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Table of Newtonian series
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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 a_n written in the form
:f(s) = \sum_^\infty (-1)^n a_n = \sum_^\infty \frac a_n
where
:
is the binomial coefficient and (s)_n is the rising factorial. Newtonian series often appear in relations of the form seen in umbral calculus.
==List==

The generalized binomial theorem gives
: (1+z)^ = \sum_^z^n =
1+z+z^2+\cdots.
A proof for this identity can be obtained by showing that it satisfies the differential equation
: (1+z) \frac = s (1+z)^s.
The digamma function:
:\psi(s+1)=-\gamma-\sum_^\infty \frac .
The Stirling numbers of the second kind are given by the finite sum
:\left\\right\}
=\frac\sum_^(-1)^ j^n.
This formula is a special case of the ''k''th forward difference of the monomial ''x''''n'' evaluated at ''x'' = 0:
: \Delta^k x^n = \sum_^(-1)^ (x+j)^n.
A related identity forms the basis of the Nörlund–Rice integral:
:\sum_^n \frac =
\frac =
\frac=
B(n+1,s-n)
where \Gamma(x) is the Gamma function and B(x,y) is the Beta function.
The trigonometric functions have umbral identities:
:\sum_^\infty (-1)^n = 2^ \cos \frac
and
:\sum_^\infty (-1)^n = 2^ \sin \frac
The umbral nature of these identities is a bit more clear by writing them in terms of the falling factorial (s)_n. The first few terms of the sin series are
:s - \frac + \frac - \frac + \cdots\,
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
:\!\sum_B_k z^k,
where ''B'' are the Bernoulli numbers. Employing the generating function its Borel sum can be evaluated as
:\sum_B_k z^k= \int_0^\infty e^ \fracd t= \sum_\frac z.
The general relation gives the Newton series
:\sum_\frac\frac= z^\zeta(s,x+z),
where \zeta is the Hurwitz zeta function and B_k(x) the Bernoulli polynomial. The series does not converge, the identity holds formally.
Another identity is
\frac 1= \sum_^\infty \sum_^k \frac,
which converges for x>a. This follows from the general form of a Newton series for equidistant nodes (when it exists, i.e. is convergent)
:f(x)=\sum_ \sum_^k (-1)^f(a+j h).

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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