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Unit Weibull distribution

The unit-Weibull distribution (UW) is a continuous probability distribution with domain on . Useful for indices and rates, or bounded variables with a domain. It was originally proposed by Mazucheli et al using a transformation of the Weibull distribution.

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Unit Weibull
Probability density function
Probability density plots of UW distributions
Cumulative distribution function
Cumulative density plots of UW distributions
Parameters α > 0 {\displaystyle \alpha >0\,} (real)
β > 0 {\displaystyle \beta >0\,} (real)
Support x ( 0 , 1 ) {\displaystyle x\in (0,1)\,}
PDF 1 x α β ( log x ) β 1 exp [ α ( log x ) β ] {\displaystyle {\frac {1}{x}}\,\alpha \,\beta \,(-\log x)^{\beta -1}\exp \left[-\alpha \,(-\log x)^{\beta }\right]}
CDF exp [ α ( log x ) β ] {\displaystyle \exp \left[-\alpha \,(-\log x)^{\beta }\right]}
Quantile exp [ ( log p α ) 1 β ] , 0 < p < 1 {\displaystyle \exp \left[-\left({\frac {-\log p}{\alpha }}\right)^{\frac {1}{\beta }}\right],\quad 0<p<1}
Skewness μ 3 3 μ 2 μ + μ 3 σ 3 {\displaystyle {\frac {\mu '_{3}-3\mu '_{2}\mu +\mu ^{3}}{\sigma ^{3}}}}
Excess kurtosis μ 4 4 μ 3 μ + 6 μ 2 μ 2 3 μ 4 σ 4 {\displaystyle {\frac {\mu '_{4}-4\mu '_{3}\mu +6\mu '_{2}\mu ^{2}-3\mu ^{4}}{\sigma ^{4}}}}
MGF n = 0 ( 1 ) n n ! α n / β Γ ( n β + 1 ) {\displaystyle \sum _{n=0}^{\infty }{\frac {(-1)^{n}}{n!\,\alpha ^{n/\beta }}}\,\Gamma \left({\frac {n}{\beta }}+1\right)}

The unit-Weibull distribution (UW) is a continuous probability distribution with domain on ( 0 , 1 ) {\displaystyle (0,1)} . Useful for indices and rates, or bounded variables with a ( 0 , 1 ) {\displaystyle (0,1)} domain. It was originally proposed by Mazucheli et al1 using a transformation of the Weibull distribution.

Definitions

Probability density function

Its probability density function is defined as:

f ( x ; α , β ) = 1 x α β ( log x ) β 1 exp [ α ( log x ) β ] {\displaystyle f(x;\alpha ,\beta )={\frac {1}{x}}\,\alpha \,\beta \,(-\log x)^{\beta -1}\exp \left[-\alpha \,(-\log x)^{\beta }\right]}

Cumulative distribution function

And its cumulative distribution function is:

F ( x ; α , β ) = exp [ α ( log x ) β ] {\displaystyle F(x;\alpha ,\beta )=\exp \left[-\alpha \,(-\log x)^{\beta }\right]}

Quantile function

The quantile function of the UW distribution is given by:

Q ( p ) = exp [ ( log p α ) 1 β ] , 0 < p < 1. {\displaystyle Q(p)=\exp \left[-\left({\frac {-\log p}{\alpha }}\right)^{\frac {1}{\beta }}\right],\quad 0<p<1.}

Having a closed form expression for the quantile function, may make it a more flexible alternative for a quantile regression model against the classical Beta regression model.

Properties

Moments

The r {\displaystyle r} th raw moment of the UW distribution can be obtained through:

μ r = E ( X r ) = E ( e r Y ) = M Y ( r ) = n = 0 ( 1 ) n n ! α n / β Γ ( n β + 1 ) . {\displaystyle \mu '_{r}=\mathbb {E} (X^{r})=\mathbb {E} (e^{-rY})=M_{Y}(-r)=\sum _{n=0}^{\infty }{\frac {(-1)^{n}}{n!\,\alpha ^{n/\beta }}}\,\Gamma \left({\frac {n}{\beta }}+1\right).}

