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Article

Dynamics of Fractional Stochastic Ginzburg–Landau Equation Driven by Nonlinear Noise

1
School of Mathematics and Statistics, Shandong University, Weihai 264209, China
2
Department of Mathematics, New Mexico Institution of Mining and Technology, Socorro, NM 87801, USA
*
Author to whom correspondence should be addressed.
Mathematics 2022, 10(23), 4485; https://doi.org/10.3390/math10234485
Submission received: 26 October 2022 / Revised: 15 November 2022 / Accepted: 23 November 2022 / Published: 28 November 2022
(This article belongs to the Section Dynamical Systems)

Abstract

:
In this work, we focus on the long-time behavior of the solutions of the stochastic fractional complex Ginzburg–Landau equation defined on R n with polynomial drift terms of arbitrary order. The well-posedness of the equation based on pathwise uniform estimates and uniform estimates on average are proved. Following this, the existence and uniqueness of weak pullback random attractors are establsihed.

1. Introduction

In this paper, we investigate the random dynamics of the stochastic fractional Ginzburg–Landau equation defined on R n with polynomial drift terms of arbitrary order. To be specific, we consider the following stochastic fractional complex Ginzburg–Landau equation on R n , for t > 0 and given α ( 0 , 1 ) ,
d u ( t ) + ( 1 + i ν ) ( Δ ) α u ( t ) d t + ( 1 + i μ ) | u ( t ) | 2 β u ( t ) d t = ρ u ( t ) d t + g ( t , x ) d t + σ ( t , ω , u ( t ) ) d W ( t ) ,
with initial condition
u ( 0 , x ) = u 0 ( x ) , x R n ,
where u ( x , t ) is a complex-valued function on R n × [ 0 , + ) . In (1), i is the imaginary unit, α , β , μ , ν and ρ are real constants with ρ > 0 and β > 0 , ( Δ ) α is fractional Laplace operator, g L l o c 2 ( R , L 2 ( R n ) ) is given, σ is a local Lipschitz nonlinear diffusion coefficient, and W is a two-sided cylindrical Wiener process in a Hilbert space defined on a complete filtered probability space ( Ω , F , { F t } t R , P ) , { F t } t R is an increasing right continuous family of sub- σ -algebras of F that contains all P-null sets. For simplicity in our discussion, we write p = 2 β + 2 and q = 2 β + 2 2 β + 1 .
The Ginzburg–Landau equation [1,2] is one of the most studied nonlinear equations in physics. It describes a vast variety of phenomena from nonlinear waves to second-order phase transitions, from superconductivity, superfluidity, and Bose–Einstein condensation to liquid crystals and strings in field theory. The Ginzburg–Landau equation with fractional derivatives [3] is used to describe processes in media with fractal dispersion or long-range interaction. In [4], the authors analyzed a one-dimensional fractional complex Ginzburg–Landau equation. In [5], the dynamics of a two-dimensional fractional complex Ginzburg–Landau equations is studied. In [6], the authors studied the dynamics of 3-D fractional complex Ginzburg–Landau equation. During the derivation of these ideal models, small perturbations (such as molecular collisions in gases and liquids and electric fluctuations in resistors) may be neglected. Therefore, one may represent the micro-effects by random perturbations in the dynamics of the macro observable through additive or multiplicative noise in the governing equation.
In the past two decades, a great deal with mathematical efforts has been devoted to the fractional Ginzburg–Landau equation which is driven by an additive noise or a linear multiplicative noise. Respectively, a fractional Ginzburg–Landau equation on the line with special nonlinearity and multiplicative noise was analyzed in [7]. A stochastic fractional complex Ginzburg–Landau equation with multiplicative noise in three spatial dimensions was studied in [8]. In [9], the author established fractional stochastic Ginzburg–Landau equation driven by colored noise with a nonlinear diffusion term to the case where α ( 1 2 , 1 ) . Time-space fractional stochastic Ginzburg–Landau equations are also studies in [10,11]. Considering the complexity of the environment, many disturbances can not be described by multiplicative noise or additive noise, and nonlinear noise can better fit the phenomenon, at this point it is very necessary to study nonlinear noise. However, in spite of quite contributions about these literature, there are no result taking into account of the existence of pathwise pullback random attractors for the stochastic equation (1) with a nonlinear diffusion term σ .
The purpose of this paper is to establish the well-posedness of (1) and (2) in L l o c 2 ( R ; L 2 ( R n ) ) and study the mean random dynamical system generated by the solution operators. The counterpart of the concept of mean random dynamical system is the pathwise random dynamical system. The global attractors for pathwise random dynamical system have been extensively studied, see, e.g., [12,13,14,15,16,17,18,19,20,21,22,23] and [24,25,26,27,28,29,30,31,32,33,34,35] for autonomous and non-autonomous stochastic equations, respectively. There are few results about mean random dynamical system ([36,37]), but these results are about real-valued functions. This paper is about complex-valued function.
In Equation (1), we assume that the diffusion coefficient σ ( t , ω , u ( t ) ) : R × Ω × H L 2 ( U , H ) is locally Lipschitz continuous in its third argument uniformly for ( t , ω ) R × Ω ; namely, for every r > 0 , there exists a positive number M r depending on r such that for all t R , ω Ω and u 1 , u 2 H with u 1 r and u 2 r ,
σ ( t , ω , u 1 ) σ ( t , ω , u 2 ) L 2 ( U , H ) M r u 1 u 2 .
In addition, σ ( t , ω , u ) grows linearly in u H uniformly for ( t , ω ) R × Ω ; that is, there exists a positive number L such that for all t , ω , u R × Ω × H ,
σ ( t , ω , u ) L 2 ( U , H ) L ( 1 + u ) .
We further assume that σ ( t , ω , u ) : R × Ω L 2 ( U , H ) is progressively measurable for every fixed u H .
The arrangement of the article is as follows. In Section 2, we introduce some related concepts and preliminaries. In Section 3, we prove the well-posedness of (1) and (2) driven by regular additive noise. In Section 4, we study the existence and uniqueness of solutions with general additive noise. In Section 5 and Section 6, we respectively investage the well-posedness of (1) and (2) with globally and locally Lipschitz continuous diffusion coefficients. In the last Section, we focus on the existence and uniqueness of weak pullback random attractor for (1) and (2).

2. Preliminaries and Notations

In this section, we first recall the concept of the fractional Laplace operator on R n as well as the definition of some spaces, norm and inner product. Then, we introduce the concept of weak pullback mean random attractors for mean random dynamical systems Φ over filtered probability spaces and the definition of solutions for the stochastic equations under investigation. At the last of this section, we list some inequalities and theorems which will be used in this paper.
Let S be the Schwartz space of rapidly decaying C functions on R n . Then by [38], we have for 0 < α < 1 the fractional Laplace operator ( Δ ) α is defined by
( Δ ) α u ( x ) = 1 2 C ( n , α ) R n u ( x + y ) + u ( x y ) 2 u ( x ) y n + 2 α d y , x R n , f o r u S ,
where C ( n , α ) is a positive constant given by
C ( n , α ) = α 4 α Γ ( n + 2 α 2 ) π n 2 Γ ( 1 α ) .
For 0 < α < 1 , the fractional Sobolev space H α ( R n ) is defined by
H α ( R n ) = { u L 2 ( R n ) : R n R n u ( x ) u ( y ) 2 x y n + 2 α d x d y < } ,
endowed with the norm
u H α ( R n ) = R n u ( x ) 2 d x + R n R n u ( x ) u ( y ) 2 x y n + 2 α d x d y 1 2 .
By [39], The norm u H α ( R n ) is equivalent to the norm ( u L 2 ( R n ) 2 + ( Δ ) α 2 u L 2 ( R n ) 2 ) 1 2 for u H α ( R n ) ; more precisely, we have
u H α ( R n ) 2 = u L 2 ( R n ) 2 + 2 C ( n , α ) ( Δ ) α 2 u L 2 ( R n ) 2 , f o r a l l u H α ( R n ) .
The inner product of H α ( R n ) in complex field is defined by
( u , v ) H α ( R n ) = R n u ( x ) v ¯ ( x ) d x + R n R n ( u ( x ) u ( y ) ) ( v ¯ ( x ) v ¯ ( y ) ) x y n + 2 α d x d y , u , v H α ( R n ) .
For convenience, we write H = L 2 ( R n ) and V = H α ( R n ) . Then, we have V H = H * V * , where H * and V * are the dual spaces of H and V, respectively, H * is identified with H by Riesz’s representation theorem. We respectively denote the norm and the inner product of L 2 ( R n ) by · and ( · , · ) . L 2 ( U , H ) is used for the space of Hilbert-Schmidt operators from a separable Hilbert space U to H with norm · L 2 ( U , H ) .
Let D be a collection of some families of nonempty bounded subsets of L 2 ( Ω , F τ ; H ) parametrized by τ R , that is
D = { D = { D ( τ ) L 2 ( Ω , F τ ; H ) : D ( τ ) b o u n d e d , τ R }
: D s a t i s f i e s lim τ e ρ τ D ( τ ) L 2 ( Ω , F τ ; H ) = 0 2 } ,
where D L 2 ( Ω , F τ ; H ) = sup u D u L 2 ( Ω , F τ ; H ) for a subset D in L 2 ( Ω , F τ ; H ) .
Definition 1
([40]). D is called inclusion-closed if D D and if D ˜ = { D ˜ ( τ ) } τ R is a random subset of H with D ˜ ( τ ) D ( τ ) for all τ R then D ˜ D .
Definition 2
([36]). A family Φ = { Φ ( t , τ ) : t R + , τ R } of mapping is called a mean random dynamical system on L 2 ( Ω , F ; H ) over L 2 ( Ω , F , { F t } t R , P ) if for all τ R and t , s R + ,
(i) 
Φ ( t , τ ) maps L 2 ( Ω , F τ , H ) to L 2 ( Ω , F t + τ , H ) ,
(ii) 
Φ ( 0 , τ ) is the identity operator on L 2 ( Ω , F τ , H ) ,
(iii) 
Φ ( t + s , τ ) = Φ ( t , τ + s ) Φ ( s , τ ) .
Definition 3
([36]). A family K = { K ( τ ) : τ R } D is called a D -pullback weakly attracting set of mean random dynamical system Φ on L 2 ( Ω , F ; H ) over L 2 ( Ω , F , { F t } t R , P ) , if for every τ R , D D and every weak neighborhood N ω ( K ( τ ) ) of K ( τ ) in L 2 ( Ω , F ; H ) , there exists T = T ( τ , D , N ω ( K ( τ ) ) ) > 0 such that for all t T ,
Φ ( t , τ t ) ( D ( τ t ) ) N ω ( K ( τ ) ) ,
where N ω ( K ( τ ) ) is the weak neighborhood of K ( τ ) . For a subset K ( τ ) L 2 ( Ω , F , H ) , every weakly open set containing K ( τ ) is called a weak neighborhood of K ( τ ) in L 2 ( Ω , F , H ) . In addition, if K ( τ ) is a weakly compact subset of L 2 ( Ω , F ; H ) for every τ R , then K = { K ( τ ) : τ R } is called a D -pullback weakly compact weakly attracting set for Φ.
Definition 4
([36]). A family A = { A ( τ ) : τ R } D is called a weak D -pullback mean random attractor for Φ on L 2 ( Ω , F ; H ) over L 2 ( Ω , F , { F t } t R , P ) if the following conditions are fulfilled,
(i) 
A ( τ ) is a weakly compact subset of L 2 ( Ω , F τ ; H ) for every τ R ,
(ii) 
A is a D -pullback weakly attracting set of Φ,
(iii) 
A is the minimal element of D with properties (i) and (ii), that is, if D = { D ( τ ) : τ R } D is a D -pullback weakly compact weakly attracting set of Φ, then A ( τ ) D ( τ ) for all τ R .
Theorem 1
([36]). Let D be an inclusion-closed collection of some families of nonempty bounded subsets of L p ( Ω , F ; H ) as given by (8). If Φ has a weakly compact D -pullback absorbing set B D on L 2 ( Ω , F ; H ) over L 2 ( Ω , F , { F t } t R , P ) , then Φ has a unique weak D -pullback mean attractor A D on L 2 ( Ω , F ; H ) over L 2 ( Ω , F , { F t } t R , P ) , which is given by, for each τ R ,
A ( τ ) = Ω ω ( B , τ ) = r 0 t r Φ ( t , τ t ) ( B ( τ t ) ) ¯ ω ,
where the closure is taken with respect to the weak topology of L 2 ( Ω , F ; H ) .
Definition 5.
Let u 0 L 2 ( Ω , H ) be F 0 -measurable. Then, a continuous H-valued F t -adapted stochastic process u is called a solution of (1) and (2) if
u L 2 ( Ω , C ( [ 0 , T ] , H ) ) L 2 ( Ω , L 2 ( 0 , T ; V ) ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) , T > 0 ,
such that for all t > 0 and ξ V L p ( R n ) ,
( u ( t ) , ξ ) + ( 1 + i ν ) 0 t ( ( Δ ) α 2 u ( s ) , ( Δ ) α 2 ξ ) d s + 0 t R n ( 1 + i μ ) | u ( s ) | 2 β u ( s ) ξ ( x ) d x d s
= ( u 0 , ξ ) + ρ 0 t ( u ( s ) , ξ ) d s + 0 t ( g ( s ) , ξ ) d s + 0 t ξ σ ( s , u ( s ) ) d W ,
P—almost surely, where ξ in the stochastic term is identified with the element in H * = H by Riesz’s representation theorem.
Note that if u is a solution of (1) and (2) in the sense of Definition 5, then by (9) we have
( Δ ) α u L 2 ( Ω , L 2 ( 0 , T ; V * ) ) .
Consequently, a continuous H-valued F t -adapted stochastic process u is a solution of (1) and (2) in the sense of Definition 5 if and only if u satisfies (9), and for all t 0 ,
u ( t ) + ( 1 + i ν ) 0 t ( Δ ) α u ( s ) d s + 0 t ( 1 + i μ ) | u ( s ) | 2 β u ( s ) d s = u 0
+ ρ 0 t u ( s ) d s + 0 t g ( s ) d s + 0 t σ ( s , u ( s ) ) d W i n ( V L p ( R n ) ) * ,
P–almost surely. In other words, (10) and (11) are equivalent.

