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Research article

Double controlled M-metric spaces and some fixed point results

  • In this article, we introduce the idea of double controlled M-metric space by employing two control functions a(u,w) and β(w,v) on the right-hand side of the triangle inequality of M-metric space. We provide some examples of double controlled M-metric spaces. We also provide some fixed point results under new type of contractions in the setting of double controlled M-metric spaces. Moreover, we give an example to highlight the importance of one of our main results.

    Citation: Fahim Uddin, Faizan Adeel, Khalil Javed, Choonkil Park, Muhammad Arshad. Double controlled M-metric spaces and some fixed point results[J]. AIMS Mathematics, 2022, 7(8): 15298-15312. doi: 10.3934/math.2022838

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  • In this article, we introduce the idea of double controlled M-metric space by employing two control functions a(u,w) and β(w,v) on the right-hand side of the triangle inequality of M-metric space. We provide some examples of double controlled M-metric spaces. We also provide some fixed point results under new type of contractions in the setting of double controlled M-metric spaces. Moreover, we give an example to highlight the importance of one of our main results.



    First, Peregrine [1] promulgated the regularized long-wave (RLW) equation to describe the propagation of unidirectional weakly nonlinear dispersive water waves. Furthermore, the authors of [2,3] engaged this equation to illuminate an enormous class of real-world problems as a substitute of the well-known Korteweg–De Vries (KdV) equation. These studies revealed that the RLW equation is more impressive than the latter one. The RLW equation takes part as a fundamental role in the study of the non-linear dispersive waves that have a lot of norms in various precise areas, e.g., magnetohydrodynamic waves as well as ion acoustic plasma waves, longitudinal dispersive and pressure waves in elastic rods and liquid-gas bubble mixtures, and rotating flow down a tube. Bona et al. [4] proposed an integer-ordered formulation of the RLW equation for describing the surface water wave's propagation in a channel.

    The RLW equation has been studied by means of numerous procedures. For instance, this equation has been approximated, numerically, by the Galerkin finite element method (FEM) [15,16,34], Petrov-Galerkin FEM [17], least squares FEM [18], CBS and least squares CBS finite element methods (FEMs) [19,25], respectively, least squares quadratic B-spline (QdBS) FEM [20], splitting methods with CBS and QdBS FEMs [21,22], respectively, quintic B-spline Galerkin finite element method (QBS-GFEM) [23], linearized implicit finite difference method (FDM) [24], splitting-up technique with CBS and QdBS [26], quartic B-spline, QBS, and fourth-order CBS collocation techniques [27,28,29], respectively, CBS differential quadrature method [30], and lumped Galerkin QdBS FEM [33].

    It is generally recognized that the trajectory's characteristic of the fractional derivatives is non-local as the remembrance outcome [5]. Many researchers prove that fractional differential equations (FDEs) are more appropriate than integer-order ones, as fractional derivatives demonstrate the memory and inherited possessions of several materials and processes [6,7,8,9].

    Furthermore, the time-fractional partial differential equations (TFDEs) have generated further consideration for a number of real-life applications such as signal processing, electrical network systems, optics, financial estimation and forecast, mathematical biology, electromagnetic control theory, fluid flows in multi-dimension, material science, acoustics, biological systems associated with predator-prey models, etc. [10,11,12,13]. The application of fractional models is rising for enhanced precision in real-life models, and points out substantial necessities for improved fractional mathematical models. In [14], the author implemented Caputo's fractional derivative for dynamical investigation of a generalized tumor model. This derivative is being used for modeling of biological systems, comprising tumor growth. In biomedical research, tumor growth models have been expansively used to examine the dynamics of tumor expansion and estimating possible treatments.

    Recently, the TFRLW equation was approximated by some analytical and numerical methods. For instant, the authors of [8] applied a method based on the q-homotopy analysis transform for approximating the TFRLW equation, while in [9], they presented a new fractional extension of the RLW equation. Besides, they used the fixed-point theorem to prove the existence and uniqueness of the solutions. Nikan et al. [35] obtained the traveling-wave solutions of the TFRLW equation using the radial basis function (RBF) collocation technique. Maarouf et al. [38] systematically examined the Lie group analysis technique of the TFRLW equation with the Riemann-Liouville fractional derivative. Naeem et al. [39] developed numerical methodologies that use the Yang transform, the homotopy perturbation method (HPM), and the Adomian decomposition method (ADM) to analyze this equation.

