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Pseudospectral method for fourth-order fractional Sturm-Liouville problems

  • Fourth-order fractional Sturm-Liouville problems are studied in this work. The numerical simulation uses the pseudospectral method, utilizing Chebyshev cardinal polynomials. The presented algorithm is implemented after converting the desired equation into an associated integral equation and gives us a linear system of algebraic equations. Then, we can find the eigenvalues by calculating the roots of the corresponding characteristic polynomial. What is most striking is that the proposed scheme accurately solves this type of equation. Numerical experiments confirm this claim.

    Citation: Haifa Bin Jebreen, Beatriz Hernández-Jiménez. Pseudospectral method for fourth-order fractional Sturm-Liouville problems[J]. AIMS Mathematics, 2024, 9(9): 26077-26091. doi: 10.3934/math.20241274

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  • Fourth-order fractional Sturm-Liouville problems are studied in this work. The numerical simulation uses the pseudospectral method, utilizing Chebyshev cardinal polynomials. The presented algorithm is implemented after converting the desired equation into an associated integral equation and gives us a linear system of algebraic equations. Then, we can find the eigenvalues by calculating the roots of the corresponding characteristic polynomial. What is most striking is that the proposed scheme accurately solves this type of equation. Numerical experiments confirm this claim.



    The Sturm-Liouville problems with integer derivatives have been a significant field of research for centuries, due to their importance in science, engineering, and mathematics [3]. This equation has many applications in various fields of science and engineering, including sea-breeze flow [23], unidirectional pressure-driven flow of a second-grade fluid in a plane channel with impermeable solid walls [10], and flow of the antarctic circumpolar current in rotating spherical coordinates [24]. It is crucial to determine both the eigenvalues and the corresponding eigenfunctions for this equation, as they play a very significant role in theory and applications. It is often difficult, if not impossible, to accurately determine the eigenvalue. Numerical methods can be extremely useful to achieve this objective, including boundary value methods [18], Legendre-Galerkin-Chebyshev collocation method [15], Numerov's method [5], the Chebyshev collocation method [36], etc.

    When dealing with a fourth-order Sturm-Liouville equation, implementing four boundary conditions makes the problem more complex. Dealing with two boundary conditions at each end of the computational domain can be a challenging problem in certain applications. For instance, an eigenvalue problem of a fourth-order differential equation is derived by analyzing the free lateral vibration of a homogeneous beam using the Euler-Bernoulli beam theory [35]. A fourth-order Sturm-Liouville equation is generally considered as

    (p(t)w)=G(t,w,w,w,λ)=(q(t)y)+(λr(t)w(t))w,t[a,b],

    appropriate boundary conditions on w, w, pw or/and (pw)qy. Here, p(t), q(t), r(t) and w(t) are piecewise continuous functions, and p(t),r(t)0 [8].

    Several numerical solutions have been found for calculating eigenvalues of fourth-order Sturm-Liouville problems, including the extend sampling method [12], the Adomian decomposition method [8], the Boubaker polynomial expansion scheme [37], variational iteration methods [31], the Haar wavelet method [34].

    Fractional calculus, which generalizes the derivative of a function to non-integer order, has remained a mystery to mathematicians for 300 years. The branch's origin dates back to a 1695 letter from Leibniz to L'Hospital. It was reported in the nineteenth century that some theoretical work was related to fractional calculus. In recent decades, there has been an increasing interest in fractional calculus due to its applications in various fields of physics and engineering. For comprehensive reviews, refer to Podlubny [29], Oldham and Spanier [28], and Miller and Ross [27]. Fractional differential equations arise in various physical phenomena, including mathematical biology, fluid mechanics, electrochemistry, and viscoelasticity [6,13,25,26]. Several analytical and numerical methods have been implemented and developed in recent years to solve the fractional differential equation, such as the multiwavelet Galerkin method [7,33], Adomian decomposition [16], the Kuratowski MNC technique [9], the B-spline collocation method [22], least-squares finite element [17], etc.

