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The orthogonal polynomials method using Gegenbauer polynomials to solve mixed integral equations with a Carleman kernel

  • The orthogonal polynomials approach with Gegenbauer polynomials is an effective tool for analyzing mixed integral equations (MIEs) due to their orthogonality qualities. This article reviewed recent breakthroughs in the use of Gegenbauer polynomials to solve mixed integral problems. Previous authors studied the problem with a continuous kernel that combined both Volterra (V) and Fredholm (F) components; however, in this paper, we focused on a singular Carleman kernel. The kernel of FI was measured with respect to position in the space L2[1,1], while the kernel of Ⅵ was considered as a function of time in the space C[0,T],T<1. The existence of a unique solution was discussed in L2[1,1]×C[0,T] space. The solution and its error stability were both investigated and commented on. Finally, numerical examples were reviewed, and their estimated errors were assessed using Maple (2022) software.

    Citation: Ahmad Alalyani, M. A. Abdou, M. Basseem. The orthogonal polynomials method using Gegenbauer polynomials to solve mixed integral equations with a Carleman kernel[J]. AIMS Mathematics, 2024, 9(7): 19240-19260. doi: 10.3934/math.2024937

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  • The orthogonal polynomials approach with Gegenbauer polynomials is an effective tool for analyzing mixed integral equations (MIEs) due to their orthogonality qualities. This article reviewed recent breakthroughs in the use of Gegenbauer polynomials to solve mixed integral problems. Previous authors studied the problem with a continuous kernel that combined both Volterra (V) and Fredholm (F) components; however, in this paper, we focused on a singular Carleman kernel. The kernel of FI was measured with respect to position in the space L2[1,1], while the kernel of Ⅵ was considered as a function of time in the space C[0,T],T<1. The existence of a unique solution was discussed in L2[1,1]×C[0,T] space. The solution and its error stability were both investigated and commented on. Finally, numerical examples were reviewed, and their estimated errors were assessed using Maple (2022) software.



    Several problems in astrophysics, including linear and nonlinear elasticity and engineering crack problems, lead to an integral equation of the first and second kinds of Fredholm integral equations (FIEs), which deal with problems having boundary conditions, while problems having initial conditions are described by the Volterra integral equation (VIE); see Popov [1] and Aleksandrovsk and Kovalenko [2]. After using Kiren's method, many spectral relationships for FIEs with discontinuous kernels were obtained (Mkhitaryan and Abdou [3]). For Carleman kernel and its importance in the nonlinear theory of plasticity, see Artinian [4]. Alalyani et al. [5] dealt with the solution of the third kind of mixed integro-differential equations with displacement using orthogonal polynomials. Gegenbauer polynomials, also known as ultraspherical polynomials, constitute a family of orthogonal polynomials that have found widespread applications in various mathematical disciplines. In recent years, researchers have increasingly turned to these polynomials for solving mixed integral equations (MIEs), which refers to problems with a Fredholm kernel in position and Volterra in time, and often arise in mathematical modeling across different fields. Using the polynomial method, Abdou and Khamis [‎6] were able to solve a first type F-VIE with a Carleman kernel. El-Gindy et al. [7] used the shifted Gegenbauer polynomials and Tau method to present numerical solutions to multi-order fractional differential equations. Atta [8] applied the shifted Gegenbauer polynomials to solve the time fractional cable problems. Nasr and Abdel-Aty [9] used the degenerate method to solve a V-FIE. Mirzaee and Samadyar [10] represented the Bernstein collocation method for solving 2D-mixed Volterra-Fredholm integral equations. Alhazmi et al. [11] used the Lerch polynomial method to solve MIEs, which had a strongly singular kernel. More details on several approaches for solving integral equations can be found in [12,13,14,15,16,17].

    In this work, we discuss innovative approaches and algorithms employed to solve MIEs and show how the Gegenbauer polynomials contribute to the efficiency and accuracy of these methods. Consider the following MIEs of two types: V-FIE and F-VIE, respectively.