    The TFRLW equation is one of the most substantial nonlinear evolution equations used to model various physical phenomena such as ion-acoustic plasma waves, shallow water waves, and longitudinal waves in elastic rods. Hossain et al. [40] used a modified simple equation integral technique in the TFRLW equation to create kink waves, anti-kink waves, brilliant and dark bell waves, double periodic waves, and combinations of solitons and periodic waves. The fractional RLW equations were used to mathematically model the nonlinear waves in the ocean, and similarly, the fractional RLW equations are used to describe the huge ocean waves known as tsunamis [41]. According to [42], the TFRLW equation can be used to study many phenomena such as plasma waves in complex media, water wave propagation in shallow water, and long-wave occupancy dynamics in the ocean, including tsunamis and tidal waves. Results in [43] can aid in understanding ion-acoustic waves in plasma, shallow water waves in oceans, and the development of a three-dimensional wave packet with finite depth on water under weak nonlinearity using the TFRLW. In [44], the authors obtained the soliton and periodic wave solutions for the TFRLW, which is the first step toward understanding ocean models' structural and physical behavior and coastal and harbor regions of the oceans. The Kudryashov approach was used to investigate the TFRLW problem in [45], which has prospective applications in applied science, nonlinear dynamics, mathematical physics, and engineering and is also important in biosciences, neurosciences, plasma physics, geochemistry, and fluid mechanics.

    The most important part of this work is that the Caputo fractional derivative is used in the RLW equation for analyzing the nature of the displacement of shallow-water waves and ion acoustic plasma waves. It takes a broad view of the RLW equation for interpretation of the water waves. In interpretation of the excessive significance of fractional derivatives, we consider a TFRLW equation emerging in ion acoustic plasma waves (1). We use the cubic CBS collocation procedure to discretize the spatial derivatives. The Caputo's definition is used for time-fractional derivative.

    αwτα+ˆγwζ+ˆβwpwζˆμ3wζ2τ=f(ζ,τ), aζb, 0<α<1, (1)

    with the initial and boundary conditions

    w(ζ,0)=ϕ(ζ), (2)
    w(a,τ)=ψ1(τ), w(b,τ)=ψ2(τ), (3)

    where p is a positive integer, ˆγ, ˆβ and dissipative term ˆμ are positive constants, w(ζ,τ) represents the vertical displacement of the water surface, and the function f(ζ,τ) denotes a source term. The notation αwτα indicates the Caputo's time-fractional derivative as

    αwτα={1Γ(1α)τ0(τυ)αw(ζ,υ)υdυ, 0<α<1w(ζ,τ)τ, α=1. (4)

    Definition 1.1. Caputo's integral and derivative of g(τ)R of order α0 are, respectively, defined by

    cJα0,τg(τ)=1Γ(α)τ0(τξ)α1g(ξ)dξ, α>0, τ>0,

    and

    cDα0,τg(τ)=1Γ(ˉkα)τ0(τξ)ˉkα1g(ˉk)(ξ)dξ, τ>0, ˉk1<α<ˉkZ+.

    This part implements the discretization process of the TFRLW equation by means of the CBS collocation procedure. First, we fix an identical partition of [0, T] with size Δτ=TN, where N is the partition's number of the time variable. Now, we discretize the fractional derivative αwτα for 0<α<1 at τ=τj+1 by the L1 formula [20,30,31] as follows:

    αwj+1iτα=a0jk=0χk(wj+1kiwjki)+ˆδj+1,j=0,1,2....N, (5)

    where a0=Δτα|¯2α, χl=(l+1)1αl1α, j=0,1,,N, and ˆδj+1 is the truncate error termed by ˆδj+1LwΔτ2α, where the constant Lw is associated to w.

    Lemma 2.1. The element χk, arising in Eq (5), fulfils the following possessions:

    {χk>0, k=0,1,...,N,1=χ0>χ1>χ2>...>χN, χN0 as N.

    Next, the CBS collocation procedure is used to discretize derivatives of the spatial variable. The domain [a, b] is apportioned consistently with h=Δζ=baM by ζi=a+ih, i=0,1,,M, such that a=ζ0<ζ1<ζ2<<ζM=b. Now, we define CBS functions Υi(x) for i=1, 0, ..., M+1 as:

    Υi(ζ)=1h3{(ζζi2)3,ζ[ζi2,ζi1)(ζζi2)34(ζζi1)3,(ζi+2ζ)34(ζi+1ζ)3,ζ[ζi1,ζi)ζ[ζi,ζi+1)(ζi+2ζ)3,ζ[ζi+1,ζi+2)0,otherwise, , (6)

    where {Υ0,Υ1,...,ΥM,ΥM+1} are preferred so that they form a basis over [a,b]. The Υi(ζ), Υi(ζ), and Υi(ζ) at knot points are valued by the subsequent table (see Table 1).