3. Existence of Solutions: Regular and Additive Noise

In this section, we study the well-posedness of solution to problem (1) and (2) with a diffusion term σ taking values in a regular space. Let V 0 be a separable Hilbert space satisfies V 0 V and V 0 L p ( R n ) . In this section, we assume that σ : R × Ω L 2 ( U , V 0 ) is a progressively measurable process such that
σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , V 0 ) ) ) f o r e v e r y T > 0 .
Considering the following stochastic equation with additive noise:
d u ( t ) + ( 1 + i ν ) ( Δ ) α u ( t ) + ( 1 + i μ ) | u ( t , x ) | 2 β u ( t , x ) d t = ρ u ( t ) d t + g ( t , x ) d t + σ ( t , ω ) d W , x R n , t > 0 ,
with the initial condition
u ( 0 , x ) = u 0 ( x ) , x R n .
We need to approximate the locally Lipschitz nonlinearity ( 1 + i μ ) | u | 2 β u by a globally Lipschitz function to prove the existence and uniqueness of solutions to (13) and (14). Therefore, for every n N , we define a function ξ n : C C by
ξ n ( s ) = s i f s n , n s s i f s > n .
Then, ξ n : C C is globally Lipschitz continuous. In fact, we have ξ n ( 0 ) = 0 ,
ξ n ( s 1 ) ξ n ( s 2 ) s 1 s 2 , f o r a l l s 1 , s 2 C ,
and
ξ n ( s ) n , ξ n ( s ) s f o r a l l s C .
Given n N , for almost all ( t , x ) [ 0 , T ] × R n , we choose a globally Lipschitz continuous function ( 1 + i μ ) | ξ n ( u ) | 2 β ξ n ( u ) ; exactly, for every n N , there exists c n > 0 such that
( 1 + i μ ) | ξ n ( u 1 ) | 2 β ξ n ( u 1 ) ( 1 + i μ ) | ξ n ( u 2 ) | 2 β ξ n ( u 2 ) c n u 1 u 2 ,
for all u 1 , u 2 C and for almost all ( t , x ) [ 0 , T ] × R n . By (17) we obtain, for almost all t [ 0 , T ] ,
( 1 + i μ ) | ξ n ( u ) | 2 β ξ n ( u ) ( 1 + i μ ) | ξ n ( v ) | 2 β ξ n ( v ) c n u v , f o r a l l u , v H .
Since ( 1 + i μ ) | ξ n ( 0 ) | 2 β ξ n ( 0 ) = 0 , by (18) we obtain, for almost all t [ 0 , T ] ,
( 1 + i μ ) | ξ n ( u ) | 2 β ξ n ( u ) c n u , f o r a l l u H .
In addition, for all t R , we infer that
Re ( 1 + i μ ) | ξ n ( u ) | 2 β ξ n ( u ) ( 1 + i μ ) | ξ n ( v ) | 2 β ξ n ( v ) , u v 0 , f o r a l l u , v H
and by the definition of ξ n , we deduce
ξ ¯ n ( u n ) u n | ξ n ( u n ) | 2 .
Given n N , consider the following approximate stochastic equation for (13) and (14) in V * for t > 0 :
d u n ( t ) + ( 1 + i ν ) ( Δ ) α u n ( t ) d t + ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) d t = ρ u n ( t ) d t + g ( t ) d t + σ ( t , ω ) d W ,
with initial condition
u n ( 0 ) = u 0 .
By (18)–(20), it follows from [41] that for every F 0 -measurable u 0 L 2 ( Ω , H ) , problem (22) and (23) has a unique solution u n in the sense that u n is an H-valued F t -adapted continuous process such that
u n L 2 ( Ω , C ( [ 0 , T ] , H ) ) L 2 ( Ω , L 2 ( 0 , T ; V ) ) , T > 0 ,
and for all t 0 ,
u n ( t ) + ( 1 + i ν ) 0 t ( Δ ) α u n ( s ) d s + 0 t ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) d s = u 0 + ρ 0 t u n ( s ) d s
+ 0 t g ( s ) d s + 0 t σ ( s ) d W ( s ) i n V * ,
P–almost surely.
Next, we will derive uniform estimates of the approximate solution u n and prove the limit of this sequence is a solution of problem (13) and (14). The first uniform estimate of u n is given below.
Lemma 1.
Suppose (12) holds, then there exists a subset Ω 0 of Ω with P ( Ω 0 ) = 1 such that for all ω Ω 0 , the solution u n of (22) and (23) satisfies
u n ( ω ) C ( [ 0 , T ] , H ) 2 + u n ( ω ) L 2 ( 0 , T ; V ) 2 + ξ n ( u n ( ω ) L p ( 0 , T ; L p ( R n ) ) p
+ ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) L q ( 0 , T ; L q ( R n ) ) q L ( T , ω ) ,
where L ( T , ω ) is a positive number depending only on T and ω, but independent of n N .
Proof. 
Let v n ( t ) = u n ( t ) 0 t σ ( s ) d W ( s ) , then we have v n ( t ) L 2 ( Ω , L 2 ( 0 , T ; V ) ) , which implies that there exists a subset Ω 1 of Ω with P ( Ω 1 ) = 1 such that for all ω Ω 1 ,
v n L 2 ( 0 , T ; V ) .
On the other hand, by (24) we find that there exists a subset Ω 2 of Ω with P ( Ω 2 ) = 1 such that for all ω Ω 2 and t 0 ,
v n ( t ) = u 0 ( 1 + i ν ) 0 t ( ( Δ ) α u n ( s ) d s 0 t ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) ) d s + ρ 0 t u n ( s ) d s + 0 t g ( s ) d s i n V * .
By (26) we obtain that for all ω Ω 2 ,
d v n d t = ( 1 + i ν ) ( Δ ) α u n ( t ) ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) + ρ u n ( t ) + g ( t ) i n L 2 ( 0 , T ; V * ) .
Let Ω 3 = Ω 1 Ω 2 . Then, we have P ( Ω 3 ) = 1 . Moreover, by (25) and (27) we obtain from [42] that, for all ω Ω 3 ,
d v n ( t ) 2 d t = 2 Re d v n d t , v n ( t ) ( V * , V )
on ( 0 , T ) in the sense of scalar distribution. It follows from (27) and (28) that for all ω Ω 3 ,
d v n ( t ) 2 d t = 2 Re ( 1 + i ν ) ( Δ ) α u n ( t ) , v n ( t )
2 Re ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) , v n ( t ) + 2 Re ρ u n ( t ) , v n ( t ) + 2 Re g ( t ) , v n ( t ) ,
for almost all t [ 0 , T ] .
We now deal with each term on the right-hand side of (29). For the first term on the right-hand side of (29), by Young’s inequality, we have
2 Re ( 1 + i ν ) ( Δ ) α u n ( t ) , v n ( t ) = 2 Re ( 1 + i ν ) ( Δ ) α u n ( t ) , u n ( t ) 0 t σ ( s ) d W ( s )
2 ( Δ ) α 2 u n ( t ) 2 + 1 2 ( Δ ) α 2 u n ( t ) 2 + 2 ( Δ ) α 2 0 t σ ( s ) d W ( s ) 2
+ 1 2 ( Δ ) α 2 u n ( t ) 2 + 2 ν 2 ( Δ ) α 2 0 t σ ( s ) d W ( s ) 2
( Δ ) α 2 u n ( t ) 2 + 2 ( 1 + ν 2 ) 0 t σ ( s ) d W ( s ) H α 2 .
For the second term on the right-hand side of (29), By (21), we have
2 Re ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) , v n ( t ) = 2 Re ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) , u n ( t ) 0 t σ ( s ) d W ( s ) = 2 R | ξ n ( u n ) | 2 β ξ n ( u n ) u ¯ n d x + 2 Re ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) , 0 t σ ( s ) d W ( s ) 2 R n | ξ n ( u n ) | 2 β + 2 d x + 2 ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) , 0 t σ ( s ) d W ( s ) .
Then, we estimate the last term on the right-hand side of above inequality. By Young’s inequality, we have
2 ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) , 0 t σ ( s ) d W ( s ) R n 2 1 + μ 2 | ξ n ( u n ) | 2 β + 1 · 0 t σ ( s ) d W ( s ) d x R n | ξ n ( u n ) | 2 β + 2 d x + c 1 R n 0 t σ ( s ) d W ( s ) 2 β + 2 d x ,
where c 1 = ( 2 1 + μ 2 ) 2 β + 2 ( 2 β + 1 ) 2 β + 1 ( 2 β + 2 ) 2 β + 2 , p = 2 β + 2 in (31). Then, we have,
2 Re ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) , v n ( t ) c 1 0 t σ ( s ) d W ( s ) V 0 p R n | ξ n ( u n ) | p d x ,
where p = 2 β + 2 in (32). For the third term on the right-hand side of (29), we have
2 ρ Re v n ( t ) + 0 t σ ( s ) d W ( s ) , v n ( t ) 2 ρ v n ( t ) 2 + 2 ρ 0 t σ ( s ) d W ( s ) · v n ( t )
( 2 ρ + ρ 2 ) v n ( t ) 2 + 0 t σ ( s ) d W ( s ) V 0 2 .
For the last term on the right-hand side of (29), we have
2 Re ( g ( t ) , v n ( t ) ) v n ( t ) 2 + g ( t ) 2 ,
for almost all t [ 0 , T ] , It follows from (29)–(34) that for all ω Ω 3 ,
d v n ( t ) 2 d t + ( Δ ) α 2 u n ( t ) 2 + R n | ξ n ( u n ( t ) ) | p d x c 2 v n ( t ) 2 + c 3 0 t σ ( s ) d W ( s ) V 0 p + g ( t ) 2 ,
for almost all t [ 0 , T ] , where c 2 = ( ρ + 1 ) 2 , c 3 = ( c 1 + 2 ν 2 + 3 ) . By (12) and Burkholder–Davis–Gundy Inequality, we obtain
E ( sup 0 t T 0 t σ ( s ) d W ( s ) V 0 2 ) c 4 E ( 0 T σ ( s ) L 2 ( U , V 0 ) 2 d s ) < ,
which implies that there exists a subset Ω 4 of Ω with P ( Ω 4 ) = 1 such that for all ω Ω 4 ,
c 5 ( T , ω ) = sup 0 t T 0 t σ ( s ) d W ( s ) V 0 < .
Let Ω 5 = Ω 3 Ω 4 . Then, P ( Ω 5 ) = 1 and for all ω Ω 5 , by (35) and (36) we obtain,
d v n ( t ) 2 d t + ( Δ ) α 2 u n ( t ) 2 + R n ξ n ( u n ( t ) ) p d x c 2 v n ( t ) 2 + g ( t ) 2 + c 3 c 5 ,
for almost all t [ 0 , T ] . Multiplying (37) by e c 2 t and then integrating on ( 0 , t ) , we obtain, for all ω Ω 5 and 0 t T ,
e c 2 t v n ( t ) 2 + 0 t e c 2 s ( Δ ) α 2 u n ( s ) 2 + R n ξ n ( u n ( s ) ) p d x d s v n ( 0 ) 2
+ 0 t e c 2 s ( g ( s ) 2 + c 3 c 5 ) d s .
Therefore,
v n ( t ) 2 ( u 0 2 + c 6 ) e c 2 t .
By (38) and (36), we have that for all ω Ω 5 ,
u n ( t ) C ( 0 , T , H ) = max 0 t T u n ( t ) H c 7 ,
where c 7 is a positive number only depending on T and ω . Integrating (37) on [ 0 , T ] , by (38) we obtain, for all ω Ω 5 ,
0 T ( Δ ) α 2 u n ( t ) 2 d t + 0 T R n ξ n ( u n ( t ) ) p d x d t c 8 ,
where c 8 is a positive number depending only T and ω . By (39) and (40) we obtain, for all ω Ω 5 ,
0 T R n ( 1 + i μ | ξ n ( u n ) | 2 β ξ n ( u n ) ) q d x d t = c 9 0 T R n ξ n ( u n ( t ) ) p d x d t ,
