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Research article

Miscellaneous reverse order laws and their equivalent facts for generalized inverses of a triple matrix product

  • Reverse order laws for generalized inverses of products of matrices are a class of algebraic matrix equalities that are composed of matrices and their generalized inverses, which can be used to describe the links between products of matrix and their generalized inverses and have been widely used to deal with various computational and applied problems in matrix analysis and applications. ROLs have been proposed and studied since 1950s and have thrown up many interesting but challenging problems concerning the establishment and characterization of various algebraic equalities in the theory of generalized inverses of matrices and the setting of non-commutative algebras. The aim of this paper is to provide a family of carefully thought-out research problems regarding reverse order laws for generalized inverses of a triple matrix product ABC of appropriate sizes, including the preparation of lots of useful formulas and facts on generalized inverses of matrices, presentation of known groups of results concerning nested reverse order laws for generalized inverses of the product AB, and the derivation of several groups of equivalent facts regarding various nested reverse order laws and matrix equalities. The main results of the paper and their proofs are established by means of the matrix rank method, the matrix range method, and the block matrix method, so that they are easy to understand within the scope of traditional matrix algebra and can be taken as prototypes of various complicated reverse order laws for generalized inverses of products of multiple matrices.

    Citation: Yongge Tian. Miscellaneous reverse order laws and their equivalent facts for generalized inverses of a triple matrix product[J]. AIMS Mathematics, 2021, 6(12): 13845-13886. doi: 10.3934/math.2021803

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  • Reverse order laws for generalized inverses of products of matrices are a class of algebraic matrix equalities that are composed of matrices and their generalized inverses, which can be used to describe the links between products of matrix and their generalized inverses and have been widely used to deal with various computational and applied problems in matrix analysis and applications. ROLs have been proposed and studied since 1950s and have thrown up many interesting but challenging problems concerning the establishment and characterization of various algebraic equalities in the theory of generalized inverses of matrices and the setting of non-commutative algebras. The aim of this paper is to provide a family of carefully thought-out research problems regarding reverse order laws for generalized inverses of a triple matrix product ABC of appropriate sizes, including the preparation of lots of useful formulas and facts on generalized inverses of matrices, presentation of known groups of results concerning nested reverse order laws for generalized inverses of the product AB, and the derivation of several groups of equivalent facts regarding various nested reverse order laws and matrix equalities. The main results of the paper and their proofs are established by means of the matrix rank method, the matrix range method, and the block matrix method, so that they are easy to understand within the scope of traditional matrix algebra and can be taken as prototypes of various complicated reverse order laws for generalized inverses of products of multiple matrices.



    Fractional differential equations (FDEs) are an effective mathematical tool to model and analyze many real life problems; it has been used by researchers and scientists to get better results than the integer order differential equations. Fractional order differential equations offer a superior framework for capturing the intricate dynamics of real-world phenomena compared to their integer-order counterparts. This superiority stems from the unique ability of fractional integrals and derivatives to account for the inherent hereditary and memory characteristics present in diverse processes and materials. By harnessing these fractional operators, models can more accurately depict the nuanced behaviors observed in nature, thereby enhancing our understanding and predictive capabilities across a wide range of disciplines and applications. Many fractional derivatives, including Caputo derivative, Atangana-Baleanu derivative, Coimbra derivative, and Riemann-Liouville (R-L) derivative, are frequently used to examine FDEs and fractional order stochastic differential equations (SDEs). In a similar vein, the Hilfer fractional derivative (HFD), which was just recently used to do so, was developed by Hilfer [21], which is a generalized version of R-L and Caputo derivatives. In actuality, fractional derivative and integrals indicate greater accuracy than integral models and also depict broader physical applications in seepage, flow in porous media, nanotechnology, fluid dynamics and traffic models [6,7,12,22,24,28,31].

    SDEs are the natural extension of deterministic systems. SDEs with impulses arise from many mathematical models of physical phenomena in different scientific fields for example, technology, physics, biology, economics, etc. They are important from the viewpoint of applications since they incorporate randomness into the mathematical description of the phenomena and provide a more accurate description of it. Certainly, in various fields like economics, bioengineering, chemistry, medicine, and biology, we often encounter situations where things change suddenly at specific points in time [5,23,29,32]. These abrupt changes can be explained by what we call "impulsive effects." These impulsive effects are like sudden pushes that happen at certain moments and have a big impact on the system, being studied. These pushes play a crucial role in understanding and modeling how things change in the aforementioned diverse fields. For the mathematical models of such phenomena, finding their solution is a challenging task. As a result, Boundani et al. [8,9] presented some specific conditions that help us to determine whether certain mathematical equations, involving randomness, can have solutions. These equations involve functional differential equations and a type of random behavior, called fractional Brownian motion.

    In [20], Hernandez and O'Regan introduced non-instantaneous (NI) impulses. Many researchers have utilized these impulses and studied the corresponding dynamical systems [3,4,27,36,39]. To better understand NI impulses, we can think about human blood sugar levels. When they have too much or too little, glucose they get insulin medication through the bloodstream, in fact it doesn't work instantly but takes some time to be absorbed [37]. This gradual effect is like NI, where the impact lasts for a while in many real situations. Sudden changes don't explain things well. For instance, in the treatment of diseases with medication, we need to describe how things change over time more smoothly. That's where NI impulsive differential equations come in handy. They help us to model these gradual changes, like how drugs affect the body in pharmacotherapy.

    Among the qualitative behaviors of different physical systems, different types of stabilities are the essential ones. One of these types of stabilities is Ulam-Hyers (UH) and Ulam-Hyers-Rassias (UHR) stability [11,16,26,30,33].

    In the literature, most of the results related to fractional stochastic differential equations (FSDEs) are given over infinite dimensional spaces [1,2,13,18,19,25,32,35,38], and very few have looked at similar results in finite spaces. There is no prior work on the specific topic of non-integers order impulses in finite-dimensional equations to the problem of fractional neutral SDEs including both noises. In FSDEs incorporating both retarded and advanced arguments, a significant characteristic emerges: The rate of change of the system at the present moment is influenced not only by its past history but also by its anticipated future states. This feature underscores the intricate interplay between past, present, and future dynamics, where the system's behavior is shaped by a combination of its memory effects and anticipatory responses.