    Table 1.  The values of Υi(ζ), Υi(ζ), and Υi(ζ) at knots.
    ζi2 ζi1 ζi ζi+1 ζi+2
    Υi(ζ) 0 σ1 σ2 σ1 0
    Υi(ζ) 0 σ3 0 σ3 0
    Υi(ζ) 0 σ4 2σ4 σ4 0

     | Show Table
    DownLoad: CSV

    where σ1=1, σ2=4, σ3=1h, and σ4=6h2. We define the approximate solutions as

    w(ζ,τj)M+1i=1Υi(ζ)Ci(τj), j=0,1,,N, (7)

    where Ci(τj) are unknown extents. The variation of w(ζ,τj) is defined by

    w(ζ,τj)=i+1m=i1Υm(ζ)Cm(τj), j=0,1,,N. (8)

    Using Eq (8), we approximate w and its first-and second-order derivatives wζ and wζζ, respectively, with respect to ζ as

    wji=σ1Cji1+σ2Cji+σ1Cji+1, (9)
    (wζ)ji=σ3Cji1+σ3Cji+1, (10)

    and

    (wζζ)ji=σ4Cji12σ4Cji+σ4Cji+1. (11)

    At τ=τj+1, using the Eq (5) for αwτα and the θ scheme, we discretize problem (1) as

    a0jk=0χk(wjk+1iwjki)+θ ˆγ(wζ)j+1i+(1θ)ˆγ(wζ)ji+θ ˆβ(wpwζ)j+1i+(1θ)ˆβ(wpwζ)jiˆμ(wζζ)j+1i(wζζ)jiΔτ=fj+1i, i=0,1,...,M, j=0,1,...,N. (12)

    Now, to linearize the nonlinear term (wpwζ)j+1i, we use the Rubin-Graves procedure as:

    (wpwζ)j+1i(wp)ji(wζ)j+1i+p(wp1)ji(wζ)jiwj+1ip(wp)ji(wζ)ji+O(Δτ2), p=1,2,.... (13)

    Taking θ=12 and using Eq (13) in (12) with some manipulation, we have

    Ajiwj+1i+Bji(wζ)j+1i+D(wζζ)j+1i=Rji, i=0,1,...,M, j=1,2,...,N, (14)

    where

    Aji=a0+12ˆβp(wp1)ji(wζ)ji,Bji=12ˆγ+12ˆβ(wp)ji,D=ˆμΔτ,Rji=a0wjia0jk=1χk(wjk+1i
    wjki)12ˆγ(wζ)ji+12ˆβ p(wp)ji(wζ)ji12ˆβ(wp)ji(wζ)ji+D(wζζ)ji+fj+1i.

    Next, using the CBS collocation technique, we get

    (σ1Ajiσ3Bji+σ4D)Cj+1i1+(σ2Aji2σ4D)Cj+1i+(σ1Aji+σ3Bji+σ4D)Cj+1i+1=Rji,i=1,2,...,M1, j=1,2,...,N, (15)

    where

    Rji=a0(σ1Cji1+σ2Cji+σ1Cji+1)a0jk=1χk{(σ1Cjk+1i1+σ2Cjk+1i+σ1Cjk+1i+1)
    (σ1Cjki1+σ2Cjki+σ1Cjki+1)}12ˆγ(σ3Cji1+σ3Cji+1)+12ˆβ(σ3Cji1+σ3Cji+1)×(σ1Cji1+σ2Cji+σ1Cji+1)p(p1)+D(σ4Cji12σ4Cji+σ4Cji+1)+fj+1i.

    The Eq (15) forms a linear system with M+1 equations and M+3 unknowns. For making it uniquely solvable, we use the boundary conditions w(a,τ)=φ1(τ) and w(b,τ)=φ2(τ) as

    (σ1Cj1+σ2Cj0+σ1Cj1)=φj1(τ), (16)
    (σ1CjM1+σ2CjM+σ1CjM+1)=φj2(τ). (17)

    From Eqs (16) and (17), we have

    Cj1=σ2σ1Cj0Cj1+1σ1φj1(τ)andCjM+1=σ2σ1CjMCjM1+1σ1φj2(τ). (18)

    For i=0 and i=M, inverting the Eq (18) in (15), we get

    (σ2σ3σ1Bj0σ2σ1ˉAj0+ˉBj0)Cj+10+2σ3Bj0Cj+11=Rj01σ1(ˉAj0σ3Bj0)φj+11, j=0,1,...,N, (19)

    and

    2σ3BjMCj+1M1+(σ2σ3σ1BjMσ2σ1ˉAjM+ˉBjM)Cj+1M=RjM1σ1(ˉAjM+σ3BjM)φj+12,j=0,1,...,N, (20)

    where

    Rj0=(σ2σ3ˆγ2σ1+σ2σ3ˆβ2σ1(φji)p(p1)σ2σ4Dσ12Dσ4)Cj0+(ˆβσ3(φji)p(p1)
    ˆγσ3)Cj1a0jk=1χk{φjk+11φjk1}+(a0σ3ˆγ2σ1σ3(p1)ˆβ2σ1(φj1)p+σ4σ1)φj1+fj+10.
    RjM=(ˆγσ3(φj2)p(p1)ˆβσ3)CjM1+(σ2σ3ˆγ2σ1σ2σ3ˆβ2σ1(p1)(φj2)pσ2σ4Dσ1+
    2Dσ4)CjMa0jk=1χk(φjk+12φjk2)+(a0+σ3ˆβ(p1)2σ1(φj2)p+σ4Dσ1σ3ˆγ2σ1)φj2+fj+1M.

