 3 p 1 C 1 p E α , α ( μ T α ) p ( T p q + ( D p + 1 ) T p 2 1 + D p ) .
For t > τ , one has
0 t ( t s ) p ( α 1 ) x ( s τ ) y ( s τ ) p d s = 0 τ + τ t ( t s ) p ( α 1 ) x ( s τ ) y ( s τ ) p d s
= τ t ( t s ) p ( α 1 ) x ( s τ ) y ( s τ ) p d s
= 0 t τ ( t τ u ) p ( α 1 ) x ( u ) y ( u ) p d u . (3.14)
From Lemma 2.2, combining (3.13) and (3.14), for each t [ 0 , T ] , we get
E ( T x ( t ) T y ( t ) p ) E p α p + 1 , 1 ( γ t p α p + 1 ) ω E p α p + 1 , 1 ( γ t p α p + 1 ) 0 t ( t s ) p α p E p α p + 1 , 1 ( γ s p α p + 1 ) d s x y γ p + ω E p α p + 1 , 1 ( γ ( t τ ) p α p + 1 ) 0 t τ ( t τ u ) p α p E p α p + 1 , 1 ( γ u p α p + 1 ) d u x y γ p 2 ω Γ ( p α p + 1 ) γ x y γ p ,
which implies that
T x T y γ ρ x y γ ,
where ρ = 2 ω Γ ( p α p + 1 ) γ 1 p .
Based on (3.9), one can obtain ρ < 1 and the operator T is a contractive. Thus, there exists a unique solution of (1.3) by using of the Banach fixed point theorem. The proof of this theorem is complete.

