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		<title>imported&gt;Hellacioussatyr: rm :-indents (MOS:INDENT)</title>
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		<summary type="html">&lt;p&gt;rm :-indents (&lt;a href=&quot;/wiki143/index.php?title=MOS:INDENT&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;MOS:INDENT (page does not exist)&quot;&gt;MOS:INDENT&lt;/a&gt;)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{short description|Mathematical function}}&lt;br /&gt;
In [[mathematics]], the family of &amp;#039;&amp;#039;&amp;#039;Debye functions&amp;#039;&amp;#039;&amp;#039; is defined by&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;D_n(x) = \frac{n}{x^n} \int_0^x \frac{t^n}{e^t - 1}\,dt.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The functions are named in honor of [[Peter Debye]], who came across this function (with &amp;#039;&amp;#039;n&amp;#039;&amp;#039; = 3) in 1912 when he analytically computed the [[heat capacity]] of what is now called the [[Debye model]].&lt;br /&gt;
&lt;br /&gt;
== Mathematical properties ==&lt;br /&gt;
&lt;br /&gt;
=== Relation to other functions ===&lt;br /&gt;
&lt;br /&gt;
The Debye functions are closely related to the [[polylogarithm]].&lt;br /&gt;
&lt;br /&gt;
=== Series expansion ===&lt;br /&gt;
They have the series expansion&amp;lt;ref&amp;gt;{{AS ref|27|998}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;D_n(x) = 1 - \frac{n}{2(n+1)} x + n \sum_{k=1}^\infty \frac{B_{2k}}{(2k+n)(2k)!} x^{2k}, \quad |x| &amp;lt; 2\pi,\ n \ge 1,&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;B_n&amp;lt;/math&amp;gt; is the {{mvar|n}}-th [[Bernoulli number]].&lt;br /&gt;
&lt;br /&gt;
=== Limiting values ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;\lim_{x \to 0} D_n(x) = 1.&amp;lt;/math&amp;gt;&lt;br /&gt;
If &amp;lt;math&amp;gt;\Gamma&amp;lt;/math&amp;gt; is the [[gamma function]] and &amp;lt;math&amp;gt;\zeta&amp;lt;/math&amp;gt; is the [[Riemann zeta function]], then, for &amp;lt;math&amp;gt;x \gg 0&amp;lt;/math&amp;gt;,&amp;lt;ref name=&amp;quot;Zwillinger_2014&amp;quot;&amp;gt;{{cite book |author-first1=Izrail Solomonovich |author-last1=Gradshteyn |author-link1=Izrail Solomonovich Gradshteyn |author-first2=Iosif Moiseevich |author-last2=Ryzhik |author-link2=Iosif Moiseevich Ryzhik |author-first3=Yuri Veniaminovich |author-last3=Geronimus |author-link3=Yuri Veniaminovich Geronimus |author-first4=Michail Yulyevich |author-last4=Tseytlin |author-link4=Michail Yulyevich Tseytlin |author-first5=Alan |author-last5=Jeffrey |editor-first1=Daniel |editor-last1=Zwillinger |editor-first2=Victor Hugo |editor-last2=Moll |editor-link2=Victor Hugo Moll |translator=Scripta Technica, Inc. |title=Table of Integrals, Series, and Products |publisher=[[Academic Press, Inc.]] |date=2015 |orig-year=October 2014 |edition=8 |language=English |isbn=978-0-12-384933-5 |lccn=2014010276 &amp;lt;!-- |url=https://books.google.com/books?id=NjnLAwAAQBAJ |access-date=2016-02-21--&amp;gt;|title-link=Gradshteyn and Ryzhik |chapter=3.411. |pages=355ff}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;D_n(x) = \frac{n}{x^n} \int_0^x \frac{t^n\,dt}{e^t-1} \sim \frac{n}{x^n}\Gamma(n + 1) \zeta(n + 1), \qquad \operatorname{Re} n &amp;gt; 0,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Derivative ===&lt;br /&gt;