    Equations (19), (15) and (20) form the following system of linear equations:

    [˜Aj02σ3Bj0000˜Bj1σ3Bj1˜Dj1˜Bj1+σ3Bj1000˜Bj2σ3Bj2˜Dj2˜Bj2+σ3Bj2000˜BjM1σ3BjM1˜DjM1˜BjM1σ3BjM10002σ3BjM˜AjM][C00C01C02C0M1C0M]=[Rj01σ1(ˉAj0σ3Bj0)φj+11Rj1Rj2RjM1RjM1σ1(ˉAjM+σ3BjM)φj+12], (21)

    where ˜Aj0=σ2σ3σ1Bj0σ2σ1ˉAj0+ˉBj0, ˜Bji=σ1Aji+σ4D, ˜Dji=σ2Aji2σ4D, and ˜AjM=σ2σ3σ1BjMσ2σ1ˉAjM+ˉBjM.

    To solve the system (21), it is necessary to define the initial vector (C00,C01,...,C0M1,C0M) from w(ζ,0)=ϑ(ζ) which provides M+1 equations with M+3 unknowns. To take out C01 and C0M+1, we use wζ(a,0)=ϑζ(a) and wζ(b,0)=ϑζ(b) which gives

    C01=C01ϑζ(a)τ3andC0M+1=C0M1+ϑζ(b)τ3. (22)

    Now using Eq (22) and the initial condition, we have the subsequent system of linear equations:

    [τ22τ1000τ1τ2τ1000τ1τ2τ1000τ1τ2τ10002τ1τ2][C00C01C02C0M1C0M]=[ϑ0+(ϑζ)0τ1/τ1τ3τ3ϑ1ϑ2ϑM1ϑM(ϑζ)Mτ1/τ1τ3τ3]. (23)

    This section establishes the stability for the discretized system of the TFRLW equation using the von Neumann scheme [32]. According to Duhamels' principle [36], the stability of an inhomogeneous system is the same as the stability of the corresponding homogeneous system. Therefore, we choose f=0, and taking (wζ)p=ˆk1p as locally constant to linearize wpwζ, and θ=12, the Eq (12) can be written as

    a0wj+1i+12(ˆγ+ˆβˆk1p)(wζ)j+1iˆμΔτ(wζζ)j+1i=a0j1k=0((χkχk+1) wjki+χj w0i)12(ˆγ+ˆβˆk1p)(wζ)jiˆμΔτ(wζζ)ji, i=0,1,...,M, j=0,1,...,N. (24)

    With the help of Eqs (9)–(11), we get

    (A+E)Cj+1i1+BCj+1i+(AE)Cj+1i1=a0j1k=0(χkχk+1) (σ1Cjki1+σ2Cjki+σ1Cjki+1)+χj(σ1C0i1+σ2C0i+σ1C0i+1)+(Eσ3σ4D)Cji1+2σ4DCji+(Eσ3σ4D)Cji+1, (25)

    where A=a0σ1σ4D, B=a0σ2+2σ4D, D=ˆμΔτ, and E=12(ˆγ+ˆβˆk1p).

    Now, using the Fourier mode's growth factor Cji=ξjeliεh, where l=1, ξ is the constraint depending on time, and we have

    (2Acosεh+B2lEsinεh)ξj+1=a0j1k=0((χkχk+1) ξjk+χjξ0)(2σ1cosεh+σ2)+(2σ4D2σ4Dcosεh+2lEσ3sinεh)ξj. (26)

    Now, we define ξmax.

    Using it in the Eq (26), and by means of the property \sum\limits_{k = 0}^{j - 1} {\left( {\left( {{\chi _k} - {\chi _{k + 1}}} \right) + {\chi _j}} \right)} = 1 , we have

    |\xi {|^2} \leqslant \frac{{{S_1}}}{{{S_1} + ({S_2} - {S_1})}} , (27)

    where {S_1} = {\left( {2{a_0}{\sigma _1}\cos \varepsilon h + {a_0}{\sigma _2} + 2{\sigma _4}D - 2{\sigma _4}D\cos \varepsilon h} \right)^2} + 4{E^*}^2{\sigma _3}^2{\sin ^2}\varepsilon h , and {S_2} = \left( {2{A^*}\cos \varepsilon h + } \right. {\left. {{B^*}} \right)^2} + 4{E^*}^2{\sin ^2}\varepsilon h . Using the values {A^*}, {B^*}, D, {\text{ }}{E^*} , {\sigma _1} , {\sigma _3} , {\sigma _4} , and simplifying terms, we have

    {S_2} - {S_1} = \left( {\frac{4}{{{h^2}}}\left( {\frac{{12}}{{\left| \!{\overline {\, {2 - \alpha } \, }} \right. {\text{ }}\Delta {\tau ^{\alpha + 1}}}} - 1} \right) + 4} \right){\sin ^2}\varepsilon h \geqslant 0 . (28)

    Hence, we conclude that |\xi | \leqslant 1 . So, the discretized system of the TFRLW equation is unconditionally stable.

