In mathematics, the secondary measure associated with a measure of positive density àwhen there is one, is a measure of positive density ü, turning the secondary polynomials associated with the orthogonal polynomials for àinto an orthogonal system.
Under certain assumptions, it is possible to obtain the existence of a secondary measure and even to express it.
For example, this can be done when working in the Hilbert space L<sup>2</sup>([0, 1], R, ÃÂ)
with
in the general case, or:
when ÃÂ satisfies a Lipschitz condition.
This application ÃÂ is called the reducer of ÃÂ.
More generally, ü et àare linked by their Stieltjes transformation with the following formula:
in which c<sub>1</sub> is the moment of order 1 of the measure ÃÂ.
Secondary measures and the theory around them may be used to derive traditional formulas of analysis concerning the Gamma function, the Riemann zeta function, and the EulerâÂÂMascheroni constant.
They have also allowed the clarification of various integrals and series, although this tends to be difficult a priori.
Finally they make it possible to solve integral equations of the form
where g is the unknown function, and lead to theorems of convergence towards the Chebyshev and Dirac measures.
Let ÃÂ be a measure of positive density on an interval I and admitting moments of any order. From this, a family {P<sub>n</sub>} of orthogonal polynomials for the inner product induced by ÃÂ can be created.
Let {Q<sub>n</sub>} be 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 can be clarified from ÃÂ, is called a secondary measure associated initial measure ÃÂ.
When àis a probability density function, a sufficient condition that allows ü to be a secondary measure associated with àwhile admitting moments of any order is that its Stieltjes Transformation is given by an equality of the type
where a is an arbitrary constant and c<sub>1</sub> indicates the moment of order 1 of ÃÂ.
For a = 1, the measure known as secondary can be obtained. For n âÂÂ¥ 1 the norm of the polynomial P<sub>n</sub> for àcoincides exactly with the norm of the secondary polynomial associated Q<sub>n</sub> when using the measure ü.
In this paramount case, and if the space generated by the orthogonal polynomials is dense in L<sup>2</sup>(I, R, ÃÂ), the operator T<sub>ÃÂ</sub> defined by
creating the secondary polynomials can be furthered to a linear map connecting space L<sup>2</sup>(I, R, ÃÂ) to L<sup>2</sup>(I, R, ü) and becomes isometric if limited to the hyperplane H<sub>ÃÂ</sub> of the orthogonal functions with P<sub>0</sub> = 1.
For unspecified functions square integrable for ÃÂ a more general formula of covariance may be obtained:
The theory continues by introducing the concept of reducible measure, meaning that the quotient ÃÂ/ü is element of L<sup>2</sup>(I, R, ü). The following results are then established:
Finally the two operators are also connected, provided the images in question are defined, by the fundamental formula of composition:
The Lebesgue measure on the standard interval [0, 1] is obtained by taking the constant density ÃÂ(x) = 1.
The associated orthogonal polynomials are called (shifted) Legendre polynomials and can be defined as
The norm of these P<sub>n</sub> is then
and the recurrence relation in three terms can be written
The reducer of this measure of Lebesgue is given by
The associated secondary measure is then clarified as
If we normalize the polynomials of Legendre, the coefficients of Fourier of the reducer ÃÂ related to this orthonormal system are null for an even index and are given by
for an odd index n.
The Laguerre polynomials are linked to the density ÃÂ(x) = e<sup>âÂÂx</sup> on the interval I = [0, âÂÂ). They are clarified by
and are normalized.
The reducer associated is defined by
The coefficients of Fourier of the reducer ÃÂ related to the Laguerre polynomials are given by
This coefficient C<sub>n</sub>(ÃÂ) 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
on I = R.
They are clarified by
and are normalized.
The reducer associated is defined by
The coefficients of Fourier of the reducer ÃÂ related to the system of Hermite polynomials are null for an even index and are given by
for an odd index n.