which together with (39)–(41) completes the proof. □
Next, we establish uniform estimates on the expectation of the solution.
Lemma 2.
Suppose (12) holds, then the solution u n ( t ) of (22) and (23) satisfies
u n ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u n ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + ξ n ( u n ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p
L 1 ( T ) ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 + σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) 2 ) ,
where L 1 ( T ) is a positive number only depending on T.
Proof. 
By (24) and integration by parts of Ito’s formula, for all 0 t T , we obtain
u n ( t ) 2 + 2 0 t ( Δ ) α 2 u n ( s ) 2 d s + 2 Re 0 t R n ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) u ¯ n d x d s = u 0 2 + 2 ρ 0 t u n ( s ) 2 d s + 2 Re 0 t R n g ( s ) u n ( s ) d x d s + 2 Re 0 t σ ( s ) u n ( s ) d W ( s ) + 0 t σ ( s ) L 2 ( U , H ) 2 d s
P–almost surely, by Riesz’s representation theorem, u n in the stochastic term is identified with the element in H * = H . For the third term on the left-hand side of (42), by (21) we have, for 0 t T ,
Re 0 t R n ( 1 + i μ ) | ξ n ( u n ) | 2 β ξ n ( u n ) u ¯ n ( s ) d x d s = 0 t R n | ξ n ( u n ) | 2 β ξ n ( u n ) u ¯ n ( s ) d x d s
0 t R n | ξ n ( u n ) | 2 β + 2 d x d s .
By Young’s inequality, we have
2 Re 0 t ( g ( s ) , u n ( s ) ) d s 2 0 t ( g ( s ) , u n ( s ) ) d s 0 t u n ( s ) 2 d s + 0 t g ( s ) 2 d s .
It follows from (42)–(44) that, for all 0 t T ,
u n ( t ) 2 + 2 0 t ( Δ ) α 2 u n ( s ) 2 d s + 0 t R n ξ n ( u n ( s ) ) p d x d s u 0 2 + ( 2 ρ + 1 ) 0 t u n ( s ) 2 d s + 0 t g ( s ) 2 d s + 0 t σ ( s ) L 2 ( U , H ) 2 d s + 2 Re 0 t u n ( s ) σ ( s ) d W ( s ) .
By (45), we imply that for all 0 t T ,
E ( sup 0 r t ( u n ( r ) 2 ) ) E ( u 0 2 ) + ( 2 ρ + 1 ) 0 t E ( sup 0 r s ( u n ( r ) 2 ) d s + 0 T g ( s ) 2 d s
+ E 0 T σ ( s ) L 2 ( U , H ) 2 d s + 2 E sup 0 r t 0 r u n ( s ) σ ( s ) d W ( s ) .
By the Burkholder–Davis–Gundy inequality, we have for all 0 t T ,
2 E sup 0 r t 0 r u n ( s ) σ ( s ) d W ( s ) c 10 E 0 t u n ( s ) 2 σ ( s ) L 2 ( U , H ) 2 d s 1 2 c 10 E sup 0 s t u n ( s ) 0 t σ ( s ) L 2 ( U , H ) 2 d s 1 2 1 2 E sup 0 r t u n ( r ) 2 + 1 2 c 10 2 E 0 t σ ( s ) L 2 ( U , H ) 2 d s .
By (46) and (47) we obtain, for all 0 t T ,
E sup 0 r t u n ( r ) 2 2 E ( u 0 2 ) + ( 4 ρ + 2 ) 0 t E ( sup 0 r s ( u n ( r ) 2 ) d s + 2 0 T g ( s ) 2 d s
+ ( c 10 2 + 2 ) E 0 T σ ( s ) L 2 ( U , H ) 2 d s .
By (48) and the Gronwall inequality, we find that for all 0 t T ,
E ( sup 0 r t u n ( r ) 2 ) c 11 e ( 4 ρ + 2 ) t ,
where c 11 = 2 E ( u 0 2 ) + 2 0 T g ( s ) 2 d s + ( c 10 2 + 2 ) 0 T E σ ( s ) L 2 ( U , H ) 2 d s .
On the other hand, by (45) with t = T , we obtain
2 E 0 T ( Δ ) α 2 u n ( s ) 2 d s + E 0 T R n ξ n ( u n ( s ) ) p d x d s
E ( u 0 2 ) + ( 2 ρ + 1 ) E 0 T u n ( s ) 2 d s + 0 T g ( s ) 2 d s
+ ( 1 + 1 2 c 10 2 ) 0 T E ( σ ( s ) L 2 ( U , H ) 2 ) d s ,
which together with (49) implies that
E 0 T ( Δ ) α 2 u n ( s ) 2 d s + E 0 T R n ξ n ( u n ( s ) ) p d x d s c 11 E ( u 0 2 ) + 0 T g ( s ) 2 d s + 0 T E ( σ ( s ) L 2 ( U , H ) 2 ) d s ,
which together with (49) and (50) completes the proof. □
We will prove the existence and uniqueness of solutions to problem (13) and (14).
Lemma 3.
Suppose (12) holds and u 0 L 2 ( Ω , H ) is F 0 -measurable, then problem (13) and (14) has a unique solution u in the sense of Definition 5. Moreover, u satisfies,
u ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + u ( t ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p L 2 ( T ) ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 + σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) 2 ) ,
where L 2 ( T ) is a positive number only depending on T.
Proof. 
We first prove the existence, then the uniqueness, and finally the measurability of the solutions.
Step 1. Existence of solutions for almost every fixed ω Ω . Let Ω 0 be the subset of Ω in Lemma 12 with P ( Ω 0 ) = 1 . Then, for every fixed ω Ω 0 , there exist u ˜ ( ω ) H and u ( ω ) L ( 0 , T ; H ) ) L 2 ( 0 , T ; V ) , χ 1 ( ω ) L p ( 0 , T ; L p ( R n ) ) , χ 2 ( ω ) L q ( 0 , T ; L q ( R n ) ) and a subsequence { n m } m = 1 of { n } n = 1 such that
u n m ( ω , T ) u ˜ ( ω ) w e a k l y i n H ,
u n m ( ω ) u ( ω ) w e a k s t a r i n L ( 0 , T ; H ) ,
u n m ( ω ) u ( ω ) w e a k l y i n L 2 ( 0 , T ; V ) ,
ξ n m ( u n m ( ω ) ) χ 1 ( ω ) w e a k l y i n L p ( 0 , T ; L p ( R n ) ) ,
and
( 1 + i μ ) | ξ n m ( u n m ( ω ) ) | 2 β ξ n m ( u n m ( ω ) ) χ 2 ( ω ) w e a k l y i n L q ( 0 , T ; L q ( R n ) ) .
Let v n m ( ω , t ) = u n m ( ω , t ) 0 t σ ( s ) d W and v ( ω , t ) = u ( ω , t ) 0 t σ ( s ) d W . Then, by (53) we have
v n m ( ω ) v ( ω ) w e a k s t a r i n L ( 0 , T ; H ) .
By (54) we obtain
{ v n m ( ω ) } m = 1 i s b o u n d e d i n L 2 ( 0 , T ; V ) .
On the other hand, by (24), we see that there exists a subset Ω 1 of Ω with P ( Ω 1 ) = 1 such that for every ω Ω 1 ,
v n m ( ω , t ) = 0 t ( 1 + i ν ) ( Δ ) α u n m ( ω , s ) d s + ρ 0 t u n m ( ω , s ) d s 0 t ( 1 + i μ ) | ξ n m ( u n m ( ω ) ) | 2 β ξ n m ( u n m ( ω , s ) ) d s + u 0 + 0 t g ( s ) d s i n V * .
Note that (59) is a deterministic equation parametrized by ω Ω 1 , which implies that for every ω Ω 1 ,
d v n m ( ω , t ) d t = ( 1 + i ν ) ( Δ ) α u n m ( ω , t ) + ρ u n m ( ω , t ) ( 1 + i μ ) | ξ n m ( u n m ( ω ) ) | 2 β ξ n m ( u n m ( ω , t ) ) + g ( t ) i n V * ,
for almost all t [ 0 , T ] . By (54), (56) and (60) we infer that
d v n m ( ω ) d t i s b o u n d e d i n L q ( 0 , T ; ( V L p ( R n ) ) * ) .
Let ρ ^ : R n [ 0 , 1 ] be a smooth function satisfies ρ ^ ( x ) = 1 if x 1 ; and ρ ^ ( x ) = 0 if x 2 . Given k N , denote by V k = { u V : u = 0 f o r a l m o s t a l l x 2 k } , H k = { u H : u = 0 f o r a l m o s t a l l x 2 k } and L k p = { u L p ( R n ) : u = 0 f o r a l m o s t a l l x 2 k } . For brevity, we also write O k = { x R n : x < k } and v ˜ n m ( ω , t , x ) = ρ ^ ( x k ) v n m ( ω , t , x ) for ω Ω , t [ 0 , T ] and x R n . Then, by (58) we have
{ v ˜ n m ( ω ) } m = 1 i s b o u n d e d i n L 2 ( 0 , T ; V k ) .
Similar to (61), by (60), we can verify that
d v ˜ n m ( ω ) d t i s b o u n d e d i n L q ( 0 , T ; ( V k L k p ) * ) .
Since the embedding V k H k is compact and H k = ( H k ) * ( V k L k p ) * is continuous, by (62) and (63) and the compactness theorem in [42] we infer from (57) that for every ω Ω 2 = Ω 0 Ω 1 and k N , there exists a further subsequence (not relabeled) such that
{ v ˜ n m ( ω ) } ρ ^ ( x k ) v ( ω ) s t r o n g l y i n L 2 ( 0 , T ; H k ) .
By (64), we have, up to a further subsequence,
v ˜ n m ( ω , t , x ) ρ ^ ( x k ) v ( ω , t , x ) f o r a l m o s t a l l ( t , x ) ( 0 , T ) × O 2 k ,
and hence
v n m ( ω , t , x ) v ( ω , t , x ) f o r a l m o s t a l l ( t , x ) ( 0 , T ) × O k .
Based on (65), by a diagonal process, we find that, up to a subsequence,
v n m ( ω , t , x ) v ( ω , t , x ) f o r a l m o s t a l l ( t , x ) ( 0 , T ) × R n .
By (66) we obtain, for ω Ω 2 ,
u n m ( ω , t , x ) u ( ω , t , x ) f o r a l m o s t a l l ( t , x ) ( 0 , T ) × R n .
By (15) we have
ξ n m ( u n m ( ω ) ) u ( ω ) ξ n m ( u n m ( ω ) ξ n m ( u ( ω ) ) + ξ n m ( u ( ω ) u ( ω ) )
u n m ( ω ) u ( ω ) + ξ n m ( u ( ω ) ) u ( ω ) ,
which together with (67) implies that, for ω Ω 2 ,
ξ n m ( u n m ( ω , t , x ) ) u ( ω , t , x ) f o r a l m o s t a l l ( t , x ) ( 0 , T ) × R n .
By (55), (68) and Mazur’s theorem, we obtain χ 1 ( ω ) = u ( ω ) and we have
ξ n m ( u n m ( ω , t , x ) ) u ( ω , t , x ) w e a k l y i n L p ( 0 , T ; L p ( R n ) ) .
In addition, by (68), for almost all ( t , x ) ( 0 , T ) × R n , we obtain
( 1 + i μ ) | ξ n m ( u n m ( ω , t , x ) ) | 2 β ξ n m ( u n m ( ω , t , x ) ) ( 1 + i μ ) | u ( ω , t , x ) | 2 β u ( ω , t , x ) .
By (56), (70) and Mazur’s theorem, we obtain χ 2 ( ω ) = ( 1 + i μ ) | u ( ω ) | 2 β u ( ω ) and
( 1 + i μ ) | ξ n m ( u n m ( ω ) ) | 2 β ξ n m ( u n m ( ω , t , x ) ) ( 1 + i μ ) | u ( ω ) | 2 β u ( ω ) w e a k l y i n L q ( 0 , T ; L q ( R n ) ) .
Next, we take the limits of (22) to prove that u ( ω ) is a solution of (13) and (14). By (60), we know that for every ω Ω 2 , ξ V L p ( R n ) and ψ C 0 ( 0 , T ) ,
0 T ( v n m ( ω , t ) , ξ ) ψ ( t ) d t + ( 1 + i ν ) 0 T ψ ( t ) ( ( Δ ) α 2 u n m ( ω , t ) , ( Δ ) α 2 ξ ) d t