    The objective of this paper is to present a simple and accurate method, based on the pseudospectral method, to find the eigenvalues of

    cDμ40(w)(t)+3i=1qi(t)cDμi0(w)(t)+q0(t)w(t)=λr(t)w(t), (1.1)

    with the boundary conditions

    3j=0sk,jDj(w)(0)=0,k=0,1,,S1,3j=0sk,jDj(w)(1)=0,k=S,,3, (1.2)

    where sk,j for k,j=0,1,,3 are given real constants, qi(t), i=1,,3, and r(t) are in L1[0,1], and μi for i=1,,4 are real numbers such that μi(i1,i]. The constant S indicates the number of conditions in point 0. D and cDμ0 indicate the derivative operator and the Caputo fractional derivative, respectively. In this problem, λ is called an eigenvalue.

    It is important to note that fractional Sturm-Liouville problems (1.1)-(2.13) arise frequently when dealing with separable linear fractional partial differential equations [4]. In [19], the authors utilized the series solution to solve this equation. This is the first report on fourth-order fractional Sturm-Liouville problems with varying coefficients. The presented work can be considered the second paper in this field, which solves the problem with a simpler method and more accurately.

    The rest of the paper is structured in the following manner: Chebyshev Cardinal polynomials and their properties are reviewed and introduced in Section 2. In Section 3, the pseudospectral method is applied to solve fourth-order fractional Sturm-Liouville problems using Chebyshev cardinal polynomials. Section 4 is dedicated to illustrate the applicability and accuracy of the method. To sum up our work, we have included a conclusion in Section 5.

    Given N0. Let R:={rj:TN+1(rj)=0,jN} be the set of the roots of the TChebyshev polynomial TN+1 in which N:={1,2,,N+1}. Recall that the TChebyshev polynomials are defined on [1,1] by

    TN+1(cos(θ))=cos((N+1)θ),N=0,1,,

    and their roots are specified by

    rj:=cos((2j1)π2N+2),jN. (2.1)

    Shifted TChebyshev polynomials for generic intervals [a,b] are related to the TChebyshev polynomials by

    TN+1(t):=TN+1(2(ta)ba1), (2.2)

    and the roots of TN+1 in its turn are obtained by tj=(rj+1)(ba)2+a, jN.

    The Chebyshev cardinal function (CCF) is one of the orthogonal polynomials' most notable cardinal functions [1,11,32]. Considering TN+1,t(tj) as the derivative of function TN+1(t) with respect to the variable t, Chebyshev cardinal functions can be denoted by

    ψj(t)=TN+1(t)TN+1,t(tj)(ttj),jN. (2.3)

    The most striking feature of these polynomials is their cardinality, i.e.,

    ψj(ti)=δji, (2.4)

    in which δji indicates the Kronecker delta. This property is mostly important as it enables us to approximate any function wHα([a,b]) (the Sobolev space Hα([a,b]) will be briefly introduced) easily and without integration in finding the coefficients, viz,

    w(t)N+1j=1w(tj)ψj(t):=wN(t). (2.5)

    In what follows, since we will need the definition of Sobolev spaces and their norm, we will provide a brief definition of it. For αN, we denote by Hα([a,b]) the sobolev space of functions w(t) which have continuous derivatives up to order α such that DβwL2([a,b]):

    Hα([a,b])={wCα([a,b]):DβwL2([a,b]),Nβα},

    with the norm

    w2Hα([a,b])=αj=0w(j)(t)2L2([a,b]), (2.6)

    and the semi-norm

    |f|2Hα,N([a,b])=Nj=min{α,N}w(j)(t)2L2([a,b]). (2.7)

    Lemma 2.1. (cf [14]) Given N0, the error of approximation (2.5), obtained using the shifted Chebyshev nodes {tj}jN, can be bounded

    wwNL2([a,b])CNα|w|Hα,N([a,b]), (2.8)

    where the constant C is independent of N. Furthermore, it can be verified that

    wwNHl([a,b])CN2l1/2α|w|Hα,N([a,b]),α1,1lα. (2.9)

