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		<id>https://en.formulasearchengine.com/w/index.php?title=Gumbel_distribution&amp;diff=3542</id>
		<title>Gumbel distribution</title>
		<link rel="alternate" type="text/html" href="https://en.formulasearchengine.com/w/index.php?title=Gumbel_distribution&amp;diff=3542"/>
		<updated>2014-01-19T03:37:21Z</updated>

		<summary type="html">&lt;p&gt;75.172.95.102: Referencing an earlier original paper by Gumbel.&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[image:Fresnel Integrals (Unnormalised).svg|250px|thumb|&lt;br /&gt;
&amp;lt;span style=&amp;quot;color:#b30000;&amp;quot;&amp;gt;&#039;&#039;S&#039;&#039;(&#039;&#039;x&#039;&#039;)&amp;lt;/span&amp;gt; and &amp;lt;span style=&amp;quot;color:#00b300;&amp;quot;&amp;gt;&#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;)&amp;lt;/span&amp;gt; The maximum of &#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;) is about 0.977451424. If π&#039;&#039;t&#039;&#039;²/2 were used instead of &#039;&#039;t&#039;&#039;², then the image would be scaled vertically and horizontally (see below).]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Fresnel integrals&#039;&#039;&#039;, &#039;&#039;S&#039;&#039;(&#039;&#039;x&#039;&#039;) and &#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;), are two [[transcendental function]]s named after [[Augustin-Jean Fresnel]] that are used in [[optics]], which are closely related to the [[error function]] (erf). They arise in the description of [[near and far field|far field]] [[Fresnel diffraction]] phenomena, and are defined through the following [[integral]] representations:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;S(x)=\int_0^x \sin(t^2)\,\mathrm{d}t,\quad C(x)=\int_0^x \cos(t^2)\,\mathrm{d}t.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The simultaneous [[parametric equation|parametric plot]] of &#039;&#039;S&#039;&#039;(&#039;&#039;x&#039;&#039;) and &#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;) is the [[Euler spiral]] (also known as the Cornu spiral or clothoid). Recently, they have been used in the design of highways and other engineering projects.&amp;lt;ref name=Stewart&amp;gt;{{cite book|last=Stewart|first=James|title=Essential Calculus|year=2007|publisher=Thomson Brooks/Cole|location=Belmont, Calif.|isbn=0-495-01442-7|page=230}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Definition ==&lt;br /&gt;
The Fresnel integrals admit the following [[power series expansion]]s that converge for all &#039;&#039;x&#039;&#039;:&lt;br /&gt;
&lt;br /&gt;
[[image:Fresnel Integrals (Normalised).svg|250px|thumb|&lt;br /&gt;
Normalised Fresnel integrals, &amp;lt;span style=&amp;quot;color:#b30000;&amp;quot;&amp;gt;&#039;&#039;S&#039;&#039;(&#039;&#039;x&#039;&#039;)&amp;lt;/span&amp;gt; and &amp;lt;span style=&amp;quot;color:#00b300;&amp;quot;&amp;gt;&#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;)&amp;lt;/span&amp;gt;. In these curves, the argument of the trigonometric function is π&#039;&#039;t&#039;&#039;&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/2, as opposed to just &#039;&#039;t&#039;&#039;&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; as above.]]&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;S(x)=\int_0^x \sin(t^2)\,\mathrm{d}t=\sum_{n=0}^{\infin}(-1)^n\frac{x^{4n+3}}{(2n+1)!(4n+3)}&amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;C(x)=\int_0^x \cos(t^2)\,\mathrm{d}t=\sum_{n=0}^{\infin}(-1)^n\frac{x^{4n+1}}{(2n)!(4n+1)}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Some authors, including [[Abramowitz and Stegun]], (eqs 7.3.1 &amp;amp;ndash; 7.3.2) use &amp;lt;math&amp;gt;\frac{\pi}{2}t^2&amp;lt;/math&amp;gt; for the argument of the integrals defining &#039;&#039;S&#039;&#039;(&#039;&#039;x&#039;&#039;) and &#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;). To get these functions, multiply the above integrals by &amp;lt;math&amp;gt;\sqrt{\frac{2}{\pi}}&amp;lt;/math&amp;gt; and multiply the argument &#039;&#039;x&#039;&#039; by &amp;lt;math&amp;gt;\sqrt{\frac{\pi}{2}}&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
