Next Article in Journal
Multi-Objective Constrained Optimization Model and Molten Iron Allocation Application Based on Hybrid Archimedes Optimization Algorithm
Next Article in Special Issue
On One Approach to Obtaining Estimates of the Rate of Convergence to the Limiting Regime of Markov Chains
Previous Article in Journal
On the Qualitative Analysis of Solutions of Two Fractional Order Fractional Differential Equations
Previous Article in Special Issue
Stochastic Growth Models for the Spreading of Fake News
 
 
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Article

The Implicit Euler Scheme for FSDEs with Stochastic Forcing: Existence and Uniqueness of the Solution

by
Kęstutis Kubilius
Faculty of Mathematics and Informatics, Vilnius University, Akademijos g. 4, LT-08412 Vilnius, Lithuania
Mathematics 2024, 12(16), 2436; https://doi.org/10.3390/math12162436
Submission received: 1 July 2024 / Revised: 1 August 2024 / Accepted: 4 August 2024 / Published: 6 August 2024

Abstract

:
In this paper, we focus on fractional stochastic differential equations (FSDEs) with a stochastic forcing term, i.e., to FSDE, we add a stochastic forcing term. Using the implicit scheme of Euler’s approximation, the conditions for the existence and uniqueness of the solution of FSDEs with a stochastic forcing term are established. Such equations can be applied to considering FSDEs with a permeable wall.

1. Introduction

We will consider stochastic differential equations of the following form:
X t = X 0 + Φ ( X t ) Φ ( X 0 ) + 0 t f ( s , X s ) d s + 0 t g ( s , X s ) d B s H , t [ 0 , T ] ,
where Φ : R R is a continuous function, f , g : [ 0 , T ] × R R are measurable functions, and B H = ( B t H ) t 0 , 1 / 2 < H < 1 , denotes a fractional Brownian motion (fBm). The stochastic integral in Equation (1) is a pathwise generalized Lebesgue–Stieltjes integral. Thus, we can use the pathwise approach to consider this FSDE. We call such an equation FSDE with a stochastic forcing term Φ .
Many authors have considered the problem of the existence and uniqueness of solutions to FSDEs without a stochastic forcing term [1,2,3,4,5,6,7,8,9,10,11,12,13,14]. The first attempt to consider the FSDE with a stochastic forcing term was made in an article by Kubilius and Medžiūnas [15]. In this article, equations with constant and strictly positive diffusion coefficients with a “soft wall” are considered. That is, the value of the function Φ ( x ) depends on the position of x to a fixed point, w, called the wall boundary. For example, we can take exponential forces with a wall (w) defined by a function
Φ ( x ) = Φ 0 exp λ ( x w )
characterized by the amplitude Φ 0 and decay constant λ . The term “soft wall” was introduced in reference [16]. It should be noted that the “soft wall” model has a permeable wall. The process may cross the wall, but it is affected by the force of the selected quantity in the opposite direction. The force acts weakly when the process is far from the wall. As it approaches or crosses the wall, the force acts stronger. An illustration of the behavior of trajectories for such a model was considered in [15,17]. There, we considered the fractional Vasicek process with the soft wall. FSDE (1) includes the “soft wall” model.
In reference [17] we consider the conditions for the existence and uniqueness of solutions to Equation (1) by using the implicit Picard iteration. In the final part of the proof, an error occurred due to an incorrect simplified notation. The theorem statement remains true, but we must use the implicit Euler approximation instead of the implicit Picard iteration. The new proof repeats the proof of Theorem 3 in [17] with estimates of other norms.
The proof of the existence and uniqueness of the solution of Equation (1) is based on estimates obtained in the article by Nualart and Rǎşcanu [10] and the conditions for the coefficients f and g are almost the same as in their article.
This paper is organized in the following way. In Section 2, we present the paper’s main results. In Section 3, we define a deterministic differential equation corresponding to FSDE (1) and consider its implicit Euler approximation properties. Moreover, it contains definitions of considered spaces of functions and a priori estimates for the Lebesgue–Stieltjes integral. In Section 4, we prove the existence and uniqueness of a solution for a deterministic differential equation. In Section 5, we consider the fractional Pearson diffusion process as an example.

2. Main Result

We will assume that the coefficients f , g satisfy the following conditions:
(A1) g ( t , x ) is differentiable in x, and there exist some constants 0 < β , δ 1 , and for every N 0 , there exists M N > 0 such that the following properties hold:
(i) Lipschitz continuity in x
| g ( t , x ) g ( t , y ) | M 0 | x y | , x , y R , t [ 0 , T ] ;
(ii) Local uniform Hölder continuity of the derivative in x
| g x ( t , x ) g x ( t , y ) | M N | x y | δ , x , y [ N , N ] , t [ 0 , T ] ;
(iii) Hölder continuity in t
| g ( s , x ) g ( t , x ) | + | g x ( s , x ) g x ( t , x ) | M 0 | t s | β , x R , t , s [ 0 , T ] ;
(A2) There exists a bounded function b 0 , and for every N 0 , there exists L N > 0 such that the following properties hold:
(i) Local uniform Lipschitz continuity in x
| f ( t , x ) f ( t , y ) | L N | x y | , x , y [ N , N ] , t [ 0 , T ] ;
(ii) The rate of growth
| f ( t , x ) | L 0 | x | + b 0 ( t ) , | b 0 ( t ) | L 0 x R , t [ 0 , T ] .
(A3) Assume the following:
(i) Function D : R R , where D ( x ) : = x Φ ( x ) = is strictly monotonic and surjective;
(ii) There is a constant d > 0 , such that we have the following:
| D ( x ) D ( y ) | d | x y | .
(A4) Assume that Φ : R R is a differentiable function, and there exist some constants 0 < c < 1 , 0 < ρ 1 , and for every N 0 , there exists K N > 0 such that we have the following:
(i) Φ ( x ) c , for all x R ,
(ii) Local uniform Hölder continuity of the derivative
| Φ x ( x ) Φ x ( y ) | K N | x y | ρ , x , y [ N , N ] .
Remark 1 
(see Remark 8 in [15]). Under assumptions ( A 4 ) , function D satisfies assumptions ( A 3 ) .
We can now formulate our main result. We set the following:
α 0 = min 1 2 , β , δ 1 + δ , α ¯ 0 = min 1 2 , β , δ 1 + δ , ρ 1 + ρ
Theorem 1. 
Suppose that the functions f ( t , x ) and g ( t , x ) satisfy the assumptions ( A 1 ) and ( A 2 ) with 1 H 1 < δ 1 , 1 H < β 1 . Let γ ( γ 0 , H ) , where γ 0 = 1 α 0 . If assumptions ( A 3 ) are satisfied, then there exists a stochastic process X C γ ( 0 , T ) satisfying FSDE (1), where C γ ( 0 , T ) is the space of γ-Hölder continuous functions. If assumptions ( A 4 ) are satisfied and γ ( γ ¯ 0 , H ) , where γ ¯ 0 = 1 α ¯ 0 , then there exists a unique stochastic process X C γ ( 0 , T ) satisfying FSDE (1).