    This division provides an example of the TFRLW equation to investigate the efficacy and validation of the projected technique. For this purpose, we use

    {L_2} = {\left( {\sum\limits_{i = 0}^M {|W({\zeta _i}, \tau ) - w({\zeta _i}, \tau ){|^2}} } \right)^{{1 \mathord{\left/ {\vphantom {1 2}} \right. } 2}}} , {\text{ }}{L_\infty } = \mathop {\max }\limits_{0 \leqslant i \leqslant M} |W({\zeta _i}, \tau ) - w{({\zeta _i}, \tau )_j}| ,

    and approximate error = \frac{{|w({\zeta _j}, {\tau _{N + 1}}) - w({\zeta _i}, {\tau _N})|}}{{|w({\zeta _j}, {\tau _{N + 1}})|}} ,

    where W represents the exact solution. The ROC is analyzed by {\text{ROC}} = \frac{{\ln \left( {err({h_1})/err({h_2})} \right)}}{{\ln \left( {{{{h_1}} / {{h_2}}}} \right)}} , where the terms err({h_1}) and err({h_2}) represents errors with {h_1} and {h_2} , in that order. The conservation possessions belonging to the TFRLW equation are measured by calculating quantities analogous to mass, momentum, and energy, respectively, as follows:

    {I_1} = \int\limits_a^b {wd\zeta \cong h\sum\limits_{i = 0}^M {{W_i}} } , (29)
    {I_2} = \int\limits_a^b {\left( {{w^2} + \hat \mu {{\left( {{w_\zeta }} \right)}^2}} \right)d\zeta } \cong h\sum\limits_{i = 0}^M {\left( {{{\left( {{W_i}} \right)}^2} + \hat \mu {{\left( {{W_\zeta }} \right)}_i}^2} \right)} , (30)
    {I_3} = \int\limits_a^b {\left( {{w^3} + 3{{\left( {{w_\zeta }} \right)}^2}} \right)d\zeta } \cong h\sum\limits_{i = 0}^M {\left( {{{\left( {{W_i}} \right)}^3} + 3{{\left( {{W_\zeta }} \right)}_i}^2} \right)} . (31)

    Now, we consider the TFRLW equation (1) with \hat \gamma = 1 = \hat \beta = \hat \mu = p together with initial and boundary conditions w(\zeta , 0) = 3\rho \sec {h^2}(\eta \zeta ) and w(a, \tau ) = w(b, \tau ) = 0 . Here, 3\rho is the amplitude and \eta = \frac{1}{2}\sqrt {\frac{\rho }{{1 + \rho }}} . When \alpha = 1, the TFRLW equation has the subsequent single solitary wave solution w(\zeta , \tau ) = 3\rho \sec {h^2}(\eta \zeta - \varpi \tau + {\zeta _0}) , where \varpi = \frac{1}{2}\sqrt {\rho (1 + \rho )} , {\zeta _0} is an arbitrary constant, and \eta and {\varpi \mathord{\left/ {\vphantom {\varpi \eta }} \right. } \eta } represent the width and velocity, respectively. For all calculations, we have chosen {\zeta _0} = 0.

    Figure 1 signifies the estimated solution w(\zeta , \tau ) with admiration of the time \tau for several values of \rho . From this figure, it can be revealed that the estimated solution w(\zeta , \tau ) increases as the value of \rho increases. The approximate solutions with h = 0.4, \Delta \tau = 0.01, \rho = 0.03 at times \tau = 5, 7, 10 and 20 are demonstrated in Figure 2 for time-fractional orders \alpha = 0.3, 0.5, 0.7, and 0.8. The figures show the influence of the Caputo order \alpha of the fractional derivative on the evolution of the obtained solutions over time. An apparent dependence of \alpha on the solutions can be seen clearly when the time is large. Table 2 shows the approximate errors together with an ROC for \alpha = 0.9 with \rho = 0.1, h = 0.2, and \tau = 0.1 with respect to various time intervals. It can be perceived that the errors are very small and the projected method is linearly convergent with respect to the time variable. Table 3 shows the approximate errors for \alpha = 0.4 with \rho = 0.03, h = 0.2, \zeta = 2 and 4 for various time intervals at \tau = 1 while Table 4 illustrates the approximate errors with \rho = 0.1, h = 0.2 for fractional orders \alpha = 0.5, and 0.7 at times \tau = 5 and 10. It can be noticed from these tables that the approximate errors are small which confirms the accuracy of the proposed technique.

