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A useful extension of the Burr III distribution
Journal of Statistical Distributions and Applications volume 4, Article number: 24 (2017)
Abstract
For any continuous baseline G distribution, Zografos and Balakrishnan (Statistical Methodology 6:344–362, 2009) introduced the gammagenerated family of distributions with an extra shape parameter. Based on this family, we define a new fourparameter extension of the Burr III distribution. It can have decreasing, unimodal and decreasingincreasingdecreasing hazard rate function. We provide a comprehensive account of some of its structural properties. We propose a new loggamma Burr III regression model, which is a feasible alternative for modeling the four existing types of failure rates. Two applications to real data sets and a simulation study illustrate the performance of the new models.
Introduction
Adding new shape parameters to expand a parent distribution plays a fundamental role to generate a larger family with a wide range of skewness and light or heavy tails. Several mathematical properties of the extended family may be easily explored using linear combination of exponentiatedG (“expG” for short) distributions. Further, this induction of parameters has been proved useful in investigating tail properties and also for improving the goodnessoffit of the generator family. The wellknown generators are the following ones: betaG by Eugene et al. (2002), KumaraswamyG (KwG) by Cordeiro and de Castro (2011), McDonaldG (McG) by Alexander et al. (2012), gammaG by Zografos and Balakrishnan (2009), among others. Recently, several distribution generators have been proposed, for example, Alzaatreh et al. (2013) proposed the the TX family of distributions, Cordeiro et al. (2014) introduced the the Lomax generator, Cordeiro et al. (2015) defined a new generalized Weibull family, Tahir et al. (2015) studied the odd generalized exponential family, Nofal et al. (2016) proposed the generalized transmutedG family and Cordeiro et al. (2017) investigated the generalized odd loglogistic family.
Zografos and Balakrishnan (2009) proposed a family of univariate distributions generated by gamma random variables with an additional shape parameter to a parent model. For any baseline cumulative distribution function (cdf) G(x), and \(x \in \mathbb {R}\), they defined the gammaG family by the probability density function (pdf) f(x) and cdf F(x) (for c>0) given by
and
respectively, where g(x)=d G(x)/d x, \(\Gamma (c)=\int _{0}^{\infty } t^{c1}\,{\mathrm {e}}^{t}dt\) denotes the gamma function, and \(\gamma (c,z)=\int _{0}^{z} t^{c1}\,{\mathrm {e}}^{t}dt\) denotes the incomplete gamma function. The gammaG family has the same parameters of the G distribution plus an extra shape parameter c. The increase of one parameter is the price to pay for adding more flexibility to the generated model compared to G. For c=1, Eq. (1) becomes the density function g(x), which is a positive point. The parameter c can provide greater flexibility in the form of the generated distribution and, consequently, it can be a very useful model for fitting positive data.
For a random variable X with pdf (1), we have \(X\overset {d}{=} G^{1}(1{\mathrm {e}}^{Z})\), where Z ∼ Gamma (c,1). If c=1, then Z∼ exp(1) and \(X\overset {d}{=} G^{1}(U)\), where U∼U(0,1).
The Burr III (BIII) cumulative distribution is given by
where α>0 and β>0 are shape parameters and s>0 is a scale parameter. The pdf corresponding to (3) is given by
The BIII distribution has been used in various fields of sciences and its features extensively analyzed. It appeared under the name of the Dagum (1977) distribution in studies of income, wage and wealth distributions. For an excellent survey on its genesis and empirical applications, see Kleiber and Kotz (2003) and Kleiber (2008). It is known as the inverse Burr distribution (see, e.g., Klugman et al. 1998) in the actuarial literature and as the kappa distribution in the meteorological area (Mielke, 1973). This distribution has also been employed in finance, environmental studies, survival analysis and reliability theory (see Lindsay et al. 1996; Gove et al. 2008).
In this paper, we define and study the fourparameter gamma Burr III (GBIII) distribution by inserting (3) and (4) in the generator density (1). The GBIII density becomes
The BIII pdf is a special case of (5) when c=1. The cdf of the GBIII distribution reduces to
Hereafter, we denote the GBIII random variable having pdf (5) by X∼GBIII(c,α,β,s). The hazard rate function (hrf) of X is given by
Figure 1 displays some plots of the density and hrf of X for selected parameter values, respectively. The hrf of X can be decreasing, unimodal and decreasingincreasingdecreasing. The GBIII model can have either positive or negative skewness.
