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Article

The Generalized Exponential Extended Exponentiated Family of Distributions: Theory, Properties, and Applications

1
Department of Statistics, The Islamia University of Bahawalpur, Bahawalpur 63100, Pakistan
2
Department of Computer Science, The Islamia University of Bahawalpur, Bahawalpur 63100, Pakistan
3
Department of Statistics, Stockholm University, SE-106 91 Stockholm, Sweden
*
Author to whom correspondence should be addressed.
Mathematics 2022, 10(19), 3419; https://doi.org/10.3390/math10193419
Submission received: 8 August 2022 / Revised: 12 September 2022 / Accepted: 16 September 2022 / Published: 20 September 2022

Abstract

:
Here, we propose a new generalized exponential extended exponentiated (NGE3) family of distributions. Some statistical properties of proposed family are gained. The most extreme probability method, maximum likelihood (ML), is utilized for parameter estimation. We explore an exceptional model called NGE3-Exponential (NGE3E). NGE3E is estimated with ML, and the performance of estimators is demonstrated by utilizing a simulation. Moreover, two applications are given to show the significance and adaptability of the proposed model in comparison to some generalized models (GMs).

1. Introduction

We propose a generalized and univariate family of distributions (FoDs) with an exponential random variable (r.v.). Exponential distribution (ED) is a popular continuous probability model that has most extensively been applied in various fields as a life testing model (Lemonte, 2013) [1]. The popularity of ED may be due to the simplicity of its cumulative distribution function (cdf). In addition, the failure rate function (FRF) of ED has a constant shape. Several contemporary classes of distributions have been developed over the last couple of years grounded in the straightforward ED to submit lifetime models that can oblige useful applications where FRFs are decreasing, increasing, bathtub (BT), and upside-down BT (UDBT) shapes since ED does not give a reasonable fit in such circumstances. To increase the flexibility of ED, Adamidis and Loukas (1998) attempted exponential geometric (EG) distribution with decreasing FRF [2]; Gupta and Kundu (2001), the exponentiated ED as extension of the ED that can fit data with decreasing and increasing FRFs [3]; Gupta and Kundu (1999) [4], the generalized ED (GED) having three parameters as an appropriate substitute to the log normal, Weibull, and gamma distributions with increasing and decreasing FRFs. Gupta and Kundu (2007) [5], the GED has a shape of falling, rising, and constant FRFs, so it has not had the ability to fit in with data that have the nonmonotonous failure shape of the UDBT and BT. For more details on the applications and extensions of the exponential distribution, we refer to Balakrishnan (2019) [6] and Johnson et al. (2019) [7]. See also Hussain et al. (2022) [8] and Martínez-Flórez et al. (2020) [9].
Furthermore, for continuous distributions, Alzaatreh et al. (2013) [10] presented the idea of transformed–transformer (T–X) FoDs (TXFoDs). Let v ( z ) be the probability density function (pdf) of r.v. Z, where Z [ a 1 , a 2 ] , a 1 < a 2 < , and let U [ F ( x ) ] ⤏ be the F ( x ) of r.v., X, satisfying the constrains specified below:
1.
U [ F ( x ) ] [ a 1 , a 2 ] , is differentiable and increases monotonically.
2.
U [ F ( x ) ] a 1 as x a 2 as x +
The cdf of TXFoDs is
G ( x ) = a 1 U [ F ( x ) ] v ( z ) d z , x R ,
The corresponding pdf of (1) is
g ( x ) = v U [ F ( x ) ] x U [ F ( x ) ] .
Taking the idea from (1), we developed new flexible FoDs called a new generalized exponential extended exponentiated-G (NGE3-G) family (NGE3GF). Let r.v. Z follow the ED with scale parameter λ > 0 and cdf as
V ( z ) = 1 e λ z , z 0 ,
The pdf related to (3) is
v ( z ) = λ e λ z , z > 0 .
Setting U [ F ( x ) ] = log θ ¯ + θ F ¯ ( x ; ξ ) a 1 log F ¯ ( x ; ξ ) a in (1), when v ( z ) ∼ (4), we define the cdf of NGE3GF as
G ( x ; θ , a , λ , ξ ) = λ 0 log θ ¯ + θ F ¯ ( x ; ξ ) a 1 log F ¯ ( x ; ξ ) a e λ z d z , = 1 θ ¯ + θ F ¯ ( x ; ξ ) a 1 log F ¯ ( x ; ξ ) a λ , θ , a , λ > 0 , x R .
where θ ¯ = 1 θ , F ¯ ( x ; ξ ) a = 1 F ( x ; ξ ) a and F ( x ; ξ ) or we can simply write F ( x ) is baseline (BL) cdf of parameter ξ .
The main motivation for (5) follows from NGE3GF succeeding in fitting lifetime data as a competitive model (CM) to widely applied classes.
NGE3GF has a pdf as follows:
g ( x ; θ , a , λ , ξ ) = a λ f ( x ; ξ ) F ( x ; ξ ) a 1 F ¯ ( x ; ξ ) a { θ ¯ + θ F ¯ ( x ; ξ ) a } λ 1 { 1 log F ¯ ( x ; ξ ) a } λ + 1 × [ θ F ¯ ( x ; ξ ) a { 1 log F ¯ ( x ; ξ ) a } + { θ ¯ + θ F ¯ ( x ; ξ ) a } ] .
The paper is organized as follows. We characterize the NGE3GF with its reliability analysis and a convenient linear representation of the pdf and cdf in Section 1. In Section 2, several of its statistical properties are determined. NGE3GF parameters are estimated in Section 3. In Section 4, a special model viz. NGE3-Exponential distribution is discussed. A simulation study, the estimation of the parameters, and empirical illustrations through two datasets of the proposed model are also provided in Section 4. Lastly, the conclusion presented in Section 5.