== Euler spiral ==&lt;br /&gt;
{{Main|Euler spiral}}&lt;br /&gt;
[[Image:Cornu Spiral.svg|250px|thumb|&lt;br /&gt;
Euler spiral (&#039;&#039;x&#039;&#039;,&amp;amp;nbsp;&#039;&#039;y&#039;&#039;)&amp;amp;nbsp;=&amp;amp;nbsp;(&#039;&#039;C&#039;&#039;(&#039;&#039;t&#039;&#039;),&amp;amp;nbsp;&#039;&#039;S&#039;&#039;(&#039;&#039;t&#039;&#039;)). The spiral converges to the centre of the holes in the image as &#039;&#039;t&#039;&#039; tends to positive or negative infinity.]]&lt;br /&gt;
The &#039;&#039;&#039;Euler [[spiral]]&#039;&#039;&#039;, also known as &#039;&#039;&#039;Cornu spiral&#039;&#039;&#039; or &#039;&#039;&#039;clothoid&#039;&#039;&#039;, is the curve generated by a [[parametric plot]] of &#039;&#039;S&#039;&#039;(&#039;&#039;t&#039;&#039;) against &#039;&#039;C&#039;&#039;(&#039;&#039;t&#039;&#039;). The Cornu spiral was created by [[Marie Alfred Cornu]] as a [[nomogram]] for diffraction computations in science and engineering.&lt;br /&gt;
&lt;br /&gt;
From the definitions of Fresnel integrals, the infinitesimals &#039;&#039;dx&#039;&#039; and &#039;&#039;dy&#039;&#039; are thus:&lt;br /&gt;
: &amp;lt;math&amp;gt; \mathrm{d}x = C&#039;(t)\mathrm{d}t = \cos(t^2) \mathrm{d}t \,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt; \mathrm{d}y = S&#039;(t)\mathrm{d}t = \sin(t^2) \mathrm{d}t \,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Thus the length of the spiral measured from the origin can be expressed as:&lt;br /&gt;
&lt;br /&gt;
: &amp;lt;math&amp;gt;L = \int_0^{t_0} {\sqrt {\mathrm{d}x^2 + \mathrm{d}y^2}} = \int_0^{t_0}{\mathrm{d}t} = t_0 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
That is, the parameter {{math| t}} is the curve length measured from the origin (0,0) and the Euler spiral has [[Infinity|infinite]] length. The vector {{math| [cos(t²), sin(t²)]}} also expresses the [[unit vector|unit]] [[tangent vector]] along the spiral, giving θ = {{math| t²}}. Since t is the curve length, the curvature, &amp;lt;math&amp;gt;\kappa&amp;lt;/math&amp;gt; can be expressed as:&lt;br /&gt;
: &amp;lt;math&amp;gt; \kappa = \tfrac {1}{R} = \tfrac {\mathrm{d}\theta}{\mathrm{d}t} = 2t &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
And the rate of change of curvature with respect to the curve length is:&lt;br /&gt;
: &amp;lt;math&amp;gt;\tfrac{\mathrm{d}\kappa}{\mathrm{d}t}=\tfrac {\mathrm{d}^2\theta}{\mathrm{d}t^2} = 2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
An Euler spiral has the property that its [[curvature]] at any point is proportional to the distance along the spiral, measured from the origin.  This property makes it useful as a [[track transition curve|transition curve]] in highway and railway engineering.&lt;br /&gt;
&lt;br /&gt;
If a vehicle follows the spiral at unit speed, the parameter {{math| t}} in the above derivatives also represents the time. That is, a vehicle following the spiral at constant speed will have a constant rate of [[angular acceleration]].&lt;br /&gt;
&lt;br /&gt;
Sections from Euler spirals are commonly incorporated into the shape of roller-coaster loops to make what are known as &amp;quot;[[clothoid loop]]s&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