4. An averaging principle

In this section, we shall investigate the averaging principle for Caputo type FSDDEs. For any t J , we consider the following standard form of (1.3)
x ϵ ( t ) = X τ , α , 1 A , B ( t + τ ) ϕ ( τ ) + τ 0 X τ , α , α A , B ( t s ) [ C D τ + α ϕ ) ( s ) A ϕ ( s ) ] d s + ϵ 0 t X τ , α , α A , B ( t s ) f ( s , x ( s ) , x ( s τ ) ) d s + ϵ 0 t X τ , α , α A , B ( t s ) σ ( s , x ( s ) , x ( s τ ) ) d W ( s ) + ϵ 0 t X τ , α , α A , B ( t s ) V g ( s , x ( s ) , x ( s τ ) , v ) N ¯ ( d s , d v ) ,
where ϵ ( 0 , ϵ 0 ] is a positive small parameter with ϵ 0 being a fixed number.
Consider the averaged form which corresponds to the standard form (4.1) as follows :
y ϵ ( t ) = X τ , α , 1 A , B ( t + τ ) ϕ ( τ ) + τ 0 X τ , α , α A , B ( t s ) [ C D τ + α ϕ ) ( s ) A ϕ ( s ) ] d s + ϵ 0 t X τ , α , α A , B ( t s ) f ^ ( s , y ( s ) , y ( s τ ) ) d s + ϵ 0 t X τ , α , α A , B ( t s ) σ ^ ( s , y ( s ) , y ( s τ ) ) d W ( s ) + ϵ 0 t X τ , α , α A , B ( t s ) V g ^ ( s , y ( s ) , y ( s τ ) , v ) N ¯ ( d s , d v ) ,
where f ^ : R n × R n R n , σ ^ : R n × R n R n × m , and g ^ : R n × R n × V R n satisfying the following averaging condition :
(H3) For any t J , x , y R n , and p 2 , there exists a positive bounded function φ i ( · ) , i = 1 , 2 , 3 such that
1 t 0 t f ( s , x , y ) f ^ ( x , y ) p d s φ 1 ( t ) ( 1 + x p + y p ) ,
1 t 0 t ( t s ) α 1 ( σ ( s , x , y ) σ ^ ( x , y ) ) p d s φ 2 ( t ) ( 1 + x p + y p ) ,
1 t 0 t V ( t s ) α 1 ( g ( s , x , y , v ) g ^ ( x , y , v ) ) p λ ( d v ) d s φ 3 ( t ) ( 1 + x p + y p ) ,
where lim t φ i ( t ) = 0 , i = 1 , 2 , 3 .
Theorem 4.1.Assume that (H1)-(H3) are satisfied. Then for a given arbitrary small number δ > 0 , p 2 with 1 1 p < α < 1 , there exist L > 0 , ϵ 1 ( 0 , ϵ 0 ] and β ( 0 , 1 ) such that
E sup t [ τ , L ϵ β ] | x ϵ ( t ) y ϵ ( t ) | p δ ,
for all ϵ ( 0 , ϵ 1 ] .
Proof. If p = 2 , it is easy to prove that (4.3) holds by using the similar method as in [20]. In the following, we will only consider the case of p > 2 . From Eqs. (4.2), (4.3), and inequality (3.2), we obtain
x ϵ ( t ) y ϵ ( t ) p 3 p 1 ϵ p 0 t X τ , α , α A , B ( t s ) [ f ( s , x ϵ ( s ) , x ϵ ( s τ ) ) f ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) ] d s p + 3 p 1 ϵ p 2 0 t X τ , α , α A , B ( t s ) [ σ ( s , x ϵ ( s ) , x ϵ ( s τ ) ) σ ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) ] d W ( s ) p + 3 p 1 ϵ p 2 0 t X τ , α , α A , B ( t s ) V [ g ( s , x ϵ ( s ) , x ϵ ( s τ ) , v ) ) g ^ ( x ϵ ( s ) , x ϵ ( s τ ) , v ) ) ] N ¯ ( d s , d v ) p .