    In the current manuscript, we investigate the following ψ-Hilfer fractional stochastic equation (HFSE):

    Dγ,βψ(ε)[Γ(ε)h(ε,Γ(ε))]=AΓ(ε)+Δ(ε,Γ(ε),Dγ,βψ(ε)Γ(ε))+ε0g(s,Γ(s),Dγ,βψ(ε)Γ(ε))dB(s)+ε0λ(s,Γ(s),Dγ,βψ(ε)Γ(ε))dBH(s),ε (sk,εk+1]J:=(0,b],k=0,1,2,,m,Γ(ε)=hk(ε,Γ(ε)),ε(εk,sk],k=1,2,,m,I1v0+Γ(ε)/ε=0=Γ0,v=γ+βγβ,Γ(ε)=ϕ(ε),ε[0r,0],Γ(ε)=φ(ε),ε[b,b+h], (1.1)

    where Dγ,βψ(ε) is the ψ– Hilfer FD of order 0<γ<1 and of type 0<β1. Let J:=[0,b], b>0. The state vector ΓRn, ARn×n and nonlinear functions h : J×RnRn, Δ:J×RnRn, g:J×RnRn×n, λ:J×RnRn×n, and hk:J×RnRn are measurable and bounded functions. Also, Γ0 is F0 measurable Rn-valued stochastic variable and B is an n-dimensional Wiener process.

    Based on the value of H, the following kinds of the fractional Brownian motion (fBm) process exist:

    (1) if H=12, then the process is a Brownian motion or a Wiener process exists;

    (2) if H>12, then the increment of the process is positively correlated;

    (3) if H<12, then the increment of the process is negatively correlated.

    The contributions of this paper are described as below:

    ● Nonlinear ψ-HFSE is considered in Rn.

    ● The existence and uniqueness results are established by using the standard Banach contraction principle.

    ● The weaker sufficient conditions are derived by using the generalized Schaefer FPT for the system with measure of non-compactness (MNC).

    ● UHR stability results are derived for ψ-HFSE with NI impulse.

    ● An example is provided for the theoretical results.

    This paper is structured as follows: In Section 2, we present a number of lemmas and some fundamental definitions for fractional calculus. Section 3 derives the solution representation of ψ-Hilfer fractional SDEs with NI impulses. To demonstrate the key results, the generalized Schaefer's and contraction mapping principles are used in Section 4. In Section 5, UHR stability of a ψ-HFSE is discussed. Example is demonstrated for the validity of theoretical results in Section 6.

    Notations:

    (Ω,F,P) represents the complete probability space along a probability measure P on Ω.

    B(ε) and BH(ε) denote, respectively, the n-dimensional Brownian motion and fBm with Hurst index 12<H<1.

    {Fε|εJ} represents the filtration generated by {B(ε):0sε}.

    L2(Ω,Fε,P,Rn) : = L2(Ω,Rn) is the space of all Fε-measurable square integrable random variables with values in Rn.

    Let Jk = (εk,εk+1], k=1,2,,m be such that impulse times satisfy 0 = ε0 = s0<ε1<s1<ε2<<εmsm<εm+1 = b. Let C(J,L2(Ω,Rn)) denote Cn(J) and be the Banach space of all continuous maps from J into L2(Ω,Rn) of Fε-adapted square integrable functions Γ(ε) and for its norm supE||Γ(ε)||2<.

    Define the space

    Y=PCvn(J)=PCvn(J,L2(Ω,Rn))={Γ:JL2(Ω,Rn),Γ/JkCn(Jk,L2(Ω,Rn)),

    and there exist Γ(εk) and Γ(ε+k) with Γ(εk)=Γ(εk), k=1,,m, endowed with the norm

    ||Γ||2Y=maxk=0,1,,msupεJk{E||(εεk)(1v)Γ(ε)||}}.

    Clearly, Y is a Banach space.

    Lemma 2.1. [39] Let p2 and fLp(J,Rn×n) such that E|b0f(s)dB(s)|p<, then

    E|b0f(s)dB(s)|p(p(p1)2)p2bp22Eb0|f(s)|pds.

    Lemma 2.2. [10] Let φ:JL02 satisfy b0||φ(s)||2L02ds<, then we get

    E||ε0φ(s)dBH(s)||22Hε2H1ε0E||φ(s)||2L02ds.

    Definition 2.1. [17] The generalized ψ-Hilfer FD of order 0<γ<1 and of type 0β1 is represented by

    Dγ,βψ(t)f(t)=Iβ(nγ)ψ(t)(1ψ(t).ddt)mI1β(nγ)ψ(t)f(t).

    Definition 2.2. [10] Let z be a bounded linear operator. The two parameter Mittage-Leffler (M-L) function is defined by

    Mγ,β(z)=r=0zrΓ(rγ+β),γ,β>0,zC.

    One of the interesting properties of the M-L function, related with their Laplace integral, is given by

    0esεεβ1Mγ,β(±aεγ)dε=sγβ(sγIa).

    That is

    L{εβ1Mγ,β(±aεγ)}(s)=sγβ(sγIa).

    Lemma 2.3. [17] For γ(n1,n], β[0,1], the following Laplace formula for the ψ-Hilfer derivative is valid:

    Lψ{0Dγ,βψ(t)f(t)}=sγLψ{f(t)}m1n=0sm(1v)+γβn1(0I(1v)(mβ)nψ(t)f)(0).

    Corollary 2.1. [17] If f is a function whose classical Laplace transform is F(s), then the generalized Laplace transform of the function fψ=f(ψ(t)) is also F(s):

    L{F(s)}=F(s)L{f(ψ(ε))}=F(s).

    Example 2.1. [17]

    (a)Lψ{(ψ(ε)μ)}=Γ(μ+1)sμ+1,fors>0.(b)Lψ{ea(ψ(ε))}=1sa,fors>a.(c)Lψ{Mμ(A(ψ(ε))μ)}=sμ1sμA.(d)Lψ{(ψ(ε))μ1Mμ,μ(A(ψ(ε))μ)}=1sμA,forRe(μ)>0and |Asμ|<1.

    Example 2.2. Assume that Re(μ)>0 and |Asμ|<1. If Mγμ,v denotes the Prabhakar function, then we have

    Lψ{(ψ(ε))v1Mγμ,v(A(ψ(ε))μ)}=L{ψ(ε)v1Mγμ,v(A(ψ(ε)μ))}=sμγv(sμA)γ.

    Consider the linear deterministic system, which is represented in the following form:

    Dγ,βψ(ε)[Γ(ε)h(ε,Γ(ε))]=AΓ(ε)+Δ(ε,Γ(ε)),I1v0+Γ(ε)/ε=0=Γ0,v=γ+βγβ.

    By the Laplace transformation, we get

    sγˆΓ(s)ˆh(s)sβ(1γ)(Γ(0)h(ε,0))=AˆΓ(s)+ˆΔ(s),(sγIA)(ˆΓ(s))=sβ(1γ)(Γ(0)h(ε,0))+ˆh(s)+ˆΔ(s),ˆΓ(s)=sβ(1γ)(sγIA)[Γ(0)h(ε,0)]+1(sγIA)ˆh(s)+1(sγIA)ˆΔ(s),

    where I is the identity matrix.

