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{{short description|Domain of convergence of power series}}
In [[mathematics]], the '''radius of convergence''' of a [[power series]] is a quantity, either a non-negative real number or ∞, that represents a domain (within the radius) in which the [[power series|series]] will [[Convergent series|converge]]. Within the radius of convergence, a power series [[absolute convergence|converges absolutely]] and [[compact convergence|uniformly on compacta]] as well. If the series converges, it is the [[Taylor series]] of the [[analytic function]] to which it converges inside its radius of convergence.
In [[mathematics]], the '''radius of convergence''' of a [[power series]] is the radius of the largest [[Disk (mathematics)|disk]] at the [[Power series|center of the series]] in which the series [[Convergent series|converges]]. It is either a non-negative real number or <math>\infty</math>. When it is positive, the power series [[absolute convergence|converges absolutely]] and [[compact convergence|uniformly on compact sets]] inside the open disk of radius equal to the radius of convergence, and it is the [[Taylor series]] of the [[analytic function]] to which it converges. In case of multiple singularities of a function (singularities are those values of the argument for which the function is not defined), the radius of convergence is the shortest or minimum of all the respective distances (which are all non-negative numbers) calculated from the center of the disk of convergence to the respective singularities of the function.


==Definition==
==Definition==
For a power series ''ƒ'' defined as:
For a power series ''f'' defined as:


:<math>f(z) = \sum_{n=0}^\infty c_n (z-a)^n, </math>
:<math>f(z) = \sum_{n=0}^\infty c_n (z-a)^n, </math>
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where
where


:''a'' is a [[complex number|complex]] constant, the center of the [[disk (mathematics)|disk]] of convergence,
*''a'' is a [[complex number|complex]] constant, the center of the [[disk (mathematics)|disk]] of convergence,
:''c''<sub>''n''</sub> is the ''n''<sup>th</sup> complex coefficient, and
*''c''<sub>''n''</sub> is the ''n''-th complex coefficient, and
:''z'' is a complex variable.
*''z'' is a complex variable.


The radius of convergence ''r'' is a nonnegative real number or such that the series converges if
The radius of convergence ''r'' is a nonnegative real number or <math>\infty</math> such that the series converges if


:<math>|z-a| < r\,</math>
:<math>|z-a| < r</math>


and diverges if
and diverges if


:<math>|z-a| > r.\,</math>
:<math>|z-a| > r.</math>


Some may prefer an alternative definition, as existence is obvious:
In other words, the series converges if ''z'' is close enough to the center and diverges if it is too far away. The radius of convergence specifies how close is close enough. On the boundary, that is, where |''z''&nbsp;&minus;&nbsp;''a''| = ''r'', the behavior of the power series may be complicated, and the series may converge for some values of ''z'' and diverge for others. The radius of convergence is infinite if the series converges for all [[complex number]]s ''z''.

: <math>r=\sup \left\{ |z-a|\ \left|\ \sum_{n=0}^\infty c_n(z-a)^n\ \text{ converges } \right.\right\} </math>

On the boundary, that is, where |''z''&nbsp;&nbsp;''a''| = ''r'', the behavior of the power series may be complicated, and the series may converge for some values of ''z'' and diverge for others. The radius of convergence is infinite if the series converges for all [[complex number]]s ''z''.<ref>{{Cite book|url=https://books.google.com/books?id=nw9eFnCSDNoC&q=radius+of+convergence|title=Mathematical Analysis-II|date=16 November 2010|publisher=Krishna Prakashan Media|language=en}}</ref>


==Finding the radius of convergence==
==Finding the radius of convergence==
Two cases arise:


Two cases arise. The first case is theoretical: when you know all the coefficients <math>c_n</math> then you take certain limits and find the precise radius of convergence. The second case is practical: when you construct a power series solution of a difficult problems you typically will only know a finite number of terms in a power series, anywhere from a couple of terms to a hundred terms. In this second case, extrapolating a plot estimates the radius of convergence.
* The first case is theoretical: when you know all the coefficients <math>c_n</math> then you take certain limits and find the precise radius of convergence.
* The second case is practical: when you construct a power series solution of a difficult problem you typically will only know a finite number of terms in a power series, anywhere from a couple of terms to a hundred terms. In this second case, extrapolating a plot estimates the radius of convergence.


===Theoretical radius===
===Theoretical radius===
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The radius of convergence can be found by applying the [[root test]] to the terms of the series. The root test uses the number
The radius of convergence can be found by applying the [[root test]] to the terms of the series. The root test uses the number


:<math>C = \limsup_{n\rightarrow\infty}\sqrt[n]{|c_n(z-a)^n|} = \limsup_{n\rightarrow\infty}\sqrt[n]{|c_n|}|z-a|</math>
:<math>C = \limsup_{n\to\infty}\sqrt[n]{|c_n(z-a)^n|} = \limsup_{n\to\infty} \left(\sqrt[n]{|c_n|}\right) |z-a|</math>


