Abstract

A new family of distributions called the Kumaraswamy Rayleigh family is defied and studied. Some of its relevant statistical properties are derived. Many new bivariate type G families using the of Farlie-Gumbel-Morgenstern, modified Farlie-Gumbel-Morgenstern copula, Clayton copula and Renyi’s entropy copula are derived. The method of the maximum likelihood estimation is used. Some special models based on log-logistic, exponential, Weibull, Rayleigh, Pareto type II and Burr type X, Lindley distributions are presented and studied. Three dimensional skewness and kurtosis plots are presented. A graphical assessment is performed. Two real life applications to illustrate the flexibility, potentiality and importance of the new family is proposed.

Highlights

  • Introduction and motivationRecently, there has been an exceptional eagerness for growing more flexible families of distributions by extending the classical cumulative distribution functions (CDFs)

  • In modeling real-life data, the new family proved its superiority against the special generalized mixture-G family, odd log-logistic-G family, Burr-Hatke-G family transmuted Topp-Leone-G family, gamma-G family, Kumaraswamy-G family, beta-G family and Exponentiated-G family

  • We introduce two formulae for the moment generating function

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Summary

Introduction and motivation

There has been an exceptional eagerness for growing more flexible families of distributions by extending the classical cumulative distribution functions (CDFs). 2. In modeling real-life data, the new family proved its superiority against the special generalized mixture-G family, odd log-logistic-G family, Burr-Hatke-G family transmuted Topp-Leone-G family, gamma-G family, Kumaraswamy-G family, beta-G family and Exponentiated-G family.

Useful expansions
Quantile function
Moments
Moment generating function
Biv-KR type via FGM copula
Biv-KR type via Clayton copula
Maximum likelihood estimation
Special models
Simulations
Applications and comparing models
12 Proportional reversed hazard rate PTII
Conclusions

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