n | n x \sin\left(\tfrac1{n}\right) | |
---|---|---|
1 | 0.841471 | |
2 | 0.958851 | |
... | ||
10 | 0.998334 | |
... | ||
100 | 0.999983 |
As the positive integer becomes larger and larger, the value becomes arbitrarily close to . We say that "the limit of the sequence equals ."
In mathematics, the limit of a sequence is the value that the terms of a sequence "tend to", and is often denoted using the
\lim
\limnan
Limits can be defined in any metric or topological space, but are usually first encountered in the real numbers.
The Greek philosopher Zeno of Elea is famous for formulating paradoxes that involve limiting processes.
Leucippus, Democritus, Antiphon, Eudoxus, and Archimedes developed the method of exhaustion, which uses an infinite sequence of approximations to determine an area or a volume. Archimedes succeeded in summing what is now called a geometric series.
Grégoire de Saint-Vincent gave the first definition of limit (terminus) of a geometric series in his work Opus Geometricum (1647): "The terminus of a progression is the end of the series, which none progression can reach, even not if she is continued in infinity, but which she can approach nearer than a given segment."[4]
Pietro Mengoli anticipated the modern idea of limit of a sequence with his study of quasi-proportions in Geometriae speciosae elementa (1659). He used the term quasi-infinite for unbounded and quasi-null for vanishing.
Newton dealt with series in his works on Analysis with infinite series (written in 1669, circulated in manuscript, published in 1711), Method of fluxions and infinite series (written in 1671, published in English translation in 1736, Latin original published much later) and Tractatus de Quadratura Curvarum (written in 1693, published in 1704 as an Appendix to his Optiks). In the latter work, Newton considers the binomial expansion of , which he then linearizes by taking the limit as tends to .
In the 18th century, mathematicians such as Euler succeeded in summing some divergent series by stopping at the right moment; they did not much care whether a limit existed, as long as it could be calculated. At the end of the century, Lagrange in his Théorie des fonctions analytiques (1797) opined that the lack of rigour precluded further development in calculus. Gauss in his etude of hypergeometric series (1813) for the first time rigorously investigated the conditions under which a series converged to a limit.
The modern definition of a limit (for any there exists an index so that ...) was given by Bernard Bolzano (Der binomische Lehrsatz, Prague 1816, which was little noticed at the time), and by Karl Weierstrass in the 1870s.
In the real numbers, a number
L
(xn)
L
See also: List of limits.
xn=c
xn\toc
xn=
1 | |
n |
xn\to0
xn=
1 | |
n |
n
xn=
1 | |
n2 |
n
xn\to0
xn+1>xn
n
\limn\toinfty\left(1+\tfrac{1}{n}\right)n
We call
x
(xn)
xn\tox
\limn\toinftyxn=x
if the following condition holds:
\varepsilon>0
N
n\geqN
|xn-x|<\varepsilon
In other words, for every measure of closeness
\varepsilon
(xn)
x
Symbolically, this is:
\forall\varepsilon>0\left(\existsN\in\N\left(\foralln\in\N\left(n\geqN\implies|xn-x|<\varepsilon\right)\right)\right)
If a sequence
(xn)
x
x
(xn)
Some other important properties of limits of real sequences include the following:
\limn\toinftyan
\limn\toinftybn
\limn\toinfty(an\pmbn)=\limn\toinftyan\pm\limn\toinftybn
\limn\toinftycan=c ⋅ \limn\toinftyan
\limn\toinfty(an ⋅ bn)=\left(\limn\toinftyan\right) ⋅ \left(\limn\toinftybn\right)
\limn\toinfty\left(
an | |
bn |
\right)=
\lim\limitsn\toinftyan | |
\lim\limitsn\toinftybn |
\limn\toinftybn\ne0
\limn\toinfty
p | |
a | |
n |
=\left(\limn\toinftyan\right)p
\limn\toinftyxn
\limn\toinftyf\left(xn\right)
an\leqbn
n
N
\limn\toinftyan\leq\limn\toinftybn
an\leqcn\leqbn
n
N
\limn\toinftyan=\limn\toinftybn=L
\limn\toinftycn=L
an
n
N
These properties are extensively used to prove limits, without the need to directly use the cumbersome formal definition. For example, once it is proven that
1/n\to0
a | |||
|
\to
a | |
b |
b\ne0
A sequence
(xn)
xn\toinfty
\limn\toinftyxn=infty
For every real number
K
N
n\geqN
xn>K
K
Symbolically, this is:
\forallK\inR\left(\existsN\in\N\left(\foralln\in\N\left(n\geqN\impliesxn>K\right)\right)\right)
Similarly, we say a sequence tends to minus infinity, written
xn\to-infty
\limn\toinftyxn=-infty
For every real number
K
N
n\geqN
xn<K
K
Symbolically, this is:
\forallK\inR\left(\existsN\in\N\left(\foralln\in\N\left(n\geqN\impliesxn<K\right)\right)\right)
If a sequence tends to infinity or minus infinity, then it is divergent. However, a divergent sequence need not tend to plus or minus infinity, and the sequence
n | |
x | |
n=(-1) |
A point
x
(X,d)
(xn)
\varepsilon>0
N
n\geqN
d(xn,x)<\varepsilon
Symbolically, this is:
\forall\varepsilon>0\left(\existsN\in\N\left(\foralln\in\N\left(n\geqN\impliesd(xn,x)<\varepsilon\right)\right)\right)
This coincides with the definition given for real numbers when
X=\R
d(x,y)=|x-y|
\varepsilon
\varepsilon
\limnxn
\limnf(xn)=f\left(\limnxn\right)
See main article: Cauchy sequence.