The Chebyshev measure of the second form. This is defined by the density
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.
Jacobi measure on (0, 1) of density
Chebyshev measure on (âÂÂ1, 1) of the first form of density
The secondary measure ü associated with a probability density function àhas its moment of order 0 given by the formula
where c<sub>1</sub> and c<sub>2</sub> indicating the respective moments of order 1 and 2 of ÃÂ.
This process can be iterated by 'normalizing' ü while defining ÃÂ<sub>1</sub> = ü/d<sub>0</sub> which becomes in its turn a density of probability called naturally the normalised secondary measure associated with ÃÂ.
From ÃÂ<sub>1</sub>, a secondary normalised measure ÃÂ<sub>2</sub> can be created. This can be iterated to obtain ÃÂ<sub>3</sub> from ÃÂ<sub>2</sub> and so on.
Therefore, a sequence of successive secondary measures, created from ÃÂ<sub>0</sub> = ÃÂ, is such that ÃÂ<sub>n+1</sub> that is the secondary normalised measure deduced from ÃÂ<sub>n</sub>
It is possible to clarify the density ÃÂ<sub>n</sub> by using the orthogonal polynomials P<sub>n</sub> for ÃÂ, the secondary polynomials Q<sub>n</sub> and the reducer associated ÃÂ. This gives the formula
The coefficient is easily obtained starting from the leading coefficients of the polynomials P<sub>nâÂÂ1</sub> and P<sub>n</sub>. The reducer ÃÂ<sub>n</sub> associated with ÃÂ<sub>n</sub>, as well as the orthogonal polynomials corresponding to ÃÂ<sub>n</sub>, can also be clarified.
The evolution of these densities when the index tends towards the infinite can be related to the support of the measure on the standard interval [0, 1]:
Let
be the classic recurrence relation in three terms. If
then the sequence {ÃÂ<sub>n</sub>} converges completely towards the Chebyshev density of the second form
These conditions about limits are checked by a very broad class of traditional densities. A derivation of the sequence of secondary measures and convergence can be found in.
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 ÃÂ has its moment of order 1 equal to c<sub>1</sub>, then these densities equinormal with ÃÂ are given by a formula of the type:
t describing an interval containing ]0, 1].
If ü is the secondary measure of ÃÂ, that of ÃÂ<sub>t</sub> will be tü.
The reducer of ÃÂ<sub>t</sub> is
by noting G(x) the reducer of ü.
Orthogonal polynomials for the measure ÃÂ<sub>t</sub> are clarified from n = 1 by the formula
with Q<sub>n</sub> secondary polynomial associated with P<sub>n</sub>.
It is remarkable also that, within the meaning of distributions, the limit when t tends towards 0 per higher value of ÃÂ<sub>t</sub> is the Dirac measure concentrated at c<sub>1</sub>.
For example, the equinormal densities with the Chebyshev measure of the second form are defined by:
with t describing ]0, 2]. The value t = 2 gives the Chebyshev measure of the first form.
In the formulas below G is Catalan's constant, ó is the Euler's constant, ò<sub>2n</sub> is the Bernoulli number of order 2n, H<sub>2n+1</sub> is the harmonic number of order 2n+1 and Ei is the Exponential integral function.
The notation indicating the 2 periodic function coinciding with on (âÂÂ1, 1).
If the measure ÃÂ is reducible and let ÃÂ be the associated reducer, one has the equality
If the measure àis reducible with ü the associated reducer, then if f is square integrable for ü, and if g is square integrable for àand is orthogonal with P<sub>0</sub> = 1, the following equivalence holds:
c<sub>1</sub> indicates the moment of order 1 of ÃÂ and T<sub>ÃÂ</sub> the operator
In addition, the sequence of secondary measures has applications in Quantum Mechanics, where it gives rise to the sequence of residual spectral densities for specialized Pauli-Fierz Hamiltonians. This also provides a physical interpretation for the sequence of secondary measures.