For any t [ 0 , u ] [ 0 , T ] , taking the expectation on both sides Eq. (4.4), we have
E sup 0 t u x ϵ ( t ) y ϵ ( t ) p 3 p 1 ϵ p E sup 0 t u 0 t X τ , α , α A , B ( t s ) [ f ( s , x ϵ ( s ) , x ϵ ( s τ ) ) f ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) ] d s p + 3 p 1 ϵ p 2 E sup 0 t u 0 t X τ , α , α A , B ( t s ) [ σ ( s , x ϵ ( s ) , x ϵ ( s τ ) ) σ ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) ] d W ( s ) p + 3 p 1 ϵ p 2 E sup 0 t u 0 t X τ , α , α A , B ( t s ) V [ g ( s , x ϵ ( s ) , x ϵ ( s τ ) , v ) ) g ^ ( x ϵ ( s ) , x ϵ ( s τ ) , v ) ) ] N ¯ ( d s , d v ) p = I 1 + I 2 + I 3 .
Applying Jensen’s inequality, we get
I 1 6 p 1 ϵ p · E sup 0 t u 0 t X τ , α , α A , B ( t s ) [ f ( s , x ϵ ( s ) , x ϵ ( s τ ) ) f ( s , y ϵ ( s ) , y ϵ ( s τ ) ) ] d s p + 6 p 1 ϵ p · E sup 0 t u 0 t X τ , α , α A , B ( t s ) [ f ( s , y ϵ ( s ) , y ϵ ( s τ ) ) f ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) ] d s p = I 11 + I 12 .
Thanks to H o ¨ lder inequality and (H2), we obtain
I 11 6 p 1 ϵ p 0 u 1 q d s p q · E sup 0 t u 0 t X τ , α , α A , B ( t s ) p f ( s , x ϵ ( s ) , x ϵ ( s τ ) ) f ( s , y ϵ ( s ) , y ϵ ( s τ ) ) p d s 6 p 1 ϵ p u p 1 C 1 p E α , α ( μ u α ) p · E sup 0 t u 0 t ( t s ) p ( α 1 ) [ x ϵ ( s ) y ϵ ( s ) p + x ϵ ( s τ ) ) y ϵ ( s τ ) ) p ] d s 6 p 1 ϵ p u p 1 C 1 p E α , α ( μ u α ) p · 0 u ( u s ) p ( α 1 ) E sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p + E sup 0 θ s x ϵ ( θ τ ) y ϵ ( θ τ ) p d s 2 · 6 p 1 ϵ p u p 1 C 1 p E α , α ( μ u α ) p 0 u ( t s ) p ( α 1 ) E sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p d s ,
since
sup 0 θ s x ϵ ( θ τ ) y ϵ ( θ τ ) p sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p .
Applying H o ¨ lder inequality, we obtain
I 12 6 p 1 ϵ p · E sup 0 t u 0 t X τ , α , α A , B ( t s ) q d s p q · 0 t f ( s , y ϵ ( s ) , y ϵ ( s τ ) ) f ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) p d s 6 p 1 ϵ p E α , α ( μ u α ) p u q α q + 1 q α q + 1 p q · u φ 1 1 + E sup 0 t u y ϵ ( t ) p + E sup 0 t u y ϵ ( t τ ) p = 6 p 1 φ 1 M 1 ( q α q + 1 ) ( p 1 ) ϵ p E α , α ( μ u α ) p u p α ,
here φ 1 = sup t [ 0 , u ] | φ 1 ( t ) | , M 1 = 1 + E sup 0 t u y ϵ ( t ) p + E sup 0 t u y ϵ ( t τ ) p .
For the second term I 2 , we have
I 2 6 p 1 ϵ p 2 E sup 0 t u 0 t X τ , α , α A , B ( t s ) [ σ ( s , x ϵ ( s ) , x ϵ ( s τ ) ) σ ( s , y ϵ ( s ) , y ϵ ( s τ ) ) ] d W ( s ) p + 6 p 1 ϵ p 2 E sup 0 t u 0 t X τ , α , α A , B ( t s ) [ σ ( s , y ϵ ( s ) , y ϵ ( s τ ) ) σ ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) ] d W ( s ) p = I 21 + I 22 .
