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The simplest type of equations in the theory of difference equations are difference equations of the type
(1) |
(2) |
with the increment being an arbitrary but fixed positive real number and with real or possibly complex . The operator is the so called first (Nörlund) difference quotient. If , we simply write and .
It is interesting to note that
The solutions of (1) are called sums of , and those of (2) alternating sums of , resp. The so-called general solution of (1) or of (2) can be represented as a sum of a particular solution and a solution of equation , or , resp. The central problem is to determine the particular solution by selection of its properties. Such particular solutions are then called principal sums. The condition are sometimes vague, and are of type:
It can be easily verified that
(3) |
formally solves equation (1) with an arbitrary constant , and that
(4) |
formally solves (2). If these series are convergent (with ) they are usually taken for principal sums. For instance,
Nörlund [1] writes constant is the form and thus equation (3) gets the form
with an arbitrary constant .
To ensure the convergence of the involved series and the integral ingenious summation tricks are necessary in general to guarantee expected form of the principal sums. The general scheme of Nörlund’s approach can be describes as follows:
Suppose firstly that is positive and continuous (complex or real) function for . Then repalce the function on the right hand side by another function with unknown and depending on a new parameter , which is chosen so that
a) ,
b) both and converge.
Then the function
solves the difference equation
(5) |
and if we let , the relation (5) reduces to the equation and the function
is the solution of the equation (1) yields the principal sums provided the limit exists uniformly and is independent of the choice subject to the conditions a) and b) above.
An analogical scheme can also be applied to the equation (2).
Nörlund introduced a special notation to denote the principal sum of equation (1)
and for the principal alternating sum of equation (2) he wrote
Nörlund applied the above scheme with
where for some , .
Sufficient conditions under which the above requirements are fulfilled are [1] , pp.48-49:
(I) has for a continuous derivative of order for some such that , and moreover
(IIa) is uniformly comvergent in the interval , and consequently in every interval for any arbitrarily large ,
(IIb) is uniformly comvergent in the interval (and consequently in every interval for any arbitrarily large ).
Here the condition (I) and (IIa) are applied when solving the equation (2), that is in the case of the principal alternating sums, and (I) with (IIb) in case of principal sums.
The principal sums satisfy the following multiplication theorem (relation) [1] , p.44:
(6) |
while for the principal alternating sums of equation (2) there holds
Equation 2 there holds
(7) |
(8) |
In addition we also have
(9) |
Example. For , we get [1] , p.53:
where , and denotes the th Bernoulli, and Euler polynomial, resp. More generally
The relations (7) and (8) contain the well-known multiplicative realtions for bernoulli and Euler polynomials discovered by Raabe in 1848 and the relation (9) the known relation bewteen Bernoulli and Euler polynomilas.
[1] | Nörlund, N. E. (1924). Vorlesungen über die Differenzenrechnung. Berlin: Springer Verlag. |
Cite this web-page as:
Štefan Porubský: Summation of Functions.