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ISSN: 2322-1666 print/2251-8436 online

NEW APPROACH FOR SOLUTION OF VOLTERRA INTEGRAL EQUATIONS USING SPLINE

QUASI-INTERPOLANT

MARYAM DERAKHSHAN KHANGHAH AND MOHAMMAD ZAREBNIA

Abstract. In this paper, we present quadratic rule for

approxi-mate solution of integrals using spline quasi-interpolant. The method is applied for solving the linear Volterra integral equations. Also the convergence analysis of the method is given. The method is applied to a few examples to illustrate the accuracy and implementation of the method.

Key Words: Spline; Quasi-interpolant; Volterra; Convergence.

2010 Mathematics Subject Classification:65R20; 41A15; 41A25.

1. Introduction

Integral and integro-differential equations are mathematical tools in many branches of science and engineering. The numerical methods for linear integral equations of the second kind studied in Delves [6]. Among these equations, Volterra integral equations arise from multiple appli-cations, for example physics and engineering such as potential theory, Dirichlet problems, electrostatics, the particle transport problems and heat transfer problems [3, 9]. Several numerical methods have been considered to approximate the solution of Volterra integral equations such as the papers [1,4, 5, 7, 10] that are concerned respectively with rational basis functions with product integration methods, collocation

Received:22 December 2019, Accepted: 1 August 2020. Communicated by Nasrin Eghbali Address correspondence to Maryam Derakhshan; E-mail: M.Derakhshan @uma.ac.ir

c

2019 University of Mohaghegh Ardabili.

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methods in certain polynomial and polynomial spline spaces with uni-form and graded meshes, the generalized Newton-Cotes uni-formulae com-bined with product integration rules, mathematical programming meth-ods and fractional linear multistep methmeth-ods. In [17], Riley approxi-mated the Volterra integral equations by sinc approximation methods. Reihani have solved Fredholm and Volterra integral equations by ratio-nalized Haar functions method [16]. Simpson’s quadrature method [13], Galerkin method with the Chebyshev polynomials [15] and repeated Simpson’s and Trapezoidal quadrature rule [2] are other works on de-veloping and analyzing numerical methods for solving Volterra integral equations.

Moreover, one can refer to other methods such as [14, 19, 20]. The linear Volterra integral equation is considered as

(1.1) u−Ku=g,

where linear integral operator K is defined as

(1.2) (Ku)(x) =

x a

k(x, t)u(t)dt,

g(x) andk(x, t) are known continuous functions andu(x) is the unknown function to be determined. Integration of a function is an important operation for many physical problems.

The organization of the paper is as follows. In Section 2, we describe the construction of quadrature rule based on spline quasi-interpolant. In Section 3, we give an application of the quadrature rule of Section 2 to the numerical solution of Volterra integral equations. In Section 4, the convergence and error analysis of the numerical solution are provided. At the end we give some numerical examples which confirm our theoretical results.

2. Quadrature rule based on a quadratic spline quasi-interpolant

Let Xn :={xk, 0 ≤k ≤n} be the uniform partition of the interval

I = [a, b] into n equal subintervals, i.e. xk := a+kh, with h = b−na. We consider the space S2 = S2(I, Xn) of quadratic splines of class C1 on this partition. Canonical basis is formed by the n+ 2 normalized B-splines, {Bk, k ∈J}, J :={1,2,· · ·, n+ 2}. Consider the quadratic spline quasi-interpolant (dQI) of a function f defined onI and given in

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[18], that is

(2.1) ϕ2f =

k∈J

υk(f)Bk,

where

υ1(f) =f1, υn+2(f) =fn+2,

υ2(f) =1/3f1+ 3/2f21/6f3 =β1f1+β2f2+β3f3,

(2.2) υn+1(f) =1/6fn+3/2fn+11/3fn+2=β3fn+β2fn+1+β1fn+2, and for 3≤j ≤n,

(2.3) υj(f) =1/8fj−1+ 5/4fj−1/8fj+1 =γ1fj−1+γ2fj+γ3fj+1, withfi =f(ti), t1 =a, tn+2 =b, ti=a+ (i−3/2)h, 2≤i≤n+ 1.The quadratic B-spline functions at knots are defined as

Bi(x) =               

(x−xi−3)2

(xi−1−xi−3)(xi−2−xi−3), xi−3 ≤x < xi−2, (xi−x)(x−xi−2)

