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[[Image:Pibmasterplot.png|325px|thumb|'''Figure 1'''. Illustration of a stretched exponential fit (with ''β''=0.52) to an empirical [[master curve]]. For comparison, a least squares single and a [[Laplace distribution|double exponential]] fit are also shown. The data are rotational [[anisotropy]] of [[anthracene]] in [[polyisobutylene]] of several [[molecular mass]]es. The plots have been made to overlap by dividing time (''t'') by the respective characteristic time constant.]]
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The '''stretched exponential function'''
:<math>f_\beta (t) = e^{ -t^\beta }</math>
is obtained by inserting a fractional [[power law]] into the [[exponential function]].
In most applications, it is meaningful only for arguments ''t'' between 0 and +∞. With ''β''=1, the usual exponential function is recovered. With a ''stretching exponent'' ''β'' between 0 and 1, the graph of log&nbsp;''f'' versus ''t'' is characteristically ''stretched'', whence the name of the function. The '''compressed exponential function''' (with ''β''>1) has less practical importance, with the notable exception of β=2, which gives the [[normal distribution]].
 
In mathematics, the stretched exponential is also known as the [[Cumulative_distribution_function#Complementary_cumulative_distribution_function_(tail_distribution)|complementary cumulative]] [[Weibull distribution]]. Furthermore, the stretched exponential is the [[characteristic function (probability theory)|characteristic function]] (basically the [[Fourier transform]]) of the [[stable distribution|Lévy symmetric alpha-stable distribution]].
 
In physics, the stretched exponential function is often used as a phenomenological description of [[Relaxation (physics)|relaxation]] in disordered systems. It was first introduced by [[Rudolf Kohlrausch]] in 1854 to describe the discharge of a capacitor;<ref>{{cite journal
| author = Kohlrausch, R.
| year = 1854
| title = Theorie des elektrischen Rückstandes in der Leidner Flasche
| journal = [[Annalen der Physik und Chemie|Annalen der Physik und Chemie (Poggendorff)]]
| volume = 91
| pages = 56–82, 179–213
| url = http://gallica.bnf.fr/ark:/12148/bpt6k15176w.pagination}}.</ref>
therefore it is also called the '''Kohlrausch function'''. In 1970, G. Williams and D.C. Watts used the [[Fourier transform]] of the stretched exponential to describe [[dielectric spectroscopy|dielectric spectra]] of polymers;<ref>{{cite journal
| author = Williams, G. and Watts, D. C.
| year = 1970
| title = Non-Symmetrical Dielectric Relaxation Behavior Arising from a Simple Empirical Decay Function
| journal = Transactions of the [[Faraday Society]]
| volume = 66
| pages = 80–85
| doi = 10.1039/tf9706600080
}}.</ref>
in this context, the stretched exponential or its Fourier transform are also called the '''Kohlrausch-Williams-Watts (KWW) function'''.
 
In phenomenological applications, it is often not clear whether the stretched exponential function should apply to the differential or to the integral distribution function -- or to neither.
In each case one gets the same asymptotic decay, but a different power law prefactor, which makes  fits more ambiguous than for simple exponentials. In a few cases <ref>{{cite journal
| author = Donsker, M. D. and Varadhan, S. R. S.
| journal = Comm. Pure Appl. Math.
| volume = 28
| pages = 1–47
| year = 1975
| title = Asymptotic evaluation of certain Markov process expectations for large time
}}</ref> <ref>{{cite journal
| author = Takano, H. and Nakanishi, H. and Miyashita, S.
| journal = Phys. Rev. B
| volume = 37
| pages = 3716 - 3719
| year = 1988
| title = Stretched exponential decay of the spin-correlation function in the kinetic Ising model below the critical temperature
|bibcode = 1988PhRvB..37.3716T |doi = 10.1103/PhysRevB.37.3716 }}</ref>
it can be shown that the asymptotic decay is a stretched exponential, but the prefactor is usually an unrelated power.
 
== Mathematical properties ==
 
=== Moments ===
 
Following the usual physical interpretation, we interpret the function argument ''t'' as a time, and ''f''<sub>β</sub>(''t'') is the differential distribution. The area under the curve
is therefore interpreted as a ''mean relaxation time''. One finds
:<math>\langle\tau\rangle \equiv \int_0^\infty dt\, e^{ - \left( {t /\tau_K } \right)^\beta  } = {\tau_K  \over \beta }\Gamma ({1 \over \beta })</math>
where Γ is the [[gamma function]]. For exponential decay, 〈τ〉 = τ<sub>''K''</sub> is recovered.
 