    Γ(s)=Lψ1sβ(1γ)(sγIA)[Γ(0)h(ε,0)]+Lψ11(sγIA)ˆh(s)+Lψ11(sγIA)ˆΔ(s).

    Substituting the LψT of the M-L function, one can obtain that

    Γ(ε)=ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,Γ(s))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,Γ(s))ds.

    Therefore, the solution of (1.1) is given as follows:

    Γ(ε)={Γ(ε)=ϕ(ε),ε[0r,0],Γ(0),ε=0,ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,Γ(s))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,Γ(s))ds,Dγ,βψ(ε)Γ(ε)+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,Γ(η)),Dγ,βψ(ε)Γ(ε)dB(η))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,Γ(η)),Dγ,βψ(ε)Γ(ε)dBH)ds,εϵ(0,ε1],hk(ε,Γ(ε)),εϵ(εk,sk],k=1,2,3,,m,(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,Γ(s))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,Γ(s))ds,Dγ,βψ(ε)Γ(ε)+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,Γ(η)),Dγ,βψ(ε)Γ(ε)dB(η))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,Γ((η,γ(η))),Dγ,βψ(ε)Γ(ε)dBH)ds,εϵ(sk,εk+1],Γ(ε)=ϕ(ε),ε[b,b+h].

    Definition 3.1. [40] The set S is called a quasi-equicontinuous in T if, for ε > 0, there exists a δ > 0, such that if ΓS,KN,τ1,τ2TKT, and |τ2τ1|<δ, then |Γ(τ2)Γ(τ1)|<ε.

    Lemma 3.1. [34] The set SPC(J,Rn) is relatively compact if

    (i) S is uniformly bounded, i.e., ||Γ||PCk for each ΓS and some k>0;

    (ii) S is quasi-equicontinous in T.

    Definition 3.2. [14] An operator T : ZZ is said to be χ-condensing of any bounded set B of Z with χ-condensing(B) > 0, χ(T(B))<χ(B), where

    χ(B)=inf{k>0,B is covered by a finite number of sets of diameter k}

    is Kuratowskii MNC of a bounded set B of Z.

    Now, we state the generalized Schaefer's type FPT with χ-condensing operators.

    Theorem 3.1. [15] Let T : ZZ be an operator and Z be a separable Banach space satisfying

    (A1) T is χ-condensing and continuous.

    (A2) The set S = {ΓZ:Γ=δT(Γ) for some 0<δ<1} is bounded, then T has a fixed point.

    For convenience, define the following:

    M1=supξJ||Mγ,v(A(ψ(ε))γ)||2;M2=supξJ||Mγ,γ(A(bψ(ε))γ)||2.

    To derive the existence result, we imposed the following assumptions:

    (H1) The functions Δ,h,g,λ, and hk k=1,2,,m are Lipschitz continuous.

    (1) E||h(ε,u1)h(ε,u2)||2 Mh||u1u2||2Y;

    (2) E||Δ(ε,u1,v1)Δ(ε,u2,v2)||2 Mf1||u1u2||2Y+Mf2||v1v2||2Y;

    (3) E||g((ε,u1,v1))g((ε,u2,v2))||2 Mg1||u1u2||2Y+Mg2||v1v2||2Y;

    (4) E||λ(ε,u1,v1)λ(ε,u2,v2)||2 Mλ1||u1u2||2Y+Mλ2||v1v2||2Y;

    (5) E|hk(ε,u1)hk(ε,v1)||2 Mhk||u1v1||2Y,

    and hkC((εk,sk],L2(Ω,Rn)), where Mh,Mf,Mg,Mλ, and Mhk are positive constants, u1,u2,v1,v2Rn, and εTk.

    (H2) There exist lh, mh,nhY with lh=supξJlf(ε), mh=supξJmh(ε), and nh=supξJ nh(ε) such that

    E||h(ε,u1,v1)||2lh(ε)+mh(ε)||u1||2+nh(ε)||v1||2 for εT,u1,v1Rn.

    (H3) There exist lf, mf,nfY with lf=supξJlf(ε), mf=supξJmf(ε), and nf=supξJnf(ε) such that

    E||Δ(ε,u1,v1)||2lf(ε)+mf(ε)||u1||2+nf(ε)||v1||2 for εT,u1,v1Rn.

    (H4) There exist lg, mgY with lg=supξJlg(ε), mg=supξJmg(ε), and ng=supξJng(ε) such that

    E||g(ε,u1,v1)||2lg(ε)+mg(ε)||u1||2+ng(ε)||v1||2 for εT,u1,v1Rn.

    (H5) There exist lλ, mh,nhY with lλ=supξJlλ(ε), mλ=supξJmλ(ε), and nλ=supξJnλ(ε) such that

    E||λ(ε,u1,u2||2lλ(ε)+mλ(ε)||u1||2+nλ(ε)||v1||2 for εT,u1,v1Rn.

    (H6) There exist Mhk>0, for all uRn, such that

    E||hk(ε,u)||2Mhk(1+||u||2Y).

    To prove the existence and uniqueness of solution first, we need to transform the problem (1.1) into a fixed point problem and define an operator H : YY by

    HΓ(ε)={Γ(ε)=ϕ(ε),ε[0r,0],Γ(0),ε=0,ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,Γ(s))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,Γ(s))ds,Dγ,βψ(ε)Γ(s)+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,Γ(η)),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,Γ(η)),Dγ,βψ(ε)Γ(β)dBH)ds,εϵ(0,ε1],hk(ε,Γ(ε)),εϵ(εk,sk],k=1,2,3,,m,(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,Γ(s))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,Γ(s))ds,Dγ,βψ(ε)Γ(s)+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,Γ(η)),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,Γ((η,γ(η))),Dγ,βψ(ε)Γ(β)dBH)ds, εϵ(sk,εk+1],Γ(ε)=φ(ε),ε[b,b+h].

    Let x:[0r,b+h]R be a function defined by

    x(ε)={Γ(ε)=ϕ(ε),ifε[0r,0],0,ifε(0,b],Γ(ε)=φ(ε),ifε[b,b+h].

    For each zC([0,b],R) with z(0)=0, we denote by u the function defined by

    u(ε)={Γ(ε)=ϕ(ε),ifε[0r,0],z(ε),ifε(0,b],Γ(ε)=φ(ε),ifε[b,b+h].

