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Subsections

3 The Markov-Bernstein majorant

3.1 What is to solve

Inequalities like $ \forall f\in S\; :\; \left\langle f' \vert f' \right\rangle \leq Cte\, \left\langle f \vert f \right\rangle $ are known as "Markov-Bernstein inequality". When dealing with polynomials, the natural choice for the sets $ S $ are the $ \mathbb{R}_{n}\left[ X\right] $, i.e. the sets of polynomials whose degree is bounded by some integer $ n $. Obviously, the bounding factor is an increasing function of $ n $, and an asymptotic estimate is of interrest.

Defining $ A_{n} $ and $ B_{n} $ by $ A_{n}\left[ j,\, k\right] =\left\langle F_{j} \vert F_{k} \right\rangle $ and $ B_{n}\left[ j,\, k\right] =\left\langle F_{j}' \vert F_{k}' \right\rangle $ where $ 1\leq j,\, k\leq n $, we obtain to $ n\times n $ matrices, the former being positive diagonal and the later being positive symmetric (and half-sparse, due to parity considerations). Defining $ \chi _{n}\left( \mu \right) $ as $ \det \left( A_{n}\, \mu -B_{n}\right) \div \det \left( A_{n}\right) $, we obtain an unitary real polynomial of degree $ n $ whose roots are positive, the greatest of them being the requested Markov-Bernstein factor. In fact, recurrence relations are easier to obtain regarding the $ \varphi _{n} $ defined as $ \varphi _{n}\left( \lambda \right) =\lambda ^{n}\, \chi _{n}\left( 1/\lambda \right) $, the Markov-Bernstein factor being now the reciprocal of the least root of $ \varphi _{n}\left( \lambda \right) $.

Let us take the example $ \alpha =0,\, n=4 $. One obtains

$\displaystyle \mu \, A_{4}-B_{4}=\left[ \begin{array}{cccc}
\frac{1}{2}\mu -1 &...
...\frac{1}{2}\mu -27 & 0\\
0 & -16 & 0 & \frac{1}{2}\mu -64
\end{array}\right] $

leading to $ \chi _{4}\left( \mu \right) =\mu ^{4}-200\, \mu ^{3}+9160\, \mu ^{2}-67712\, \mu +73728 $, whose roots are $ 72+8\, \sqrt{65}\approx 136.498 $, $ 72-8\, \sqrt{65}\approx 7.502 $, $ 28+2\, \sqrt{178}=54.683 $ and $ 28-2\, \sqrt{178}=1.317 $. The coordinates of the eigenvectors are $ \left[ \, 0,\, \frac{-7\pm \sqrt{65}}{4},\, 0,\, 1\, \right] $ and $ \left[ \, \frac{-13\pm \sqrt{178}}{3},\, 0,\, 1,\, 0\, \right] $, the corresponding polynomials being $ t^{4}+\frac{-23\pm \sqrt{65}}{16}\, t^{2}+\frac{11\mp \sqrt{65}}{32} $ and $ t^{3}+\frac{-22\pm \sqrt{178}}{12}\, t $. Therefore the Markov-Bernstein factor (relative to the Chebyschev scalar product) is $ 28+2\sqrt{178} $ over $ \mathbb{R}_{3}\left[ X\right] $ and $ 72+8\sqrt{65} $ over $ \mathbb{R}_{4}\left[ X\right] $.

3.2 Recurence over the $ \chi _{n}$

From EQ. 20, it can be seen that $ r_{n}\doteq \left\langle F_{m}' \vert F_{n}' \right\rangle \div \left\langle F_{m}' \vert F_{n+2}' \right\rangle $ is, for a given $ n $, constant for all $ m $ such that $ n-m\in 2\mathbb{N}$. Therefore, it is convenient to introduce the triangular sparse matrix $ \mathrm{T}_{n} $ defined by $ T_{j,\, j}=1 $, $ T_{j+2,\, j}=-r_{j}=-\frac{\left( j+1\right) \left( j+2\right) }{\left( \alpha +j\right) \left( \alpha +j+1\right) } $ and $ T_{j,\, k}=0 $ elsewhere. Defining the matrix $ \mathrm{M}_{n}\doteq \mathrm{T}_{n}\, \left( \mu \, \mathrm{A}_{n}-\mathrm{B}_{n}\right) \, ^{t}\mathrm{T}_{n} $, we have the obvious relation $ \chi _{n}\left( \mu \right) =\det \mathrm{M}_{n}\div \det \mathrm{A}_{n} $, and now $ M_{j,\, k}=0 $ except when $ j-k\in \left\{ -2,\, 0,\, 2\right\} $. Some computations give :

\begin{displaymath}
\begin{array}{rcl}
M_{j,\, j} & = & \left( \frac{\mu \, \lef...
... \, \frac{\alpha !\, j!}{\left( \alpha +j\right) !}
\end{array}\end{displaymath}

except from $ M_{2,\, 2} $ whose value remains $ \mu \frac{2}{\left( \alpha +4\right) \left( \alpha +1\right) }-\frac{4\left( \alpha +2\right) }{\left( \alpha +1\right) ^{2}} $ since no eliminations are occurring.

