Processing math: 100%
Research article

Solitonic effect on relativistic string cloud spacetime attached with strange quark matter

  • Received: 28 February 2024 Revised: 29 March 2024 Accepted: 02 April 2024 Published: 22 April 2024
  • MSC : 53B30, 53C44, 53C50, 53C80

  • In this research paper, we discussed some geometric axioms of a relativistic string cloud spacetime attached with strange quark matter. We determined the conformal η-Ricci soliton on a relativistic string cloud spacetime attached with strange quark matter with a φ(Ric)-vector field. In addition, we illustrated some physical significance of conformal pressure P in terms of conformal η-Ricci soliton with the same vector field. Besides this, we deduced a generalized Liouville equation from the conformal η-Ricci soliton. Furthermore, we examine the harmonic relevance of conformal η-Ricci soliton on string cloud spacetime attached with strange quark matter with a potential function ψ. Finally, we turned up a necessary and sufficient condition for the 1-form η, which is the g-dual of the vector field γ on a string cloud spacetime attached with strange quark matter to be a solution for the Schrödinger-Ricci equation.

    Citation: Yanlin Li, Mohd Danish Siddiqi, Meraj Ali Khan, Ibrahim Al-Dayel, Maged Zakaria Youssef. Solitonic effect on relativistic string cloud spacetime attached with strange quark matter[J]. AIMS Mathematics, 2024, 9(6): 14487-14503. doi: 10.3934/math.2024704

    Related Papers:

    [1] Fahad Alsharari, Ahmed O. M. Abubaker, Islam M. Taha . On r-fuzzy soft γ-open sets and fuzzy soft γ-continuous functions with some applications. AIMS Mathematics, 2025, 10(3): 5285-5306. doi: 10.3934/math.2025244
    [2] Jinguo Zhang, Dengyun Yang, Yadong Wu . Existence results for a Kirchhoff-type equation involving fractional p(x)-Laplacian. AIMS Mathematics, 2021, 6(8): 8390-8403. doi: 10.3934/math.2021486
    [3] Cenap Ozel, M. A. Al Shumrani, Aynur Keskin Kaymakci, Choonkil Park, Dong Yun Shin . On δb-open continuous functions. AIMS Mathematics, 2021, 6(3): 2947-2955. doi: 10.3934/math.2021178
    [4] Ibtesam Alshammari, Islam M. Taha . On fuzzy soft β-continuity and β-irresoluteness: some new results. AIMS Mathematics, 2024, 9(5): 11304-11319. doi: 10.3934/math.2024554
    [5] Sang-Eon Han . Semi-topological properties of the Marcus-Wyse topological spaces. AIMS Mathematics, 2022, 7(7): 12742-12759. doi: 10.3934/math.2022705
    [6] Samirah Alzahrani, A. A. Nasef, N. Youns, A. I. EL-Maghrabi, M. S. Badr . Soft topological approaches via soft γ-open sets. AIMS Mathematics, 2022, 7(7): 12144-12153. doi: 10.3934/math.2022675
    [7] Nicky K. Tumalun, Philotheus E. A. Tuerah, Marvel G. Maukar, Anetha L. F. Tilaar, Patricia V. J. Runtu . An application of generalized Morrey spaces to unique continuation property of the quasilinear elliptic equations. AIMS Mathematics, 2023, 8(11): 26007-26020. doi: 10.3934/math.20231325
    [8] Dina Abuzaid, Samer Al-Ghour . Supra soft Omega-open sets and supra soft Omega-regularity. AIMS Mathematics, 2025, 10(3): 6636-6651. doi: 10.3934/math.2025303
    [9] Syafrizal Sy, Rinovia Simanjuntak, Tamaro Nadeak, Kiki Ariyanti Sugeng, Tulus Tulus . Distance antimagic labeling of circulant graphs. AIMS Mathematics, 2024, 9(8): 21177-21188. doi: 10.3934/math.20241028
    [10] Mesfer H. Alqahtani, Alaa M. Abd El-latif . Separation axioms via novel operators in the frame of topological spaces and applications. AIMS Mathematics, 2024, 9(6): 14213-14227. doi: 10.3934/math.2024690
  • In this research paper, we discussed some geometric axioms of a relativistic string cloud spacetime attached with strange quark matter. We determined the conformal η-Ricci soliton on a relativistic string cloud spacetime attached with strange quark matter with a φ(Ric)-vector field. In addition, we illustrated some physical significance of conformal pressure P in terms of conformal η-Ricci soliton with the same vector field. Besides this, we deduced a generalized Liouville equation from the conformal η-Ricci soliton. Furthermore, we examine the harmonic relevance of conformal η-Ricci soliton on string cloud spacetime attached with strange quark matter with a potential function ψ. Finally, we turned up a necessary and sufficient condition for the 1-form η, which is the g-dual of the vector field γ on a string cloud spacetime attached with strange quark matter to be a solution for the Schrödinger-Ricci equation.



    Since shunting inhibitory cellular neural networks were proposed by Bouzerdoum and Pinter [1] as a new type of neural networks, they have received more and more attention and have been widely applied in optimisation, psychophysics, speech and other fields. At the same time, since time delays are ubiquitous, many research results have been obtained on the dynamics of shunting inhibitory cellular neural networks with time delays [2,3,4,5,6].

    On the one hand, the quaternion is a generalization of real and complex numbers [7]. The skew field of quaternions is defined by

    H:={q=qR+iqI+jqJ+kqK},

    where qR,qI,qJ,qKR and the elements i,j and k obey the Hamilton's multiplication rules:

    ij=jk=k,jk=kj=i,ki=ik=j,i2=j2=k2=1.

    For q=qR+iqI+jqJ+kqK, we denote ˇq=iqI+jqJ+kqK and qR=qˇq. The norm of q is defined by qH=(qR)2+(qI)2+(qJ)2+(qK)2. For y=(y1,y2,,yn)THn, we define yHn=max1pn{yH}, then (Hn,Hn) is a Banach space. As we all know, quaternion-valued neural networks include real-valued neural networks and complex-valued neural networks as their special cases. Compared with complex-valued neural networks, quaternion-valued neural networks only needs half of the connection weight parameters of complex-valued neural networks when dealing with multi-level information [8]. In recent years, quaternion-valued neural networks have attracted the attention of many researchers, and their various dynamic behaviors, including fractional-order and stochastic quaternion-valued neural networks, have been extensively studied [9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24].

    On the other hand, because periodic and almost periodic oscillations are important dynamics of neural networks, the periodic and almost periodic oscillations of neural networks have been studied a lot in the past few decades [25,26,27,28,29,30,31,32,33]. Weyl almost periodicity is a generalization of Bohr almost periodicity and Stepanov almost periodicity [34,35,36,37]. It is a more complex recurrent oscillation. Because the spaces composed of Bohr almost periodic functions and Stepanov almost periodic functions are Banach spaces, it brings some convenience to study the existence of almost periodic solutions in these two senses of differential equations. Therefore, many results have been obtained on the Bohr almost periodic oscillation and Stepanov almost periodic oscillation of neural networks. However, the space composed of Weyl almost periodic functions is incomplete [38]. Therefore, the results of Weyl almost periodic solutions of neural networks are still very rare. Therefore, it is a meaningful and challenging work to study the existence of Weyl almost periodic solutions of neural networks.