    Let us set Γ(ε)=z(ε)+x(ε) such that yε=zε+xε for each ε(0,b], where

    Γ(ε)={Γ(0),ε=0,ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,Γs)ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,Γs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,Γη),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,Γη),Dγ,βψ(ε)ΓβdBH)ds,εϵ(0,ε1],hk(ε,Γ(ε)),εϵ(εk,sk],k=1,2,3,,m,(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,Γs)ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,Γs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,Γη),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,Γ((η,γη)),Dγ,βψ(ε)Γ(η)dBH)ds,  εϵ(sk,εk+1].
    z(ε)={Γ(0),ε=0,ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,zs+xs)ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,zs+xs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,zη+xη),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,zη+xη),Dγ,βψ(ε)Γ(η)dBH)ds,εϵ(0,ε1],hk(ε,Γ(ε)),εϵ(εk,sk],k=1,2,3,,m,(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,zs+xs)ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,zs+xs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,zη+xη),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,zη+xη),Dγ,βψ(ε)Γ(η)dBH)ds,  εϵ(sk,εk+1].

    Let Φ:YY be an operator given by

    Φz(ε)={0,ε[0r,0],Γ(0),ε=0,ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,zs+xs)ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,zs+xs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,zη+xη),Dγ,βψ(ε)Γ(s)dB(η))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,zη+xη),Dγ,βψ(ε)Γ(η)dBH)ds,εϵ(0,ε1],hk(ε,Γ(ε)),εϵ(εk,sk],k=1,2,3,,m,(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,zs+xs)ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,zs+xs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,zη+xη),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,zη+xη),Dγ,βψ(ε)Γ(η)dBH)ds,  εϵ(sk,εk+1],0,ε[b,b+h].

    To show that the operator H has a fixed point, for this it is sufficient to show that the operator Φ has a fixed point and this fixed point will correspond to a solution of problem (1.1).

    Theorem 4.1. Assume that the Hypothesis (H1) holds, then the solution (1.1) has a unique solution of the problem (1.1), provided

    L0=max{L1,Lk,Lk}<1,k=1,2,,m, (4.1)

    where

    L1=3M2ψ(ε)2γγ2[(Mh+Mf1+ψ(ε1)Mg1+2Hψ(ε1)2HMλ1)+(Mf2+ψ(ε1)Mg2+2Hψ(ε1)2HMλ2)×||A||+Mh+Mf1+ψ(ε)Mg1+2Hψ(ε1)2HMλ11(Mf2+ψ(ε)Mg2+2Hψ(ε1)2HMλ2)],Lk=Mhk,Lk=4[bv1M1Mhk+M2(b)2γγ2{(Mh+Mf1+bMg1+2Hb2HMλ1)+(Mf2+bMg2+2Hb2HMλ2)×||A||+Mh+Mf1+bMg1+2Hb2HMλ11(Mf2+bMg2+2Hb2HMλ2)}].

    Proof. Consider the operator Φ : YY defined by

    Φz(ε)={0,ε[0r,0],Γ(0),ε=0,ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,zs+xs)ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,zs+xs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,zη+xη),Dγ,βψ(ε)Γ(s)dB(η))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,zη+xη),Dγ,βψ(ε)Γ(η)dBH)ds,εϵ(0,ε1],hk(ε,Γ(ε)),εϵ(εk,sk],k=1,2,3,,m,(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,zs+xs)ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,zs+xs)ds,Dγ,βψ(ε)Γ(s)+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,zη+xη),Dγ,βψ(ε)Γ(η)dB(η))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,zη+xη),Dγ,βψ(ε)Γ(η)dBH)ds, εϵ(sk,εk+1],0,ε[b,b+h]. (4.2)

    As Δ, h, g, λ, hk are all continuous, we have to prove that Φ is a contraction.

    Case 1. For z, yY and for ε[0,ε1], we have

    E||(Φz)(ε)(Φy)(ε)||23{(M2ψ(ε)2γγ2Mh||z(ϵ)y(ε)||2+M2ψ(ε)2γγ2Mf1||z(ϵ)y(ε)||2+M2ψ(ε)2γ+1γ2Mg1||z(ϵ)y(ε)||2+M2ψ(ε)2γ+1γ22Hψ(ε)2H1Mλ1||z(ϵ)y(ε)||2)+(M2ψ(ε)2γγ2Mf2||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2+M2ψ(ε)2γ+1γ2Mg2||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2+M2ψ(ε)2γ+1γ22Hψ(ε)2H1Mλ2||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2)}.

    This implies

    ||(Φz)(ε)(Φy)(ε)||2Y3M2ψ(ε)2γγ2[(Mh+Mf1+ψ(ε1)Mg1+2Hb2HMλ1)×||z(ϵ)y(ε)||2Y+3M2ψ(ε)2γγ2(Mf2+ψ(ε1)Mg2+2Hb2HMλ2)×||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2],||(Φz)(ε)(Φy)(ε)||2Y3M2ψ(ε)2γγ2[(Mh+Mf1+ψ(ε1)Mg1+Hψ(ε1)2HMλ1)+(Mf2+ψ(ε1)Mg2+Hψ(ε1)2HMλ2)×||A||+Mh+Mf1+ψ(ε)Mg1+2Hψ(ε1)2HMλ11(Mf2+ψ(ε)Mg2+2Hψ(ε1)2HMλ2)]||z(ε)y(ε)||2.

    Thus we take

    L1=3M2ψ(ε)2γγ2[(Mh+Mf1+ψ(ε1)Mg1+Hψ(ε1)2HMλ1)+(Mf2+ψ(ε1)Mg2+Hψ(ε1)2HMλ2)×||A||+Mh+Mf1+ψ(ε)Mg1+2Hψ(ε1)2HMλ11(Mf2+ψ(ε)Mg2+2Hψ(ε1)2HMλ2)].

    So, we get

    ||(Φz)(ε)(Φy)(ε)||2YL1||z(ε)y(ε)||2Y.

    Case 2. For ε(εk,sk], k=1,2,,m, we have

    E||(Φz)(ε)(Φy)(ε)||2YE||hk(ε,z(ε))hk(ε,y(ε))||2,||(Φz)(ε)(Φy)(ε)||2YMhk||z(ε)y(ε)||2Y.

    Take Lk:=Mhk and therefore,

    ||(Φz)(ε)(Φy)(ε)||2YLk||z(ε)y(ε)||2Y.

    Case 3. For z,yY and for ε(sk,εk+1], we have

    E||(Φz)(ε)(Φy)(ε)||24{(ψ(ε)sk)v1M1Mhk||z(ε)y(ε)||2+(M2(ψ(ε)sk)2γγ2Mh||z(ϵ)y(ε)||2+M2(ψ(ε)sk)2γγ2Mf1||z(ϵ)y(ε)||2+M2(ψ(ε)sk)2γγ2Mg1||z(ϵ)y(ε)||2+M2(ψ(ε)sk)2γγ22Hψ(ε)2H1Mλ1||z(ϵ)y(ε)||2)+(M2(ψ(ε)sk)2γγ2Mf2||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2+M2(ψ(ε)sk)2γγ2Mg2||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2+M2(ψ(ε)sk)2γγ22Hψ(ε)2H1Mλ2||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2)}.||(Φz)(ε)(Φy)(ε)||24{(ψ(ε)k+1sk)v1M1Mhk+(M2(ψ(ε)sk)2γγ2×[Mh+Mf1+(ψ(εk+1)sk)Mg1+2Hψ(ε)2HMλ1]×||z(ε)y(ε)||2)+(M2(ψ(ε)sk)2γγ2×[Mf2+(ψ(εk+1)sk)Mg2+2Hψ(ε)2HMλ2]×||Dγ,βψ(ε)z(s)Dγ,βψ(ε)y(s)||2)}.