(xi−xi−2)(xi−1−xi−2) +

(x−xi−3)(xi−1−x)

(xi−1−xi−3)(xi−1−xi−2), xi−2 ≤x < xi−1, (xi−x)2

(xi−xi−2)(xi−xi−1), xi−1 ≤x < xi. We consider the quadrature rule defined by

(2.4) Iϕ2f(x) :=

x

a

Q2fa)dˆa. By considering ∫axBj forh= 1, n= 10 we can get ∫ x

a

B1(ξ)=

  

0, x≤0,

x−x2+ 13x3, 0< x≤1,

1

3, else,

x a

B2(ξ)=

      

0, x≤0,

1

2(2x2−x3), 0< x≤1,

2

3 + 2x−x2+ 1

6x3, 1< x≤2, 2

3, else,

x a

B11(ξ)=

      

0, x≤8,

256

3 + 32x−4x 2+1

6x

3, 8< x9, 1202

3 130x+ 14x 21

2x

3, 9< x10, 2

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x a

B12(ξ)=

  

0, x≤9,

243 + 81x−9x2+31x3, 9< x≤10,

1

3, else,

and for 3≤j≤n,

x

a

Bj(ξ)=                       

0 f or 3−j+x≤2, 4

3 + 2(x+ 3−j)(x+ 3−j) 2+ 1

6(x+ 3−j) 3

f or 2< x+ 3−j≤3,

73 6

23

2(x+ 3−j) + 7

2(x+ 3−j)2+ 1

3(x+ 3−j)3

f or 3< x+ 3−j≤4, 119

6 + 25

2 (x+ 3−j) 5

2(x+ 3−j) 2+1

6(x+ 3−j) 3

f or 4< x+ 3−j≤5,

1, else.

Quadrature formulaIϕ2f(x) can be obtained as

Iϕ2f(x) = ˜ζ1(x)f1+ 3

j=1

βj( ˜ζ2(x)fj+ ˜ζn+2(x)fn+3−j)

+ nj=3 ˜

ζj(x)(γ1fj−1+γ2fj +γ3fj+1) + ˜ζn+2(x)fn+2, (2.5)

where

˜

ζ1(x) =

x

a

B1(ξ)=

{

x− 1hx2+3h12x3, 0≤x&&h−x >0, 0, else,

˜

ζ2(x) =

x

a

B2(ξ)=

      

0, x≤0,

1

2h2(2hx2−x3), 0≤x &&h−x >0, 2x−h1x2+6h12x3, h−x≤0&&2h−x >0, 0, else,

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˜

ζn+1(x) =

x

a

Bn+1(ξ)=

    

(n−2)2

2 x−

(n−2) 2h x

2+ 1

6h2x3, (n−2)h−x≤0&&(n−1)h−x >0,

3n24n

2 x+

(3n−2) 2h x

2 1

2h2x3, (n−1)h−x≤0&&nh−x >0,

0, else,

˜

ζn+2(x) =

x a

Bn+2(ξ)=

{

(n−1)2x−(nh1)x2+3h12x3, (n−1)h−x≤0&&nh−x >0,

0, else,

and for 3≤j ≤n,

˜

ζj(x) = ∫ x

a

Bj(ξ)

=                    1

6h2(x+ 3h−jh)3

f or x+ 3h−jh≥0&&−x−2h+jh >0, 3

2(x+ 3h−jh) + 3

2h(x+ 3h−jh) 2 1

3h2(x+ 3h−jh)3

f or −x−2h+jh≤0&&−x−h+jh >0,

9

2(x+ 3h−jh) 3

2h(x+ 3h−jh) 2+ 1

6h2(x+ 3h−jh)3

f or −x−h+jh≤0&&−x+jh >0,

0, else.

This quadrature formula can be written as

(2.6) Iϕ2f(x) = 3

j=1

ψj(x)fj+ n−1

j=4

ηj(x)fj+ n+2

j=n

θj(x)fj,

where

ψ1(x) = ˜ζ1(x) 1

3ζ˜2(x), θn(x) = ˜ζn+2(x) 1

3ζ˜n+1(x),

ψ2(x) = 3

2ζ˜2(x) 1

8ζ˜3(x), θn+1(x) = 3

2ζ˜n+1(x) 1 8ζ˜n(x),

ψ3(x) = 1 6 ˜

ζ2(x) + 5 4 ˜

ζ3(x) 1 8 ˜

ζ4(x), θn+2(x) = 1 6 ˜

ζn+1(x) + 5 4 ˜

ζn(x) 1 8 ˜

ζn−1(x),

ηj(x) =1

8ζ˜j+1(x) + 5

4ζ˜j(x) 1

8ζ˜j−1(x), 4≤j≤n−1. (2.7)

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Theorem 2.1. For any partition X of I, the infinity norm of Q is uni-formly bounded by3. If the partition is uniform, one has ∥ϕ∥= 305207 1.4734.