    Motivated by the above, in this paper, we consider the following shunting inhibitory cellular neural networks with time-varying delays:

    ˙xij(t)=aij(t)xij(t)CklNr(i,j)Bklij(t)fij(xkl(t))xij(t)CklNs(i,j)Cklij(t)gij(xkl(tτkl(t)))xij(t)+Iij(t), (1.1)

    where ij{11,12,,1n,,m1,m2,,mn}:=Λ, Cij denotes the cell at the (i,j) position of the lattice. The r-neighborhood Nr(i,j) of Cij is given as

    Nr(i,j)={Ckl:max(|ki|,|lj|)r,1km,1ln},

    and Ns(i,j) is similarly specified; xij(t)H denotes the activity of the cell of Cij, Iij(t)H is the external input to Cij, aij(t)H is the coefficient of the leakage term, which represents the passive decay rate of the activity of the cell Cij, Bklij(t)0 and Cklij(t)0 represent the connection or coupling strength of postsynaptic of activity of the cell transmitted to the cell Cij, the activity functions fij,gij:HH are continuous functions representing the output or firing rate of the cell Cij, τkl(t) corresponds to the transmission delay and satisfies 0τkl(t)τ.

    The purpose of this paper is to use the fixed point theorem and a variant of Gronwall inequality to establish the existence and global exponential stability of Weyl almost periodic solutions for a class of quaternion-valued shunting inhibitory cellular neural networks whose coefficients of the leakage terms are quaternions. This is the first paper to study the existence and global exponential stability of Weyl almost periodic solutions of system (1.1) by using the fixed point theorem and a variant of Gronwall inequality. Our result of this paper is new, and our method can be used to study other types of quaternion-valued neural networks.

    For convenience, we introduce the following notations:

    am=minijΛ{inftR{aij(t)}},aM=maxijΛ{suptR{aij(t)}},ˇaMij=suptRˇaij(t)H,
    BklMij=suptR{Bklij(t)},CklMij=suptR{Cklij(t)},τMij=suptR{τij(t)},τ=maxklΛ{suptR{τkl(t)}}.

    The initial condition of system (1.1) is given by

    xij(s)=φij(s),s[τ,0],

    where φijC(R,H),ijΛ.

    Throughout this paper, we assume that:

    (H1) For ij,klΛ, functions aRij,Bklij,CklijAP(R,R+), ˇaijAP(R,H), IijAPWp(R,H), τklAP(R,R+)C1(R,R) and τ<1.

    (H2) For ijΛ, there exist positive constants Lfij and Lgij such that for all x,yH,

    fij(x)fij(y)HLfijxyH,gij(x)gij(y)HLgijxyH,

    and fij(0)=gij(0)=0.

    The rest of this paper is arranged as follows. In Section 2, we introduce some definitions and lemmas. In Section 3, we study the existence and global exponential stability of Weyl almost periodic solutions of (1.1). In Section 4, an example is given to verify the theoretical results. This paper ends with a brief conclusion in Section 5.

    Let (X,X) be a Banach space and BC(R,X) be the set of all bounded continuous functions from R to X.

    Definition 2.1. [38] A function fBC(R,X) is said to be almost periodic, if for every ϵ>0, there exists a constant l=l(ϵ)>0 such that in every interval of length l(ϵ) contains at least one σ such that

    f(t+σ)f(t)X<ϵ,tR.

    Denote by AP(R,X) the set of all such functions.

    For p[1,), we denote by Lploc(R,X) the space of all functions from R into X which are locally p-integrable. For fLploc(R,X), we define the following seminorm:

    fWp=limr+supβR(1rβ+rβf(t)pXdt)1p.

    Definition 2.2. [38] A function fLploc(R,X) is said to be p-th Weyl almost periodic (Wp-almost periodic for short), if for every ϵ>0, there exists a constant l=l(ϵ)>0 such that in every interval of length l(ϵ) contains at least one σ such that

    f(t+σ)f(t)Wp<ϵ.

    This σ is called on ϵ-translation number of f. The set of all such functions will be denoted by APWp(R,X).

    Remark 2.1. By Definitions 2.1 and 2.2, it is easy to see that if fAP(R,X), then fAPWp(R,X).

    Similar to the proofs of the lemma on page 83 and the lemma on page 84 of [39], it is not difficult to prove the following two lemmas.

    Lemma 2.1. If fAPWp(R,X), then f is bounded and uniformly continuous on R withrespect to the seminorn Wp.

    Using the argumentation contained in the proof of Proposition 3.21 in [38], one can easily prove the following.

    Lemma 2.2. If fkAPWp(R,X), k=1,2,,n. Then, for every ϵ>0, there exist common ϵ-translation numbers for these functions.

    Lemma 2.3. [40]Let g:RR be a continuous function such that, for every tR,

    0g(t)ρ(t)+γ1teη1(ts)g(s)ds++γnteηn(ts)g(s)ds (2.1)

    for some locally integrable function ρ:RR, and for some constantsγ1,,γn0, and some constants η1,,ηnγ, whereγ=np=1γp. We assume that the integrals in the right hand side of (2.1)are convergent. Let η=min{η1,,ηn}. Then, for every ξ(0,ηγ]such that 0eξsρ(s)ds converges, we have, for every tR,

    g(t)ρ(t)+γteξ(ts)ρ(s)ds.

    In particular, if ρ(t) is constant, we have

    g(t)ρηηγ.

    Let BUC(R,Hm×n) be a collection of bounded and uniformly continuous functions from R to Hm×n, then, the space BUC(R,Hm×n) with the norm x=suptRx(t)Hm×n is a Banach space, where xBUC(R,Hm×n).

    Denote ϕ0=(ϕ011,,ϕ01n,ϕ021,,ϕ02n,,ϕ0m1,,ϕ0mn)T, where

    ϕ0ij(t)=tetsaRij(v)dvIij(s)ds,ijΛ.

    We will show that ϕ0 is well defined under assumption (H1). In fact, by IijAPWp(R,H) and Lemma 2.1, there exists a constant M>0 such that IijWpM for all ijΛ. According to the Hölder inequality, one has

    ϕ0ij(t)Hteam(ts)Iij(s)dsHr=0(trt(r+1)eamq(ts)ds)1q(trt(r+1)Iij(s)pHds)1pr=0eamrM<+, (3.1)

    where 1p+1q=1, which means that ϕ0 is well defined.

    Take a positive constant αϕ0. Let

    Ω={ϕBUC(R,Hm×n)|ϕϕ0α}.

    Then, for every ϕΩ, one has

    ϕϕϕ0+ϕ02α.

    Theorem 3.1. Assume (H1)(H2) hold. Furthermore, suppose that

    (H3)

    κ=maxijΛ{2am[ˇaMij+CklNr(i,j)2BklMijLfijα+CklNs(i,j)2CklMijLgijα]}<1,

    (H4)for p>2,

    maxijΛ{24(2p4amp)p2(4amp)2[2(ˇaMij)p+2(CklNr(i,j)2BklMijLfijα)p+(1+2ep4amτ1τ)(CklNs(i,j)2CklMijLgijα)p]}<1,

    and, for p=2,

    maxijΛ{24(2am)2[2(ˇaMij)2+2(CklNr(i,j)2BklMijLfijα)2+(1+2e12amτ1τ)(CklNs(i,j)2CklMijLgijα)2]}<1,

    then system (1.1) has a unique Wp-almost periodic solution in Ω.

    Proof. It is easy to check that if x=(x11,,x1n,x21,,x2n,,xm1,,xmn)TΩ is a solution of the integral equation

    xij(t)=tetsaRij(v)dv[ˇaij(s)xij(s)CklNr(i,j)Bklij(s)fij(xkl(s))xij(s)CklNs(i,j)Cklij(s)gij(xkl(sτkl(s)))xij(s)+Iij(s)]ds,ijΛ, (3.2)

    then x is a solution of system (1.1).

    Define an operator T:ΩHm×n by

    (Tϕ)(t)=((T11ϕ)(t),,(T1nϕ)(t),(T21ϕ)(t),,(T2nϕ)(t),,(Tm1ϕ)(t),,(Tmnϕ)(t))T,

    where

    (Tijϕ)(t)=tetsaRij(v)dv[ˇaij(s)ϕij(s)CklNr(i,j)Bklij(s)fij(ϕkl(s))ϕij(s)CklNs(i,j)Cklij(s)gij(ϕkl(sτkl(s)))ϕij(s)+Iij(s)]ds,ijΛ.