"lim&nbsp;sup" denotes the [[limit superior]]. The root test states that the series converges if ''C''&nbsp;<&nbsp;1 and diverges if&nbsp;''C''&nbsp;>&nbsp;1. It follows that the power series converges if the distance from ''z'' to the center ''a'' is less than
"lim&nbsp;sup" denotes the [[limit superior]]. The root test states that the series converges if ''C''&nbsp;<&nbsp;1 and diverges if&nbsp;''C''&nbsp;>&nbsp;1. It follows that the power series converges if the distance from ''z'' to the center ''a'' is less than


:<math>r = \frac{1}{\limsup_{n\rightarrow\infty}\sqrt[n]{|c_n|}}</math>
:<math>r = \frac{1}{\limsup_{n\to\infty}\sqrt[n]{|c_n|}}</math>


and diverges if the distance exceeds that number; this statement is the [[Cauchy–Hadamard theorem]]. Note that ''r''&nbsp;=&nbsp;1/0 is interpreted as an infinite radius, meaning that ''ƒ'' is an [[entire function]].
and diverges if the distance exceeds that number; this statement is the [[Cauchy–Hadamard theorem]]. Note that ''r''&nbsp;=&nbsp;1/0 is interpreted as an infinite radius, meaning that ''f'' is an [[entire function]].


The limit involved in the [[ratio test]] is usually easier to compute, and when that limit exists, it shows that the radius of convergence
The limit involved in the [[ratio test]] is usually easier to compute, and when that limit exists, it shows that the radius of convergence is finite.


<!-- NOTE: The ratio test as usually stated involves c_{n+1}/c_n, but THIS statement correctly uses c_{n+1}/c_n. -->
<!-- NOTE: The ratio test as usually stated involves c_{n+1}/c_n, but THIS statement correctly uses c_{n+1}/c_n. -->
:<math>r = \lim_{n\rightarrow\infty} \left| \frac{c_n}{c_{n+1}} \right|.</math>
:<math>r = \lim_{n\to\infty} \left| \frac{c_{n}}{c_{n+1}} \right|.</math>
<!-- NOTE: The ratio test as usually stated involves c_{n+1}/c_n, but THIS statement correctly uses c_n/c_{n+1}. -->
<!-- NOTE: The ratio test as usually stated involves c_{n+1}/c_n, but THIS statement correctly uses c_n/c_{n+1}. -->


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: <math> |z - a| < \frac{1}{\lim_{n\to\infty} \frac{|c_{n+1}|}{|c_n|}} = \lim_{n\to\infty} \left|\frac{c_n}{c_{n+1}}\right|. </math>
: <math> |z - a| < \frac{1}{\lim_{n\to\infty} \frac{|c_{n+1}|}{|c_n|}} = \lim_{n\to\infty} \left|\frac{c_n}{c_{n+1}}\right|. </math>


===Practical estimation of radius===
==={{anchor|Domb–Sykes plot|Domb–Sykes plot}} Practical estimation of radius in the case of real coefficients ===
<!-- [[Domb–Sykes plot]] redirects here (and so in [[MOS:BOLD|boldface]] -->
[[File:Domb Sykes plot Hinch.svg|thumb|right|400px|Plots of the function <math>f(\varepsilon)=\frac{\varepsilon(1+\varepsilon^3)}{\sqrt{1+2\varepsilon}}.</math> <br>
The solid green line is the [[straight line|straight-line]] [[asymptote]] in the Domb–Sykes plot,<ref>See Figure 8.1 in: {{citation| first=E.J. |last=Hinch |year=1991 |title=Perturbation Methods |series=Cambridge Texts in Applied Mathematics |volume=6 |publisher=Cambridge University Press |isbn=0-521-37897-4 |page=146}}</ref> plot (b), which intercepts the vertical axis at −2 and has a slope +1. Thus there is a singularity at <math>\varepsilon=-1/2</math> and so the radius of convergence is <math>r=1/2.</math>]]
Usually, in scientific applications, only a finite number of coefficients <math>c_n</math> are known. Typically, as <math>n</math> increases, these coefficients settle into a regular behavior determined by the nearest radius-limiting singularity. In this case, two main techniques have been developed, based on the fact that the coefficients of a Taylor series are roughly exponential with ratio <math>1/r</math> where ''r'' is the radius of convergence.