    μΦ(u,t)λt011k(|yu|)f(t,s)Φ(y,s)dyds=F(u,t), (1a)
    μΦ(u,t)λt0f(t,s)Φ(u,s)dsλ11k(|yu|)Φ(y,t)dy=H(u,t), (1b)

    with the dynamical condition

    11Φ(u,t)du=P(t),t[0,T],T<1. (2)

    Condition (2) is of particular importance in applied sciences, as all the unknown functions during the integration period do not exceed the pressure exerted on the bodies and are changing with time.

    Here, the function f(t,s)C[0,T]2,T<1. The singular kernel k(|yu|) takes the Carleman function form. The constants μ and λ have several physical meanings. The given function

    F(u,t)L2[1,1]×C[0,T],

    while function Φ(u,t) will be determined in the same space of the function F(u,t).

    The paper is structured as follows: Using the fixed-point theorem and under certain conditions in Section 2, the existence of a unique solution is established. In Section 3, the convergence and the error stability of the solution are discussed. In Section 4, we use the separation variables technique to obtain a Fredholm equation of the second type with the Carleman kernel. In Section 5, the orthogonal polynomials method and Gegenbauer polynomials are used to convert the system of FIEs with time parameters to an algebraic system, where its convergence is considered in Section 6. The numerical results are given in Section 7. Finally, Section 8 presents our conclusions from the present research study.

    Consider the following assumptions:

    (a) The kernel k(|yu|) in L2[1,1] space in which its discontinuity condition is

    [1111k2(|yu|)dudy]12=α,(αisaconstant).

    (b) For t,s[0,T],T<1, the time function f(t,s)C[0,T] and satisfies

    f(t,s)β,(βisaconstant).

    (c) The given function F(u,t)L2[1,1]×C[0,T] is well-defined and its norm

    F=max0tT|t0[11F2(u,s)du]12ds|=M,whereMisaconstant.

    To discuss the existence of a unique solution for Eq (1a), we write it in the integral operator form as

    χΦ(u,t)=1μ[F(u,t)+KΦ], (3)

    where

    KΦ=λt011k(|yu|)f(t,s)Φ(y,s)dyds. (4)

    Theorem 1 (Existence and uniqueness for V-FIE). There exists a unique solution for the MIE (1a) under the condition

    Tαβ|λ|<|μ|,T<1. (5)

    Proof. To demonstrate this theorem, we use the following results:

    Lemma 1. Under the condition of Theorem 1, χ is a bounded operator.

    Proof. The normality of Eq (3) leads to

    χΦ1|μ|[F+KΦ],KΦ=|λ|t011f(t,s)k(|xy|)Φ(y,s)dyds. (6)

    The conditions (a), (b), and the Cauchy-Schwarz inequality lead to

    KΦ|λ|f[1111k2(|uy|)dxdy]12TΦ|λ|αβTΦ. (7)

    Hence, (6) becomes

    χΦ1|μ|[M+|λ|αβTΦ]. (8)

    Therefore, the operator χ transforms the ball SrL2[1,1]×C[0,T] into itself, where

    r=δ1ρ,δ=Mμ,andϱ=Tαβ|λ||μ|.

    Since r>0, under the hypothesis condition Tαβ|λ|<|μ|, the operator K is bounded and, accordingly, χ is bounded .

    Lemma 2. In the space of integration, the operator χ is a contraction.

    Proof. Let Φ1, Φ2 be two different solutions of Eq (1a); hence, formula (3), once using (4), leads to

    χΦ1χΦ2T|μ|[|λ|αβΦ1Φ2]. (9)

    So, we have the continuity of χ.

    Furthermore, under the condition αβ|λ|T<|μ|, χ is a contraction mapping.

    By the fixed-point theorem, since χ is a bounded and continuous operator, and moreover, it is a contraction mapping, then the solution of Eq (1a) has a unique solution.

    Theorem 2 (Existence and uniqueness for F-VIE) (without proof). There exists a unique solution for the MIE (1b) under the condition

    (α+βT)|λ|<|μ|.

    To study the solution behavior of Eq (1a), we construct the sequence

    {Φ0(u,t),Φ1(u,t),Φ2(u,t),,Φn1(u,t),Φn(u,t),}.