Inverting F(x)=u, we obtain the quantile function (qf) of X as
for 0<u<1, where Q ^{−1}(c,u) is the inverse function of Q(c,x)=1−γ(c,x)/Γ(c); see, for details, http://functions.wolfram.com/GammaBetaErf/InverseGammaRegularized/. One can also use (8) for simulating GBIII variates: if U is a uniform random variable on the unit interval (0,1), then X=Q(U) will be a GBIII random variable.
The rest of the paper is outlined as follows. In Section Structural properties of the GBIII distribution, we obtain some structural properties of the GBIII distribution and estimate the model parameters by maximum likelihood. We propose a new regression model based on the logarithm of this distribution in Section The loggamma Burr III regression model. Two applications to real data and a simulation study are addressed in Section Applications and simulation to prove empirically the flexibility of the new models. Finally, some conclusions are offered in Section Conclusions.
Structural properties of the GBIII distribution
In the following subsections, we obtain a linear representation for the density function and a power series for the qf of the new distribution and estimate its parameters. These expressions can be computed numerically in platforms such as MAPLE, MATHEMATICA, Ox and R using a large number in the upper limit instead of infinity.
Linear representation
Here, we demonstrate that the GBIII density can be expressed as a linear combination of BIII densities. The binomial coefficient generalized to real arguments is given by \({x \choose y} = \Gamma (x+1)/[\Gamma (y+1) \Gamma (xy+1)]\). For any real parameter c>0, the convergent series holds (http://functions.wolfram.com/ElementaryFunctions/Log/06/01/04/03/)
where G _{ α,β,s }(x)^{c+k−1}=G _{ α,(c+k−1)β,s }(x) and the constants p _{ j,k } can be determined recursively (for j≥0) as
for k=1,2,… and p _{ j,0}=1.
For a real parameter c>0, we define
By using this result, the pdf f(x) can be expressed as a linear combination
where g _{ α,(c+k)β,s }(x) denotes the BIII pdf in (4) with parameters α, (c+k)β and s. So, several mathematical properties of the GBIII distribution can be obtained from those of the BIII distribution using (10) in platforms such as MAPLE and MATHEMATICA.
Equation (10) holds for any real parameter c>0 and then some mathematical properties of the new model are valid in the same parameter space, where those properties of the BIII model hold. Evidently, the integrals for the ordinary and incomplete moments and generating function of X can also be computed numerically in Ox and R.
Quantile expansion
We use throughout the paper an equation by Gradshteyn and Ryzhik (2000, Section 0.314) for a power series raised to a positive integer n
where the coefficients c _{ n,i } (for n≥0 and i=1,2,…) are determined from the recurrence equation using any algebraic or numerical software
and \(c_{n,0}=a_{0}^{n}\).
If V∼G a m m a(c,1), the qf Q _{ V }(u) of V admits the power series
where m _{0}=0, m _{1}=1 and any coefficient m _{ i+1} (for i≥1) can be determined by the cubic recurrence equation
where Δ(i)=0 if i<2 and Δ(i)=1 if i≥2. The first few coefficients are m _{2}=1/(c+1), m _{3}=(3c+5)/[2(c+1)^{2}(c+2)],… Let m _{0}=0 and define q _{ i }=m _{ i+1} Γ(c+1)^{(i+1)/2} (for i=0,1,2…).
For m≥1, we define J _{ m }={(i,k),i+k=m;i,k=0,1,2,…}. Then, we can rewrite the GBIII qf from (8) as
Next, using Eq. (11), we obtain
where (for k≥0) \(d_{k,0}=q_{0}^{k}\) and, for i=1,2…, \(d_{k,i}=(i\,q_{0})^{1}\,\sum _{j=1}^{i}[j(k+1)i]\,q_{j}\,d_{k,ij}\).