* The basic case is when the coefficients ultimately share a common sign or alternate in sign. As pointed out earlier in the article, in many cases the limit <math display="inline">\lim_{n\to \infty} {c_n / c_{n-1}}</math> exists, and in this case <math display="inline">1/r = \lim_{n \to \infty} {c_n / c_{n-1}}</math>. Negative <math>r</math> means the convergence-limiting singularity is on the negative axis. Estimate this limit, by plotting the <math>c_n/c_{n-1}</math> versus <math>1/n</math>, and graphically extrapolate to <math>1/n=0</math> (effectively <math>n=\infty</math>) via a [[Linear Regression|linear fit]]. The intercept with <math>1/n=0</math> estimates the reciprocal of the radius of convergence, <math>1/r</math>. This plot is called a '''Domb–Sykes plot'''.<ref>{{citation |first1=C. |last1=Domb |first2=M.F. |last2=Sykes |title=On the susceptibility of a ferromagnetic above the Curie point |journal=Proc. R. Soc. Lond. A |volume=240 |pages=214–228 |year=1957 |issue=1221 |doi=10.1098/rspa.1957.0078 |bibcode=1957RSPSA.240..214D |s2cid=119974403 }}</ref>
Suppose you only know a finite number of coefficients <math>c_n</math>, say ten to a hundred. Typically, as <math>n</math> increases, these coefficients settle into a regular behavior determined by the nearest radius-limiting singularity.
* The more complicated case is when the signs of the coefficients have a more complex pattern. Mercer and Roberts proposed the following procedure.<ref>{{citation |first1=G.N. |last1=Mercer |first2=A.J. |last2=Roberts |title=A centre manifold description of contaminant dispersion in channels with varying flow properties |journal=SIAM J. Appl. Math. |volume=50 |pages=1547–1565 |year=1990 |doi=10.1137/0150091 |issue=6}}</ref> Define the associated sequence <math display="block">b_n^2=\frac{c_{n+1}c_{n-1} - c_n^2}{c_n c_{n-2} - c_{n-1}^2} \quad n=3,4,5,\ldots.</math> Plot the finitely many known <math>b_n</math> versus <math>1/n</math>, and graphically extrapolate to <math>1/n=0</math> via a linear fit. The intercept with <math>1/n=0</math> estimates the reciprocal of the radius of convergence, <math>1/r</math>.{{pb}} This procedure also estimates two other characteristics of the convergence limiting singularity. Suppose the nearest singularity is of degree <math>p</math> and has angle <math>\pm\theta</math> to the real axis. Then the slope of the linear fit given above is <math>-(p+1)/r</math>. Further, plot <math display="inline">\frac{1}{2} \left(\frac{c_{n-1}b_n}{c_n} + \frac{c_{n+1}}{c_n b_n}\right)</math> versus <math display="inline">1/n^2</math>, then a linear fit extrapolated to <math display="inline">1/n^2=0</math> has intercept at <math>\cos\theta</math>.

When the behavior of the coefficients is one of constant sign or alternating sign, Domb and Sykes<ref>C. Domb and M. F. Sykes, On the susceptibility of a ferromagnet above the Curie point, ''Proc. Roy. Soc. Lond. A'' 240:214-228, 1957.</ref> proposed plotting <math>c_n/c_{n-1}</math> against <math>1/n</math>, fitting a straight line extrapolation, and taking the intercept of this line as an estimate the reciprocal <math>1/r</math> of the radius of convergence. Negative <math>r</math> means the convergence-limiting singularity is on the negative axis. Naturally, this is called a Domb-Sykes plot.

When the coefficients settle into having a periodic pattern of signs then use a test proposed by Mercer and Roberts.<ref>G. N. Mercer and A. J. Roberts, A centre manifold description of contaminant dispersion in channels with varying flow properties, ''SIAM J.~Appl. Math.'' 50:1547-1565, 1990.</ref> Compute <math>b_n</math> from <math>b_n^2=(c_{n+1}c_{z-1}-c_n^2)/(c_nc_{n-2}-c_{n-1}^2)</math> and plot <math>b_n</math> versus <math>1/n</math>. Extrapolate to <math>1/n=0</math> to again estimate the reciprocal <math>1/r</math> of the radius of convergence.

You may also estimate two subsidiary quantities. Estimate the exponent <math>p</math> of the convergence limiting singularity because the slope of the straight line extrapolation is <math>-(p+1)/r</math>. Estimate the angle <math>\theta</math>, from the real axis, of the convergence limiting singularities by plotting <math>(c_{n-1}b_n/c_n+c_{n+1}/c_n/b_n)/2</math> versus <math>1/n^2</math>. Then extrapolating to <math>1/n^2=0</math> estimates <math>\cos\theta</math>.


== Radius of convergence in complex analysis ==
== Radius of convergence in complex analysis ==
A power series with a positive radius of convergence can be made into a [[holomorphic function]] by taking its argument to be a complex variable. The radius of convergence can be characterized by the following theorem:
A power series with a positive radius of convergence can be made into a [[holomorphic function]] by taking its argument to be a complex variable. The radius of convergence can be characterized by the following theorem:

:The radius of convergence of a power series ''f'' centered on a point ''a'' is equal to the distance from ''a'' to the nearest point where ''f'' cannot be defined in a way that makes it holomorphic.
: The radius of convergence of a power series ''f'' centered on a point ''a'' is equal to the distance from ''a'' to the nearest point where ''f'' cannot be defined in a way that makes it holomorphic.

The set of all points whose distance to ''a'' is strictly less than the radius of convergence is called the ''disk of convergence''.
The set of all points whose distance to ''a'' is strictly less than the radius of convergence is called the ''disk of convergence''.

[[File:TaylorComplexConv.png|thumb|300px|Radius of convergence (white) and Taylor approximations (blue) for <math>\frac{1}{1+z^2}</math>.]]