Skewness and kurtosis

The skewness and kurtosis measures can be obtained upon substituting the raw moments from the expressions:

s k e w n e s s = μ 3 3 μ 2 μ + μ 3 σ 3 , k u r t o s i s = μ 4 4 μ 3 μ + 6 μ 2 μ 2 3 μ 4 σ 4 {\displaystyle {\mathit {skewness}}={\frac {\mu '_{3}-3\mu '_{2}\mu +\mu ^{3}}{\sigma ^{3}}},{\mathit {kurtosis}}={\frac {\mu '_{4}-4\mu '_{3}\mu +6\mu '_{2}\mu ^{2}-3\mu ^{4}}{\sigma ^{4}}}}

Hazard rate

The hazard rate function of the UW distribution is given by:

h ( x ; α , β ) = f ( x ; α , β ) 1 F ( x ; α , β ) = α β ( log x ) β 1 exp [ α ( log x ) β ] x ( 1 exp [ α ( log x ) β ] ) , 0 < x < 1. {\displaystyle h(x;\alpha ,\beta )={\frac {f(x;\alpha ,\beta )}{1-F(x;\alpha ,\beta )}}={\frac {\alpha \beta \,(-\log x)^{\beta -1}\exp \left[-\alpha (-\log x)^{\beta }\right]}{x\left(1-\exp \left[-\alpha (-\log x)^{\beta }\right]\right)}},\quad 0<x<1.}

Parameter estimation

Let x = ( x 1 , , x n ) {\displaystyle \mathbf {x} =(x_{1},\ldots ,x_{n})} be a random sample of size n {\displaystyle n} from the UW distribution with probability density function defined before. Then, the log-likelihood function of θ = ( α , β ) {\displaystyle {\boldsymbol {\theta }}=(\alpha ,\beta )} is:

( θ ; x ) = n ( log α + log β ) i = 1 n log x i + ( β 1 ) i = 1 n log ( log x i ) α i = 1 n ( log x i ) β {\displaystyle {\begin{aligned}\ell ({\boldsymbol {\theta }};\mathbf {x} )&=n(\log \alpha +\log \beta )-\sum _{i=1}^{n}\log x_{i}+(\beta -1)\sum _{i=1}^{n}\log(-\log x_{i})-\alpha \sum _{i=1}^{n}(-\log x_{i})^{\beta }\end{aligned}}}

The likelihood estimate θ ^ {\displaystyle {\hat {\boldsymbol {\theta }}}} of θ {\displaystyle {\boldsymbol {\theta }}} is obtained by solving the non-linear equations

α = n α i = 1 n ( log x i ) β = 0 , {\displaystyle {\frac {\partial \ell }{\partial \alpha }}={\frac {n}{\alpha }}-\sum _{i=1}^{n}(-\log x_{i})^{\beta }=0,}

and

β = n β + i = 1 n log ( log x i ) α i = 1 n ( log x i ) β log ( log x i ) = 0. {\displaystyle {\frac {\partial \ell }{\partial \beta }}={\frac {n}{\beta }}+\sum _{i=1}^{n}\log(-\log x_{i})-\alpha \sum _{i=1}^{n}(-\log x_{i})^{\beta }\log(-\log x_{i})=0.}

The expected Fisher information matrix of θ = ( α , β ) {\displaystyle {\boldsymbol {\theta }}=(\alpha ,\beta )} based on a single observation is given by

I ( θ ) = [ I i j ] = ( 1 α 1 α β ( 1 γ log α ) 1 α β ( 1 γ log α ) 1 β 2 [ π 2 6 + ( 1 γ log α ) 2 ] ) , {\displaystyle \mathbf {I} ({\boldsymbol {\theta }})=[I_{ij}]={\begin{pmatrix}{\frac {1}{\alpha }}&{\frac {1}{\alpha \beta }}(1-\gamma -\log \alpha )\\{\frac {1}{\alpha \beta }}(1-\gamma -\log \alpha )&{\frac {1}{\beta ^{2}}}\left[{\frac {\pi ^{2}}{6}}+(1-\gamma -\log \alpha )^{2}\right]\end{pmatrix}},}

where π 3.141593 {\displaystyle \pi \simeq 3.141593} and γ 0.577216 {\displaystyle \gamma \simeq 0.577216} is the Euler’s constant.