Further, we have
and then we rewrite Eq. (12) as
where (for m≥1)
We now consider the delta expansion given by
where \(\tau _{n}=\prod _{j=0}^{n1} (\gamma j)\). Based on this expansion, we can write Q(u) as
where ν _{0}=−1. Then, using again (11), we obtain
where (for m≥0) \(s_{m}=\sum _{n=1}^{\infty }\frac {\tau _{n}}{n!}\,\delta _{n,m}\), and (for n≥1) \(\delta _{n,m}=(m\,\nu _{0})^{1}\,\sum _{p=1}^{m}\,[p\,(n+1)m]\,\nu _{m}\,\delta _{n,mp}\), and \(\delta _{n,0}=\nu _{0}^{n}\).
Hence, Eq. (13) reveals that the GBIII qf can be expressed as a power series raised to − 1/α. Let W(·) be any integrable function in a positive real line. We can write
Equations (13) and (14) are the main results of this section since we can obtain from them various GBIII mathematical quantities (moments, generating function, etc). In fact, some of them follow by using the right integral for special W(·) functions, which are sometimes simpler than if they are based on the left integral.
Maximum likelihood estimation
The maximum likelihood estimates (MLEs) enjoy desirable properties and can be used when constructing confidence intervals. Firstorder asymptotic theory for these estimates delivers simple approximations that may work well in finite samples. In this section, we consider the estimation of the unknown parameters of the GBIII distribution by maximum likelihood. Let x _{1}⋯,x _{ n } be a random sample from (5) and θ=(c,α,β,s)^{T} be the parameter vector. The loglikelihood function ℓ(θ)= logL(θ) for θ is given by
Maximization of (15) can be performed by using well established routines like nlminb or optimize in the R statistical package. The routines are able to locate the maximum in all cases if we take different starting values for the parameters. However, it is desirable to have reasonable starting values, which can be chosen using the estimates from the fitted BIII distribution.
The MLEs in θ, say \(\widehat {\boldsymbol {\theta }}\), can also be determined numerically as simultaneous solutions of the equations ∂ ℓ(θ)/∂ θ=0. For interval estimation of the components in θ, we require the observed information matrix for θ, say \(\ddot {\mathbf {L}}(\boldsymbol {\theta })=\{L_{rv}\}\) (r,v=c,α,β,s), whose elements can be obtained from the authors upon request.
The loggamma Burr III regression model
Different forms of regression models have been studied in survival analysis. Among them, the locationscale regression model (Lawless 2003) is distinguished since it is frequently used in clinical trials. We propose a new locationscale regression model based on the logarithm of the GBIII random variable named the loggamma Burr III (LGBIII) regression model as a feasible alternative for modeling the four existing types of hazard rates.
If X is a random variable having the GBIII density function (5), we define Y=log(X). The pdf of Y obtained by replacing s=e^{μ} and α=1/σ is given by
where \(y \in \mathbb {R}\), \(\mu \in \mathbb {R}\) is the location parameter, σ>0 is the scale parameter, and c>0 and β>0 are shape parameters. We refer to Eq. (16) as the LGBIII distribution, say Y∼LGBIII(c,β,σ,μ). The density of the random variable Z=(Y−μ)/σ follows from (16).
The survival function of Y is
In many practical applications, parametric models with explanatory variables are used to estimate univariate survival functions for censored data. A parametric model that provides a good fit to lifetime data tends to yield more precise estimates for the quantities of interest. Based on the LGBIII density, we propose a linear locationscale regression model linking the response variable y _{ i } and the explanatory variable vector \(\mathbf {v}_{i}^{T}=(v_{i1},\ldots,v_{ip})\) as
where the random error z _{ i } has density function (16) with μ=0 and σ=1, τ=(τ _{1},…,τ _{ p })^{T}, σ>0, c>0 and β>0 are unknown parameters. The parameter \(\mu _{i}=\mathbf {v}_{i}^{T} {\boldsymbol {\tau }}\) is the location of y _{ i }. The location parameter vector μ=(μ _{1},…,μ _{ n })^{T} is represented by a linear model μ=V τ, where V=(v _{1},…,v _{ n })^{T} is a known model matrix. The LGBIII regression model (18) opens new possibilities for fitting many different types of data. For example, it contains as submodel the logBurr III (LBIII) regression model when c=1.