    Thus,

    ||(Φz)(ε)(Φy)(ε)||24{bv1M1Mhk+M2(b)2γγ2{Mh+Mf1+bMg1+2Hb2HMλ1+(Mf2+bMg2+2Hb2HMλ2)}×||A||+Mh+Mf1+bMg1+2Hb2HMλ11(Mf2+bMg2+2Hb2HMλ2)}||z(ε)y(ε)||2:=Lk||z(ε)y(ε)||2Y.

    From the above three cases, we obtain that ||(Φz)(ε)(Φy)(ε)||2 L0||z(ε)y(ε)||2Y as per (4.1), Φ is contraction, and, thus, (1.1) has a unique fixed point z, which is a solution to problem (1.1).

    Remark 4.1. Banach contraction principle provides not only the existence results, but also uniqueness is assured. Also, the nonlinear functions could satisfy only Lipschitz conditions to prove existence and uniqueness results, even though conditions are stronger.

    Remark 4.2. It is to be noted that the assumption L0<1 in Theorem 4.1 shows a restrictive smallness on Lipschitz constants for the nonlinear functions h, g, Δ, and λ when compared with the periods of time, while the impulses are active or vice-versa. In order to relax such a kind of smallness, the generalized Schaefer's FPT is introduced.

    Theorem 4.2. Assume that (H2)(H5) hold, then the nonlinear operator Φ:YY has a fixed point, which is a solution of problem (1.1)

    Proof. Since Φ is well defined, we will present the proof by the following four steps.

    First, we prove that Φ is completely continuous (CC), that is, T is continuous, maps bounded sets into bounded sets, and maps bounded sets into quasi-equicontinuous sets.

    Step 1. To prove Φ is continuous.

    Since h, g, Δ,λ, and hK are all continuous, then it is clear that the operator Φ is continuous on J.

    Step 2. To prove Φ maps bounded sets in Y.

    In fact, it is sufficient to show that for any r>0, there exists an η>0 such that for each zBr={zY:||z||2Yz}.

    Case 1. For ε[0,ε1],zY

    ||(Φz)(ε)||2Y4{ψ(ε1)ν1M1||Γ0h(ε,0)||2Y+M2ψ(ε1)2γγ2||h(ε,zs+xs),Dγ,βψ(ε)Γ(s)||+M2ψ(ε1)2γγ2||Δ(ε,zs+xs,Dγ,βψ(ε)Γ(s))||+M2ψ(ε1)2γ+1γ2||g(ε,zη+xη,Dγ,βψ(ε)Γ(s))||+2Hψ(ε)2H1M2ψ(ε1)2γ+1γ2||λ(ε,zη+xη,Dγ,βψ(ε)Γ(s))||}.

    Using (H2)(H4) and Lemmas 2.1 and 2.2, one can enumerate

    ||(Φz)(ε)||2Y4{M1||Γ0h(ε,0)||2Y+M2ψ(ε1)2γγ2(lh(ε)+mh(ε)||zs+xs||2Y)+M2ψ(ε1)2γγ2(lf(ε)+mf(ε)||zs+xs||2Y+nf(ε)||Dγ,βψ(ε)Γ(s)||2Y)+M2ψ(ε1)2γ+1γ2(lg(ε)+mg(ε)||zηxη||2Y+ng||Dγ,βψ(ε)Γ(s)||2)+2Hψ(ε)2H1M2ψ(ε1)2γ+1γ2(lλ(ε)+mλ(ε)||zη+xη||2Y+||Dγ,βψ(ε)Γ(s)||2)}4{M1||Γ0h(ε,0)||2Y+M2ψ(ε1)2γγ2(lh)+M2ψ(ε1)2γγ2(lf)+M2ψ(ε1)2γ+1γ2(lg)+M22Hψ(ε1)2Hγ2(lλ)}+4{M2ψ(ε1)2γγ2(mh)+M2ψ(ε1)2γγ2(mf)+M2ψ(ε1)2γ+1γ2(mg)+M22Hψ(ε1)2Hγ2(mλ)}||z||+4{M2ψ(ε1)2γγ2nf+M2ψ(ε1)2γ+1γ2ng+M2ψ(ε1)2γ+1γ2nλ}||Dγ,βψ(ε)Γ(s)||24{M1||Γ0h(ε,0)||2+M2ψ(ε1)2γγ2(lh+lf+ψ(ε)lg+2Hψ(ε)2Hlλ)}+4{M1||Γ0h(ε,0)||2+M2ψ(ε1)2γγ2(mh+mf+ψ(ε)mg+2Hψ(ε)2Hmλ)+(lh+lf+ψ(ε)lg+ψ(ε)lλ+(mh+mf+ψ(ε)mg+ψ(ε)mλ)1(nf+ψ(ε)ng+ψ(ε)mλ)}z:=η0.

    Case 2. For ε(εk,sk], k = 1, 2, , m,

    ||(Φz)(ε)||2E||hk(ε,zs+xs)||2Mhk(1+||z||2)ψ(ε)1vMhk(1+||z||2)maxψ(ε)1vMhk(1+z):=ηk,   k=1,2,3,m.

    Case 3. For ε(sk,εk+1], k=1,2,,m, ΓY, we have

    E||(Φz)(ε)||24{E||(ψ(ε)k+1sk)v1Mγ,v(A(sk)γ)hk(sk,Γ(sk))||2+E||ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,zs+xs)ds||2+E||ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,zs+xs,Dγ,βψ(ε)Γ(s))ds||2+E||ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,zη+xη,Dγ,βψ(ε)Γ(s))dB(η))ds||2+E||ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ((η,zη+xη,Dγ,βψ(ε)Γ(s))dBH)ds||2}.