    Hence, consider a specific equation

    μΦn(u,t)=F(x,t)+λt011k(|yu|)f(t,s)Φn1(y,s)dyds,Φ0=F(u,t)μ. (10)

    We define

    Ψn=ΦnΦn1,Ψ0(u,t)=Φ0, (11)

    to establish

    Φn(x,t)=ni=0Ψi.

    In view of (11), we can adapt Eq (10) to take the form

    μΨn(u,t)=λt011k(|yu|)f(t,s)Ψn1(y,s)dyds. (12)

    Theorem 3 (Convergence of the solution for V-FIE). A sequence {Ψn}n=0 of the solution to (12), under condition (5), is uniformly convergent.

    Proof. Formula (12), when using the Cauchy-Schwarz inequality, yields

    |μ|Ψn(u,t)|λ||t011k(|yu|)f(t,s)dyds|Ψn1(u,t). (13)

    Then, by using assumptions (a)–(c), we have

    |μ|Ψn(u,t)|λ|αβTΨn1(u,t). (14)

    Therefore,

    |μ|Ψn|λ|αβTΨn1. (15)

    Hence, with the use of (11), we get

    ΨnϱnF,ϱ=Tαβ|λ||μ|. (16)

    So, Φn(x,t)=ni=0Ψi is uniformly convergent, provided that ϱ<1.

    If n, then Φn(x,t)Φ(x,t), i.e., Φ(x,t) is uniformly convergent.

    As an approximation of Eq (1a), we have

    μΦn(u,t)=Fn(u,t)+λt011k(|yu|)f(t,s)Φn(y,s)dyds, (17)

    where Fn(u,t)F(u,t) as n.

    By considering Eq (1a), we get the equation of the error as follows:

    Let the error function be defined as

    Rn(x,t)=Φ(x,t)Φn(x,t).

    Hence, we get

    μRn(u,t)λt011k(|yu|)f(t,s)Rn(y,s)dyds=Hn(u,t),(Hn(u,t)=FFn). (18)

    Theorem 4 (Convergence of the error for V-FIE). A sequence {Rn} of error for Eq (18) is uniformly convergent under condition (5).

    Proof. After constructing the sequence of errors {R0(u,t),R1(u,t),,Rn1(u,t),Rn(u,t),}, and considering

    Rn=RnRn1,R0(x,t)=H0(u,t)μ,Rn(u,t)=ni=0Ri, (19)

    then by using assumptions (a)–(c), we get

    |μ|Rn|λ|αβTRn1. (20)

    By induction,

    Rnϱnf,ϱ=Tαβ|λ||μ|. (21)

    So, under the inequality ϱ<1, Rn(x,t) is convergent.

    If n, Rn(u,t)R(u,t), then the error function R(u,t) is convergent.

    μΦ(x,t)λt011ts|xy|νΦ(y,s)dyds=F(x,t),

    where

    α=[1111|yu|2νdudy]12

    and β=T2. So, there exist numerical solutions under the convergence condition λαβTμ<1. The convergence condition for a given μ=1 and various values of ν,λ, and T are displayed in Table 1:

    Table 1.  Convergence condition for μ=1 and different values of ν,λ, and T.
    T ν α λ Convergence condition
    0.005 0.07 2.130 0.018
    0.700
    4.79×109
    1.80×107
    0.09 0.018
    0.700
    2.70×105
    0.001
    0.7 0.018
    0.700
    0.013
    0.510
    0.005 0.4 4.375 0.018
    0.700
    9.83×109
    3.80×107
    0.09 0.018
    0.700
    5.70×105
    0.002
    0.7 0.018
    0.700
    0.027
    1.050

     | Show Table
    DownLoad: CSV

    From Table 1, there is a fast convergence to the solution whenever we have decreasing ν,λ, and T, and for example, there is a divergence when ν=0.4, T=0.7, and λ=0.7.

    μΦ(x,t)λt0tsΦ(x,s)dyλ11|xy|νΦ(y,t)dy=F(x,t).

