Secondary measure

In mathematics, the secondary measure associated with a measure of positive density \rho when there is one, is a measure of positive density \mu, turning the secondary polynomials associated with the orthogonal polynomials for \rho into an orthogonal system.

Contents

Introduction

Under certain assumptions that we will specify further, it is possible to obtain the existence of a secondary measure and even to express it.

For example if one works in the Hilbert space L^2([0,1],\R,\rho)

 \forall x \in [0,1], \;
\mu(x)=\frac{\rho(x)}{\frac{\varphi^2(x)}{4} %2B \pi^2\rho^2(x)}

with

 
\varphi(x) = \lim_{\varepsilon \to 0%2B}
2\int_0^1\frac{(x-t)\rho(t)}{(x-t)^2%2B\varepsilon^2} \, dt

in the general case,

or:

 
\varphi(x) = 
2\rho(x)\text{ln}\left(\frac{x}{1-x}\right) - 2 \int_0^1\frac{\rho(t)-\rho(x)}{t-x} \, dt

when \rho satisfy a Lipschitz condition.

This application \varphi is called the reducer of \rho.

More generally,  \mu et  \rho are linked by their Stieltjes transformation with the following formula:


S_{\mu}(z)=z-c_1-\frac{1}{S_{\rho}(z)}

in which c_1 is the moment of order 1 of the measure  \rho .

These secondary measures, and the theory around them, lead to some surprising results, and make it possible to find in an elegant way quite a few traditional formulas of analysis, mainly around the Euler Gamma function, Riemann Zeta function, and Euler's constant.

They also allowed the clarification of integrals and series with a tremendous effectiveness, though it is a priori difficult.

Finally they make it possible to solve integral equations of the form

 
f(x)=\int_0^1\frac{g(t)-g(x)}{t-x}\rho(t)\,dt

where g is the unknown function, and lead to theorems of convergence towards the Chebyshev and Dirac measures.

The broad outlines of the theory

Let \rho be a measure of positive density on an interval I and admitting moments of any order. We can build a family (P_n)_{n\in \N} of orthogonal polynomials for the inner product induced by \rho. Let us call (Q_n)_{n \in \N} the sequence of the secondary polynomials associated with the family P. Under certain conditions there is a measure for which the family Q is orthogonal. This measure, which we can clarify from \rho is called a secondary measure associated initial measure \rho.

When \rho is a probability density function, a sufficient condition so that \mu , while admitting moments of any order can be a secondary measure associated with \rho is that its Stieltjes Transformation is given by an equality of the type:

S_{\mu}(z)=a\left(z-c_1-\frac{1}{S_{\rho}(z)}\right),

a is an arbitrary constant and \, c_1 indicating the moment of order 1 of \rho.

For a=1 we obtain the measure known as secondary, remarkable since for n\geq1 the norm of the polynomial P_n for \rho coincides exactly with the norm of the secondary polynomial associated Q_n when using the measure \mu.

In this paramount case, and if the space generated by the orthogonal polynomials is dense in L^2\left(I,\mathbf R,\rho \right), the operator T_\rho defined by f(x) \mapsto \int_I \frac{f(t)-f(x)}{t-x}\rho (t)dt creating the secondary polynomials can be furthered to a linear map connecting space L^2\left(I,\mathbf R,\rho \right) to L^2\left(I,\mathbf R,\mu \right) and becomes isometric if limited to the hyperplane H_\rho of the orthogonal functions with P_0=1.

For unspecified functions square integrable for \rho we obtain the more general formula of covariance:

 \langle f/g \rangle_\rho - \langle f/1 \rangle_\rho\times \langle g/1\rangle_\rho = \langle T_\rho(f)/T_\rho (g) \rangle_\mu.

The theory continues by introducing the concept of reducible measure, meaning that the quotient \frac{\rho}{\mu} is element of L^2\left(I,\mathbf R,\mu \right). The following results are then established:

The reducer \varphi of \rho is an antecedent of \frac{\rho}{\mu} for the operator T_\rho. (In fact the only antecedent which belongs to H_\rho).

For any function square integrable for \rho, there is an equality known as the reducing formula:  \langle f/\varphi \rangle_\rho = \langle T_\rho (f)/1 \rangle_\rho.