1.1. Reliability Analysis

If an r.v. X NGE3-G ( θ , a , λ , ξ ) with Density (6), reliability analysis including (i) reliability function (RF) S ( x ) , (ii) failure rate function (FRF) h ( x ) , (iii) cumulative FRF H ( x ) , and (iv) reversed FRF τ ( x ) of X is given below.
S ( x ; θ , a , λ , ξ ) = { [ θ ¯ + θ F ¯ ( x ) a ] [ 1 log F ¯ ( x ) a ] 1 } λ ,
h ( x ; θ , a , λ , ξ ) = a λ f ( x ) F ( x ) a 1 [ θ { θ ¯ + θ F ¯ ( x ) a } 1 + { F ¯ ( x ) a [ 1 log F ¯ ( x ) a ] } 1 ] ,
H ( x ; θ , a , λ , ξ ) = λ [ log { θ ¯ + θ F ¯ ( x ) a } log { 1 log F ¯ ( x ) a } ] ,
and
τ ( x ; θ , a , λ , ξ ) = a λ f ( x ) F ( x ) a 1 [ θ F ¯ ( x ) a { θ ¯ + θ F ¯ ( x ) a } λ 1 + { 1 log F ¯ ( x ) a } 1 { θ ¯ + θ F ¯ ( x ) a } λ ] F ¯ ( x ) a [ { 1 log F ¯ ( x ) a } λ { θ ¯ + θ F ¯ ( x ) a } λ ] .

1.2. Useful Expansion of the NGE3-G Family

In this subsection, we present a useful expansion to the pdf and cdf of NGE3GF. Using (6), we obtain
g ( x ; θ , a , λ , ξ ) = a λ θ f ( x ) F ( x ) a 1 { 1 θ F ( x ) a } λ 1 { 1 log [ 1 F ( x ) a ] } λ + a λ f ( x ) F ( x ) a 1 [ 1 F ( x ) a ] 1 { 1 θ F ( x ) a } λ × { 1 log [ 1 F ( x ) a ] } ( λ + 1 ) ,
Using the binomial series (BS),
( 1 Z ) β = i = 0 ( 1 ) i β i Z i ,
By applying (12) in (11), we obtain
g ( x ; θ , a , λ , ξ ) = i = 0 ( 1 ) i θ i + 1 a λ λ 1 i f ( x ) F ( x ) a ( i + 1 ) 1 { 1 log [ 1 F ( x ) a ] } λ + i = 0 ( 1 ) i θ i a λ λ i f ( x ) F ( x ) a ( i + 1 ) 1 [ 1 F ( x ) a ] 1 { 1 log [ 1 F ( x ) a ] } ( λ + 1 ) ,
By applying the generalized BS (GBS)
( 1 Z ) β = j = 0 β + j 1 j Z j ,
where a real number β : | β | > 0 . By applying (14) in (13) the pdf becomes
g ( x ; θ , a , λ , ξ ) = i = 0 ( 1 ) i θ i + 1 a λ λ 1 i f ( x ) F ( x ) a ( i + 1 ) 1 { 1 log [ 1 F ( x ) a ] } λ + i , j = 0 ( 1 ) i θ i a λ λ i f ( x ) F ( x ) a ( i + j + 1 ) 1 { 1 log [ 1 F ( x ) a ] } ( λ + 1 ) ,
Again using the GBS (14) in (15), it becomes
g ( x ; θ , a , λ , ξ ) = i , k = 0 ( 1 ) i + k θ i + 1 a λ λ 1 i λ + k 1 k f ( x ) F ( x ) a ( i + 1 ) 1 × [ log [ 1 F ( x ) a ] ] k + i , j , k = 0 ( 1 ) i + k θ i a λ λ i λ + k k f ( x ) F ( x ) a ( i + j + 1 ) 1 × [ log [ 1 F ( x ) a ] ] k ,
Every real parameter A ( 0 , 1 ) and c tend to prove that
[ log ( 1 A ) ] c = A c + c l = 0 p l ( c + l ) A l + c + 1 ,
where p l ( c ) are Stirling polynomials. The demonstration of (17) is provided in Flajonet and Odlyzko (1990) [11], and Flajonet and Sedgewich (2009) [12]. Here, polynomials p l ( w ) are utilized as per Nielson (1906) [13] and Ward (1934) [14].
By applying (17) to (16), the pdf becomes
g ( x ; θ , a , λ , ξ ) = i , k = 0 ( 1 ) i + k θ i + 1 a λ λ 1 i λ + k 1 k f ( x ) [ F ( x ) a ( i + k + 1 ) 1 + k l = 0 p l ( k + l ) F ( x ) a ( i + k + l + 2 ) 1 ] + i , j , k = 0 ( 1 ) i + k θ i a λ λ i λ + k k × f ( x ) F ( x ) a ( i + j + k + 1 ) 1 + k l = 0 p l ( k + l ) F ( x ) a ( i + j + k + l + 2 ) 1 ,
By using the concept of power series,
Z β = m = 0 n = m ( 1 ) n + m β n n m Z m ,
Applying (19) in (18), the pdf can be written as
g ( x ; θ , a , λ , ξ ) = m = 0 η m f ( x ) F ( x ) m ,
where
η m = i , k , n = 0 ( 1 ) i + k + n + m a λ θ i + 1 n m λ 1 i λ + k 1 k [ a ( i + k + 1 ) 1 n + k l = 0 p l ( k + l ) a ( i + k + l + 2 ) 1 n ] + i , j , k , n = 0 ( 1 ) i + k + n + m a λ θ i n m λ i × λ + k k a ( i + j + k + 1 ) 1 n + k l = 0 p l ( k + l ) a ( i + j + k + l + 2 ) 1 n ,
From (20), we can extract another form of the pdf that provides infinite linear combinations:
g ( x ) = m = 0 W m h m + 1 ( x ) .
where m + 1 is a power parameter, W m = η m m + 1 , and h m + 1 ( x ) = ( m + 1 ) f ( x ) F ( x ) m is the density of exponentiated-G (Exp-G).
Further, the expansion of [ G ( x ; θ , a , λ , ξ ) ] h is derived, and “h” is an integer. By applying (12) to (5), we obtain
[ G ( x ; θ , a , λ , ξ ) ] h = i , j = 0 ( 1 ) i + j θ j h i λ i j F ( x ) a j { 1 log [ 1 F ( x ) a ] } λ i ,
Again, by applying (14) and (17) to (21), (21) becomes
[ G ( x ; θ , a , λ , ξ ) ] h = i , j , k = 0 ( 1 ) i + j + k θ j λ i + k 1 k λ i j h i F ( x ) a ( j + k ) + k l = 0 p l ( k + l ) F ( x ) a ( j + k + l + 1 ) ,
By using (19), [ G ( x ; θ , a , λ , ξ ) ] h becomes
[ G ( x ; θ , a , λ , ξ ) ] h = m 1 = 0 S m 1 F ( x ) m 1 ,
where
S m 1 = n 1 , k , j , i = 0 ( 1 ) n 1 + m 1 + k + j + i θ j h i n 1 m 1 λ i + k 1 k λ i j a ( j + k ) n 1 + k l = 0 p l ( k + l ) a ( j + k + l + 1 ) n 1 ,
From (23), we can extract another form
[ G ( x ) ] h = m 1 = 0 S m 1 H m 1 ( x ) .
where H m 1 ( x ) = F ( x ) m 1 specifies the cdf of the Exp-G ( m 1 ) family.