== Properties ==&lt;br /&gt;
* &#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;) and  &#039;&#039;S&#039;&#039;(&#039;&#039;x&#039;&#039;) are [[odd function]]s of &#039;&#039;x&#039;&#039;.&lt;br /&gt;
* Using the power series expansions above, the Fresnel integrals can be extended to the domain of [[complex number]]s, and they become [[analytic function]]s of a complex variable.&lt;br /&gt;
* The Fresnel integrals can be expressed using the [[error function]] as follows:&amp;lt;ref&amp;gt;functions.wolfram.com, [http://functions.wolfram.com/GammaBetaErf/FresnelS/27/01/ Fresnel integral S: Representations through equivalent functions] and [http://functions.wolfram.com/GammaBetaErf/FresnelC/27/01/ Fresnel integral C: Representations through equivalent functions].  Note: Wolfram uses the Abramowitz &amp;amp; Stegun convention, which differs from the one in this article by factors of &amp;lt;math&amp;gt;\sqrt{\pi/2}&amp;lt;/math&amp;gt;&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
::&amp;lt;math&amp;gt;S(z)=\sqrt{\frac{\pi}{2}} \frac{1+i}{4} \left[ \operatorname{erf}\left(\frac{1+i}{\sqrt{2}}z\right) -i \operatorname{erf}\left(\frac{1-i}{\sqrt{2}}z\right) \right],&amp;lt;/math&amp;gt;&lt;br /&gt;
::&amp;lt;math&amp;gt;C(z)=\sqrt{\frac{\pi}{2}}\frac{1-i}{4} \left[ \operatorname{erf}\left(\frac{1+i}{\sqrt{2}}z\right) + i \operatorname{erf}\left(\frac{1-i}{\sqrt{2}}z\right) \right].&amp;lt;/math&amp;gt;&lt;br /&gt;
::or &amp;lt;math&amp;gt;S(z) + i C(z) = \sqrt{\frac{\pi}{2}}\frac{1+i}{2} \operatorname{erf}\left(\frac{1+i}{\sqrt{2}}z\right)&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;C&#039;&#039; and  &#039;&#039;S&#039;&#039; are [[entire function]]s.&lt;br /&gt;
* The integrals defining &#039;&#039;C&#039;&#039;(&#039;&#039;x&#039;&#039;) and &#039;&#039;S&#039;&#039;(&#039;&#039;x&#039;&#039;) cannot be evaluated in the [[closed-form expression|closed form]] in terms of [[elementary function]]s, except in special cases. The [[limit of a function|limits]] of these functions as &#039;&#039;x&#039;&#039; goes to infinity are known:&lt;br /&gt;
&lt;br /&gt;
::&amp;lt;math&amp;gt;\int_{0}^{\infty} \cos t^2\,\mathrm{d}t = \int_{0}^{\infty} \sin t^2\,\mathrm{d}t = \frac{\sqrt{2\pi}}{4} = \sqrt{\frac{\pi}{8}}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Evaluation ===&lt;br /&gt;
[[Image:Fresnel Integral Contour.svg|right|250px|thumb|The sector contour used to calculate the limits of the Fresnel integrals]]&lt;br /&gt;
The limits of &#039;&#039;C&#039;&#039; and &#039;&#039;S&#039;&#039; as the argument tends to infinity can be found by the methods of [[complex analysis]]. This uses the [[contour integral]] of the function&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;e^{-\frac{1}{2}t^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
around the boundary of the [[Circular sector|sector]]-shaped region in the [[complex plane]] formed by the positive &#039;&#039;x&#039;&#039;-axis, the half-line &#039;&#039;y&#039;&#039;&amp;amp;nbsp;=&amp;amp;nbsp;&#039;&#039;x&#039;&#039;, &#039;&#039;x&#039;&#039; ≥ 0, and the circle of radius &#039;&#039;R&#039;&#039; centered at the origin.&lt;br /&gt;
&lt;br /&gt;
As &#039;&#039;R&#039;&#039; goes to infinity, the integral along the circular arc tends to 0, the integral along the real axis tends to the [[Gaussian integral]]&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \int_{0}^{\infty} e^{-\frac{1}{2}t^2}\mathrm{d}t = &lt;br /&gt;