The operator f\mapsto {\varphi\times f -T_\rho (f)} defined on the polynomials is prolonged in an isometry S_\rho linking the closure of the space of these polynomials in L^2\left(I,\mathbf R,\frac {\rho^2}{\mu}\right) to the hyperplane H_\rho provided with the norm induced by \rho.

Under certain restrictive conditions the operator S_\rho acts like the adjoint of T_\rho for the inner product induced by \rho.

Finally the two operators are also connected, provided the images in question are defined, by the fundamental formula of composition:

T_\rho\circ S_\rho \left( f\right)=\frac{\rho}{\mu}\times \left(f \right).

Case of the Lebesgue measure and some other examples

The Lebesgue measure on the standard interval \left[0,1\right] is obtained by taking the constant density \rho(x)=1.

The associated orthogonal polynomials are called Legendre polynomials and can be clarified by P_n(x)=\frac{d^{(n)}}{dx^n}\left(x^n(1-x)^n\right). The norm of P_n is worth \frac{n!}{\sqrt{2n%2B1}}. The recurrence relation in three terms is written:

2(2n%2B1)XP_n(X)=-P_{n%2B1}(X)%2B(2n%2B1)P_n(X)-n^2P_{n-1}(X).

The reducer of this measure of Lebesgue is given by \varphi(x)=2\ln\left(\frac{x}{1-x}\right). The associated secondary measure is then clarified as : \mu(x)=\frac{1}{\ln^2\left(\frac{x}{1-x}\right)%2B\pi^2}.

If we normalize the polynomials of Legendre, the coefficients of Fourier of the reducer \varphi related to this orthonormal system are null for an even index and are given by C_n(\varphi)=-\frac{4\sqrt{2n%2B1}}{n(n%2B1)} for an odd index n.

The Laguerre polynomials are linked to the density \rho(x)=e^{-x} on the interval I = \left[0,%2B\infty \right).

They are clarified by

L_n(x)=\frac{e^x}{n!}\frac{d^n}{dx^n}(x^ne^{-x})=\sum_{k=0}^{k=n}\binom{n}{k}(-1)^k\frac{x^k}{k!}

and are normalized.

The reducer associated is defined by

\varphi(x)=2\left[\ln(x)-\int_0^{%2B\infty}e^{-t}\ln|x-t|dt\right].

The coefficients of Fourier of the reducer \varphi related to the Laguerre polynomials are given by

C_n(\varphi)=-\frac{1}{n}\sum_{k=0}^{k=n-1}\frac{1}{\binom{n-1}{k}}.

This coefficient C_n(\varphi) is no other than the opposite of the sum of the elements of the line of index n in the table of the harmonic triangular numbers of Leibniz.

The Hermite polynomials are linked to the Gaussian density

\rho(x)=\frac{e^{-\frac{x^2}{2}}}{\sqrt{2\pi}} on I=\ R.

They are clarified by

H_n(x)=\frac{1}{\sqrt{n!}}e^{\frac{x^2}{2}}\frac{d^n}{dx^n}\left(e^{-\frac{x^2}{2}}\right)

and are normalized.

The reducer associated is defined by

\varphi(x)=-\frac{2}{\sqrt{2\pi}}\int_{-\infty}^{%2B\infty}te^{-\frac{t^2}{2}}\ln|x-t|\,dt.

The coefficients of Fourier of the reducer \varphi related to the system of Hermite polynomials are null for an even index and are given by

C_n(\varphi)=(-1)^{\frac{n%2B1}{2}}\frac{\left(\frac{n-1}{2}\right)!}{\sqrt{n!}}

for an odd index n.

The Chebyshev measure of the second form. This is defined by the density \rho(x)=\frac{8}{\pi}\sqrt{x(1-x)} on the interval [0,1].

It is the only one which coincides with its secondary measure normalised on this standard interval. Under certain conditions it occurs as the limit of the sequence of normalized secondary measures of a given density.

Examples of non reducible measures.

Jacobi measure of density \rho(x)=\frac{2}{\pi}\sqrt{\frac{1-x}{x}} on (0, 1).

Chebyshev measure of the first form of density \rho(x)=\frac{1}{\pi\sqrt{1-x^2}} on (−1, 1).