''The nearest point'' means the nearest point in the [[complex plane]], not necessarily on the real line, even if the center and all coefficients are real. For example, the function
''The nearest point'' means the nearest point in the [[complex plane]], not necessarily on the real line, even if the center and all coefficients are real. For example, the function


:<math>f(z)=\frac{1}{1+z^2}</math>
: <math>f(z)=\frac 1 {1+z^2}</math>


has no singularities on the real line, since <math>1+z^2</math> has no real roots. Its Taylor series about 0 is given by
has no singularities on the real line, since <math>1+z^2</math> has no real roots. Its Taylor series about 0 is given by
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:<math>\sum_{n=0}^\infty (-1)^n z^{2n}.</math>
:<math>\sum_{n=0}^\infty (-1)^n z^{2n}.</math>


The root test shows that its radius of convergence is 1. In accordance with this, the function ''&fnof;''(''z'') has singularities at&nbsp;±''i'', which are at a distance 1 from&nbsp;0.
The root test shows that its radius of convergence is 1. In accordance with this, the function ''f''(''z'') has singularities at&nbsp;±''i'', which are at a distance 1 from&nbsp;0.


For a proof of this theorem, see [[analyticity of holomorphic functions]].
For a proof of this theorem, see [[analyticity of holomorphic functions]].


===A simple example===
===A simple example===
The arctangent function of [[trigonometry]] can be expanded in a power series familiar to calculus students:
The arctangent function of [[trigonometry]] can be expanded in a power series:


:<math>\arctan(z)=z-\frac{z^3}{3}+\frac{z^5}{5}-\frac{z^7}{7}+\cdots .</math>
:<math>\arctan(z)=z-\frac{z^3} 3 + \frac{z^5} 5 -\frac{z^7} 7 +\cdots .</math>


It is easy to apply the root test in this case to find that the radius of convergence is 1.
It is easy to apply the root test in this case to find that the radius of convergence is 1.
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Consider this power series:
Consider this power series:


:<math>\frac{z}{e^z-1}=\sum_{n=0}^\infty \frac{B_n}{n!} z^n </math>
:<math>\frac z {e^z-1}=\sum_{n=0}^\infty \frac{B_n}{n!} z^n </math>


where the rational numbers ''B''<sub>''n''</sub> are the [[Bernoulli numbers]]. It may be cumbersome to try to apply the ratio test to find the radius of convergence of this series. But the theorem of complex analysis stated above quickly solves the problem. At ''z'' = 0, there is in effect no singularity since [[removable singularity|the singularity is removable]]. The only non-removable singularities are therefore located at the ''other'' points where the denominator is zero. We solve
where the rational numbers ''B''<sub>''n''</sub> are the [[Bernoulli numbers]]. It may be cumbersome to try to apply the ratio test to find the radius of convergence of this series. But the theorem of complex analysis stated above quickly solves the problem. At ''z'' = 0, there is in effect no singularity since [[removable singularity|the singularity is removable]]. The only non-removable singularities are therefore located at the ''other'' points where the denominator is zero. We solve


:<math>e^z-1=0\,</math>
:<math>e^z - 1 = 0</math>


by recalling that if ''z'' = ''x''&nbsp;+&nbsp;''iy'' and ''e''<sup>&nbsp;''iy''</sup>&nbsp;=&nbsp;cos(''y'')&nbsp;+&nbsp;''i''&nbsp;sin(''y'') then
by recalling that if {{math|1=''z'' = ''x'' + ''iy''}} and {{math|1=''e''{{i sup|''iy''}} = cos(''y'') + ''i'' sin(''y'')}} then


:<math>e^z = e^x e^{iy} = e^x(\cos(y)+i\sin(y)),\,</math>
:<math>e^z = e^x e^{iy} = e^x(\cos(y)+i\sin(y)),</math>


and then take ''x'' and ''y'' to be real. Since ''y'' is real, the absolute value of cos(''y'')&nbsp;+&nbsp;''i''&nbsp;sin(''y'') is necessarily 1. Therefore, the absolute value of ''e''<sup>&nbsp;''z''</sup> can be 1 only if ''e''<sup>&nbsp;''x''</sup> is 1; since ''x'' is real, that happens only if ''x'' = 0. Therefore ''z'' is pure imaginary and cos(''y'')&nbsp;+&nbsp;''i''&nbsp;sin(''y'') = 1. Since ''y'' is real, that happens only if cos(''y'') = 1 and sin(''y'') = 0, so that ''y'' is an integral multiple of&nbsp;. Consequently the singular points of this function occur at
and then take ''x'' and ''y'' to be real. Since ''y'' is real, the absolute value of {{math|cos(''y'') + ''i'' sin(''y'')}} is necessarily 1. Therefore, the absolute value of ''e''{{i sup|''z''}} can be 1 only if ''e''{{i sup|''x''}} is 1; since ''x'' is real, that happens only if ''x'' = 0. Therefore ''z'' is purely imaginary and {{math|1=cos(''y'') + ''i'' sin(''y'') = 1}}. Since ''y'' is real, that happens only if cos(''y'') = 1 and sin(''y'') = 0, so that ''y'' is an integer multiple of&nbsp;2{{pi}}. Consequently the singular points of this function occur at


:''z'' = a nonzero integer multiple of&nbsp;''i''.
: ''z'' = a nonzero integer multiple of&nbsp;2{{pi}}''i''.