+ 0 T ψ ( t ) ( ( 1 + i μ ) | ξ n m ( u n m ) | 2 β ξ n m ( u n m ) , ξ ) d t
= ρ 0 T ψ ( t ) ( u n m ( ω , t ) , ξ ) d t + 0 T ( g ( t ) , ξ ) ψ ( t ) d t .
Letting m in (72), by (54), (57) and (71), we have
0 T v ( ω , t ) , ξ ψ ( t ) d t + ( 1 + i ν ) 0 T ψ ( t ) ( Δ ) α 2 u ( ω , t ) , ( Δ ) α 2 ξ d t
+ 0 T ψ ( t ) ( 1 + i μ ) | u | 2 β u , ξ d t = ρ 0 T ψ ( t ) ( u ( ω , t ) , ξ ) d t + 0 T ( g ( t ) , ξ ) ψ ( t ) d t .
By (73) for every ω Ω 2 and ξ V L p ( R n ) , we infer that
d ( v ( ω ) , ξ ) d t + ( 1 + i ν ) ( ( Δ ) α 2 u ( ω ) , ( Δ ) α 2 ξ ) + R n ( 1 + i μ ) | u ( ω ) | 2 β u ( ω ) ξ ( x ) d x = ρ ( u ( ω , t ) , ξ ) + ( g ( t ) , ξ )
on ( 0 , T ) in the sense of scalar distribution.
We next prove v ( ω ) : [ 0 , T ] H is continuous. Firstly, by (54), (71) and (74) we have
d v ( ω ) d t i s i n L 2 ( 0 , T ; V * ) L q ( 0 , T ; L q ( R n ) ) .
By (54) and (69) we see that
u ( ω ) i s i n L 2 ( 0 , T ; V ) L p ( 0 , T ; L p ( R n ) ) ,
and hence
v ( ω ) i s i n L 2 ( 0 , T ; V ) L p ( 0 , T ; L p ( R n ) ) .
By (75) and (76), it follows from [36] that v ( ω ) C ( [ 0 , T ] , H ) and
d v ( ω ) 2 d t = 2 d v ( ω ) d t , v ( ω ) ( V * L q ( R n ) , V L p ( R n ) ) ,
in the sense of scalar distribution on ( 0 , T ) . As a result, we find that u ( ω ) C ( [ 0 , T ] , H ) . Next, we show that u ( ω ) has initial condition u 0 ( ω ) when t = 0 . By (60), we infer that for every ω Ω 2 , ξ V L p ( R n ) and ψ C ( [ 0 , T ] ) ,
v n m ( ω , T ) , ξ ψ ( T ) ( v n m ( ω , 0 ) , ξ ) ψ ( 0 ) 0 T ( v n m ( ω , t ) , ξ ) ψ ( t ) d t
+ ( 1 + i ν ) 0 T ( ( Δ ) α 2 u n m ( ω , t ) , ( Δ ) α 2 ξ ) ψ ( t ) d t
+ 0 T R n ( 1 + i μ ) | ξ n m ( u n m ) | 2 β ξ n m ( u n m ) ξ ( t ) ψ ( t ) d x d t
= ρ 0 T ψ ( t ) ( u n m ( ω , t ) , ξ ) d t + 0 T ( g ( t ) , ξ ) ψ ( t ) d t .
Letting m in (77), it follows from (52), (54), (57), (69) and (71) that
u ˜ ( ω ) 0 T σ ( s ) d W , ξ ψ ( T ) ( u 0 ( ω ) , ξ ) ψ ( 0 ) 0 T ( v ( ω ) , ξ ) ψ ( t ) d t
+ ( 1 + i ν ) 0 T ( Δ ) α 2 u ( ω , t ) , ( Δ ) α 2 ξ ψ ( t ) d t
+ 0 T R n ( 1 + i μ ) | ξ n m ( u n m ) | 2 β ξ n m ( u n m ) ξ ( t ) ψ ( t ) d x d t
= ρ 0 T ψ ( t ) ( u ( ω , t ) , ξ ) d t + 0 T ( g ( t ) , ξ ) ψ ( t ) d t .
On the other hand, by (74), we obtain
u ( ω , T ) 0 T σ ( s ) d W , ξ ψ ( T ) ( u ( ω , 0 ) , ξ ) ψ ( 0 ) 0 T ( v ( ω ) , ξ ) ψ ( t ) d t + ( 1 + i ν ) 0 T ( ( Δ ) α 2 u ( ω , t ) , ( Δ ) α 2 ξ ) ψ ( t ) d t + 0 T R n ( 1 + i μ ) | u ( ω , t ) | 2 β u ( ω , t ) ξ ( t ) ψ ( t ) d x d t = ρ 0 T ψ ( t ) ( u ( ω , t ) , ξ ) d t + 0 T ( g ( t ) , ξ ) ψ ( t ) d t .
By (78) and (79), we obtain
u ( ω , T ) u ˜ ( ω ) , ξ ψ ( T ) = ( u ( ω , 0 ) u 0 ( ω ) , ξ ) ψ ( 0 ) .
Choosing ψ C ( [ 0 , T ] ) with ψ ( 0 ) = 1 and ψ ( T ) = 0 , we obtain from (80) that for every ω Ω 2 and ξ V L p ( R n ) ,
( u ( ω , 0 ) u 0 ( ω ) , ξ ) = 0 ,
which shows that
u ( ω , 0 ) = u 0 ( ω ) i n H .
Similarly, choosing ψ C ( [ 0 , T ] ) with ψ ( 0 ) = 0 and ψ ( T ) = 1 , we can obtain from (80) that for every ω Ω 2 ,
u ( ω , T ) = u ˜ ( ω ) i n H .
By (52) and (82), we know that
u n m ( ω , T ) u ( ω , T ) w e a k l y i n H .
By (83), we can also infer that for every t [ 0 , T ] ,
u n m ( ω , t ) u ( ω , t ) w e a k l y i n H .
By (74) we find that for every ω Ω 2 , ξ V L p ( R n ) and t [ 0 , T ] ,
( v ( ω , t ) , ξ ) + ( 1 + i ν ) 0 t ( ( Δ ) α 2 u ( ω , s ) , ( Δ ) α 2 ξ ) d s
+ 0 t R n ( 1 + i μ ) | u ( ω , s ) | 2 β u ( ω , s ) ξ ( x ) d x d s
= ( v ( ω , 0 ) , ξ ) + ρ 0 t ( u ( ω , s ) , ξ ) d s + 0 t ( g ( s ) , ξ ) d s .
By (81) and (85) we obtain, for every ω Ω 2 , ξ V L p ( R n ) and t [ 0 , T ] ,
( u ( ω , t ) , ξ ) + ( 1 + i ν ) 0 t ( ( Δ ) α 2 u ( ω , s ) , ( Δ ) α 2 ξ ) d s
+ 0 t R n ( 1 + i μ ) | u ( ω , s ) | 2 β u ( ω , s ) ξ ( x ) d x d s
= ( u 0 ( ω ) , ξ ) + ρ 0 t ( u ( ω , s ) , ξ ) d s + 0 t ( g ( s ) , ξ ) d s + 0 t ξ σ ( s ) d W ( s ) .
Note that for every fixed ω Ω 2 ,
u ( ω ) C ( [ 0 , T ] , H ) L 2 ( 0 , T ; V ) L p ( 0 , T ; L p ( R n ) ) .
Next, we prove the uniqueness of solutions to (86) with property (87).
Step 2. Uniqueness of solutions for almost every fixed ω Ω . Given ω Ω 2 , let u 1 ( ω ) and u 2 ( ω ) be the solutions of (86) satisfying (87). We want to show u 1 ( ω , t ) = u 2 ( ω , t ) in H for all t [ 0 , T ] .
Let u ( ω , t ) = u 1 ( ω , t ) u 2 ( ω , t ) . Then by (87) we have
u ( ω ) C ( [ 0 , T ] , H ) L 2 ( 0 , T ; V ) L p ( 0 , T ; L p ( R n ) ) .
On the other hand, by (86) we obtain, for all ξ V L p ( R n ) and t [ 0 , T ] ,
( u ( ω , t ) , ξ ) + ( 1 + i ν ) 0 t ( ( Δ ) α 2 u ( ω , s ) , ( Δ ) α 2 ξ ) d s = ρ 0 t ( u ( ω , s ) , ξ ) d s
0 t R n ( 1 + i μ ) | u 1 ( ω , s ) | 2 β u 1 ( ω , s ) ( 1 + i μ ) | u 2 ( ω , s ) | 2 β u 2 ( ω , s ) ξ ( x ) d x d s ,
which together with (88) implies that
d u ( ω ) d t = ( 1 + i ν ) ( Δ ) α u ( ω ) + ρ u ( ω ) ( ( 1 + i μ ) | u 1 ( ω ) | 2 β u 1 ( ω ) ( 1 + i μ ) | u 2 ( ω ) | 2 β u 2 ( ω ) ) ,
in L 2 ( 0 , T ; V * ) L q ( 0 , T ; L q ( R n ) ) .
By (88) and (89) we obtain
d u ( ω , t ) 2 d t = 2 Re d u ( ω , t ) d t , u ( ω , t ) ( V * L q ( R n ) , V L p ( R n ) ) = 2 ( Δ ) α 2 u ( ω ) 2 + 2 ρ u ( ω ) 2 2 Re ( 1 + i μ | u 1 | 2 β u 1 ( 1 + i μ | u 2 | 2 β u 2 ) , u ( ω ) .
According to (20), we obtain
d u ( ω , t ) 2 d t 2 ρ u ( ω , t ) 2 ,
which together with Gronwall’s inequality, we obtain that for all t [ 0 , T ] ,
u ( ω , t ) 2 e 2 ρ t u ( ω , 0 ) 2 ,
and u ( ω , 0 ) = u 0 ( ω ) u 0 ( ω ) = 0 , therefore, u 1 ( ω , t ) = u 2 ( ω , t ) for all t [ 0 , T ] .
Step 3. Measurability and regularity of solutions. By (84) we know that for every ω Ω 2 , there exists a subsequence { u n m ( ω ) } m = 1 of { u n ( ω ) } n = 1 , which may depend on ω , such that
u n m ( ω , t ) u ( ω , t ) w e a k l y i n H .
Since u ( ω ) is the unique solution of (86) with property (87), we know from (92) that the entire sequence u n ( ω , t ) (not just a subsequence) weakly converges in H; namely, for every ω Ω 2 and t [ 0 , T ] ,
u n ( ω , t ) u ( ω , t ) w e a k l y i n H .
Since for each n N , the process u n is F t -adapted, it follows from (93) that u is also F t -adapted.
Next, we show the measurability of u : Ω L 2 ( 0 , T ; V ) . By Lemma 2, we see that u n is bounded in L 2 ( Ω , L 2 ( 0 , T ; V ) ) , hence there exists u L 2 ( Ω , L 2 ( 0 , T ; V ) ) and a subsequence (not relabeled) such that
u n u w e a k l y i n L 2 ( Ω , L 2 ( 0 , T ; V ) ) .
By (94), (67) and Mazur’s theorem, we obtain that u ( ω ) = u ( ω ) in L 2 ( 0 , T ; V ) for almost all ω Ω , and hence u : Ω L 2 ( 0 , T ; V ) is measurable and
u L 2 ( Ω , L 2 ( 0 , T ; V ) ) 2 lim inf n u n L 2 ( Ω , L 2 ( 0 , T ; V ) ) 2 .
We now prove the measurability of u : Ω L p ( 0 , T ; L p ( R n ) ) . As before, given ω Ω 2 , since u ( ω ) is the unique solution of (86) with property (87), by (69) we obtain, for every ω Ω 2 ,
ξ n ( u n ( ω ) ) u ( ω ) w e a k l y i n L p ( 0 , T ; L p ( R n ) ) .
In addition, by Lemma 2, the sequence { ξ n ( u n ) } n = 1 is bounded in L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) , and hence there exists ξ L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) and a subsequence (not relabeled) such that
ξ n ( u n ) ξ w e a k l y i n L p ( 0 , T ; L p ( R n ) ) .
By (96) and (97) and Mazur’s theorem, we find that u ( ω ) = ξ ( ω ) in L p ( 0 , T ; L p ( R n ) ) for almost all ω Ω . This implies u : Ω L p ( 0 , T ; L p ( R n ) ) is measurable and
u L p ( Ω , L p ( 0 , T ; v ) ) p lim inf n u n L p ( Ω , L p ( 0 , T ; V ) ) p .
Note that u is a continuous H-valued F t -adapted process. Therefore, u : Ω C ( [ 0 , T ] , H ) is measurable. By (53) and the uniqueness of solution of (86), for every ω Ω 2 ,
u n ( ω ) u ( ω ) w e a k s t a r i n L ( 0 , T ; H ) ,
which implies
u ( ω ) L ( 0 , T ; H ) lim inf n u n ( ω ) L ( 0 , T ; H ) .
By (99) and Fatou’s lemma we obtain
Ω u ( ω ) L ( 0 , T ; H ) 2 d P Ω lim inf n u n ( ω ) L ( 0 , T ; H ) 2 d P lim inf n Ω u n ( ω ) L ( 0 , T ; H ) d P .
By (100) and Lemma 2, we obtain Ω u ( ω ) L ( 0 , T ; H ) 2 d P < , which along with the path continuity of u implies u L 2 ( Ω , C ( [ 0 , T ] , H ) ) . By (86) and the above measurability of u, we see that u is a solution of (13) and (14) in the sense of Definition 5. We obtain the uniqueness of the solutions follows from Step2, and the uniform estimates of (51) follows from (95), (98), (100) and Lemma 2. □

