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A Heavy Tailed Model Based on Power XLindley Distribution with Actuarial Data Applications

Mohammed Elgarhy1, Amal S. Hassan2, Najwan Alsadat3, Oluwafemi Samson Balogun4, Ahmed W. Shawki5, Ibrahim E. Ragab6,*

1 Department of Basic Sciences, Higher Institute of Administrative Sciences, Belbeis, 44621, Egypt
2 Faculty of Graduate Studies for Statistical Research, Cairo University, Giza, 12613, Egypt
3 Department of Quantitative Analysis, College of Business Administration, King Saud University, Riyadh, 11587, Saudi Arabia
4 Department of Computing, University of Eastern Finland, Joensuu, 80130, Finland
5 Central Agency for Public Mobilization & Statistics (CAPMAS), Cairo, 11819, Egypt
6 Department of Basic Sciences, Egyptian Institute of Alexandria Academy for Management and Accounting, EIA, Alexandria, 21919, Egypt

* Corresponding Author: Ibrahim E. Ragab. Email: email

Computer Modeling in Engineering & Sciences 2025, 142(3), 2547-2583. https://doi.org/10.32604/cmes.2025.058362

Abstract

Accurately modeling heavy-tailed data is critical across applied sciences, particularly in finance, medicine, and actuarial analysis. This work presents the heavy-tailed power XLindley distribution (HTPXLD), a unique heavy-tailed distribution. Adding one more parameter to the power XLindley distribution improves this new distribution, especially when modeling leptokurtic lifetime data. The suggested density provides greater flexibility with asymmetric forms and different degrees of peakedness. Its statistical features, like the quantile function, moments, extropy measures, incomplete moments, stochastic ordering, and stress-strength parameters, are explored. We further investigate its use in actuarial science through the computation of pertinent metrics, such as value-at-risk, tail value-at-risk, tail variance, and tail variance premium. To obtain the point and interval parameter estimates, we use the maximum likelihood estimation approach. We do many simulation tests to evaluate the performance of our proposed estimator. Metrics like bias, relative bias, mean squared error, root mean squared error, average interval length, and coverage probability will be used in these tests to assess the estimator’s performance. To illustrate the practical value of our proposed model, we apply it to analyze three real-world datasets. We then compare its performance to established competing models, highlighting its advantages.

Keywords

Power XLindley; heavy-tailed-G family; extropy measure; stochastic ordering; parametric estimation; asymmetric dataset

1  Introduction

An essential area of statistics is lifetime data analysis, which models and examines the duration until a phenomenon fails or survives. It is useful in a wide range of disciplines, including biology, ecology, medicine, social sciences, and reliability engineering. The exponential distribution, with its constant failure rate function and memoryless quality, is one of the most popular distributions for lifespan data. Nevertheless, certain data types, such as those that show growing, declining, unimodal, or bathtub-shaped failure rate functions, might not be well-modeled by the exponential distribution. To get around the drawbacks of the exponential distribution and offer improved flexibility, many alternative distributions have been put forth in the literature. In this sense, one of the most flexible and straightforward lifespan models is the XLindley distribution (XLD), which was introduced by Chouia et al. [1] as a combination of the Lindley and the exponential distributions. The probability density function (PDF) and cumulative distribution function (CDF) of the XLD are defined as:

f(x;β)=(β2(2+β+x)(1+β)2)eβx;x>0,

and

F(x;β)=1(1+βx(1+β)2)eβx;x>0,

where β>0 is the scale parameter. Many academics have recently proposed various methods for incorporating new probability distributions. A strategy that increases the flexibility of the resulting distribution is the power transformation of the research variable with an additional shape parameter such as the power half-logistic distribution [2], power length-biased Suja distribution [3], power Lindley-G family [4], power weighted Sujayha distribution [5], power Lomax distribution [6], power Lomax Poisson distribution [7], power-modified Kies-exponential distribution [8], and power-transmuted inverse Rayleigh distribution [9]. In contrast to XLD, the power XLD (PXLD) produced by Meriem et al. [10] has an additional shape parameter that we will be focusing on here. The PDF and CDF of the PXLD are provided as below:

f(y;ϑ,β)=(ϑβ2(2+β+yϑ)yϑ1(1+β)2)eβyϑ;y>0,(1)

and

F(y;ϑ,β)=1(1+βyϑ(1+β)2)eβyϑ;y>0,(2)

where β>0 and ϑ>0 are scale and shape parameters, respectively.

In numerous fields of study during the past decades, including economics, actuarial science, engineering, environmental research, lifespan, medical science, and many more, it has been determined that the classical distributions do not match the data well. To construct many unique models tailored for certain datasets, the authors have gone into great detail in their explanation. The classical distributions may be made more flexible by introducing additional parameters or by performing various transformations on the baseline distribution, which will improve its capacity to handle complex situations. To strengthen the flexibility of models in this context, many classes of distributions have been generated by using various processes, resulting in a more powerful and adaptable distribution for dataset modeling; for instance, Marshall-Olkin-G [11], beta-G [12], Kumaraswamy-G [13], transformed-transformer [14], Weibull-G [15], Dinesh-Umesh-Sanjay-G by [16], type I half-logistic-G [17], exponentiated half-logistic-G [18], Topp-Leone-G [19], Gompertz-G [20], beta odd Lindley-G [21], truncated power Lomax-G [22], Kavya-Manoharan-G [23], odd inverted Topp-Leone [24], Weibull Marshall-Olkin-G [25], sec-G [26], length-biased truncated Lomax-G [27], generalized logarithmic-X [28], alpha log power transformed-G [29], Marshall-Olkin-exponentiated half logistic-G [30] among others.