In view of the Burkholder-Davis-Gundy’s inequality, H o ¨ lder’s inequality and Doob’s martingale inequality, and (H1), one has
I 21 6 p 1 ϵ p 2 E sup 0 t u 0 t X τ , α , α A , B ( t s ) 2 σ ( s , x ϵ ( s ) , x ϵ ( s τ ) ) σ ( s , y ϵ ( s ) , y ϵ ( s τ ) ) 2 d s p 2 6 p 1 ϵ p 2 E sup 0 t u 0 t 1 p p 2 d s p 2 p · p 2 · 0 t X τ , α , α A , B ( t s ) p σ ( s , x ϵ ( s ) , x ϵ ( s τ ) ) σ ( s , y ϵ ( s ) , y ϵ ( s τ ) ) p d s 6 p 1 ϵ p 2 C 1 p u p 2 1 E α , α ( μ u α ) · 0 u ( u s ) p α p E sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p + E sup 0 θ s x ϵ ( θ τ ) y ϵ ( θ τ ) p d s 2 · 6 p 1 ϵ p 2 C 1 p u p 2 1 E α , α ( μ u α ) 0 u ( u s ) p α p E sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p d s .
Applying (H3) and an estimation method similar to Eq. (4.10), we get
I 22 6 p 1 ϵ p 2 u p 2 1 E sup 0 θ u 0 t X τ , α , α A , B ( t s ) p σ ( s , y ϵ ( s ) , y ϵ ( s τ ) ) σ ^ ( y ϵ ( s ) , y ϵ ( s τ ) ) p d s 6 p 1 ϵ p 2 u p 2 1 E α , α ( μ u α ) p u φ 2 1 + E sup 0 t u | y ϵ ( t ) | p + E sup 0 t u | y ϵ ( t τ ) | p = 6 p 1 M 1 φ 2 ϵ p 2 E α , α ( μ u α ) p u p 2 .
For the third term I 3 , we have
I 3 3 p 1 ϵ p 2 E sup 0 t u 0 t V X τ , α , α A , B ( t s ) [ g ( s , x ϵ ( s ) , x ϵ ( s τ ) , v ) g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) ] N ¯ ( d s , d v ) . p . + 3 p 1 ϵ p 2 E sup 0 t u 0 t V X τ , α , α A , B ( t s ) [ g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) g ^ ( y ϵ ( s ) , y ϵ ( s τ ) , v ) ] N ¯ ( d s , d v ) . p . = I 31 + I 32 .
From Lemma 2.3, similar to the proof of (3.8), one has
I 31 3 p 1 ϵ p 2 D p E sup 0 t u 0 t V X τ , α , α A , B ( t s ) 2 g ( s , x ϵ ( s ) , x ϵ ( s τ ) , v ) g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) 2 λ ( d v ) d s p 2 + 3 p 1 ϵ p 2 E sup 0 t u 0 t V X τ , α , α A , B ( t s ) p g ( s , x ϵ ( s ) , x ϵ ( s τ ) , v ) g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) p λ ( d v ) d s 3 p 1 ϵ p 2 ( D p u p 2 1 + 1 ) · E sup 0 t u 0 t V X τ , α , α A , B ( t s ) p g ( s , x ϵ ( s ) , x ϵ ( s τ ) , v ) g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) p λ ( d v ) d s 3 p 1 ϵ p 2 ( D p u p 2 1 + 1 ) E α , α ( μ u α ) p C 1 p · 0 u ( u s ) p α p E sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p + E sup 0 θ s x ϵ ( θ τ ) y ϵ ( θ τ ) p d s 2 · 3 p 1 C 1 p ϵ p 2 ( D p u p 2 1 + 1 ) E α , α ( μ u α ) p 0 u ( t s ) p α p E sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p d s .
Moreover, by (H3), we also have
I 32 3 p 1 ϵ p 2 D p E sup 0 t u 0 t V X τ , α , α A , B ( t s ) 2 g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) g ^ ( y ϵ ( s ) , y ϵ ( s τ ) , v ) 2 λ ( d v ) d s p 2
