Unit 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 (real)
β>0 (real)
Support x(0,1)
PDF 1xαβ(logx)β1exp[α(logx)β]
CDF exp[α(logx)β]
Quantile exp[(logpα)1β],0<p<1
Skewness μ'33μ'2μ+μ3σ3
Excess kurtosis μ'44μ'3μ+6μ'2μ23μ4σ4
MGF n=0(1)nn!αn/βΓ(nβ+1)

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

Definitions

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Probability density function

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It's probability density function is defined as:

f(x;α,β)=1xαβ(logx)β1exp[α(logx)β]

Cumulative distribution function

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And it's cumulative distribution function is:

F(x;α,β)=exp[α(logx)β]

Quantile function

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The quantile function of the UW distribution is given by:

Q(p)=exp[(logpα)1β],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

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Moments

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The rth raw moment of the UW distribution can be obtained through:

μ'r=𝔼(Xr)=𝔼(erY)=MY(r)=n=0(1)nn!αn/βΓ(nβ+1).

Skewness and kurtosis

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

𝑠𝑘𝑒𝑤𝑛𝑒𝑠𝑠=μ'33μ'2μ+μ3σ3,𝑘𝑢𝑟𝑡𝑜𝑠𝑖𝑠=μ'44μ'3μ+6μ'2μ23μ4σ4

Hazard rate

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

h(x;α,β)=f(x;α,β)1F(x;α,β)=αβ(logx)β1exp[α(logx)β]x(1exp[α(logx)β]),0<x<1.

Parameter estimation

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Let 𝐱=(x1,,xn) be a random sample of size n from the UW distribution with probability density function defined before. Then, the log-likelihood function of 𝜽=(α,β) is:

(𝜽;𝐱)=n(logα+logβ)i=1nlogxi+(β1)i=1nlog(logxi)αi=1n(logxi)β

The likelihood estimate 𝜽^ of 𝜽 is obtained by solving the non-linear equations

α=nαi=1n(logxi)β=0,

and

β=nβ+i=1nlog(logxi)αi=1n(logxi)βlog(logxi)=0.

The expected Fisher information matrix of 𝜽=(α,β) based on a single observation is given by

𝐈(𝜽)=[Iij]=(1α1αβ(1γlogα)1αβ(1γlogα)1β2[π26+(1γlogα)2]),

where π3.141593 and γ0.577216 is the Euler’s constant.

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When β=1, x follows the power function distribution and the rth raw moment of the UW distribution becomes:

μ'r=𝔼(Xr)=αr+α,r=1,2,.

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

μ=α1+α,σ2=α(1+α)2(2+α),
𝑠𝑘𝑒𝑤𝑛𝑒𝑠𝑠=2(1α)(2+α)1+2α,𝑘𝑢𝑟𝑡𝑜𝑠𝑖𝑠=3(2+α)(2α+3α2)α(3+α)(4+α).

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

μ=12,σ2=112,𝑠𝑘𝑒𝑤𝑛𝑒𝑠𝑠=0,𝑘𝑢𝑟𝑡𝑜𝑠𝑖𝑠=95.

For the case of β=2, x follows the unit-Rayleigh distribution, and:

μ'r=𝔼(Xr)=1π2αrer2/(4α)erfc(r2α),r=1,2,,

where

erfc(z)=2πzex2dx,z>0,

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

μ=1π2αe1/αerfc(12α),σ2=1παe1/αerfc(1α)[1π2αe1/αerfc(12α)]2.

Applications

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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

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References

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  1. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  2. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).