That special form of matrix $ \mathrm{M}_{n} $ induces the recurrence

$\displaystyle \det \mathrm{M}_{n}=M_{n,\, n}\, \det \mathrm{M}_{n-1}-M_{n,\, n-...
..._{n-3}+\left( M_{n,\, n-2}\, M_{n-1,\, n-3}\right) ^{2}\, \det \mathrm{M}_{n-4}$

Going back to the $ \chi _{n}$, and then to the $ \psi _{n} $, we obtain :

$\displaystyle \chi _{n}=\left\{ \begin{array}{l}
\chi _{n-1}\left( \mu \; \frac...
...n+\alpha \right) ^{2}\, \left( \alpha +n-3\right) }\right)
\end{array}\right. $

$\displaystyle \psi _{n}=\left\{ \begin{array}{l} \psi _{n-1}\left( -\lambda \; ...
...\alpha +n-2\right) ^{2}\, \left( \alpha +n-3\right) }\right) \end{array}\right.$ (21)

3.3 Factorisation of the recurrence relation

Let us define $ \mathbb{E}_{p }\doteq \mathrm{Span}\left( X^{2},\, X^{4},\, \cdots \, X^{2p} \right) =X^{2}\, \mathbb{R}_{p-1}\left[ X^{2}\right] $ (excluding the constants), together with $ \mathbb{O}_{p }\doteq \mathrm{Span}\left( X^{1},\, X^{3},\, \cdots \, X^{2p-1} \right) =X\, \mathbb{R}_{p-1}\left[ X^{2}\right] $, and assume $ n=2p $. The space $ \mathbb{R}_{n}\left[ X\right] $ splits as $ \mathbb{R}\oplus \mathbb{O}_{p }\oplus \mathbb{E}_{p } $, while $ \mathbb{R}_{n+1}\left[ X\right] $ splits as $ \mathbb{R}\oplus \mathbb{O}_{p+1 }\oplus \mathbb{E}_{p } $. Both spaces have the same even subspace in common, and therefore $ \psi _{2p} $ and $ \psi _{2p+1} $ must have a common factor of degree $ p $ (say $ \theta _{2p} $). For the same reason, $ \psi _{2p-1} $ and $ \psi _{2p} $ must have a common factor of degree $ p $ (say $ \theta _{2p-1} $). Therefore, it can be hoped that each polynomial $ \psi _{n} $ splits into $ \psi _{n}=\theta _{n}\, \theta _{n-1} $, the $ \theta _{n}$ being defined by $ \theta _{n}=Cte\, \gcd \left( \psi _{n+1},\, \psi _{n}\right) $ where the $ Cte $ is chosen such that $ \theta _{n}\left( 0\right) =1 $.

This suggest that the $ \theta _{n}$ can be related by a recurrence relation of the form $ \theta _{n}\left( \lambda \right) =\left( \lambda \, a_{n}+b_{n}\right) \theta _{n-2}\left( \lambda \right) +c_{n}\, \theta _{n-4}\left( \lambda \right) $ i.e. a relation dealing separately with odd and even $ \theta _{n}$. Substituting this relation, together with $ \psi _{n}=\theta _{n}\, \theta _{n-1} $ into EQ. 21 and identifying, we obtain

$\displaystyle \theta _{n}=\left\{ \begin{array}{l} \theta _{n-2}\left( -\lambda...
... \, \left( \alpha +n-1\right) \, \left( \alpha +n-2\right) } \end{array}\right.$ (22)

with respective initial conditions $ \theta _{-1}=1,\, \theta _{1}=1-\lambda \left( \alpha +2\right) $ and $ \theta _{0}=1,\, \theta _{2}=1-\lambda \left( \alpha +2\right) \frac{2\left( \alpha +4\right) }{\alpha +1} $. A backwards recurrence a la Fermat shows that $ \theta _{n}$ and $ \theta _{n-2} $ are coprime for all $ n $, and therefore $ \psi _{n} $ and $ \psi _{n-2} $ are also coprime for all $ n $, as expected when trying the $ \psi _{n}=\theta _{n}\, \theta _{n-1} $ decomposition.

From EQ. 22, the recurrence involving the coefficients of $ \theta _{n}$ can easily be obtained. Defining $ c_{j}\left( n\right) $ by $ \theta _{n}\left( \lambda \right) =\sum c_{j}\left( n\right) \lambda ^{j} $, we have

$\displaystyle c_{j}\left( n\right) =\left\{ \begin{array}{l} \frac{\left( \alph...
...ft( \alpha +2n\right) }{\alpha +n-1}c_{j-1}\left( n-2\right) \end{array}\right.$ (23)

As it should be from the very definitions, $ c_{0}\left( n\right) =1 $ satisfies this relation.