    Now, we will prove that Tϕ is well defined. Actually, by (H1)(H3) and (3.1), for ijΛ, one deduces that

    (Tijϕ)(t)HtetsaRij(v)dvˇaij(s)ϕij(s)CklNr(i,j)Bklij(s)(fij(ϕkl(s))fij(0))ϕij(s)CklNs(i,j)Cklij(s)(gij(ϕkl(sτkl(s)))gij(0))ϕij(s)Hds+tetsaRij(v)dvIij(s)Hds1am(ˇaMij+CklNr(i,j)BklMijLfijϕ+CklNs(i,j)CklMijLgijϕ)ϕ+tetsaRij(v)dvIij(s)Hds<+. (3.3)

    That is, Tϕ is well defined.

    We will divide the rest of the proof into four steps.

    Step 1, we will prove that TϕBUC(R,Hm×n), for every ϕΩ.

    In fact, by (3.3), we see that Tϕ is bounded on R. So, we only need to show that Tϕ is uniformly continuous on R. Based on the Hölder inequality for 0h1 and q1 with 1p+1q=1, one has

    (Tijϕ)(t+h)(Tijϕ)(t)H=t+het+hsaRij(v)dv(ˇaij(s)ϕij(s)CklNr(i,j)Bklij(s)fij(ϕkl(s))ϕij(s)CklNs(i,j)Cklij(s)×gij(ϕkl(sτkl(s)))ϕij(s)+Iij(s))dstetsaRij(v)dv(ˇaij(s)ϕij(s)CklNr(i,j)Bklij(s)×fij(ϕkl(s))ϕij(s)CklNs(i,j)Cklij(s)gij(ϕkl(sτkl(s)))ϕij(s)+Iij(s))dsHt|et+hsaRij(v)dvetsaRij(v)dv|ˇaij(s)ϕij(s)+CklNr(i,j)Bklij(s)fij(ϕkl(s))ϕij(s)+CklNs(i,j)Cklij(s)×gij(ϕkl(sτkl(s)))ϕij(s)Hds+t|et+hsaRij(v)dvetsaRij(v)dv|Iij(s)Hds+t+htet+hsaRij(v)dvˇaij(s)ϕij(s)+CklNr(i,j)Bklij(s)fij(ϕkl(s))ϕij(s)+CklNs(i,j)Cklij(s)×gij(ϕkl(sτkl(s)))ϕij(s)Hds+t+htet+hsaRij(v)dvIij(s)Hds(ˇaMij+CklNr(i,j)BklMijLfijϕ+CklNs(i,j)CklMijLgijϕ)ϕt(etsaRij(v)dvt+htaRij(v)dv)ds+t(etsaRij(v)dvt+htaRij(v)dv)Iij(s)Hds+(ˇaMij+CklNr(i,j)BklMijLfijϕ+CklNs(i,j)CklMijLgijϕ)ϕt+htetsaRij(v)dvds+t+htetsaRij(v)dvIij(s)HdsaMh(ˇaMij+CklNr(i,j)BklMijLfijϕ+CklNs(i,j)CklMijLgijϕ)ϕteam(ts)ds+aMhtetsaRij(v)dvIij(s)Hds+(ˇaMij+CklNr(i,j)BklMijLfijϕ+CklNs(i,j)CklMijLgijϕ)ϕ×t+hteam(ts)ds+(t+hteqam(ts)ds)1q(t+htIij(s)pHds)1paMam(ˇaMij+CklNr(i,j)BklMijLfijϕ+CklNs(i,j)CklMijLgijϕ)ϕh+aMhtetsaRij(v)dvIij(s)Hds+eamh(ˇaMij+CklNr(i,j)BklMijLfijϕ+CklNs(i,j)CklMijLgijϕ)ϕh+eamhIijWph,

    where ijΛ. Hence, letting h0+, by (3.1), we have

    (Tijϕ)(t+h)(Tijϕ)(t)H0,

    which means that (Tijϕ) is uniformly continuous on R, ijΛ. Therefore, TϕBUC(R,Hm×n).

    Step 2, we will prove that T is a self-mapping from Ω to Ω.

    Actually, for arbitrary ϕΩ, from (H2)(H3), we have

    Tϕϕ0suptR{maxijΛ[tetsaRij(v)dvˇaij(s)ϕij(s)+CklNr(i,j)Bklij(s)(fij(ϕkl(s))f(0))ϕij(s)+CklNs(i,j)Cklij(s)(gij(ϕkl(sτkl(s)))gij(0))ϕij(s)Hds]}maxijΛ{1am[ˇaMij+CklNr(i,j)2BklMijLfijα+CklNs(i,j)2CklMijLgijα]}ϕκαα,

    which implies that TϕΩ. Consequently, T is a self-mapping from Ω to Ω.

    Step 3, we will prove T is a contraction mapping.

    As a matter of fact, in view of (H1)(H2), for any ϕ,νΩ, we can get

    TϕTνsuptR{maxijΛ[team(ts)(ˇaMijϕij(s)νij(s)H+CklNr(i,j)BklMijfij(ϕkl(s))(ϕij(s)νij(s))+(fij(ϕkl(s))fij(νkl(s)))νij(s)H+CklNs(i,j)CklMijgij(ϕkl(sτkl(s)))(ϕij(s)νij(s))+(gij(ϕkl(sτkl(s)))gij(νkl(sτkl(s))))νij(s)H)ds]}suptR{maxijΛ[team(ts)[ˇaMijϕij(s)νij(s)H+CklNr(i,j)BklMij(2Lfijαϕij(s)νij(s)H+2Lfijαϕkl(s)νkl(s)H)+CklNs(i,j)CklMij(2Lgijαϕij(s)νij(s)H2Lgijαϕkl(sτkl(s))νkl(sτkl(s))H)]ds]}maxijΛ{1am[ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)4CklMijLgijα]}ϕν.

    From this and (H3), one has

    ||TϕTν||κϕν.

    Noticing that κ<1, T is a contraction mapping. Consequently, system (1.1) has a unique solution x in Ω.

    Step 4, we will prove that the unique solution xΩ is Wp-almost periodic.

    Indeed, since x=(x11,,x1n,x21,,x2n,,xm1,,xmn)TΩ, x is bounded and uniformly continuous. Hence, for every ϵ>0, there exists a δ(0,ϵ) such that for any t1,t2R with |t1t2|<δ and ijΛ, we have

    xij(t1)xij(t2)H<ϵ. (3.4)

    Also, for this δ, in view of (H1) and Lemma 2.2, we see that there exists a common δ-translation number σ such that

    limr+supβR(1rβ+rβIij(t+σ)Iij(t)pHdt)1p<δ<ϵ, (3.5)
    |Bklij(t+σ)Bklij(t)|<ϵ, (3.6)
    |Cklij(t+σ)Cklij(t)|<ϵ, (3.7)
    |aRij(t+σ)aRij(t)|<ϵ,ˇaij(t+σ)ˇaij(t)H<ϵ (3.8)

    and

    |τij(t+σ)τij(t)|<δ, (3.9)

    where ij,klΛ. Consequently, from (3.4) and (3.9), we get

    xij(tτij(t+σ))xij(tτij(t))H<ϵ. (3.10)

