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Untitled - Cdm.unimo.it

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Numerical Integration 53<br />

The proof is completed using (2.2.10). For the weights relative to the endpoints, we<br />

wr<strong>it</strong>e<br />

(3.5.5) 0 =<br />

1<br />

−1<br />

= 2un(−1)u ′ n−1(−1) ˜w (n)<br />

0<br />

unu ′ n−1(1 − x)w dx =<br />

n<br />

m=0<br />

(unu ′ n−1)(η (n)<br />

m )(1 − η (n)<br />

m ) ˜w (n)<br />

m<br />

− 2α+β (2n + α + β)Γ(n + α)Γ(n + β)<br />

(n + α + β + 1) n! Γ(n + α + β)<br />

n−1 <br />

m=1<br />

(1 − η (n)<br />

m ).<br />

The first equal<strong>it</strong>y in (3.5.5) is due to orthogonal<strong>it</strong>y, while in the last equal<strong>it</strong>y we used<br />

the expression of the weights obtained above for 1 ≤ m ≤ n − 1. Then, by (1.3.3) and<br />

(3.1.18) we deduce the value of ˜w (n)<br />

0 . In the same way one gets the value of ˜w (n)<br />

n .<br />

In the ultraspherical case, since the polynomials are even or odd, the nodes are<br />

symmetrically distributed in [−1,1]. Therefore, when α = β we have n−1<br />

j=m η(n)<br />

m = 0.<br />

Hence, in the Legendre case we obtain<br />

(3.5.6) ˜w (n)<br />

j<br />

=<br />

⎧<br />

2<br />

⎪⎨ n(n + 1)<br />

⎪⎩<br />

−2<br />

<br />

Pn(η<br />

n + 1<br />

(n)<br />

j )P ′ n−1(η (n)<br />

−1 j )<br />

if j = 0 or j = n,<br />

if 1 ≤ j ≤ n − 1.<br />

For the Chebyshev case, relations (3.5.2) are drastically simplified and give<br />

(3.5.7) ˜w (n)<br />

j<br />

=<br />

⎧<br />

π<br />

⎪⎨ 2n<br />

⎪⎩<br />

π<br />

n<br />

if j = 0 or j = n,<br />

if 1 ≤ j ≤ n − 1.<br />

This is a consequence of (3.1.15) and the relation T ′ n−1(η (n)<br />

j ) = −(n − 1)(−1) j+n ,<br />

1 ≤ j ≤ n − 1.<br />

Also for Gauss-Lobatto formulas <strong>it</strong> is possible to prove that the weights are pos<strong>it</strong>ive.<br />

More about the subject can be found in engels(1980) or davis and rabinow<strong>it</strong>z(1984).<br />

Integration formulas of Gauss-Lobatto type allow the determination of the weighted

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