Probability distributions with a significant number of values in the tail of the distribution that is more than what would be predicted from a normal distribution are referred to as heavy-tailed (HT) distributions. This means that HT distributions assign a higher probability to extreme events or outliers. These distributions are valuable tools in various fields for understanding and managing the risk associated with rare but impactful events. The necessity of the HT distributions in actuarial practice has prompted actuaries to develop new flexible distributions (see [3133]). Reference [34] covered the characteristics, estimates, and fundamental ideas of HT distributions, whereas reference [35] examined the estimation issue of HT distributions in extreme value theory. Moreover, several specific HT distributions have been introduced, including the HT Gleser distribution by [36], Type-I HT-G distributions by [37], Type I HT odd power generalized Weibull-G by [38], and HT generalized Topp-Leone-G by [39]. Many actual application studies in a variety of fields, including hydrology, biology, agriculture, production, survival, and finance, may be shown using the HT class of distributions. In recent times, Ahmed et al. [40] have introduced a new class of distributions dubbed the HT class of distributions. To better examine the underlying patterns of the data sets, this new addition is a useful tool for creating new models that are suitable for analyzing HT, symmetric, complicated, and skewed data sets. The HT-G family of distributions’ CDF and PDF may be written as follows, in that order:

G(y;δ;υ)=δF(y;υ)δ1+F(y;υ),δ>1,yR,(3)

and

g(y;δ;υ)=δ(δ1)f(y;υ)[δ1+F(y;υ)]2,δ>1,yR,(4)

where F(y;υ), and f(y;υ) are the CDF and PDF of the baseline random variable with vector parameter υ.

The field of statistics has a large collection of probability distributions, each with its strengths and weaknesses. It is not possible to represent or express important aspects in every scenario using a single distribution. In response to this limitation, we introduce a novel extension of the PXLD with the assistance of the HT-G family, named the heavy-tailed PXLD (HTPXLD). This paper aims to achieve the following objectives:

•   Create a flexible distribution that can display declining, right-skewed, and unimodal data. Its hazard rate function (HRF) can be growing, decreasing, unimodal, right-skewed, or reverse J-shaped.

•   To construct and evaluate some of the key mathematical properties, including moments, linear representation of density function, incomplete moments (IMs), quantile function (QF), Bonferroni and Lorenz curves, stochastic ordering (SO), extropy measures, and stress-strength (SS) reliability parameter.

•   To obtain the point and approximate confidence interval (CI) estimators of the unknown parameters of the HTPXLD using the maximum likelihood (ML) estimation method. Through the implementation of the Monte Carlo simulation approach, the accuracy of the proposed model estimates is evaluated.

•   A comparative analysis of the proposed model against well-known alternatives is performed using three diverse real-world datasets to assess its practical applicability.

The paper proceeds as follows: Section 2 introduces the HTPXLD. Section 3 delves into its mathematical features. Few actuarial measures are examined in Section 4. In Section 5, we describe the process of estimating model parameters using the ML approach and create CIs for the unknown parameters of the model. A Monte Carlo simulation study is performed in Section 6 to demonstrate the consistency of the suggested estimate. Practical applications of the model are presented in Section 7. Section 8 concludes the paper with some final considerations and key findings.

2  Heavy-Tailed Power XLindley Distribution

This section introduces the core concepts behind the HTPXLD, including PDF, CDF, survival function (SF), HRF, and reversed HRF (RHRF). It also provides visualizations for the PDF and HRF. The CDF of the HTPXLD is created by inserting CDF (2) in CDF (3), resulting in the following expression:

G(y;ω)=δ[1(1+βyϑ)eβyϑ]δ(1+βyϑ)eβyϑ,y;>0,β,ϑ>0,δ>1,(5)

where β=β(1+β)2, ω=(δ,β,ϑ) is the set of parameters. The PDF of the HTPXLD is given by

g(y;ω)=δ(δ1)βϑβ(2+β+yϑ)yϑ1eβyϑ[δ(1+βyϑ)eβyϑ]2,y>0,δ>1,ϑ,β>0.(6)

For ϑ=1, the PDF (6) reduces to the HT XLD (HTXLD) as a special new sub-model. A key idea in survival analysis, reliability engineering, and other domains is the SF, sometimes referred to as the reliability function. It gives the probability that a system or component will operate perfectly for a predetermined amount of time. The SF of the HTXLD is given by

ˉG(y;ω)=(δ1)(1+βyϑ)eβyϑδ(1+βyϑ)eβyϑ.

A mathematical notion utilized in survival analysis, reliability engineering, and other domains is the HRF, represented by h(y;ω). It measures the immediate risk of failure for a system or object that has so far survived at a given time (y). The HRF of the HTXLD is given by

h(y;ω)=δβϑβ(2+β+yϑ)yϑ1(1+βyϑ)[δ(1+βyϑ)eβyϑ].

The RHRF of the HTXLD is given by

ˉh(y;ω)=(δ1)βϑβ(2+β+yϑ)yϑ1eβyϑ[1(1+βyϑ)eβyϑ][δ(1+βyϑ)eβyϑ].

The PDF plots of the HTPXLD for particular parameter values are shown in Fig. 1. The HRF of the HTPXLD for the chosen parameter values is then shown in Fig. 2. From Figs. 1 and 2, we can note that the PDF can be right-skewed, unimodal, or decreasing, but the HRF can be increasing, decreasing, or upside-down.

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Figure 1: Plots of the PDF for the HTPXLD

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Figure 2: Plots of the HRF for the HTPXLD

3  Statistical Properties

A number of statistical properties, such as QF, moments, IMs, PDF linear expansion, Bonferroni and Lorenz curves, SO, SS parameters, and extropy measures that shed light on the structure of the distribution, will be covered here.