Consider a sample (y _{1},v _{1}),⋯,(y _{ n },v _{ n }) of n independent observations, where each random response is defined by y _{ i }= min{log(x _{ i }), log(c _{ i })}. We assume noninformative censoring such that the observed lifetimes and censoring times are independent. Let F and C be the sets of individuals for which y _{ i } is the loglifetime or logcensoring, respectively. Conventional likelihood estimation techniques can be applied here. The loglikelihood function for θ=(c,β,σ,τ ^{T})^{T} from model (18) is given by \(l({\boldsymbol {\theta }})=\sum \limits _{i \in F}l_{i}({\boldsymbol {\theta }})+\sum \limits _{i \in C}l_{i}^{(c)}({\boldsymbol {\theta }})\), where l _{ i }(θ)= log[f(y _{ i })], \(l_{i}^{(c)}({\boldsymbol {\theta }})=\log [S(y_{i})]\), f(y _{ i }) is the density (16) and S(y _{ i }) is the survival function (17) of Y _{ i }. The total loglikelihood function for θ reduces to
where \(z_{i}=(y_{i}\mathbf {v}_{i}^{T}{\boldsymbol {\tau }})/\sigma \) and r is the number of the uncensored observations (failures). The MLE \(\widehat {{\boldsymbol {\theta }}}\) can be evaluated by maximizing (19). We use the NLMixed procedure in SAS to obtain \(\widehat {{\boldsymbol {\theta }}}\). Initial values for τ and σ are taken from the fitted LBIII regression model (with c=1). We can fit the LBIII model to the uncensored observations only and then take the parameter estimates as initial values to fit the LGBIII regression model.
The estimated survival function for y _{ i } follows from the fitted LGBIII model (\(\hat {z}_{i}=(y_{i}\mathbf {v}_{i}^{T}\hat {{\boldsymbol {\tau }}})/\hat {\sigma }\)) as
Under firstorder asymptotic theory, the (p+3)×(p+3) asymptotic covariance matrix K(θ)^{−1} of \(\widehat {\boldsymbol {\theta }}\), where K(θ) is the expected information matrix for θ, can be approximated by the inverse of the observed information matrix \(\ddot {\mathbf {L}}({\boldsymbol {\theta }})\). The elements of this matrix can be computed numerically to construct approximate confidence intervals for the parameters in θ. We can use likelihood ratio (LR) statistics for comparing some submodels with the LGBIII model in the classical way.
Applications and simulation
Application of GBIII to cigarettes data
In order to illustrate the estimation results in Section 3, we work with carbon monoxide measurements made in several brands of cigarettes in 1994. The data have been collected by the Federal Trade Commission (FTC), which is an independent agency of the United States Government, whose main mission is the promotion of consumer protection.
The data can be found at http://www.econdataus.com/cigrs94.html and contain n=384 observations. We analyze the carbon monoxide (CO), measured in milligrams per cigarette, from several cigarette brands. We fit the GBIII, BIII and other submodels to these data by the method of maximum likelihood. We also fit two more models to the current data: the beta Burr III (BBIII) (Gomes et al. 2013) and beta Weibull (BW) (Lee et al. 2007) distributions. The MLEs of the parameters, their standard errors (SEs) and the Akaike Information Criterion (AIC) for the fitted models are listed in Table 1. The required numerical evaluations are implemented using the nlminb function of the R language. When the GBIII model (5) is evaluated at c=1,β=1 it gives rise to the loglogistic (LL) model. For α=1 and c=1, we have as a special case the exponentiated loglogistic (ELL) model. From the figures in Table 1, we note that the smallest AIC value corresponds to the GBIII model.
A comparison of the new distribution with three of its submodels using LR statistics is described in Table 2. These statistics indicate that the new distribution is the most adequate model to these data.
The plots of the fitted densities of the GBIII distribution and its submodels along with the fitted densities of the BBIII and BW models are displayed in Fig. 2. They reveal that the GBIII distribution provides a better fit to the current data than those of the other models.