    Since x is a solution of system (1.1), by (3.2), for ijΛ, we have

    xij(t+σ)xij(t)HtetsaRij(v+σ)dv(ˇaij(s+σ)xij(s+σ)ˇaij(s)xij(s))dsH+tetsaRij(v+σ)dvCklNr(i,j)[Bklij(s+σ)fij(xkl(s+σ))xij(s+σ)Bklij(s)fij(xkl(s))xij(s)]dsH+tetsaRij(v+σ)dvCklNs(i,j)[Cklij(s+σ)×gij(xkl(s+στkl(s+σ)))xij(s+σ)Cklij(s)gij(xkl(sτkl(s)))xij(s)]dsH+tetsaRij(v+σ)dv[Iij(s+σ)Iij(s)]dsH+t(etsaRij(v+σ)dvetsaRij(v)dv)ˇaij(s)xij(s)dsH+t(etsaRij(v+σ)dvetsaRij(v)dv)CklNr(i,j)Bklij(s)fij(xkl(s))xij(s)dsH+t(etsaRij(v+σ)dvetsaRij(v)dv)CklNs(i,j)Cklij(s)gij(xkl(sτkl(s)))xij(s)dsH+t(etsaRij(v+σ)dvetsaRij(v)dv)Iij(s)dsH:=8l=1Blij(t). (3.11)

    When p>2, it follows from Hölder's inequality (2p,p2p), Hölder's inequality (12,12) and (H2) that

    B2ij(t)team(ts)CklNr(i,j)Bklij(s+σ)fij(xkl(s+σ))(xij(s+σ)xij(s))Hds+team(ts)CklNr(i,j)Bklij(s+σ)(fij(xkl(s+σ))fij(xkl(s)))xij(s)Hds+team(ts)CklNr(i,j)(Bklij(s+σ)Bklij(s))fij(xkl(s))xij(s)Hds(tep2p4am(ts)ds)p2p[tep4am(ts)(CklNr(i,j)2BklMijLfijαxij(s+σ)xij(s))H)p2ds]2p+(tep2p4am(ts)ds)p2p[tep4am(ts)(CklNr(i,j)2BklMijLfijαxkl(s+σ)xkl(s)H)p2ds]2p+(tep2p4am(ts)ds)p2p[tep4am(ts)(CklNr(i,j)4Lfijα2|Bklij(s+σ)Bklij(s)|ds)p2ds]2p(2p4amp)p2p{[tep4am(ts)(CklNr(i,j)2BklMijLfijαxij(s+σ)xij(s))H)p2ds]2p+[tep4am(ts)(CklNr(i,j)2BklMijLfijαxkl(s+σ))xkl(s)H)p2ds]2p+[tep4am(ts)(CklNr(i,j)4Lfijα2|Bklij(s+σ)Bklij(s)|ds)p2ds]2p}(2p4amp)p2p{[(tep4am(ts)ds)12(tep4am(ts)(CklNr(i,j)2BklMijLfijαxij(s+σ)xij(s))H)pds)12]2p+[(tep4am(ts)ds)12(tep4am(ts)(CklNr(i,j)2BklMijLfijα×xkl(s+σ))xkl(s)H)pds)12]2p+[(tep4am(ts)ds)12(tep4am(ts)×(CklNr(i,j)4Lfijα2|Bklij(s+σ)Bklij(s)|)pds)12]2p}(2p4amp)p2p(4amp)1p{[tep4am(ts)(CklNr(i,j)2BklMijLfijαxij(s+σ)xij(s))H)pds]1p+[tep4am(ts)(CklNr(i,j)2BklMijLfijαxkl(s+σ))xkl(s)H)pds]1p+[tep4am(ts)(CklNr(i,j)4Lfijα2|Bklij(s+σ)Bklij(s)|)pds]1p}, (3.12)

    for ijΛ. Similarly, we have

    B1ij(t)(2p4amp)p2p(4amp)1p{ˇaMij[tep4am(ts)xij(s+σ)xij(s)pHds]1p+2α[tep4am(ts)ˇaij(s+σ)˘aij(s)pHds]1p}, (3.13)
    B3ij(t)(2p4amp)p2p(4amp)1p{[tep4am(ts)(CklNs(i,j)2CklMijLgijαxij(s+σ)xij(s))H)pds]1p+[tep4am(ts)(CklNs(i,j)2CklMijLgijαxkl(s+στkl(s+σ))xkl(sτkl(s))H)pds]1p+[tep4am(ts)(CklNs(i,j)4Lgijα2|Cklij(s+σ)Cklij(s))|)pds]1p} (3.14)

    and

    B4ij(t)(2p4amp)p2p(4amp)1p(tep4am(ts)Iij(s+σ)Iij(s)pHds)1p, (3.15)

    for ijΛ.

    Besides, combining with Hölder's inequality (2p,p2p), Hölder's inequality (12,12) and (H2) that

    B5ij(t)2ˇaMijαteam(ts)(ts|aRij(v+σ)aRij(v)|dv)ds2ˇaMijα(tep2p4am(ts)ds)p2p[tep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)p2ds]2p(2p4amp)p2p2ˇaMijα[(tep4am(ts)ds)12(tep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)pds)12]2p(2p4amp)p2p(4amp)1p2ˇaMijα[tep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)pds]1p, (3.16)

    for ijΛ. In a similar way, one can get that

    B6ij(t)(2p4amp)p2p(4amp)1pCklNr(i,j)4BklMijLfijα2[tep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)pds]1p, (3.17)
    B7ij(t)(2p4amp)p2p(4amp)1pCklNs(i,j)4CklMijLgijα2[tep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)pds]1p (3.18)

    and

    B8ij(t)(2p4amp)p2p(4amp)1p[tep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)pIij(s)pHds]1p, (3.19)

    for ijΛ. Hence, together with a change of variables, Fubini's theorem, Hölder's inequality, (3.8) and (3.13), we derive that

    1rβ+rβBp1ij(t)dt(2p4amp)p24amp{1rβ+rβ[[ˇaMijtep4am(ts)xij(s+σ)xij(s)pHds]1p+2α[tep4am(ts)ˇaij(s+σ)˘aij(s)pHds]1p]pdt}(2p4amp)p28amp{(ˇaMij)p1rβ+rβtep4am(ts)xij(s+σ)xij(s)pHdsdt+(2α)p1rβ+rβtep4am(ts)ˇaij(s+σ)˘aij(s)pHdsdt}(2p4amp)p28amp{(ˇaMij)pβep4am(βs)(1rs+rsxij(t+σ)xij(t)pHdt)ds+(2α)pβep4am(βs)(1rs+rsˇaij(t+σ)˘aij(t)pHdt)ds}=(ˇaMij)p(2p4amp)p28ampβep4am(βs)Θσ,r(s)ds+ρ1ij,

    where

    Θσ,r(s):=1rs+rsx(t+σ)x(t)pHndt

    and

    ρ1ij:=2(2p4amp)p2(4amp)2(2αϵ)p, (3.20)

    and, together with a change of variables, Fubini's theorem, Hölder's inequality, (3.6) and (3.12), we derive that

    1rβ+rβBp2ij(t)dt(2p4amp)p24amp{1rβ+rβ[(tep4am(ts)(CklNr(i,j)2BklMijLfijαxij(s+σ)xij(s))H)pds)1p+(tep4am(ts)(CklNr(i,j)2BklMijLfijαxkl(s+σ)xkl(s)H)pds)1p+(tep4am(ts)(CklNr(i,j)4Lfijα2|Bklij(s+σ)Bklij(s)|)pds)1p]pdt}(2p4amp)p212amp{1rβ+rβtep4am(ts)(CklNr(i,j)2BklMijLfijαxij(s+σ)xij(s)H)pdsdt+1rβ+rβtep4am(ts)(CklNr(i,j)2BklMijLfijαxkl(s+σ)xkl(s)H)pdsdt+1rβ+rβtep4am(ts)(CklNr(i,j)4Lfijα2|Bklij(s+σ)Bklij(s)|)pdsdt}(2p4amp)p212amp[(CklNr(i,j)2BklMijLfijα)p1rβ+rβtep4am(ts)x(s+σ)x(s)pHm×ndsdt+(CklNr(i,j)2BklMijLfijα)p1rβ+rβtep4am(ts)x(s+σ)x(s)Hm×ndsdt+1rβ+rβtep4am(ts)(4mnLfijα2ϵ)pdsdt](2p4amp)p212amp[(CklNr(i,j)2BklMijLfijα)pβep4am(βs)(1rs+rsx(t+σ)x(t)pHm×ndt)ds+(CklNr(i,j)2BklMijLfijα)pβep4am(βs)(1rs+rsx(t+σ)x(t)Hm×ndt)ds+4amp(4mnLfijα2ϵ)p]=(2p4amp)p224amp(CklNr(i,j)2BklMijLfijα)pβep4am(βs)Θσ,r(s)ds+ρ2ij,

    where

    ρ2ij:=3(2p4amp)p2(4amp)2(4mnLfijα2ϵ)p. (3.21)