    Thus

    E||(ΦΓ)(ε)||24{(ψ(ε)v1M1Mhk(1+||Γ(sk)||2Y))+M2(ψ(ε)k+1sk)2γγ2[lh+lf+(ψ(ε)k+1sk)lg+2H(ψ(ε)k+1sk)2Hlλ]}+4{(ψ(ε)v1M1Mhk(1+||Γ(sk)||2Y))+M2(ψ(ε)k+1sk)2γγ2[mh+mf+(ψ(ε)k+1sk)mg+2H(ψ(ε)k+1sk)2Hlλ]}+4{M2ψ(ε1)2γγ2nf+M2ψ(ε1)2γ+1γ2ng+M2ψ(ε1)2γ+1γ2nλ}||Dγ,βψ(ε)Γ(s)||24{bv1M1Mhk+M2b2γγ2[lh+lf+blg+2Hb2Hlλ]}+4{bv1M1Mhk+M2b2γγ2[mh+mf+bmg+2Hb2Hmλ]+[lh+lf+blg+blλ+(mh+mf+bmg+bmλ)14(nf)+bng+bmλ]}z:=ηb.

    Let η = {η0,ηk,ηb}, k=1,2,,m, then {ψ1v(Φz)(ε):zB} is a bounded set in Y, i.e., ||Φz||2Y η.

    Step 3. Φ is a quasi-equicontinous set in Y.

    Case 1. Let τ1, τ2 [0,ε1] with 0τ1τ2ε1. One could establish the following estimate:

    ||(Φz)(τ2)(Φz)(τ1)||2=sup{E||τ1v2(ΦΓ)(τ2)τ1v1(ΦΓ)(τ1)||2}8{E||Mγ,v(Aτγ2)||Γ0h(ε,0)||Mγ,v(Aτγ1)||Γ0h(ε,0)||||2+τ2τ20||τ1v2(τ2s)γ1Mγ,γ(A(τ2s)γ)τ1v1(τ1s)γ1Mγ,γ(A(τ1s)γ)||2(lh+mhE||zs+xs||2+nh||Dγ,βψ(ε)Γ(s)||2)ds+(τ2τ1)τ20τ2(1v)2(τ2s)2γ2||Mγ,γ(A(τ2s)γ)||2(lh+mhE||zs+xs||2+nh||Dγ,βψ(ε)Γ(s)||2)ds+τ2τ20||τ1v2(τ2s)γ1Mγ,γ(A(τ2s)γ)τ1v1(τ1s)γ1Mγ,γ(A(τ1s)γ)||2(lf+mfE||zs+xs||2+nf||Dγ,βψ(ε)Γ(s)||2)ds+(τ2τ1)τ20τ2(1v)2(τ2s)2γ2||Mγ,γ(A(τ2s)γ)||2(lf+mfE||zs+xs||2+nf||Dγ,βψ(ε)Γ(s)||2)ds+τ2τ20||τ1v2(τ2s)γ1Mγ,γ(A(τ2s)γ)τ1v1(τ1s)γ1Mγ,γ(A(τ1s)γ)||2(lg+mgE||zη+xη||2+ng||Dγ,βψ(ε)Γ(s)||2)ds+(τ2τ1)τ20τ2(1v)2(τ2s)2γ2||Mγ,γ(A(τ2s)γ)||2(lg+mgE||zs+xs||2+ng||Dγ,βψ(ε)Γ(s)||2)ds+2Hτ2H12τ20||τ1v2(τ2s)γ1Mγ,γ(A(τ2s)γ)τ1v1(τ1s)γ1Mγ,γ(A(τ1s)γ)||2(lλ+mλE||zs+xs||2+nλ||Dγ,βψ(ε)Γ(s)||2)ds+2H(τ2τ1)2H1τ20τ2(1v)2(τ2s)2γ2||Mγ,γ(A(τ2s)γ)||2×(lλ+mλE||zs+xs||2+nλ||Dγ,βψ(ε)Γ(s)||2)ds}.

    We conclude that as τ2τ10 with ε sufficiently small, the right hand side of the above inequality tends to zero independently of zBr. Furthermore, the similar results are true for εk<τ1<τ2sk and sk<τ1<τ2εk+1 for k=1,2,,m. It proves the equicontinuous of Φ on Y. Thus, for τ1,τ2[0,b](εk,εk+1], k=1,2,,m, whenever B is a bounded set of Y as in Step 2, let zBr, then

    ||(Φz)(τ1)(Φy)(τ2)||2YM(r)(τ2τ1).

    Thus, Φ is quasi-equicontinuous, then Φ(z) is relatively compact by Lemma 3.1, which implies that Φ(z) is CC.

    Step 4. Φ has a Prior bound.

    It remains to estimate that the set (Φ)={zY:z=ΘΦz,0<Θ<1} is bounded.

    Let zΠ(Φ), then z=ΘΦ(z) for some Θ(0,1), by following the proof of Step 2 that ||z||Yη. This proves that the set Π(Φ) is bounded. Hence, by Theorem 3.1, Φ has a fixed point, which is the required solution on J.

    Here, we derive the UHR stability for (1.1). Let ω>0, ϕ0, and ζPC(J,Rn) be nondecreasing. Consider the following inequalities.

    E||Dγ,βψ(ε)[˜Γ(ε)h(ε,˜Γ(ε))]A˜Γ(ε)Δ(ε,˜Γ(ε),Dγ,βψ(ε)Γ(s))ε0g(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dB(s)ε0λ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dBH(s)||ωζ(ε),ε (sk,εk+1],k=0,1,2,,m,E||Γ(ε)hk(ε,Γ(ε))||2ωϕ,ε(εk,sk],k=1,2,,m,E||I1v0+Γ(ε)Γ0||2ωϕ,Γ(ε)=ϕ(ε),ε[0r,0],Γ(ε)=φ(ε),ε[b,b+h].

    Define a vector space as χ:

    χ=PC(J,Rn)C((sk,tk+1],Rn).

    Definition 5.1. System (1.1) is UHR stable with respect to (ζ,ϕ) if there exists C(M,L,P,ζ)>0 such that for each solution ˜Γχ of the inequality (5.1), there exists solution ΓPC(J,Rn) of (1.1) with

    E||˜Γ(ε)Γ(ε)||2C(M,L,p,ζ)ω(ζ(ε)+ϕ),εJ.

    Remark 5.1. A function ˜Γχ is a solution of (5.1) there is QKi=0 ((sk,εk+1],Rn] and qKi=0((εk,sk],Rn) such that:

    (1) E||Q(ε)||2ωζ(ε),εKi=0(sk,εk+1];E||q(ε)||2ωϕ,εKi=0(tk,sk];

    (2) Dγ,βψ(ε)[˜Γ(ε)h(ε,˜Γ(ε))]=A˜Γ(ε)+Δ(ε,˜Γ(ε),Dγ,βψ(ε)˜Γ(s)))+ε0g(s,˜Γ(s),Dγ,βψ(ε)˜Γ(s)))dB(s) +ε0λ(s,˜Γ(s),Dγ,βψ(ε)˜Γ(s)))dBH(s)+Q(ε),ε (sk,εk+1],k=0,1,2,,m,

    (3) ˜Γ(ε)=hk(ε,˜Γ(ε))+q(ε),ε(εk,sk],k=0,1,2,,m.