The measures of skewness and kurtosis for the GBIII distribution are, respectively, 0.3001116 and 0.05107192.
Further, we apply the Cramér–von Mises (W ^{∗}) and Anderson–Darling (A ^{∗}) goodnessoffit statistics in order to verify which model yields the best fit to these data. These statistics are described by Chen and Balakrishnan (1995). In general, the smaller the values of these statistics indicates a better fit. The values of W ^{∗} and A ^{∗} for six fitted models to the current data are listed in Table 3. The figures in this table reveal that the GBIII model provides the best fit among the fitted models.
Some computing issues and a simulation study
As mentioned before, the optimization for estimating the parameters can be performed by minimizing the negative loglikelihood and, for that, we use the nlminb function of the R language. Optimization can also be tackled through simulated annealing (Kirkpatrick et al. 1983) using the optim function of the R. Reasonable starting values are chosen such that the estimated pdf of a submodel fits well the histogram of the data. We now discuss some estimation issues related to the GBIII distribution. Mäkeläinen et al. (1981), in their Theorem 2.1, have established conditions for existence and uniqueness of the MLEs. However, proving that the likelihood function satisfies those conditions is a very hard task that could be addressed in a separate paper.
We conduct a Monte Carlo simulation study to assess the finite sample behaviour of the MLEs of the GBIII parameters. Random samples from the GBIII model are obtained using the qf given by (8). We consider as the true parameter values the average between two parameter vector estimates obtained for the cigarettes data when two different starting points where chosen. Even though those starting points differ substantially, the estimates do not.
Let θ=(α,β,s,c)=(17.11192,0.02785,1.49817,2.64952) be the true parameter vector. For each simulated sample, we estimate the true parameter vector using as starting points the socalled initial point 1 and initial point 2, which correspond to the estimated vectors of θ of the submodels 1 and 2 given in Table 1. The results are obtained from k=500 replicates for each of the sample sizes n=50,100,500,1,000 and 5,000. For a specified sample size and k=500 estimated values obtained using one of the two referred starting values, we evaluate the average of those estimated vectors and the square root mean squared errors (SRMSEs). Afterwards, we take the averages of the results obtained using each of the starting points to produce Table 4. As we can observe from the figures in this table, the estimated expected vector does approach the true vector, but the SRMSEs decrease slowly.
In Fig. 3, we compare the GBIII density for the true vector and the corresponding estimated expected vectors obtained for the cases when the sample sizes are 50,100,500,1,000 and 5,000, when we use the initial points 1 and 2. Regarding the consistency of the GBIII parameter estimators, Fig. 3 shows that when the sample size increases, the estimated vector tends to the true parameter vector, regardless of the initial values used in the estimation procedure. However, as mentioned before, the convergence seems rather slow.
In order to provide some empirical evidence about the asymptotic distribution of the MLEs of the GBIII density, we simulate 5,000 samples of size 10,000 from the GBIII model evaluated at the true vector. Figure 4 displays the histograms of the corresponding 5,000 estimates of the parameters. Each curve represents the normal density with the mean and standard deviation parameters fixed, respectively, at the average and sample standard deviation of the 5,000 parameter estimates. The vertical dotted lines represent the true parameter values. We can note, for each of the parameters, that the normal model provides a good approximation of the distributions of the parameter estimates. In summary, the simulations confirm that the GBIII estimators are consistent and their distributions can be approximated by the normal distribution in accordance with the firstorder likelihood theory.
An application of the LGBIII regression model
In this section, we fit the LGBIII regression model defined in Section 3 to a data set obtained from a study carried out at the Department of Entomology of the Luiz de Queiroz School of Agriculture, University of São Paulo, which aims to assess the longevity of the mediterranean fruit fly (ceratitis capitata). The need for this fly to seek food just after emerging from the larval stage has permitted the use of toxic baits for its management in Brazilian orchards for at least fifty years. This pest control technique consists of using small portions of food laced with an insecticide, generally an organophosphate, that quickly kills the flies, instead of using an insecticide alone. Recently, there have been reports of the insecticidal effect of extracts of the neem tree leading to proposals to adopt various extracts (aqueous extract of the seeds, methanol extract of the leaves and dichloromethane extract of the branches) to control pests such as the mediterranean fruit fly. The experiment was completely randomized with eleven treatments, consisting of different extracts of the neem tree, at concentrations of 39, 225 and 888 ppm. After preliminary statistical analysis, these eleven treatments were allocated into two groups, namely:

Group 1: Control 1 (deionized water); Control 2 (acetone  5%); aqueous extract of seeds (AES) (39 ppm); AES (225 ppm); AES (888 ppm); methanol extract of leaves (MEL) (225 ppm); MEL (888 ppm); and dichloromethane extract of branches (DMB) (39 ppm).