3. Deterministic Differential Equations

3.1. Preliminaries

3.1.1. Spaces of Functions and Norms

Let us introduce some function spaces that will be used to analyze solutions of (1).
We denote by W 0 α , ( 0 , T ) , where 0 < α < 1 / 2 , the space of real-valued measurable functions f : [ 0 , T ] R such that we have the following:
f α , : = sup s [ 0 , T ] | f ( s ) | + 0 s | f ( s ) f ( u ) | ( s u ) 1 + α d u < .
The space W 0 α , ( 0 , T ) is a Banach space with respect to the norm f α , , and for λ 0 , the equivalent norm is defined by the following:
f α , λ : = sup t [ 0 , T ] e λ t | f ( t ) | + 0 t | f ( t ) f ( s ) | ( t s ) 1 + α d s .
For any μ ( 0 , 1 ] , denote by C μ ( 0 , T ) the space of μ -Hölder continuous functions f : [ 0 , T ] R equipped with a norm f μ : = | f | + | f | μ , where we have the following:
| f | μ : = sup 0 s < t T | f ( t ) f ( s ) | | s t | μ , | f | : = sup t [ 0 , T ] | f ( t ) | .
Clearly, we have C 1 α ( 0 , T ) W 0 , α ( 0 , T ) for 0 < α < 1 / 2 and
f α , λ f 1 α 1 + T 1 2 α 1 2 α .
We denote by W T 1 α , ( 0 , T ) , 0 < α < 1 / 2 , the space of measurable functions g : [ 0 , T ] R such that we have the following:
g 1 α , , T : = sup 0 s < t < T | g ( t ) g ( s ) | ( t s ) 1 α + s t | g ( y ) g ( s ) | ( y s ) 2 α d y < .
Note that W T 1 α , ( 0 , T ) C 1 α ( 0 , T ) (see [10]).
We also denote by W 0 α , 1 ( 0 , T ) , 0 < α < 1 / 2 , the space of measurable functions f on [ 0 , T ] such that we have the following:
f α , 1 : = 0 T | f ( s ) | s α d s + 0 T 0 s | f ( s ) f ( y ) | | s y | 1 + α d y d s < .
Fix p ( 0 , ) . Let ϰ = { { t 0 , , t n } : 0 = t 0 < < t n = T , n 1 } denote a set of all possible partitions of [ 0 , T ] . For any f : [ 0 , T ] R , we define the following:
v p f ; [ 0 , T ] = sup ϰ k = 1 n | f ( t k ) f ( t k 1 ) | p , V p f ; [ 0 , T ] = v p 1 / p f ; [ 0 , T ] .
Recall that v p is called the p-variation of f on [ 0 , T ] . We denote by W p ( [ a , b ] ) (resp. C W p ( [ a , b ] ) ) the class of (resp. continuous) functions on [ 0 , T ] with bounded p-variation, p ( 0 , ) .
Define V p ( f ) : = V p ( f ; [ 0 , T ] ) , which is a seminorm on W p ( [ 0 , T ] ) , and V p ( f ) is 0 if and only if f is constant. For each f, V p ( f ) is a non-increasing function of p 1 , i.e., if 1 q < p , then V p ( f ) V q ( f ) . Thus, W q ( [ 0 , T ] ) W p ( [ 0 , T ] ) if 1 q < p < . If f W p ( [ a , b ] ) , then f is bounded.
Let p 1 and V p , ( f ) : = V p , ( f ; [ 0 , T ] ) = V p ( f ) + | f | . Then V p , ( f ) is a norm, and is W p ( [ 0 , T ] ) equipped with the p-variation norm is a Banach space.

3.1.2. Riemann–Stieltjes Integral

Assume that f W 0 α , 1 ( 0 , T ) and h W T 1 α , ( 0 , T ) , where 0 < α < 1 / 2 . The generalized Lebesgue–Stieltjes integral (see [10]) 0 t f d h exists for all t [ 0 , T ] and for any 0 s < t T
s t f d h Λ α ( h ) s t | f ( r ) | ( r s ) α d r + s t s r | f ( r ) f ( y ) | | r y | α + 1 d y d r ,
where
Λ α ( h ) 1 Γ ( 1 α ) Γ ( α ) h 1 α , , T
and Γ ( · ) is a Gamma function. Furthermore, the integral 0 t f d h exists if f W 0 α , ( 0 , T ) .
If f C ν ( a , b ) and h C μ ( a , b ) with ν + μ > 1 , then the generalized Lebesgue–Stieltjes integral exists and coincides with the Riemann–Stieltjes integral (see [18]).
From Young’s Stieltjes integrability theorem [19] (see p. 264) the Riemann–Stieltjes integral 0 t f d h can be defined for functions having bounded p-variation on [ 0 , T ] (see [20]).
Let f W q ( [ a , b ] ) and h W p ( [ a , b ] ) with p > 0 , q > 0 , 1 / p + 1 / q > 1 . If f and h have no common discontinuities, then the extended Riemann–Stieltjes integral a b f d h exists, and the Love–Young inequality.
| a b f d h f ( y ) h ( b ) h ( a ) | C p , q V q f ; [ a , b ] V p h ; [ a , b ]
holds for any y [ a , b ] , where C p , q = ζ ( p 1 + q 1 ) , ζ ( s ) denotes the Riemann zeta function, i.e., ζ ( s ) = n 1 n s .

3.1.3. Estimation of the Generalized Lebesgue–Stieltjes Integrals

From now on, we fix 0 < α < 1 / 2 . For any function u W 0 α , ( 0 , T ) define
F t ( f ) ( u ) = 0 t f ( s , u s ) d s ,
where f satisfies the assumptions ( A 2 ) .
Proposition 1 
(see [10]). Assume that f satisfies the assumptions ( A 2 ) . If u W 0 α , ( 0 , T ) then F ( f ) ( u ) C 1 α ( 0 , T ) and we have the following:
( 1 ) F ( f ) ( u ) 1 α c ( 1 ) 1 + | u | , ( 2 ) F ( f ) ( u ) α , λ c ( 2 ) λ 1 2 α 1 + u α , λ
for all λ 1 , where c ( i ) , i { 1 , 2 } , are positive constants depending only on α, T, L 0 .
If u , v W 0 α , ( 0 , T ) are such that | u | N and | v | N , then we have the following:
F ( f ) ( u ) F ( f ) ( v ) α , λ c N λ 1 α u v α , λ
for all λ 1 , where c N = C α , T L N Γ ( 1 α ) depends only on α, T, and L N from ( A 2 ) .
Given two functions, h W T 1 α , ( 0 , T ) and u W 0 α , ( 0 , T ) , we denote the following:
G t ( u ) = 0 t u s d h s , G t ( g ) ( u ) = 0 t g ( s , u s ) d h s ,
where g satisfies the assumptions ( A 1 ) with constant β > α .
Proposition 2 
(see Proposition 4.1 [10]). If u W 0 α , 1 ( 0 , T ) , then we have the following:
G t ( u ) + 0 t G t ( u ) G s ( u ) ( t s ) 1 + α d s Λ α ( h ) 0 t c α ( 1 ) ( t r ) 2 α + 1 r α | u ( r ) ) | d r + 0 t 0 r u ( r ) u ( v ) ( r v ) 1 + α ( t v ) α + α d v d r ,
where c α ( 1 ) = B ( 2 α , 1 α ) , B ( · , · ) is the Beta function.
Proposition 3 
(see [10]). If u W 0 α , ( 0 , T ) then G ( g ) ( u ) C 1 α ( 0 , T ) and
( 1 ) G ( g ) ( u ) 1 α Λ α ( h ) C ( 1 ) 1 + u α , , ( 2 ) G ( g ) ( u ) α , λ Λ α ( h ) C ( 2 ) λ 1 2 α 1 + u α , λ
for all λ 1 , where the constants C ( 1 ) and C ( 2 ) are independent of λ, u, h (they depend on T and the constants | g ( 0 , 0 ) | , M 0 , α, β from ( A 1 ) ) .
If u , v W 0 α , ( 0 , T ) are such that | u | N and | v | N , then we have the following:
G ( g ) ( u ) G ( g ) ( v ) α , λ Λ α ( h ) C N ( 3 ) λ 1 2 α 1 + Δ ( u ) + Δ ( v ) u v α , λ
for all λ 1 , where
Δ ( u ) = sup r [ 0 , T ] 0 r | u r u s | δ | r s | 1 + α d s ,
and the constant C N ( 3 ) is independent of λ, u, v, h ( C N ( 3 ) depends on T and the constants from ( A 2 ) ) .
Remark 2. 
If u C 1 α ( 0 , T ) and δ 1 + δ > α then
Δ ( u ) | u | 1 α sup r [ 0 , T ] 0 r | r s | ( 1 α ) δ | r s | 1 + α d s = T δ α ( 1 + δ ) δ α ( 1 + δ ) | u | 1 α .