The singularities nearest 0, which is the center of the power series expansion, are at ±''i''. The distance from the center to either of those points is , so the radius of convergence is&nbsp;.
The singularities nearest 0, which is the center of the power series expansion, are at ±2{{pi}}''i''. The distance from the center to either of those points is 2{{pi}}, so the radius of convergence is&nbsp;2{{pi}}.


== Convergence on the boundary ==
== Convergence on the boundary ==
If the power series is expanded around the point ''a'' and the radius of convergence is ''r'', then the set of all points ''z'' such that |''z''&nbsp;&minus;&nbsp;''a''| = ''r'' is a [[circle]] called the ''boundary'' of the disk of convergence. A power series may diverge at every point on the boundary, or diverge on some points and converge at other points, or converge at all the points on the boundary. Furthermore, even if the series converges on the boundary, it does not necessarily converge absolutely.
If the power series is expanded around the point ''a'' and the radius of convergence is {{math|''r''}}, then the set of all points {{math|''z''}} such that {{math|1={{mabs|''z''''a''}} = ''r''}} is a [[circle]] called the ''boundary'' of the disk of convergence. A power series may diverge at every point on the boundary, or diverge on some points and converge at other points, or converge at all the points on the boundary. Furthermore, even if the series converges everywhere on the boundary (even uniformly), it does not necessarily converge absolutely.


Example 1: The power series for the function ƒ(''z'') = (1&nbsp;&minus;&nbsp;''z'')<sup>&minus;1</sup>, expanded around ''z'' = 0, has radius of convergence 1 and diverges at every point on the boundary.
Example 1: The power series for the function {{math|1=''f''(''z'') = 1/(1''z'')}}, expanded around {{math|1=''z'' = 0}}, which is simply
:<math> \sum_{n=0}^\infty z^n,</math>
has radius of convergence 1 and diverges at every point on the boundary.

Example 2: The power series for {{math|1=''g''(''z'') = −ln(1 − ''z'')}}, expanded around {{math|1=''z'' = 0}}, which is
:<math> \sum_{n=1}^\infty \frac{1}{n} z^n,</math>
has radius of convergence 1, and diverges for {{math|1=''z'' = 1}} but converges for all other points on the boundary. The function {{math|''f''(''z'')}} of Example 1 is the [[derivative]] of {{math|''g''(''z'')}}.


Example 2: The power series for ''g''(''z'') = ln(1&nbsp;&minus;&nbsp;''z'') has radius of convergence ''r'' = 1 expanded around ''z'' = 0, and diverges for ''z'' = 1 but converges for all other points on the boundary. ƒ(''z'') in Example 1 is the [[derivative]] of the negative of ''g''(''z'').
[[Image:TaylorComplexConv.png|thumb|300px|A graph of the functions explained in the text: Approximations in red and blue, circle of convergence in white]]
Example 3: The power series
Example 3: The power series
:<math> \sum_{n=1}^\infty \frac 1 {n^2} z^n </math>

has radius of convergence 1 and converges everywhere on the boundary absolutely. If {{math|''h''}} is the function represented by this series on the unit disk, then the derivative of ''h''(''z'') is equal to ''g''(''z'')/''z'' with ''g'' of Example 2. It turns out that {{math|''h''(''z'')}} is the [[dilogarithm]] function.
:<math> \sum_{n=1}^\infty \frac{1}{n^2} z^n </math>

has radius of convergence 1 and converges everywhere on the boundary. If ''h''(''z'') is the function represented by this series, then the derivative of ''h''(''z'') is ''g''(''z'') divided by ''z'' in Example 2. It turns out that ''h''(''z'') is the [[dilogarithm]] function.


Example 4: The power series
Example 4: The power series
:<math>\sum_{i=1}^\infty a_i z^i \text{ where } a_i = \frac{(-1)^{n-1}}{2^nn}\text{ for }2^{n-1}\le i < 2^n.</math>
:<math>\sum_{i=1}^\infty a_i z^i \text{ where } a_i = \frac{(-1)^{n-1}}{2^nn}\text{ for } n = \lfloor\log_2(i)\rfloor+1\text{, the unique integer with }2^{n-1}\le i < 2^n,</math>
has radius of convergence 1 and converges [[uniform convergence|uniformly]] on the entire boundary {{math|1={{mabs|''z''}} = 1}}, but does not [[Absolute convergence|converge absolutely]] on the boundary.<ref>{{cite journal |url=https://eudml.org/doc/215384|title=O szeregu potęgowym, który jest zbieżny na całem swem kole zbieżności jednostajnie, ale nie bezwzględnie|journal=Prace Matematyczno-Fizyczne|year=1918|volume=29|issue=1|pages=263–266|last1=Sierpiński|first1=W.|author-link=Wacław Sierpiński}}</ref>


