Clausen function: Difference between revisions

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In [[mathematics]], the family of '''Debye functions''' is defined by
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:<math>D_n(x) = \frac{n}{x^n} \int_0^x \frac{t^n}{e^t - 1}\,dt.</math>
 
The functions are named in honor of [[Peter Debye]], who came across this function (with ''n'' = 3) in 1912 when he analytically computed the [[heat capacity]] of what is now called the [[Debye model]].
 
== Mathematical properties ==
 
=== Relation to other functions ===
 
The Debye functions are closely related to the [[Polylogarithm]].
 
=== Limiting values ===
 
For <math>x \rightarrow 0</math> :
:<math>D_n(0)=1.</math>
 
For <math>x >> 1</math> : <math>D_n</math> is given by the [[Gamma function]] and the [[Riemann zeta function]]:
:<math>D_n(x)\propto\int_0^\infty{\rm d}t\frac{t^{n}}{\exp(t)-1} = \Gamma(n + 1) \zeta(n + 1).   \quad [\Re \, n > 0]</math> <ref>Gradshteyn, I. S., & Ryzhik, I. M. (1980). Table of integrals. Series, and Products (Academic, New York, 1980), (3.411).</ref>
 
== Applications in solid-state physics ==
 
=== The Debye model ===
 
The [[Debye model]] has a [[density of vibrational states]]
:<math>g_{\rm D}(\omega)=\frac{9\omega^2}{\omega_{\rm D}^3}</math> for <math>0\le\omega\le\omega_{\rm D}</math>
with the ''Debye frequency'' ''&omega;''<sub>D</sub>.
 
=== Internal energy and heat capacity ===
 
Inserting ''g'' into the internal energy
:<math>U=\int_0^\infty{\rm d}\omega\,g(\omega)\,\hbar\omega\,n(\omega)</math>
with the [[Bose-Einstein distribution]]
:<math>n(\omega)=\frac{1}{\exp(\hbar\omega/k_{\rm B}T)-1}</math>.
one obtains
:<math>U=3 k_{\rm B}T\, D_3(\hbar\omega_{\rm D}/k_{\rm B}T)</math>.
The heat capacity is the derivative thereof.
 
=== Mean squared displacement ===
 
The intensity of [[X-ray diffraction]] or [[neutron diffraction]] at wavenumber ''q'' is given by
the [[Debye-Waller factor]] or the [[Lamb-Mössbauer factor]].
For isotropic systems it takes the form
:<math>\exp(-2W(q))=\exp(-q^2\langle u_x^2\rangle</math>).
In this expression, the [[mean squared displacement]] refers to just once Cartesian component
''u<sub>x</sub>'' of the vector '''u''' that describes the displacement of atoms from their equilibrium positions.
Assuming harmonicity and developing into normal modes,<ref>Ashcroft & Mermin 1976, App. L,</ref>
one obtains
:<math>2W(q)=\frac{\hbar^2 q^2}{6M k_{\rm B}T}\int_0^\infty{\rm d}\omega\frac{k_{\rm B}T}{\hbar\omega}g(\omega)\coth\frac{\hbar\omega}{2k_{\rm B}T}=\frac{\hbar^2 q^2}{6M k_{\rm B}T}\int_0^\infty{\rm d}\omega\frac{k_{\rm B}T}{\hbar\omega}g(\omega)\left[\frac{2}{\exp(\hbar\omega/k_{\rm B}T)-1}+1\right].</math>
Inserting the density of states from the Debye model, one obtains
:<math>2W(q)=\frac{3}{2}\frac{\hbar^2 q^2}{M\hbar\omega_{\rm D}}\left[2\left(\frac{k_{\rm B}T}{\hbar\omega_{\rm D}}\right)D_1\left(\frac{\hbar\omega_{\rm D}}{k_{\rm B}T}\right)+\frac{1}{2}\right]</math>.
 
==References==
{{Reflist}}
 
==Further reading==
 
* {{AS ref|27|998}}
* [http://mathworld.wolfram.com/DebyeFunctions.html "Debye function" entry in MathWorld], defines the Debye functions without prefactor ''n''/''x<sup>n</sup>''
 
== Implementations ==
* [http://www.netlib.org/toms/757 Fortran 77 code] by [[Allan MacLeod]] from [[Transactions on Mathematical Software]]
* [http://www.csit.fsu.edu/~burkardt/f_src/toms757/toms757.html Fortran 90 version]
* [http://www.gnu.org/software/gsl/manual/html_node/Debye-Functions.html C version] of the [[GNU Scientific Library]]
 
[[Category:Special functions]]

Revision as of 18:41, 13 February 2014

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