On some interpolatory iterative methods for the second degree polynomial operators (II)

Abstract

In this paper we apply some iterative methods obtained by inverse interpolation, in order to solve some specific classes of equations: the Ricatti equation, a Fredholm type equation, and the eigenvalue problem for a class of linear operators.

We obtain some semilocal convergence results, showing the r-convergence orders of the iterates.

Authors

Keywords

inverse interpolation iterative methods; Ricatti equation; Fredholm type equation; eigenvalue problem; semilocal convergence results; r-convergence order.

Cite this paper as:

E. Cătinaş, I. Păvăloiu, On some interpolatory iterative methods for the second degree polynomial operators (II), Rev. Anal. Numér. Théor. Approx., 28 (1999) no. 2, pp. 133-143.

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Editions de l’Academie Roumaine.

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On some Interpolatory Iterative Methods for the Second Degree Polynomial Operators (II)

On some Interpolatory Iterative Methods
for the Second Degree Polynomial Operators (II)

Emil Cătinaş and Ion Păvăloiu

1. The approximation of the solutions of Riccati differential equations

††1991 AMS Subject Classification: 65J20, 65H17.

Consider the differential equation

(1) y′=a0⁢(x)⁢y2+a1⁢(x)⁢y+a2⁢(x)

where the applications a0,a1,a2:[a,b]→ℝ are continuous on the interval [a,b], a<b and a2 is not the null function.

We are interested to approximate the solution of (1) with the condition

(2) y⁢(a)=ya.

The solution will be searched in the space C1⁢[a,b]. For this purpose we consider the operator F:C1⁢[a,b]→C⁢[a,b] given by

(3) F⁢(y)⁢(x)=y′⁢(x)−a0⁢(x)⁢y2⁢(x)−a1⁢(x)⁢y⁢(x)−a2⁢(x).

The first and second order divided differences of F are given by

(4) [y1,y2;F]⁢h⁢(x)=h′⁢(x)−(a0⁢(x)⁢(y1⁢(x)+y2⁢(x))+a1⁢(x))⁢h⁢(x)

respectively

(5) [y1,y2,y3;F]⁢h⁢(x)⁢k⁢(x)=−a0⁢(x)⁢h⁢(x)⁢k⁢(x),

for all y1,y2,y3,h,k∈C1⁢[a,b].

Formula (5) shows that the divided differences of order higher than two are the null multilinear operators.

Let y0,y1∈C1⁢[a,b] be given. The chord iterates yk∈C1⁢[a,b], k=2,3,… are constructed by

(6) [yk−1,yk;F]⁢(yk+1−yk)+F⁢(yk)=0,k=1,2,…

As we shall see, the above equations lead to some first order linear nonhomogeneous differential equations.

Replacing in (6) the expression (4) of F we get for yk+1 the following differential equation.

(7) yk+1′⁢(x)=φk⁢(x)⁢yk+1⁢(x)+ψk⁢(x),

where we have denoted

φk⁢(x) = a0⁢(x)⁢(yk−1⁢(x)+yk⁢(x))+a1⁢(x)and
ψk⁢(x) = −a0⁢(x)⁢yk⁢(x)⁢yk−1⁢(x)+a2⁢(x).

For solving (7) consider the condition

(8) yk+1⁢(a)=ya,

so we are led to the expression of yk+1:

(9) yk+1⁢(x)=exp⁡(∫axφk⁢(s)⁢𝑑s)⁢(ya+∫axψk⁢(s)⁢exp⁡(−∫asφk⁢(t)⁢𝑑t)⁢𝑑s).

We are interested to find a bound for ‖[y0,y1;F]−1‖.

For this purpose consider the problem

{[y0,y1;F]⁢h⁢(x)=u⁢(x),u∈C⁢[a,b]h⁢(a)=0

which has the solution

h⁢(x)=exp⁡(∫axφ1⁢(s)⁢𝑑s)⁢∫axu⁢(s)⁢exp⁡(−∫asφ1⁢(t)⁢𝑑t)⁢𝑑s.

This equality yields

(10) ‖[y0,y1;F]−1‖≤supx∈[a,b]exp⁡(∫axφ1⁢(s)⁢𝑑s)⁢∫axexp⁡(−∫asφ1⁢(t)⁢𝑑t)⁢𝑑s.

For the second order divided differences we have

(11) ‖[u,v,w;F]‖≤supx∈[a,b]|a0⁢(x)|.