When β = 1 {\displaystyle \beta =1} , x {\displaystyle x} follows the power function distribution and the r {\displaystyle r} th raw moment of the UW distribution becomes:

μ r = E ( X r ) = α r + α , r = 1 , 2 , . {\displaystyle \mu '_{r}=\mathbb {E} (X^{r})={\frac {\alpha }{r+\alpha }},\quad r=1,2,\ldots .}

In this case, the mean, variance, skewness and kurtosis, are:

μ = α 1 + α , σ 2 = α ( 1 + α ) 2 ( 2 + α ) , {\displaystyle \mu ={\frac {\alpha }{1+\alpha }},\qquad \sigma ^{2}={\frac {\alpha }{(1+\alpha )^{2}(2+\alpha )}},}
skewness = 2 ( 1 α ) ( 2 + α ) 1 + 2 α , kurtosis = 3 ( 2 + α ) ( 2 α + 3 α 2 ) α ( 3 + α ) ( 4 + α ) . {\displaystyle {\textit {skewness}}={\frac {2(1-\alpha )}{(2+\alpha )}}{\sqrt {1+{\frac {2}{\alpha }}}},\qquad {\textit {kurtosis}}={\frac {3(2+\alpha )(2-\alpha +3\alpha ^{2})}{\alpha (3+\alpha )(4+\alpha )}}.}

The skewness can be negative, zero, or positive when α < 1 , α = 1 , α > 1 {\displaystyle \alpha <1,\alpha =1,\alpha >1} . And if α = 1 {\displaystyle \alpha =1} , with β = 1 {\displaystyle \beta =1} , x {\displaystyle x} follows the standard uniform distribution, and the measures becomes:

μ = 1 2 , σ 2 = 1 12 , skewness = 0 , kurtosis = 9 5 . {\displaystyle \mu ={\frac {1}{2}},\qquad \sigma ^{2}={\frac {1}{12}},\qquad {\textit {skewness}}=0,\quad {\textit {kurtosis}}={\frac {9}{5}}.}

For the case of β = 2 {\displaystyle \beta =2} , x {\displaystyle x} follows the unit-Rayleigh distribution, and:

μ r = E ( X r ) = 1 π 2 α r e r 2 / ( 4 α ) e r f c ( r 2 α ) , r = 1 , 2 , , {\displaystyle \mu '_{r}=\mathbb {E} (X^{r})=1-{\frac {\sqrt {\pi }}{2{\sqrt {\alpha }}}}\,r\,e^{r^{2}/(4\alpha )}\,\mathrm {erfc} \left({\frac {r}{2{\sqrt {\alpha }}}}\right),\qquad r=1,2,\ldots ,}

where

e r f c ( z ) = 2 π z e x 2 d x , z > 0 , {\displaystyle \mathrm {erfc} (z)={\frac {2}{\sqrt {\pi }}}\int _{z}^{\infty }e^{-x^{2}}\,dx,\qquad z>0,}

Is the complementary error function. In this case, the measures of the distribution are:

μ = 1 π 2 α e 1 / α e r f c ( 1 2 α ) , σ 2 = 1 π α e 1 / α e r f c ( 1 α ) [ 1 π 2 α e 1 / α e r f c ( 1 2 α ) ] 2 . {\displaystyle \mu =1-{\frac {\sqrt {\pi }}{2{\sqrt {\alpha }}}}\,e^{1/\alpha }\,\mathrm {erfc} \left({\frac {1}{2{\sqrt {\alpha }}}}\right),\sigma ^{2}=1-{\frac {\sqrt {\pi }}{\sqrt {\alpha }}}\,e^{1/\alpha }\,\mathrm {erfc} \left({\frac {1}{\sqrt {\alpha }}}\right)-\left[1-{\frac {\sqrt {\pi }}{2{\sqrt {\alpha }}}}\,e^{1/\alpha }\,\mathrm {erfc} \left({\frac {1}{2{\sqrt {\alpha }}}}\right)\right]^{2}.}

Applications

It was shown to outperform, against other distributions, like the Beta and Kumaraswamy distributions, in: maximum flood level, petroleum reservoirs, risk management cost effectiveness,2 and recovery rate of CD34+cells data.

See also

See also

References

References

  1. Mazucheli, J.; Menezes, A. F. B.; Ghitany, M. E. (2018). "The Unit-Weibull Distribution And Associated Inference". Journal of Applied Probability and Statistics. 13.
  2. Mazucheli, J.; Menezes, A. F. B.; Fernandes, LB; de Oliveira, RP; Ghitany, ME (2019). "The unit-Weibull distribution as an alternative to the Kumaraswamy distribution for the modeling of quantiles conditional on covariates". Journal of Applied Statistics. 47 (6): 954–974. doi:10.1080/02664763.2019.1657813. PMC 9041746. PMID 35706917.