    By Remark 5.1, we have

    Dγ,βψ(ε)[˜˜Γ(ε)h(ε,˜Γ(ε))]=A˜Γ(ε)+Δ(ε,˜Γ(ε),Dγ,βψ(ε)˜Γ(s)))+ε0g(s,˜Γ(s),Dγ,βψ(ε)˜Γ(s)))dB(s)+ε0λ(s,˜Γ(s),Dγ,βψ(ε)˜Γ(s)))dBH(s)+Q(ε),ε (sk,εk+1],k=0,1,2,,m,˜Γ(ε)=hk(ε,˜Γ(ε))+q(ε),ε(εk,sk],k=0,1,2,,m,I1v0+˜Γ(ε)/ε=0=Γ0.

    Lemma 5.1. Let β[0,1], γ(0,1). If a function ˜Γχ is a solution of (5.1) then we have:

    (i)E||˜Γ(ε)ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds||2ψ2γ(ε)γ2M2ωε0ζ(s)ds,ε[0,ε1].
    (ii)E||(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,˜Γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds||2b2γγ2M2ωεskζ(s)ds, ε(sk,εk+1],k=1,2,,m.

    By Remark 5.1, we have:

    Case 1. For ε[0,ε1], we have

    Dγ,βψ(ε)[˜Γ(ε)h(ε,˜Γ(ε))]=A˜Γ(ε)+Δ(ε,˜Γ(ε),Dγ,βψ(ε)Γ(s))+ε0g(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dB(s)+ε0λ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dBH(s)+Q(ε).

    Thus

    ˜Γ(ε)=ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s),Dγ,βψ(ε)Γ(s))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds+ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Q(s)ds.

    From above, we obtain

    E||˜Γ(ε)ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds||2E||ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Q(s)ds||2ψ2γ(ε)γ2M2ωε0ζ(s)ds.

    Case 2. For ε(εk,sk], we have

    E||˜Γ(ε)hk(ε,˜Γ(ε))||2ωϕ.

    Case 3. For ε(sk,εk+1], we get

    Dγ,βψ(ε)[˜Γ(ε)h(ε,˜Γ(ε))]=A˜Γ(ε)+Δ(ε,˜Γ(ε),Dγ,βψ(ε)Γ(s))+ε0g(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dB(s)+ε0λ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dBH(s)+Q(ε),then,˜Γ(ε)=(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,γ(sk))+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s),Dγ,βψ(ε)Γ(s))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))ds+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds,+ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Q(s)ds.

    Thus

    E||˜Γ(ε)(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,˜Γ(sk))ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ((η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds||2E||ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Q(s)ds||2(ψ(ε)sk)2γγ2M2ωε0ζ(s)dsb2γγ2M2εε0ζ(s)ds.

    In order to prove stability, we assume the following assumptions:

    (H7) There exist positive constants Mk(k=1,2,,m) such that

    E||hk(ε,Γ(ε))hk(ε,z(ε))||2mk=1MkE||Γ(ε)z(ε)||2Yε(εk,sk].

    (H8) Let ζC(J,Rn) be a nondecreasing function if there exists cζ>0 such that ε0ζ(s)ds<cζζ(ε), εJ.

    Lemma 5.2. Let P0=P0 where p=1,2,,m, and the following inequality holds

    Γ(ε)a(ε)+ε0b(s)Γ(s)ds+Σ0<εk<εαkΓ(εˉk),ε0,

    where Γ,a,bPC(R+,R+), a is nondecreasing and b(ε)>0, αk>0, kP. For εR+,

    Γ(ε)a(ε)(1+α)Ke(ε0b(s)ds),ε(εK,εK+1],KP0,

    where α=supKP{αK} and ε0=0.

    Theorem 5.1. If the assumptions (H1),(H7), and (H8) are satisfied, then (1.1) is UHR stable with respect to (ζ,ϕ).

    Proof. Let ˜Γχ be a solution of inequality (5.1) and Γ be the unique solution of (1.1).

    Case 1. For ε[0,ε1], we have:

    E||˜Γ(ε)ψ(ε)v1Mγ,v(A(ψ(ε)γ)[Γ0h(ε,0)]ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))dsψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds||2=E||ψ(ε)0(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Q(s)ds||2ψ2γ(ε)γ2M2εε0ψ(s)dsψ2γ(ε)γ2M2ωcζζ(ε)b2γγ2M2ωcζζ(ε)cpcζζ(ε),

    where cp=b2γγ2M2.

    Case 2. For ε(εk,sk], we have

    E||˜Γ(ε)hk(ε,˜Γ(ε))||2ωϕ.

    Case 3. For ε(sk,εk+1], we have

    E||˜Γ(ε)(ψ(ε)sk)v1Mγ,v(A(sk)γ)hk(sk,Γ(sk))ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)h(s,˜Γ(s))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Δ(s,˜Γ(s),Dγ,βψ(ε)Γ(s))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0g(η,˜Γ(η),Dγ,βψ(ε)Γ(s))dB(η))dsψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)(s0λ((η,˜Γ(η),Dγ,βψ(ε)Γ(s))dBH)ds||2=E||ψ(ε)sk(ψ(ε)s)γ1Mγ,γ(A(ψ(ε)s)γ)Q(s)ds||2(ψ(ε)sk)2γγ2M2ωε0ζ(s)dsb2γγ2M2ωcζζ(ε)cpcζζ(ε).

    Hence, for ε[0,ε1], we have:

    E||Γ(ε)˜Γ(ε)||2ψ(ε)2γγ2M2[ωcζζ(ε)+((Mh+Mf1+ψ(ε1)Mg1+Hψ(ε1)2HMλ1)+(Mf2+ψ(ε1)Mg2+2Hψ(ε1)2HMλ2)×||A||+Mh+Mf1+ψ(ε)Mg1+2Hψ(ε1)2HMλ11(Mf2+ψ(ε)Mg2+2Hψ(ε1)2HMλ2))||Γ(s)˜Γ(s)||2]b2γγ2M2[ωcζζ(ε)+((Mh+Mf1+bMg1+Hb2HMλ1)+(Mf2+bMg2+Hb2HMλ2)×||A||+Mh+Mf1+bMg1+Hb2HMλ11(Mf2+bMg2+2Hb2HMλ2))||Γ(s)˜Γ(s)||2]. (5.1)

    For ε(εk,sk], we get

    E||Γ(ε)˜Γ(ε)||2=E||Γ(ε)hk(sk,˜Γ(sk))||2=E||Γ(ε)hk(sk,Γ(sk))+hk(sk,Γ(sk))hk(sk,˜Γ(sk))||22{E||Γ(ε)hk(sk,Γ(sk))||2+E||hk(sk,Γ(sk))hk(sk,˜Γ(sk))||2}2{ωϕ+Σki=0Mk||Γ(ε)˜Γ(ε)||2}. (5.2)