    Figure 1.  The approximate solutions comportment for distinctive values of \rho with h = 0.1, \Delta \tau = 0.01 for \alpha = 0.9 (left) and \alpha = 0.5 (right) of Example 1.
    Figure 2.  The approximate solutions with h = 0.4, \Delta \tau = 0.01, \rho = 0.03 at times (a) \tau = 5, (b) \tau = 7, (c) \tau = 10, and (d) \tau = 20 (right) for different values of fractional order \alpha for Example 1.
    Table 2.  The approximate errors for \alpha = 0.9 with \rho = 0.1, h = 0.2, and \tau = 0.1 for various time intervals.
    \Delta \tau \zeta = 2 ROC \zeta = 4 ROC
    0.05 2.08570e-04 -- 4.03268e-04 --
    0.001 1.04198e-04 1.0010 2.01542e-04 1.0006
    0.0005 5.20759e-05 1.0006 1.00746e-04 1.0004
    0.00025 2.60318e-05 1.0003 5.03664e-05 1.0002
    0.0002 2.08245e-05 1.0002 4.02919e-05 1.0001
    0.000125 1.30143e-05 1.0001 2.51814e-05 1.000
    0.00001 1.04112e-05 1.0001 2.01448e-05 1.000

     | Show Table
    DownLoad: CSV
    Table 3.  The approximate errors for \alpha = 0.4 with \rho = 0.03, h = 0.2, and \tau = 1 for various time intervals.
    \Delta \tau \zeta = 2 ROC \zeta = 4 ROC
    0.05 3.126e-05 -- 7.786e-04 --
    0.025 1.181e-05 1.40 3.791e-04 1.04
    0.0125 5.020e-06 1.23 1.870e-04 1.02
    0.01 3.879e-06 1.56 1.493e-04 1.01
    0.008 3.017e-06 1.13 1.192e-04 1.01
    0.00625 2.299e-06 1.10 9.295e-05 1.01

     | Show Table
    DownLoad: CSV
    Table 4.  The approximate errors with \rho = 0.1, h = 0.2, and \tau = 10 at \zeta = 4 for various time intervals.
    \Delta \tau \alpha = 0.5, \tau = 5 \alpha = 0.5, \tau = 10 \alpha = 0.7, \tau = 5 \alpha = 0.7, \tau = 10
    0.05 3.0576e-04 5.9194e-04 1.1811e-03 2.0957e-03
    0.025 1.5319e-04 2.9497e-04 5.9586e-04 1.0434e-03
    0.0125 7.6638e-05 1.4723e-04 2.9914e-04 5.2055e-04
    0.01 6.1314e-05 1.1775e-04 2.3950e-04 4.1626e-04
    0.008 4.9054e-05 9.4173e-05 1.9171e-04 3.3289e-04
    0.001 3.0660e-05 5.8834e-05 1.1992e-04 2.0794e-04

     | Show Table
    DownLoad: CSV

    Table 5 shows the ROC with respect to the space variable including errors in invariants for \alpha = 1 with \rho = 0.1, \Delta \tau = 0.01 at \tau = 1. It can be noticed from this table that the projected method is second-order convergent in space as well as that the small difference among the numerical and analytical values of {I_1} , {I_2} , and {I_3} that extends in the invariants remains almost inconsistent for the duration of the computer run.

    Table 5.  The order of convergence including errors on invariants for \alpha = 1 with \rho = 0.1, \Delta \tau = 0.01, at \tau = 1.
    h {L_2} ROC {L_\infty } ROC \Delta {I_1} \Delta {I_2} \Delta {I_3}
    0.8 1.232e-04 -- 5.282e-05 -- 1.324e-05 4.253e-07 1.982e-09
    0.5 4.675e-05 2.06 2.023e-05 2.04 1.358e-05 3.550e-08 1.253e-10
    0.4 2.976e-05 2.02 1.295e-05 2.00 1.369e-05 3.645e-09 3.864e-11
    0.25 1.166e-05 1.99 5.050e-06 2.00 1.389e-05 5.448e-09 2.081e-12
    0.2 7.558e-06 1.94 3.235e-06 1.99 1.389e-05 5.448e-09 2.081e-12
    0.125 3.290e-06 1.77 1.725e-06 1.34 1.397e-05 2.662e-09 1.059e-12

     | Show Table
    DownLoad: CSV

    Table 6 demonstrates a comparison between the projected method and those available in refs. [18,19,33,34] in terms of {L_2} and {L_\infty } errors. The values of the single solitary wave's invariants are also compared for \alpha = 1 with \rho = 0.1, h = 0.125, \Delta \tau = 0.1, and \zeta \in {\text{ }}[ - 40, 60] at various times. It is observed from Table 6 that the magnitudes in the invariants keep almost insistent in the course of the computer run. At \tau = 16, the difference among the numerical and analytical values of the conservation constants are \Delta {I_1} = 4.815941e-05, \Delta {I_2} = 1.856193e-06, \Delta {I_3} = 2.651635e-08. It is obvious from the table that the {L_\infty } error norms at each time achieved by the projected method are much lower than those given in refs. [18,19,33,34], However, the {L_2} error norm is only higher than in [18] and is lower than the others. Also, the {L_2} and {L_\infty } errors in [33] are slightly smaller than those achieved by the projected method.