Proof. For proof, refer to [18]. □

According [18], there exists a constantC such that

∥f −ϕ2f ∥∞≤Ch3 ∥D3f ∥∞.

3. Application to Volterra integral equations

In this section, we illustrate an application of the quadrature rule to numerical solution of Volterra integral equation

u(x)x

a

k(x, t)u(t)dt=g(x),

wherek(., .)∈C([a, b]×[a, b]) and g(x)∈C([a, b]) are known functions and u(x) is the unknown function to be determined. We use spline quasi-interpolant method for Volterra integral equation. The method associated with the quadrature formula

(3.1) (Knu)(x) = ∫ x

a

ϕ2(k(x, .)u(.))(ˆa)dˆa=Iϕ2ku(x), we obtain

u(x)(Knu)(x) =g(x), consists in looking for a solutionu satisfying

u(x)( 3

j=1

ψj(x)k(x, tj)uj+ n1

j=4

ηj(x)k(x, tj)uj (3.2)

+ n+2

j=n

θi(x)k(x, tj)uj) =g(x).

In summary, we can write

u(x) n+2

j=1

𝟋j(x)k(x, tj)uj =g(x), where

𝟋j =   

ψj(x), 1≤j 3

ηj(x), 4≤j ≤n−1,

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By replacing xi,we have

(3.3) u(xi)

n+2

j=1

𝟋j(xi)k(xi, tj)uj =g(xi). Equation (3.3) can be simplified in the matrix form

(3.4) (I−K∗)U =G,

where

U = [u1, u2, . . . , un+2]T,

K∗ = [𝟋j(xi)k(xi, tj)]i,j, i, j = 1, . . . , n+ 2,

G= [g(x1), g(x2), . . . , g(xn+2)]T.

Having used the solution uj, j = 1, . . . , n+ 2,in the system (3.4), we employ a method similar to the Nystrom’s idea for the Volterra integral equation, i.e. we used

(3.5) un(x) =

n+2

j=1

𝟋j(x)k(x, tj)u(tj) +g(x).

4. Convergence Analysis

In this section, we shall provide the convergence analysis of the pro-posed method. For this purpose, we consider the following theorem. Theorem 4.1. Letr˜nerror term for the spline quasi interpolant method.

Furthermore, let M0 = max|𝟋j(xi)||k(xi, tj)| and χj = max|k(xi, tj)|.

Then

|ϵn,i| ≤

O(h4) 1−M0

exp( n+1

j=1

χj 1−M0

).

Proof. In fact

un(xi) = n+2

j=1

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Thus

un(xi)−u(xi) = n+2

j=1

𝟋j(xi)k(xi, tj)(un(tj)−uj)+ n+2

j=1

𝟋j(xi)k(xi, tj)u(xi)−xi

a

k(xi, s)u(s)ds.

Let

ϵn,i=un(xi)−u(xi), and

˜

rn(xi) = n+2

j=1

𝟋j(xi)k(xi, tj)u(xi)xi

a

k(xi, s)u(s)ds.

Hence

ϵn,i= n+2

j=1

𝟋j(xi)k(xi, tj)ϵn,j+ ˜rn(xi). Thus

|ϵn,i| ≤ n+2

j=1

|𝟋j(xi)||k(xi, tj)||ϵn,j|+|r˜n(xi)|, so that

|ϵn,i| ≤ n+1

j=1

|𝟋j(xi)||k(xi, tj)||ϵn,j|+|𝟋n(xi)k(xi, tn)||ϵn,n|+|r˜n(xi)|. Now using the Gronwall Lemma [8], we obtain

|ϵn,i| ≤

O(h4) 1−M0

exp( n+1

j=1

χj 1−M0

).

Theorem 4.2. Let k∈C([a, b]×[a, b]) andu∈C[a, b]. Then we have

∥un−u∥∞≤∥(I−Kn)1 ∥∥(Kn−K)u∥∞.