    In this example, there exist numerical solutions under the convergence condition |λ|(α+βT)|μ|<1. The convergence condition for a given μ=1 and various values of ν,λ, and T are displayed in Table 2:

    Table 2.  Convergence condition for μ=1 and different values of ν,λ, and T.
    T ν α λ Convergence condition
    0.005 0.07 2.130 0.018
    0.100
    0.0383
    0.2131
    0.09 0.018
    0.100
    0.0384
    0.2130
    0.7 0.018
    0.100
    0.0445
    0.2473
    0.005 0.4 4.375 0.018
    0.100
    0.0788
    0.4375
    0.09 0.018
    0.100
    0.0788
    0.4376
    0.7 0.018
    0.100
    0.0849
    0.4718

     | Show Table
    DownLoad: CSV

    From Table 2, there is a straightforward time effect, while when ν and λ decrease, there is rapid convergence.

    Some researchers have solved the integral equations at zero time using the earlier technique; see, for example, [9]. In other studies, time and position may be separated using the Laplace or Fourier transforms; however, this method has drawbacks when trying to identify inverse transformers. Another technique is to divide the time into periods to create an entire set of integral equations that are especially applicable to the position.

    The approach of separating variables using explicit functions in position and time makes the discussion of the time impact more comprehensible.

    Assume the unknown and given functions, respectively, take the form

    Φ(u,t)=A(t)ψ(u),F(u,t)=g(u)B(t). (22)

    Hence, when using formula (22), Eq (1a) yields

    μψ(u)λ11k(|yu|)ψ(y)dy=g(u), (23)

    where

    λ=λB(t)t0f(t,s)A(s)dτ,μ=A(t)B(t). (24)

    In all previous research, the solution to MIEs cannot be discussed in view of time. Also, μ determines the kind of the integral equation. If μ=0, we have an IE of the first kind, while if μ=constant0, we have an IE of the second kind. A third kind of IE can be obtained if μ=μ(u). The significance of the separation method came from obtaining a quadratic FIE with a time-related coefficient. In this case, the time can be computed explicitly at any point.

    The solution of Eq (23) will be discussed using Gegenbauer polynomials of the order ν2, which is

    C(υ2)n(u)=n2k=0(1)kΓ(nk+υ2)(2u)n2kΓ(υ2)k!(n2k)!.

    So, we write the unknown function ψ(x) and the given function g(x) in the following forms:

    ψ(u)=n=0bn(1u2)υ12C(υ2)n(u),(bnareunknownconstants). (25a)
    g(u)=n=0gn(1u2)υ12C(υ2)n(u),gn=n!(n+υ2)Γ2(υ2)π21υΓ(n+υ)11g(u)C(υ2)n(u)du. (25b)

    Now, consider the following relationships (see [18]).

    a) Spectral relationship:

    11(1y2)υ12|uy|νC(υ2)n(y)dy=πΓ(n+υ)Γ(υ)Γ(n+1)cos(πυ2)C(υ2)n(u). (26a)

    b) Orthogonal relationship:

    11(1y2)υ12C(υ2)n(y)C(υ2)m(y)dy=π21υΓ(n+υ)n!(n+υ2)Γ2(υ2)δm,n. (26b)

    In (25a), bn,n0 are called the eigenvalues of the unknown function ψ(x). The function (1x2)υ12 is the weight function of Gegenbauer polynomials of order (υ2).

    Truncate formula (25a) as an approximate solution to take the form

    ψN(u)=Nn=0bn(1u2)υ12C(υ2)n(u),limNψN(u)=ψ(u). (27)

    So, Eq (24) takes the form

    μNn=0bn(1u2)υ12C(υ2)n(u)λ11Nn=0bn|yu|υ(1y2)υ12C(υ2)n(y)dy=Nn=0gn(1u2)υ12C(υ2)n(u). (28)

    By using Eq (26a), we get

    μNn=0bn(1u2)υ12C(υ2)n(u)λNn=0bnπΓ(n+υ)Γ(υ)Γ(n+1)cos(πυ2)C(υ2)n(u)=Nn=0gn(1u2)υ12C(υ2)n(u). (29)