3.1.4. Integration with Respect to fBm

The trajectories of B H = ( B t H ) t 0 , 0 < H < 1 , are almost surely locally γ -Hölder continuous functions for all γ ( 0 , H ) . To be more precise, for all γ ( 0 , H ) and T > 0 , there exists a nonnegative random variable G γ , T such that E ( | G γ , T | p ) < for all p 1 , and
| B t H B s H | G γ , T | t s | γ a . s .
for all s , t [ 0 , T ] .
The pathwise generalized Lebesgue–Stieltjes integral for one-dimensional fBm B H can be defined as follows:
a b f ( s ) d B H ( s ) = ( 1 ) α a b ( D a + α f ) ( s ) ( D b 1 α B H ) ( s ) d s
if D a + α f L 1 ( a , b ) (see [6,21] p. 225), where D a + α f and D b 1 α B H are fractional derivatives.
For 1 / 2 < H < 1 , we can choose α such that 1 H < α < 1 / 2 . An easy computation shows that almost all trajectories of B H belong to the space W T 1 α , ( 0 , T ) . Indeed, since H > 1 α , then for any H > γ > 1 α , we have the following:
B H ( ω ) 1 α , , T sup 0 s < t < T G γ , T ( ω ) | t s | γ ( t s ) 1 α + s t G γ , T ( ω ) | u s | γ ( u s ) 2 α d u G γ , T ( ω ) ( 1 T ) 1 + 1 γ 1 + α .
Thus B H ( ω ) W T 1 α , ( 0 , T ) for almost all ω .
If u = { u ( t ) , t [ 0 , T ] } is a stochastic process whose trajectories belong to the space W T α , 1 ( 0 , T ) , then the pathwise generalized Lebesgue–Stieltjes integral a b u ( s ) d B H ( s ) exists and we can express it according to (13). Moreover, if the trajectories of the process u belong to the space W 0 α , ( 0 , T ) , then the indefinite integral 0 t u ( s ) d B H ( s ) is a Hölder continuous function of order 1 α (see [10]).