    Moreover, based on a change of variables, Fubini's theorem, Hölder's inequality, (3.7), (3.10) and (3.14), we deduce that

    1rβ+rβBp3ij(t)dt(2p4amp)p24amp{1rβ+rβ[(tep4am(ts)(CklNs(i,j)2CklMijLgijαxij(s+σ)xij(s))H)pds)1p+(tep4am(ts)(CklNs(i,j)2CklMijLgijαxkl(s+στkl(s+σ))xkl(sτkl(s))H)pds)1p+(tep4am(ts)(CklNs(i,j)4Lgijα2(Cklij(s+σ)Cklij(s))H)pds)1p]pdt}(2p4amp)p212amp{1rβ+rβtep4am(ts)(CklNs(i,j)2CklMijLgijαxij(s+σ)xij(s))H)pdsdt+1rβ+rβtep4am(ts)(CklNs(i,j)2CklMijLgijαxkl(s+στkl(s+σ))xkl(sτkl(s))H)pdsdt+1rβ+rβtep4am(ts)(CklNs(i,j)4Lgijα2|Cklij(s+σ)Cklij(s))|)pdsdt}(2p4amp)p212amp{1rβ+rβtep4am(ts)(CklNs(i,j)2CklMijLgijαxij(s+σ)xij(s))H)pdsdt+1rβ+rβ[2tep4am(ts)(CklNs(i,j)2CklMijLgijαxkl(s+στkl(s+σ))xkl(sτkl(s+σ))H)pds+2tep4am(ts)(CklNs(i,j)4CklMijLgijα2xkl(sτkl(s+σ))xkl(sτkl(s))H)pds]dt+1rβ+rβtep4am(ts)(4mnLgijα2ϵ)pdsdt}(2p4amp)p212amp{1rβ+rβtep4am(ts)(CklNs(i,j)2CklMijLgijαxij(s+σ)xij(s))H)pdsdt+1rβ+rβ[21τtτkl(t+σ)ep4am(tuτ)(CklNs(i,j)2CklMijLgijαxkl(u+σ)xkl(u)H)pdu+2(CklNs(i,j)2CklMijLgijαϵ)ptep4am(ts)ds]dt+4amp(4mnLgijα2ϵ)p}(2p4amp)p212amp{1rβ+rβtep4am(ts)(CklNs(i,j)2CklMijLgijαxij(s+σ)xij(s))H)pdsdt+1rβ+rβ[2ep4amτ1τtep4am(ts)(CklNs(i,j)2CklMijLgijαxkl(s+σ)xkl(s)H)pds]dt+8amp(CklNs(i,j)2CklMijLgijαϵ)p+4amp(4mnLgijα2ϵ)p}(2p4amp)p212amp[(CklNs(i,j)2CklMijLgijα)pβep4am(βs)(1rs+rsx(t+σ)x(t))Hm×ndt)ds+2ep4amτ1τ(CklNs(i,j)2CklMijLgijα)pβep4am(βs)(1rs+rsx(t+σ)x(t)pHm×ndt)ds+8amp(CklNs(i,j)2CklMijLgijαϵ)p+4amp(4mnLgijα2ϵ)p]=(2p4amp)p212amp(1+2ep4amτ1τ)(CklNs(i,j)2CklMijLgijα)pβep4am(βs)Θσ,r(s)ds+ρ3ij,

    where

    ρ3ij:=3(2p4amp)p2(4amp)2[2(CklNs(i,j)2CklMijLgijα)p+(4mnLgijα2)p]ϵp. (3.22)

    In view of (3.5), (3.8) and (3.15)–(3.19), we can easily obtain that

    1rβ+rβBp4ij(t)dt(2p4amp)p24ampβep4am(βs)(1rs+rsIij(t+σ)Iij(t)pHdt)ds(2p4amp)p2(4amp)2ϵp:=ρ4ij, (3.23)
    1rβ+rβBp5ij(t)dt(2p4amp)p24amp(2ˇaMijα)p[1rβ+rβtep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)pdsdt](2p4amp)p24amp(2ˇaMijαϵ)p0ep4amsspds:=ρ5ij, (3.24)
    1rβ+rβBp6ij(t)dt(2p4amp)p24amp(CklNr(i,j)4BklMijLfijα2)p[1rβ+rβtep4am(ts)×(ts|aRij(v+σ)aRij(v)|dv)pdsdt](2p4amp)p24amp(CklNr(i,j)4BklMijLfijα2ϵ)p0ep4amsspds:=ρ6ij, (3.25)
    1rβ+rβBp7ij(t)dt(2p4amp)p24amp(CklNs(i,j)4CklMijLgijα2)p[1rβ+rβtep4am(ts)×(ts|aRij(v+σ)aRij(v)|dv)pdsdt](2p4amp)p24amp(CklNs(i,j)4CklMijLgijα2ϵ)p0ep4amsspds:=ρ7ij (3.26)

    and

    1rβ+rβBp8ij(t)dt(2p4amp)p24amp[1rβ+rβtep4am(ts)(ts|aRij(v+σ)aRij(v)|dv)pIij(s)pHdsdt]ϵp(2p4amp)p24amp[1rβ+rβtep4am(ts)(ts)pIij(s)pHdsdt](2p4amp)p24ampIijpWpϵp0ep4amsspds:=ρ8ij, (3.27)

    for ijΛ. Consequently, combining with (3.11) and (3.20)–(3.27), we obtain

    Θσ,r(β)maxijΛ{88l=11rβ+rβBplij(t)dt}ρ+γβeη(βs)Θσ,r(s)ds,

    where η=p4am,

    ρ=86l=1maxijΛ{ρlij}=8maxijΛ{(2p4amp)p24amp[8amp(2α)p+12amp(4mnLfijα2)p+24amp(CklNs(i,j)2CklMijLgijα)P+12amp(4mnLgijα2)p+4amp+[(2ˇaMijα)p+(CklNr(i,j)4BklMijLfijα2)p+(CklNs(i,j)4CklMijLgijα2)p+IijpWp]0ep4amsspds]}ϵp

    and

    γ=8maxijΛ{(2p4amp)p212amp[23(ˇaMij)p+2(CklNr(i,j)2BklMijLfijα)p+(1+2ep4amτ1τ)(CklNs(i,j)2CklMijLgijα)p]}.

    By (H4), we have γ<η. Thus, it follows from Lemma 2.3 that

    1rβ+rβx(t+σ)x(t)pHm×ndtρηηγ.

    Hence, xAPWp(R,Hm×n).

    When p=2, similar to the proof of the case of p>2, one can obtain

    Θσ,r(β)˜ρ+˜γβe˜η(βs)Θσ,r(s)ds,

    where ˜η=am2,

    ˜ρ=88l=1maxijΛ{˜ρlij}=maxijΛ{16am[4am(2α)2+6am(4mnLfijα2ϵ)2+12am(2CklNs(i,j)CklMijLgijα)2+6am(4mnLgijα2)2+2am+[(2ˇaMijα)2+(CklNr(i,j)4BklMijLfijα2)2+(CklNs(i,j)4CklMijLgijα2)2+Iij2W2]0e12amss2ds]}ϵ2

    and

    ˜γ=maxijΛ{48am[23(ˇaMij)2+2(CklNr(i,j)2BklMijLfijα)2+(1+2e12amτ1τ)(CklNs(i,j)2CklMijLgijα)2]}.