    Multiplying (29) by C(υ2)m(u) and integrating it with respect to u, u[1,1], we get

    μNn=0bnπ21υΓ(n+υ)n!(n+υ2)Γ2(υ2)λNn=0bnπΓ(n+υ)Γ(υ)Γ(n+1)cos(πυ2)11C(υ2)n(u)C(υ2)m(u)du=Nn=0gnπ21υΓ(n+υ)n!(n+υ2)Γ2(υ2). (30)

    By using the Gegenbauer relations (see [18]),

    Cυm(u)Cυn(u)=m+nk=|mn|[(1(k+m+n)mod2)(k+υ)k!Γ(12(k+m+n+2υ))Γ(12(k+mn+2υ))Γ(12(km+n+2υ))Γ(12(k+m+n+4υ))]/[Γ(12(k+m+n+2))Γ(12(k+mn+2))Γ(12(km+n+2))Γ(12(k+m+n+2υ+2))Γ(k+2υ)Γ2(υ)]Cυk(u), (31a)
    11Cυn(x)dx=Cυ1n+1(1)Cυ1n+1(1)2(υ1), (31b)
    Cυn(1)=Γ(2υ+n)Γ(2υ)Γ(n+1), (31c)
    Cυn(1)=Γ(2υ+n)Γ(2υ)Γ(n+1)cos(π(υ+n))sec(πυ), (31d)

    and we have the following linear algebraic system (LAS):

    μbnλ(n+υ2)Γ2(υ2)21υ(υ2)Γ(υ)cos(πυ2)m+nk=|mn|bmχk,n,m(Γ(υ+k1)Γ(υ2)Γ(k+2){1cos(πυ2+πk)sec(πυ2π)})=gn, (32)

    where n=0,1,2,3,,N and χk,n,m is given by

    χk,n,m=[(1(k+m+n)mod2)(k+υ2)k!Γ(12(k+m+n+υ))Γ(12(k+mn+υ))Γ(12(km+n+υ))Γ(12(k+m+n+2υ))]/[Γ(12(k+m+n+2))Γ(12(k+mn+2))Γ(12(km+n+2))Γ(12(k+m+n+υ+2))Γ(k+υ)Γ2(υ2)]. (33)

    We write the LAS (32) in the operator form

    Qbn=1μgn+1μQbm,Qbm=λω(n,υ)m+nk=|mn|bmC(k,υ)χk,n,m, (34)

    where

    (a)ω(n,υ)=(n+υ2)Γ2(υ2)21υ(υ2)Γ(υ)cos(πυ2),
    (b)C(k,υ)=(Γ(υ+k1)Γ(υ2)Γ(k+2){1cos(πυ2+πk)sec(πυ2π)}).

    To prove the convergence of (34), we assume

    (I)χk,n,m=maxNm+nk=|mn||χk,n,m|=β1,N={max(m+n),min|mn|.
    (II)|gn|=γ,
    (III)ω(n,υ)=maxn|ω(n,υ)|=δ1,
    (IV)C(k,υ)=maxNm+nk=|mn||C(k,υ)|=δ2.

    Then, we state the following theorem.

    Theorem 5. The LAS (32) or (34) is convergent in l space, under the above assumptions, and has a unique solution under the condition:

    β1δ1δ2λ<μ. (35)

    Proof. From Eq (34), we have

    |Qbm||λ||ω(n,υ)|m+nk=|mn||bmC(k,υ)χk,n,m|.

    The above inequality takes the form

    Qbmmaxn|ω(n,υ)||λ|(maxm,nm+nk=|mn||χk,n,m|)(maxm,nm+nk=|mn||C(k,υ)|)|bm|.

    Hence, we have

    Qbmβ1δ1δ2|λ||bm|. (36)

    Finally, we get

    Qbn1|μ|{γ+β1δ1δ2|λ||bm|}. (37)

    Formula (36) leads to the convergence of the linear algebraic system, while inequality (37) leads to the uniqueness of the system under the given condition (35).

    An illustrative example

    Consider the V-FIE

    μΦ(x,t)λt011ts|xy|νΦ(y,s)dyds=F(x,t).