3.2. The Implicit Euler Approximation and Auxiliary Results

Let 0 < α < 1 / 2 be fixed. Let h W T 1 α , , h 0 = 0 . Consider the deterministic differential equation on R , as follows:
x t = x 0 + Φ ( x t ) Φ ( x 0 ) + 0 t f ( s , x s ) d s + 0 t g ( s , x s ) d h s , t [ 0 , T ] ,
where x 0 R , the coefficients f , g : R R satisfy assumptions ( A 1 ) and ( A 2 ) , and the function Φ : R R satisfies assumption ( A 3 ) .
Let π n = { t k n = k n T , 1 k n } be a sequence of uniform partitions of the interval [ 0 , T ] , and let Δ n = t k n t k 1 n , 1 k n , Δ n < 1 . We define the implicit Euler approximations for the Equation (14) as follows:
y n ( t k + 1 n ) Φ ( y n ( t k + 1 n ) ) = y n ( t k n ) Φ ( y n ( t k n ) ) + f ( t k n , y n ( t k n ) ) Δ n + g ( t k n , y n ( t k n ) ) h ( t k + 1 n ) h ( t k n ) , y n ( 0 ) = x 0 ,
and their continuous interpolations are as follows:
y n ( t ) Φ ( y t n ) = x 0 Φ ( x 0 ) + 0 t f ( τ s n , y n ( τ s n ) ) d s + 0 t g ( τ s n , y n ( τ s n ) ) d h s ,
where τ s n = t k 1 n and y n ( τ s n ) = y n ( t k 1 n ) if s [ t k 1 n , t k n ) , 1 k n .
We rewrite implicit Euler approximations (15) and (16) in a more compact way, as follows:
D ( y n ( t k + 1 n ) ) = D ( y n ( t k n ) ) + f ( t k n , y n ( t k n ) ) Δ n + g ( t k n , y n ( t k n ) ) h ( t k + 1 n ) h ( t k n )
with y n ( 0 ) = x 0 and
D y t n = D ( x 0 ) + F t ( f , τ n ) y n + G t ( g , τ n ) y n , y n ( 0 ) = x 0 .
where
F t ( f , τ n ) ( y n ) = 0 t f ( τ s n , y n ( τ s n ) ) d s , G t ( g , τ n ) ( y n ) = 0 t g ( τ s n , y n ( τ s n ) ) d h s .
The implicit Euler approximations scheme (17) is correctly defined. From the recursive expression (17), we calculate D ( y n ( t k + 1 n ) ) . The properties of the function D ( x ) give us a single value of y n ( t k + 1 n ) . Since D ( y t n ) is a continuous function, then y n is a continuous function. Indeed, since D 1 ( x ) and D ( y t n ) are continuous functions, then y n is a continuous function.
Now, we consider the properties of the implicit Euler approximation.
Lemma 1. 
Let Assumption ( A 3 ) be satisfied. Then y n , F ( f , τ n ) ( y n ) , G ( g , τ n ) ( y n ) C 1 α ( 0 , T ) for any fixed n 1 .
Proof. 
We first note that the functions f ( τ n , y n ( τ n ) ) and g ( τ n , y n ( τ n ) ) have bounded variations on [ 0 , T ] for a fixed n. Thus, for the fixed n, they are bounded and have p-bounded variation, where p = ( 1 α ) 1 . From now on, we assume that p = ( 1 α ) 1 .
First, observe that for s < t
F t ( f , τ n ) ( y n ) F s ( f , τ n ) ( y n ) = s t f ( τ u n , y n ( τ u n ) ) d u f ( τ n , y n ( τ n ) ) ( t s ) .
Thus, F ( f , τ n ) ( y n ) C 1 ( 0 , T ) C 1 α ( 0 , T ) for fixed n 1 .
Now consider G ( g , τ n ) ( y n ) . Since h W T 1 α , ( 0 , T ) C 1 α ( 0 , T ) then h C W p ( [ 0 , T ] ) and
V p ( h ; [ s , t ] ) | h | 1 α ( t s ) 1 α .
Assume that s [ t k n , t k + 1 n ) for some 0 k n 1 and t t k + 1 n T . Then
s t g ( τ u n , y n ( τ u n ) ) d h u = g ( τ n , y n ( τ n ) ) | h | 1 α ( t s ) 1 α .
If t > t k + 1 n , then from (20) and the Love–Young inequality, we obtain the following:
G t ( g , τ n ) ( y n ) G s ( g , τ n ) ( y n ) s t k + 1 n g ( τ u n , y n ( τ u n ) ) d h u + t k + 1 n t g ( τ u n , y n ( τ u n ) ) d h u s t k + 1 n g ( τ u n , y n ( τ u n ) ) d h u + C 1 , p V 1 , g ( τ n , y n ( τ n ) ) ; [ t k + 1 n , t ] V p h ; [ t k + 1 n , t ] 2 C 1 , p V 1 , g ( τ n , y n ( τ n ) ) ; [ 0 , T ] | h | 1 α ( t s ) 1 α .
From Assumption ( A 3 ) , we have the following:
y n ( t ) y n ( s ) d 1 D ( y n ( t ) ) D ( y n ( s ) ) d 1 F t ( f , τ n ) ( y n ) F s ( f , τ n ) ( y n ) + G t ( g , τ n ) ( y n ) G s ( g , τ n ) ( y n ) .
Since | y n | is bounded for any fixed n 1 , then y n C 1 α ( 0 , T ) for any fixed n 1 . □
The next lemma enables us to apply the estimate (6) to the integral G ( g , τ n ) ( y n ) .
Lemma 2. 
Let Assumptions ( A 1 ) and ( A 3 ) be satisfied. If y n W 0 α , 1 ( 0 , T ) for any fixed n 1 , then g ( τ n , y n ( τ n ) ) W 0 α , 1 ( 0 , T ) for any fixed n 1 and β > α .
Proof. 
From Lemma 1, it follows that y n W 0 α , 1 ( 0 , T ) for any fixed n 1 . We prove this. The following is evident:
0 t | g ( τ s n , y n ( τ s n ) ) | s α d s g ( τ n , y n ( τ n ) ) ( 1 α ) 1 t 1 α .
Now, we estimate the second term of the norm (5). From Lemma 1, it follows that there exists a constant C n , depending on n, such that we have the following:
y n ( τ s n ) y n ( τ u n ) C n ( τ s n τ u n ) 1 α .
Note that τ s n = τ u n for τ s n u < s . Therefore, we have
0 t 0 s g ( τ s n , y n ( τ s n ) ) g ( τ u n , y n ( τ u n ) ) ( s u ) 1 + α d u d s = 0 t 0 τ s n g ( τ s n , y n ( τ s n ) ) g ( τ u n , y n ( τ u n ) ) ( s u ) 1 + α d u d s M 0 0 t 0 τ s n | τ s n τ u n | β ( s u ) 1 + α d u d s + M 0 0 t 0 τ s n | y n ( τ s n ) y n ( τ u n ) | ( s u ) 1 + α d u d s M 0 0 t 0 τ s n | τ s n τ u n | β ( s u ) 1 + α d u d s + M 0 C n 0 t 0 τ s n | τ s n τ u n | 1 α ( s u ) 1 + α d u d s .
Since τ s n τ u n s u + Δ n and (see [22] p. 494)