    Let Ψ(t) be a vector function with entries {ψj}jN. We specify the operational matrix of derivatives for CCFs as

    D(Ψ)(t)=DΨ(t). (2.10)

    To evaluate the elements of D, they can be obtained via the following process using the approximation (2.5). It follows from (2.5) that

    Dj,i=D(ψj)(ti). (2.11)

    It is worth noting that there is another presentation of CCFs [2]

    ψj(t)=ϱN+1κ=1,κj(ttκ), (2.12)

    where ϱ=22N+1/((ba)N+1TN+1,t(tj)). When the operator D acts on both sides of (2.12) and taking into account (2.3), we obtain

    D(ψj)(t)=ϱN+1κ=1κjD(ttκ)=ϱN+1k=1kjN+1κ=1κj,k(ttκ)=N+1k=1kjTN+1(t)(ttj)(ttk)TN+1,t(tj)=N+1k=1kj1(ttk)ψj(t). (2.13)

    It can be shown by (2.11) and (2.13) that

    D(ψj)(ti)={N+1k=1kj1(titk),j=i,ϱN+1k=1kj,i(titk),ji.

    Considering the interval [0,1], the fractional integral is defined as

    Iμ0(w)(t):=1Γ(μ)t0(tζ)μ1w(ζ)dζ,t[0,1],μR+, (2.14)

    where Γ(μ) denotes the Gamma function.

    Note that there is a square matrix Iμ such that the acting of the fractional integral operator on Ψ(x) can be represented by it, viz,

    Iμ0(Ψ(t))IμΨ(t),t(0,1). (2.15)

    It is straightforward to show that the elements of this matrix can be obtained by

    (Iμ)j,i=Iμ0(ψj(ti)). (2.16)

    After performing some simple calculations, it can be inferred from [30] that

    N+1κ=1κj(ttκ)=Nκ=0ωj,κtNκ, (2.17)

    in which

    ωj,0=1,ωj,κ=1κκk=0χj,kωj,κk, j=1,,N+1,κ=1,,N,

    and

    χj,k=N+1i=1ijtki, j=1,,N+1,k=1,,N.

    Motivated by (2.12), the CCFs can be determined by

    ψj(t)=ϱNκ=0ωj,κtNκ. (2.18)

    Using this definition of CCFs, (2.16) leads to

    Iμ0(ψj(t))=ϱIμ0(Nκ=0ωj,κtNκ)=ϱNκ=0ωj,κIμ0(tNκ)=ϱNκ=0ωj,κΓ(Nκ+1)Γ(Nκ+μ+1)tNκ+μ.

    So it can be concluded from (2.16) that

    (Iμ)j,i=Iμ0(ψj(ti))=ϱNκ=0ωj,κΓ(Nκ+1)Γ(Nκ+μ+1)tNκ+μi. (2.19)

    Definition 2.1. [21] Let μR+ and m:=μN (. denotes the ceiling function). The Caputo fractional derivative is denoted by

    cDμ0(w)(t):=1Γ(mμ)t0f(m)(ζ)dζ(tζ)μm+1=:Imμ0Dm(w)(t), (2.20)

    where Dm:=dmdtm.

    Lemma 2.2. [21, cf Corollary 2.3(a)] Let μR+, m:=μN and μN0. Then we have

    cDμ0(w)C1Γ(mμ)(mμ+1)wCm. (2.21)

    Taking into account Definition 2.1 and the operational matrices of derivative D and fractional integral Iμ, when the Caputo derivative operator acts on Ψ(x), it follows that

    cDμ0(Ψ)(t)=Imμ0Dm(Ψ(t))Dm(Imμ)Ψ(t). (2.22)

    So, the operational matrix for the Caputo operator is specified by

    Dμ=Dm(Imμ). (2.23)