4. Existence of Solutions: General Additive Noise

In this section, we study the existence and uniqueness of solutions to problem (1) and (2) with a general additive noise,
d u ( t ) + ( 1 + i ν ) ( Δ ) α u ( t ) d t + ( 1 + i μ ) | u ( t ) | 2 β u ( t ) d t = ρ u ( t ) d t + g ( t , x ) d t + σ ( t , ω ) d W ,
with initial condition
u ( 0 ) = u 0 ,
where σ : R × Ω L 2 ( U , H ) is a progressively measurable process such that
σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) f o r e v e r y T > 0 .
We investigate the existence and uniqueness of solutions to problem (101) and (102) under condition (103).
Lemma 4.
Suppose (103) holds and u 0 L 2 ( Ω , H ) is F 0 -measurable, then problem (101) and (102) has a unique solution u in the sense of Definition 5. Moreover, u satisfies,
u ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + u ( t ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p L 3 ( T ) ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 + σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) 2 ) ,
where L 3 ( T ) is a positive number depending only on T.
Proof. 
We first approximate the drift coefficient σ with (103) by regular drift terms and construct a sequence of approximate solutions. We then derive uniform estimates, and prove that the limit of the approximate solution is a solution of (101) and (102). Finally, we show the uniqueness of the solutions.
Step 1. Approximate solutions. We first approximate σ with (103) by regular functions. Therefore, we choose a positive integer k 0 such that k 0 > ( p 2 ) n 4 p . Then, we obtain that H 2 k 0 ( R n ) L p ( R n ) . Given m N , denote by
σ m = ( I 1 m Δ ) k 0 σ .
Then we have σ m L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , V 0 ) ) ) . By Lemma 3 we find that, for every m N , there exists a unique continuous H-valued F t -adapted stochastic process u m with
u m ( ω ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) L 2 ( Ω , L 2 ( 0 , T ; V ) ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) , T > 0 ,
such that for all t 0 and ξ V L p ( R n ) ,
( u m ( ω , t ) , ξ ) + ( 1 + i ν ) 0 t ( ( Δ ) α 2 u m ( ω , s ) , ( Δ ) α 2 ξ ) d s + 0 t R n ( 1 + i μ ) | u m ( ω , s ) | 2 β u m ( ω , s ) ξ ( x ) d x d s = ( u 0 ( ω ) , ξ ) + ρ 0 t ( u m ( ω , s ) , ξ ) d s + 0 t ( g ( s ) , ξ ) d s + 0 t ξ σ m ( s ) d W ( s ) ,
P–almost surely. Where ξ in the stochastic term is considered as an element of H * by Riesz’s representation theorem. Moreover, by (51), Lemma 3 and the contractility of the operator ( I 1 m Δ ) k 0 , we find that for all m N , there exists a positive number C 1 = C 1 ( T ) independent of m such that
u m ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u m ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + u m L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p
C 1 ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 + σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) 2 ) .
By (41) and (106) we obtain that, for all m N ,
( 1 + i μ ) | u m | 2 β u m L q ( Ω , L q ( 0 , T ; L q ( R n ) ) ) q
c 9 C 1 ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 + σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) 2 ) .
Next, we derive further uniform estimates of the approximate solutions.
Step 2. Uniform estimates on { u m } m = 1 . Note that by the proof of Lemma 3, for every m N , the solution u m of (105) is given by the limit of the solution u m , n of the following equation in V * ,
u m , n ( t ) + ( 1 + i ν ) 0 t ( ( Δ ) α u m , n ( s ) + ( 1 + i μ ) | ξ n ( u m , n ( s ) ) | 2 β ξ n ( u m , n ( s ) ) d s
= u 0 + ρ 0 t u m , n ( s ) d s + 0 t g ( s , x ) d s + 0 t σ m ( s , ω ) d W .
By (108) and integration by parts of Ito’s formula, we obtain, for all m 1 , m 2 N , with u ^ m , n ( t ) = u m 1 , n ( t ) u m 2 , n ( t ) ,
u ^ m , n ( t ) 2 + 2 0 t ( Δ ) α 2 u ^ m , n ( s ) 2 d s + 2 R e 0 t R n ( 1 + i μ ) | ξ n ( u m 1 , n ( s ) ) | 2 β ξ n ( u m 1 , n ( s ) ) | ξ n ( u m 2 , n ( s ) ) | 2 β ξ n ( u m 2 , n ( s ) ) d x d s = 2 ρ 0 t u ^ m , n 2 d s + 0 t σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s + 2 R e 0 t u ^ m , n ( s ) ( σ m 1 ( ω ) σ m 2 ( ω ) ) d W .
Together with (20), we obtain
u ^ m , n ( t ) 2 + 2 0 t ( Δ ) α 2 u ^ m , n ( s ) 2 d s 2 ρ 0 t u ^ m , n 2 d s
+ 0 t σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s + 2 R e 0 t u ^ m , n ( s ) ( σ m 1 ( ω ) σ m 2 ( ω ) ) d W ,
from which we can deduce that, for each T > 0 ,
E ( sup 0 r t u ^ m , n ( r ) 2 ) 2 ρ 0 t E ( sup 0 r s u ^ m , n ( r ) 2 ) d s + E 0 T σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s + 2 E sup 0 r t 0 r u ^ m , n ( s ) ( σ m 1 ( ω ) σ m 2 ( ω ) ) d W ( s ) .
By the Burkholder–Davis–Gundy inequality and Young’s inequality, we infer
2 E sup 0 r t 0 r u ^ m , n ( s ) ( σ m 1 ( ω ) σ m 2 ( ω ) ) d W ( s )
1 2 E ( sup 0 r t u ^ m , n ( r ) 2 ) + c 12 E 0 t σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s .
Therefore, we have
E ( sup 0 r t u ^ m , n ( r ) 2 ) 4 ρ 0 t E ( sup 0 r s u ^ m , n ( r ) 2 ) d s + 2 ( 1 + c 12 ) E 0 T σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s .
Applying the Gronwall inequality, for all t [ 0 , T ] , we deduce,
E ( sup 0 r t u ^ m , n ( r ) 2 ) 2 ( 1 + c 12 ) e 4 ρ t E 0 T σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s .
By (109), we obtain
2 E 0 T ( Δ ) α 2 u ^ m , n 2 d s 2 ρ E 0 T u ^ m , n 2 d s + ( c 12 + 1 ) E 0 T σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s ,
which together above we can deduce, there exists a positive number c 13 = c 13 ( T ) independent of m 1 , m 2 and n such that
E sup 0 t T u m 1 , n ( t ) u m 2 , n ( t ) 2 + E 0 T u m 1 , n ( t ) u m 2 , n ( t ) H α 2 d t
c 13 E 0 T σ m 1 ( ω ) σ m 2 ( ω ) L 2 ( U , H ) 2 d s ,
where c 13 = 2 ( 1 + c 12 ) e 4 ρ T [ 1 + T + 2 ρ T C ( n , α ) ] + c 12 + 1 C ( n , α ) .
Note that the proof of Lemma 3, we know that there exists a subset Ω 1 of Ω with P ( Ω 1 ) = 1 such that for every ω Ω 1 and every fixed m N , as n ,
u m , n ( ω ) u m ( ω ) w e a k s t a r i n L ( 0 , T ; H ) ,
u m , n ( ω ) u m ( ω ) w e a k l y i n L 2 ( 0 , T ; V ) ,
ξ n ( u m , n ) ( ω ) u m ( ω ) w e a k l y i n L p ( 0 , T ; L p ( R n ) ) ,
( 1 + i μ ) | ξ n ( u m , n ( ω ) ) | 2 β ξ n ( u m , n ( ω ) ) ( 1 + i μ ) | u m , n ( ω ) | 2 β u m , n ( ω ) w e a k l y i n L q ( 0 , T ; L q ( R n ) ) .
By (112) and Fatou’s lemma, we obtain
E u m 1 u m 2 L 2 ( 0 , T ; V ) 2 lim inf n E u m 1 u m 2 L 2 ( 0 , T ; V ) 2 c 13 E 0 T σ m 1 σ m 2 L 2 ( U , H ) 2 d s .
Similarly, we obtain
E u m 1 u m 2 C ( 0 , T ; H ) 2 c 13 E 0 T σ m 1 σ m 2 L 2 ( U , H ) 2 d s .
Note that σ m σ in L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) as m , and hence { σ m } m = 1 is a Cauchy sequence in L 2 ( Ω , C ( [ 0 , T ] , H ) ) L 2 ( Ω , L 2 ( 0 , T ; V ) ) such that
lim m u m = u i n L 2 ( Ω , C ( [ 0 , T ] , H ) ) L 2 ( Ω , L 2 ( 0 , T ; V ) ) .
By (117) we see that u is a continuous H-valued F t -adapted process. On the other hand, by (117) we infer that, up to a subsequence (not relabeled) such that
u m u a l m o s t e v e r y w h e r e i n Ω × [ 0 , T ] × R n .
By (107), there exists χ L q ( Ω , L q ( 0 , T ; L q ( R n ) ) ) such that, up to a subsequence,
( 1 + i μ ) | u m | 2 β u m χ w e a k l y i n L q ( Ω , L q ( 0 , T ; L q ( R n ) ) ) .
By (118) and (119) and Mazur’s theorem, we obtain χ = ( 1 + i μ ) | u | 2 β u and thus
( 1 + i μ ) | u m | 2 β u m ( 1 + i μ ) | u | 2 β u w e a k l y i n L q ( Ω , L q ( 0 , T ; L q ( R n ) ) ) .
Similarly, by (106) and (118), we obtain
u m u w e a k l y i n L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) .
Next, we take the limit of (105) as m .
Step 3. Limit of approximate equation. Let ϕ L ( Ω , R ) and ξ V L p ( R n ) . Then, by (117) we obtain, for all t [ 0 , T ] ,
E ( ( u m ( t ) , ξ ) ϕ ) E ( ( u ( t ) , ξ ) ϕ ) .
In addition, for each t [ 0 , T ] , by (117) we obtain
E ϕ 0 t ( ( Δ ) α 2 u m ( s ) , ( Δ ) α 2 ξ ) d s = E 0 T ( ( Δ ) α 2 u m ( s ) , 1 [ 0 , t ] ( s ) ϕ ( Δ ) α 2 ξ ) d s
E 0 T ( ( Δ ) α 2 u ( s ) , 1 [ 0 , t ] ( s ) ϕ ( Δ ) α 2 ξ ) d s = E ϕ 0 t ( ( Δ ) α 2 u ( s ) , ( Δ ) α 2 ξ ) d s .
Similarly, for each t [ 0 , T ] , by (120), we obtain
E ϕ 0 t R n ( 1 + i μ ) | u m ( s ) | 2 β u m ( s ) ξ ( x ) d x d s E ϕ 0 t R n ( 1 + i μ ) | u ( s ) | 2 β u ( s ) ξ ( x ) d x d s .
Since σ m σ in L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) , we obtain, for each t [ 0 , T ] ,
E ϕ 0 t ξ σ m ( s ) d W ( s ) E ϕ 0 t ξ σ ( s ) d W ( s ) .
Multiplying Equation (105) by ϕ , taking the expectation, and then letting m , by (117) and (122)–(125) we obtain, for each t [ 0 , T ] and ξ V L p ( R n ) ,
E ( ϕ ( u ( t ) , ξ ) ) + ( 1 + i ν ) E ϕ 0 t ( ( Δ ) α 2 u ( s ) , ( Δ ) α 2 ξ ) d s + E ϕ 0 t R n ( 1 + i μ ) | u ( s ) | 2 β u ( s ) ξ ( x ) d x d s = E ( ϕ ( u 0 , ξ ) ) + ρ E ϕ 0 t ( u ( s ) , ξ ) d s + E ϕ 0 t ( g ( s ) , ξ ) d s + E ϕ 0 t ξ σ ( s ) d W ( s ) .
Since ϕ L ( Ω , R ) is arbitrary, by (126), we infer that for every t [ 0 , T ] and ξ V L p ( R n ) , there exists a subset Ω 2 (depending on t and ξ ) of Ω with P ( Ω 2 ) = 0 such that for all ω Ω Ω 2 ,
( u ( t ) , ξ ) + ( 1 + i ν ) 0 t ( ( Δ ) α 2 u ( ω , s ) , ( Δ ) α 2 ξ ) d s + 0 t R n ( 1 + i μ ) | u ( ω , s ) | 2 β u ( ω , s ) ξ ( x ) d x d s
= ( u 0 ( ω ) , ξ ) + ρ 0 t ( u ( ω , s ) , ξ ) d s + 0 t ( g ( s ) , ξ ) d s + 0 t ξ σ ( s ) d W ( s ) .
Note that the subset Ω 2 may depend on t [ 0 , T ] and ξ V L p ( R n ) in general. However, since every term in (127) is continuous in t and the space ξ V L p ( R n ) is separable, we are able to choose a subset Ω 2 of P-probability zero, which is independent of t and ξ , such that (127) is valid for all ω Ω Ω 2 , for all t [ 0 , T ] and ξ V L p ( R n ) . By (117) and (121), we have
u L 2 ( Ω , C ( [ 0 , T ] , H ) ) L 2 ( Ω , L 2 ( 0 , T ; V ) ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) .
Moreover, taking the limit in (106) with respect to m, by (128), we know that
u ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + u L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p
C 1 ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 + σ L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) 2 ) .
By (127)–(129) we see that u is a solution of (101) and (102) with the desired estimates.
Step 4. Uniqueness of solutions. Suppose u 1 and u 2 be the solutions of (101) and (102) in the sense of Definition 5 with initial conditions u 0 , 1 and u 0 , 2 , Let u ^ = u 1 u 2 , then we have, for all ξ V L p ( R n ) and t [ 0 , T ] , P–almost surely,
( u ^ ( t ) , ξ ) + ( 1 + i ν ) 0 t ( ( Δ ) α 2 u ^ ( s ) , ( Δ ) α 2 ξ ) d s
= ( u 0 , 1 u 0 , 2 , ξ ) 0 t R n ( ( 1 + i μ ) | u 1 | 2 β u 1 ( 1 + i μ ) | u 2 | 2 β u 2 ) ξ ( x ) d x d s + ρ 0 t ( u ^ ( s ) , ξ ) d s .
Similar to (91), we obtain that
u ^ ( ω , t ) 2 e c 14 t u ^ ( ω , 0 ) 2 ,
which implies that
E u 1 u 2 C ( [ 0 , T ] , H ) 2 e c 14 T E ( u 0 , 1 u 0 , 2 2 ) ,
and hence the solution is unique. □