Group 2: MEL (39 ppm); DMB (225ppm) and DMB (888 ppm).
For more details, see Silva et al. (2013). The response variable in the experiment is the lifetime of the adult flies in days after exposure to the treatments. The experimental period is set at 51 days, so that the numbers of larvae that survived beyond this period are considered as censored data. The total sample size is n=72, because four observations are lost. Therefore, we use the following variables: t _{ i }lifetime of ceratitis capitata adults in days, δ _{ i }censoring indicator, v _{ i1}sex of the larvae and v _{ i2}group (0=group 1, 1=group 2). Next, we present results by fitting the regression model
where the random variable z _{ i } has the LGBIII density (16) (with μ=0 and σ=1) for i=1,…,72. The MLEs of the model parameters are evaluated using the NLMixed procedure in SAS. Iterative maximization of the loglikelihood function (19) starts with initial values for β and σ taken from the fit of the LBIII regression model with c=1, i.e. β=0.4, σ=0.2, τ _{0}=3.4, τ _{1}=0.04 and τ _{2}=−0.3. Table 5 lists the MLEs of the model parameters. The values of the AIC, CAIC and BIC statistics are smaller for the LGBIII regression model when compared to those values for the LBIII regression model.
A comparison of the new distribution with its LBIII submodel using the LR statistic w is presented in Table 6. The value of w indicates that the LGBIII distribution provides a better fit to these data than the null model.
We note from the fitted LGBIII regression model that x _{1} is not significant at 5%. So, the final model is given by
The MLEs of the parameters in the final model are listed in Table 7.
Note again that the values of the AIC, CAIC and BIC statistics are smaller for the LGBIII regression model when compared to those values for the LBIII regression model. In order to assess if the model is appropriate, the plots comparing the empirical survival function and the estimated survival function by the LGBIII regression model, see Eq. (20), are displayed in Fig. 5. Based on these plots, it is evident that the LGBIII model provides a superior fit.
Conclusions
Providing a new class of distributions is always precious for statisticians. There has been an increased interest in developing generalized classes of distributions by adding a single shape parameter to a baseline distribution. There is no doubt that some of these classes have attracted several applied researchers. Following this idea, Zografos and Balakrishnan (2009) introduced a gammagenerated family of distributions by adding an extra positive shape parameter to a baseline model. In this paper, we study some mathematical properties of the new fourparameter gamma Burr III distribution based on the gammagenerated family. We prove empirically that the proposed distribution can provide a better fit than important generated models such as the beta Burr III (Gomes et al. 2013) and beta Weibull (Lee et al. 2007) distributions. Finally, we propose a new loggamma Burr III regression model and illustrate its importance by means of one application to a real data set.
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GMC proposed the gamma Burr III model, wrote some parts of Sections 1 to 2, and also drafted the manuscript. AEG wrote some parts of Section 2. CQdS wrote some parts of Section 2, subsections 4.1 and 4.2 and prepared Figs. 1, 2, 3 and 4. EMMO proposed the loggamma Burr III model described in Section 3, performed the application in subsection 4.3, and also prepared Fig. 5. All authors read and approved the final manuscript.
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Cordeiro, G., Gomes, A., daSilva, C. et al. A useful extension of the Burr III distribution. J Stat Distrib App 4, 24 (2017). https://doi.org/10.1186/s404880170079y
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DOI: https://doi.org/10.1186/s404880170079y
Keywords
 Estimation
 Gamma distribution
 GammaG family
 Moment
 Regression model