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Stretched exponential function
Mathematical function common in physics
Mathematical function common in physics
The stretched exponential function f_\beta (t) = e^{ -t^\beta } 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 , the usual exponential function is recovered. With a stretching exponent β between 0 and 1, the graph of log f versus t is characteristically stretched, hence the name of the function. The compressed exponential function (with ) has less practical importance, with the notable exceptions of , which gives the normal distribution, and of compressed exponential relaxation in the dynamics of amorphous solids.
In mathematics, the stretched exponential is also known as the complementary cumulative Weibull distribution. The stretched exponential is also the characteristic function, basically the Fourier transform, of the Lévy symmetric alpha-stable distribution.
In physics, the stretched exponential function is often used as a phenomenological description of relaxation in disordered systems. It was first introduced by Rudolf Kohlrausch in 1854 to describe the discharge of a capacitor;{{cite journal |name-list-style=amp | year = 1970
In phenomenological applications, it is often not clear whether the stretched exponential function should be used to describe the differential or the integral distribution function—or 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,{{cite journal |name-list-style=amp | journal = Comm. Pure Appl. Math.
Mathematical properties
Moments
Following the usual physical interpretation, we interpret the function argument t as time, and fβ(t) is the differential distribution. The area under the curve can thus be interpreted as a mean relaxation time. One finds \langle\tau\rangle \equiv \int_0^\infty dt, e^{-(t/\tau_K)^\beta} = {\tau_K \over \beta } \Gamma {\left( \frac 1 \beta \right)} where Γ is the gamma function. For exponential decay, is recovered.
The higher moments of the stretched exponential function are \langle\tau^n\rangle \equiv \int_0^\infty dt, t^{n-1}, e^{-(t/\tau_K)^\beta} = {{\tau_K}^n \over \beta }\Gamma {\left(\frac n \beta \right)}.
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 e^{-t^\beta} = \int_0^\infty du,\rho(u), e^{-t/u}.
Alternatively, a distribution G = u \rho (u) is used.
ρ can be computed from the series expansion:{{cite journal | name-list-style=amp | year = 1980 For a more recent and general discussion, see {{cite journal \rho (u ) = -{ 1 \over \pi u} \sum_{k = 0}^\infty {(-1)^k \over k!} \sin (\pi \beta k)\Gamma (\beta k + 1) u^{\beta k}
For rational values of β, ρ(u) can be calculated in terms of elementary functions. But the expression is in general too complex to be useful except for the case where G(u) = u \rho(u) = { 1 \over 2\sqrt{\pi}} \sqrt{u} e^{-u/4}
Figure 2 shows the same results plotted in both a linear and a log representation. The curves converge to a Dirac delta function peaked at as β approaches 1, corresponding to the simple exponential function.
| **Figure 2**. Linear and log-log plots of the stretched exponential distribution function G vs t/\tau |
|---|
The moments of the original function can be expressed as \langle\tau^n\rangle = \Gamma(n) \int_0^\infty d\tau, t^n , \rho(\tau).
The first logarithmic moment of the distribution of simple-exponential relaxation times is \langle\ln\tau\rangle = \left( 1 - {1 \over \beta} \right) {\rm Eu} + \ln \tau_K where Eu is the Euler constant.{{cite journal
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. The series here as well as the one for the distribution function are special cases of the Fox–Wright function.{{cite journal | article-number = 061510 | doi-access = free
History and further applications
As said in the introduction, the stretched exponential was introduced by the German 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,{{cite journal | display-authors=etal | doi-access = free}} and the production from unconventional gas wells.
In probability
If the integrated distribution is a stretched exponential, the normalized probability density function is given by p(\tau \mid \lambda, \beta)~d\tau = \frac{\lambda}{\Gamma(1 + \beta^{-1})} ~ e^{-(\tau \lambda)^\beta} ~ d\tau
Note that confusingly some authors have been known to use the name "stretched exponential" to refer to the Weibull distribution.{{cite book
Modified functions
A modified stretched exponential function f_\beta (t) = e^{ -t^{\beta(t)} } with a slowly t-dependent exponent β has been used for biological survival curves.{{cite journal |name-list-style=amp | year = 2009 | article-number = 19554
Wireless communications
In wireless communications, a scaled version of the stretched exponential function has been shown to appear in the Laplace Transform for the interference power I when the transmitters' locations are modeled as a 2D Poisson Point Process with no exclusion region around the receiver.{{cite book
The Laplace transform can be written for arbitrary fading distribution as follows: L_I(s) = \exp\left(-\pi \lambda \mathbb{E}{\left[g^\frac{2}{\eta} \right]} \Gamma{\left(1 - \frac{2}{\eta} \right)} s^\frac{2}{\eta}\right) = \exp\left(- t s^\beta \right) where g is the power of the fading, \eta is the path loss exponent, \lambda is the density of the 2D Poisson Point Process, \Gamma(\cdot) is the Gamma function, and \mathbb{E}[x] is the expectation of the variable x.
The same reference also shows how to obtain the inverse Laplace Transform for the stretched exponential \exp\left(-s^\beta \right) for higher order integer \beta = \beta_q \beta_b from lower order integers \beta_a and \beta_b.
Internet streaming
The stretched exponential has been used to characterize Internet media accessing patterns, such as YouTube and other stable streaming media sites. The commonly agreed power-law accessing patterns of Web workloads mainly reflect text-based content Web workloads, such as daily updated news sites.
References
References
- (2021-06-14). "Slow stretched-exponential and fast compressed-exponential relaxation from local event dynamics". Journal of Physics: Condensed Matter.
- Holm, Sverre. (2020). "Time domain characterization of the Cole-Cole dielectric model". Journal of Electrical Bioimpedance.
- (2015). "Table of Integrals, Series, and Products". [[Academic Press, Inc.]].
- Dishon et al. 1985.
- (1 July 2002). "Friction on Small Objects and the Breakdown of Hydrodynamics in Solution: Rotation of Anthracene in Poly(isobutylene) from the Small-Molecule to Polymer Limits". The Journal of Physical Chemistry B.
- (2010-01-01). "A Better Way To Forecast Production From Unconventional Gas Wells". Society of Petroleum Engineers.
- Lei Guo, Enhua Tan, Songqing Chen, Zhen Xiao, and Xiaodong Zhang. (2008). ""The Stretched Exponential Distribution of Internet Media Access Patterns"".
- (2000). "Power-Law Distribution of the World Wide Web". Science.
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