\sqrt{\frac{\pi}{2}}, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and after routine transformations, the integral along the bisector of the first quadrant can be related to the limit of the Fresnel integrals.&lt;br /&gt;
&lt;br /&gt;
== Generalization ==&lt;br /&gt;
The integral&lt;br /&gt;
&amp;lt;math&amp;gt;\int x^m \exp(ix^n)\mathrm{d}x = \int\sum_{l=0}^\infty\frac{i^lx^{m+nl}}{l!}\mathrm{d}x&lt;br /&gt;
 = \sum_{l=0}^\infty \frac{i^l}{(m+nl+1)}\frac{x^{m+nl+1}}{l!}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
is a [[confluent hypergeometric function]] and also an [[incomplete Gamma function]]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\int x^m \exp(ix^n)\mathrm{d}x =\frac{x^{m+1}}{m+1}\,_1F_1\left(\begin{array}{c}\frac{m+1}{n}\\1+\frac{m+1}{n}\end{array}\mid ix^n\right)&lt;br /&gt;
=\frac{1}{n}i^{(m+1)/n}\gamma(\frac{m+1}{n},-ix^n),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
which reduces to Fresnel integrals if real or imaginary parts are taken:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\int x^m\sin(x^n)\mathrm{d}x = \frac{x^{m+n+1}}{m+n+1}&lt;br /&gt;
\,_1F_2\left(\begin{array}{c}\frac{1}{2}+\frac{m+1}{2n}\\&lt;br /&gt;
\frac{3}{2}+\frac{m+1}{2n},\frac{3}{2}\end{array}\mid -\frac{x^{2n}}{4}\right)&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
The leading term in the asymptotic expansion is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;_1F_1\left(\begin{array}{c}\frac{m+1}{n}\\1+\frac{m+1}{n}\end{array}\mid ix^n\right)\sim \frac{m+1}{n}\Gamma(\frac{m+1}{n})&lt;br /&gt;
e^{i\pi(m+1)/(2n)} x^{-m+1}&amp;lt;/math&amp;gt;,&lt;br /&gt;
&lt;br /&gt;
and therefore&lt;br /&gt;
&amp;lt;math&amp;gt;\int_0^\infty x^m \exp(ix^n)\mathrm{d}x=\frac{1}{n}\Gamma(\frac{m+1}{n})e^{i\pi(m+1)/(2n)}&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
For &#039;&#039;m=0&#039;&#039;, the imaginary part of this equation in particular is&lt;br /&gt;
&amp;lt;math&amp;gt;\int_0^\infty\sin(x^a)\ \mathrm{d}x = \Gamma\left(1+\frac{1}{a}\right)\sin(\frac{\pi}{2a})&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
with the left-hand side converging for &#039;&#039;a&amp;gt;1&#039;&#039; and the right-hand side being its analytical extension to the whole plane less where lie the poles of &amp;lt;math&amp;gt;\Gamma(a^{-1})&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
The Kummer transformation of the confluent hypergeometric function is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; \int x^m \exp(ix^n)\mathrm{d}x = V_{n,m}(x)e^{ix^n}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
with&lt;br /&gt;
&amp;lt;math&amp;gt;V_{n,m}:=\frac{x^{m+1}}{m+1}\,_1F_1\left(\begin{array}{c}1\\1+\frac{m+1}{n}\end{array}\mid -ix^n\right)&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
== Applications ==&lt;br /&gt;
The Fresnel integrals were originally used in the calculation of the field intensity in an environment related to the bending of light around opaque objects.&amp;lt;ref name=Beatty&amp;gt;{{cite web|last=Beatty|first=Thomas|title=How to evaluate Fresnel Integrals|url=http://www.thomasbeatty.com/MATH%20PAGES/ARCHIVES%20-%20NOTES/Complex%20Variables/How%20to%20evaluate%20Fresnel%20Integrals.pdf|work=FGCU MATH - SUMMER 2013|accessdate=27 July 2013}}&amp;lt;/ref&amp;gt; More recently, they have been used in the design of highways and railways, specifically their curvature transition zones&amp;lt;ref name=Stewart /&amp;gt; and roller coasters.&amp;lt;ref name=Beatty /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
* [[Augustin-Jean Fresnel]]&lt;br /&gt;
* [[Fresnel zone]]&lt;br /&gt;
* [[Track transition curve]]&lt;br /&gt;
* [[Euler spiral]]&lt;br /&gt;