2. Statistical Properties of NGE3-G Family (NGE3GF)

Here, we derive some statistical properties of NGE3GF: quantile function, skewness and kurtosis, probability weighted moments, ordinary moments, moment generating function, the mean deviation, order statistics, and Renyi entropy.

2.1. Quantile Function (QF)

Let X∼ pdf (6) be the QF; Q ( u ) of X is below as
Q ( u ) = F 1 1 ( 1 u ) 1 λ θ W θ ( 1 u ) 1 λ exp ( 1 ( 1 u ) 1 λ 1 θ ( 1 u ) 1 λ ) 1 a .
Maple (2016) [15] was used to obtain (25), where 0 < u < 1 , F 1 ( . ) is the inverse function of F ( . ) , and W ( . ) denotes the Lambert W function (LWF). The LWF for every complex T is the solution of equation g ( T ) = T e T . Setting u = 0.75 , 0.50 , and 0.25 , we obtained the third, the second, and the first quartiles for X, respectively. These are shown below:
Q ( 3 4 ) = F 1 1 0 . 25 1 λ θ W θ 0 . 25 1 λ exp ( 1 0 . 25 1 λ ( 1 θ 0 . 25 1 λ ) ) 1 a ,
Q ( 1 2 ) = F 1 1 0 . 50 1 λ θ W θ 0 . 50 1 λ exp ( 1 0 . 50 1 λ ( 1 θ 0 . 50 1 λ ) ) 1 a ,
Q ( 1 4 ) = F 1 1 0 . 75 1 λ θ W θ 0 . 75 1 λ exp ( 1 0 . 75 1 λ ( 1 θ 0 . 75 1 λ ) ) 1 a .

2.2. Skewness and Kurtosis

Skewness and kurtosis investigate variability in a dataset, and classical measures can be susceptible to outliers. Given the QF, (25), the Moor’s kurtosis (Moors, 1998) [16] octile dependent is given as follows.
M K = Q 7 8 Q 1 8 Q 5 8 + Q 3 8 Q 6 8 Q 2 8 ,
Quartile-dependent Bowley’s skewness measures (Kenney and Keeping, 1962) [17] are given as follows.
B S K = 2 Q 2 4 Q 1 4 Q 3 4 Q 1 4 Q 3 4 .

2.3. Probability Weighted Moments (PWMs)

The PWMs of X can be determined by expression as follows.
τ r , s = E [ X r G ( x ; θ , a , λ , ξ ) s ] = x r g ( x ; θ , a , λ , ξ ) [ G ( x ; θ , a , λ , ξ ) ] s d x ,
By replacing h with s, and substituting (20) and (23) into (28), we obtained the PWMs of the NGE3-G family as follows.
τ r , s = m , m 1 = 0 η m S m 1 x r f ( x ) [ F ( x ) ] m + m 1 d x ,
Then,
τ r , s = m , m 1 = 0 η m S m 1 τ r , m + m 1 ,
where
τ r , m + m 1 = x r f ( x ) [ F ( x ) ] m + m 1 d x .

2.4. Moments

In statistical analysis and real data applications, moments of a probability distribution perform a significant role. Therefore, an rth moment expression for the NGE3GF is acquired. Assuming that X follows (20), the rth moment is
μ r = x r g ( x ; θ , a , λ , ξ ) d x , = m = 0 η m τ r , m .
where τ r , m = x r f ( x ) [ F ( x ) ] m d x is the PWMs of BL distribution (BLD).

2.5. Moment Generating Function (mgf)

Using (29), the mgf of X that follows the NGE3-G family is
M X ( t ) = E ( e t x ) = r = 0 t r r ! μ r = r = 0 m = 0 t r r ! η m τ r , m .

2.6. Mean Deviation (MD)

The MD of the NGE3-G family regarding the mean and median for r.v. X with pdf (20) g ( x ; θ , a , λ , ξ ) , cdf (5) G ( x ; θ , a , λ , ξ ) , are defined as
Δ 1 = 2 G ( μ 1 ) μ 1 2 T ( μ 1 ) , Δ 2 = μ 1 2 T ( M ) .
respectively, where μ 1 = m = 0 η m τ 1 , m from (29), M = Q ( 1 2 ) from (25), and T ( q ) = q x g ( x ; θ , a , λ , ξ ) d x , the 1st incomplete moment.

2.7. Order Statistics (OS)

If X follows the NGE3-G family, and X 1 , n < X 2 , n < < X n , n is a set of ordered r.v. of size n, according to Smith et al. (2007) [18], the pdf of rth OS is
g X ( r ) ( x ( r ) , θ , a , λ , ξ ) = g ( x ( r ) , θ , a , λ , ξ ) B ( r , n r + 1 ) u = 0 n r ( 1 ) u n r u G ( x ( r ) , θ , a , λ , ξ ) u + r 1 ,
Replacing h with u + r 1 , and by placing (20) and (23) in (32), we obtain the pdf of the rth OS for NGE3GF as below:
g X ( r ) ( x ( r ) , θ , a , λ , ξ ) = 1 B ( r , n r + 1 ) m = 0 η m f ( x ( r ) ) F ( x ( r ) ) m u = 0 n r ( 1 ) u n r u m 1 = 0 S m 1 F ( x ( r ) ) m 1 ,
After simplifying, we obtain
g X ( r ) ( x ( r ) , θ , a , λ , ξ ) = f ( x ( r ) ) B ( r , n r + 1 ) m , m 1 = 0 u = 0 n r η m ρ m 1 , u F ( x ( r ) ) m + m 1 .
where ρ m 1 , u = ( 1 ) u S m 1 n r u .
Further, for the NGE3-G family, the kth moment of the rth OS is
E ( X ( r ) k ) = x ( r ) k g ( x ( r ) , θ , a , λ , ξ ) d x ( r ) ,
Putting (33) into (34) leads to
E ( X ( r ) k ) = 1 B ( r , n r + 1 ) m , m 1 = 0 u = 0 n r ρ m 1 , u η m τ k , m + m 1 .
where
τ k , m + m 1 = x ( r ) k f ( x ( r ) ) F ( x ( r ) ) m + m 1 d x ( r ) .