5. Existence of Solutions: Globally Lipschitz Noise

In this section, we suppose that σ : R × Ω × H L 2 ( U , H ) is globally Lipschitz continuous in its third argument uniformly for ( t , ω ) R × Ω ; namely, there exists a positive number L 0 such that for all t R , ω Ω and u 1 , u 2 H ,
σ ( t , ω , u 1 ) σ ( t , ω , u 2 ) L 2 ( U , H ) L 0 u 1 u 2 .
In addition, σ satisfies (4). We suppose that for every fixed u H , σ ( · , · , u ) : R × Ω L 2 ( Ω , H ) is progressively measurable.
Lemma 5.
Suppose (131) holds and u 0 L 2 ( Ω , H ) is F 0 -measurable, then problem (1) and (2) has a unique solution u in the sense of Definition 5. Moreover, the solution u is continuous in u 0 from L 2 ( Ω , H ) to L 2 ( Ω , C ( [ 0 , T ] ; H ) ) L 2 ( Ω , L 2 ( Ω , L 2 ( 0 , T ; V ) ) ) and u satisfies the energy equation
u ( t ) 2 + 2 0 t ( Δ ) α 2 u ( s ) 2 d s + 2 0 t R n | u | 2 β + 2 d x d s
= u 0 2 + 2 ρ 0 t u ( s , x ) 2 d s + 2 R e 0 t ( u ( s ) , g ( s ) ) d s + 2 R e 0 t u ( s ) σ ( s , ω ( s ) ) d W
+ 0 t σ ( s , u ( s ) ) L 2 ( U , H ) 2 d s ,
for all t [ 0 , T ] , P–almost surely. In addition,
u ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + u ( t ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p
L 4 ( T ) ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 ) ,
where L 4 ( T ) is a positive number only depending on T.
Proof. 
For an F 0 -measurable initial condition u 0 L 2 ( Ω , H ) and a given progressively measurable process z L 2 ( Ω , L 2 ( 0 , T ; H ) ) , we investigate the following stochastic equation:
d u ( t ) + ( 1 + i ν ) ( Δ ) α u ( t ) d t + ( 1 + i μ ) | u ( t ) | 2 β u ( t ) d t = ρ u ( t ) d t + g ( t ) d t + σ ( t , z ( t ) ) d W ,
with initial condition
u ( 0 ) = u 0 .
Since z L 2 ( Ω , L 2 ( 0 , T ; H ) ) is a progressively measurable process. By (4) and (131), we notice that σ ( · , z ( · ) ) L 2 ( Ω , L 2 ( 0 , T ; L 2 ( U , H ) ) ) is also progressively measurable. Then, for every F 0 -measurable u 0 L 2 ( Ω , H ) , by Lemma 4, problem (133) and (134) has a unique solution u in the sense of Definition 5 which satisfies (104). We define a map G : L 2 ( Ω , L 2 ( 0 , T ; H ) ) L 2 ( Ω , L 2 ( 0 , T ; H ) ) , for every z L 2 ( Ω , L 2 ( 0 , T ; H ) ) , G ( z ) = u , where u is the unique solution of (133) and (134).
Next we prove that G is a contraction when L 2 ( Ω , L 2 ( 0 , T ; H ) ) is endowed with an equivalent norm using Banach fixed point theorem.
Step 1. Contractility of G . Let z 1 , z 2 be progressively measurable in L 2 ( Ω , L 2 ( 0 , T ; H ) ) , and u 1 , u 2 be the solution of (133) and (134) given by Lemma 4. Let u ^ = u 1 u 2 and z ^ = z 1 z 2 . Then, we have
u ^ ( t ) + ( 1 + i ν ) 0 t ( Δ ) α u ^ ( s ) d s + 0 t ( ( 1 + i μ ) | u 1 | 2 β u 1 ( 1 + i μ ) | u 2 | 2 β u 2 ) d s
= ρ 0 t u ^ ( s ) d s + 0 t ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) d W ( s ) i n V L p ( R n ) * .
Let k 0 be a positive integer such that k 0 > ( 2 q ) n 4 q . Then we have W 2 k 0 , q ( R n ) L 2 ( R n ) . We set that
u ^ ε = ( I ε Δ ) k 0 u ^ ,
f ε ( t ) = ( I ε Δ ) k 0 ( ( 1 + i μ ) | u 1 | 2 β u 1 ( 1 + i μ ) | u 2 | 2 β u 2 ) ,
σ ε ( t ) = ( I ε Δ ) k 0 ( σ ( t , z 1 ) σ ( t , z 2 ) ) .
Hence, we obtain
u ^ ε ( t ) + ( 1 + i ν ) 0 t ( Δ ) α u ^ ε ( s ) d s + 0 t f ε ( s ) d s = ρ 0 t u ^ ε ( s ) d s + 0 t σ ε ( s ) d W ( s ) i n H .
Let θ 0 be a fixed constant, u ^ ε θ = e θ t u ^ ε , u ^ θ = e θ t u ^ . By (136), we obtain that
u ^ ε θ ( t ) + θ 0 t u ^ ε θ ( s ) d s + ( 1 + i ν ) 0 t ( Δ ) α u ^ ε θ ( s ) d s + 0 t e μ s f ε ( s ) d s = ρ 0 t u ^ ε θ ( s ) d s + 0 t e θ s σ ε ( s ) d W ( s )
in H. By (137) and integration by parts of Ito’s formula, we obtain
u ^ ε θ ( t ) 2 + 2 θ 0 t u ^ ε θ ( t ) 2 d s + 2 0 t ( Δ ) α 2 u ^ ε θ ( s ) 2 d s + 2 R e 0 t e θ s ( f ε ( s ) , u ^ ε θ ( s ) ) d s
= 2 ρ 0 t u ^ ε θ ( s ) 2 d s + 2 Re 0 t e θ s u ^ ε θ ( s ) σ ε ( s ) d W ( s ) + 0 t e θ s σ ε ( s ) L 2 ( U , H ) 2 d s .
For all r ( 1 , ) , h L r ( R n ) , we have
( I ε Δ ) 1 h L r ( R n ) h L r ( R n ) a n d lim ε 0 ( I ε Δ ) 1 h h L r ( R n ) = 0 .
By (139) and the dominated convergence theorem, we obtain that, for every t [ 0 , T ] ,
lim ε 0 u ^ ε θ ( t ) 2 = u ^ θ ( t ) 2 ,
lim ε 0 0 t u ^ ε θ ( s ) 2 d s = 0 t u ^ θ ( s ) 2 d s ,
lim ε 0 0 t ( Δ ) α 2 u ^ ε θ ( s ) 2 d s = 0 t ( Δ ) α 2 u ^ θ ( s ) 2 d s ,
lim ε 0 0 t e θ s σ ε ( s ) L 2 ( U , H ) 2 d s = 0 t e θ s σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) L 2 ( U , H ) 2 d s ,
lim ε 0 f ε ( s ) ( ( 1 + i μ ) | u 1 ( s ) | 2 β u 1 ( s ) ( 1 + i μ ) | u 2 ( s ) | 2 β u 2 ( s ) ) L q ( R n ) = 0 ,
and
lim ε 0 u ^ ε θ ( s ) u ^ θ ( s ) L p ( R n ) = 0 .
Then, we obtain
lim ε 0 f ε ( s ) u ^ ε θ ( s ) ( ( 1 + i μ ) | u 1 ( s ) | 2 β u 1 ( s ) ( 1 + i μ ) | u 2 ( s ) | 2 β u 2 ( s ) ) u ^ θ ( s ) L 1 ( R n ) = 0 .
By (139) and the dominated convergence theorem, we obtain
lim ε 0 0 t e θ s Re ( f ε ( s ) , u ^ ε θ ( s ) ) d s = 0 t e θ s R n u ^ θ ( s ) ( ( 1 + i μ ) | u 1 ( s ) | 2 β u 1 ( s ) ( 1 + i μ ) | u 2 ( s ) | 2 β u 2 ( s ) ) d x d s .
To prove the stochastic term in (138), we need to prove the convergence of quadratic variation,
Re 0 t e θ s u ^ ε θ ( s ) σ ε ( s ) d W ( s ) Re 0 t e θ s u ^ θ ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) d W ( s ) ) T 1 2
= Re ( e θ s u ^ ε θ ( s ) σ ε ( s ) ) Re ( e θ s u ^ θ ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) ) L 2 ( 0 , T ; L 2 ( U , R ) )
e θ s u ^ ε θ ( s ) σ ε ( s ) e θ s u ^ ε θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( 0 , T ; L 2 ( U , R ) )
+ e θ s ( u ^ ε θ ( s ) u ^ θ ( s ) ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( 0 , T ; L 2 ( U , R ) ) .
By (139), we have, for s [ 0 , T ] ,
e θ s u ^ ε θ ( s ) σ ε ( s ) e θ s u ^ ε θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( U , R ) )
e θ s u ^ θ ( s ) σ ε ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( U , R ) 0 a s ε 0 .
By (139) and (146), we obtain
e θ s u ^ ε θ ( s ) σ ε ( s ) e θ s u ^ ε θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( U , R )
2 e θ s u ^ θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( U , R ) ) .
It follows from (146) and (147) and the dominated convergence theorem, we have
lim ε 0 e θ s u ^ ε θ ( s ) σ ε ( s ) e θ s u ^ ε θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( 0 , T ; L 2 ( U , R ) ) = 0
and
lim ε 0 e θ s ( u ^ ε θ ( s ) u ^ θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( 0 , T ; L 2 ( U , R ) ) = 0 .
By (145) and (148) and (149), we obtain
lim ε 0 0 t e θ s u ^ ε θ ( s ) σ ε ( s ) d W ( s ) 0 t e θ s u ^ θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) d W ( s ) T 1 2 = 0
in probability, and hence
lim ε 0 0 t e θ s u ^ ε θ ( s ) σ ε ( s ) d W ( s ) = 0 t e θ s u ^ θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) d W ( s ) ,
in probability uniformly for t [ 0 , T ] . Letting ε 0 in (138). By (140)–(144) and (150), for t [ 0 , T ] we infer
u ^ θ ( t ) 2 + 2 θ 0 t u ^ θ ( s ) 2 d s + 2 0 t ( Δ ) α 2 u ^ θ 2 d s
+ 2 Re 0 t e θ s R n ( ( 1 + i μ ) | u 1 ( s ) | 2 β u 1 ( s ) ( 1 + i μ ) | u 2 ( s ) | 2 β u 2 ( s ) ) u ^ θ ( s ) d x d s
= 2 ρ 0 t u ^ θ ( s ) 2 d s + 2 Re 0 t e θ s u ^ θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) d W ( s )
+ 0 t e θ s ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( U , H ) 2 d s .
Taking the expectation of (151), and applying in (131), we obtain
2 θ E 0 T e θ s ( u 1 ( s ) u 2 ( s ) ) 2 d s
2 ρ E 0 T e θ s ( u 1 ( s ) u 2 ( s ) ) 2 d s + 2 E sup 0 t T Re 0 t e θ s u ^ θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) d W ( s )
+ E 0 T e θ s ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) L 2 ( U , H ) 2 d s .
By the Burkholder–Davis–Gundy inequality and Young’s inequality, we obtain
2 E sup 0 t T 0 t e θ s u ^ θ ( s ) ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) d W ( s )
c 15 E 0 T u ^ θ ( s ) 2 e θ s σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) L 2 ( U , H ) 2 1 2
c 15 2 4 E 0 T u ^ θ ( s ) 2 d s + E 0 T e θ s ( σ ( s , z 1 ( s ) ) σ ( s , z 2 ( s ) ) ) 2 d s .
Hence, we have
2 θ E 0 T e θ s ( u 1 ( s ) u 2 ( s ) ) 2 d s
( 2 ρ + c 15 2 4 ) E 0 T e θ s ( u 1 ( s ) u 2 ( s ) ) 2 d s + 2 L 0 2 E 0 T e θ s ( z 1 ( s ) z 2 ( s ) ) 2 d s .
For fixed θ 0 , denote by L θ 2 ( Ω , L 2 ( 0 , T ; H ) ) the space L 2 ( Ω , L 2 ( 0 , T ; H ) ) equipped with the equivalent norm
u L θ 2 ( Ω , L 2 ( 0 , T ; H ) ) = E 0 T e θ s u ( s ) 2 1 2 f o r u L 2 ( Ω , L 2 ( 0 , T ; H ) ) ) .
Then by (152) we obtain, for θ > ρ + c 15 2 8 ,
G ( z 1 ) G ( z 2 ) L θ 2 ( Ω , L 2 ( 0 , T ; H ) ) = u 1 u 2 L θ 2 ( Ω , L 2 ( 0 , T ; H ) ) 2 L 0 2 θ 2 ρ c 15 2 4 z 1 z 2 L θ 2 ( Ω , L 2 ( 0 , T ; H ) ) .
We choose a positive number θ large enough such that 2 L 0 2 θ 2 ρ c 15 2 4 < 1 . Then, we obtain that G is a contraction. Therefore, it has a unique fixed point, which is the unique solution of (133) and (134) in the sense of Definition 5.
Step 2. Continuity of solutions in initial date. Let u 0 , 1 , u 0 , 2 L 2 ( Ω , H ) be F 0 -measurable, u 1 = G ( u 1 ) , u 2 = G ( u 2 ) be the fixed points of G corresponding to initial date u 0 , 1 and u 0 , 2 . Denote by u ^ = u 1 u 2 , u ^ 0 = u 0 , 1 u 0 , 2 . By (151) with θ = 0 , for t [ 0 , T ] , we obtain
u ^ ( t ) 2 + 2 0 t ( Δ ) α 2 u ^ ( s ) 2 d s u ^ 0 2 + 2 ρ 0 t u ^ ( s ) 2 d s
+ 2 R e 0 t u ^ ( s ) ( σ ( s , u 1 ( s ) ) σ ( s , u 2 ( s ) ) ) d W ( s ) + 0 t σ ( s , u 1 ( s ) ) σ ( s , u 2 ( s ) ) L 2 ( U , H ) 2 d s .
By (154), we find that for all 0 t T ,
E sup 0 r t u ^ ( r ) 2 E ( u ^ 0 2 ) + 2 ρ 0 t E sup 0 r s u ^ ( r ) 2 d s
+ 2 E sup 0 r t 0 r u ^ ( s ) ( σ ( s , u 1 ( s ) ) σ ( s , u 2 ( s ) ) ) d W ( s )
+ E 0 T σ ( s , u 1 ( s ) ) σ ( s , u 2 ( s ) ) L 2 ( U , H ) 2 d s .
By the Burkholder–Davis–Gundy inequality and (131), we deduce, for all 0 t T ,
2 E sup 0 r t 0 r u ^ ( s ) ( σ ( s , u 1 ( s ) ) , σ ( s , u 2 ( s ) ) ) d W ( s )
c 16 E 0 t u ^ ( s ) 2 σ ( s , u 1 ( s ) ) σ ( s , u 2 ( s ) ) L 2 ( U , H ) 2 d s 1 2
c 16 E sup 0 s t u ^ ( s ) 0 t σ ( s , u 1 ( s ) ) σ ( s , u 2 ( s ) ) L 2 ( U , H ) 2 d s 1 2
1 2 E sup 0 r t u ^ ( r ) 2 + 1 2 c 16 2 E 0 t σ ( s , u 1 ( s ) ) σ ( s , u 2 ( s ) ) L 2 ( U , H ) 2 d s
1 2 E sup 0 r t u ^ ( r ) 2 + 1 2 c 16 2 L 0 2 E 0 t u 1 ( s ) u 2 ( s ) 2 d s
1 2 E sup 0 r t u ^ ( r ) 2 + 1 2 c 16 2 L 0 2 0 t E sup 0 r s u ^ ( r ) 2 d s .
By (131), (155) and (156), we obtain, for all 0 t T ,
E sup 0 r t u ^ ( r ) 2 2 E ( u ^ ( 0 ) 2 ) + ( c 16 2 L 0 2 + 2 L 0 2 + 4 ρ ) 0 t E sup 0 r s u ^ ( r ) 2 d s .
By (157) and the Gronwall inequality, we find that for all 0 t T ,
E sup 0 r t u ^ ( r ) 2 2 e ( c 16 2 L 0 2 + 2 L 0 2 + 4 ρ ) t E ( u ^ ( 0 ) 2 ) .
In addition, by (156), (158) and (154) with t = T , we obtain
E 0 T ( Δ ) α 2 u ^ ( s ) 2 d s c 17 E ( u ^ 0 2 ) ,
where c 17 > 0 depending only on T. By (158) and (159), we obtain
u 1 u 2 L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u 1 u 2 L 2 ( Ω , L 2 ( 0 , T ; V ) ) 2 c 20 u 0 , 1 u 0 , 2 L 2 ( Ω , H ) 2 .
Therefore, the solution is continuous in initial data.
Step 3. Uniform estimates of solutions. We suppose u is the solution of (1) and (2) with initial data u 0 L 2 ( Ω , H ) , Then we have
u ( t ) + ( 1 + i ν ) 0 t ( Δ ) α u ( s ) d s + 0 t ( 1 + i μ ) | u ( s ) | 2 β u ( s ) d s = u 0 + ρ 0 t u ( s ) d s + 0 t g ( s ) d s
+ 0 t σ ( s , u ( s ) ) d W i n ( V L p ( R n ) ) * ,
P–almost surely. We set
u ε ( t ) = ( I ε Δ ) k 0 u ( t ) , u 0 , ε = ( I ε Δ ) k 0 u 0 , g ε ( t ) = ( I ε Δ ) k 0 g ( t )
and
f ε ( t ) = ( I ε Δ ) k 0 ( 1 + i μ ) | u ( t ) | 2 β u ( t ) , σ ε ( t ) = ( I ε Δ ) k 0 σ ( t , u ( t ) ) .
Then by (161) we obtain, for t [ 0 , T ] ,
u ε ( t ) + ( 1 + i ν ) 0 t ( Δ ) α u ε ( s ) d s + 0 t f ε ( s ) d s ,
= u 0 , ε + ρ 0 t u ε ( s ) d s + 0 t g ε ( s ) d s + 0 t σ ε ( s ) d W ( s ) i n H ,
P–almost surely. By (162) and integration by parts of Ito’s formula, we obtain, for every t [ 0 , T ] ,
u ε ( t ) 2 + 2 0 t ( Δ ) α 2 u ε ( s ) 2 d s + 2 Re 0 t R n f ε ( s , x , u ( s ) ) u ¯ ε ( s ) d x d s
= u 0 , ε 2 + 2 ρ 0 t u ε ( s , x ) 2 d x d s + 2 Re 0 t R n g ε ( s ) u ¯ ε ( s ) d x d s + 2 Re 0 t u ε ( s ) σ ε ( s , ω ( s ) ) d W
+ 0 t σ ε ( s , u ( s ) ) L 2 ( U , H ) 2 d s ,
P–almost surely. Taking the limit of (163) as ε 0 , we obtain, for t [ 0 , T ] ,
u ( t ) 2 + 2 0 t ( Δ ) α 2 u ( s ) 2 d s + 2 Re 0 t R n ( 1 + i μ ) | u ( s ) | 2 β u ( s ) u ¯ ( s ) d x d s
= u 0 2 + 2 ρ 0 t u ( s , x ) 2 d x d s + 2 Re 0 t ( u ( s ) , g ( s ) ) d s + 2 Re 0 t u ( s ) σ ( s , ω ( s ) ) d W
+ 0 t σ ( s , u ( s ) ) L 2 ( U , H ) 2 d s ,
P–almost surely. Similar to the proof of Lemma 2 and by (4), we can derive the uniform estimates (132). □