==Rate of convergence==
has radius of convergence 1 and converges [[uniform convergence|uniformly]] on the boundary {|''z''|&nbsp;=&nbsp;1}, but does not [[Absolute convergence|converge absolutely]] on the boundary.<ref>{{citation|last=Sierpiński|first=Wacław|author-link=Wacław Sierpiński|year=1918|title=O szeregu potęgowym który jest zbieżny na całem swem kole zbieżności jednostajnie ale nie bezwzględnie|periodical=Prace matematyka-fizyka|volume=29|pages=263&ndash;266}}</ref>

==Comments on rate of convergence==


If we expand the function
If we expand the function


:<math>f(x)=\sin x = \sum^{\infin}_{n=0} \frac{(-1)^n}{(2n+1)!} x^{2n+1} = x - \frac{x^3}{3!} + \frac{x^5}{5!} - \cdots\text{ for all } x</math>
:<math>\sin x = \sum^{\infty}_{n=0} \frac{(-1)^n}{(2n+1)!} x^{2n+1} = x - \frac{x^3}{3!} + \frac{x^5}{5!} - \cdots\text{ for all } x</math>

around the point ''x'' = 0, we find out that the radius of convergence of this series is <math>\scriptstyle\infty</math> meaning that this series converges for all complex numbers. However, in applications, one is often interested in the precision of a [[numerical analysis|numerical answer]]. Both the number of terms and the value at which the series is to be evaluated affect the accuracy of the answer. For example, if we want to calculate ƒ(0.1) = sin(0.1) accurate up to five decimal places, we only need the first two terms of the series. However, if we want the same precision for ''x'' = 1, we must evaluate and sum the first five terms of the series. For ƒ(10), one requires the first 18 terms of the series, and for ƒ(100), we need to evaluate the first 141 terms.

So the fastest convergence of a power series expansion is at the center, and as one moves away from the center of convergence, the [[rate of convergence]] slows down until you reach the boundary (if it exists) and cross over, in which case the [[Series (mathematics)|series]] will diverge.

== A graphical example==
Consider the function 1/(''z''<sup>2</sup>&nbsp;+&nbsp;1).

This function has poles at&nbsp;''z''&nbsp;=&nbsp;±''i''.


around the point ''x'' = 0, we find out that the radius of convergence of this series is <math>\infty</math> meaning that this series converges for all complex numbers. However, in applications, one is often interested in the precision of a [[numerical analysis|numerical answer]]. Both the number of terms and the value at which the series is to be evaluated affect the accuracy of the answer. For example, if we want to calculate {{math|sin(0.1)}} accurate up to five decimal places, we only need the first two terms of the series. However, if we want the same precision for {{math|1=''x'' = 1}} we must evaluate and sum the first five terms of the series. For {{math|sin(10)}}, one requires the first 18 terms of the series, and for {{math|sin(100)}} we need to evaluate the first 141 terms.
As seen in the first example, the radius of convergence of this function's series in powers of (''z''&nbsp;&minus;&nbsp;0) is 1, as the distance from 0 to each of those poles is&nbsp;1.


So for these particular values the fastest convergence of a power series expansion is at the center, and as one moves away from the center of convergence, the [[rate of convergence]] slows down until you reach the boundary (if it exists) and cross over, in which case the [[Series (mathematics)|series]] will diverge.
Then the [[Taylor series]] of this function around ''z''&nbsp;=&nbsp;0 will only converge if |''z''|&nbsp;<&nbsp;1, as depicted on the example on the right.


==Abscissa of convergence of a Dirichlet series==
==Abscissa of convergence of a Dirichlet series==


An analogous concept is the '''abscissa of convergence of a [[Dirichlet series]]
An analogous concept is the [[abscissa of convergence|abscissa of convergence of a Dirichlet series]]


:<math>\sum_{n=1}^\infty {a_n \over n^s}.</math>
:<math>\sum_{n=1}^\infty \frac{a_n}{n^s}.</math>


Such a series converges if the real part of ''s'' is greater than a particular number depending on the coefficients ''a''<sub>''n''</sub>: the [[abscissa]] of convergence.
Such a series converges if the real part of ''s'' is greater than a particular number depending on the coefficients ''a''<sub>''n''</sub>: the [[abscissa]] of convergence.
Line 156: Line 158:
==References==
==References==
* {{Citation | last1=Brown | first1=James | last2=Churchill | first2=Ruel | title=Complex variables and applications | publisher=[[McGraw-Hill]] | location=New York | isbn=978-0-07-010905-6 | year=1989}}
* {{Citation | last1=Brown | first1=James | last2=Churchill | first2=Ruel | title=Complex variables and applications | publisher=[[McGraw-Hill]] | location=New York | isbn=978-0-07-010905-6 | year=1989}}
* {{Citation | last1=Stein | first1=Elias | authorlink=Elias M. Stein |last2=Shakarchi | first2=Rami | title=Complex Analysis | publisher=[[Princeton University Press]] | location=Princeton, New Jersey | isbn=0-691-11385-8 | year=2003}}
* {{Citation | last1=Stein | first1=Elias | author-link=Elias M. Stein |last2=Shakarchi | first2=Rami | title=Complex Analysis | publisher=[[Princeton University Press]] | location=Princeton, New Jersey | isbn=0-691-11385-8 | year=2003}}

==See also==
* [[Abel's theorem]]
* [[Convergence tests]]
* [[Root test]]


==External links==
==External links==
*[http://www.lassp.cornell.edu/sethna/Cracks/What_Is_Radius_of_Convergence.html What is radius of convergence?]
*[http://www.lassp.cornell.edu/sethna/Cracks/What_Is_Radius_of_Convergence.html What is radius of convergence?]