0 t ( s τ s n ) α d s 0 T ( s τ s n ) α d s = k = 1 n 1 t k n t k + 1 n ( s τ s n ) α d s = k = 1 n 1 t k n t k + 1 n ( s t k n ) α d s n ( 1 α ) 1 Δ n 1 α = ( 1 α ) 1 T Δ n α
then
M 0 0 t 0 τ s n | τ s n τ u n | β ( s u ) 1 + α d u d s M 0 0 t 0 τ s n | s u | β + Δ n β ( s u ) 1 + α d u d s M 0 ( β α ) 1 0 t s β α d s + M 0 α 1 Δ n β 0 t ( s τ s n ) α d s M 0 ( β α ) 1 T β α + 1 + M 0 α 1 ( 1 α ) 1 T .
By a similar argument, we obtain the following:
M 0 C n 0 t 0 τ s n | τ s n τ u n | 1 α ( s u ) 1 + α d u d s M 0 C n ( 1 2 α ) 1 T 2 2 α + M 0 C n α 1 ( 1 α ) 1 T .
Consequently, g ( τ n , y n ( τ n ) ) has the claimed property. □
The following result is crucial to prove our main results.
Proposition 4. 
Let 1 H < α < α 0 and the functions f ( s , x ) and g ( s , x ) satisfy assumptions ( A 1 ) ( i ) , ( i i i ) , and ( A 2 ) ( i i ) , respectively. Moreover, let assumption ( A 3 ) hold. Then there exists a constant C such that we have the following:
sup n y n α , C .
Proof. 
Set
u , α , t : = sup s [ 0 , t ] u α , s , u α , s : = | u ( s ) | + | u | α , s , | u | α , s : = 0 s | u ( s ) u ( r ) | ( s r ) 1 + α d r , u , t : = sup s [ 0 , t ] | u ( s ) | .
It is easy to check that
y n α , t | x 0 | + d 1 F ( f , τ n ) ( y n ) α , t + G ( g , τ n ) ( y n ) α , t .
Indeed, we note that
| y t n | | x 0 | + 0 t | y t n y s n | | t s | 1 + α d s | y t n x 0 | + 0 t | y t n y s n | | t s | 1 + α d s d 1 | D ( y t n ) D ( x 0 ) | + 0 t | D ( y t n ) D ( y s n ) | | t s | 1 + α d s d 1 ( | F t ( f , τ n ) ( y n ) | + | G t ( g , τ n ) ( y n ) | + 0 t | F t ( f , τ n ) ( y n ) F s ( f , τ n ) ( y n ) | + | G t ( g , τ n ) ( y n ) G s ( g , τ n ) ( y n ) | | t s | 1 + α d s ) .
From Lemma 1, we have that for any fixed n 1 , the norms y n , α , t , F ( f , τ n ) ( y n ) , α , t , G ( g , τ n ) ( y n ) , α , t are finite.
The proof of the estimate F ( f , τ n ) ( y n ) α , t is similar to the proof of the estimate ( 4.27 ) in [10]
F ( f , τ n ) ( y n ) α , t 0 t | f ( τ s n , y n ( τ s n ) ) | d s + 0 t ( t s ) α 1 s t | f ( τ s n , y n ( τ s n ) ) | d s C α , T 0 t | f ( τ s n , y n ( τ s n ) ) | ( t s ) α d s C α , T L 0 0 t | y n ( τ s n ) | ( t s ) α d s + ( 1 α ) 1 T 1 α C α , T L 0 0 t y n , α , s ( t s ) α d s + ( 1 α ) 1 T 1 α ,
where C α , T = T α + 1 α .
Since α < α 0 , we have β > α . From Lemma 2, it follows that for the integral G ( g , τ n ) ( y n ) t , we can apply the estimate (6). Applying Proposition 2, we obtain the following:
G t ( g , τ n ) ( y n ) α , t Λ α ( h ) ( 0 t c α ( 1 ) ( t r ) 2 α + 1 r α | g ( τ r n , y n ( τ r n ) ) | d r + 0 t 0 r g ( τ r n , y n ( τ r n ) ) g ( τ v n , y n ( τ v n ) ) ( r v ) 1 + α ( t v ) α + α d v d r ) ,
where c α ( 1 ) = B ( 2 α , 1 α ) , B ( · , · ) is the Beta function.
Note that
g ( τ r n , y n ( τ r n ) ) g ( τ r n , y n ( τ r n ) ) M 0 | τ r n τ v n | β + M 0 y n ( τ r n ) y n ( τ v n ) M 0 | τ r n τ v n | β + M 0 y n ( τ r n ) y r n + | y r n y v n | + y v n y n ( τ v n ) .
Since
g ( τ r n , y n ( τ r n ) ) g ( τ r n , y n ( τ r n ) ) g ( 0 , 0 ) + | g ( 0 , 0 ) | g ( τ r n , y n ( τ r n ) ) g ( 0 , y n ( τ r n ) ) + g ( 0 , y n ( τ r n ) ) g ( 0 , 0 ) + | g ( 0 , 0 ) | M 0 ( τ r n ) β + M 0 | y n ( τ r n ) | + | g ( 0 , 0 ) | M 0 T β + M 0 | y n | , r + | g ( 0 , 0 ) | ,
it follows that
y r n y n ( τ r n ) d 1 D ( y r n ) D ( y n ( τ r n ) ) = d 1 f ( τ r n , y n ( τ r n ) ) ( r τ r n ) + g ( τ r n , y n ( τ r n ) ) ( h ( r ) h ( τ r n ) ) λ ( α ) ( 1 + | y n | , r ) ( r τ r n ) 1 α ,
where
λ ( α ) = d 1 max L 0 + ( M 0 T β + | g ( 0 , 0 ) | ) | h | 1 α , ( L 0 + M 0 | h | 1 α ) .
From (28), (29), and inequality
α + ( t v ) α T α r α + ( t v ) 2 α
we have the following:
G ( g , τ n ) ( y n ) α , t Λ α ( h ) M 0 0 t 0 τ r n | τ r n τ v n | β ( r v ) 1 + α ( t v ) α + α d v d r + Λ α ( h ) c α , T 0 t ( t r ) 2 α + r α ( | g ( τ r n , y n ( τ r n ) ) | + M 0 0 τ r n y n ( τ r n ) y r n + | y r n y v n | + y v n y n ( τ v n ) ( r v ) 1 + α d v ) d r ,
where c α , T = max { c α ( 1 ) , 1 } + T α , and
c α , T 1 α ( 1 α ) + T α .
First, observe that
0 t 0 τ r n | τ r n τ v n | β ( r v ) 1 + α ( t v ) α + α d v d r 0 t ( t r ) α + α 0 τ r n | r v | β + Δ n β ( r v ) 1 + α d v d r ( β α ) 1 0 t ( t r ) α + α r β α d r + α 1 Δ n β 0 t ( t r ) α + α ( r τ r n ) α d r ( β α ) 1 t β α + α 1 Δ n β α ( 1 2 α ) 1 + 1 ( 1 T ) c α , β , T ( 1 ) .
where
c α , β , T ( 1 ) : = ( β α ) 1 T β α + α 1 ( 1 2 α ) 1 + 1 ( 1 T ) .
Furthermore, from (30), we have the following:
0 t ( t r ) 2 α + r α | g ( τ r n , y n ( τ r n ) ) | d r ( M 0 T β + | g ( 0 , 0 ) | ) 0 t ( t r ) 2 α + r α d r + M 0 0 t ( t r ) 2 α + r α | y n | , r d r 2 1 2 α M 0 T β + | g ( 0 , 0 ) | ( t 1 ) + M 0 0 t ( t r ) 2 α + r α | y n | , r d r c α , β , T ( 2 ) 1 + 0 t ( t r ) 2 α + r α y n , r d r
and
0 t ( t r ) 2 α + r α 0 τ r n | y r n y v n | ( r v ) 1 + α d v d r 0 t ( t r ) 2 α + r α y n α , r d r ,
where
c α , β , T ( 2 ) = max 2 1 2 α M 0 T β + | g ( 0 , 0 ) | ( T 1 ) , M 0 .
Applying (31), we obtain the following:
0 t ( t r ) 2 α + r α 0 τ r n y n ( τ r n ) y n ( r ) ( r v ) 1 + α d v d r λ ( α ) 0 t ( t r ) 2 α + r α 0 τ r n ( 1 + y n , r ) ( r τ r n ) 1 α ( r v ) 1 + α d v d r λ ( α ) α 1 ( 1 α ) 1 T Δ n 1 2 α 0 t ( t r ) 2 α + r α ( 1 + y n , r ) d r λ ( α ) α 1 ( 1 α ) 1 T 2 ( T 1 ) 1 2 α + 0 t ( t r ) 2 α + r α y n , r d r c α , T ( 3 ) 1 + 0 t ( t r ) 2 α + r α y n , r d r
and
0 t ( t r ) 2 α + r α 0 τ r n y n ( v ) y n ( τ v n ) ( r v ) 1 + α d v d r λ ( α ) 0 t ( t r ) 2 α + r α 0 τ r n ( 1 + y n , v ) ( v τ v n ) 1 α ( r v ) 1 + α d v d r λ ( α ) 0 t ( t r ) 2 α + r α ( 1 + y n , r ) 0 τ r n ( v τ v n ) 1 α ( r v ) 1 + α d v d r λ ( α ) Δ n 1 α 0 t ( t r ) 2 α + r α ( 1 + y n , r ) 0 τ r n 1 ( r v ) 1 + α d v d r λ ( α ) α 1 ( 1 α ) 1 T Δ n 1 2 α 0 t ( t r ) 2 α + r α ( 1 + y n , r ) d r c α , T ( 3 ) 1 + 0 t ( t r ) 2 α + r α y n , r d r ,
where
c α , T ( 3 ) = λ ( α ) α 1 ( 1 α ) 1 T max 2 ( T 1 ) 1 2 α , 1 .
Consequently,
G ( g , τ n ) ( y n ) α , t C 1 + C 2 0 t ( t r ) 2 α + r α y n , α , r d r ,
where
C 1 = Λ α ( h ) M 0 c α , β , T ( 1 ) + c α , T c α , β , T ( 2 ) + 2 M 0 c α , T ( 3 ) , C 2 = Λ α ( h ) c α , T c α , β , T ( 2 ) + 2 M 0 c α , T ( 3 ) + 1 .
From (25), (27), and (33), we have the following:
y n , α , t | x 0 | + d 1 C α , T L 0 0 t y n , α , s ( t r ) α d r + d 1 ( C 0 + C 1 ) + d 1 C 2 0 t ( t r ) 2 α + r α y n , α , r d r ,
where
C 0 = C α , T L 0 ( 1 α ) 1 T 1 α .
Note that for r < t we have the following:
( t r ) α t 2 α ( t r ) α r 2 α ( t r ) 2 α t 3 α r 2 α ( t r ) 2 α T α t 2 α r 2 α ( t r ) 2 α , r α + ( t r ) 2 α r α t 2 α r 2 α ( t r ) 2 α + r 2 α r 2 α ( t r ) 2 α ( T α + 1 ) t 2 α r 2 α ( t r ) 2 α .
Thus,
y n , α , t | x 0 | + d 1 C α , T L 0 + C 2 ( T α + 1 ) t 2 α 0 t y n , α , r r 2 α ( t r ) 2 α d r + d 1 ( C 0 + C 1 )
and from Lemma 7.6 in [10]
y n , α , t a d α exp c α t b 1 / ( 1 2 α )
where c α and d α are positive constants depending only on α ,
a = | x 0 | + d 1 ( C 0 + C 1 ) b = d 1 ( C α , T L 0 + C 2 ) ( T α + 1 ) .
Now, we can strengthen the result of Lemma 1.
Proposition 5. 
Under the assumptions of Proposition 4, we obtain sup n y n 1 α < .
Proof. 
Recall that from Lemma 1, we have y n , F ( f , τ n ) ( y n ) , G ( g , τ n ) ( y n ) C 1 α ( 0 , T ) for any fixed n 1 . Thus, for any fixed n 1 , we have the following:
y n 1 α | x 0 | + d 1 F ( f , τ n ) y n 1 α + G ( g , τ n ) y n 1 α .
Indeed, similar to how we proved (26), we have the following:
| y t n | | x 0 | + | y t n y s n | | t s | 1 α d 1 ( | F t ( f , τ n ) ( y n ) | + | G t ( g , τ n ) ( y n ) | + | F t ( f , τ n ) ( y n ) F s ( f , τ n ) ( y n ) | + | G t ( g , τ n ) ( y n ) G s ( g , τ n ) ( y n ) | ( t s ) 1 α ) .
First, observe that for s < t
F t ( f , τ n ) ( y n ) F s ( f , τ n ) ( y n ) L 0 1 + | y n | ( t s ) .
Thus,
F ( f , τ n ) y n 1 α L 0 1 + | y n | T + L 0 1 + | y n | T α = ( T + T α ) L 0 1 + | y n |
and the boundedness of the norm F ( f , τ n ) ( y n ) 1 α follows from Proposition 4.
From (6), it follows that
G t ( g , τ n ) ( y n ) G s ( g , τ n ) ( y n ) Λ α ( h ) s t | g ( τ r n , y n ( τ r n ) ) | ( r s ) α d r + s t s τ r n g ( τ r n , y n ( τ r n ) ) g ( τ v n , y n ( τ v n ) ) ( r v ) 1 + α d v d r .
Furthermore, from (30), we obtain the following:
s t | g ( τ r n , y n ( τ r n ) ) | ( r s ) α d r M 0 ( T β + | y n | , r ) + | g ( 0 , 0 ) | ( 1 α ) 1 ( t s ) 1 α .
We obtain the proof of the estimate for the second term in (34) in the same way as presented in Lemma 2. We first compute the following integral:
s t ( r τ r n ) α d r .
Assume that t i 1 n s < t i n , τ t n = t k n , and k i . Similar to proofs (23) and (24), we have the following:
s t ( r τ r n ) α d r = t k n t ( r t k n ) α d r + j = i k 1 t j n t j + 1 n ( r t j n ) α d r + s t i n ( r t i 1 n ) α d r = ( 1 α ) 1 ( t t k n ) 1 α + j = i k 1 Δ n 1 α + [ ( t i n t i 1 n ) 1 α ( s t i 1 n ) 1 α ] ( 1 α ) 1 ( t s ) 1 α + ( t k n t i n ) Δ n α + ( t i n s ) 1 α ( 1 α ) 1 [ 2 ( t s ) 1 α + ( t s ) Δ n α ]
and
s t s τ r n | τ r n τ v n | β ( r v ) 1 + α d v d r s t s τ r n | r v | β + Δ n β ( r v ) 1 + α d v d r ( β α ) 1 Δ n β α ( t s ) + Δ n β α 1 s t ( r τ r n ) α d r ( β α ) 1 ( t s ) + Δ n β α 1 ( 1 α ) 1 [ 2 ( t s ) 1 α + ( t s ) Δ n α ] [ ( β α ) 1 + α 1 ( 1 α ) 1 ] ( t s ) + 2 α 1 ( 1 α ) 1 ( t s ) 1 α ( β α ) 1 T α + α 1 ( 1 α ) 1 ( T α + 2 ) ( t s ) 1 α .
Applying (31), we obtain the following:
s t s τ r n y n ( τ r n ) y r n ( r v ) 1 + α d v d r λ ( α ) s t s τ r n ( 1 + y n , r ) ( r τ r n ) 1 α ( r v ) 1 + α d v d r λ ( α ) α 1 Δ n 1 2 α s t ( 1 + y n , r ) d r λ ( α ) α 1 ( 1 + y n , t ) ( t s )
and
s t s τ r n y n ( v ) y n ( τ v n ) ( r v ) 1 + 2 α d v d r λ ( α ) s t s τ r n ( 1 + y n , v ) ( v τ v n ) 1 α ( r v ) 1 + α d v d r λ ( α ) Δ n 1 α ( 1 + y n , t ) s t s τ r n 1 ( r v ) 1 + α d v d r λ ( α ) Δ n 1 α ( 1 + y n , t ) α 1 ( 1 α ) 1 [ 2 ( t s ) 1 α + ( t s ) Δ n α ] λ ( α ) α 1 ( 1 α ) 1 ( 2 + T α ) ( 1 + y n , t ) ( t s ) 1 α .
Finally,
s t s τ r n y n ( r ) y n ( v ) ( r v ) 1 + α d v d r y n α , ( t s ) .
Thus the norm G ( g , τ n ) y n 1 α is bounded for all n and the proof is complete. □