Proof. For eachx∈[a, b], Let κ(., .) set by

κ(x, t) = {

k(x, t), a≤t≤x,

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The method associated with the quadrature formula

(Knu)(x) = ∫ b

a

ϕ2(k(x, .)u(.))(t)dt= n+2

j=1

𝟋j(x)k(x, tj)u(tj), a≤x≤b. There exists a constantM such that

n+2

j=1

|𝟋j(x)| ≤M, a≤x≤b.

We get

∥Knu∥∞≤M max|κ(x, t)| ∥u∥∞. Further, for allx1, x2 [a, b], we have

∥Knu(x1)−Knu(x2)∥∞≤M max|κ(x1, t)−κ(x2, t)| ∥u∥∞. On the other

I−Kn=I−K+K−Kn. Then

I −Kn= (I −K)[I+ (I−K)1(K−Kn)]. From equation (3.4) we obtain

un−u= (I−Kn)−1g−(I−K)1g. Thus

un−u= (I−Kn)−1(Kn−K)(I−K)1g

= (I−K)1(I+ (I−K)1(K−Kn))1g−(I−K)1g = ((I + (I−K)1(K−Kn))1−I)(I−K)1g

= (((I−Kn)(I−K)1)1−I)(I−K)1g

= (I−Kn)1(Kn−K)(I−K)1g. Hence

un−u= (I−Kn)1(Kn−K)u, and we deduce

∥un−u∥∞≤∥(I −Kn)1 ∥∥(Kn−K)u∥∞.

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5. Numerical example

In this section, in order to illustrate the performance of the presented method in solving Volterra integral equations and justify the accuracy and efficiency of the method, we consider the following examples.

Example 5.1. Consider the following Volterra integral equation

u(x)

x

0

(x+t)u(t)dt= 7 12x

4+5 3x

3+5 2x

2+ 2x+ 1,

where the exact solution is u(x) = (1 +x)2. In Table 1, numerical re-sults are presented for rules Iϕ2f. We obtain an approximation to the solution of (3.4). Numerical results illustrate accuracy of the proposed quadrature rule. By increasing the value of n, the errors have been de-creased. In Table 2, we present the absolute errors of algorithm combines Trapezoidal and Simpson rules [12] for different values of n. A numeri-cal comparison between Tables 1,2 shows that spline quasi-interpolant method is more accurate than of algorithm combines Trapezoidal and Simpson rules [12].

Table 1. Max. Abs. Err. for Example 5.1 (IQ2f)

n ∥u−un∥∞ order 19 7.43928×107 23 3.48711×107 3.96587 35 6.55478×108 3.98106 45 2.40445×108 3.99051 55 1.0788×108 3.99397 65 5.534×109 3.99585 75 3.12346×109 3.99697 85 1.89379×109 3.99767 95 1.21395×109 3.99818

Example 5.2. Consider the following Volterra integral equation

u(x) + ∫ x

0

(xt2+x2t)u(t)dt=x+ 7 12x

5,

where the exact solution is u(x) =x. In Table 3, numerical results are presented for ruleIϕ2f. In table 4, we compare the absolute errors of the

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Table 2. Max. Abs. Err. [12] n ∥u−un∥∞ 19 8.36×105 23 4.77×105 35 1.33×105 45 6.29×106 55 3.44×106 65 2.08×106 75 1.36×106 85 9.35×107 95 6.70×107

spline quasi-interpolant method for n = 32 with numerical expansion-iterative method [11]. The results show the efficiency and rate of con-vergence of the method. Figure 1 shows the maximum absolute errors for the proposed method.

Table 3. Max. Abs. Err. for Example 5.2 (IQ2f)

n ∥u−un∥∞ 20 3.88179×107 40 2.42884×108 60 4.79842×109

80 1.5183×109

100 6.21901×1010

Example 5.3. Consider the following Volterra integral equation

u(x) +

x

0

xtu(t)dt=e−x2 +x(1−e −x2

)

2 ,

where the exact solution isu(x) =e−x2.In Table 5, numerical results are presented for ruleIϕ2f. In table 6, we compare the absolute errors of the spline quasi-interpolant method for n = 32 with numerical expansion-iterative method [11]. Figure 2 shows the maximum absolute errors for the proposed method.