6. Existence of Solutions: Locally Lipschitz Noise

In this section, we prove the existence and uniqueness of solutions to problem (1) and (2) with a locally Lipschitz continuous diffusion term.
Let σ : R n × Ω × H L 2 ( U , H ) which satisfies condition (3) be locally Lipschitz continuous in its third argument uniformly for ( t , ω ) R × Ω , we introduce a truncation operator η n : H H given by
η n ( u ) = u i f u n , n u u i f u > n .
Then η n : H H is globally Lipschitz continuous with unit Lipschitz coefficient,
η n ( u 1 ) η n ( u 2 ) u 1 u 2 , f o r a l l u 1 , u 2 H ,
and
η n ( u ) n , f o r a l l u H .
Given n N , we set σ n ( t , ω , u ) = σ ( t , ω , η n ( u ) ) for t R , ω Ω and u H . By (3) and (4) and (165) and (166), we infer
σ n ( t , ω , u 1 ) σ n ( t , ω , u 2 ) L 2 ( U , H ) M n u 1 u 2 ,
and
σ n ( t , ω , u ) L 2 ( U , H ) L ( 1 + u ) .
Therefore, we can apply Lemma 5 to approximate σ by globally Lipschitz continuous function σ n . Given n N , we consider the following stochastic equation:
d u n ( t ) + ( 1 + i ν ) ( Δ ) α u n ( t ) d t + ( 1 + i μ ) | u n ( t ) | 2 β u n ( t ) d t = ρ u n ( t ) d t + g ( t , x ) d t + σ n ( t , x , u n ) d W ,
with initial condition
u n ( 0 ) = u 0 .
By (167) and (168), for every F 0 -measurable u 0 L 2 ( Ω , H ) , problem (169) and (170) has a unique solution u n as given by Lemma 5. In addition, u n satisfies (132) and the energy equation
u n ( t ) 2 + 2 0 t ( Δ ) α 2 u n ( s ) 2 d s + 2 0 t R n | u n ( s ) | 2 β + 2 d x d s = u 0 2 + 2 ρ 0 t u n ( s , x ) 2 d x d s + 2 Re 0 t ( u n ( s ) , g ( s , x ) ) d s + 2 Re 0 t u n ( s ) σ n ( s , x , u n ( s ) ) d W ( s ) + 0 t σ n ( s , u n ( s ) ) L 2 ( U , H ) 2 d s ,
for all t [ 0 , T ] , P–almost surely.
Next, we establish the uniform estimates on the sequence { u n } n = 1 and prove its limit is a solution of problem (1) and (2).
We define a stopping τ n (for each n N ) by
τ n = inf { t 0 : u n ( t ) > n } T ,
where inf { t 0 : u n ( t ) > n } = + if { t 0 : u n ( t ) > n } . We write u n τ n ( t ) = u n ( t τ n ) . We will prove { u n τ n } n = 1 is consistent.
Lemma 6.
Suppose (3) and (4) hold. Let u n be the solution of (169) and (170) and τ n be the stopping time given by (172). Then, u n + 1 τ n = u n τ n and τ n + 1 = τ n a.s. for all n N .
Proof. 
Let u ^ n = u n + 1 u n . Then, we obtain
d u ^ n + ( 1 + i ν ) ( Δ ) α u ^ n d t + ( ( 1 + i μ ) | u n + 1 | 2 β u n + 1 ( 1 + i μ ) | u n | 2 β u n ) d t = ρ u ^ n d t
+ ( σ n + 1 ( t , u n + 1 ) σ n ( t , u n ) ) d W .
Similar to (151) with θ = 0 , we can obtain that for t [ 0 , T ] ,
u ^ n ( t τ n ) 2 + 2 Re 0 t τ n R n ( ( 1 + i μ ) | u n + 1 | 2 β u n + 1 ( 1 + i μ ) | u n | 2 β u n ) u ^ n ( s ) d x d s
+ 2 0 t τ n ( Δ ) α 2 u ^ n 2 d s = 2 Re 0 t τ n u ^ n ( s ) ( σ n + 1 ( s , u n + 1 ( s ) ) σ n ( s , u n ( s ) ) ) d W ( s ) +
2 ρ 0 t τ n u ^ n ( s ) 2 d s + 0 t τ n σ n + 1 ( s , u n + 1 ( s ) ) σ n ( s , u n ( s ) ) L 2 ( U , H ) 2 d s .
By the definition of η n , we infer from σ n ( s , u n ( s ) ) = σ n + 1 ( s , u n ( s ) ) for s [ 0 , τ n ] , for t [ 0 , T ] ,
u ^ n ( t τ n ) 2 = u n + 1 τ n ( t ) u n τ n ( t ) 2 2 ρ 0 t τ n u n + 1 ( s ) u n ( s ) 2 d s
+ 2 Re 0 t τ n ( u n + 1 ( s ) u n ( s ) ) ( σ n + 1 ( s , u n + 1 ( s ) ) σ n + 1 ( s , u n ( s ) ) ) d W ( s )
+ 0 t τ n σ n + 1 ( s , u n + 1 ( s ) ) σ n + 1 ( s , u n ( s ) ) L 2 ( U , H ) 2 d s .
By (167), we imply that for t [ 0 , T ] ,
E sup 0 r t u n + 1 τ n ( r ) u n τ n ( r ) 2 2 ρ 0 t E sup 0 r s u n + 1 τ n ( r ) u n τ n ( r ) 2 d s
+ 2 E sup 0 r t τ n 0 r ( u n + 1 ( s ) u n ( s ) ) ( σ n + 1 ( s , u n + 1 ( s ) ) σ n + 1 ( s , u n ( s ) ) ) d W ( s )
+ M n + 1 2 0 t E sup 0 r s u n + 1 τ n ( r ) u n τ n ( r ) 2 d s .
For the second term on the right-hand side of (175), we have
2 E sup 0 r t τ n 0 r ( u n + 1 ( s ) u n ( s ) ) ( σ n + 1 ( s , u n + 1 ( s ) ) σ n + 1 ( s , u n ( s ) ) ) d W ( s )
c 18 E 0 t τ n u n + 1 ( s ) u n ( s ) 2 σ n + 1 ( s , u n + 1 ( s ) ) σ n + 1 ( s , u n ( s ) ) L 2 ( U , H ) 2 d s 1 2
c 18 M n + 1 E sup 0 r t u n + 1 τ n ( r ) u n τ n ( r ) 0 t u n + 1 τ n ( s ) u n τ n ( s ) 2 d s 1 2
1 2 E sup 0 r t u n + 1 τ n ( r ) u n τ n ( r ) 2 + 1 2 c 18 M n + 1 2 0 t E sup 0 r s u n + 1 τ n ( r ) u n τ n ( r ) 2 d s .
It follows from (175) and (176) that for t [ 0 , T ] ,
E sup 0 r t u n + 1 τ n ( r ) u n τ n ( r ) 2
( 4 ρ + c 18 M n + 1 2 + 2 M n + 1 2 ) 0 t E sup 0 r s u n + 1 τ n ( r ) u n τ n ( r ) 2 d s .
By Gronwall inequality, we obtain, for t [ 0 , T ] ,
E sup 0 r t u n + 1 τ n ( r ) u n τ n ( r ) 2 = 0 .
Therefore, u n + 1 τ n = u n τ n . By (172), we can get that for all n N , we can infer τ n + 1 τ n . □
Since τ n + 1 τ n a.s., the stopping time τ is well-defined:
τ = lim n τ n = sup n N τ n .
Next, we prove τ = T almost everywhere.
Lemma 7.
Suppose (3) and (4) hold and u 0 L 2 ( Ω , H ) is F 0 -measurable. Let τ be the stopping time given by (177). Then, τ = T almost surely.
Proof. 
For all n N these estimates are independent of the Lipschitz coefficient M n of σ n in (167), therefore, the solution u n of (169) and (170) satisfies the estimates given by (132). In addition, by (172) we have { τ n < T } { u n C ( [ 0 , T ] , H ) n } , applying Chebyshev’s inequality and Lemma 5 yields
P { τ n < T } P { u n C ( [ 0 , T ] , H ) n } 1 n 2 E ( u n C ( [ 0 , T ] , H ) 2 ) c 19 n 2 .
By the Borel-Cantelli lemma, we have
P ( k = 1 n = k { τ n < T } ) = 0 .
As a result, there exists a subset Ω 0 of Ω with P ( Ω ) = 0 such that for each ω Ω \ Ω 0 , there exists n 0 = n 0 ( ω ) such that τ n ( ω ) = T for all n n 0 . Then, τ ( ω ) = lim n τ ( n ) = T for all ω Ω \ Ω 0 . □
Next we prove the existence and uniqueness of solution (1) and (2).
Theorem 2.
Suppose (3) and (4) hold and u 0 L 2 ( Ω , H ) is F 0 -measurable. Then, problem (1) and (2) has a unique solution u in the sense of Definition 5. Moreover, u satisfies the energy equation:
u ( t ) 2 + 2 0 t ( Δ ) α 2 u ( s ) 2 d s + 2 0 t R n | u ( s ) | 2 β + 2 d x d s
= u 0 2 + 2 ρ 0 t u ( s , x ) 2 d s + 2 R e 0 t ( u ( s ) , g ( s ) ) d s + 2 R e 0 t u ( s ) σ ( s , ω ( s ) ) d W
+ 0 t σ ( s , u ( s ) ) L 2 ( U , H ) 2 d s ,
for all t [ 0 , T ] , P–almost surely. In addition,
u ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + u ( t ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p
L 5 ( T ) ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 ) .
where L 5 ( T ) is a positive number depending only on T.
Proof. 
By Lemma 6 and Lemma 7, we know that there exists a measurable set Ω 0 of Ω such that P ( Ω 0 ) = 1 and for all ω Ω 0 ,
τ ( ω ) = T a n d u n τ m ( ω ) = u m τ m ( ω ) , n m .
we define a function u : [ 0 , T ] × Ω H by
u ( t , ω ) = u n ( t , ω ) i f ω Ω 0 a n d t [ 0 , τ n ( ω ) ] ; u 0 ( ω ) i f ω Ω \ Ω 0 a n d t [ 0 , T ] .
By above definitions, we can conclude that u is a continuous H-valued F t -adapted process and the fact:
lim n u n ( t , ω ) = u ( t , ω ) , f o r a l l t [ 0 , T ] a n d ω Ω 0 .
By Lemma 5, the solution u n satisfies (132) for all n N . By (182) and Fatou’s lemma, we conclude that there exists a positive number L 5 ( T ) depending only on T such that
u ( t ) L 2 ( Ω , C ( [ 0 , T ] , H ) ) 2 + u ( t ) L 2 ( Ω , L 2 ( [ 0 , T ] , V ) ) 2 + u ( t ) L p ( Ω , L p ( 0 , T ; L p ( R n ) ) ) p
L 5 ( T ) ( u 0 L 2 ( Ω , H ) 2 + g L 2 ( 0 , T ; H ) 2 ) ,
which gives (179). We are now prove that u satisfies (1) and (2). u n is the solution of (169) and (170), then we have, for t [ 0 , T ] ,
u n ( t τ n ) + ( 1 + i ν ) 0 t τ n ( Δ ) α u n ( s ) d s + 0 t τ n ( 1 + i μ ) | u n ( s ) | 2 β u n ( s ) d s
= u 0 + ρ 0 t τ n u n ( s ) d s + 0 t τ n g ( s ) d s + 0 t τ n σ n ( s , u n ( s ) ) d W ( s ) i n ( V L p ( R n ) ) * ,
P-almost surely. By (181), we know that u n ( t τ n ) = u ( t τ n ) for t [ 0 , T ] and σ n ( s , u n ( s ) ) = σ ( s , u ( s ) ) , for s [ 0 , τ n ] a.s., then, by (184) we obtain, for all t [ 0 , T ] ,
u ( t τ n ) + ( 1 + i ν ) 0 t τ n ( Δ ) α u ( s ) d s + 0 t τ n ( 1 + i μ ) | u ( s ) | 2 β u ( s ) d s
= u 0 + ρ 0 t τ n u ( s ) d s + 0 t τ n g ( s ) d s + 0 t τ n σ ( s , u ( s ) ) d W ( s ) i n ( V L p ( R n ) ) * ,
P–almost surely. Letting n in (185) we obtain, for all t [ 0 , T ] ,
u ( t ) + ( 1 + i ν ) 0 t ( Δ ) α u ( s ) d s + 0 t ( 1 + i μ ) | u ( s ) | 2 β u ( s ) d s = u 0 + ρ 0 t u ( s ) d s + 0 t g ( s ) d s
+ 0 t σ ( s , u ( s ) ) d W ( s ) i n ( V L p ( R n ) ) * ,
P-almost surely. We make t = t τ n with (171), letting n , we can obtain the energy equation (178). □