2.8. Renyi Entropy (RE)

To measure variation in uncertainty in various fields such as finance, economics, electronics, engineering, and physics, entropy is used. Renyi (1961) [19] described that entropy as follows.
I Δ ( X ) = 1 1 Δ log g ( x ; θ , a , λ , ξ ) Δ d x , Δ > 0 a n d Δ 1 ,
To obtain g ( x ; θ , a , λ , ξ ) Δ , we apply binomial theory (12) and (14), Stirling polynomials (17), and the concept of power series (19) in (6). Then, the pdf can be communicated as
g ( x ; θ , a , λ , ξ ) Δ = n 1 = 0 t n 1 f ( x ) Δ F ( x ) m ,
where
t n 1 = n 2 , l , k , j , i = 0 ( 1 ) n 2 + n 1 + k + j + i ( a λ ) Δ θ i + j Δ i Δ λ i j i Δ k i Δ ( λ + 1 ) l n 2 n 1 × a ( Δ + j + k + l ) Δ n 2 + l m = 0 p m ( l + m ) a ( Δ + j + k + m + l + 1 ) Δ n 2 ,
Therefore, the RE of NGE3-G family of distributions is
I Δ ( X ) = 1 1 Δ log n 1 = 0 t n 1 f ( x ) Δ F ( x ) m d x .

3. Maximum Likelihood (ML) Method

Here, NGE3GF is estimated by utilizing the ML method. Given that X 1 , X 2 , , X n are observed values from NGE3GF, log-likelihood function (LLF), L ( Θ ) for parameter vector Θ = ( θ , a , λ , ξ ) T has form
L = L ( Θ ) = n log ( a λ ) + i = 1 n log f ( x i ) + ( a 1 ) i = 1 n log F ( x i ) i = 1 n log [ 1 F ( x i ) a ] + ( λ 1 ) i = 1 n log [ 1 θ F ( x i ) a ] ( λ + 1 ) i = 1 n log [ 1 log { 1 F ( x i ) a } ] + i = 1 n log [ θ { 1 F ( x i ) a } { 1 log [ 1 F ( x i ) a ] } + { 1 θ F ( x i ) a } ] .
By maximizing (40), we can obtain ML estimates (MLEs) Θ ^ of Θ . The elements of the score function (SFn) with respect to θ , a , λ and ξ are
L θ = ( 1 λ ) i = 1 n F ( x i ) a θ ¯ + θ F ¯ ( x i ) a + i = 1 n F ¯ ( x i ) a [ 1 log F ¯ ( x i ) a ] F ( x i ) a θ F ¯ ( x i ) a [ 1 log F ¯ ( x i ) a ] + [ θ ¯ + θ F ¯ ( x i ) a ] ,
L a = n a + i = 1 n log F ( x i ) + i = 1 n F ( x i ) a log F ( x i ) F ¯ ( x i ) a θ ( λ 1 ) i = 1 n log F ( x i ) F ( x i ) a θ ¯ + θ F ¯ ( x i ) a ( λ + 1 ) i = 1 n F ( x i ) a log F ( x i ) [ 1 log F ¯ ( x i ) a ] F ¯ ( x i ) a i = 1 n θ F ( x i ) a [ 1 log F ¯ ( x i ) a ] log F ( x i ) θ F ¯ ( x i ) a [ 1 log F ¯ ( x i ) a ] + [ θ ¯ + θ F ¯ ( x i ) a ] ,
L λ = n λ + i = 1 n log [ θ ¯ + θ F ¯ ( x i ) a ] i = 1 n log [ 1 log F ¯ ( x i ) a ] ,
L ξ = i = 1 n f i ξ f ( x i ) + ( a 1 ) i = 1 n F i ξ F ( x i ) + a i = 1 n F i ξ F ( x i ) a 1 F ¯ ( x i ) a + ( 1 λ ) a θ i = 1 n F ( x i ) a 1 F i ξ θ ¯ + θ F ¯ ( x i ) a a ( λ + 1 ) i = 1 n F i ξ F ( x i ) a 1 [ 1 log F ¯ ( x i ) a ] F ¯ ( x i ) a a θ i = 1 n [ 1 log F ¯ ( x i ) a ] F ( x i ) a 1 F i ξ θ F ¯ ( x i ) a [ 1 log F ¯ ( x i ) a ] + [ θ ¯ + θ F ¯ ( x i ) a ] .
where f i ξ = f ( x i ; ξ ) ξ and F i ξ = F ( x i ; ξ ) ξ are p length column vectors, of ξ .
Setting SFn elements to zero gives the set of normal equations (NEs). Analytically obtaining solutions for the set of NEs is tedious, but in the R language [20], the solutions are obtained numerically through iterative Newton–Raphson algorithms (NRAs).
Let J ( Θ ) = { J i j } ( p + 3 ) × ( p + 3 ) be the matrix of observed information (for i , j = θ , a , λ , ξ ), whose elements can be obtained numerically. By utilizing the estimated distribution of multivariate normal N p + 3 ( 0 , J ( Θ ) 1 ) regarding Θ ^ , we can develop approximate confidence bounds and testing hypotheses for model parameters.

4. NGE3-Exponential Distribution (NGE3ED)

We presently characterize NGE3ED by considering the exponential as a BLD with cdf F ( x ; γ ) = 1 exp ( γ x ) and pdf f ( x ; γ ) = γ exp ( γ x ) . Then, cdf and pdf of NGE3ED are, respectively,
G N G E 3 E ( x ) = 1 1 θ 1 exp ( γ x ) a 1 log 1 1 exp ( γ x ) a λ ,
and
g N G E 3 E ( x ) = a λ γ exp ( γ x ) 1 θ 1 exp ( γ x ) a λ 1 1 exp ( γ x ) a 1 1 log 1 1 exp ( γ x ) a λ + 1 1 1 exp ( γ x ) a × [ θ 1 1 exp ( γ x ) a 1 log 1 1 exp ( γ x ) a + 1 θ 1 exp ( γ x ) a ] ,
Henceforth, an r.v. X NGE3E ( θ , a , λ , γ ) with density (46). The FRF of X has the form
h ( x ) = a λ γ exp ( γ x ) 1 exp ( γ x ) a 1 [ θ 1 θ 1 exp ( γ x ) a + 1 { 1 log 1 1 exp ( γ x ) a } { 1 1 exp ( γ x ) a } ] .

