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Debye function

From Wikipedia, the free encyclopedia

In mathematics, the family of Debye functions is defined by Dn(x)=nxn∫0xtnet−1dt.

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

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Relation to other functions

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The Debye functions are closely related to the polylogarithm.

Series expansion

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They have the series expansion[1] Dn(x)=1−n2(n+1)x+n∑k=1∞B2k(2k+n)(2k)!x2k,|x|<2π, n≥1, where Bn is the n-th Bernoulli number.

Limiting values

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limx→0Dn(x)=1. If Γ is the gamma function and ζ is the Riemann zeta function, then, for x≫0,[2] Dn(x)=nxn∫0xtndtet−1∼nxnΓ(n+1)ζ(n+1),Re⁡n>0,

Derivative

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The derivative obeys the relation xDn′(x)=n(B(x)−Dn(x)), where B(x)=x/(ex−1) is the Bernoulli function.

Applications in solid-state physics

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The Debye model

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The Debye model has a density of vibrational states gD(ω)=9ω2ωD3,0≤ω≤ωD with the Debye frequency ωD.

Internal energy and heat capacity

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Inserting g into the internal energy U=∫0∞dωg(ω)ℏωn(ω) with the Bose–Einstein distribution n(ω)=1exp⁡(ℏω/kBT)−1. one obtains U=3kBTD3(ℏωD/kBT). The heat capacity is the derivative thereof.

Mean squared displacement

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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 exp⁡(−2W(q))=exp⁡(−q2⟨ux2⟩). In this expression, the mean squared displacement refers to just once Cartesian component ux of the vector u that describes the displacement of atoms from their equilibrium positions. Assuming harmonicity and developing into normal modes,[3] one obtains 2W(q)=ℏ2q26MkBT∫0∞dωkBTℏωg(ω)coth⁡ℏω2kBT=ℏ2q26MkBT∫0∞dωkBTℏωg(ω)[2exp⁡(ℏω/kBT)−1+1]. Inserting the density of states from the Debye model, one obtains 2W(q)=32ℏ2q2MℏωD[2(kBTℏωD)D1(ℏωDkBT)+12]. From the above power series expansion of D1 follows that the mean square displacement at high temperatures is linear in temperature 2W(q)=3kBTq2MωD2. The absence of ℏ indicates that this is a classical result. Because D1(x) goes to zero for x→∞ it follows that for T=0 2W(q)=34ℏ2q2MℏωD (zero-point motion).

References

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  1. ↑ Abramowitz, Milton; Stegun, Irene Ann, eds. (1983) [June 1964]. "Chapter 27". Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. Applied Mathematics Series. Vol. 55 (Ninth reprint with additional corrections of tenth original printing with corrections (December 1972); first ed.). Washington D.C.; New York: United States Department of Commerce, National Bureau of Standards; Dover Publications. p. 998. ISBN 978-0-486-61272-0. LCCN 64-60036. MR 0167642. LCCN 65-12253.
  2. ↑ Gradshteyn, Izrail Solomonovich; Ryzhik, Iosif Moiseevich; Geronimus, Yuri Veniaminovich; Tseytlin, Michail Yulyevich; Jeffrey, Alan (2015) [October 2014]. "3.411.". In Zwillinger, Daniel; Moll, Victor Hugo (eds.). Table of Integrals, Series, and Products. Translated by Scripta Technica, Inc. (8 ed.). Academic Press, Inc. pp. 355ff. ISBN 978-0-12-384933-5. LCCN 2014010276.
  3. ↑ Ashcroft & Mermin 1976, App. L,

Further reading

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Implementations

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