Sequence of secondary measures

The secondary measure \mu associated with a probability density function \rho has its moment of order 0 given by the formula d_0 =c_2 -(c_1)^2 , (c_1 and c_2 indicating the respective moments of order 1 and 2 of \rho).

To be able to iterate the process then, one 'normalizes' \mu while defining \rho_1 =\frac{\mu}{d_0} which becomes in its turn a density of probability called naturally the normalised secondary measure associated with \rho.

We can then create from \rho_1 a secondary normalised measure \rho_2, then defining \rho_3 from \rho_2 and so on. We can therefore see a sequence of successive secondary measures, created from \rho_0=\rho, is such that \rho_{n%2B1} that is the secondary normalised measure deduced from \rho_{n}

It is possible to clarify the density \rho_n by using the orthogonal polynomials P_n for \rho, the secondary polynomials Q_n and the reducer associated \varphi. That gives the formula

\rho_n(x)=\frac{1}{d_0^{n-1}} \frac{\rho(x)}{\left(P_{n-1}(x) \frac{\varphi(x)}{2}-Q_{n-1}(x)\right)^2 %2B \pi^2\rho^2(x) P_{n-1}^2(x)}.

The coefficient d_0^{n-1} is easily obtained starting from the leading coefficients of the polynomials P_{n-1} and P_n. We can also clarify the reducer \varphi_n associated with \rho_n, as well as the orthogonal polynomials corresponding to \rho_n.

A very beautiful result relates the evolution of these densities when the index tends towards the infinite and the support of the measure is the standard interval \left[0,1\right].

Let xP_n (x)=t_nP_{n%2B1}(x)%2Bs_nP_n(x)%2Bt_{n-1}P_{n-1}(x) be the classic recurrence relation in three terms.

If \lim_{n \mapsto \infty}t_n=\frac{1}{4} and \lim_{n \mapsto \infty}s_n=\frac{1}{2}, then the sequence n\mapsto \rho_n converges completely towards the Chebyshev density of the second form \rho_{tch}(x)=\frac{8}{\pi}\sqrt{x(1-x)}.

These conditions about limits are checked by a very broad class of traditional densities.

Equinormal measures

One calls two measures thus leading to the same normalised secondary density. It is remarkable that the elements of a given class and having the same moment of order 1 are connected by a homotopy. More precisely, if the density function \rho has its moment of order 1 equal to c_1, then these densities equinormal with \rho are given by a formula of the type: \rho_{t}(x)=\frac{t\rho(x)}{\left[\left(t-1\right)(x-c_1)\frac{\varphi\left(x\right)}{2}-t\right]^2%2B\pi^2\rho^2(x)(t-1)^2(x-c_1)^2} , t describing an interval containing]0, 1].

If \mu is the secondary measure of \rho,that of \rho_t will be t\mu.

The reducer of \rho_t is : \varphi_t(x)=\frac{2\left(x-c_1\right)-tG(x)}{\left((x-c_1)-t\frac{G(x)}{2}\right)^2%2Bt^2\pi^2\mu^2(x)} by noting G(x) the reducer of \mu.

Orthogonal polynomials for the measure \rho_t are clarified from n=1 by the formula

P_n^t(x)=\frac{1}{\sqrt{t}}\left[tP_n(x)%2B(1-t)(x-c_1)Q_n(x)\right] with Q_n secondary polynomial associated with P_n

It is remarkable also that, within the meaning of distributions, the limit when t tends towards 0 per higher value of \rho_t is the Dirac measure concentrated at c_1.

For example, the equinormal densities with the Chebyshev measure of the second form are defined by: \rho_t(x)=\frac{2t\sqrt{1-x^2}}{\pi\left[t^2%2B4(1-t)x^2\right]} , with t describing]0,2]. The value t=2 gives the Chebyshev measure of the first form.

A few beautiful applications

\forall p >1 \qquad\frac{1}{\ln(p)}=\frac{1}{p-1}%2B\int_0^{%2B\infty}\frac{dx}{(x%2Bp)(\ln^2(x)%2B\pi^2)}.\qquad
\gamma=\int_0^{%2B\infty}\frac{\ln(1%2B\frac{1}{x})dx}{\ln^2(x)%2B\pi^2}\qquad. (with \gamma the Euler's constant).
\gamma=\frac{1}{2}%2B\int_0^{%2B\infty}\frac{\overline {(x%2B1)\cos(\pi x)} dx}{x%2B1}.