[[Category:Complex analysis]]
[[Category:Analytic functions]]
[[Category:Mathematical series]]
[[Category:Convergence (mathematics)]]
[[Category:Mathematical physics]]

[[Category:Radii]]
[[ca:Radi de convergència]]
[[de:Konvergenzradius]]
[[es:Radio de convergencia]]
[[fr:Rayon de convergence]]
[[it:Raggio di convergenza]]
[[ja:収束半径]]
[[pt:Raio de convergência]]
[[ru:Круг сходимости]]
[[sl:Konvergenčni polmer]]
[[sv:Konvergensradie]]
[[tr:Yakınsaklık yarıçapı]]
[[zh:收斂半徑]]

Latest revision as of 00:14, 9 September 2024

In mathematics, the radius of convergence of a power series is the radius of the largest disk at the center of the series in which the series converges. It is either a non-negative real number or . When it is positive, the power series converges absolutely and uniformly on compact sets inside the open disk of radius equal to the radius of convergence, and it is the Taylor series of the analytic function to which it converges. In case of multiple singularities of a function (singularities are those values of the argument for which the function is not defined), the radius of convergence is the shortest or minimum of all the respective distances (which are all non-negative numbers) calculated from the center of the disk of convergence to the respective singularities of the function.

Definition

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For a power series f defined as:

where

  • a is a complex constant, the center of the disk of convergence,
  • cn is the n-th complex coefficient, and
  • z is a complex variable.

The radius of convergence r is a nonnegative real number or such that the series converges if

and diverges if

Some may prefer an alternative definition, as existence is obvious:

On the boundary, that is, where |z − a| = r, the behavior of the power series may be complicated, and the series may converge for some values of z and diverge for others. The radius of convergence is infinite if the series converges for all complex numbers z.[1]

Finding the radius of convergence

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Two cases arise:

  • The first case is theoretical: when you know all the coefficients then you take certain limits and find the precise radius of convergence.
  • The second case is practical: when you construct a power series solution of a difficult problem you typically will only know a finite number of terms in a power series, anywhere from a couple of terms to a hundred terms. In this second case, extrapolating a plot estimates the radius of convergence.

Theoretical radius

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The radius of convergence can be found by applying the root test to the terms of the series. The root test uses the number

"lim sup" denotes the limit superior. The root test states that the series converges if C < 1 and diverges if C > 1. It follows that the power series converges if the distance from z to the center a is less than

and diverges if the distance exceeds that number; this statement is the Cauchy–Hadamard theorem. Note that r = 1/0 is interpreted as an infinite radius, meaning that f is an entire function.

The limit involved in the ratio test is usually easier to compute, and when that limit exists, it shows that the radius of convergence is finite.

This is shown as follows. The ratio test says the series converges if

That is equivalent to

Practical estimation of radius in the case of real coefficients

[edit]
Plots of the function
The solid green line is the straight-line asymptote in the Domb–Sykes plot,[2] plot (b), which intercepts the vertical axis at −2 and has a slope +1. Thus there is a singularity at and so the radius of convergence is

Usually, in scientific applications, only a finite number of coefficients are known. Typically, as increases, these coefficients settle into a regular behavior determined by the nearest radius-limiting singularity. In this case, two main techniques have been developed, based on the fact that the coefficients of a Taylor series are roughly exponential with ratio where r is the radius of convergence.

  • The basic case is when the coefficients ultimately share a common sign or alternate in sign. As pointed out earlier in the article, in many cases the limit exists, and in this case . Negative means the convergence-limiting singularity is on the negative axis. Estimate this limit, by plotting the versus , and graphically extrapolate to (effectively ) via a linear fit. The intercept with estimates the reciprocal of the radius of convergence, . This plot is called a Domb–Sykes plot.[3]
  • The more complicated case is when the signs of the coefficients have a more complex pattern. Mercer and Roberts proposed the following procedure.[4] Define the associated sequence Plot the finitely many known versus , and graphically extrapolate to via a linear fit. The intercept with estimates the reciprocal of the radius of convergence, .
    This procedure also estimates two other characteristics of the convergence limiting singularity. Suppose the nearest singularity is of degree and has angle to the real axis. Then the slope of the linear fit given above is . Further, plot versus , then a linear fit extrapolated to has intercept at .

Radius of convergence in complex analysis

[edit]

A power series with a positive radius of convergence can be made into a holomorphic function by taking its argument to be a complex variable. The radius of convergence can be characterized by the following theorem:

The radius of convergence of a power series f centered on a point a is equal to the distance from a to the nearest point where f cannot be defined in a way that makes it holomorphic.