&lt;br /&gt;
The derivative obeys the relation&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;x D^{\prime}_n(x) = n \left(B(x) - D_n(x)\right),&amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;B(x) = x/(e^x-1)&amp;lt;/math&amp;gt; is the Bernoulli function.&lt;br /&gt;
&lt;br /&gt;
== Applications in solid-state physics ==&lt;br /&gt;
&lt;br /&gt;
=== The Debye model ===&lt;br /&gt;
&lt;br /&gt;
The [[Debye model]] has a [[Density of states|density of vibrational states]]&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;g_\text{D}(\omega) = \frac{9\omega^2}{\omega_\text{D}^3} \,, \qquad 0\le\omega\le\omega_\text{D}&amp;lt;/math&amp;gt;&lt;br /&gt;
with the {{em|Debye frequency}} {{math|&amp;#039;&amp;#039;ω&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;D&amp;lt;/sub&amp;gt;}}.&lt;br /&gt;
&lt;br /&gt;
=== Internal energy and heat capacity ===&lt;br /&gt;
&lt;br /&gt;
Inserting {{math|&amp;#039;&amp;#039;g&amp;#039;&amp;#039;}} into the internal energy &lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;U = \int_0^\infty d\omega\,g(\omega)\,\hbar\omega\,n(\omega)&amp;lt;/math&amp;gt;&lt;br /&gt;
with the [[Bose–Einstein distribution]]&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;n(\omega) = \frac{1}{\exp(\hbar\omega / k_\text{B} T)-1}.&amp;lt;/math&amp;gt;&lt;br /&gt;
one obtains&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;U = 3 k_\text{B}T \, D_3(\hbar\omega_\text{D} / k_\text{B}T).&amp;lt;/math&amp;gt;&lt;br /&gt;
The heat capacity is the derivative thereof.&lt;br /&gt;
&lt;br /&gt;
=== Mean squared displacement ===&lt;br /&gt;
&lt;br /&gt;
The intensity of [[X-ray diffraction]] or [[neutron diffraction]] at wavenumber &amp;#039;&amp;#039;q&amp;#039;&amp;#039; is given by the [[Debye-Waller factor]] or the [[Lamb-Mössbauer factor]].&lt;br /&gt;
For isotropic systems it takes the form&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;\exp(-2W(q)) = \exp\left(-q^2\langle u_x^2\rangle\right).&amp;lt;/math&amp;gt;&lt;br /&gt;
In this expression, the [[mean squared displacement]] refers to just once Cartesian component {{math|&amp;#039;&amp;#039;u&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;#039;&amp;#039;}} of the vector {{math|&amp;#039;&amp;#039;&amp;#039;u&amp;#039;&amp;#039;&amp;#039;}} that describes the displacement of atoms from their equilibrium positions.&lt;br /&gt;
Assuming harmonicity and developing into normal modes,&amp;lt;ref&amp;gt;Ashcroft &amp;amp; Mermin 1976, App. L,&amp;lt;/ref&amp;gt;&lt;br /&gt;
one obtains&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;2W(q) = \frac{\hbar^2 q^2}{6M k_\text{B}T} \int_0^\infty d\omega \frac{k_\text{B}T}{\hbar\omega}g(\omega) \coth\frac{\hbar\omega}{2k_\text{B}T}=\frac{\hbar^2 q^2}{6M k_\text{B}T} \int_0^\infty d\omega \frac{k_\text{B}T}{\hbar\omega} g(\omega) \left[\frac{2}{\exp(\hbar\omega/k_\text{B}T)-1}+1\right].&amp;lt;/math&amp;gt;&lt;br /&gt;
Inserting the density of states from the Debye model, one obtains&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;2W(q) = \frac{3}{2} \frac{\hbar^2 q^2}{M\hbar\omega_\text{D}} \left[2\left(\frac{k_\text{B}T}{\hbar\omega_\text{D}}\right) D_1{\left(\frac{\hbar\omega_\text{D}}{k_\text{B}T}\right)} + \frac{1}{2}\right].&amp;lt;/math&amp;gt;&lt;br /&gt;