+ 3 p 1 ϵ p 2 E sup 0 t u 0 t V X τ , α , α A , B ( t s ) p g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) g ^ ( y ϵ ( s ) , y ϵ ( s τ ) , v ) p λ ( d v ) d s
3 p 1 ϵ p 2 ( D p u p 2 1 + 1 )
· E sup 0 t u 0 t V X τ , α , α A , B ( t s ) p g ( s , y ϵ ( s ) , y ϵ ( s τ ) , v ) g ^ ( y ϵ ( s ) , y ϵ ( s τ ) , v ) p λ ( d v ) d s
3 p 1 ϵ p 2 ( D p u p 2 1 + 1 ) E α , α ( μ u α ) p u φ 3 1 + E sup 0 t u y ϵ ( t ) p + E sup 0 t u y ϵ ( t τ ) p
3 p 1 M 1 φ 3 ϵ p 2 E α , α ( μ u α ) p ( D p u p 2 + u ) . (4.14)
From (4.5)-(4.14), for u ( 0 , T ] , we obtain
E sup 0 t u x ϵ ( t ) y ϵ ( t ) p A ( u ) + B ( u ) 0 u ( u s ) p α p E sup 0 θ s x ϵ ( θ ) y ϵ ( θ ) p d s ,
(4.15)
where
A ( u ) = 6 p 1 φ 1 M 1 ( q α q + 1 ) ( p 1 ) ϵ p E α , α ( μ u α ) p u p α + 6 p 1 M 1 φ 2 ϵ p 2 E α , α ( μ u α ) p u p 2 + 3 p 1 M 1 φ 3 ϵ p 2 E α , α ( μ u α ) p ( D p u p 2 + u ) ,
and
B ( u ) = 2 · 6 p 1 C 1 p ϵ p E α , α ( μ u α ) p u p 1 + 2 · 6 p 1 C 1 p ϵ p 2 E α , α ( μ u α ) p u p 2 1 + 2 · 3 p 1 C 1 p ϵ p 2 E α , α ( μ u α ) p ( D p u p 2 1 + 1 ) .
By using of Lemma 2.4, we get
E sup 0 t u x ϵ ( t ) y ϵ ( t ) p A ( u ) E p ( α 1 ) + 1 B ( u ) Γ ( p ( α 1 ) + 1 ) u p ( α 1 ) + 1 .
Choose L > 0 and β ( 0 , 1 ) such that for all t ( 0 , L ϵ β ] ( 0 , T ] satisfies the following
E sup 0 < t L ϵ β x ϵ ( t ) y ϵ ( t ) p A ¯ ( ϵ ) E p ( α 1 ) + 1 ( B ¯ ( ϵ ) Γ ( p ( α 1 ) + 1 ) ) ϵ 1 β ,
where
A ¯ ( ϵ ) = 6 p 1 E α , α ( μ T α ) p φ 1 M 1 ( q α q + 1 ) ( p 1 ) L p α ϵ p ( 1 α β ) + 6 p 1 M 1 φ 2 E α , α ( μ T α ) p L p 2 ϵ p 2 ( 1 β ) + 3 p 1 M 1 φ 3 E α , α ( μ T α ) p ( D p L p 2 ϵ p 2 ( 1 β ) + L ϵ p 2 β ) ,
and
B ¯ ( ϵ ) = 2 · 6 p 1 C 1 p E α , α ( μ T α ) p L p 1 ϵ p ( p 1 ) β + 2 · 6 p 1 C 1 p E α , α ( μ T α ) p L p 2 1 ϵ p 2 ( p 2 1 ) β + 2 · 3 p 1 C 1 p E α , α ( μ T α ) p ( D p L p 2 1 ϵ p 2 ( p 2 1 ) β + ϵ p 2 ) .
are two constants. Thus, for any given number δ > 0 , there exists ϵ 1 ( 0 , ϵ 0 ] such that for each ϵ ( 0 , ϵ 1 ] and t [ 0 , L ϵ β ] J ,
E sup t [ 0 , L ϵ β ] x ϵ ( t ) y ϵ ( t ) p δ .
Remark 4.1. If p = 2 and g 0 , then FSDDEs (1.3) reduces to FSDEs (1.1) in [14]. Therefore, Theorem 3.1 generalizes the main result of [14].
By using Theorem 4.1 and Chebyshev-Markov inequality, we can obtain the following Corollary.
Corollary 4.1.Assume that (H1)-(H3) are satisfied. Then for a given arbitrary small number δ > 0 , p 2 with 1 1 p < α < 1 , then for arbitrarily number δ ¯ > 0 such that for L > 0 , ϵ 1 ( 0 , ϵ 0 ] and β ( 0 , 1 ) satisfying for all ϵ ( 0 , ϵ 1 ]
lim ϵ 0 P sup t [ 0 , L e β ] x ϵ ( t ) y ϵ p > δ ¯ = 0 .