4. Existence and Uniqueness of the Solution

We find conditions when the deterministic differential Equation (14) has a unique solution.
Theorem 2. 
Let 1 H < α < α 0 and the functions f ( s , x ) and g ( s , x ) satisfy assumptions ( A 1 ) and ( A 2 ) , respectively, where α 0 is defined in (3). If assumptions ( A 3 ) are satisfied, then for any α ^ , such that α < α ^ < δ 1 + δ , Equation (14) has a solution x C 1 α ^ ( 0 , T ) . If assumptions ( A 4 ) are satisfied and α < α ^ < ρ 1 + ρ , then Equation (14) has a unique solution x C 1 α ^ ( 0 , T ) .
Proof. 
Existence of the solution. From Proposition 5 and assumption α ^ > α , we have that the sequence of functions ( y n ) is relatively compact in C 1 α ^ ( 0 , T ) .
Thus, we can choose a subsequence y n k , which converges in C 1 α ^ ( 0 , T ) to a limit x C 1 α ^ ( 0 , T ) , i.e.,
y n k x 1 α ^ n k 0 .
We show that x is a solution to Equation (14). For simplicity of notation, we write n instead of n k . Recall the following:
D y t n = D ( x 0 ) + 0 t f τ s n , y n ( τ s n ) d s + 0 t g τ s n , y n ( τ s n ) d h s .
Thus,
| D ( x ) D ( x 0 ) 0 f ( s , x s ) d s 0 g ( s , x s ) d h s | | D ( x ) D y n | + | 0 f τ s n , y n ( τ s n ) f ( s , x s ) d s | + | 0 g τ s n , y n ( τ s n ) g ( s , x s ) d h s | .
Since | x y n | 0 and function D is continuous, the first term converges to zero. It remains to be proven that the second and third terms also converge to zero.
First, observe that there exists a constant, N, such that sup n y n 1 α ^ N and x 1 α ^ N . It follows from Proposition 5 and (35).
Next, we estimate the second term in (36). Since y n , x W 0 α ^ , ( 0 , T ) , then from Proposition 1, it follows that F ( f ) ( y n ) , F ( f ) ( x ) W 0 α ^ , ( 0 , T ) . Applying (4) to any λ 0 , we obtain the following:
| F ( f ) ( y n ) F ( f ) ( x ) | e λ T F ( f ) ( y n ) F ( f ) ( x ) α ^ , λ e λ T c N λ 1 α ^ 1 + T 1 2 α ^ 1 2 α ^ x y n 1 α ^ n 0 .
To estimate the third term in (36), we note that h W T 1 α ^ , ( 0 , T ) for α ^ > α and G ( g ) ( y n ) , G ( g ) ( x ) W 0 α ^ , ( 0 , T ) . Applying Proposition 3, Remark 2, and (4), we obtain the following:
| G ( g ) ( y n ) G ( g ) ( x ) | e λ T G ( g ) ( y n ) G ( g ) ( x ) α ^ , λ Λ α ^ ( h ) C N ( 3 ) e λ T λ 1 2 α ^ 1 + C N ( 4 ) x y n α ^ , λ Λ α ^ ( h ) C N ( 3 ) e λ T λ 1 2 α ^ 1 + C N ( 4 ) 1 + T 1 2 α ^ 1 2 α ^ x y n 1 α ^ n 0 ,
where
C N ( 4 ) : = T δ α ^ ( 1 + δ ) δ α ^ ( 1 + δ ) sup n y n 1 α ^ + x 1 α ^ 2 N T δ α ^ ( 1 + δ ) δ α ^ ( 1 + δ ) .
From the definition of α ^ , it follows that δ α ^ ( 1 + δ ) > 0 . The proof is completed. □
To prove the uniqueness of the solution, we need the following result:
Lemma 3 
(see Lemma 7.1 in [10]). Let Φ be a function satisfying assumptions ( A 4 ) . Then for all N > 0 and | x r | , | x v | , | x ˜ r | , | x ˜ v | N , we have the following:
Φ ( x r ) Φ ( x v ) ) ( Φ ( x ˜ r ) Φ ( x ˜ v ) ) c | ( x r x ˜ r ) ( x v x ˜ v ) | + K N | x v x ˜ v | · [ | x r x v | ρ + | x ˜ r x ˜ v | ρ ] .
Proof. 
By the mean value theorem, we can write the following:
( Φ ( x r ) Φ ( x v ) ) ( Φ ( x ˜ r ) Φ ( x ˜ v ) ) = ( x r x ˜ r ) ( x v x ˜ v ) 0 1 Φ θ x r + ( 1 θ ) x ˜ r d θ + ( x v x ˜ v ) 0 1 Φ θ x r + ( 1 θ ) x ˜ r Φ θ x v + ( 1 θ ) x ˜ v d θ .
From the conditions of the lemma, we obtain the statement of the lemma. □
Uniqueness of the solution. Let x and x ˜ be two solutions belonging to C 1 α ^ ( 0 , T ) . Then there exists N, such that x 1 α ^ N and x ˜ 1 α ^ N . Furthermore, x , x ˜ W 0 α ^ , ( 0 , T ) and F ( f ) ( x ) , F ( f ) ( x ˜ ) , G ( g ) ( x ) , G ( g ) ( x ˜ ) W 0 α ^ , ( 0 , T ) (see Propositions 1 and 3) and Φ ( x ) , Φ ( x ˜ ) W 0 α ^ , ( 0 , T ) . Thus, we have the following:
x x ˜ α ^ , λ Φ ( x ) Φ ( x ˜ ) α ^ , λ + F ( f ) ( x ) F ( f ) ( x ˜ ) α ^ , λ + G ( g ) ( x ) G ( g ) ( x ˜ ) α ^ , λ .
We will obtain estimates of the second and third terms from Propositions 1 and 3. It remains to evaluate the first term. From Lemma 3, we have the following:
e λ t Φ ( x t ) Φ ( x ˜ t ) + 0 t ( Φ ( x t ) Φ ( x ˜ t ) ) ( Φ ( x s ) Φ ( x ˜ s ) ) ( t s ) 1 + α ^ d s c e λ t | x s x ˜ s | + 0 t | ( x t x ˜ t ) ( x s x ˜ s ) | ( t s ) 1 + α ^ d s + K N e λ t 0 t | x s x ˜ s | · [ | x t x s | ρ + | x ˜ t x ˜ s | ρ ] ( t s ) 1 + α ^ d s c x x ˜ α ^ , λ + K N sup 0 t T 0 t e λ ( t s ) e λ s | x s x ˜ s | · [ | x t x s | ρ + | x ˜ t x ˜ s | ρ ] ( t s ) 1 + α ^ d s c x x ˜ α ^ , λ + K N x x ˜ α , λ | x | 1 α ^ + | x ˜ | 1 α ^ 0 t e λ ( t s ) ( t s ) 1 α ^ + ρ ( 1 α ^ ) d s c x x ˜ α ^ , λ + 2 N K N x x ˜ α ^ , λ λ α ^ ρ ( 1 α ^ ) 0 y 1 α ^ + ρ ( 1 α ^ ) e y d y c x x ˜ α ^ , λ + 2 N K N λ α ^ ρ ( 1 α ^ ) Γ ( ρ ( 1 α ^ ) α ^ ) x x ˜ α ^ , λ
for ρ > α ^ 1 α ^ . Thus,
x x ˜ α ^ , λ c x x ˜ α ^ , λ + 2 N K N λ α ^ ρ ( 1 α ^ ) Γ ( ρ ( 1 α ^ ) α ^ ) x x ˜ α ^ , λ + c N λ 1 α ^ x x ˜ α , λ + Λ α ^ ( h ) C N ( 3 ) λ 1 2 α ^ 1 + C N ( 4 ) x y n α ^ , λ .
For any ε > 0 , c + ε < 1 , we can choose a sufficiently large λ , such that we have the following:
2 K N N λ α ^ ρ ( 1 α ^ ) Γ ( δ ( 1 α ^ ) α ^ ) + c N λ 1 α ^ + Λ α ^ ( h ) C N ( 3 ) λ 1 2 α ^ 1 + C N ( 4 ) < ε .
Thus, | x x ˜ | = 0 and, consequently, x = x ˜ .
Proof of Theorem 1. 
Fix γ ( γ 0 , H ) . Let ε > 0 be such that γ + ε < H . Denote α = 1 γ ε and α ^ = 1 γ . Then 1 H < α < α ^ < α 0 = 1 γ 0 . Since
γ > γ 0 = 1 α 0 , α 0 β , and α 0 δ 1 + δ
then α 0 > 1 γ , β > 1 γ > 1 H , and δ 1 + δ > 1 γ . Note that from the inequality δ 1 + δ > 1 γ = α ^ it follows that δ > γ 1 1 > H 1 1 .
If γ ( γ ¯ 0 , H ) then α ¯ 0 ρ 1 + ρ and ρ 1 + ρ > α ^ . This completes the proof. □

5. Example of a Fractional Pearson Diffusion with a Stochastic Force

Consider the Pearson diffusion process with a stochastic force, as follows:
D ( X t ) = D ( x 0 ) + 0 t α ( X s ) d s + 0 t σ ( X s ) d B s H , t 0 ,
where
α ( x ) = b a x , σ ( x ) = σ 0 + σ 1 x + σ 2 x 2 .
Assume that the coefficients σ i , i = 0 , 1 , 2 , are such that σ 2 > 0 and σ 1 2 4 σ 2 σ 0 < 0 . Then σ ( x ) > 0 .
For the existence of a unique solution to problem (37), it is necessary to check the conditions of Theorem 1. Note the following:
| α ( x ) | | a | , σ ( x ) = σ 1 + 2 σ 2 x 2 σ ( x ) , 0 < σ ( x ) = 4 σ 2 σ 0 σ 1 2 4 σ 3 ( x ) 4 σ 2 σ 0 σ 1 2 4 σ 3 ( x 0 ) ,
where x 0 = σ 1 2 σ 2 is a critical point of the function σ ( x ) .
An easy computation shows the following:
σ 2 ( x ) σ 2 x + σ 1 2 σ 2 2 = 1 4 σ 2 2 σ 2 x + σ 1 2
and
( σ ( x ) ) 2 4 σ 2 ( σ 1 + 2 σ 2 x ) 2 4 ( 2 σ 2 x + σ 1 ) 2 = σ 2 , σ ( x ) σ 2 .
Thus, the Pearson diffusion process with a stochastic force has a unique solution under the above conditions.