    By (H4), we have ˜γ<˜η. Thus, it follows from Lemma 2.3 that

    1rβ+rβx(t+σ)x(t)pHm×ndt˜ρ˜η˜η˜γ,

    which means that xAPW2(R,Hm×n). The proof is complete.

    Definition 3.1. [14] Let x be a solution of system (1.1) with the initial value φ and y be an arbitrary solution of system (1.1) with the initial value ψ, respectively. If there exist positive constants λ and M such that

    x(t)y(t)Hm×nMeλtφψτ,tR+,

    where φψτ=supt[τ,0]φ(t)ψ(t)Hm×n. Then the solution x of system (1.1) is said to be globally exponentially stable.

    Theorem 3.2. Assume that (H1)(H3) hold, then system (1.1) has a unique Wp-almost periodic solution that is globallyexponentially stable.

    Proof. Let x(t) be the Wp-almost periodic solution with the initial value φ(t) and y(t) be an arbitrary solution with the initial value ψ(t). Taking

    zij(t)=xi(t)yij(t),ϕij(t)=φij(t)ψij(t),ijΛ,

    we have

    ˙zij(t)=aij(t)zij(t)CklNr(i,j)Bklij(t)(fij(xkl(t))xij(t)fij(ykl(t))yij(t)CklNs(i,j)Cklij(t)(gij(xkl(tτkl(t)))xij(t)gij(ykl(tτkl(t)))yij(t)),ijΛ. (3.28)

    For ijΛ, we define the following functions:

    Πij(u)=amu(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeuτMij+CklNs(i,j)2CklijLgijα).

    From (H3), we get

    Πij(0)=am(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)4CklMijLgijα)>0,ijΛ.

    Since Πij(u) is continuous on [0,+) and Πij(u) as u, there exists ζij>0 such that Πij(ζij)=0 and Πij(u)>0, for u(0,ζij), ijΛ. Let ς=minijΛ{ζij}, then we have Πij(ς)0,ijΛ. Hence, we can choose a positive constant λ such that 0<λ<min{ς,am} and Πij(λ)>0. Thus, one has

    1amλ(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeλτMij+CklNs(i,j)2CklijLgijα)<1, (3.29)

    where ijΛ. Take a constant M=maxiΛ{amˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)4CklMijLgijα}, then by (H3), we have M>1. Thus,

    1M1amλ(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeλτMij+CklNs(i,j)2CklijLgijα)<0,ijΛ. (3.30)

    From (3.28), we have

    ˙zij(t)+aRij(t)zij(t)=ˇaij(t)zij(t)CklNr(i,j)Bklij(t)(fij(xkl(t))xij(t)fij(ykl(t))yij(t))CklNs(i,j)Cklij(t)(gij(xkl(tτkl(t)))xij(t)gij(ykl(tτkl(t)))yij(t)),ijΛ. (3.31)

    Multiplying both sides of (3.31) by et0aRij(v)dv and integrating over [0,t], we have

    zij(t)=ϕij(0)et0aRij(v)dv+t0etsaRij(v)dv[ˇaij(t)zij(s)CklNr(i,j)Bklij(t)(fij(xkl(t))xij(t)fij(ykl(t))yij(t))CklNs(i,j)Cklij(t)(gij(xkl(tτkl(t)))xij(t)gij(ykl(tτkl(t)))yij(t))]ds,ijΛ.

    Hence, for any ϵ>0, it is easy to see that

    z(t)Hm×n<(ϕτ+ϵ)eλt<M(ϕτ+ϵ)eλt,t(τ,0].

    We claim that

    z(t)Hm×n<M(ϕτ+ϵ)eλt,t[0,+). (3.32)

    Otherwise, there exists t>0 such that

    z(t)Hm×n=M(ϕτ+ϵ)eλt (3.33)

    and

    z(t)Hm×n<M(ϕτ+ϵ)eλt,t<t. (3.34)

    From (3.29), (3.30) and (3.34), we get

    zij(t)Hϕij(0)Hetam+t0etam[ˇaMijzij(s)H+CklNr(i,j)Bklij(t)×(fij(xkl(t))(xij(t)yij(t))H+(fij(xkl(t))fij(ykl(t)))yij(t)H)+CklNs(i,j)Cklij(t)(gij(xkl(tτkl(t)))(xij(t)yij(t))H+(gij(xkl(tτkl(t)))gij(ykl(tτkl(t))))yij(t)H)]ds(ϕτ+ϵ)eamt+M(ϕτ+ϵ)t0e(ts)am(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeλτMij+CklNs(i,j)2CklijLgijα)eλsds(ϕτ+ϵ)eλte(λam)t+M(ϕτ+ϵ)eλt(1e(λam)t)amλ(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeλτMij+CklNs(i,j)2CklijLgijα)=M(ϕτ+ϵ)eλt[e(λam)tM+1e(λam)tamλ(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeλτMij+CklNs(i,j)2CklijLgijα)]=M(ϕτ+ϵ)eλt[(1M1amλ(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeλτMij+CklNs(i,j)2CklijLgijα)e(λam)t+1amλ(ˇaMij+CklNr(i,j)4BklMijLfijα+CklNs(i,j)2CklijLgijαeλτMij+CklNs(i,j)2CklijLgijα)]<M(ϕτ+ϵ)eλt,ijΛ,

    which contradicts the Eq (3.33). Hence, (3.32) holds. Letting ϵ0+, from (3.32), we have

    z(t)Hm×nMϕτeλt,t>0.

    Therefore, the Wp-almost periodic solution of system (1.1) is globally exponentially stable. This completes the proof.

    Example 4.1. In system (1.1), let i,j=1,2, r=s=1 and take

    xij(t)=xRij(t)+ixIij(t)+jxJij(t)+kxKij(t)H,
    a11(t)=32sin2(3t)+i25cos(2t)j25sin(5t)+k1100cos2(3t),
    a21(t)=39|cos(2t)|i210sin(2t)+j310sin2(7t)+k3100cos(t),
    a12(t)=33cos2(t)i36sin(5t)j14cos3(5t)+k16cos2(3t)
    a22(t)=37sin4(3t)+i14cos(7t)j2916|sin(11t)|+k18cos2(5t),
    τ11(t)=232sin8(2t),τ12(t)=116cos2(3t),τ21(t)=141sin2(25t),τ22(t)=129sin4(37t),
    B11(t)=13|cos(2t)|,B12(t)=16sin(4t)+12B21(t)=34sin(2t)+1,B22(t)=14sin2(5t),
    C11(t)=cos(3t)+3,C12(t)=|sin(5t)|,C21(t)=2sin2(7t),C22(t)=14sin(2t)+74,
    f11(x)=f12(x)=15sin(14xR+36xK)i15|324xI+35xJ|+k14sin(15xR),
    f21(x)=f22(x)=14|23xI+37xK|i28sin(15xR+25xK)+k23sin(15xIj),
    g11(x)=g12(x)=120sin(922xR)i340sin(75xK)+j220sin(13xJ+34xI),
    g21(x)=g22(x)=225|13xJ+23xI|i340sin(75xK+xR)+j121sin(42xR),
    I11(t)=I21(t)=2sint+i43e|t|+k23cos(12t),
    I12(t)=I22(t)=i23sin2tj15cos2t+ke|t|.