5. An Example

Example 5.1. Consider the following Caputo fractional stochastic delay differential equation (FSDDEs) with Poisson jumps :
( C D 0 0.7 x ) t ) = A x ( t ) + B x ( t 0.4 ) + f ( t , x ( t ) , x ( t 0.4 ) ) + σ ( t , x ( t ) , x ( t 0.4 ) ) d W ( t ) d t + V g ( t , x ( t ) , x ( t 0.4 ) , v ) N ¯ ( d t , d v ) , t J , x ( t ) = ϕ ( t ) , 0.4 t 0 ,
where α = 0.9 , τ = 0.4 , J = [ 0 , 4 ] , x ( t ) = ( x 1 ( t ) , x 2 ( t ) ) T , and
A = 0.3 0.1 0.15 0.2 , B = 0.2 0.1 0.15 0.25 , ϕ ( t ) = 1 1 2 ,
and
f ( t , x ( t ) , x ( t 0.4 ) ) = 1 3 e 2 t sin ( x 1 ( t ) ) + 1 4 e t sin 3 t arctan ( x 1 ( t 0.4 ) ) + 1 7 1 3 e 2 t cos ( x 2 ( t ) ) + 1 4 e t cos 3 t arctan ( x 2 ( t 0.4 ) ) + 1 6 ,
and
σ ( t , x ( t ) , x ( t 0.4 ) ) = 1 4 e t arctan ( x 1 ( t ) ) + 1 3 e 2 t cos 2 t sin ( x 1 ( t 0.4 ) ) + 1 3 1 4 e t sin ( x 2 ( t ) ) + 1 3 e t sin 2 t arctan ( x 2 ( t 0.4 ) ) + 1 6 ,
and
g ( t , x ( t ) , x ( t 0.4 ) , v ) = 1 2 1 3 .
For each x ( t ) , y ( t ) Υ and t [ 0 , T ] , we have
f ( t , x ( t ) , x ( t 0.4 ) ) f ( t , y ( t ) , y ( t 0.4 ) ) 1 3 | x 1 ( t ) y 1 ( t ) | + 1 4 | x 1 ( t 0.4 ) y 1 ( t 0.4 ) | + 1 3 | x 2 ( t ) y 2 ( t ) | + 1 4 | x 2 ( t 0.4 ) y 2 ( t 0.4 ) | 1 3 ( x ( t ) y ( t ) + x ( t 0.4 ) y ( t 0.4 ) ) .
Thus
f ( t , x ( t ) , x ( t 0.4 ) ) f ( t , y ( t ) , y ( t 0.4 ) ) 3 2 2 3 3 ( x ( t ) y ( t ) 3 + x ( t 0.4 ) y ( t 0.4 ) 3 ) ,
which implies that the function f satisfy the assumption (H1) and (H2). Similarly, we can obtain that the functions σ and g satisfy the assumption (H1) and (H2).
Let p = 3 . By calculation, we have μ = A + B = 0.8 , f L p = 0 4 f ( t , 0 , 0 ) 3 d t = 0.0651 , σ ( · , 0 , 0 ) = 1 2 , g ( · , 0 , 0 ) = 5 6 , C 1 = 4 27 and
Ξ = 0.4 0 ( C D 0 . 4 + 0.9 ϕ ) ( s ) A ϕ ( s ) 3 2 d s 2 2 0.4 0 ( ( C D 0 . 4 + 0.9 ϕ ) ( s ) 3 2 + A ϕ ( s ) 3 2 ) d s 2 2 0.4 0 1 Γ ( 0.1 ) 0.4 s ( s t ) 0.9 d t 1 2 Γ ( 0.1 ) 0.4 s ( s t ) 0.9 d t 3 2 + 0.35 0.25 3 2 2 2 0.4 0 3 2 Γ ( 1.1 ) 3 2 ( s + 0.4 ) 0.15 + 0 . 6 1.5 d s 2 = 1.5722 .
Hence, we may choose a suitable value γ > 0 such that
2 · 3 2 C 1 3 E 0.9 , 0.9 ( 0.8 · 4 0.9 ) 3 ( 4 2 + ( D 3 + 1 ) 2 + 1 ) Γ ( 0.7 ) < γ .
By Theorem 3.1, FSDDEs (5.1) has a unique solution x H 3 ( [ 0 , 4 ] ) .
In the following, we consider the standard form (4.1) as follows
