Kaniadakis statistics (also known as κ-statistics) is a generalization of Boltzmann–Gibbs statistical mechanics, based on a relativistic generalization of the classical Boltzmann–Gibbs–Shannon entropy (commonly referred to as Kaniadakis entropy or κ-entropy). Introduced by the Greek Italian physicist Giorgio Kaniadakis in 2001, κ-statistical mechanics preserve the main features of ordinary statistical mechanics and have attracted the interest of many researchers in recent years. The κ-distribution is currently considered one of the most viable candidates for explaining complex physical, natural or artificial systems involving power-law tailed statistical distributions. Kaniadakis statistics have been adopted successfully in the description of a variety of systems in the fields of cosmology, astrophysics, condensed matter, quantum physics, seismology, genomics, economics, epidemiology, and many others.
Mathematical formalism The mathematical formalism of κ-statistics is generated by κ-deformed functions, especially the κ-exponential function.
κ-exponential function
The Kaniadakis exponential (or κ-exponential) function is a one-parameter generalization of an exponential function, given by:
exp κ ( x ) = { ( 1 + κ 2 x 2 + κ x ) 1 κ if 0 < κ < 1. exp ( x ) if κ = 0 , {\displaystyle \exp _{\kappa }(x)={\begin{cases}{\Big (}{\sqrt {1+\kappa ^{2}x^{2}}}+\kappa x{\Big )}^{\frac {1}{\kappa }}&{\text{if }}0<\kappa <1.\\[6pt]\exp(x)&{\text{if }}\kappa =0,\\[8pt]\end{cases}}}
with exp − κ ( x ) = exp κ ( x ) {\displaystyle \exp _{-\kappa }(x)=\exp _{\kappa }(x)} . The κ-exponential for 0 < κ < 1 {\displaystyle 0<\kappa <1} can also be written in the form:
exp κ ( x ) = exp ( 1 κ arsinh ( κ x ) ) . {\displaystyle \exp _{\kappa }(x)=\exp {\Bigg (}{\frac {1}{\kappa }}{\text{arsinh}}(\kappa x){\Bigg )}.}
The first five terms of the Taylor expansion of exp κ ( x ) {\displaystyle \exp _{\kappa }(x)} are given by:
exp κ ( x ) = 1 + x + x 2 2 + ( 1 − κ 2 ) x 3 3 ! + ( 1 − 4 κ 2 ) x 4 4 ! + ⋯ {\displaystyle \exp _{\kappa }(x)=1+x+{\frac {x^{2}}{2}}+(1-\kappa ^{2}){\frac {x^{3}}{3!}}+(1-4\kappa ^{2}){\frac {x^{4}}{4!}}+\cdots }
where the first three are the same as a typical exponential function. Basic properties The κ-exponential function has the following properties of an exponential function:
exp κ ( x ) ∈ C ∞ ( R ) {\displaystyle \exp _{\kappa }(x)\in \mathbb {C} ^{\infty }(\mathbb {R} )}
d d x exp κ ( x ) > 0 {\displaystyle {\frac {d}{dx}}\exp _{\kappa }(x)>0}
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![Kaniadakis statistics: [click on the figure] Plot of the κ-sine and κ-cosine functions for
κ
=
0
{\displaystyle \kappa =0}
(black curve) and
κ
=
0.1
{\displaystyle \kappa =0.1}
(blue curve).](https://upload.wikimedia.org/wikipedia/commons/thumb/2/20/Kappa_trigonometric_sink_cosk.gif/500px-Kappa_trigonometric_sink_cosk.gif?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)