    By computing, we obtain

    Lf11=Lf12=310,Lf21=Lf22=16,Lg11=Lg12=920,Lg21=Lg22=821,
    am=32,ˇaM11=12,ˇaM12=25,ˇaM21=512,ˇaM22=716,τ=116,τ=12,
    CklN1(1,1)BklM11=CklN1(1,2)BklM12=CklN1(2,1)BklM21=CklN1(2,2)BklM22=4,
    CklN1(1,1)CklM11=CklN1(1,2)CklM12=CklN1(2,1)CklM21=CklN1(2,2)CklM22=8.

    Choose a constant α=116ϕ0, for i,j=1,2, we obtain that

    κ=maxijΛ{2am[ˇaMij+CklNr(i,j)2BklMijLfijα+CklNs(i,j)2CklMijLgijα]}=0.06875<1.

    For i,j=1,2, take p=3, it is easy to obtain that

    maxijΛ{96(23am)3[23(ˇaMij)3+2(CklNr(i,j)2BklMijLfijα)3+(1+2e34amτ1τ)(CklNs(i,j)2CklMijLgijα)3]}=0.0016<1.

    Take p=2, we have

    maxijΛ{24(2am)2[23(ˇaMij)2+2(CklNr(i,j)2BklMijLfijα)2+(1+2e12amτ1τ)(CklNs(i,j)2CklMijLgijα)2]}=0.2832<1.

    Thus, conditions (H1)(H4) of Theorems 3.1 and Theorems 3.2 are satisfied. Hence, system (1.1) has a unique Wp-almost periodic solution that is globally exponentially stable (see Figures 1, 2).

    Figure 1.  Curves of (xl11(t),xl12(t))T of system (1.1) with the initial values (xl11(0),xl12(0))T=(1,2)T,(3,4)T,(5,5)T,(7,7)T,(9,9)T, l = R, I, J, K.
    Figure 2.  Curves of (xl21(t),xl22(t))T of system (1.1) with the initial values (xl21(0),xl22(0))T=(8,1)T,(9,3)T,(5,5)T,(7,2)T,(9,4)T, l = R, I, J, K.

    Remark 4.1. No known results are available to give the results of Example 4.1.

    In this paper, the existence and global exponential stability of Weyl almost periodic solutions for a class of quaternion-valued neural networks with time-varying delays are established. Even when the system we consider is a real-valued system, our results are brand-new. In addition, the method in this paper can be used to study the existence of Weyl almost periodic solutions for other types of neural networks.

    This work is supported by the National Natural Science Foundation of China under Grant 11861072.

    The authors declare no conflict of interest in this paper.



