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Table of Newtonian series : ウィキペディア英語版 | Table of Newtonian series In mathematics, a Newtonian series, named after Isaac Newton, is a sum over a sequence written in the form : where : is the binomial coefficient and is the rising factorial. Newtonian series often appear in relations of the form seen in umbral calculus. ==List==
The generalized binomial theorem gives : A proof for this identity can be obtained by showing that it satisfies the differential equation : The digamma function: : The Stirling numbers of the second kind are given by the finite sum : This formula is a special case of the ''k''th forward difference of the monomial ''x''''n'' evaluated at ''x'' = 0: : A related identity forms the basis of the Nörlund–Rice integral: : where is the Gamma function and is the Beta function. The trigonometric functions have umbral identities: : and : The umbral nature of these identities is a bit more clear by writing them in terms of the falling factorial . The first few terms of the sin series are : which can be recognized as resembling the Taylor series for sin ''x'', with (''s'')''n'' standing in the place of ''x''''n''. In analytic number theory it is of interest to sum : where ''B'' are the Bernoulli numbers. Employing the generating function its Borel sum can be evaluated as : The general relation gives the Newton series : where is the Hurwitz zeta function and the Bernoulli polynomial. The series does not converge, the identity holds formally. Another identity is
which converges for . This follows from the general form of a Newton series for equidistant nodes (when it exists, i.e. is convergent) :
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