    The present chapter will be focused on solving fourth-order fractional Sturm-Liouville equations (SLEs) with the Caputo operator using an efficient and accurate scheme based on the pseudospectral method. As mentioned above, we consider the fourth-order fractional Sturm-Liouville equation (SLE)

    cDμ40(w)(t)+3i=1qi(t)cDμi0(w)(t)+q0(t)w(t)=λr(t)w(t), (3.1)

    equipped with the boundary conditions

    3j=0sk,jDj(w)(0)=0,k=0,1,,S1,3j=0sk,jDj(w)(1)=0,k=S,,3, (3.2)

    where sk,j for k,j=0,1,,3 are given real constants, qi(t), i=1,,3, and r(t) are in L1[0,1], and μi for i=1,,4 are real numbers such that μi(i1,i]. The constant S indicates the number of conditions in point 0. In this problem, λ is called an eigenvalue and is not given in advance. Our objective while solving the Sturm-Liouville equation is to determine the eigenvalues.

    One of the common schemes that is used to solve a differential equation is based on converting it to an integral equation. To give rise to such a conversion for Eq (3.1)-(3.2), we reformulate it as

    w(t)3i=0w(i)(0)i!(t)i+Iμ40(3i=1qicDμi0(w)+q0wλrw)(t)=0. (3.3)

    Equation (3.3) is written due to the following formula [21]:

    Iμ0cDμ0(w)(t)=w(t)μ1i=0w(i)(0)i!(t)i.

    In this equation, we either have the values of the w(t) function and its derivatives at zero or assume them as unknowns and add them to our unknowns.

    Pseudospectral scheme

    To obtain the pseudospectral discretization of Eq (3.3), the unknown solution w is approximated using Chebyshev cardinal polynomials as

    w(t)N+1j=1wjψj(t)=WTΨ(t):=wN(t), (3.4)

    where the (N+1)-dimensional vector W consists of the unknowns (wj)N+1j=1. Substituting wN instead of w in (3.3), we have

    wN(t)ˉw(t)+Iμ40(3i=1qicDμi0(wN)+q0wNλrwN)(t)=0, (3.5)

    in which ˉw(t)=3i=0w(i)(0)i!(t)i. Now, we approximate all terms in (3.4) as follows:

    ● Using the Chebyshev cardinal polynomials, ˉw can be approximated as

    ˉw(t)N+1j=1ˉw(tj)ψj(t)=ˉWTΨ(t), (3.6)

    where ˉW is a (N+1)-dimensional vector whose elements may be known or unknown according to the boundary conditions.

    ● Let us put gi(t):=cDμi0(wN)(t), i=1:3. Taking into account the operational matrices of derivative or the operational matrix for the Caputo operator, we obtain

    gi(t)WTDμiΨ(t):=˜gi(t),i=1,,3. (3.7)

    By approximating qi(t)˜gi(t) using CCFs, one can write

    qi(t)˜gi(t)QTiΨ(t),i=1,,3, (3.8)

    where Qi is a (N+1)-dimensional vector whose elements consist of unknowns wj, j=1,,N+1. Finally, taking the fractional integral from both sides of (3.8) and taking into account the operational matrix of the fractional integral, we obtain

    Iμ40(qicDμi0(wN))(t)QTiIμ4Ψ(t)=WTGiIμ4Ψ(t),i=1,,3, (3.9)

    in which Gi is an (N+1)-dimensional matrix with constant entries.

    ● Putting g0:=q0wN and then approximating it using CCFs leads to

    g0(t)QT0Ψ(t)=WTG0Ψ(t), (3.10)

    in which Q0 is a (N+1)-dimensional vector whose elements consist of unknowns wj, j=1,,N+1, and G0 is an (N+1)-dimensional matrix with constant entries. Taking the fractional integral from both sides of (3.10) and motivated by the operational matrix of the fractional integral, it is easy to achieve

    Iμ40(q0wN)(t)WTG0Iμ4Ψ(t). (3.11)

    ● Similar to the previous one, the term Iμ40(rwN)(t) can be approximated by

    Iμ40(rwN)(t)WT˜GIμ4Ψ(t), (3.12)

    where ˜G is an (N+1)-dimensional matrix with constant entries.