3.1 Series Representation

To analyze most of the statistical properties of HTPXLD, we can express the PDF as a linear combination of simpler functions. Using the following power series:

(1+z)n=j1=0(1)j1(n+j11j1)zj1,|z|<1,n>0,(7)

in PDF defined in Eq. (6) provides

f(y;ω)=j1=0(j1+1)(1)j1(δ1)βϑβδj1+1(1+βyϑ)j1(2+β+yϑ)yϑ1eβ(j1+1)yϑ.(8)

Again, using a binomial expansion in PDF (8) yields

f(y;ω)=j1=0τj1,j2ϑ(2+β+yϑ)yϑ(j2+1)1eβ(j1+1)yϑτj1,j2=j1j2=0(j1j2)(j1+1)(1)j1(δ1)β(j2+1)βδj1+1}.(9)

3.2 Quantile Function

In statistical modeling, the QF is essential because it makes it possible to estimate certain percentiles, offers valuable insights into the data distribution, and supports a range of inferential and decision-making procedures. One may determine the QF of the HTPXLD, denoted as Q(u), by solving F(Q(u))=u for u(0,1). Therefore, we must create the following equation:

u=δ[1(1+β(Q(u))ϑ)eβ(Q(u))ϑ]δ(1+β(Q(u))ϑ)eβ(Q(u))ϑ,

which leads to

uδδuδ=(1+β(Q(u))ϑ)eβ(Q(u))ϑ.(10)

By multiplying the two sides of Eq. (10) by e(β+1)2, one may find the Lambert equation (see [41]), which gives

Q(u)=[(β+1)2β1βW1{(uδδuδ)(β+1)2e(β+1)2}]1/ϑ,u(0,1).(11)

Setting u to be equal 0.25,0.5, and 0.75 in Eq. (11) yields the first (Q1), second (Q2), and third (Q3) quartiles of the HTPXLD. These quartiles help assess the symmetry (skewness) and peakedness (kurtosis) of the data. Bowley’s skewness (η1) ([42]) and Moor’s kurtosis (η2) ([43]) are statistics calculated using these quartiles to quantify these characteristics precisely. The equations for η1 and η2 are provided below:

η1=Q(0.75)2Q(0.5)+Q(0.25)Q(0.75)Q(0.25),

and

η2=Q(0.875)Q(0.625)Q(0.375)+Q(0.125)Q(0.75)Q(0.25).

Table 1 presents quantile values (Q1, Q2, Q3), η1 and η2 of the HTPXLD for various parameter values and u values. The table reveals several trends: The data show that increasing ϑ leads to higher values for Q1, Q2, and Q3, while η1 and η2 decrease. Values are generally higher at β=0.5 compared to β=0.8, and there is a consistent trend where Q1, Q2, and Q3 increase with δ, while η1 and η2 decrease.

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3.3 Moments

Moments of distribution offer valuable insights into its shape. They reveal measures like central tendency (average), dispersion (spread), skewness (asymmetry), and kurtosis (peakedness). Therefore, deriving the moments is crucial for understanding any new distribution. The k-th moment about the origin of the HTPXLD is obtained by using PDF (9) as follows:

μk=j1=0τj1,j2ϑ0(2+β+yϑ)yk+ϑ(j2+1)1eβ(j1+1)yϑdy=j1=0τj1,j2ϑ[0(2+β)yk+ϑ(j2+1)1eβ(j1+1)yϑdy+0yk+ϑ(j2+2)1eβ(j1+1)yϑdy].(12)

Using the transformation z=β(j+1)yϑ in (12), we have

μk=j1=0τj1,j2[(2+β)β(j1+1)j2+1+(k/ϑ)0zj2+(k/ϑ)ezdz+1β(j1+1)j2+2+(k/ϑ)0zj2+(k/ϑ)+1ezdz]=j1=0τj1,j2Γ(j2+1+(k/ϑ))β(j1+1)j2+1+(k/ϑ)[(2+β)+j2+1+(k/ϑ)β(j1+1)],(13)

where Γ(.) stands for gamma function (GF). For n=1 in (13), the mean of the HTPXLD is produced. Moreover, the k-th central moment of Y may be calculated in the way that follows by utilizing moments around the origin.

μk=E(Yμ1)k=ku=0(1)u(ku)μu1μku.

Then, using the formulas, κ1=μ3/(μ2)1.5 and κ2=μ4/(μ2)2, one may find the coefficients of skewness and kurtosis, respectively. They play crucial roles in establishing the asymmetry and flatness of the provided distribution. Also, another important measure is the coefficient of variation (CV), defined by CV =σμ1, where μ1 is the first moment and σ is the standard deviation.

Likewise, the k-th incomplete moment of the HTPXLD, based on PDF (9), is determined as follows:

λk(x)=j1=0τj1,j2ϑx0(2+β+yϑ)yk+ϑ(j2+1)1eβ(j1+1)yϑdy=xj1=0τj1,j2ϑ[x0(2+β)yk+ϑ(j2+1)1eβ(j1+1)yϑdy+x0yk+ϑ(j2+2)1eβ(j1+1)yϑdy].(14)

Using the transformation z=β(j+1)yϑ in (14), we have

λk(x)=j1=0τj1,j2[(2+β)β(j1+1)j2+1+(k/ϑ)β(j+1)xϑ0zj2+(k/ϑ)ezdz+1β(j1+1)j2+2+(k/ϑ)β(j+1)xϑ0zj2+(k/ϑ)+1ezdz]=j1=0τj1,j2{(2+β)γ(j2+(k/ϑ)+1,β(j+1)xϑ)[β(j1+1)]j2+(k/ϑ)+1+γ(j2+(k/ϑ)+2,β(j+1)xϑ)[β(j1+1)]j2+(k/ϑ)+2},(15)

where γ(.,x) is the lower incomplete GF. One can find applications of incomplete moments by [44].

Tables 2 and 3 present numerical outcomes for the first four moments, variance (σ2), σ, κ1, κ2 and CV for the HTPXLD for some selected parameter values. Based on the positive values of κ1>0, the HTPXLD exhibits right-skewed. The distribution is characterized as leptokurtic for κ1>3 and platykurtic for κ1<3.