4.1. Relationship among Submodels of NGE3ED

The pdf (46) contains some new distributions. The special submodels of the NGE3E model are listed below.
1.
For λ = 1 , the NGE3E ( θ , a , λ , γ ) model reduces to new generalized extended exponentiated exponential NGE2E ( θ , a , γ ) model.
2.
For a = 1 , the NGE3E ( θ , a , λ , γ ) model reduces to new generalized exponential extended exponential model NGEEE ( θ , λ , γ ).
3.
For a = 1 , λ = 1 , the NGE3E ( θ , a , λ , γ ) model reduces to new generalized extended exponential model NGEE ( θ , γ ).
4.
For a = 1 , λ = 1 , θ = 1 , the NGE3E ( θ , a , λ , γ ) model reduces to new generalized exponential model NGE-1 ( γ ).
5.
For θ = 0 , a = 1 , λ = 1 , the NGE3E ( θ , a , λ , γ ) model reduces to the NGE-2 model ( γ ).
The relationships among the above models are presented in Figure 1. For some selected parameter values, pdf and FRF plots for NGE3ED are shown in Figure 2 and Figure 3.

4.2. Quantile Function and Simulation Study

If X NGE3ED ( θ , a , λ , γ ) has cdf (45), G N G E 3 E ( x ; θ , a , λ , γ ) , the QF of X is
x p = 1 γ log 1 1 ( 1 p ) 1 λ θ W θ ( 1 p ) 1 λ exp ( 1 ( 1 p ) 1 λ [ 1 θ ( 1 p ) 1 λ ] ) 1 a .
where p ( 0 , 1 ) , and W ( . ) the LWF.
Here, we give a Monte Carlo simulation study (MCSS) to assess the performance and accuracy of MLEs of NGE3ED parameters. The simulation study was performed with generation observations from parameter scenarios (I) a = 4.10 , λ = 2.99 , θ = 2.11 , γ = 0.21 , and (II): a = 3.30 , λ = 4.88 , θ = 1.52 , γ = 0.31 .
The number of MCSS replications was N = 10,000 with sample sizes n = 50, 300, 550, 800, 1050, 1300, 1550, 1800, 2050. We used the optim ( ) R-function for maximizing the LLF of a probabilistic model. We examined the performance of MLEs for model “NGE3E” (a specific case of family) by computing the (i) average estimates (AEs), (ii) mean square errors (MSEs), and (iii) absolute biases (ABs).
B i a s ( Θ ^ ) = i = 1 10 , 000 Θ ^ i 10 , 000 Θ ,
and
M S E ( Θ ^ ) = 1 10 , 000 i = 1 10 , 000 ( Θ ^ i Θ ) 2 .
The numerical and graphical results of MCSS are presented in Table 1 and Figure 4, Figure 5 and Figure 6. According to expectations, under the theory of first-order asymptotics, the MSEs and ABs decreased when n increased for Scenarios I and II. In this manner, the MLEs of NGE3ED parameters performed well.

4.3. Estimation

Let a sample of size n be x 1 , x 2 , , x n from NGE3ED that has apdf in (46). The LLF for Θ = ( θ , a , λ , γ ) T is
L = L ( θ , a , λ , γ ) = n log ( a γ λ ) γ i = 1 n x i + ( a 1 ) i = 1 n log [ 1 exp ( γ x i ) ] i = 1 n log [ 1 1 exp ( γ x i ) a ] + ( λ 1 ) i = 1 n log [ 1 θ 1 exp ( γ x i ) a ] ( λ + 1 ) i = 1 n log [ 1 log { 1 1 exp ( γ x i ) a } ] + i = 1 n log [ θ { 1 1 exp ( γ x i ) a } { 1 log [ 1 1 exp ( γ x i ) a ] } + { 1 θ 1 exp ( γ x i ) a } ] .
The LLF given in (49) can be maximized by utilizing the AdequacyModel package to obtain the MLEs of Θ . The components of the score function regarding θ , a , λ and γ are
L θ = ( 1 λ ) i = 1 n 1 exp ( γ x i ) a 1 θ 1 exp ( γ x i ) a + i = 1 n { 1 1 exp ( γ x i ) a } { 1 log [ 1 1 exp ( γ x i ) a ] } 1 exp ( γ x i ) a θ { 1 1 exp ( γ x i ) a } { 1 log [ 1 1 exp ( γ x i ) a ] } + { 1 θ 1 exp ( γ x i ) a } ,
L a = n a + i = 1 n log [ 1 exp ( γ x i ) ] + i = 1 n 1 exp ( γ x i ) a log [ 1 exp ( γ x i ) ] 1 1 exp ( γ x i ) a θ ( λ 1 ) × i = 1 n 1 exp ( γ x i ) a log [ 1 exp ( γ x i ) ] 1 θ 1 exp ( γ x i ) a ( λ + 1 ) i = 1 n 1 exp ( γ x i ) a log [ 1 exp ( γ x i ) ] { 1 log [ 1 1 exp ( γ x i ) a ] } { 1 1 exp ( γ x i ) a } i = 1 n θ 1 exp ( γ x i ) a { 1 log [ 1 1 exp ( γ x i ) a ] } log [ 1 exp ( γ x i ) ] θ { 1 1 exp ( γ x i ) a } { 1 log [ 1 1 exp ( γ x i ) a ] } + { 1 θ 1 exp ( γ x i ) a } ,
L λ = n λ + i = 1 n log [ 1 θ 1 exp ( γ x i ) a ] i = 1 n log [ 1 log [ 1 1 exp ( γ x i ) a ] ] ,
L γ = n γ i = 1 n x i + ( a 1 ) i = 1 n x i exp ( γ x i ) 1 exp ( γ x i ) + a i = 1 n x i 1 exp ( γ x i ) a 1 exp ( γ x i ) 1 1 exp ( γ x i ) a + a ( 1 λ ) θ × i = 1 n 1 exp ( γ x i ) a 1 x i exp ( γ x i ) 1 θ 1 exp ( γ x i ) a a ( 1 + λ ) i = 1 n x i exp ( γ x i ) 1 exp ( γ x i ) a 1 { 1 log [ 1 1 exp ( γ x i ) a ] } { 1 1 exp ( γ x i ) a } a θ i = 1 n x i { 1 log [ 1 1 exp ( γ x i ) a ] } 1 exp ( γ x i ) a 1 exp ( γ x i ) θ { 1 1 exp ( γ x i ) a } { 1 log [ 1 1 exp ( γ x i ) a ] } + { 1 θ 1 exp ( γ x i ) a } .
Setting
L θ = 0 ,
L a = 0 ,
L λ = 0 ,
L γ = 0 .
The MLEs Θ ^ of Θ can be acquired by tackling NEs (54)–(57). These NEs cannot be tackled analytically, and to obtain the estimates numerically, a statistical package can be utilized. We can utilize iterative methods, for example, NRAs to obtain Θ ^ by utilizing a wide range of initial values.

