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Untitled - Cdm.unimo.it

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Numerical Integration 57<br />

the first part. Subst<strong>it</strong>uting x = η (n)<br />

j , 1 ≤ j ≤ n − 1, the terms containing u ′ n vanish.<br />

When (3.8.4) is achieved, the proof is straightforward w<strong>it</strong>h the help of (3.5.2), (3.1.17)<br />

and (3.1.18).<br />

In particular, when α = −1 2 , (3.8.4) yields<br />

(3.8.5) Tn 2 w,n = π, ∀n ≥ 1.<br />

For any fixed n ≥ 1, the two norms · w and · w,n defined in Pn are equivalent.<br />

This means that <strong>it</strong> is possible to find two constants γ1 > 0,γ2 > 0, such that<br />

(3.8.6) γ1 pw,n ≤ pw ≤ γ2 pw,n, ∀p ∈ Pn.<br />

This is not surprising, since in a fin<strong>it</strong>e dimensional space (such as Pn) any two norms<br />

are always equivalent. More important is the following statement, which we prove in<br />

the ultraspherical case.<br />

Theorem 3.8.2 - The constants γ1 and γ2 in (3.8.6) do not depend on n.<br />

Proof - Expanding p w<strong>it</strong>h respect to the orthogonal basis {uk}0≤k≤n, we can wr<strong>it</strong>e<br />

p = cnun + r, where r ∈ Pn−1. Using that (3.5.1) is true in P2n−1, one obtains<br />

(3.8.7) p 2 w,n = c 2 n un 2 w,n + 2cn (un,r)w,n + r 2 w,n<br />

= c 2 n un 2 w,n + 2cn(un,r)w + r 2 w = c 2 n<br />

<br />

un 2 w,n − un 2 2<br />

w + pw, ∀p ∈ Pn.<br />

By direct comparison of (2.2.10) and (3.8.3) we get un 2 w,n ≥ un 2 w, ∀n ≥ 1. This<br />

implies γ2 = 1. On the other hand by (2.3.7) and by the Schwarz inequal<strong>it</strong>y (2.1.7), we<br />

get<br />

(3.8.8) c 2 n =<br />

Thus, subst<strong>it</strong>uting in (3.8.7),<br />

(p,un)w<br />

un 2 w<br />

2<br />

≤ p2 w<br />

un2 , ∀p ∈ Pn.<br />

w

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