7. Weak Mean Random Attractors

In this section, we prove the existence and uniqueness of weak pullback mean random attractors. For ρ > 0 , we consider the following stochastic equation, for t > τ ,
d u ( t ) + ( 1 + i ν ) ( Δ ) α u ( t ) d t + ( 1 + i μ ) | u ( t ) | 2 β u ( t ) d t = ρ u ( t ) d t + g ( t , x ) d t + σ ( t , x , u ) d W ( s ) ,
with initial condition
u ( τ ) = u 0 .
By Theorem (165), we obtain that for every τ R and every F τ -measurable u 0 in L 2 ( Ω , H ) , the problem (187) and (188) has a unique continuous H-valued F t -adapted solution u ( t , τ , u 0 ) with initial condition u 0 at τ in the sense of Definition 5. Note that u ( t , τ , u 0 ) L 2 ( Ω , C ( [ τ , τ + T ] , H ) ) for all T > 0 , which implies that u C ( [ τ , ) , L 2 ( Ω , H ) ) .
Suppose that Φ is the mean random dynamical system generated by (187) and (188) on L 2 ( Ω , F ; H ) . We will investigate the existence and uniqueness of weak pullback mean random attractors for Φ .
We use D to denote the collection of all families of nonempty bounded sets satisfying (8), and assume that for all ( t , ω , u ) R × Ω × H , the function g ( t ) satisfies that
τ e λ t g ( t ) 2 d t < , τ R .
The next lemma is concerned with the uniform estimates of the solutions in L 2 ( Ω , H ) .
Lemma 8.
Suppose (189) holds. Then, for every τ R and D D , there exists T = T ( τ , D ) > 0 such that for all t T , the solution u of (187) and (188) satisfies
E ( u ( τ , τ t , u 0 ) 2 ) M 1 + M 1 τ e ρ ( s τ ) g ( s ) 2 d s ,
where u 0 D ( τ t ) , and M 1 is a positive constant independent of τ and D.
Proof. 
By the energy Equation (178), we have
d E ( u ( t ) 2 ) d t + 2 E ( Δ ) α 2 u ( t ) 2 + 2 Re E ( 1 + i μ ) | u ( t ) | 2 β u ( t ) , u ( t ) = 2 ρ E ( u ( t ) 2 )
+ 2 Re E u ( t ) , g ( t ) + E σ ( t , u ( t ) ) L 2 ( U , H ) 2 .
By (4) and Young’s inequality, we deduce
d E ( u ( t ) 2 ) d t + 2 E ( u ( t ) p ) + ρ E ( u ( t ) 2 ) ( 7 ρ 2 + 2 L 2 ) E ( u ( t ) 2 ) + 2 ρ E ( g ( t ) 2 ) + 2 L 2 .
Applying Young’s Inequality again, we have
d E ( u ( t ) 2 ) d t + ρ E ( u ( t ) 2 ) 2 ρ E ( g ( t ) 2 ) + c ( ρ ) .
Applying Gronwall’s inequality on the interval ( τ t , τ ) , we get
E ( u ( τ , τ t , u 0 ) 2 ) e ρ t E ( u 0 2 ) + c ( ρ ) ρ + 2 ρ τ t τ e ρ ( s τ ) g ( s ) 2 d s .
Due to u 0 D ( τ t ) and D D , we have
e ρ t E ( u 0 2 ) e ρ t D ( τ t ) 2 0 , a s t .
which completes the proof. □
Next, we prove the existence of weak D -pullback mean random attractors for Φ .
Theorem 3.
Suppose (189) holds, then problem (187) and (188) has a unique weak D -pullback mean random attractor as Definition 5 A = { A ( τ ) : τ R } D in L 2 ( Ω , F ; H ) over ( Ω , F , { F t } t R , P ) .
Proof. 
Given τ R , denote by
D ( τ ) = { u L 2 ( Ω , F τ ; H ) : E ( u 2 ) L ( τ ) } ,
where
L ( τ ) = M 1 + M 1 τ e ρ ( s τ ) g ( s ) 2 d s .
Since D ( τ ) is a closed ball in L 2 ( Ω , F τ ; H ) centered at the origin, we know that D ( τ ) is weakly compact in L 2 ( Ω , F τ ; H ) . On the other hand, by (190), we have
lim τ e ρ τ D ( τ ) L 2 ( Ω , F τ ; H ) 2 = M 1 lim τ e ρ τ + M 1 lim τ τ e ρ s g ( s ) 2 d s = 0 ,
and hence D = { D ( τ ) : τ R } D . By Lemma 8, we infer that D is a weakly compact D -pullback absorbing set for Φ . According to Theorem 1, we conclude that the existence and uniqueness of weak D -pullback mean random attractors for Φ . □
We emphasize that via Theorem 3, we obtain the long time behavior of the solution of (1) and (2).

8. Conclusions

In this work, we consider the long-time behavior of the stochastic Ginzburg–Landau equation driven by nonlinear noise. The existence and uniqueness of the solution of the equation in the corresponding space is established with detailed discussion in Section 3 (with regular additive noise), Section 4 (with general additive noise), Section 5 (with global Lipschitz continuity noise) and Section 6 (with local Lipschitz continuity noise). Meanwhile, the corresponding estimate of the solution in the corresponding space is obtained respectively. In our analysis for the estimate of the solution, we employ the tools of the Ito’s formula, Gronwall’s inequality, Young’s inequality and Burkholder–Davis–Gundy inequality. We point out that in Section 7, based on the theory of weak pullback attractors established in [36], we obtain the existence of weak pullback random attractors for the mean stochastic dynamical systems constructed through the Equations (1) and (2).
The detailed discussion in current work will naturally lead us to investigate the existence of invariant measures for the distribution of solutions of stochastic fractional Ginzburg–Landau equations. Furthermore, when the parameters, functions and initial values in the Equation (1) are determined and satisfy the corresponding conditions, the specific form of the solution can be studied by numerical methods (see [43] for some discussion).
To end this section, we demonstrate that the method used to study the stochastic Ginzburg–Landau equation is quite different from those employed to analyze the deterministic one. To be specific, for the deterministic equations, one obtains the estimate for solutions, the so-called a priori estimates, by first constructing the energy equation through inner products, then applying suitable inequalities to the resulting energy equations. Based on the discussion, one then can prove the existence of pullback attractor (for more detailed discussion, one may refer to [6]). For the stochastic one, one mainly employ the Ito formula to obtain the estimate of the solutions, and then prove the existence of weak pullback attractors as analyzed in current work.

Author Contributions

Conceptualization, H.L. and M.Z.; methodology, H.L.; formal analysis, L.W.; writing—original draft preparation, H.L. and L.W.; writing—review and editing, M.Z.; funding acquisition, H.L. and M.Z. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by the NSF of Shandong Province (No.ZR2021MA055), and Simons Foundation of USA (No. 628308).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Not applicable.

Acknowledgments

The authors appreciate the valuable suggestions and advice from the nonymous reviewers, which greatly improve the manuscript.

Conflicts of Interest

The authors declare no conflict of interest.

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Lu, H.; Wang, L.; Zhang, M. Dynamics of Fractional Stochastic Ginzburg–Landau Equation Driven by Nonlinear Noise. Mathematics 2022, 10, 4485. https://doi.org/10.3390/math10234485

AMA Style

Lu H, Wang L, Zhang M. Dynamics of Fractional Stochastic Ginzburg–Landau Equation Driven by Nonlinear Noise. Mathematics. 2022; 10(23):4485. https://doi.org/10.3390/math10234485

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Lu, Hong, Linlin Wang, and Mingji Zhang. 2022. "Dynamics of Fractional Stochastic Ginzburg–Landau Equation Driven by Nonlinear Noise" Mathematics 10, no. 23: 4485. https://doi.org/10.3390/math10234485

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