    By using formula (24), we have

    μψ(x)λ11|xy|νψ(y)dy=g(x).

    If A(t)=B(t), we have

    |λ|=|λ|T3,|μ|=1.

    The convergent approximate solution can be obtained under the condition β1δ1δ2|λ||μ|<1, which can be shown in Table 3.

    Table 3.  Convergence condition for different values of ν,λ, and N with T=0.7.
    ν n N β1 δ1 δ2 λ λ Convergence condition
    0.07 4 8 0.0265 62.963 5.0×104 0.018
    0.700
    0.006
    0.240
    5.0×106
    2.0×104
    8 16 0.0177 125.381 7.0×105 0.018
    0.700
    0.006
    0.240
    9.0×107
    3.0×105
    16 32 0.0133 250.215 1.0×105 0.018
    0.700
    0.006
    0.240
    2.0×107
    8.0×106
    0.4 4 8 0.4794 20.340 0.004 0.018
    0.700
    0.006
    0.240
    2.0×104
    0.008
    8 16 0.5266 39.711 6.0×104 0.018
    0.700
    0.006
    0.240
    7.0×105
    0.003
    16 32 0.6241 78.453 1.0×104 0.018
    0.700
    0.006
    0.240
    3.0×105
    0.001

     | Show Table
    DownLoad: CSV

    From Table 3, we deduce that there is fast convergence whenever Nincreases, while there is slow convergence when the values of ν and λincrease.

    In this section, we present some examples to demonstrate the accuracy and applicability of the presented techniques by considering the requirements for the existence of a solution and its numerical convergence, shown by Tables 13.

    Example 1. Consider the V-FIE

    μΦ(x,t)λt011ts|xy|νΦ(y,s)dyds=F(x,t),0tT<1. (38)

    Here, F(x,t) is given by sitting Φ(x,t)=x2t2 as an exact solution, and its error function is given by RN=|Φ(x,t)ΦN(x,t)|. Under the assumption λαβTμ<1 for some values of λ and for the given values ν=0.07 and T=0.09, shown in Table 1, mean errors and their rate of convergence for different values of N are represented in Table 4.

    Table 4.  Mean errors and their rate of convergence.
    λ N Mean error Convergence rate
    0.018 4 9.02×104 2.25
    8 1.91×104 1.32
    16 7.60×105 1.84
    32 2.13×105 ---
    0.7 4 9.03×104 2.07
    8 2.15×104 1.49
    16 7.64×105 1.84
    32 2.15×105 ---

     | Show Table
    DownLoad: CSV

    From Table 4, the error decreases with increasing values of N, and its approximate numerical solution is stable with increasing values of λ under the convergence condition.

    Example 2. Consider the V-FIE

    Φ(x,t)0.18t011t2s2|xy|νΦ(y,s)dyds=F(x,t), (39)

    where F(x,t) is specified by setting Φ(x,t)=(x2+x5)(0.005+0.03t+0.7t3) as an accurate solution.

    In Table 5, the errors are presented for different values of ν, demonstrating that the errors increase with time T and are stable.

    Table 5.  The solution Φ(x,t) and its corresponding errors where N=16 for different values of time and υ.
    T x υ=0.07 υ=0.4
    Φ(x,t) Error (RN) Φ(x,t) Error (RN)
    0.005 –0.8 0.0016164 0.0000079 0.0016204 0.0000119
    –0.4 0.0007548 0.0000164 0.0007523 0.0000189
    0.0 –0.0000122 0.0000122 – 0.0000141 0.0000141
    0.4 0.0008726 0.0000041 0.0008738 0.0000029
    0.8 0.0050392 0.0000555 0.0050360 0.0000523
    0.09 –0.8 0.0025769 0.0000126 0.0025833 0.0000191
    –0.4 0.0012033 0.0000262 0.0011993 0.0000302
    0.0 –0.0000195 0.0000195 –0.0000224 0.0000224
    0.4 0.0013911 0.0000066 0.0013930 0.0000047
    0.8 0.0080335 0.0000886 0.0080284 0.0000834
    0.7 –0.8 0.0825486 0.0005598 0.0824931 0.0006153
    –0.4 0.0380344 0.0018165 0.03770211 0.0021488
    0.0 –0.0015983 0.0015983 –0.0018176 0.0018176
    0.4 0.0440846 0.0012165 0.0437332 0.0015679
    0.8 0.2592969 0.0017963 0.2579618 0.0004611

     | Show Table
    DownLoad: CSV

    By taking υ=0.4, for example, the error increases with time and decreases by increasing the number of iterations; see Figures 14.