* [[Zone plate]]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
*{{cite book|first1= A. |last1=van Wijngaarden&lt;br /&gt;
|first2= W. L. |last2=Scheen&lt;br /&gt;
|title=Table of Fresnel Integrals&lt;br /&gt;
|year=1949&lt;br /&gt;
|series= Verhandl. Konink. Ned. Akad. Wetenschapen&lt;br /&gt;
|volume=19&lt;br /&gt;
|number=4&lt;br /&gt;
}}&lt;br /&gt;
*{{cite journal|first1=J. |last1=Boersma&lt;br /&gt;
|title=Computation of Fresnel Integrals&lt;br /&gt;
|journal=Math. Comp.&lt;br /&gt;
|volume=14&lt;br /&gt;
|year=1960&lt;br /&gt;
|pages=380-380&lt;br /&gt;
|mr=0121973&lt;br /&gt;
|doi=10.1090/S0025-5718-1960-0121973-3 &lt;br /&gt;
}}&lt;br /&gt;
* {{AS ref|7|297}}&lt;br /&gt;
*{{cite journal|first1=Roland| last1=Bulirsch&lt;br /&gt;
|title=Numerical calculation of the sine, cosine and Fresnel integrals&lt;br /&gt;
|year=1967&lt;br /&gt;
|volume=9&lt;br /&gt;
|number=5&lt;br /&gt;
|pages=380–385&lt;br /&gt;
|journal=Numer. Math.&lt;br /&gt;
|doi=10.1007/BF02162153&lt;br /&gt;
}}&lt;br /&gt;
*{{cite journal|first1=R. J.|last1=Hangelbroek&lt;br /&gt;
|title=Numerical approximation of Fresnel integrals by means of Chebyshev polynomials&lt;br /&gt;
|journal=J. Eng. Math.&lt;br /&gt;
|year=1967&lt;br /&gt;
|volume=1&lt;br /&gt;
|number=1&lt;br /&gt;
|pages=37–50&lt;br /&gt;
|doi=10.1007/BF01793638&lt;br /&gt;
|bibcode = 1967JEnMa...1...37H }}&lt;br /&gt;
*{{Citation | last1=Press | first1=WH | last2=Teukolsky | first2=SA | last3=Vetterling | first3=WT | last4=Flannery | first4=BP | year=2007 | title=Numerical Recipes: The Art of Scientific Computing | edition=3rd | publisher=Cambridge University Press |  publication-place=New York | isbn=978-0-521-88068-8 | chapter=Section 6.8.1. Fresnel Integrals | chapter-url=http://apps.nrbook.com/empanel/index.html#pg=297}}&lt;br /&gt;
*{{cite web|first1=R. |last1=Nave&lt;br /&gt;
|url=http://hyperphysics.phy-astr.gsu.edu/hbase/phyopt/cornu.html#c1&lt;br /&gt;
|title=The Cornu spiral&lt;br /&gt;
|year=2002}} &#039;&#039;(Uses πt²/2 instead of t².)&#039;&#039;&lt;br /&gt;
*{{dlmf|id=7|title=Error Functions, Dawson’s and Fresnel Integrals|first=N. M. |last=Temme}}&lt;br /&gt;
*{{cite arxiv|first1=Mohammad |last1=Alazah&lt;br /&gt;
|title=Computing fresnel integrals via modified trapezium rules&lt;br /&gt;
|year=2012&lt;br /&gt;
|eprint=1209.3451&lt;br /&gt;
}}&lt;br /&gt;
*{{cite arxiv|first1 =R. J. | last1=Mathar&lt;br /&gt;
|title=Series Expansion of Generalized Fresnel Integrals |year=2012 |eprint=1211.3963&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
*[http://ab-initio.mit.edu/Faddeeva Faddeeva Package], [[Free and open source software|free/open-source]] C++/C code to compute complex error functions (from which the Fresnel integrals can be obtained), with wrappers for Matlab, Python, and other languages.&lt;br /&gt;
* {{springer|title=Fresnel integrals|id=p/f041720}}&lt;br /&gt;
*{{cite web&lt;br /&gt;
|url=http://fy.chalmers.se/LISEBERG/eng/loop_pe.html&lt;br /&gt;
|title=Roller Coaster Loop Shapes&lt;br /&gt;
|accessdate=2008-08-13}} {{Dead link|date=September 2010|bot=H3llBot}}&lt;br /&gt;
*{{mathworld|title=Fresnel Integrals|urlname=FresnelIntegrals}}&lt;br /&gt;
*{{mathworld|title=Cornu Spiral|urlname=CornuSpiral}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Integral calculus]]&lt;br /&gt;
[[Category:Spirals]]&lt;br /&gt;
[[Category:Optics]]&lt;br /&gt;
[[Category:Special functions]]&lt;br /&gt;
[[Category:Special hypergeometric functions]]&lt;br /&gt;
[[Category:Analytic functions]]&lt;/div&gt;</summary>
		<author><name>75.172.95.102</name></author>
	</entry>
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