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\sum_{n=1}^\infty \frac{1}{2^n} = \frac{1}{2}+ \frac{1}{4}+ \frac{1}{8}+\cdots+ \frac{1}{2^n}+\cdots.

The terms of the series are often produced according to a certain rule, such as by a formula, or by an algorithm. As there are an infinite number of terms, this notion is often called an infinite series. Unlike finite summations, infinite series need tools from mathematical analysis to be fully understood and manipulated. In addition to their ubiquity in mathematics, infinite series are also widely used in other quantitative disciplines such as physics and computer science.

Basic properties

Series can be composed of terms from any one of many different sets including real numbers, complex numbers, and functions. The definition given here will be for real numbers, but can be generalized.

Given an infinite sequence of real numbers { an }, define

S_N =\sum_{n=0}^N a_n=a_0+a_1+a_2+\cdots+a_N.

Call SN the partial sum to N of the sequence { an }, or partial sum of the series. A series is the sequence of partial sums, { SN }.

Potential confusion

When talking about series, one can refer either to the sequence { SN } of the partial sums, or to the sum of the series,

\sum_{n=0}^\infty a_n

i.e., the limit of the sequence of partial sums (see the formal definition in the next section) – it is clear which one is meant from context. To make a distinction between these two completely different objects (sequence vs. summed value), one sometimes omits the limits (atop and below the sum's symbol), as in

\sum_{n} a_n\

in order to refer to the formal series, that may or may not have a definite sum.

Convergent series

A series  ∑an  is said to 'converge' or to 'be convergent' when the sequence SN of partial sums has a finite limit. If the limit of SN is infinite or does not exist, the series is said to diverge. When the limit of partial sums exists, it is called the sum of the series

\sum_{n=0}^\infty a_n = \lim_{N\to\infty} S_N = \lim_{N\to\infty} \sum_{n=0}^N a_n.

The easiest way that an infinite series can converge is if all the an are zero for n sufficiently large. Such a series can be identified with a finite sum, so it is only infinite in a trivial sense.

Working out the properties of the series that converge even if all the terms are non-zero is the essence of the study of series. Consider the example

 1 + \frac{1}{2}+ \frac{1}{4}+ \frac{1}{8}+\cdots+ \frac{1}{2^n}+\cdots.

It is possible to "visualize" its convergence on the real number line: we can imagine a line of length 2, with successive segments marked off of lengths 1, ½, ¼, etc. There is always room to mark the next segment, because the amount of line remaining is always the same as the last segment marked: when we have marked off ½, we still have a piece of length ½ unmarked, so we can certainly mark the next ¼. This argument does not prove that the sum is equal to 2 (although it is), but it does prove that it is at most 2. In other words, the series has an upper bound. Proving that the series is equal to 2 requires only elementary algebra, however. If the series is denoted S, it can be seen that

S/2 = \frac{1+ \frac{1}{2}+ \frac{1}{4}+ \frac{1}{8}+\cdots}{2} = \frac{1}{2}+ \frac{1}{4}+ \frac{1}{8}+ \frac{1}{16} +\cdots

Therefore,

S-S/2 = 1 \Rightarrow S = 2.\,\!

Mathematicians extend the idiom discussed earlier to other, equivalent notions of series. For instance, when we talk about a recurring decimal, as in

x = 0.111\dots \,

we are talking, in fact, just about the series

\sum_{n=1}^\infty \frac{1}{10^n}

But since these series always converge to real numbers (because of what is called the completeness property of the real numbers), to talk about the series in this way is the same as to talk about the numbers for which they stand. In particular, it should offend no sensibilities if we make no distinction between 0.111… and 1/9. Less clear is the argument that 9 × 0.111… = 0.999… = 1, but it is not untenable when we consider that we can formalize the proof knowing only that limit laws preserve the arithmetic operations. See 0.999... for more.