From the above [[power series]] expansion of &amp;lt;math&amp;gt;D_1&amp;lt;/math&amp;gt; follows that the mean square displacement at high temperatures is linear in temperature&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;2W(q) = \frac{3 k_\text{B}T q^2}{M\omega_\text{D}^2}.&amp;lt;/math&amp;gt;&lt;br /&gt;
The absence of &amp;lt;math&amp;gt;\hbar&amp;lt;/math&amp;gt; indicates that this is a [[Classical Physics|classical]] result. Because &amp;lt;math&amp;gt;D_1(x)&amp;lt;/math&amp;gt; goes to zero for &amp;lt;math&amp;gt;x \to \infty&amp;lt;/math&amp;gt; it follows that for &amp;lt;math&amp;gt;T = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;2W(q)=\frac{3}{4}\frac{\hbar^2 q^2}{M\hbar\omega_\text{D}}&amp;lt;/math&amp;gt; ([[Zero-point energy|zero-point motion]]).&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
==Further reading==&lt;br /&gt;
&lt;br /&gt;
* {{AS ref|27|998}}&lt;br /&gt;
* [http://mathworld.wolfram.com/DebyeFunctions.html &amp;quot;Debye function&amp;quot; entry in MathWorld], defines the Debye functions without prefactor &amp;#039;&amp;#039;n&amp;#039;&amp;#039;/&amp;#039;&amp;#039;x&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
== Implementations ==&lt;br /&gt;
* {{cite journal|first1=E. W.|last1=Ng| first2=C. J. |last2=Devine|title=On the computation of Debye functions of integer orders|journal=Math. Comp.|year=1970|volume=24|issue=110 |pages=405–407|doi=10.1090/S0025-5718-1970-0272160-6|mr=0272160|doi-access=free}}&lt;br /&gt;
* {{cite journal|first1=I.|last1=Engeln|first2=D.|last2=Wobig| title=Computation of the generalized Debye functions delta(x,y) and D(x,y)|journal=Colloid &amp;amp; Polymer Science|volume=261|year=1983|pages=736–743|doi=10.1007/BF01410947|s2cid=98476561 }}&lt;br /&gt;
* {{cite journal|first1=Allan J.|last1=MacLeod|title=Algorithm 757: MISCFUN, a software package to compute uncommon special functions|journal=ACM Trans. Math. Software|year=1996|volume=22|number=3|pages=288–301|doi=10.1145/232826.232846|s2cid=37814348 |doi-access=free}} [http://www.netlib.org/toms/757 Fortran 77 code]&lt;br /&gt;
* [http://www.csit.fsu.edu/~burkardt/f_src/toms757/toms757.html Fortran 90 version]&lt;br /&gt;
* {{cite journal|first1=Leonard C.|last1=Maximon|title=The dilogarithm function for complex argument|journal=Proc. R. Soc. A|year=2003|volume=459|number=2039| pages=2807–2819| doi=10.1098/rspa.2003.1156|bibcode=2003RSPSA.459.2807M |s2cid=122271244 }}&lt;br /&gt;
* {{cite journal|first1=I. I.|last1=Guseinov| first2=B. A. |last2=Mamedov|title=Calculation of Integer and noninteger n-Dimensional Debye Functions using Binomial Coefficients and Incomplete Gamma Functions|year=2007|journal=Int. J. Thermophys.|volume=28|issue=4 |pages=1420–1426|doi=10.1007/s10765-007-0256-1|bibcode=2007IJT....28.1420G |s2cid=120284032 }}&lt;br /&gt;
* [https://www.gnu.org/software/gsl/doc/html/specfunc.html#debye-functions C version] of the [[GNU Scientific Library]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Special functions]]&lt;br /&gt;
[[Category:Peter Debye]]&lt;/div&gt;</summary>
		<author><name>imported&gt;Hellacioussatyr</name></author>
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