Kaniadakis Gaussian distribution

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Short description: Continuous probability distribution
κ-Gaussian distribution
Probability density function
Cumulative distribution function
Parameters 0<κ<1 shape (real)
β>0 rate (real)
Support x
PDF Zκexpκ(βx2);Zκ=2βκπ(1+12κ)Γ(12κ+14)Γ(12κ14)
CDF 12+12erfκ(βx) 
Mean 0
Median 0
Mode 0
Variance σκ2=1β2+κ2κ4κ49κ2[Γ(12κ+14)Γ(12κ14)]2
Skewness 0
Kurtosis 3[πZκ2β2/3σκ4(2κ)5/21+52κΓ(12κ54)Γ(12κ+54)1]

The Kaniadakis Gaussian distribution (also known as κ-Gaussian distribution) is a probability distribution which arises as a generalization of the Gaussian distribution from the maximization of the Kaniadakis entropy under appropriated constraints. It is one example of a Kaniadakis κ-distribution. The κ-Gaussian distribution has been applied successfully for describing several complex systems in economy,[1] geophysics,[2] astrophysics, among many others.

The κ-Gaussian distribution is a particular case of the κ-Generalized Gamma distribution.[3]

Definitions

Probability density function

The general form of the centered Kaniadakis κ-Gaussian probability density function is:[3]

fκ(x)=Zκexpκ(βx2)

where |κ|<1 is the entropic index associated with the Kaniadakis entropy, β>0 is the scale parameter, and

Zκ=2βκπ(1+12κ)Γ(12κ+14)Γ(12κ14)

is the normalization constant.

The standard Normal distribution is recovered in the limit κ0.

Cumulative distribution function

The cumulative distribution function of κ-Gaussian distribution is given by

Fκ(x)=12+12erfκ(βx)

where

erfκ(x)=(2+κ)2κπΓ(12κ+14)Γ(12κ14)0xexpκ(t2)dt

is the Kaniadakis κ-Error function, which is a generalization of the ordinary Error function

erf(x)

as

κ0

.

Properties

Moments, mean and variance

The centered κ-Gaussian distribution has a moment of odd order equal to zero, including the mean.

The variance is finite for κ<2/3 and is given by:

Var[X]=σκ2=1β2+κ2κ4κ49κ2[Γ(12κ+14)Γ(12κ14)]2

Kurtosis

The kurtosis of the centered κ-Gaussian distribution may be computed thought:

Kurt[X]=E[X4σκ4]

which can be written as

Kurt[X]=2Zκσκ40x4expκ(βx2)dx

Thus, the kurtosis of the centered κ-Gaussian distribution is given by:

Kurt[X]=3πZκ2β2/3σκ4|2κ|5/21+52|κ|Γ(1|2κ|54)Γ(1|2κ|+54)

or

Kurt[X]=3β11/62κ2|2κ|5/21+52|κ|(1+12κ)(2κ2+κ)2(49κ24κ)2[Γ(12κ14)Γ(12κ+14)]3Γ(1|2κ|54)Γ(1|2κ|+54)

κ-Error function

Template:Infobox mathematical function

The Kaniadakis κ-Error function (or κ-Error function) is a one-parameter generalization of the ordinary error function defined as:[3]

erfκ(x)=(2+κ)2κπΓ(12κ+14)Γ(12κ14)0xexpκ(t2)dt

Although the error function cannot be expressed in terms of elementary functions, numerical approximations are commonly employed.

For a random variable X distributed according to a κ-Gaussian distribution with mean 0 and standard deviation β, κ-Error function means the probability that X falls in the interval [x,x].

Applications

The κ-Gaussian distribution has been applied in several areas, such as:

  • In economy, the κ-Gaussian distribution has been applied in the analysis of financial models, accurately representing the dynamics of the processes of extreme changes in stock prices.[4]
  • In inverse problems, Error laws in extreme statistics are robustly represented by κ-Gaussian distributions.[2][5][6]
  • In astrophysics, stellar-residual-radial-velocity data have a Gaussian-type statistical distribution, in which the K index presents a strong relationship with the stellar-cluster ages.[7][8]
  • In nuclear physics, the study of Doppler broadening function in nuclear reactors is well described by a κ-Gaussian distribution for analyzing the neutron-nuclei interaction.[9][10]
  • In cosmology, for interpreting the dynamical evolution of the Friedmann–Robertson–Walker Universe.
  • In plasmas physics, for analyzing the electron distribution in electron-acoustic double-layers[11] and the dispersion of Langmuir waves.[12]