4.4. Empirical Illustrations of the NGE3E Model

In this section, we match NGE3ED with some prominent generalized distributions. To illustrate the capability of NGE3ED, we analyze two real datasets. We compare the NGE3E model with the Weibull exponential (WE) (Oguntunde et al., 2015) [21], exponentiated WE (EWE) (Elgarhy et al., 2017) [22], exponentiated exponential Weibull (EEW) (Al Sulami, 2020) [23], beta exponential Fréchet (BEF) (Mead et al., 2017) [24], odd generalized exponential (OGE) Weibull (OGEW), OGE Fréchet (OGEFr) (Tahir et al., 2015) [25], exponentiated Kumaraswamy exponential (EKE) (Rodrigues and Silva, 2015) [26], Kumaraswamy weibull (KwW) (Cordeiro et al. 2010) [27], and Weibull Lomax (WL) (Tahir et al., 2014) [28] models through real-life datasets that are depicted below.

4.4.1. Dataset 1: Guinea Pig (GP) Data

From Bjerkedal (1960) [29], the survival time in days was taken from the dataset, consisting of 72 GPs infected with virulent tubercle bacilli. The observations are below:
0.100.330.440.560.590.720.740.770.920.93
0.961.01.01.021.051.077.00.081.081.081.09
1.121.131.151.161.201.211.221.221.241.301.34
1.361.391.441.461.531.591.601.631.631.681.71
1.721.761.831.951.961.972.022.132.152.162.22
2.302.312.402.452.512.532.542.542.782.933.27
3.423.473.614.024.324.585.55

4.4.2. Dataset 2: Bladder Cancer (BC) Data

As reported by Ademola (2021) [30], a random sample, in months, of the remission times of 128 BC patients. The observations are as follows:
0.082.0922.6912.633.484.878.656.936.948.66
3.362.0713.1123.6321.7312.070.202.236.763.363.52
4.982.0220.286.979.0212.038.5313.290.406.544.51
2.263.573.312.025.067.099.2212.0213.808.3725.74
6.250.504.502.463.253.461.765.0919.137.2611.98
9.478.2614.245.8525.824.400.511.462.5418.103.70
11.795.177.937.285.719.744.3414.763.0226.311.40
0.814.3317.362.8311.641.267.8746.125.6217.122.87
7.631.3579.055.4117.144.2611.252.757.661.195.49
43.0110.6616.627.595.344.1810.757.622.695.410.90
4.2334.262.6914.831.0510.3436.667.3915.965.323.88
2.6432.1514.7710.067.325.323.822.62
The descriptive statistics (DSs) for the GP and BC datasets are presented in Table 2, and their box plots are shown in Figure 7a and Figure 8a, which demonstrate that distribution was skewed to the right. TTT plot of GP data displayed in Figure 7b reveal that the FRF was concave, suggesting an increasing failure rate shape, while the TTT plot of BC data in Figure 8b moved from concave to convex, giving an indication of UDBT-shaped failure rate. Accordingly, the NGE3E model could be suitable for fitting these datasets.
The pdfs of CMs are as follows:
  • The EWE distribution
    g ( x ; a , α , β , λ ) = a α β λ exp ( λ x ) 1 β 1 e α exp ( λ x ) 1 β λ x 1 e α exp ( λ x ) 1 β a 1 ; x > 0 , a , α , β , λ > 0 .
  • WE distribution:
    g ( x ; λ , β , α ) = λ β α 1 exp ( λ x ) β 1 exp ( α ( exp ( λ x ) 1 ) β + λ β x ) ; x > 0 , λ , β , α > 0 .
  • EEW distribution:
    g ( x ; λ , α , γ , β ) = λ α γ β γ x γ 1 exp ( λ β γ x γ ) 1 exp ( λ β γ x γ ) α 1 ; x > 0 , λ , α , γ , β > 0 .
  • BEF distribution:
    g ( x ; α , β , λ , γ , θ ) = γ λ θ γ B ( α , β ) x ( 1 + γ ) exp ( θ γ x γ ) 1 exp ( θ γ x γ ) λ β 1 1 1 exp ( θ γ x γ ) λ α 1 ; x > 0 , θ , γ , λ , β , α > 0 .
  • OGEW distribution:
    g ( x ; λ , α , θ , β ) = α λ β θ x β 1 exp λ λ exp ( θ x β ) exp ( θ x β ) 1 exp λ λ exp ( θ x β ) α 1 ; x > 0 , α , β , θ , λ > 0 .
  • OGEFr distribution:
    g ( x ; θ , α , β , λ ) = λ α β θ β x ( β + 1 ) e ( θ x ) β 1 e ( θ x ) β 2 exp λ e ( θ x ) β 1 e ( θ x ) β 1 exp λ e ( θ x ) β 1 e ( θ x ) β α 1 ; x > 0 , θ , α , β , λ > 0 .
  • EKE distribution:
    g ( x ; β , λ , θ , α ) = θ λ β α 1 e α x β 1 e α x 1 1 e α x β λ 1 1 1 ( 1 e α x ) β λ θ 1 ; x > 0 , λ , β , θ , α > 0 .
  • KwW distribution:
    g ( x ; γ , a , α , β ) = γ a α β x a 1 e γ x a 1 e γ x a α 1 1 1 e γ x a α β 1 ; x > 0 , γ , a , α , β > 0 .
  • WL distribution:
    g ( x ; a , β , γ , α ) = a β γ α 1 + γ x α ( β 1 ) 1 1 + γ x α β 1 exp a 1 + γ x α 1 β ; x > 0 , a , β , γ , α > 0 .
During the comparative analysis of the models, the AdequacyModel package of R was utilized to compute the application results. We adopted well-known goodness-of-fit measures (GFMs) such as L ^ where L ^ , is the maximized LLF, the Akaike information criterion (IC) (AIC), consistent AIC (CAIC), Bayesian IC (BIC), Cramer–von Mises (CM), Anderson–Darling (AD), and Kolmogorov–Smirnov (KS) statistics. In general, the model is the best fit with lower GFM values and a high p-value of the KS statistic.
MLEs with standard errors (SEs) for NGE3ED and CMs (EWE, WE, EEW, BEF, OGEW, OGEFr, EKE, KwW and WL) fitted to the guinea-pig and bladder-cancer datasets are listed in Table 3 and Table 4. The values of GFMs in Table 5 and Table 6 indicate that the NGE3E model gave small values of -L, AIC, CAIC, BIC, KS, CM, and AD, and a higher corresponding p-value. Hence, it showed a relatively better data fit than that of the CMs. Further, plots in Figure 9 and Figure 10 also support this conclusion.