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Tables 2 and 3 reveal several trends: As β and δ increase, it κ1 shows a decrease in kurtosis, with values in Table 3 being lower than those in Table 2, indicating reduced kurtosis at ϑ=2.5 compared to ϑ=1.8. The values of σ2, σ, and CV follow similar trends across the tables, increasing with higher β and δ in both cases.

3.4 Stochastic Ordering

A concept in probability distributions that has been studied in great detail is stochastic ordering, which is crucial for analyzing comparative behavior among random variables in reliability theory and other fields. Stochastic ordering is a powerful tool used in probability and statistics to compare the behavior of random variables. It allows us to understand which random variable is “less risky” or has a “lower probability of taking on extreme values” compared to another. A random variable Y1 is regarded as less than a random variable Y2 in the following ways:

•   SO (represented by Y1stY2) if FY1(y)FY2(y) y.

•   hazard rate order (represented by Y1hrY2) if hY1(y)hY2(y) y.

•   likelihood ratio order (represented by Y1lrY2) if fY1(y)fY2(y) decreases in y.

According to Shaked et al. [45], the following impacts are widely recognized:

Y1lrY2Y1hrY2Y1stY2.

Let Y1 HTPXLD (ω1), ω1(δ1,β,ϑ1) and Y2 HTPXLD (ω2), ω2(δ2,β,ϑ2), then the likelihood ratio ordering is as follows:

f1(y;ω1)f2(y;ω2)=δ1(δ11)ϑ1(2+β+yϑ1)yϑ11eβyϑ1[δ2(1+βyϑ2)eβyϑ2]2δ2(δ21)ϑ2(2+β+yϑ2)yϑ21eβyϑ2[δ1(1+βyϑ1)eβyϑ1]2,

then

ddylog[f1(y;ω1)f2(y;ω2)]=ϑ1yϑ11(2+β+yϑ1)ϑ2yϑ21(2+β+yϑ2)2ϑ2yϑ21eβyϑ2[ββ(1+βyϑ2)][δ2(1+βyϑ2)eβyϑ2]ϑ21y+ϑ11yβϑ1yϑ11+βϑ2yϑ21+2ϑ1yϑ11eβyϑ1[ββ(1+βyϑ1)][δ2(1+βyϑ1)eβyϑ1].

For ϑ2<ϑ1,δ2<δ1, we get ddylog[f1(y;ω1)f2(y;ω2)]<0, for all y0, hence ddylog[f1(y;ω1)f2(y;ω2)]<0, is decreasing in y and hence Y1lrY2.

3.5 Extropy Measures

The extropy (Ext), which is the double complement of the entropy [46], was developed as an alternative uncertainty measure by Lad et al. [47]. The Ext can be statistically utilized to evaluate the accuracy of predicted distributions through the total log scoring method. For a non-negative random variableY, Ext is defined as follows:

Ξ=120f2(y)dy{.}(16)

Thus, using PDF (6) in (16), the extropy of the HTPXLD may be represented as follows:

Ξ=12δ20(βϑ(δ1)β)2(2+β+yϑ)2y2(ϑ1)e2βyϑ[1(1+βyϑ)eβyϑδ]4dy{.}(17)

Using the expansion (7) in (17) gives

Ξ=12j1=0(1)j1(β(δ1)ϑβ)2δ2+j1(3+j1j1)0(2+β+yϑ)2y2(ϑ1)e2βyϑ(1+βyϑ)j1eβj1yϑdy{.}(18)

Using binomial expansion in (18), we have

Ξ=12j1=0j1j2=0(3+j1j1)(j2j1)(1)j1(β)2+j(ϑ(δ1)β)2δ2+j10(2+β+yϑ)2y2(ϑ1)+ϑj2e(2β+βj1)yϑdy,

Then after some simplified form, the previous equation will be

Ξ=12j1=0pj1.j2ϑ[0(2+β)2y2(ϑ1)+ϑj2e(2β+βj1)yϑdy+(2+β)0y2(ϑ1)+ϑj2+ϑe(2β+βj1)yϑdy+0y2(2ϑ1)+ϑj2e(2β+βj1)yϑdy].(19)

Using the transformation z=β(j+1)yϑ in (19), the extropy measure of HTPXLD thus has the following structure after some simplification:

Ξ=12j1=0pj1.j2[(2+β)2Γ(2+j2(1/ϑ))(2β+βj1)(2+j2(1/ϑ))+(2+β)Γ(3+j2(1/ϑ))(2β+βj1)(3+j2(1/ϑ))+Γ(4+j2(1/ϑ))(2β+βj1)(4+j2(1/ϑ))]{,}

where pj1.j2=j1j2=0(3+j1j1)(j2j1)(1)j1(β)2+jϑ((δ1)β)2δ2+j1.

Weighted extropy (WExt), introduced by [48], offers an alternative perspective to traditional entropy. Unlike entropy, it assigns greater weight to larger values within a probability distribution. It can be expressed, mathematically, by

Ξw=120yf2(y)dy{.}(20)

Then by inserting PDF (6) in (20), then the WExt is

Ξw=12δ20(βϑ(δ1)β)2(2+β+yϑ)2y2ϑ1e2βyϑ[1(1+βyϑ)eβyϑδ]4dy{.}

Using the similar procedure discussed above, then Ξw is as follows:

Ξw=12j1=0pj1.j2[(2+β)2Γ(2+j2)(2β+βj1)(2+j2)+(2+β)Γ(3+j2)(2β+βj1)(3+j2)+Γ(4+j2)(2β+βj1)(4+j2)]{.}

The residual extropy (RExt) at the time t of residual lifespan Zt is given by

ΞR=12ˉG2(t)tf2(z)dz{.}(21)

Then, by inserting PDF (6) in (21) and using the similar procedure discussed above, the RExt will be

ΞR=12ˉG2(t)j1=0pj1.j2[(2+β)2Γ(2+j2(1/ϑ),(2β+βj1)tϑ)(2β+βj1)(2+j2(1/ϑ))+(2+β)Γ(3+j2(1/ϑ),(2β+βj1)tϑ)(2β+βj1)(3+j2(1/ϑ))+Γ(4+j2(1/ϑ),(2β+βj1)tϑ)(2β+βj1)(4+j2(1/ϑ))],

where Γ(.,x) is the upper incomplete GF. According to Table 4, for both values of ϑ, there is a discernible trend in the Ext and RExt measures towards becoming less negative with rising β. Both Ext and RExt exhibit a decline in negativity as β rises. On the other hand, WExt’s negativity steadily drops as β rises. When ϑ=2.5 is used instead of ϑ=1.8, the decline in WExt is more gradual and more noticeable at higher β values.