    Let us consider G:=3i=0Gi. By this assumption, the residual function can be determined by

    r(t):=(WT(I+G+λ˜G)Iμ4ˉWT)Ψ(t). (3.13)

    Our goal is to make r(t) as close to zero as possible. By utilizing the shifted Chebyshev nodes {tj}jN and taking into account Eq (2.4), the pseudospectral method results in

    WT(I+G+λ˜G)Iμ4=ˉWT. (3.14)

    Setting ΥT:=(I+G+λ˜G)Iμ4, we have

    WTΥTˉWT=0, (3.15)

    or equivalently, we have

    ΥWˉW=0. (3.16)

    To determine the ˉw function, 4s unknowns are undetermined. So, (3.16) consists of N+1 equations with N+5s unknowns. We add 4s equations to this system of equations according to the boundary conditions (3.2), and then we obtain a new system

    A(λ)ˆW=0, (3.17)

    in which ˆW consists of all unknowns, including wj, j=1,,N+1, and 4s unknowns of function ˉw. Also, A(λ) is a matrix whose elements are functions of λ. In order for Eq (3.17) to have a non-zero eigenvector, it is necessary that the matrix A(λ) is singular when λ is an eigenvalue. Equivalently, we have

    det(A(λ))=0. (3.18)

    Note that det(A(λ)) refers to the characteristic polynomial, and λ represents its root. To calculate the roots, the Maple software can be used.

    It is worth realizing that the eigenvector ˆW associated with λ belongs to

    ker(A(λ))={ˆW(CN+5s or RN+5s):A(λ)ˆW=0}. (3.19)

    Since ˆW must be nonzero, the matrix A(λ) has a nonzero kernel. On the other hand, since we obtain the eigenvalues approximately, the characteristic polynomial det(A(λ)) does not become exactly zero in these eigenvalues. Still, it will have a value very close to zero. To find the eigenvector we are looking for, we need to identify the eigenvalue of A(λ) that is the smallest and then select the eigenvector corresponding to that eigenvalue. Finally, we obtain the eigenvector corresponding to the eigenvalue λ, via

    wN(t)=N+1j=1(ˆW)jψj(t)/N+1j=1(ˆW)jψj(t). (3.20)

    Example 4.1. As the first illustrative example, the fourth-order fractional SLE is considered

    cDμ0(w)(t)=λw(t),t[0,1], μ(3,4],

    with conditions

    w(0)=w(0)=w(1)=w(1)=0.

    The exact eigenvalues can be calculated by λl=(lπ)4 [19,20] for μ=4.

    Table 1 is tabulated to demonstrate the approximation of the first three eigenvalues for different values of μ when the value of N is fixed. As we vary μ from 3.7 to 4, we aim to verify that the eigenvalues approach the eigenvalues for μ=4 when μ values approach the exact ones for 4. What is important is that eigenvalues approach the exact ones, when μ tends to 4.

    Table 1.  Approximation of the first three eigenvalues for different values of μ, taking N=14, for Example 4.1.
    Proposed method Exact λl=(lπ)4 |λexactλapp|
    λl μ=3.7 μ=3.9 μ=3.9999 μ=4 μ=4 μ=4
    1 91.412589 93.533296 97.404401 97.409091 97.409091 6.788699×1014
    2 944.783464 1324.152539 1558.289749 1558.545458 1558.545457 1.110047×106
    3 4543.822643 6455.773848 7888.357324 7890.136319 7890.136374 5.477432×105

     | Show Table
    DownLoad: CSV

    Table 2 illustrates the convergence of the method. To this end, we simulate the method for different values of N when the μ value is fixed. Motivated by this, we can deduce that the presented scheme is accurate.

    Table 2.  The approximate values of the first 3 eigenvalues of Example 4.1.
    N 8 10 12 14
    μ=3.7 λ1 91.377000 91.416368 91.413186 91.412589
    λ2 953.287633 944.426910 944.756238 944.783464
    λ3 15055.665758 4386.905998 4558.717081 4543.822643
    μ=4 λ1 97.409088 97.409091 97.409091 97.409091
    λ2 1558.316284 1558.550994 1558.545364 1558.545458
    λ3 7894.315144 7890.054147 7890.138950 7890.136319

     | Show Table
    DownLoad: CSV

    For more illustration, the approximate eigenfunctions corresponding to the first 3 eigenvalues are plotted in Figure 1. This figure shows that for each eigenvalue λl, the corresponding eigenfunction wl has l1 zeros.