Examples

1 + {1 \over 2} + {1 \over 4} + {1 \over 8} + {1 \over 16} + \cdots=\sum_{n=0}^\infty{1 \over 2^n}. In general, the geometric series \sum_{n=0}^\infty z^n converges if and only if |z| < 1. 1 + {1 \over 2} + {1 \over 3} + {1 \over 4} + {1 \over 5} + \cdots =\sum_{n=1}^\infty {1 \over n}. The harmonic series is divergent. 1 - {1 \over 2} + {1 \over 3} - {1 \over 4} + {1 \over 5} - \cdots =\sum_{n=1}^\infty (-1)^{n+1} {1 \over n}. \sum_{n=1}^\infty\frac{1}{n^r} converges if r > 1 and diverges for r ≤ 1, which can be shown with the integral criterion described below in convergence tests. As a function of r, the sum of this series is Riemann's zeta function. \sum_{n=1}^\infty (b_n-b_{n+1}) converges if the sequence bn converges to a limit L as n goes to infinity. The value of the series is then b1L.

Properties of series

Series are classed not only by whether they converge or diverge: they can also be split up based on the properties of the terms an (absolute or conditional convergence); type of convergence of the series (pointwise, uniform); the class of the term an (whether it is a real number, arithmetic progression, trigonometric function); etc.

Non-negative terms

When an is a non-negative real number for every n, the sequence SN of partial sums is non-decreasing. It follows that a series ∑an with non-negative terms converges if and only if the sequence SN of partial sums is bounded.

For example, the series

\sum_{n \ge 1} \frac{1}{n^2}

is convergent, because the inequality

\frac1 {n^2} \le \frac{1}{n-1} - \frac{1}{n}, \quad n \ge 2,

and a telescopic sum argument imply that the partial sums are bounded by 2.

Absolute convergence

A series

\sum_{n=0}^\infty a_n

is said to converge absolutely if the series of absolute values

\sum_{n=0}^\infty \left|a_n\right|

converges. It can be proved that this is sufficient to make not only the original series converge to a limit, but also for any reordering of it to converge to the same limit.

Conditional convergence

A series of real or complex numbers is said to be conditionally convergent (or semi-convergent) if it is convergent but not absolutely convergent. A famous example is the alternating series

\sum\limits_{n=1}^\infty {(-1)^{n+1}  \over n} = 1 - {1 \over 2} + {1 \over 3} - {1 \over 4} + {1 \over 5} - \cdots

which is convergent (and its sum is equal to ln 2), but the series formed by taking the absolute value of each term is the divergent harmonic series. The Riemann series theorem says that any conditionally convergent series can be reordered to make a divergent series, and moreover, if the an are real and S is any real number, that one can find a reordering so that the reordered series converges with sum equal to S.

Abel's test is an important tool for handling semi-convergent series. If a series has the form

\sum a_n = \sum \lambda_n b_n

where the partial sums BN = b0 + ··· + bn are bounded, λn has bounded variation, and lim λnBn exists:

\sup_N \Bigl| \sum_{n=0}^N b_n \Bigr| < \infty, \ \ \sum |\lambda_{n+1} - \lambda_n| < \infty\ \text{and} \ \lambda_n B_n \ \text{converges,}

then the series ∑ an is convergent. This applies to the pointwise convergence of many trigonometric series, as in

\sum_{n=2}^\infty \frac{\sin(n x)}{\ln n}

with 0 < x < 2π. Abel's method consists in writing bn+1 = Bn+1 − Bn, and in performing a transformation similar to integration by parts (called summation by parts), that relates the given series ∑ an to the absolutely convergent series

 \sum (\lambda_n - \lambda_{n+1}) \, B_n.

Convergence tests

Series of functions

A series of real- or complex-valued functions

\sum_{n=0}^\infty f_n(x)

converges pointwise on a set E, if the series converges for each x in E as an ordinary series of real or complex numbers. Equivalently, the partial sums

s_N(x) = \sum_{n=0}^N f_n(x)

converge to ƒ(x) as N → ∞ for each x ∈ E.

A stronger notion of convergence of a series of functions is called uniform convergence. The series converges uniformly if it converges pointwise to the function ƒ(x), and the error in approximating the limit by the Nth partial sum,