    Table 6.  Invariants with {L_2} and {L_\infty } errors for the single solitary wave for \alpha = 1 with \rho = 0.1, h = 0.125, \Delta \tau = 0.1, \zeta \in {\text{ }}[ - 40, 60] at various times.
    Time Methods {L_2} {L_\infty } {I_1} {I_2} {I_3}
    \tau = 4 Present 5.279e-05 2.118e-05 3.979955 0.810463 2.579007
    Ref. [33] 4.8e-05 1.9e-05 3.97993 0.810465 2.57901
    Ref. [19] 1.09e-03 4.87e-04 3.98041 0.810111 2.57785
    Ref. [18] 1.00e-05 1.46e-04 3.97709 0.809641 2.57630
    Ref. [34] 1.16e-04 5.4e-05 3.98039 0.810610 2.57950
    \tau = 8 Present 1.05e-04 4.252e-05 3.979976 0.810463 2.579007
    Ref. [33] 9.4e-05 3.8e-05 3.97993 0.810465 2.57901
    Ref. [19] 2.109e-03 8.92e-04 3.98085 0.809749 2.57666
    Ref. [18] 3.0e-06 5.79e-04 3.97332 0.808320 2.57194
    Ref. [34] 2.24e-04 1.00e-04 3.98083 0.810752 2.57996
    \tau =12 Present 1.5395e-04 6.216e-05 3.9799927 0.810463 2.579007
    Ref. [33] 1.38e-04 5.6e-05 3.97992 0.810465 2.57901
    Ref. [19] 3.049e-03 1.224e-03 3.98128 0.809390 2.57547
    Ref. [18] 6.0e-06 9.22e-04 3.97911 0.806774 2.56684
    Ref. [34] 3.25e-04 1.39e-04 3.98125 0.810884 2.58041
    \tau =16 Present 2.012e-04 7.994e-05 3.979997 0.810464 2.579007
    Ref. [33] 1.80e-04 7.1e-05 3.97991 0.810465 2.57901
    Ref. [19] 3.905e-03 1.510e-03 3.98169 0.809030 2.57428
    Ref. [18] 1.2e-05 1.215e-03 3.96534 0.805461 2.56251
    Ref. [34] 4.17e-04 1.71e-04 3.98165 0.811014 2.58083

     | Show Table
    DownLoad: CSV

    Table 7 compares the projected method and existing methods refs. [19,23,33,34,37] in terms of {L_2} and {L_\infty } errors as well as invariants for \alpha = 1 with \rho = 0.1, h = 0.125, \Delta \tau = 0.1, and \zeta \in [ - 40, 60] at time \tau = 20. It can be perceived from this table that the {L_2} and {L_\infty } error norms achieved by the projected method are very much smaller than those obtained in [19,23,33,34,37], whereas, the errors obtained by the QBGM1 are almost similar to the projected method. The magnitudes in the invariants keep on nearly consistent in the course of the computer run. It is found that the difference among the numerical and analytical values of {I_1} , {I_2} , and {I_3} are \Delta {I_1} = 2.496862e-05, \Delta {I_2} = 2.642822e-06, and \Delta {I_3} = 3.886086e-08. Table 8 compares the invariants obtained by the projected method with ref. [37] and analytical quantities for \alpha = 0.5 with \rho = 0.03, h = 0.1, \Delta \tau = 0.0001 at various times \tau . It can be remarked from this table that the obtained invariant quantities are very close to analytical values and are much better than what is presented in ref. [37]. Table 9 shows the absolute errors in the invariants obtained by the projected method and analytical quantities for \alpha = 0.6 with \rho = 0.03, h = 0.2, \Delta \tau = 0.001 at various times \tau . It can be seen that the invariant quantities are nearly {10^{ - 3}} accurate.

    Table 7.  The comparison of {L_2} and {L_\infty } errors and invariants obtained by the projected method and existing methods for \alpha = 1 with \rho = 0.1, h = 0.125, \Delta \tau = 0.1, \zeta \in {\text{ }}[ - 40, 60] at \tau = 20.
    Methods {L_2} {L_\infty } {I_1} {I_2} {I_3}
    Present 2.4627e-04 9.6078e-05 3.979975 0.810465 2.579007
    Ref. [19] 4.688e-03 1.755e-03 3.98203 0.808650 2.57302
    Ref. [37] 2.20e-04 8.60e-05 3.97989 0.810467 2.57902
    Ref. [33] 2.19e-04 8.60e-05 3.97988 0.810465 2.57901
    QBGM1 (Ref. [23]) 1.9215e-04 7.337e-05 3.9798832 0.8104612 2.5790031
    QBGM2 (Ref. [23]) 3.5489e-04 1.2848e-04 3.9798830 0.8104616 2.5790043
    Ref. [34] 5.11e-04 1.98e-04 3.98206 0.811164 2.58133