    Figure 1.  The error of Example 2, where N=16,T=0.09.
    Figure 2.  The error of Example 2, where N=16,T=0.7.
    Figure 3.  The error of Example 2, where N=8,T=0.09.
    Figure 4.  The error of Example 2, where N=8,T=0.7.

    Figure 5 represents the approximate solution Φ(x,t) of Example 2 in 3-dimensional space.

    Figure 5.  The approximate solution Φ(x,t) of Example 2, where N=8.

    Example 3. Consider the F-VIE

    μΦ(x,t)λt0t2s2Φ(x,s)dsλ11|xy|νΦ(y,t)dy=F(x,t). (40)

    Figures 611 show the solution and the associated errors for the F-VIE with a Carleman kernel. We noticed that the errors declined as the values of ν decreased.

    Figure 6.  The error of Example 3, where N=16,T=0.09, and ν=0.4.
    Figure 7.  The error of Example 3, where N=16,T=0.25, and ν=0.4.
    Figure 8.  The error of Example 3, where N=16,T=0.55, and ν=0.4.
    Figure 9.  The error of Example 3, where N=8,T=0.25, and ν=0.4.
    Figure 10.  The error of Example 3, where N=16,T=0.25, and ν=0.007.
    Figure 11.  The error of Example 3, where N=8,T=0.25, and ν=0.007.

    Figure 12 represents the approximate solution Φ(x,t) of Example 3 in 3-dimensional space

    Figure 12.  The approximate solution Φ(x,t) of Example 3, where N=8.

    This study aimed to deepen our understanding of the role that Gegenbauer polynomials play in solving mixed integral equations. By combining a rigorous exploration of mathematical principles with insights from recent references, this study aimed to contribute to the ongoing discourse in the field and provide a valuable resource for researchers and experts seeking the potential of Gegenbauer polynomials in the solution of MIEs. From the previous results, we conclude the following:

    The separation variables technique is a strategy that assists in solving the scientific deficiencies of previous approaches, as it allows researchers to control the time required to solve the problem in a specific way.

    The method of separation of variables was used in this research to transform the mixed integral equation in position and time into an integral equation in position and with coefficients in time. Furthermore, spectral relationships can be derived, which helps in solving many mathematical physics problems.

    Using the orthogonal polynomials technique and certain special functions, we may quickly express that the solution is a linear relationship between the eigenvalues and the eigenfunctions.

    In Example 2, we considered a V-FIE with a Carleman kernel for different values of ν and time. We observed that the errors increased with time and were extremely stable for different values of ν (see Table 5).

    By increasing the iteration number N, the errors decreased, which can be observed in Figures 14, while the approximate solution Φ(x,t) of Example 2 appears in Figure 5.

    In Example 3, we numerically presented the solution of a F-VIE with a Carleman kernel. The solution and its corresponding errors are displayed in Figures 611, and we observed that by decreasing the values of ν, the errors decreased. The approximate solution Φ(x,t) is also illustrated in Figure 12.

    Conceptualization, M.A.A.; Methodology, A.A. and M.B.; Software, A.A. and M.B.; Validation, M.A.A.; Formal analysis, A.A., M.A.A., and M.B.; Resources, A.A. and M.B.; Writing - original draft, A.A. and M.B.; Writing - review & editing, A.A., M.A.A., and M.B.; Project administration, A.A.; Funding acquisition, A.A. and M.B. All authors have read and agreed to the published version of the manuscript.

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

    The authors would like to thank the editor and referees for their valuable comments and suggestions on the manuscript.

    The authors declare that they have no conflicts of interest to report regarding the publication of this article.



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