3.4 Even and odd numbers

Let us now examine the even case in more details. Starting with $ j=1 $, EQ. 23 can be solved by $ c_{1}\left( n\right) =polynomial\left( n\right) +u\, f\left( n\right) +v\, g\left( n\right) $ where $ f,\, g $ are two independant solutions of the linear equation associated with EQ. 23. Obviously, $ f=1 $ is one of them, and it can be checked that $ g\left( n\right) =\frac{2^{\alpha }\Gamma \left( 2m+3\right) }{8\, \Gamma \left( 2m+\alpha \right) } $ is another ($ \alpha =3 $ appears to be special). By identification, one obtains $ c_{1}\left( n\right) =-\frac{n\left( n+2\right) \left( \alpha +n\right) \left( \alpha +n+2\right) }{4\left( \alpha +1\right) }+u+v\, g\left( n\right) $. Using initial conditions issued from $ \theta _{0} $ and $ \theta _{2} $, it appears that $ u=v=0 $, and $ c_{1}\left( n\right) $ is a polynomial and $ \mathrm{dg}\left( c_{1} \right) =4 $. Iterating the process, we obtain that $ c_{2} $ is a polynomial, with $ \mathrm{dg}\left( c_{2} \right) =8 $, etc.

Rewitting EQ. 23 as $ c_{j}\left( n\right) +\clubsuit c_{j}\left( n-2\right) +\clubsuit c_{j}\left( n-4\right) =\clubsuit c_{j-1}\left( n-2\right) $ and taking the equivalents $ c_{j}\left( n\right) \sim a\, n^{p} $ and $ c_{j-1}\left( n\right) \sim b\, n^{q} $, we obtain $ n^{p-2}\left( 4\alpha \, p\, a+4p^{2}\, a-12p\, a\right) \sim -4n^{q+2}b $, i.e. $ p=q+4 $ and $ a=-\frac{b}{\left( q+4\right) \, \left( q+\alpha +1\right) } $. By recurrence

$\displaystyle c_{j}\left( n\right) \sim n^{4j}\: \prod _{k=1}^{j}\frac{-1}{4k\, \left( \alpha +k-3\right) }$ (24)

Applying the same computations to the odd case, we obtain $ \widehat{c_{1}}\left( n\right) =c_{1}\left( n\right) -\frac{\alpha -1}{4} $, where $ \widehat{c_{1}} $ is the coefficient when $ n $ is odd and $ c_{1}\left( n\right) $ is what is obtained when applying the even formula (to odd numbers, i.e. outside it's domain of validity). Since $ \widehat{c_{1}} $ and $ c_{1} $ are equivalents, the former recurrence shows that EQ. 24 holds for odd numbers too.

3.5 Some results

Let us introduce the new variable $ \nu =\frac{n^{4}}{\mu }=n^{4}\, \lambda $. By EQ. 24, the polynomial in $ \nu $ defined by $ \theta _{n}\left( \nu /n^{4}\right) $ converges towards a series whose coefficients do not depend on $ n $, and it is easy to write that series as an hypergeometric function. We obtain

$\displaystyle \theta _{n}\left( \frac{\nu }{n^{4}}\right) =1-\frac{\nu }{4\left...
...1\right] ,\, \left[ 2,\, \frac{5+\alpha }{4}\right] ,\, -\frac{\nu }{16}\right)$ (25)

Applying this formula to the Chebyschev's polynomials, the smallest root of $ \theta _{n}\left( \frac{\nu }{n^{4}}\right) $ appears to be $ \nu \approx 4.5 $ (cf FIG. 1) leading to $ \mu \approx n^{4}\times .2231266815 $.

FIG.  1: Asymptotic behaviour of $ \theta _{n}$ in the Chebyschev case.
\resizebox*{10cm}{4.5cm}{\includegraphics{asym_cheb.eps}}

For other values of $ \alpha $, one obtains FIG. 2. It appears that $ \alpha =1 $ and $ \alpha =5 $ are special, since the hypergeometric functions can be rewritten in a simpler form : $ 1-\frac{\nu }{8}\mathrm{hypergeom}\left( \left[ 1\right] ,\, \left[ 3/2,\, 2\right] ,\, -\frac{\nu }{16}\right) =\cos \left( \frac{1}{2}\sqrt{\nu }\right) $ and $ 1-\frac{\nu }{24}\mathrm{hypergeom}\left( \left[ 1\right] ,\, \left[ 2,\, 5/2\...
...sin \left( \frac{1}{2}\sqrt{\nu }\right) /\left( \frac{1}{2}\sqrt{\nu }\right) $.

FIG.  2: Markov-Bernstein factor for some $ \alpha $.
\begin{figure}{\centering\begin{tabular}{\vert c\vert c\vert c\vert}
\hline
\( ...
...i ^{2} \)&
\( n^{4}/16\pi ^{2} \)\\
\hline
\end{tabular}\par }
\par\end{figure}


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Previous: 2 Orthogonal polynomials over Up: About Orthogonal Polynomials Next: Bibliography   Contents


douillet@ensait.fr
2002-01-30