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Table 4. Numerical results for Example 5.2 x Absolute error Absolute error[11]

0 0 1.5625×102

0.1 8.55709×109 9.375×103 0.2 1.86236×108 3.125×103 0.3 2.78283×108 3.125×103 0.4 3.36708×108 9.375×103 0.5 3.80447×108 1.5625×102 0.6 4.72105×108 9.375×103 0.7 5.65627×108 3.68045×103 0.8 5.83707×108 3.125×103 0.9 4.9622×108 9.375×103

50 60 70 80 90 100 n

5.´10-9

1.´10-8

1.5´10-8

2.´10-8

error

Figure 1. The absolute error∥u−un∥∞for different values of

nfor Example 5.2.

Example 5.4. Consider the following Volterra integral equation

u(x) +

x

0

(x−t) cos(x−t)u(t)dt= cos(x),

where the exact solution isu(x) = 13(2 cos3t+1).In Table 7, numerical results are presented for rule Iϕ2f. In table 8, we compare the absolute

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Table 5. Max. Abs. Err. for Example 5.3 (IQ2f)

n ∥u−un∥∞ 20 4.78517×107 40 3.07465×108 60 6.10838×109 80 1.93431×109 100 7.92292×1010

Table 6. Numerical results for Example 5.3 x Absolute error Absolute error[11]

0 0 3.25×104

0.1 7.99755×109 2.02×103 0.2 1.41309×108 1.28×103 0.3 1.37384×108 1.647×103 0.4 5.21359×109 6.295×103 0.5 8.52356×109 1.2284×102 0.6 2.59421×108 7.87×103 0.7 4.61481×108 2.669×103 0.8 6.24702×108 2.661×103 0.9 6.84528×108 7.562×103

errors of the spline quasi-interpolant method for n= 64 with Rational-ized Haar functions method [16]. Figure 3 shows the maximum absolute errors for the proposed method.

Table 7. Max. Abs. Err. for Example 5.4 (IQ2f)

n ∥u−un∥∞ 20 8.97969×107 40 5.75157×108 60 1.14124×108 80 3.61664×109 100 1.48246×109

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Table 8. Numerical results for Example 5.4 x Absolute error Absolute error[16]

0 0 0.6×105

0.1 8.57026×109 4.23×104 0.2 7.42193×109 3.45×104 0.3 6.67605×109 4.55×104 0.4 6.28758×109 2.7×105 0.5 4.13835×109 0.7×104 0.6 3.59153×109 3.7×104 0.7 1.79297×109 1.52×104 0.8 2.97626×1010 6.7×105 0.9 1.00404×109 2.4×104

6. Conclusion

In this article, we illustrated a rule based on spline quasi-interpolant. In following, we employed this rule to the solution of a Volterra inte-gral equation. The numerical examples were presented to illustrate the accuracy and the implementation of the method.

50 60 70 80 90 100 n

5.´10-9

1.´10-8

1.5´10-8

2.´10-8

2.5´10-8

3.´10-8

error

Figure 2. The absolute error∥u−un∥∞for different values of

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40 50 60 70 80 n 5.´10-8

1.´10-7

1.5´10-7

error

Figure 3. The absolute error∥u−un∥∞for different values of

nfor Example 5.4.

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Maryam Derakhshan Khanghah

Department of Mathematics, University of Mohaghegh Ardabili, P.O.Box 56199-11367, Ardabil, Iran

Email: [email protected]

Mohammad Zarebnia

Department of Mathematics, University of Mohaghegh Ardabili, P.O.Box 56199-11367, Ardabil, Iran

Figure

Table 1. Max. Abs. Err. for Example 5.1 (I Q 2 f ) n ∥ u − u n ∥ ∞ order 19 7.43928 × 10 −7 − 23 3.48711 × 10 −7 3.96587 35 6.55478 × 10 −8 3.98106 45 2.40445 × 10 −8 3.99051 55 1.0788 × 10 −8 3.99397 65 5.534 × 10 −9 3.99585 75 3.12346 × 10 −9 3.99697 85
Table 2. Max. Abs. Err. [12] n ∥ u − u n ∥ ∞ 19 8.36 × 10 −5 23 4.77 × 10 −5 35 1.33 × 10 −5 45 6.29 × 10 −6 55 3.44 × 10 −6 65 2.08 × 10 −6 75 1.36 × 10 −6 85 9.35 × 10 −7 95 6.70 × 10 −7
Table 4. Numerical results for Example 5.2 x Absolute error Absolute error[11]
Table 6. Numerical results for Example 5.3 x Absolute error Absolute error[11]
+3

References

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