     | Show Table
    DownLoad: CSV
    Table 8.  The comparison of invariants obtained by the projected method with ref. [37] and analytical quantities for \alpha = 0.5 with \rho = 0.03, h = 0.1, \Delta \tau = 0.0001 at various times \tau .
    \tau Methods {I_1} {I_2} {I_3}
    0.01 Present 2.104795105493023 0.127311100687075 0.388792279082409
    Exact values 2.109407499749634 0.127301718625667 0.388805990353852
    Ref. [37] 0.197709389335031 0.126849748687847 0.387166785333068
    0.02 Present 2.104793676163467 0.127306603010193 0.388778144598822
    Exact values 2.109407499749634 0.127301718625667 0.388805990353852
    Ref. [37] 0.197709389335031 0.126832805997773 0.387113999130940
    0.03 Present 2.104792339908470 0.127301823129927 0.388763112448558
    Exact values 2.109407499749634 0.127301718625667 0.388805990353852
    Ref. [37] 0.197705310408835 0.126802946718958 0.387058367254051
    0.04 Present 2.104791052954834 0.127296885458673 0.388747577127724
    Exact values 2.109407499749634 0.127301718625667 0.388805990353852
    Ref. [37] 0.197698761277219 0.126780218019371 0.387001260827619
    0.05 Present 2.104789799868593 0.127291842792910 0.388731706486992
    Exact values 2.109407499749634 0.127301718625667 0.388805990353852
    Ref. [37] 0.197690652584066 0.126757804752181 0.386943215828569

     | Show Table
    DownLoad: CSV
    Table 9.  The absolute errors in invariants obtained by the projected method and analytical quantities for \alpha = 0.6 with \rho = 0.03, h = 0.2, \Delta \tau = 0.001 at various times \tau .
    \tau {I_1} {I_2} {I_3}
    0.01 4.750272418178e-03 3.379346449474130e-04 1.087110202561e-03
    0.02 4.755032046523e-03 3.758097931880755e-04 1.206502603342e-03
    0.03 4.756680570585e-03 3.896019672482709e-04 1.249979299056e-03
    0.04 4.757509362131e-03 3.967863361757640e-04 1.272626452249e-03
    0.05 4.758004486260e-03 4.012071170268194e-04 1.286562027427e-03

     | Show Table
    DownLoad: CSV

    Figure 3 demonstrates the plots of the estimate solution w(\zeta , \tau ) contrasted with spatial as well as time variables \zeta and \tau , respectively, for the values of \alpha = 0.5 and \alpha = 0.75 showing that the appearances of this figure are stable with ref. [35] (Figures 2 and 3). Figure 4 illustrates the approximate errors for \alpha = 0.5 with \rho = 0.1, h = 0.1 for various time interval sizes \Delta \tau at \tau = 0.1. It can be seen from this figure that the approximate errors are decreasing on increasing \Delta \tau . Also, it is observed that the approximate errors are less than {10^{ - 5}} which shows the accuracy of the projected method. The 3D plot of the approximate errors for \alpha = 0.9 with \rho = 0.1, h = 0.2, \Delta \tau = 0.001, and \tau \in [0, 0.1] is depicted in Figure 5. The depiction of single solitary wave solutions with absolute errors by assuming \alpha = 1, h = 0.3, \Delta \tau = 0.1 for \rho = 0.1 and \rho = 0.03 at \tau = 1 is described in Figure 6.

    Figure 3.  The surface behaviors of the numerical w(\zeta , \tau ) for \alpha = 0.5 (left), and \alpha = 0.75 (right) with \rho = 0.3, h = 0.2, \tau \in [0, 0.1] , and \Delta \tau = 0.01 for Example 1.
    Figure 4.  The approximate errors for \alpha = 0.5 with \rho = 0.1, h = 0.1 for various \Delta \tau at \tau = 0.1.
    Figure 5.  The 3D plot of the approximate errors for \alpha = 0.9 with \rho = 0.1, h = 0.2, \Delta \tau = 0.001, and \tau \in [0, 0.1] .
    Figure 6.  The single solitary wave solutions' performance with absolute errors with \alpha = 1, h = 0.3, \Delta \tau = 0.1 for \rho = 0.1 (up) and \rho = 0.03 (down) at \tau = 1 .

    The traveling-wave solutions are obtained for the TFRLW equation via a CBS collocation technique. The spatial derivatives are discretized by the aforesaid technique while the time-fractional derivative is discretized through Caputo's definition. The nonlinear term is commenced by the Rubin-Graves linearization procedure. The von-Neumann analysis confirms that the discretized structure of the TFRLW equation is enthusiastically stable. It is also established that the technique is second-order convergent in the spatial variable while linearly convergent in time. Three invariant capacities corresponding to mass, momentum, and energy are assessed for further justification. It is demonstrated that these invariants remain almost inconsistent for the duration of the computer run, and absolute errors are very small, approximately \approx {10^{ - 8}} to {10^{ - 5}} . It is also observed that the obtained results by the projected technique are much better than the existing ones in [18,19,23,33,34,37].

    All authors of this article have been contributed equally. All authors have read and approved the final version of the manuscript for publication.

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

    The authors gratefully acknowledge the funding of the Deanship of Graduate Studies and Scientific Research, Jazan University, Saudi Arabia, through project number RG24-S011.

    There is no competing interest among the authors regarding the publication of the article.



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