5. Conclusions

In this paper, the NGE3GF of distributions was characterized and examined. Various properties of this family were obtained, and special model of NGE3-Exponential (NGE3E) distribution was studied. Using popular GFM testing statistics, we compared NGE3ED with well-known GMs. NGE3ED provided better estimates with minimal GFMs and a high p value. On the basis of graphical and numerical analysis, the NGE3E distribution outclassed that of well-established CMs. We hope that NGE3GF will be able to attract researchers.
As future work, this study can be extended through a Bayesian technique to estimate the parameters of the different models derived from this proposed family. Moreover, other datasets in different areas can be used to check the flexibility of the derived models. This work can also be extended for bivariate Exponential Extended Exponentiated G-family of Distributions.

Author Contributions

Conceptualization, S.H., M.U.H. and R.A.; Data curation, M.S.R.; Investigation, S.H., M.U.H. and R.A.; Methodology, S.H., M.S.R., M.U.H. and R.A.; Software, M.U.H.; Validation, M.S.R.; Visualization, S.H.; Writing—original draft, S.H., M.S.R. and M.U.H.; Writing—review & editing, R.A. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Data Availability Statement

The data are fully available in the article and the mentioned reference.

Acknowledgments

The authors are thankful to the reviewers for their valuable corrections and suggestions that improved the article.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. Relationship among submodels of the NGE3ED.
Figure 1. Relationship among submodels of the NGE3ED.
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Figure 2. Pdf plots of NGE3ED.
Figure 2. Pdf plots of NGE3ED.
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Figure 3. FRF plots of NGE3ED.
Figure 3. FRF plots of NGE3ED.
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Figure 4. MLE plots of NGE3ED for Set I: a = 4.10 , λ = 2.99 , θ = 2.11 , γ = 0.21 and Set II: a = 3.30 , λ = 4.88 , θ = 1.52 , γ = 0.31 .
Figure 4. MLE plots of NGE3ED for Set I: a = 4.10 , λ = 2.99 , θ = 2.11 , γ = 0.21 and Set II: a = 3.30 , λ = 4.88 , θ = 1.52 , γ = 0.31 .
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Figure 5. Estimated MSE plots of NGE3ED in MCSS.
Figure 5. Estimated MSE plots of NGE3ED in MCSS.
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Figure 6. Estimated AB plots of NGE3ED in MCSS.
Figure 6. Estimated AB plots of NGE3ED in MCSS.
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Figure 7. (a) Box plot and (b) TTT plot for GP data.
Figure 7. (a) Box plot and (b) TTT plot for GP data.
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Figure 8. (a) Box plot (b) and TTT plot for BC data.
Figure 8. (a) Box plot (b) and TTT plot for BC data.
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Figure 9. Estimated (a) pdf, (b) cdf, (c) Kaplan–Meier (K-M), and (d) hazard rate for guinea-pig data.
Figure 9. Estimated (a) pdf, (b) cdf, (c) Kaplan–Meier (K-M), and (d) hazard rate for guinea-pig data.
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Figure 10. Estimated (a) pdf, (b) cdf, (c) Kaplan–Meier (K-M), (d) hazard rate for bladder-cancer data.
Figure 10. Estimated (a) pdf, (b) cdf, (c) Kaplan–Meier (K-M), (d) hazard rate for bladder-cancer data.
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Table 1. Simulation results for NGE3ED.
Table 1. Simulation results for NGE3ED.
Set I: a = 4.10 , λ = 2.99 , θ = 2.11 , γ = 0.21 Set II: a = 3.30 , λ = 4.88 , θ = 1.52 , γ = 0.31
nParameterMLEMSEABMLEMSEAB
50 a ^ 4.1780520.7132670.0780523.5667451.0418720.266745
λ ^ 2.6393182.2419140.3506823.6070514.0743131.272949
θ ^ 2.9961422.8929540.8861422.5429164.6629881.022916
γ ^ 0.2229990.0072900.0129990.3834630.0421890.073464
300 a ^ 4.3228330.3808540.2228333.6252640.4609630.325264
λ ^ 2.7098521.5470250.2801483.4344034.5842521.445597
θ ^ 2.2431130.9181950.1331131.7034760.7131680.183476
γ ^ 0.2438760.0069060.0338760.4324560.0471540.122456
550 a ^ 4.2652270.2736290.1652273.5262550.2454410.226255
λ ^ 2.8524061.2605320.1375943.6942863.4337491.185714
θ ^ 2.1948560.5860330.0848561.6102120.3116430.090212
γ ^ 0.2333970.0047860.0233970.3981960.0267870.088196
800 a ^ 4.2385380.2178780.1385383.4714470.1566260.171447
λ ^ 2.8926691.0540430.0973313.8754552.7208221.004546
θ ^ 2.1680200.4318180.0580201.5818290.1809270.061829
γ ^ 0.2288800.0037380.0188800.3783630.0176200.068363
1050 a ^ 4.2110640.1702390.1110643.4464620.1132530.146462
λ ^ 2.9191160.8953490.0708843.9713392.3219430.908661
θ ^ 2.1570620.3344940.0470621.5586900.1196220.038690
γ ^ 0.2251600.0029680.0151600.3685240.0129580.058524
1300 a ^ 4.1974590.1402230.0974593.4163370.0842500.116337
λ ^ 2.9260140.7649600.0639864.0781041.9702760.801896
θ ^ 2.1413500.2577250.0313501.5644150.1010340.044415
γ ^ 0.2232260.0024440.0132260.3582110.0099420.048211