A Cauchy sequence is a sequence whose terms ultimately become arbitrarily close together, after sufficiently many initial terms have been discarded. The notion of a Cauchy sequence is important in the study of sequences in metric spaces, and, in particular, in real analysis. One particularly important result in real analysis is the Cauchy criterion for convergence of sequences: a sequence of real numbers is convergent if and only if it is a Cauchy sequence. This remains true in other complete metric spaces.
A point
x\inX
(X,\tau)
\left(xn\right)n
U
x
N\in\N
n\geqN
xn\inU
This coincides with the definition given for metric spaces, if
(X,d)
\tau
d
A limit of a sequence of points
\left(xn\right)n
T
\N
\N\cup\lbrace+infty\rbrace
T
n
+infty
\N
In a Hausdorff space, limits of sequences are unique whenever they exist. This need not be the case in non-Hausdorff spaces; in particular, if two points
x
y
x
y
The definition of the limit using the hyperreal numbers formalizes the intuition that for a "very large" value of the index, the corresponding term is "very close" to the limit. More precisely, a real sequence
(xn)
xH
xH-L
xH
L={\rmst}(xH)
Thus, the limit can be defined by the formula
\limnxn={\rmst}(xH)
Sometimes one may also consider a sequence with more than one index, for example, a double sequence
(xn,)
L
L
xn,=c
xn,m\toc
xn,=
1 | |
n+m |
xn,\to0
xn,=
n | |
n+m |
We call
x
(xn,)
xn,\tox
\lim\begin{smallmatrixn\toinfty\ m\toinfty \end{smallmatrix}}xn,=x
if the following condition holds:
\varepsilon>0
N
n,m\geqN
|xn,-x|<\varepsilon
\varepsilon
(xn,)
x
Symbolically, this is:
\forall\varepsilon>0\left(\existsN\in\N\left(\foralln,m\in\N\left(n,m\geqN\implies|xn,-x|<\varepsilon\right)\right)\right)
The double limit is different from taking limit in n first, and then in m. The latter is known as iterated limit. Given that both the double limit and the iterated limit exists, they have the same value. However, it is possible that one of them exist but the other does not.
A sequence
(xn,m)
xn,m\toinfty
\lim\begin{smallmatrixn\toinfty\ m\toinfty \end{smallmatrix}}xn,m=infty
For every real number
K
N
n,m\geqN
xn,m>K
K
Symbolically, this is:
\forallK\inR\left(\existsN\in\N\left(\foralln,m\in\N\left(n,m\geqN\impliesxn,>K\right)\right)\right)
Similarly, a sequence
(xn,m)
xn,m\to-infty
\lim\begin{smallmatrixn\toinfty\ m\toinfty \end{smallmatrix}}xn,m=-infty
For every real number
K
N
n,m\geqN
xn,m<K
K
Symbolically, this is:
\forallK\inR\left(\existsN\in\N\left(\foralln,m\in\N\left(n,m\geqN\impliesxn,<K\right)\right)\right)
If a sequence tends to infinity or minus infinity, then it is divergent. However, a divergent sequence need not tend to plus or minus infinity, and the sequence
xn,m=(-1)n+m
For a double sequence
(xn,m)
n\toinfty
(ym)
xn,\toym pointwise
\limnxn,=ym pointwise
which means:
\varepsilon>0
m
N(\varepsilon,m)>0
n\geqN
|xn,-ym|<\varepsilon
Symbolically, this is:
\forall\varepsilon>0\left(\forallm\inN\left(\existsN\in\N\left(\foralln\in\N\left(n\geqN\implies|xn,-ym|<\varepsilon\right)\right)\right)\right)
When such a limit exists, we say the sequence
(xn,)
(ym)
The second one is called uniform limit, denoted
xn,\toym uniformly
\limnxn,=ym uniformly
xn,\rightrightarrowsym
\underset{n\toinfty}{unif\lim} xn,=ym
which means:
\varepsilon>0
N(\varepsilon)>0
m
n\geqN
|xn,-ym|<\varepsilon
Symbolically, this is:
\forall\varepsilon>0\left(\existsN\in\N\left(\forallm\inN\left(\foralln\in\N\left(n\geqN\implies|xn,-ym|<\varepsilon\right)\right)\right)\right)
In this definition, the choice of
N
m
N
m
If
xn,\toym
xn,\toym
When such a limit exists, we say the sequence
(xn,)
(ym)
For a double sequence
(xn,m)
n\toinfty
(ym)
m\toinfty
y
\limm\limnxn,=\limmym=y
This limit is known as iterated limit of the double sequence. The order of taking limits may affect the result, i.e.,
\limm\limnxn,\ne\limn\limmxn,
A sufficient condition of equality is given by the Moore-Osgood theorem, which requires the limit
\limnxn,=ym
N=1
n\geqN
|xn-c|=0<\varepsilon
N=\left\lfloor
1 | |
\varepsilon |
\right\rfloor+1
n\geqN
|xn-0|\lexN=
1 | |
\lfloor1/\varepsilon\rfloor+1 |
<\varepsilon