Now denote

b¯0 = supx∈[a,b]exp⁡(∫axφ1⁢(s)⁢𝑑s)⁢∫axexp⁡(−∫asφ1⁢(t)⁢𝑑t)⁢𝑑s;
α¯ = supx∈[a,b]|a0⁢(x)|
d¯0 = supx∈[a,b]|y1⁢(x)−y0⁢(x)|
B¯r¯⁢(y0) = {y∈C1⁢[a,b]|supx∈[a,b]|y⁢(x)−y0⁢(x)|≤r¯}.

With the above notations and taking into account relations (10) and (11), Theorem 4.1 from [6] implies:

Theorem 1.1.

Assume the functions y0,y1∈C1⁢[a,b],a0,a1,a2∈C⁢[a,b] and the real positive numbers b¯0, α¯, d¯0 and r¯ satisfy the following conditions:

a) b¯0⁢α¯⁢(2⁢r¯+d¯0)=q<1;

b) ε0=α¯⁢b¯⁢supx∈[a,b]|F⁢(y0)⁢(x)|<1,α¯⁢b¯⁢supx∈[a,b]|F⁢(y1)⁢(x)|≤ε0l, where b¯=b¯01−q and l=1+52;

c) ε0lα¯⁢b¯⁢(1−ε0)+d¯0≤r¯.

Then the sequence (yk)k≥0 given by (9) converges uniformly and its elements lie in the ball B¯r¯⁢(y0). Denoting y∗=limk→∞yk then y∗ is a solution of (1)-(2). Moreover, the following estimation hold:

supx∈[a,b]|y∗⁢(x)−yk⁢(x)|≤ε0lkα¯⁢b¯⁢(1−ε0l),k=2,3,…

2. The approximation of the solutions of Fredholm integral equations

Consider the integral equation

(12) φ⁢(t)=λ⁢∫aba1⁢(t,s)⁢φ⁢(s)⁢𝑑s+μ⁢∫aba2⁢(t,s)⁢φ2⁢(s)⁢𝑑s+f⁢(t),

where λ,μ∈ℝ, a1,a2∈C⁢[a,b]2 and f∈C⁢[a,b].

Here we take the operator F:C⁢[a,b]→C⁢[a,b] given by

(13) F⁢(φ)⁢(t)=φ⁢(t)−λ⁢∫aba1⁢(t,s)⁢φ⁢(s)⁢𝑑s−μ⁢∫aba2⁢(t,s)⁢φ2⁢(s)⁢𝑑s−f⁢(t)

The first and the second order divided differences of F on u,v,w∈C⁢[a,b] are given by the following relations:

(14) [u,v;F]⁢h⁢(t)=h⁢(t)−λ⁢∫aba1⁢(t,s)⁢h⁢(s)⁢𝑑s−μ⁢∫aba2⁢(t,s)⁢[u⁢(s)+v⁢(s)]⁢h⁢(s)⁢𝑑s[u,v,w;F]⁢h⁢(t)⁢k⁢(t)=−μ⁢∫aba2⁢(t,s)⁢h⁢(s)⁢k⁢(s)⁢𝑑s

where h,k∈C⁢[a,b].

Let φ0,φ1∈C⁢[a,b] be given. As in the previous section, we shall construct the sequence (φk)k≥0⊂C⁢[a,b] with the solutions of the following linear integral equations

(15) [φk−1,φk;F]⁢(φk+1−φk)+F⁢(φk)=0,k=1,2,…

From (15), by (13) and (14) we get for φk+1 the following linear integral Fredholm equation

(16) φk+1⁢(t)= λ⁢∫aba1⁢(t,s)⁢φk+1⁢(s)⁢𝑑s
+μ⁢∫aba2⁢(t,s)⁢(φk−1⁢(s)+φk⁢(s))⁢φk+1⁢(s)⁢𝑑s+Gk⁢(t)

where

(17) Gk⁢(t)=f⁢(t)−μ⁢∫aba2⁢(t,s)⁢(φk−1⁢(s)+φk⁢(s))⁢𝑑s.

In order to consider Theorem 4.1 [6] for the convergence of the sequence (φk)k≥0 we need a bound for the operator [φ0,φ1;F]−1. In this respect we take the following equation

[φ0,φ1;F]⁢h⁢(t)=u⁢(t), with ⁢λ≠0,

i.e.

(18) h⁢(t)=λ⁢∫aba1⁢(t,s)⁢h⁢(s)⁢𝑑s+μ⁢∫aba2⁢(t,s)⁢(φ0⁢(s)+φ1⁢(s))⁢h⁢(s)⁢𝑑s+u⁢(t).