6. Discussion

The mathematical literature has extensively analyzed stochastic differential equations (SDEs) driven by a fractional Brownian motion. Most of these efforts have been motivated by problems arising in the financial applications of SDEs, such as option pricing, stochastic volatility, and interest rate modeling. However, there are few results concerning SDEs with boundary conditions. Typically, SDEs involving reflection at the boundary are considered. Our focus is on introducing and solving stochastic differential equations that are subject to a force allowing a process to cross a boundary while preventing it from moving far from it. Examining such a model can be interpreted as studying the influence of the environment on the behavior of the process. These types of processes can be applied in the natural sciences. This work represents an initial attempt to consider such processes. Introducing two- or three-dimensional SDEs with such a force would be of great practical interest.

Funding

This research received no external funding.

Data Availability Statement

The original contributions presented in the study are included in the article, further inquiries can be directed to the corresponding author.

Acknowledgments

The author would like to thank Mohamed Erraoui, who brought to his attention an error in the proof of Theorem 3 in [17].

Conflicts of Interest

The author declares no conflict of interest.

References

  1. Duncan, T.; Nualart, D. Existence of strong solutions and uniqueness in law for stochastic differential equations driven by fractional Brownian motion. Stoch. Dyn. 2009, 9, 423–435. [Google Scholar] [CrossRef]
  2. Guerra, J.; Nualart, D. Stochastic differential equations driven by fractional Brownian motion and standard Brownian motion. Stoch. Anal. Appl. 2008, 26, 1053–1075. [Google Scholar] [CrossRef]
  3. Kubilius, K. The existence and uniqueness of the solution of an integral equation driven by a p-semimartingale of special type. Stoch. Process. Appl. 2002, 98, 289–315. [Google Scholar] [CrossRef]
  4. Kubilius, K. Estimation of the Hurst index of the solutions of fractional SDE with locally Lipschitz drift. Nonlinear Anal. Model. Control 2020, 25, 1059–1078. [Google Scholar] [CrossRef]
  5. Li, Z.; Zhan, W.; Xu, L. Stochastic differential equations with time-dependent coefficients driven by fractional Brownian motion. Physica A 2019, 530, 121565. [Google Scholar] [CrossRef]
  6. Mishura, Y.; Shevchenko, G. Existence and Uniqueness of the Solution of Stochastic Differential Equation Involving Wiener Process and Fractional Brownian Motion with Hurst Index H>1/2. Commun. Stat. Theory Methods 2011, 40, 3492–3508. [Google Scholar] [CrossRef]
  7. Mishura, Y.; Shevchenko, G. Mixed stochastic differential equations with long-range dependence: Existence, uniqueness and convergence of solutions. Comput. Math. Appl. 2012, 64, 3217–3227. [Google Scholar] [CrossRef]
  8. Mishura, Y.; Yurchenko-Tytarenko, A. Fractional Cox-Ingersoll-Ross process with non-zero “mean”. Mod. Stoch. Theory Appl. 2018, 5, 99–111. [Google Scholar] [CrossRef]
  9. Nualart, D.; Ouknine, Y. Regularization of differential equations by fractional noise. Stoch. Process Their Appl. 2002, 102, 103–116. [Google Scholar] [CrossRef]
  10. Nualart, D.; Rǎşcanu, A. Differential equations driven by fractional Brownian motion. Collect. Math. 2002, 53, 55–81. [Google Scholar]
  11. Pei, B.; Xu, Y. On the non-Lipschitz stochastic differential equations driven by fractional Brownian motion. Adv. Differ. Equ. 2016, 2016, 194. [Google Scholar] [CrossRef]
  12. da Silva, J.L.; Erraoui, M.; Essaky, E.H. Mixed Stochastic Differential Equations: Existence and Uniqueness Result. J. Theor. Probab. 2018, 31, 1119–1141. [Google Scholar] [CrossRef]
  13. Xu, Y.; Luo, J. Stochastic differential equations driven by fractional Brownian motion. Stat. Probab. Lett. 2018, 142, 102–108. [Google Scholar] [CrossRef]
  14. Zhang, S.Q.; Yuan, C. Stochastic differential equations driven by fractional Brownian motion with locally Lipschitz drift and their Euler approximation. Proc. R. Soc. Edinb. A 2021, 151, 1278–1304. [Google Scholar] [CrossRef]
  15. Kubilius, K.; Medžiūnas, A. A class of the fractional stochastic differential equations with a soft wall. Fractal Fract. 2023, 7, 110. [Google Scholar] [CrossRef]
  16. Vojta, T.; Halladay, S.; Skinner, S.; Janušonis, S.; Guggenberger, T.; Metzler, R. Reflected fractional Brownian motion in one and higher dimensions. Phys. Rev. E 2020, 102, 032108. [Google Scholar] [CrossRef]
  17. Kubilius, K. Fractional SDEs with stochastic forcing: Existence, uniqueness, and approximation. Nonlinear Anal. Model. Control 2023, 28, 1196–1225. [Google Scholar] [CrossRef]
  18. Zähle, M. Integration with respect to fractal functions and stochastic calculus, I. Probab. Theory Relat. Fields 1998, 111, 333–374. [Google Scholar] [CrossRef]
  19. Young, L.C. An inequality of the Hölder type, connected with Stieltjes integration. Acta Math. 1936, 67, 251–282. [Google Scholar] [CrossRef]
  20. Dudley, R.M.; Norvaiša, R. Differentiability of Six Operators on Nonsmooth Functions and p-Variation; Lecture Notes in Mathematics; Springer: New York, NY, USA, 1999; Volume 1703. [Google Scholar]
  21. Samko, S.; Kilbas, A.; Marichev, O. Fractional Integrals and Derivatives. Theory and Applications; Gordon and Breach Science Publishers: New York, NY, USA, 1993. [Google Scholar]
  22. Mishura, Y.; Shevchenko, G. The rate of convergence for Euler approximations of solutions of stochastic differential equations driven by fractional Brownian motion. Stochastics 2008, 80, 489–511. [Google Scholar] [CrossRef]
Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content.

Share and Cite

MDPI and ACS Style

Kubilius, K. The Implicit Euler Scheme for FSDEs with Stochastic Forcing: Existence and Uniqueness of the Solution. Mathematics 2024, 12, 2436. https://doi.org/10.3390/math12162436

AMA Style

Kubilius K. The Implicit Euler Scheme for FSDEs with Stochastic Forcing: Existence and Uniqueness of the Solution. Mathematics. 2024; 12(16):2436. https://doi.org/10.3390/math12162436

Chicago/Turabian Style

Kubilius, Kęstutis. 2024. "The Implicit Euler Scheme for FSDEs with Stochastic Forcing: Existence and Uniqueness of the Solution" Mathematics 12, no. 16: 2436. https://doi.org/10.3390/math12162436

Note that from the first issue of 2016, this journal uses article numbers instead of page numbers. See further details here.

Article Metrics

Back to TopTop