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3.6 Stress-Strength Model

The SS model is a powerful tool in reliability engineering used to assess the probability of a component surviving under operational conditions. It considers two random variables: strength (X), which stands for the component’s intrinsic ability to withstand stress (Y). Therefore, the core concept of the SS model is captured by the following equation: R=P(Y<X), where R represents the reliability, or the probability of the component functioning successfully. This model has a wide range of applications across various scientific fields. Let the strength X HTPXLD (δ1,β1,ϑ) and stress Y HTPXLD (δ2,β2,ϑ), then the SS parameter for the HTPXLD is given by

R=0δ1(δ11)β1ϑβ1(2+β1+xϑ)xϑ1eβ1xϑ[δ1(1+β1xϑ)eβ1xϑ]2δ2[1(1+β2xϑ)eβ2xϑ]δ2(1+β2xϑ)eβ2xϑdx,(22)

where β1=β1(1+β1)2, and β2=β2(1+β2)2. Using expansion (7) twice for the numerator of Eq. (22) gives

R=u1,u2=0A0ϑ(2+β1+xϑ)(1+β1xϑ)u1(1+β2xϑ)u2xϑ1e[β1(u1+1)+β2u2]xϑ×[1(1+β2xϑ)eβ2xϑ]dx,(23)

where A=(1)u1+u2(u1+1)β1β1(δ1)u1+1(δ2)u2. Again, employing the binomial expansion in (23), we get

R=u1,u2=0u1v1=0u2v2=0(u1v1)(u2v2)A0ϑ(2+β1+xϑ)(β1)v1xv1ϑ(β2)v2xv2ϑxϑ1eβ1(u1+u2+1)xϑdx  u1,u2=0u1v1=0u2v2=0(u1v1)(u2+1v2)A0ϑ(2+β1+xϑ)β1)v1xv1ϑ(β2)v2xv2ϑxϑ1e[β1(u1+u2+1)+β2]xϑdx.(24)

After simplifying Eq. (24), we get

R=u1,u2=0A0ϑ(2+β1+xϑ)(β1)v1xv1ϑ(β2)v2xv2ϑxϑ1e[β1(u1+1)+β2(u2+1)]xϑdx  u1,u2=0{B}0ϑ(2+β1+xϑ)(β1)v1xv1ϑ(β2)v2xv2ϑxϑ1e[β1(u1+1)+β2(u2+1)]xϑdx,(25)

where A=u1v1=0u2v2=0(u1v1)(u2v2)A and {B}=u1v1=0u2v2=0(u1v1)(u2+1v2)A.

Note that the integrals in Eq. (25) can be obtained as follows:

I1=u1,u2=0A0ϑ(2+β1)(β1)v1xv1ϑ+ν2ϑ+ϑ1(β2)v2eβ1(u1+u2+1)xϑdx=u1,u2=0A(2+β1)(β1)v1(β2)v2Γ(v1+v2+1)[β1(u1+u2+1)]v1+v2+1,

I2=u1,u2=0A0ϑ(β1)v1xv1ϑ+v2ϑ+2ϑ1(β2)v2eβ1(u1+u2+1)xϑdx=u1,u2=0A(β1)v1(β2)v2Γ(v1+v2+2)[β1(u1+u2+1)]v1+v2+2,

I3=u1,u2=0B0ϑ(2+β1)β1)v1xv1ϑ+v2ϑ+ϑ1(β2)v2xv2ϑe[β1(u1+u2+1)+β2]xϑ=u1,u2=0B(2+β1)(β1)v1(β2)v2Γ(v1+v2+1)[β1(u1+u2+1)+β2]v1+v2+1,

and

I4=u1,u2=0B0ϑ(β1)v1xv1ϑ+ν2ϑ+2ϑ1(β2)v2e[β1(u1+u2+1)+β2]xϑdx,=u1,u2=0B(β1)v1(β2)v2Γ(v1+v2+2)[β1(u1+u2+1)+β2]v1+v2+2.

Then, by inserting I1,I2,I3 and I4, in the Eq. (25), the SS parameter of HTPXLD is as follows:

R=u1,u2=0[(2+β1)A(β1)v1(β2)v2Γ(v1+v2+1)[β1(u1+1)+β2u2]v1+v2+1+A(β1)v1(β2)v2Γ(v1+v2+2)[β1(u1+1)+β2u2]v1+v2+2]u1,u2=0[(2+β1){B}(β1)v1(β2)v2Γ(v1+v2+1)[β1(u1+1)+β2(u2+1)]v1+v2+1+{B}(β1)v1(β2)v2Γ(v1+v2+2)[β1(u1+1)+β2(u2+1)]v1+v2+2].

4  Actuarial Measures

This section introduces several well-known risk measures for the developed model. These measures include Value-at-Risk (VaR), Tail Value-at-Risk (TVaR), Tail Variance (TV), and Tail Variance Premium (TVP).

4.1 Value-at-Risk

As outlined in reference [49], the q-th quantile of a random variable’s CDF corresponds to its VaR. The VaR for the HTPXLD is given by

VaR=[(β+1)2β1βW1{(qδδqδ)(β+1)2e(β+1)2}]1/ϑ.(26)

4.2 Tail Value-at-Risk

TVaR is a crucial risk measure that evaluates the expected loss beyond a specified probability level, once an event has occurred. For the HTPXLD, the TVaR is defined as

TVaR=11qVaRqyf(y;ω)dy.