The higher [[moment (mathematics)|moments]] of the stretched exponential function are:<ref>I.S. Gradshteyn (И.С. Градштейн), I.M. Ryzhik (И.М. Рыжик); Alan Jeffrey, Daniel Zwillinger, editors. ''Table of Integrals, Series, and Products'', fourth edition. Academic Press, 1980. Integral 3.478.</ref>
: <math>\langle\tau^n\rangle \equiv \int_0^\infty dt\, t^{n-1}\, e^{ - \left( {t /\tau_K } \right)^\beta  } = {{\tau_K }^n  \over \beta }\Gamma ({n \over \beta })</math>.
 
===Distribution function===
 
In physics, attempts have been made to explain stretched exponential behaviour as a linear superposition of simple exponential decays. This requires a nontrivial distribution of relaxation times, ''ρ(u)'', which is implicitly defined by
: <math>e^{ - t^\beta} = \int_0^\infty du\,\rho(u)\, e^{-t/u}</math>.
Alternatively, a distribution
: <math>G=u \rho (u)\,</math>
is used.
 
ρ can be computed from the series expansion:<ref>{{cite journal
| author = Lindsey, C. P. and Patterson, G. D.
| year = 1980
| title = Detailed comparison of the Williams-Watts and Cole-Davidson functions
| journal = [[Journal of Chemical Physics]]
| volume = 73
| pages = 3348–3357
| doi = 10.1063/1.440530|bibcode = 1980JChPh..73.3348L }}.
For a more recent and general discussion, see {{cite journal
| author = Berberan-Santos, M.N., Bodunov, E.N. and Valeur, B.
| year = 2005
| title = Mathematical functions for the analysis of luminescence decays with underlying distributions 1. Kohlrausch decay function (stretched exponential)
| journal = [[Chemical Physics]]
| volume = 315
| pages = 171–182
| doi = 10.1016/j.chemphys.2005.04.006
|bibcode = 2005CP....315..171B }}.</ref> <math>
\rho (u ) =  -{ 1 \over {\pi u }} \sum\limits_{k = 0}^\infty
    {{( - 1)^k } \over {k!}}\sin (\pi \beta k)\Gamma (\beta k + 1) u^{\beta k }
</math>
 
Figure 2 shows the same results plotted in both a [[linear]] and a [[Logarithm|log]] representation. The curves converge to a [[Dirac delta function]] peaked at u=1 as β approaches 1, corresponding to the simple exponential function.
{| class="wikitable" style="margin: 1em auto 1em auto"
|
{|
|-
| [[Image:KWW dist. function linear.png|300px]] || [[Image:KWW dist. funct. log.png|300px]]
|}
|-
|'''Figure 2'''. Linear and log-log plots of the stretched exponential distribution function <math>G</math> vs <math>t/\tau</math>
for values of the stretching parameter ''β'' between 0.1 and 0.9.
|}
 
The moments of the original function can be expressed as
: <math>\langle\tau^n\rangle = \Gamma(n) \int_0^\infty d\tau\, t^{n}\, \rho(\tau)</math>.
 
The first logarithmic moment of the distribution of simple-exponential relaxation times is
: <math>\langle\ln\tau\rangle = \left( 1 - { 1 \over \beta } \right) {\rm Eu} + \ln \tau_K </math>
where Eu is the [[Euler constant]].<ref>{{cite journal
| doi = 10.1063/1.1446035
| author = Zorn, R.
| year = 2002
| title = Logarithmic moments of relaxation time distributions
| journal = [[Journal of Chemical Physics]]
| volume = 116
| pages = 3204–3209
|bibcode = 2002JChPh.116.3204Z }}</ref>
 
