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On maximum entropy principle, superstatistics, power-law distribution and Renyi parameter

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  • Bashkirov, A.G

Abstract

The equilibrium distributions of probabilities are derived on the basis of the maximum entropy principle (MEP) for the Renyi and Tsallis entropies. New S-forms for the Renyi and Tsallis distribution functions are found which are normalised with corresponding entropies in contrast to the usual Z-forms normalised with partition functions Z. The superstatistics based on the Gibbs distribution of energy fluctuations gives rise to a distribution function of the same structure that the Renyi and Tsallis distributions have. The long-range “tail” of the Renyi distribution is the power-law distribution with the exponent −s expressed in terms of the free Renyi parameter q as s=1/(1−q). The condition s>0 gives rise to the requirement q<1. The parameter q can be uniquely determined with the use of a further extension of MEP as the condition for maximum of the difference between the Renyi and Boltzmann entropies for the same power-law distribution dependent on q. It is found that the maximum is realized for q within the range from 0.25 to 0.5 and the exponent s varies from 1.3 to 2 in dependence on parameters of stochastic systems.

Suggested Citation

  • Bashkirov, A.G, 2004. "On maximum entropy principle, superstatistics, power-law distribution and Renyi parameter," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 340(1), pages 153-162.
  • Handle: RePEc:eee:phsmap:v:340:y:2004:i:1:p:153-162
    DOI: 10.1016/j.physa.2004.04.002
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    Cited by:

    1. Lubashevsky, Ihor & Friedrich, Rudolf & Heuer, Andreas & Ushakov, Andrey, 2009. "Generalized superstatistics of nonequilibrium Markovian systems," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 388(21), pages 4535-4550.
    2. Koltcov, Sergei, 2018. "Application of Rényi and Tsallis entropies to topic modeling optimization," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 512(C), pages 1192-1204.

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