We shall assume that this equation has a unique solution. Denote K0⁢(t,s,λ,μλ) the corresponding ”resolvent” kernel. Then the solution of (18) has the following form:

(19) h⁢(t)=u⁢(t)+λ⁢∫abK0⁢(t,s,λ,μλ)⁢u⁢(s)⁢𝑑s.

It can be easily seen by the above considerations that the following hold:

(20) ‖[φ0,φ1;F]−1‖≤1+|λ|⁢(b−a)⁢supa≤t,s≤b|K0⁢(t,s,λ,μλ)|.

At the same time, the norm of [u,v,w;F] is bounded by

‖[u,v,w;F]‖≤|μ|⁢(b−a)⁢supa≤t,s≤b|a2⁢(t,s)|.

We make the following notations:

b~0 = 1+|λ|⁢(b−a)⁢supa≤t,s≤b|K0⁢(t,s,λ,μλ)|
α~ = |μ|⁢(b−a)⁢supa≤t,s≤b|a2⁢(t,s)|
d~0 = supt∈[a,b]|φ1⁢(t)−φ0⁢(t)|
B¯r~⁢(φ0) = {φ∈C⁢[a,b]|supt∈[a,b]|φ⁢(t)−φ0⁢(t)|≤r~}

Theorem 4.1 from [6] then implies the next result.

Theorem 2.1.

Assume the functions a1,a2∈C⁢([a,b]2) and the real numbers λ,μ,b~0,α~,d~0 and r~ satisfy the following conditions:

a) b~0⁢α~⁢(2⁢r~+d~0)=q~<1;

b) ε0=α~⁢b~2⁢‖F⁢(φ0)‖<1,ρ1=α~⁢b~⁢‖F⁢(φ1)‖≤ε0l, where
‖F⁢(φi)‖=supt∈[a,b]|F⁢(φi)⁢(t)|,i=1,2;b~=b~01−q~ and l=1+52;

c) ε0lα~⁢b~⁢(1−ε0)+d~0≤r~.

Then the sequence (φk)k≥0 generated by (16) converges uniformly and its elements lie in B¯r~⁢(φ0). Denoting φ∗=limk→∞φk then φ∗ is a solution of the integral equation (12) and the following estimations hold:

supt∈[a,b]|φ∗⁢(t)−φk⁢(t)|≤ε0lkα~⁢b~⁢(1−ε0l),k=2,3,…

As we have seen, the chord method requires the solving of a linear integral Fredholm equation at each iteration step. The problem takes a simplified form from the practical viewpoint when the kernels a1 and a2 from (12) are degenerate. In this case the linear integral equations (16) will be also with degenerate kernels, as can be easily seen. We shall consider in the following this particular case.

Let αi,βi∈C⁢[a,b], i=1,…,p two sets containing p linear independent functions and also γi,δi∈C⁢[a,b], i=1,…,m two other sets with the same properties.

Assume the kernels a1 and a2 have the following form:

a1⁢(t,s) = ∑i=1pαi⁢(t)⁢βi⁢(s)and
a2⁢(t,s) = ∑i=1mγi⁢(t)⁢δi⁢(s).

It can be verified without difficulty that the solution φk+1 of equation (16) has the form

(21) φk+1⁢(t)=λ⁢∑i=1pαi⁢(t)⁢∫abβi⁢(s)⁢φk+1⁢(s)⁢𝑑s++μ⁢∑i=1mγi⁢(t)⁢∫abδi⁢(s)⁢(φk−1⁢(s)+φk⁢(s))⁢φk+1⁢(s)⁢𝑑s+Gk⁢(t).

Consider the following notations:

xi(k+1)=∫abβi⁢(s)⁢φk+1⁢(s)⁢𝑑s,i=1,…,pyi(k+1)=∫abδi⁢(s)⁢(φk−1⁢(s)+φk⁢(s))⁢φk+1⁢(s)⁢𝑑s,i=1,…,mai⁢j=∫abαi⁢(t)⁢βj⁢(t)⁢𝑑t,i,j=1,…,pbi⁢j=∫abγi⁢(t)⁢βj⁢(t)⁢𝑑t,i=1,…,m,j=1,…,pAj⁢i(k+1)=∫abαi⁢(t)⁢δj⁢(t)⁢(φk⁢(t)+φk−1⁢(t))⁢𝑑t,i=1,…,p,j=1,…,mBj⁢i(k+1)=∫abγi⁢(t)⁢δj⁢(t)⁢(φk⁢(t)+φk−1⁢(t))⁢𝑑ti,j=1,…,mθj(k+1)=∫abβj⁢(t)⁢Gk⁢(t)⁢𝑑tj=1,…,pεj(k+1)=∫abδj⁢(t)⁢(φk⁢(t)+φk−1⁢(t))⁢Gk⁢(t)⁢𝑑tj=1,…,m