== Fourier Transform ==
 
To describe results from spectroscopy or inelastic scattering, the sine or cosine Fourier transform of the stretched exponential is needed. It must be calculated either by numeric integration, or from a series expansion.<ref>Dishon et al. 1985.</ref> The series here as well as the one for the distribution function are special cases of the [[Fox-Wright function]].<ref>{{cite journal
| author = Hilfer, J.
| year = 2002
| title = ''H''-function representations for stretched exponential relaxation and non-Debye susceptibilities in glassy systems
| journal = [[Physical Review]] E
| volume = 65
| pages = 061510
  }}</ref> For practical purposes, the Fourier transform may be approximated by the [[Havriliak-Negami relaxation|Havriliak-Negami function]],<ref>{{cite journal
| author = Alvarez, F., Alegría, A. and Colmenero, J.
| year = 1991
| title = Relationship between the time-domain Kohlrausch-Williams-Watts and frequency-domain Havriliak-Negami relaxation functions
| journal = [[Physical Review]] B
| volume = 44
| pages = 7306–7312
| doi = 10.1103/PhysRevB.44.7306
|bibcode = 1991PhRvB..44.7306A }}</ref>
though nowadays the numeric computation can be done so efficiently<ref>{{cite journal
| author = Wuttke, J.
| year = 2012
| title = Laplace–Fourier Transform of the Stretched Exponential Function: Analytic Error Bounds, Double Exponential Transform, and Open-Source Implementation "libkww"
| journal = [[Algorithms]]
| volume = 5
| pages = 604–628
| doi = 10.3390/a5040604}}</ref> that there is no longer any reason not to use the Kohlrausch-Williams-Watts function in the frequency domain.
 
== History and further applications ==
 
As said in the introduction, the stretched exponential was introduced by the [[Germans|German]] [[physics|physicist]] [[Rudolf Kohlrausch]] in 1854 to describe the discharge of a capacitor ([[Leyden jar]]) that used glass as dielectric medium. The next documented usage is by [[Friedrich Kohlrausch]], son of Rudolf, to describe torsional relaxation. [[A. Werner]] used it in 1907 to describe complex luminescence decays; [[Theodor Förster]] in 1949 as the fluorescence decay law of electronic energy donors.
 
Outside condensed matter physics, the stretched exponential has been used to describe the removal rates of small, stray bodies in the solar system,<ref>{{cite journal
| author = Dobrovolskis, A., Alvarellos, J. and Lissauer, J.
| year = 2007
| title = Lifetimes of small bodies in planetocentric (or heliocentric) orbits
| journal = [[Icarus (journal)|Icarus]]
| volume = 188
| pages = 481–505
| doi = 10.1016/j.icarus.2006.11.024|bibcode = 2007Icar..188..481D }}</ref>
and the diffusion-weighted MRI signal in the brain.<ref>{{cite journal
| author = Bennett, K. ''et al.''
| year = 2003
| title = Characterization of Continuously Distributed Water Diffusion Rates in Cerebral Cortex with a Stretched Exponential Model
| journal = Magn. Reson. Med.
| volume = 50
| pages = 727–734
| doi = 10.1002/mrm.10581}}</ref>
 
=== In probability ===
 
If the integrated distribution is a stretched exponential, the normalized [[Probability distribution|probability density function]] is given by,
 
:<math>p(\tau \mid \lambda, \beta)~d\tau = \frac{\lambda}{\Gamma(1 + \beta^{-1})}~e^{-(\tau \lambda)^\beta}~d\tau</math>
 
Note that confusingly some authors<ref>{{cite book
| author = Sornette, D.
| year = 2004
| title = Critical Phenomena in Natural Science: Chaos, Fractals, Self-organization, and Disorder}}.</ref>
have been known to use the name "stretched exponential" to refer to the [[Weibull distribution]].
 
=== Modified functions ===
 
A modified function
:<math>f_\beta (t) = e^{ -t^{\beta(t)} }</math>
with a slowly ''t''-dependent exponent ''&beta;'' has been used for biological survival curves.<ref>{{cite journal
| author = B. M. Weon and J. H. Je
| year = 2009
| title = Theoretical estimation of maximum human lifespan
| journal = Biogerontology
| volume = 10
| pages = 65–71
| doi = 10.1007/s10522-008-9156-4}}</ref>
 
==References==
<references/>
 
==External links==
* J. Wuttke: [http://apps.jcns.fz-juelich.de/kww libkww] C library to compute the Fourier transform of the stretched exponential function
 
{{DEFAULTSORT:Stretched Exponential Function}}
[[Category:Exponentials]]

Latest revision as of 19:28, 8 November 2014

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