(the notation x\mapsto \overline {(x%2B1)\cos(\pi x)} indicating the 2 periodic function coinciding with x\mapsto (x%2B1) \cos(\pi x) on (−1, 1)).

\gamma = \frac{1}{2} %2B \sum_{k=1}^{k=n} \frac{\beta_{2k}}{2k} - \frac{\beta_{2n}}{\zeta(2n)} \int_1^{%2B\infty} \frac{E(t)\cos(2\pi t)dt}{t^{2n%2B1}}

(with E is the floor function and \beta_{2n} the Bernoulli number of order 2n).

\beta_k = \frac{(-1)^kk!}{\pi} Im\left(\int_{-\infty}^{\infty} \frac{e^x \, dx}{(1%2Be^x)(x-i\pi)^k}\right).
\int_0^1\ln^{2n}\left(\frac{x}{1-x}\right)\,dx = (-1)^{n%2B1}2(2^{2n-1}-1)\beta_{2n}\pi^{2n}.
\int_0^1 \int_0^1\cdots \int_0^1 \left(\sum_{k=1}^{k=2n} \frac{ln(t_k)} {\prod_{i\not=k}(t_k-t_i)}\right) \, dt_1 \, dt_2\cdots dt_{2n} = \frac{(-1)^{n%2B1}(2\pi)^{2n}\beta_{2n}}{2}.
\qquad \int_0^{%2B\infty}\frac{e^{-\alpha x}dx} {\Gamma(x%2B1)} = e^{e^{-\alpha}} - 1 %2B \int_0^{%2B\infty} \frac{1-e^{-x}}{\left[(\ln(x)%2B\alpha)^2%2B\pi^2\right]} \frac{dx}{x}.

(for any real \alpha)

\sum_{n=1}^{n=%2B\infty} \left(\frac{1}{n}\sum_{k=0}^{k=n-1} \frac{1}{\binom{n-1}{k}}\right)^2 = \frac{4\pi^2}{9}=\int_0^{%2B\infty}4[\mathrm {Ei} (1,-x)%2Bi\pi]^2e^{-3x} \, dx.

(Ei indicate the integral exponentiel function here).

\frac{23}{15}-\ln(2) = \sum_{n=0}^{n=%2B\infty} \frac{1575}{2(n%2B1)(2n%2B1)(4n-3)(4n-1)(4n%2B1)(4n%2B5)(4n%2B7)(4n%2B9)}
 \mbox{Catalan } = \sum_{k=0}^{k=%2B\infty} \frac{(-1)^k}{4^{k%2B1}} \left(\frac{1}{(4k%2B3)^2}%2B\frac{2}{(4k%2B2)^2}%2B\frac{2}{(4k%2B1)^2}\right)%2B\frac{\pi\ln(2)}{8}
\mbox{Catalan} = \frac{\pi\ln(2)}{8}%2B\sum_{n=0}^{n=\infty}(-1)^n\frac{H_{2n%2B1}}{2n%2B1}.

(The Catalan's constant is defined as \sum_{n=0}^{n=\infty}\frac{(-1)^n}{(2n%2B1)^2} and H_{2n%2B1}=\sum_{k=1}^{k=2n%2B1}\frac{1}{k}) is the harmonic number of order 2n%2B1.

If the measure \rho is reducible and let \varphi be the associated reducer, one has the equality

\int_I\varphi^2(x)\rho(x) \, dx = \frac{4\pi^2}{3}\int_I\rho^3(x) \, dx.

If the measure \rho is reducible with \mu the associated reducer, then if f is square integrable for \mu, and if g is square integrable for \rho and is orthogonal with P_0=1 one has equivalence:

f(x)=\int_I\frac{g(t)-g(x)}{t-x}\rho(t)dt\Leftrightarrow g(x) = (x-c_1)f(x) - T_{\mu}(f(x)) = \frac{\varphi(x)\mu(x)}{\rho(x)}f(x)-T_{\rho} \left(\frac{\mu(x)}{\rho(x)}f(x)\right)

(c_1 indicates the moment of order 1 of \rho and T_{\rho} the operator g(x)\mapsto \int_I\frac{g(t)-g(x)}{t-x}\rho(t)\,dt).

See also

External links