4.3 Tail Variance and Tail Variance Premium

Landsman [50] first introduced the TV risk measure, which is defined by the variance of the loss distribution above a certain critical threshold. The TV for the HTPXLD can be expressed as

TV=E(Y2Y>yq)(TVaR)2.

4.4 Tail Variance Premium

The TVP combines statistics related to both the central tendency and dispersion of the data, making it a significant risk measure. The TVP for the HTPXLD is given by

TVP=TVaR+κTV,κ>0.

Table 5 demonstrates several key trends: Increasing ϑ values lead to higher VaR and TVaR values, indicating an overall increase in risk measures. For example, higher ϑ values correspond to higher risk estimates. For a given δ, higher ϑ results in greater TVP values across all κ levels. This indicates a more pronounced sensitivity to risk with increasing ϑ. Within the same ϑ and δ settings, TVP values rise with κ, reflecting a higher quantile level and, consequently, increased risk assessment.

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5  Parameter Estimation

Our main goal in this section is to use the ML estimation method to obtain the point and interval estimates of the unknown parameters of the HTPXLD. Assume that y1,,yn, a sample of size n, is taken from the HTPXLD specified by the PDF (6). For the vector of parameters ω=(δ,β,ϑ)T, the log-likelihood function can be written as

logl=nlog(δ(δ1)ϑβ2(1+β)2)+ni=1log(2+β+yϑi)ni=1βyϑi2ni=1log[δ(1+βyϑi)eβyϑi].

Regarding the model parameters δ,β, and ϑ, the partial derivatives of logl are obtained, respectively, as follows:

loglδ=2n(δ1)δ(δ1)ni=12[δ(1+βyϑi)eβyϑi],(27)

loglβ=2nβ(1+β)+ni=11(2+β+yϑi)ni=1yϑi+ni=12yϑieβyϑi{M}(yi,β,ϑ)[δ(1+βyϑi)eβyϑi],(28)

where, {M}(yi,β,ϑ)=[1β(1+β)3β(1+β)yϑi(1+β)3], and

loglϑ=nϑ+ni=1yϑilnyi(2+β+yϑi)ni=1βyϑilnyi2ni=1yϑlnyieβyϑ[β(1+βyϑ)β][δ(1+βyϑi)eβyϑi].(29)

The non-linear Eqs. (27)(29) are equated with zero to obtain the ML estimates (MLEs) ˆδ,ˆβ, and ˆϑ. As seen, it is difficult to formulate easily, making it challenging to solve them directly for the vector parameter ω=(δ,β,ϑ)T. Consequently, iterative techniques are used, such as the Newton-Raphson to get MLEs ˆδ,ˆβ, and ˆϑ.

Instead of determining point estimates for the unknown parameters, it would be more helpful to identify a range of values that, with a specified probability, encompass them. These ranges are referred to as interval estimates. To build the parameters CIs, the asymptotic distribution of MLE of ω=(δ,β,ϑ)T will be used, that is

(ˆω_ω_)DN3(0,I1(ˆω_)),

where ˆω is the MLE of ω and I1(ω) is the inverse of the observed information matrix of ω, and it is given by

I1(ˆω)=(2loglδ22loglδβ2loglδϑ2loglβ22loglβϑ2loglϑ2)1ˆω=(ˆδ,ˆβ,ˆϑ)=(ˆσ211ˆσ212ˆσ213ˆσ222ˆσ223ˆσ233).

Asymptotic normality of the MLEs allows for the construction of the 100(1φ)% asymptotic CIs of and for δ,β, and ϑ, respectively.

ˆδ±zφ/2ˆσ11,ˆβ±zφ/2ˆσ22,ˆϑ±zφ/2ˆσ33,

where is the upper φ/2th percentile point of the standard normal distribution.

6  Simulation

This section presents a simulation study to assess the performance of MLEs for the HTPXLD parameters (ϑ,δ,β). The R package is utilized to compute the mean, relative bias (RBias), bias, mean squared error (MSE), root mean squared error (RMSE), average interval length (AIL) of 95%, and coverage probability (CP) of 95% for the estimated values of ϑ, δ, and β. The simulation process is outlined as follows:

1)   Generate 5000 random samples from the HTPXLD with sizes n = 50, 100, 150, 200, 250, 300, 350, and 400.

2)   Choose parameter values for the simulations as follows: set1 = (ϑ = 0.8, δ = 1.5, β = 0.7), set2 = (ϑ = 0.5, δ = 1.5, β = 0.7), set3 = (ϑ = 0.5, δ = 1.2, β = 0.3), set4 = (ϑ = 0.7, δ = 1.6, β = 0.4), set5 = (ϑ = 1.1, δ = 1.9, β = 0.7), and set6 = (ϑ = 0.4, δ = 1.7, β = 0.9).

3)   Compute the MLEs, RBiases, Biases, RMSEs, and MSEs for each sample size and parameter set. Additionally, calculate the AIL and CP at a 95% confidence level for all sample sizes and parameter sets.

4)   Present the numerical results in Tables 68. The performance of the estimated parameters is analyzed based on complete samples.

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The results show in Tables 68 that bias, MSE, and RMSE all significantly decrease with increasing sample size (n). Furthermore, higher sample sizes increase CP and AIL, producing more accurate and trustworthy estimates and confidence ranges.

•   Greater sample sizes lead to improvements in MSE. As the sample size increases, the parameter estimates converge closer to the real values, indicating that the MLEs are becoming more exact, as indicated by lower MSE values.

•   As the sample size grows, the CP gets better, indicating that the CIs created for the parameter estimates get more trustworthy. The robustness of the estimates is improved by higher CP values, which indicate a higher probability that the intervals include the genuine parameter values.

•   As the sample size grows, the values of AIL become lower.

