Debye Function

In mathematics, the family of Debye functions is defined by

:$D_n(x) = \frac \int_0^x \frac\,dt.$

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.

Series expansion

They have the series expansion

:$D_n(x) = 1 - \frac x + n \sum_^\infty \frac x^, \quad , x, < 2\pi,\ n \ge 1,$
where $B_n$ is the n-th Bernoulli number.

Limiting values

:$\lim_ D_n(x) = 1.$

If $\Gamma$ is the gamma function and $\zeta$ is the Riemann zeta function, then, for $x \gg 0$,
:$D_n(x) = \frac \int_0^x \frac \sim \frac\Gamma(n + 1) \zeta(n + 1), \qquad \operatorname n > 0,$

Derivative

The derivative obeys the relation
:$xD^_n(x) = n(B(x)-D_n(x)),$
where $B(x)=x/(e^x-1)$ is the Bernoulli function.

Applications in solid-state physics

The Debye model

The Debye model has a density of vibrational states
:$g_(\omega)=\frac$ for $0\le\omega\le\omega_$
with the ''Debye frequency'' ''ω''_D.

Internal energy and heat capacity

Inserting ''g'' into the internal energy
:$U=\int_0^\infty d\omega\,g(\omega)\,\hbar\omega\,n(\omega)$
with the Bose–Einstein distribution
:$n(\omega)=\frac$.
one obtains
:$U=3 k_T\, D_3(\hbar\omega_/k_T)$.
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
:$\exp(-2W(q))=\exp(-q^2\langle u_x^2\rangle$).
In this expression, the mean squared displacement refers to just once Cartesian component
''u_x'' of the vector u that describes the displacement of atoms from their equilibrium positions.
Assuming harmonicity and developing into normal modes,Ashcroft & Mermin 1976, App. L,
one obtains
:2W(q)=\frac\int_0^\infty d\omega\fracg(\omega)\coth\frac=\frac\int_0^\infty d\omega\fracg(\omega)\left frac+1\right
Inserting the density of states from the Debye model, one obtains
:2W(q)=\frac\frac\left \left(\frac\right)D_1\left(\frac\right)+\frac\right/math>.
From the above power series expansion of $D_1$ follows that the mean square displacement at high temperatures is linear in temperature
:$2W(q)=\frac$.
The absence of $\hbar$ indicates that this is a classical result. Because $D_1(x)$ goes to zero for $x\to\infty$ it follows that for $T=0$
:$2W(q)=\frac\frac$ ( zero-point motion).

References

Further reading

*

"Debye function" entry in MathWorld
defines the Debye functions without prefactor ''n''/''xⁿ''

Implementations

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Fortran 77 code


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* {{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


of the GNU Scientific Library

Special functions
Peter Debye