    Figure 1.  The approximate eigenfunctions corresponding to the first 3 eigenvalues for Example 4.1.

    Example 4.2. For the second example, the fourth-order fractional Sturm-Liouville equation

    cDμ0w(t)0.02x2w(t)0.04xw(t)+(0.0001x40.02)w(t)=λw(t),t[0,5],

    with conditions

    w(0)=w(0)=w(5)=w(5)=0,

    is considered [20,37].

    Table 3 presents the numerical results for the first three eigenvalues. In this table, we can find the results of the differential quadrature method [37] and the polynomial expansion and integral technique [20] with the presented technique results and compare them.

    Table 3.  Approximation of the first three eigenvalues for different values of μ, taking N=14, for Example 4.2.
    Proposed method [20] [37]
    λl μ=3.7 μ=3.9 μ=3.99 μ=4 μ=4(N=18) μ=4(N=18)
    1 0.333934329 0.245006699 0.217754219 0.215050864 0.215050864 0.215050864
    2 2.737183568 2.763022355 2.755635985 2.754809934 2.754809934 2.754809934
    3 12.50376002 12.75075971 13.16177525 13.21535154 13.21535154 13.21535154

     | Show Table
    DownLoad: CSV

    Table 4 illustrates the convergence of the method. To this end, we simulate the method for different values of N when the μ value is fixed.

    Table 4.  The approximate values of the first 3 eigenvalues of Example 4.2.
    N 10 12 14 16 18
    μ=4 λ1 0.215050831 0.215050864 0.21505086436957 0.21505086436978 0.21505086436971
    λ2 2.754825011 2.754809613 2.75480993456002 2.75480993461635 2.75480993468371
    λ3 13.21563660 13.21533073 13.2153515442156 13.2153515095064 13.2153515413336

     | Show Table
    DownLoad: CSV

    Finally, for more illustration, the approximate eigenfunctions corresponding to the first 3 eigenvalues are plotted in Figure 2. This figure shows that for each eigenvalue λl, the corresponding eigenfunction wl has l1 zeros.

    Figure 2.  The approximate eigenfunctions corresponding to the first 3 eigenvalues for Example 4.2.

    The Sturm-Liouville problem is a significant ordinary differential equation with numerous applications in various fields of science. Thus, solving it and obtaining its eigenvalues and eigenfunctions can be an intriguing task. In this study, we propose a method for solving the fourth-order fractional Sturm-Liouville equation using Chebyshev cardinal polynomials and the pseudospectral method, which is highly efficient. This field has only seen a few numerical methods to solve this type of equation. This paper is the second of its kind. The numerical examples that have been solved confirm the accuracy and efficiency of the method used.

    According to the experimental observations, the following can be concluded:

    (1) The proposed schemes are effective for solving these types of equations.

    (2) The eigenvalues approach the exact ones when μ tends to 4.

    (3) The presented method is convergent.

    (4) The abilities of the presented method are simplicity, high accuracy, and reduction of computational cost by avoiding integration in finding coefficients.

    In the future, we plan to extend our numerical approaches for solving higher-order fractional Sturm-Liouville equations and fractional Dirac equations.

    Haifa Bin Jebreen: Conceptualization, Methodology, Software, Validation, Formal analysis, Investigation, Writing–original draft, Writing–review & editing, Funding acquisition; Beatriz Hernández-Jiménez: Formal analysis, Invesigation, Software, Validation, Investigation, Writing–original draft, Writing–review & editing. All authors have read and agreed to the published version of the manuscript.

    This project was supported by Researchers Supporting Project number (RSP2024R210), King Saud University, Riyadh, Saudi Arabia.

    The authors declare that they have no conflicts of interest.



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