7  Applications

This section demonstrates the applicability of the HTPXLD in fitting real-world data by evaluating it against three actual datasets. The HTPXLD is compared with several alternative models, including XLD [1], Lindley (LD) [51], exponentiated generalized XLD (EGXLD) [52], power exponentiated LD (PELD) [53], Kumaraswamy LD (KLD) [54], Weibull power LD (WPLD) [15], exponentiated generalized power LD (EGLD) [55], power LD (PLD) [56], Weibull LD (WLD) [57], extended LD (EXLD) [58], and PXLD.

We use nine well-established goodness-of-fit measures to compare these models, including the Kolmogorov-Smirnov (6) statistic, its p-value (7), Anderson-Darling statistics (10), its p-value (11), the Hannan-Quinn Information Criterion (5), Akaike Information Criterion (2), Bayesian Information Criterion (3), Consistent 2 (4), Cramér-von Mises statistic (8), and its p-value (9). The optimal model is identified based on the highest values for 7, 11, and 9, and the lowest values for 6, 10, 8, 5, 2, 4, and 3.

7.1 The First Dataset

The first dataset consists of repair times for an airborne communication transceiver, provided by [59]. The recorded times are: 0.50, 0.60, 0.60, 0.70, 0.70, 0.70, 0.80, 0.80, 1.00, 1.00, 1.00, 1.00, 1.10, 1.30, 1.50, 1.50, 1.50, 1.50, 2.00, 2.00, 2.20, 2.50, 2.70, 3.00, 3.00, 3.30, 4.00, 4.00, 4.50, 4.70, 5.00, 5.40, 5.40, 7.00, 7.50, 8.80, 9.00, 10.20, 22.00, 24.50. Table 9 displays the results of the descriptive analysis for this dataset.

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For the first dataset, Table 10 presents the MLEs along with their standard errors (SEs). Table 11 provides the numerical values for the 6 statistic, its 7, 10, its 11, 8, its 9, as well as the 2, 3, 4, and 5 statistics. Fig. 3 includes the histogram, violin plot, QQ (quantile-quantile) plot, box plot with strip chart, and TTT (total time in test) plot. The estimated PDFs of competing models for the first dataset are shown in Fig. 4, while Fig. 5 displays the estimated CDFs of the competitive models. Additionally, Fig. 6 illustrates the PP plots of the competing models. Figs. 46 demonstrate the fit of our distribution to the actual data.

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Figure 3: Some basic non-parametric plots for the first dataset

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Figure 4: Estimated PDFs for the competing models for the first dataset

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Figure 5: Estimated CDFs for the competing models for the first dataset

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Figure 6: PP plots of competing models for the first dataset

7.2 The Second Dataset

The data set provided by [60] shows the monthly remission periods of 128 individuals with bladder cancer who were selected at random. the data set that we work with is 0.08, 2.09, 3.48, 4.87, 6.94, 8.66, 13.11, 23.63, 0.2, 2.23, 3.52, 4.98, 6.97, 9.02, 13.29, 0.4, 2.26, 3.57, 5.06, 7.09, 9.22, 13.8, 25.74, 0.5, 2.46, 3.64, 5.09, 7.26, 9.47, 14.24, 25.82, 0.51, 2.54, 3.7, 5.17, 7.28, 9.74, 14.76, 6.31, 0.81, 2.62, 3.82, 5.32, 7.32, 10.06, 14.77, 32.15, 2.64, 3.88, 5.32, 7.39, 10.34, 14.83, 34.26, 0.9, 2.69, 4.18, 5.34, 7.59, 10.66, 15.96, 36.66, 1.05, 2.69, 4.23, 5.41, 7.62, 10.75, 16.62, 43.01, 1.19, 2.75, 4.26, 5.41, 7.63, 17.12, 46.12, 1.26, 2.83, 4.33, 5.49, 7.66, 11.25, 17.14, 79.05, 1.35, 2.87, 5.62, 7.87, 11.64, 17.36, 1.4, 3.02, 4.34, 5.71, 7.93, 11.79, 18.1, 1.46, 4.4, 5.85, 8.26, 11.98, 19.13, 1.76, 3.25, 4.5, 6.25, 8.37, 12.02, 2.02, 3.31, 4.51, 6.54, 8.53, 12.03, 20.28, 2.02, 3.36, 6.76, 12.07, 21.73, 2.07, 3.36, 6.93, 8.65, 12.63, 22.69.

Table 12 displays the results of the descriptive analysis for this dataset.

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For the second dataset, Table 13 presents the MLEs along with their SEs. Table 14 provides the numerical values for the 6 statistic, its 7, 10, its 11, 8, its 9, as well as the 2, 3, 4, and 5 statistics. Fig. 7 includes the histogram, violin plot, QQ plot, box plot with strip chart, and TTT plot. The estimated PDFs of competing models for the second dataset are shown in Fig. 8, while Fig. 9 displays the estimated CDFs of the competitive models. Additionally, Fig. 10 illustrates the PP plots of the competing models. Figs. 810 demonstrated the fit of our distribution to the actual data.

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Figure 7: Some basic non-parametric plots for the second dataset

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Figure 8: Estimated PDFs for the competing models for the second dataset

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Figure 9: Estimated CDFs for the competing models for the second dataset

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Figure 10: Estimated CDFs for the competing models for the second dataset

7.3 The Third Dataset

The third data set represents values for the inflation rate in several countries that were recorded in June 2024. The term “inflation rate” describes how prices for products and services vary over time. The electronic address from which it was taken is as follows: https://tradingeconomics.com/ (accessed on 07 February 2025). The data set is reported in Table 15. Table 16 displays the results of the descriptive analysis for this dataset.