    [1] B. O'Nill, Semi-Riemannian geometry with applications to relativity, Londan: Academic Press Limited, 1983.
    [2] S. Weinberg, Gravitation and cosmology: Principles and applications of the general theory of relativity, Hoboken: Willy, 1972.
    [3] L. Jäntschi, Eigenproblem basics and algorithms, Symmetry, 15 (2023), 2046. https://doi.org/10.3390/sym15112046 doi: 10.3390/sym15112046
    [4] L. Euler, Du mouvement d'un corps solide quelconque lorsqu'il tourne autour d'un axe mobile, Mémoires de l'académie des sciences de Berlin, 16 (1767), 176–227.
    [5] J. Lagrange, Nouvelle solution du problème du mouvement de rotation d'un corps de figure quelconque qui n'est animé par aucune force accélératrice, In: Œuvres de Lagrange [Tome 3], Beijing: Higher Education Press, 1869,577–616.
    [6] P. S. Laplace, Mémoire sur les solutions particulières des équations différentielles et sur les inégalités séculaires des planètes, In: Dans Œuvres complètes de Laplace, tome huitième, Paris: Gauthier-Villars et fils, 1891,325–366.
    [7] J. B. Fourier, Thèorie cnalytique de la chaleur, Cambridge: Cambridge University Press, 1822. https://doi.org/10.1017/CBO9780511693229
    [8] A. Cauchy, Sur 1'équation à l'aide de laquelle on determine les inégalités séculaires des mouvements des planètes, In: Oeuvres complètes, Cambridge: Cambridge University Press, 1891,174–195. https://doi.org/10.1017/CBO9780511702686.009
    [9] S. H. Tye, Brane inflation: String theory viewed from the cosmos, Lect. Notes Phys., 737 (2008), 949–974.
    [10] P. S. Letelier, Clouds of strings on general relativity, Phys. Rev. D, 20 (1979), 1294–1302. https://doi.org/10.1103/PhysRevD.20.1294 doi: 10.1103/PhysRevD.20.1294
    [11] M. D. Siddiqi, M. A. Khan, I. Al-Dayel, K. Masood, Geometrization of string cloud spacetime in general relativity, AIMS Mathematics, 8 (2023), 29042–29057. https://doi.org/10.3934/math.20231487 doi: 10.3934/math.20231487
    [12] E. Herscovich, M. G. Richarte, Black holes in Einstein-Gauss-Bonnet gravity with a string cloud background, Phys. Lett. B, 689 (2010), 192–200. https://doi.org/10.1016/j.physletb.2010.04.065 doi: 10.1016/j.physletb.2010.04.065
    [13] S. G. Ghosh, U. Papnoi, S. D. Maharaj, Cloud of strings in third order Lovelock gravity, Phys. Rev. D, 90 (2014), 044068. https://doi.org/10.1103/PhysRevD.90.044068 doi: 10.1103/PhysRevD.90.044068
    [14] M. G. Richarte, C. Simeone, Traversable wormholes in a string cloud, Int. J. Mod. Phys. D, 17 (2008), 1179–1196. https://doi.org/10.1142/S0218271808012759 doi: 10.1142/S0218271808012759
    [15] A. K. Yadav, V. K. Yadav, L. Yadav, Cylindrically symmetric inhomogeneous universes with a cloud of strings, Int. J. Theor. Phys., 48 (2009), 568–578. https://doi.org/10.1007/s10773-008-9832-9 doi: 10.1007/s10773-008-9832-9
    [16] A. Ganguly, S. G. Ghosh, S. D. Maharaj, Accretion onto a black hole in a string cloud background, Phys. Rev. D, 90 (2014), 064037. https://doi.org/10.1103/PhysRevD.90.064037 doi: 10.1103/PhysRevD.90.064037
    [17] M. Novello, M. J. Reboucas, The stability of a rotating universe, Astrophys. J., 225 (1978), 719–724.
    [18] R. Jackiw, V. P. Nair, S. Y. Pi, A. P. Polychronakos, Perfect fluid theory and its extensions, J. Phys. A: Math. Gen., 37 (2004), R327. https://doi.org/10.1088/0305-4470/37/42/R01 doi: 10.1088/0305-4470/37/42/R01
    [19] S. Guler, S. A. Demirbağ, A study of generalized quasi-Einstein spacetimes with applications in general relativity, Int. J. Theor. Phys., 55 (2016), 548–562. https://doi.org/10.1007/s10773-015-2692-1 doi: 10.1007/s10773-015-2692-1
    [20] M. C. Chaki, On generalized quasi Einstein manifolds, Publ. Math. Debrecen, 58 (2001), 683–691.
    [21] L. O. Pimental, Energy-momentum tensor in the general scalar-tensor theory, Class. Quantum Grav., 6 (1989), L263. https://doi.org/10.1088/0264-9381/6/12/005 doi: 10.1088/0264-9381/6/12/005
    [22] V. Faraoni, J. Cote, Imperfect fluid description of modified gravity, Phys. Rev., 98 (2018), 084019. https://doi.org/10.1103/PhysRevD.98.084019 doi: 10.1103/PhysRevD.98.084019
    [23] I. Sawicki, I. D. Saltas, L. Amendola, M. Kunz, Consistent perturbations in an imperfect fluid, J. Cosmol. Astropart. P., 2013 (2013), 004. https://doi.org/10.1088/1475-7516/2013/01/004 doi: 10.1088/1475-7516/2013/01/004
    [24] K. L. Duggal, Almost Ricci solitons and physical applications, International Electronic Journal of Geometry, 10 (2017), 1–10.
    [25] R. S. Hamilton, The Ricci flow on surfaces, mathematics and general relativity, Contemp. Math., 7 (1988), 237–261.
    [26] A. E. Fischer, An introduction to conformal Ricci flow, Class. Quantum Grav., 21 (2004), S171. https://doi.org/10.1088/0264-9381/21/3/011 doi: 10.1088/0264-9381/21/3/011
    [27] N. Basu, A. Bhattacharyya, Conformal Ricci soliton in Kenmotsu manifold, Global Journal of Advanced Research on Classical and Modern Geometries, 4 (2015), 15–21.
    [28] M. D. Siddiqi, Conformal η-Ricci solitons in δ-Lorentzian Trans Sasakian manifolds, International Journal of Maps in Mathematics, 1 (2018), 15–34.
    [29] M. Ali, Z. Ahsan, Ricci solitons and symmetries of spacetime manifold of general relativity, Journal of Advanced Research on Classical and Modern Geometries, 1 (2014), 75–84.
    [30] A. M. Blaga, Solitons and geometrical structures in a perfect fluid spacetime, Rocky Mountain J. Math., 50 (2020), 41–53. https://doi.org/10.1216/rmj.2020.50.41 doi: 10.1216/rmj.2020.50.41
    [31] Venkatesha, H. A. Kumara, Ricci solitons and geometrical structure in a perfect fluid spacetime with torse-forming vector field, Afr. Mat., 30 (2019), 725–736. https://doi.org/10.1007/s13370-019-00679-y doi: 10.1007/s13370-019-00679-y
    [32] M. D. Siddiqi, S. A. Siddiqui, Conformal Ricci soliton and geometrical structure in a perfect fluid spacetime, Int. J. Geom. Methods M., 17 (2020), 2050083. https://doi.org/10.1142/s0219887820500838 doi: 10.1142/s0219887820500838
    [33] A. N. Siddiqui, M. D. Siddiqi, Almost Ricci-Bourguignon solitons and geometrical structure in a relativistic perfect fluid spacetime, Balk. J. Geom. Appl., 26 (2021), 126–138.
    [34] M. D. Siddiqi, F. Mofarreh, A. N. Siddiqui, S. A. Siddiqui, Geometrical structure in a relativistic thermodynamical fluid spacetime, Axioms, 12 (2023), 138. https://doi.org/10.3390/axioms12020138 doi: 10.3390/axioms12020138
    [35] M. D. Siddiqi, F. Mofarreh, S. K. Chaubey, Solitonic aspect of relativistic Magneto-fluid spacetime with some specific vector fields, Mathematics, 11 (2023), 1596. https://doi.org/10.3390/math11071596 doi: 10.3390/math11071596
    [36] M. D. Siddiqi, A. H. Alkhaldi, M. A. Khan, A. N. Siddiqui, Conformal η-Ricci solitons on riemannian submersions under canonical variation, Axioms, 11 (2022), 594. https://doi.org/10.3390/axioms11110594 doi: 10.3390/axioms11110594
    [37] A. H. Alkhaldi, M. D. Siddiqi, M. A. Khan, L. S. Alqahtani, Imperfect fluid generalized robertson walker spacetime admitting Ricci-Yamabe metric, Adv. Math. Phys., 2021 (2021), 2485804. https://doi.org/10.1155/2021/2485804 doi: 10.1155/2021/2485804
    [38] K. A. Bronnikov, S. W. Kim, M. V. Skvortsova, The Birkhohff theorem and string clouds, Class. Quantum Grav., 33 (2016), 195006. https://doi.org/10.1088/0264-9381/33/19/195006 doi: 10.1088/0264-9381/33/19/195006
    [39] C. Alcock, E. Farhi, A. Olinto, Strange stars, Astrophys. J., 310 (1986), 261. https://doi.org/10.1086/164679 doi: 10.1086/164679
    [40] P. Haensel, J. L. Zdunik, R. Sehaffer, Strange quark stars, Astron. Astrophys., 160 (1986), 121–128.
    [41] K. S. Cheng, Z. G. Dai, T. Lu, Strange stars and related astrophysical phenomena, Int. J. Mod. Phys. D, 7 (1998), 139–176. https://doi.org/10.1142/S0218271898000139 doi: 10.1142/S0218271898000139
    [42] I. Yavuz, I. Yilmaz, H. Baysal, Strange quark matter attached to the string cloud in the spherically symmetric space-time admitting conformal motion, Int. J. Mod. Phys. D, 14 (2005), 1365–1372. https://doi.org/10.1142/S0218271805007061 doi: 10.1142/S0218271805007061
    [43] K. Johnson, The M.I.T bag model, Acta Phys. Pol., B6 (1975), 865–892.
    [44] J. I. Kapusta, Finite-temperature field theory, Cambridge: Cambridge University Press, 2006. https://doi.org/10.1088/0954-3899/15/3/005
    [45] Z. H. Liu, J. C. Niu, Vibrational energy flow model for functionally graded beams, Compos. Struct., 186 (2018), 17–28. https://doi.org/10.1016/j.compstruct.2017.11.026 doi: 10.1016/j.compstruct.2017.11.026
    [46] J. Satish, R. Venkateswarlu, Bulk viscous fluid cosmological models in f(R,T) gravity, Chinese J. Phys., 54 (2016), 830–838. https://doi.org/10.1016/j.cjph.2016.08.008 doi: 10.1016/j.cjph.2016.08.008
    [47] H. Sotani, K. Kohri, T. Harada, Restriction quark matter models by gravitational wave observation, Phys. Rev. D, 69 (2004), 084008. https://doi.org/10.1103/PhysRevD.69.084008 doi: 10.1103/PhysRevD.69.084008
    [48] I. Hinterleither, V. A. Kiosak, φ(Ric)-Vector field in Riemannian spaces, Arch. Math., 44 (2008), 385–390. http://eudml.org/doc/250510
    [49] M. Katz, Liouville's equation for curvature and systolic defect, 2011, arXiv: 1105.0553.
    [50] A. G. Popov, Exact formula for constructing solutions of the Liouville equation Δ2u=eu from solutions of the Laplace equation Δ2v=0, Dokl. Akad. Nauk., 333 (1993), 440–441.
    [51] B. Chow, S. C. Chu, D. Glickenstein, C. Guenther, J. Isenberg, T. Ivey, et al., The Ricci flow: techniques and applications, part Ⅰ: geometric aspects, Rhode Island: American Mathematical Society, 2007. http://doi.org/10.1090/surv/163
    [52] A. M. Blaga, Harmonic aspects in an η-Ricci soliton, Int. Electron. J. Geom., 13 (2020), 41–49. https://doi.org/10.36890/iejg.573919 doi: 10.36890/iejg.573919
  • This article has been cited by:

    1. Adnène Arbi, Najeh Tahri, New results on time scales of pseudo Weyl almost periodic solution of delayed QVSICNNs, 2022, 41, 2238-3603, 10.1007/s40314-022-02003-0
    2. Marko Kostić, Weyl ρ-Almost Periodic Functions in General Metric, 2023, 73, 1337-2211, 465, 10.1515/ms-2023-0035
    3. Qi Shao, Yongkun Li, Almost periodic solutions for Clifford-valued stochastic shunting inhibitory cellular neural networks with mixed delays, 2024, 9, 2473-6988, 13439, 10.3934/math.2024655
    4. Adnène Arbi, Najeh Tahri, Synchronization analysis of novel delayed dynamical Clifford-valued neural networks on timescales, 2024, 18, 1748-3018, 10.1177/17483026241241492
  • Reader Comments
  • © 2024 the Author(s), licensee AIMS Press. This is an open access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0)
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Metrics

Article views(882) PDF downloads(33) Cited by(11)

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return

Catalog