    For ε(sk,εk+1], k = 1, 2, , m,

    E||Γ(ε)˜Γ(ε)||25b2γγ2M2[ωcζζ(ε)+((Mh+Mf1+bMg1+Hb2HMλ1)+(Mf2+bMg2+Hb2HMλ2)×||A||+Mh+Mf1+bMg1+Hb2HMλ11(Mf2+bMg2+Hb2HMλ2))||Γ(s)˜Γ(s)||2].+5bv1M1Σki=1Mk||Γ(s)~Γ(s)||2. (5.3)

    Combining (5.2)–(5.4), one can get an inequality of the form given in Lemma 5.2. For εJ, since ε(εk,εk+1], KP0, we have

    E||Γ(ε)˜Γ(ε)||25{cpωcζζ(ε)+bv1M1Σki=1Mk||Γ(ε)˜Γ(ε)||2+cp[(Mh+Mf1+bMg1+Hb2HMλ1)+(Mf2+bMg2+Hb2HMλ2)×||A||+Mh+Mf1+bMg1+Hb2HMλ11(Mf2+bMg2+Hb2HMλ2)]||Γ(s)˜Γ(s)||2+5bv1M1Σki=1Mk||Γ(s)~Γ(s)||2}+2ωϕ5cpωcζ(ζ(ε)+ϕ)(1+M)keε0Lds,

    where

    M=sup{bv1M1Mk},L=cp[(Mh+Mf1+bMg1+Hb2HMλ1)+(Mf2+bMg2+Hb2HMλ2)×||A||+Mh+Mf1+bMg1+Hb2HMλ11(Mf2+bMg2+Hb2HMλ2)].

    Thus,

    E||Γ(ε)˜Γ(ε)||25C(M,L,p,ζ)ω(ζ(ε)+ϕ),εJ,

    where C(M,L,p,ζ) is a constant depending on M,L,p,ζ. Hence, (1.1) is UHR stable w.r.t (ζ,ϕ).

    Consider the following nonlinear ψ-HFSE with NI impulses driven by both noises. This type of fractional SDE can be applied in pharmacotherapy.

    D12,34ψ(ε)Γ1(ε)=Γ2(ε)+15(Γ1(ε)1+Γ21(ε)+Γ22(ε))+15(Γ1(ε)1+Γ21(ε)+Γ22(ε),Dγ,βψ(ε)Γ(s))
    +Γ1(ε)eψ(ε)3β1(ε),Dγ,βψ(ε)Γ(s)+Γ1(ε)e2ψ(ε)5βH1(ε),Dγ,βψ(ε)Γ(s),
    D12,34ψ(ε)Γ2(ε)=Γ1(ε)+15(Γ2(ε)1+Γ21(ε)+Γ22(ε))+15(Γ2(ε)1+Γ21(ε)+Γ22(ε),Dγ,βψ(ε)Γ(s))
    +Γ2(ε)eψ(ε)3β2(ε),Dγ,βψ(ε)Γ(s)+Γ2(ε)e2ψ(ε)3βH2(ε),Dγ,βψ(ε)Γ(s),
    ε(sk,εk+1],k=0,1,,m,
    Γ(ε)=14Γ(ε,εk),ε(0.9,sk),k=1,2,,m,
    Γ(0)=Γ0,ψ(ε)=sin(ε),

    where ΓR2, Γ12, β=34, 0<ε0<s0<ε1<<sm=1 are prefixed numbers, J=[0,1]. Here

    A=(0110),Δ(ε,Γ(ε))=(Γ1(ε)5(1+Γ21(ε)+Γ22(ε))00Γ2(ε)5(1+Γ21(ε)+Γ22(ε))),
    h(ε,Γ(ε))=(Γ1(ε)5(1+Γ21(ε)+Γ22(ε))00Γ2(ε)5(1+Γ21(ε)+Γ22(ε))),
    g(ε,Γ(ε))=(Γ1(ε)eψ(ε)300Γ2(ε)eψ(ε)3),λ(ε,Γ(ε))=(Γ1(ε)e2ψ(ε)500εΓ2(ε)eψ(ε)5).

    Calculate the M-L function by using [12]. We have

    Mγ,ν(Aψ(ε)γ)=(S1S2S3S4),

    where

    S1=S4=j=0(1)jb2jγΓ(1+2jγ)=0.3377,
    S2=S3=j=0(1)jb(2j+1)γΓ(1+(2j+1)γ)=1.666.

    Also calculate

    Mγ,ν(A(bs)γ)=(P1P2P3P4),

    where

    P1=P4=j=0(1)j(bs)2jγΓ(2jγ+γ)=0.7477,
    P2=P3=j=0(1)j(bs)(2j+1)γΓ[(2j+1)γ]=0.4203.

    Therefore, we need to check the hypotheses of nonlinear functions:

    E||h(ε,u1)h(ε,u2)||2130||u1u2||2,
    E||Δ(ε,u1,v1)Δ(ε,u2,v2)||2125||u1u2||2+135||v1v2||2,
    E||g(ε,u1,v1)g(ε,u2,v2)||219e2||u1u2||2+110e3||v1v2||2,
    E||λ(ε,u1,v1λ(ε,u2,v2)||2125e4ψ(ε)||u1u2||2+120e5ψ(ε)||v1v2||2,
    E||hk(ε,u)hk(ε,v||2116||uv||2,k=1,2,,m.

    We get M1=0.0862, M2=0.3824, Mhk=0.065, and γ=0.5. Hence we have L=max{L0,Lk,Lk}=0.52<1. Also,

    E||Γ(ε)˜Γ(ε)||25C(M,L,p,ζ)ε(ζ(ε)+ϕ),εJ,0.218.

    In this example, all the conditions stated in Theorems 4.1 and 5.1 are satisfied, so the example has a unique solution and is also UHR stable.

    With the help of Schaefer's FPT and the Banach contraction principles, we obtained the existence and uniqueness results for HSFEs with retarded and advanced arguments, selected the non-instantaneous impulses with both multiplicative and fractional noises, and obtained the UHR stability for HSFEs. UHR stability gives bounds between the exact and approximation solution, which is why this theory is very important in the numerical analysis as well as in approximation theory. We are hoping that our findings will have a great importance in the mentioned theories. Finally, a case study is provided to demonstrate the efficacy of the suggested outcomes. In the future, we can use the findings to investigate the controllability of HSFEs.

    The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.

    This work was supported by Anhui Province Natural Science Research Foundation (2023AH051810).

    The authors declare no conflicts of interest.



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