1550 a ^ 4.1725820.1163560.0725823.4079950.0717010.107995
λ ^ 2.9386820.6511320.0513184.1323921.7633640.747608
θ ^ 2.1505510.2272990.0405511.5530200.0805650.033020
γ ^ 0.2202650.0020230.0102650.3540000.0083160.044000
1800 a ^ 4.1745250.1049860.0745253.3919800.0567670.091980
λ ^ 2.9385280.5943110.0514724.2005791.5434660.679421
θ ^ 2.1362630.1987130.0262631.5479780.0657080.027978
γ ^ 0.2201220.0018310.0101220.3483730.0066570.038373
2050 a ^ 4.1648150.0925210.0648153.3821710.0490890.082171
λ ^ 2.9406500.5234060.0493504.2420651.4097280.637934
θ ^ 2.1387910.1750370.0287911.5500370.0590960.030037
γ ^ 0.2187640.0016100.0087640.3448380.0058180.034838
Table 2. DSs for Datasets 1 and 2.
Table 2. DSs for Datasets 1 and 2.
DatasetMin. Q 1 Median Q 3 Max.MeanVarianceSkewnessKurtosis
10.0801.0801.5602.3037.0001.8371.4781.7554.152
20.0803.3486.39511.83879.0509.366110.4253.28715.483
Table 3. MLEs with SE (in parentheses) of CMs for guinea-pig data.
Table 3. MLEs with SE (in parentheses) of CMs for guinea-pig data.
Dist. a ^ λ ^ θ ^ γ ^ α ^ β ^
NGE3E2.322725.563850.101870.31452
(0.49245)(7.00899)(1.27805)(0.18822)
EWE2.298550.0419921.895761.04688
(1.21005)(0.02975) (19.11364)(0.25627)
WE0.0328259.897891.54046
(0.04996) (162.26158)(0.16146)
EEW1.009061.156662.038441.33014
(31.52095) (0.27759)(0.99803)(35.93074)
BEF0.6507291.127590.4090313.596325.60806
(0.36349)(41.07691)(0.06542)(52.52073)(21.90342)
OGEW21.138240.039532.422301.02483
(38.08836)(0.08007) (1.41950)(0.32531)
OGEFr43.9576945.570000.681690.44654
(31.45097)(32.38208) (0.35684)(0.08105)
EKE16.656561.764290.080301.29005
(65.36980)(1.20989) (0.28969)(0.58900)
KwW0.864320.531772.731003.21403
(0.82088) (0.46183)(3.05683)(9.65113)
WL21.277630.705340.253532.19835
(55.95618) (0.84875)(0.22020)(0.54623)
Table 4. MLEs with SE (in parentheses) of CMs for bladder-cancer data.
Table 4. MLEs with SE (in parentheses) of CMs for bladder-cancer data.
Dist. a ^ λ ^ θ ^ γ ^ α ^ β ^
NGE3E1.469883.172800.041420.06681
(0.22276)(1.65586)(0.76421)(0.04233)
EWE4.037070.011717.072120.52346
(2.10918)(0.00599) (2.37210)(0.11822)
WE0.0069113.771300.98836
(0.00218) (5.32372)(0.06271)
EEW0.756440.654422.795982.18408
(41.90063) (0.13484)(1.26511)(184.93870)
BEF154.7273692.017020.05378153.632921.85484
(256.89845)(426.07475)(0.03714)(249.12744)(2.52944)
OGEW12.710150.048983.746160.53393
(16.73725)(0.07842) (1.99784)(0.15390)
OGEFr0.032610.023602.532620.67782
(0.03068)(0.02448) (1.01072)(0.12675)
EKE5.103153.890710.013870.48930
(3.05943)(3.16005) (0.00977)(0.23850)
KwW0.462550.493324.081362.87041
(0.39433) (0.42793)(4.52386)(6.00747)
WL14.275670.171420.174971.52178
(26.47401) (0.16655)(0.15495)(0.28860)
Table 5. GFMs of CMs for guinea-pig data.
Table 5. GFMs of CMs for guinea-pig data.
Dist.-LAICCAICBICKSp-ValueCMAD
NGE3E102.134212.267212.864221.3740.0950.540.083600.57473
EWE102.976213.952214.548223.0580.1010.45690.115190.75801
WE104.486214.972215.325221.8020.1190.26320.172741.04466
EEW102.810213.620214.217222.7260.1010.44990.110080.72722
BEF105.026220.052220.962231.4360.5210.00000.120840.76687
OGEW102.979213.959214.556223.0650.1020.44210.113610.75265
OGEFr105.679219.353219.950228.4600.1310.16740.153071.07003
EKE102.764213.528214.125222.6350.1000.47040.110840.72641
KwW102.710213.420214.017222.5260.1010.45590.107710.71078
WL102.781213.562214.159222.6680.1050.40450.112420.73235
Table 6. GFMs of CMs for bladder-cancer data.
Table 6. GFMs of CMs for bladder-cancer data.
Dist.-LAICCAICBICKSp-ValueCMAD
NGE3E409.823827.645827.971839.0530.0370.99540.021470.14416
EWE411.320830.641830.966842.0490.0480.92440.056580.37454
WE415.905837.811838.004846.3670.0800.38400.165410.98962
EEW410.680829.360829.685840.7680.0450.95760.043670.28848
BEF415.946841.892842.384856.1520.9870.00000.200201.48189
OGEW410.922829.844830.169841.2520.0470.94270.048450.32110
OGEFr410.838829.676830.001841.0840.0440.96130.047670.31411
EKE411.000830.000830.325841.4080.0460.94590.052220.33891
KwW410.569829.138829.464840.5460.0450.96000.041450.27310
WL410.165828.329828.655839.7370.0430.97210.032960.21647
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Hussain, S.; Sajid Rashid, M.; Ul Hassan, M.; Ahmed, R. The Generalized Exponential Extended Exponentiated Family of Distributions: Theory, Properties, and Applications. Mathematics 2022, 10, 3419. https://doi.org/10.3390/math10193419

AMA Style

Hussain S, Sajid Rashid M, Ul Hassan M, Ahmed R. The Generalized Exponential Extended Exponentiated Family of Distributions: Theory, Properties, and Applications. Mathematics. 2022; 10(19):3419. https://doi.org/10.3390/math10193419

Chicago/Turabian Style

Hussain, Sajid, Muhammad Sajid Rashid, Mahmood Ul Hassan, and Rashid Ahmed. 2022. "The Generalized Exponential Extended Exponentiated Family of Distributions: Theory, Properties, and Applications" Mathematics 10, no. 19: 3419. https://doi.org/10.3390/math10193419

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