The set of all points whose distance to a is strictly less than the radius of convergence is called the disk of convergence.

Radius of convergence (white) and Taylor approximations (blue) for .

The nearest point means the nearest point in the complex plane, not necessarily on the real line, even if the center and all coefficients are real. For example, the function

has no singularities on the real line, since has no real roots. Its Taylor series about 0 is given by

The root test shows that its radius of convergence is 1. In accordance with this, the function f(z) has singularities at ±i, which are at a distance 1 from 0.

For a proof of this theorem, see analyticity of holomorphic functions.

A simple example

[edit]

The arctangent function of trigonometry can be expanded in a power series:

It is easy to apply the root test in this case to find that the radius of convergence is 1.

A more complicated example

[edit]

Consider this power series:

where the rational numbers Bn are the Bernoulli numbers. It may be cumbersome to try to apply the ratio test to find the radius of convergence of this series. But the theorem of complex analysis stated above quickly solves the problem. At z = 0, there is in effect no singularity since the singularity is removable. The only non-removable singularities are therefore located at the other points where the denominator is zero. We solve

by recalling that if z = x + iy and eiy = cos(y) + i sin(y) then

and then take x and y to be real. Since y is real, the absolute value of cos(y) + i sin(y) is necessarily 1. Therefore, the absolute value of ez can be 1 only if ex is 1; since x is real, that happens only if x = 0. Therefore z is purely imaginary and cos(y) + i sin(y) = 1. Since y is real, that happens only if cos(y) = 1 and sin(y) = 0, so that y is an integer multiple of 2π. Consequently the singular points of this function occur at

z = a nonzero integer multiple of 2πi.

The singularities nearest 0, which is the center of the power series expansion, are at ±2πi. The distance from the center to either of those points is 2π, so the radius of convergence is 2π.

Convergence on the boundary

[edit]

If the power series is expanded around the point a and the radius of convergence is r, then the set of all points z such that |za| = r is a circle called the boundary of the disk of convergence. A power series may diverge at every point on the boundary, or diverge on some points and converge at other points, or converge at all the points on the boundary. Furthermore, even if the series converges everywhere on the boundary (even uniformly), it does not necessarily converge absolutely.

Example 1: The power series for the function f(z) = 1/(1 − z), expanded around z = 0, which is simply

has radius of convergence 1 and diverges at every point on the boundary.

Example 2: The power series for g(z) = −ln(1 − z), expanded around z = 0, which is

has radius of convergence 1, and diverges for z = 1 but converges for all other points on the boundary. The function f(z) of Example 1 is the derivative of g(z).

Example 3: The power series

has radius of convergence 1 and converges everywhere on the boundary absolutely. If h is the function represented by this series on the unit disk, then the derivative of h(z) is equal to g(z)/z with g of Example 2. It turns out that h(z) is the dilogarithm function.

Example 4: The power series

has radius of convergence 1 and converges uniformly on the entire boundary |z| = 1, but does not converge absolutely on the boundary.[5]

Rate of convergence

[edit]

If we expand the function

around the point x = 0, we find out that the radius of convergence of this series is meaning that this series converges for all complex numbers. However, in applications, one is often interested in the precision of a numerical answer. Both the number of terms and the value at which the series is to be evaluated affect the accuracy of the answer. For example, if we want to calculate sin(0.1) accurate up to five decimal places, we only need the first two terms of the series. However, if we want the same precision for x = 1 we must evaluate and sum the first five terms of the series. For sin(10), one requires the first 18 terms of the series, and for sin(100) we need to evaluate the first 141 terms.

So for these particular values the fastest convergence of a power series expansion is at the center, and as one moves away from the center of convergence, the rate of convergence slows down until you reach the boundary (if it exists) and cross over, in which case the series will diverge.

Abscissa of convergence of a Dirichlet series

[edit]

An analogous concept is the abscissa of convergence of a Dirichlet series

Such a series converges if the real part of s is greater than a particular number depending on the coefficients an: the abscissa of convergence.

Notes

[edit]
  1. ^ Mathematical Analysis-II. Krishna Prakashan Media. 16 November 2010.
  2. ^ See Figure 8.1 in: Hinch, E.J. (1991), Perturbation Methods, Cambridge Texts in Applied Mathematics, vol. 6, Cambridge University Press, p. 146, ISBN 0-521-37897-4
  3. ^ Domb, C.; Sykes, M.F. (1957), "On the susceptibility of a ferromagnetic above the Curie point", Proc. R. Soc. Lond. A, 240 (1221): 214–228, Bibcode:1957RSPSA.240..214D, doi:10.1098/rspa.1957.0078, S2CID 119974403
  4. ^ Mercer, G.N.; Roberts, A.J. (1990), "A centre manifold description of contaminant dispersion in channels with varying flow properties", SIAM J. Appl. Math., 50 (6): 1547–1565, doi:10.1137/0150091
  5. ^ Sierpiński, W. (1918). "O szeregu potęgowym, który jest zbieżny na całem swem kole zbieżności jednostajnie, ale nie bezwzględnie". Prace Matematyczno-Fizyczne. 29 (1): 263–266.

References

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See also

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