We obtain then for φk+1 the expression

(22) φk+1⁢(t)=λ⁢∑i=1pxi(k+1)⁢αi⁢(t)+μ⁢∑i=1myi(k+1)⁢γi⁢(t)+Gk⁢(t),

where xi(k+1), i=1,…,p and yi(k+1), i=1,…,m represent the solution of the linear system

(23) X(k+1) = λ⁢U⁢X(k+1)+μ⁢V⁢Y(k+1)+θ(k+1)
Y(k+1) = λ⁢W(k+1)⁢X(k+1)+μ⁢T(k+1)⁢Y(k+1)+ε(k+1)

where

U = (aj⁢i)1≤i,j≤p,V=(bj⁢i)1≤i≤p1≤j≤m,
W(k+1) = (Aj⁢i)1≤i≤p1≤j≤m,T(k+1)=(Bj⁢i)1≤i,j≤m,
X(k+1) = (x1(k+1),x2(k+1),…,xp(k+1))T,
Y(k+1) = (y1(k+1),y2(k+1),…,ym(k+1))T,
θ(k+1) = (θ1(k+1),θ2(k+1),…,θp(k+1))T,
ε(k+1) = (ε1(k+1),ε2(k+1),…,εm(k+1))T.

It can be easily seen that under the conditions of Theorem 2.1 the sequences (Xk)k≥0 and (Yk)k≥0 converge.

3. The approximation of the eigenpairs of matrices

Denote V=𝕂n and let A∈ 𝕂n×n where 𝕂=ℝ or ℂ. As we have seen in [6], for computing the eigenpairs of A we may consider a mapping G:V→𝕂 with G⁢(0)≠1. The eigenvalues and eigenvectors are the solutions of the nonlinear system

(24) F⁢(x)=(A⁢v−λ⁢vG⁢(v)−1)=0,

where x=(vλ)∈V×𝕂=𝕂n+1. Denoting v=(x(1),x(2),…,x(n)) and λ=x(n+1) then the first n components of F, Fi, i=1,…,n, are given by

Fi⁢(x)=ai⁢1⁢x(1)+⋯+ai,i−1⁢x(i−1)+(ai⁢i−x(n+1))⁢x(i)+ai,i+1⁢x(i+1)+⋯+ai⁢n⁢x(n).

If we take G as

G⁢(v)=a⁢‖v‖2

for some fixed a∈ℝ then

Fn+1⁢(x)=a⁢((x(1))2+⋯+(x(n))2)−1.

The matrices associated to the first order divided differences of F at the points x1,x2∈𝕂n+1 are

[x1,x2;F]=(b11a12⋯a1⁢na1,n+11a21b22⋯a2⁢na2,n+11⋮⋮⋮⋮an⁢1an⁢2⋯bn⁢nan,n+11an+1,1an+1,2⋯an+1,n0)

where bi⁢i=ai⁢i−12⁢(x2(n+1)+x1(n+1)), ai,n+11=−12⁢(x2(i)+x1(i)) and an+1,i=a⁢(x1(i)+x2(i)) for i=1,…,n.

The second order divided differences of F on x1,x2,x3 are given by

[x1,x2,x3;F]⁢h⁢k=(−12⁢k(n+1)0⋯0−12⁢k(1)0−12⁢k(n+1)⋯0−12⁢k(2)⋮⋮⋮⋮00⋯−12⁢k(n+1)−12⁢k(n)a⁢k(1)a⁢k(2)⋯a⁢k(n)0)⁢(h(1)h(2)⋮h(n)h(n+1))

for all h,k∈𝕂n+1.

We shall consider the max norm on V and taking ‖x‖=max⁡{‖v‖∞,|λ|} for all x=(vλ)∈𝕂n+1 we are led to the max norm on 𝕂n+1. It can be easily verified that

‖[x1,x2,x3;F]‖∞≤max⁡{1,n⁢|a|}.

Let x0,x1∈𝕂n+1 be such that [x0,x1,F] is nonsingular. Denote b^0=‖[x0,x1;F]−1‖∞, d^0=‖x0−x1‖∞, α^=max⁡{1,n⁢|a|} and
B¯r^={x∈𝕂n+1|‖x−x0‖∞≤r^}. Applying Theorem 4.1 from [6] we get

Theorem 3.1.