See also

References

  1. Moretto, Enrico; Pasquali, Sara; Trivellato, Barbara (2017). "A non-Gaussian option pricing model based on Kaniadakis exponential deformation" (in en). The European Physical Journal B 90 (10): 179. doi:10.1140/epjb/e2017-80112-x. ISSN 1434-6028. Bibcode2017EPJB...90..179M. http://link.springer.com/10.1140/epjb/e2017-80112-x. 
  2. 2.0 2.1 da Silva, Sérgio Luiz E. F.; Carvalho, Pedro Tiago C.; de Araújo, João M.; Corso, Gilberto (2020-05-27). "Full-waveform inversion based on Kaniadakis statistics" (in en). Physical Review E 101 (5). doi:10.1103/PhysRevE.101.053311. ISSN 2470-0045. PMID 32575242. Bibcode2020PhRvE.101e3311D. https://link.aps.org/doi/10.1103/PhysRevE.101.053311. 
  3. 3.0 3.1 3.2 Kaniadakis, G. (2021-01-01). "New power-law tailed distributions emerging in κ-statistics (a)". Europhysics Letters 133 (1). doi:10.1209/0295-5075/133/10002. ISSN 0295-5075. Bibcode2021EL....13310002K. https://iopscience.iop.org/article/10.1209/0295-5075/133/10002. 
  4. Moretto, Enrico; Pasquali, Sara; Trivellato, Barbara (2017). "A non-Gaussian option pricing model based on Kaniadakis exponential deformation" (in en). The European Physical Journal B 90 (10): 179. doi:10.1140/epjb/e2017-80112-x. ISSN 1434-6028. Bibcode2017EPJB...90..179M. http://link.springer.com/10.1140/epjb/e2017-80112-x. 
  5. Wada, Tatsuaki; Suyari, Hiroki (2006). "κ-generalization of Gauss' law of error" (in en). Physics Letters A 348 (3–6): 89–93. doi:10.1016/j.physleta.2005.08.086. Bibcode2006PhLA..348...89W. https://linkinghub.elsevier.com/retrieve/pii/S0375960105013630. 
  6. da Silva, Sérgio Luiz E.F.; Silva, R.; dos Santos Lima, Gustavo Z.; de Araújo, João M.; Corso, Gilberto (2022). "An outlier-resistant κ -generalized approach for robust physical parameter estimation" (in en). Physica A: Statistical Mechanics and Its Applications 600. doi:10.1016/j.physa.2022.127554. Bibcode2022PhyA..60027554D. https://linkinghub.elsevier.com/retrieve/pii/S0378437122003855. 
  7. Carvalho, J. C.; Silva, R.; do Nascimento jr., J. D.; Soares, B. B.; De Medeiros, J. R. (2010-09-01). "Observational measurement of open stellar clusters: A test of Kaniadakis and Tsallis statistics". EPL (Europhysics Letters) 91 (6). doi:10.1209/0295-5075/91/69002. ISSN 0295-5075. Bibcode2010EL.....9169002C. https://iopscience.iop.org/article/10.1209/0295-5075/91/69002. 
  8. Carvalho, J. C.; Silva, R.; do Nascimento jr., J. D.; De Medeiros, J. R. (2008). "Power law statistics and stellar rotational velocities in the Pleiades". EPL (Europhysics Letters) 84 (5). doi:10.1209/0295-5075/84/59001. ISSN 0295-5075. Bibcode2008EL.....8459001C. https://iopscience.iop.org/article/10.1209/0295-5075/84/59001. 
  9. Guedes, Guilherme; Gonçalves, Alessandro C.; Palma, Daniel A.P. (2017). "The Doppler Broadening Function using the Kaniadakis distribution" (in en). Annals of Nuclear Energy 110: 453–458. doi:10.1016/j.anucene.2017.06.057. https://linkinghub.elsevier.com/retrieve/pii/S030645491730155X. 
  10. de Abreu, Willian V.; Gonçalves, Alessandro C.; Martinez, Aquilino S. (2019). "Analytical solution for the Doppler broadening function using the Kaniadakis distribution" (in en). Annals of Nuclear Energy 126: 262–268. doi:10.1016/j.anucene.2018.11.023. https://linkinghub.elsevier.com/retrieve/pii/S0306454918306224. 
  11. Gougam, Leila Ait; Tribeche, Mouloud (2016). "Electron-acoustic waves in a plasma with a κ -deformed Kaniadakis electron distribution" (in en). Physics of Plasmas 23 (1): 014501. doi:10.1063/1.4939477. ISSN 1070-664X. Bibcode2016PhPl...23a4501G. http://aip.scitation.org/doi/10.1063/1.4939477. 
  12. Chen, H.; Zhang, S. X.; Liu, S. Q. (2017). "The longitudinal plasmas modes of κ -deformed Kaniadakis distributed plasmas" (in en). Physics of Plasmas 24 (2): 022125. doi:10.1063/1.4976992. ISSN 1070-664X. Bibcode2017PhPl...24b2125C. http://aip.scitation.org/doi/10.1063/1.4976992.