( C D 0 0.7 x ϵ ) t ) = A x ϵ ( t ) + B x ϵ ( t 0.4 ) + ϵ f ( t , x ϵ ( t ) , x ϵ ( t 0.4 ) ) + ϵ σ ( t , x ϵ ( t ) , x ϵ ( t 0.4 ) ) d W ( t ) d t + ϵ V g ( t , x ϵ ( t ) , x ϵ ( t 0.4 ) , v ) N ¯ ( d t , d v ) , t J , x ϵ ( t ) = ϕ ( t ) , 0.4 t 0 ,
where x ϵ ( t ) = ( x 1 , ϵ ( t ) , x 2 , ϵ ( t ) ) T , and
f ( t , x ϵ ( t ) , x ϵ ( t 0.4 ) ) = 1 3 e 2 t sin ( x 1 , ϵ ( t ) ) + 1 4 e t sin 3 t arctan ( x 1 , ϵ ( t 0.4 ) ) + 1 7 1 3 e 2 t cos ( x 2 , ϵ ( t ) ) + 1 4 e t cos 3 t arctan ( x 2 , ϵ ( t 0.4 ) ) + 1 6 ,
and
σ ( t , x ϵ ( t ) , x ϵ ( t 0.4 ) ) = 1 4 e t arctan ( x 1 , ϵ ( t ) ) + 1 3 e 2 t cos 2 t sin ( x 1 , ϵ ( t 0.4 ) ) + 1 3 1 4 e t sin ( x 2 , ϵ ( t ) ) + 1 3 e 2 t sin 2 t arctan ( x 2 , ϵ ( t 0.4 ) ) + 1 6 ,
and
g ( t , x ϵ ( t ) , x ϵ ( t 0.4 ) , v ) = 1 2 1 3 .
Under conditions (H1) and (H2), by Theorem 3.1, FSDDEs (5.2) has a unique solution x ϵ given by
x ϵ ( t ) = X 0.4 , 0.9 , 1 A , B ( t + 0.4 ) ϕ ( 0.4 ) + 0.4 0 X 0.4 , 0.9 , 0.9 A , B ( t s ) [ C D 0 . 4 + 0.9 ϕ ) ( s ) A ϕ ( s ) ] d s + ϵ 0 t X 0.4 , 0.9 , 0.9 A , B ( t s ) f ( s , x ϵ ( s ) , x ϵ ( s 0.4 ) ) d s + ϵ 0 t X 0.4 , 0.9 , 0.9 A , B ( t s ) σ ( s , x ϵ ( s ) , x ϵ ( s 0.4 ) ) d W ( s ) + ϵ 0 t X 0.4 , 0.9 , 0.9 A , B ( t s ) V g ( s , x ϵ ( s ) , x ϵ ( s 0.4 ) , v ) N ¯ ( d s , d v ) .
By calculation, one has
f ¯ ( x ε ( t ) , x ε ( t τ ) ) = lim t 1 t 0 t f ( s , x ϵ ( s ) , x ϵ ( s τ ) ) d s = 1 7 1 6 ,
σ ¯ ( x ε ( t ) , x ε ( t τ ) ) = lim t 1 t 0 t σ ( s , x ε ( s ) , x ε ( s τ ) ) d s = 1 3 1 6 ,
g ¯ ( x ε ( t ) , x ε ( t τ ) , v ) = lim t 1 t 0 t g ( s , x ε ( s ) , x ε ( s τ ) , v ) d s = 1 2 1 3 .
We now check that the condition (H3) is satisfied. In fact, one has
1 t 0 t f ( s , x ε ( s ) , x ε ( s τ ) ) f ¯ ( x ε ( s ) , x ε ( s τ ) ) p d s = 1 t 0 t 1 3 e 2 s sin ( x 1 , ϵ ( s ) ) + 1 4 e s sin 3 s arctan ( x 1 , ϵ ( s 0.4 ) ) 1 3 e 2 s cos ( x 2 , ϵ ( s ) ) + 1 4 e s cos 3 s arctan ( x 2 , ϵ ( s 0.4 ) ) p d s = 1 3 p t 0 t ( e s ( | x 1 , ϵ ( s ) | + | x 2 , ϵ ( s ) | ) + e s ( | x 1 , ϵ ( s 0.4 ) | + | x 2 , ϵ ( s 0.4 ) | ) ) p d s = 1 3 p t 0 t ( e p s ( x ϵ ( s ) + x ϵ ( s 0.4 ) ) p d s 2 p 1 3 p t ( x ϵ ( s ) p + x ϵ ( s 0.4 ) p ) 0 t e p s d s = 2 p 1 ( 1 e p t ) 3 p p t ( 1 + x ϵ ( s ) p + x ϵ ( s 0.4 ) p ) .
1 t 0 t ( t s ) α 1 ( σ ( s , x ϵ ( s ) , x ϵ ( s τ ) ) σ ¯ ( x ϵ ( s ) , x ϵ ( s τ ) ) ) p d s = 1 t 0 t 1 4 ( t s ) α 1 e s arctan ( x 1 , ϵ ( s ) ) + 1 3 ( t s ) α 1 e 2 s cos 2 s sin ( x 1 , ϵ ( s 0.4 ) ) 1 4 ( t s ) α 1 e s sin ( x 2 , ϵ ( s ) ) + 1 3 ( t s ) α 1 e s sin 2 s arctan ( x 2 , ϵ ( s 0.4 ) ) p d s 2 p 1 3 p t ( x ϵ ( s ) p + x ϵ ( s 0.4 ) p ) 0 t ( t s ) p α p d s = 2 p 1 ( p α p + 1 ) 3 p t p α p ( 1 + x ϵ ( s ) p + x ϵ ( s 0.4 ) p ) .