Assume that the matrix [x0,x1;F] is nonsingular and the numbers b^0,d^,α^ and r^ satisfy :

a) b^0⁢(2⁢r^+d^0)=q^<1;

b) ε0=b2⁢‖F⁢(x0)‖∞<1,b2⁢‖F⁢(x0)‖≤ε0l where b=b^01−q^ and l=1+52;

c) ε0lb⁢(1−ε0)+d^0≤r^.

Then the sequence (xk)k≥0 given by the iterations [xk−1,xk;F]⁢(xk+1−xk)+F⁢(xk)=0, k=1,2,… lie in the ball B¯r^⁢(x0) and converges. Denoting x∗=limk→∞xk then F⁢(x∗)=0 and the following estimations hold

‖x∗−xk‖∞≤ε0lkb⁢(1−ε0l),k=2,3,…

4. Numerical examples

We shall consider two test matrices††These matrices are available from MatrixMarket at the following address: http://math.nist.gov/MatrixMarket/. in order to study the behavior of the chord method for approximating the eigenpairs. The programs were written in Matlab††MATLAB is a registered trademark of the MathWorks, Inc. and were run on a PC.

Pores1 matrix. This matrix arise from oil reservoir simulation. It is real, unsymmetric, of dimension 30 and has 20 real eigenvalues. We have chosen to study the largest eigenvalue λ∗=−1.836 3⋅10+1. The initial approximations were taken λ0=λ∗+0.5 and λ1=λ∗+0.25; for the initial vector v0 we perturbed the solution v∗ (computed by Matlab and then properly scaled to fulfill the norming equation) with random vectors having the components uniformly distributed on (-ε,ε), ε=0.2; for the vector v1 we halved the perturbation. The following results are typical for the runs made (we have considered here the same vector ε for the four initial approximations), where for choice I we took in G a=12, while for choice II a=12⁢n.

Fidap002 matrix. This real symmetric matrix of dimension n=441 arise from finite element modeling. Its eigenvalues are all simple and range from

Choice I Choice II
k ‖x∗−xk‖ ‖F⁢(xk)‖ ‖x∗−xk‖ ‖F⁢(xk)‖
0 8.533 3⋅10-01 1.793 8⋅10+06 8.533 3⋅10-01 1.793 8⋅10+06
1 4.266 7⋅10-01 8.969 1⋅10+05 4.266 7⋅10-01 8.969 0⋅10+05
2 7.860 1⋅10-02 2.060 9⋅10-01 1.624 5⋅10-02 1.722 1⋅10-01
3 6.683 1⋅10-03 9.518 0⋅10-03 2.908 6⋅10-04 1.967 7⋅10-03
4 1.764 7⋅10-04 2.500 7⋅10-04 2.978 3⋅10-07 2.140 5⋅10-06
5 2.370 6⋅10-07 3.345 8⋅10-07 7.586 2⋅10-11 9.143 0⋅10-10
6 4.662 4⋅10-10 8.231 7⋅10-10

Table 1. The chord method for Pores1.

−7⋅108 to 3⋅106. We have chosen to study the smallest eigenvalue, which is well separated. The initial approximations were taken λ0=λ∗+102=−6.9996⋅108+100, resp. λ1=λ∗+10; for the initial vector v0 we perturbed the solution v∗ with random vectors having the components uniformly distributed on (-ε,ε), ε=0.5; for the vector v1 we halved the perturbation. The following results are typical for the runs made (we have considered a common vector ε).

Choice I Choice II
k ‖x∗−xk‖ ‖F⁢(xk)‖ ‖x∗−xk‖ ‖F⁢(xk)‖
0 1.000 3⋅10+2 1.746 7⋅10+09 2.510 7⋅10+00 1.746 7⋅10+09
1 1.007 8⋅10+1 8.733 5⋅10+08 1.255 3⋅10+00 8.733 5⋅10+08
2 3.485 3⋅10+1 1.646 2⋅10+02 5.287 7⋅10-02 3.564 1⋅10-03
3 2.136 8⋅10+0 2.337 3⋅10+01 6.180 4⋅10-05 4.904 8⋅10-06
4 4.476 1⋅10-1 6.352 1⋅10-01 5.985 8⋅10-07 4.430 9⋅10-06
5 6.521 4⋅10-3 9.223 8⋅10-03
6 1.561 7⋅10-5 2.296 1⋅10-05
7 5.960 5⋅10-7 8.564 7⋅10-08

Table 2. The secant method for Fidap002.

References

Received: March 3, 1998.

Romanian Academy

P.O. Box 68

3400 Cluj-Napoca 1

Romania

1999

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