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For the third dataset, Table 17 presents the MLEs along with their SEs. Table 18 provides the numerical values for the 6 statistic, its 7, 10, its 11, 8, its 9, as well as the 2, 3, 4, and 5 statistics. Fig. 11 includes the histogram, violin plot, QQ plot, box plot with strip chart, and TTT plot. The estimated PDFs of competing models for the third dataset are shown in Fig. 12, while Fig. 13 displays the estimated CDFs of the competitive models. Additionally, Fig. 14 illustrates the PP plots of the competing models. Figs. 1214 demonstrate the fit of our distribution to the actual data.

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Figure 11: Some basic non-parametric plots for the third dataset

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Figure 12: Estimated PDFs for the competing models for the third dataset

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Figure 13: Estimated CDFs for the competing models for the third dataset

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Figure 14: PP plots of competing models for the third dataset

From the numerical values in Tables 11, 14, and 18 the HTPXLD is better than XLD, LD, EGXLD, PELD, KLD, WPLD, EGLD, PLD, WLD, EXLD, and PXLD for the three datasets.

The actuarial measures VaR, TVaR, TV, and TVP of the HTPXLD, PXLD, PLD, EGXLD, WLD, KLD, EXLD, and WPLD are computed and compared using the third data set in the following. Tables 19 and 20 present the numerical findings.

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We find that for different significance levels q and different values of ω, the HTPXLD model has greater values of the risk measures VaR, TVaR, TV, and TVP from Tables 19 and 20 and the Figs. 15 and 16. This suggests that compared to the PXLD, PLD, EGXLD, WLD, KLD, EXLD, and WPLD, the HTPXLD has a heavier tail.

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Figure 15: Competing model VaR, TVaR, and TV plots for the third dataset

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Figure 16: Competing model TVP plots for the third dataset

8  Conclusion

In the applied sciences, modeling heavy-tailed datasets is an important task, especially in domains like finance, medicine, and actuarial analysis. This paper constructs a novel heavy-tailed distribution by combining the PXLD with a heavy-tailed family. Especially when modeling leptokurtic lifespan data, that is, data with thicker tails this novel distribution presents a strongly modified version of the PXLD. With asymmetric forms and different degrees of peakedness, our suggested density gives more versatility, and its hazard rate function has various shapes. We delve into its statistical properties, deriving the quantile function, moments, incomplete moments, stochastic ordering, SS reliability parameter, and some extropy measures. We employ the ML procedure to estimate the model parameters. To assess the effectiveness of our proposed estimators, we conduct various simulation experiments. These experiments will evaluate the estimator’s performance using metrics like an average estimate, relative bias, bias, mean squared error, root mean squared error, average interval length, and coverage probability. We employ our suggested model to examine three real-world datasets to demonstrate its usefulness. The simulation analysis provided evidence that MLEs exhibit improved accuracy with increasing sample size. This is supported by the observed decrease in MSE, which is consistent with the theoretical expectation of parameter estimates converging toward their true values as the sample size grows. As sample numbers rise, the CP of the approximate CIs improves. As a result, we can be more certain that the actual parameter values fall inside the stated confidence intervals. Next, we evaluate its effectiveness in comparison to well-known rival models, emphasizing its benefits. A limitation of this study lies in its exclusive reliance on deriving point and interval estimates using the maximum likelihood method in the case of a complete sample. The simulation analysis presented in this work focuses specifically on scenarios with large sample sizes. Future studies should examine how well the HTPXLD performs in more realistic settings, such as those requiring ranked set sampling. Future studies should examine the HTPXLD’s performance on a larger variety of datasets with a range of attributes to fully evaluate its adaptability.

Acknowledgement: The authors thank King Saud University, Riyadh, Saudi Arabia for Supporting this research by Project Number (RSPD2025R548).

Funding Statement: This research is supported by researchers Supporting Project Number (RSPD2025R548), King Saud University, Riyadh, Saudi Arabia.

Author Contributions: Mohammed Elgarhy: Writing—original draft, Validation, Methodology, Formal analysis, Conceptualization, Writing—review, Investigation. Amal S. Hassan: Writing—original draft, Validation, Methodology, Formal analysis, Conceptualization, Writing—review, Investigation. Najwan Alsadat: Writing—original draft, Validation, Methodology, Formal analysis, Conceptualization, Writing—review, Investigation. Oluwafemi Samson Balogun: Writing—original draft, Validation, Methodology, Formal analysis, Conceptualization, Writing—review, Investigation. Ahmed W. Shawki: Writing—original draft, Validation, Methodology, Formal analysis, Conceptualization, Writing—review, Investigation. Ibrahim E. Ragab: Writing—original draft, Validation, Methodology, Formal analysis, Conceptualization, Writing—review, Investigation. All authors reviewed the results and approved the final version of the manuscript.

Availability of Data and Materials: All data generated or analyzed during this study are included in this published article.

Ethics Approval: Not applicable.

Conflicts of Interest: The authors declare no conflicts of interest to report regarding the present study.

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Cite This Article

APA Style
Elgarhy, M., Hassan, A.S., Alsadat, N., Balogun, O.S., Shawki, A.W. et al. (2025). A Heavy Tailed Model Based on Power XLindley Distribution with Actuarial Data Applications. Computer Modeling in Engineering & Sciences, 142(3), 2547–2583. https://doi.org/10.32604/cmes.2025.058362
Vancouver Style
Elgarhy M, Hassan AS, Alsadat N, Balogun OS, Shawki AW, Ragab IE. A Heavy Tailed Model Based on Power XLindley Distribution with Actuarial Data Applications. Comput Model Eng Sci. 2025;142(3):2547–2583. https://doi.org/10.32604/cmes.2025.058362
IEEE Style
M. Elgarhy, A. S. Hassan, N. Alsadat, O. S. Balogun, A. W. Shawki, and I. E. Ragab, “A Heavy Tailed Model Based on Power XLindley Distribution with Actuarial Data Applications,” Comput. Model. Eng. Sci., vol. 142, no. 3, pp. 2547–2583, 2025. https://doi.org/10.32604/cmes.2025.058362


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