1 t 0 t V ( t s ) α 1 ( g ( s , x ϵ ( s ) , x ϵ ( s 0.4 ) , v ) g ^ ( x ϵ ( s ) , x ϵ ( s 0.4 ) , v ) p λ ( d v ) d s = 1 t 0 t V 1 2 ( t s ) α 1 1 3 ( t s ) α 1 p λ ( d v ) d s = 1 t 5 6 p λ ( V ) 0 t ( t s ) p ( α 1 ) d s 5 p λ ( V ) ( p α p + 1 ) 6 p t p α p ( 1 + x ϵ ( s ) p + x ϵ ( s 0.4 ) p ) .
Thus, (H3) is satisfied with
φ 1 ( t ) = 2 p 1 ( 1 e p t ) 3 p p t , φ 2 ( t ) = 2 p 1 ( p α p + 1 ) 3 p t p α p , and φ 3 ( t ) = 5 p | Ω | ( p α p + 1 ) 6 p t p α p .
It is easy to check that the conditions of Theorem 4.1 and Corollary 4.1 are satisfied. So, as ϵ 0 , the original solution x ϵ ( · ) y ϵ ( · ) in the sense of p square ( p = 3 ) and in the probability, where
y ϵ ( t ) = X 0.4 , 0.9 , 1 A , B ( t + 0.4 ) ϕ ( 0.4 ) + 0.4 0 X 0.4 , 0.9 , 0.9 A , B ( t s ) [ C D 0 . 4 + 0.9 ϕ ) ( s ) A ϕ ( s ) ] d s + ϵ 0 t X 0.4 , 0.9 , 0.9 A , B ( t s ) f ^ ( y ϵ ( s ) , y ϵ ( s 0.4 ) ) d s + ϵ 0 t X 0.4 , 0.9 , 0.9 A , B ( t s ) σ ^ ( y ϵ ( s ) , y ϵ ( s 0.4 ) ) d W ( s ) + ϵ 0 t X 0.4 , 0.9 , 0.9 A , B ( t s ) V g ^ ( y ϵ ( s ) , y ϵ ( s 0.4 ) , v ) N ¯ ( d s , d v ) .

6. Conclusion

In this article, we established and proved the existence and uniqueness theorem for solutions of Caputo type fractional stochastic delay differential systems (FSDDSs) with Poisson jumps. By utilizing H o ¨ lders inequality, Jensen’s inequality, Burkholder-Davis-Gundys inequality, Doobs martingale inequality and fractional Gronwall’s inequality, we proved the averaging principle for FSDDEs in the sense of L p . Our results generalize the cases of p = 2 and enriched the field of fractional stochastic delay differential equations. Finally, we provided an example to show the usefulness of our results.

Author Contributions

Conceptualization, Z.B. and C.B.; formal analysis, Z.B.; investigation, Z.B., C.B.; and writing—review and editing, Z.B. and C.B. All authors have read and agreed to the published version of the manuscript.

Funding

This work was supported by Natural Science Foundation of China (11571136).

Data Availability Statement

Not applicable.

Conflicts of Interest

The authors declare that there are no conflicts of interest.

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