EUROPEAN JOURNAL OF PURE AND APPLIED MATHEMATICS 2025, Vol. 18, Issue 4, Article Number 6653 ISSN 1307-5543 – ejpam.com Published by New York Business Global The Mgamma Distribution: Statistical Properties and Application to Real-Life Data M. I. Khan1, Molay Kumar Ruidas2,∗ 1 Department of Mathematics, Islamic University of Madinah, Madinah, Kingdom of Saudi Arabia, 42351 2 Department of Statistics, Trivenidevi Bhalotia College, Kazi Nazrul University, Raniganj, West Bengal, India, 713347 Abstract. We propose a new one-parameter continuous distribution, termed the Mgamma dis- tribution, obtained as a finite mixture of two Gamma components having different shapes. Key statistical properties are derived, including moments, generating functions, stochastic ordering, and reliability measures such as hazard rate and mean residual life. Parameter estimation is addressed using the method of moments and maximum likelihood, with simulation studies confirming the consistency and efficiency of estimators. The applicability of the Mgamma distribution is demon- strated on four real datasets from engineering, hydrology, medicine, and queueing systems. Model selection criteria (AIC, BIC, CAIC) and goodness-of-fit tests (KS, Cramér–von Mises, Anderson– Darling) consistently show that Mgamma provides a superior fit compared to classical models such as Exponential, Lindley, Xgamma, Shanker, and Akash distributions. These findings establish Mgamma as a flexible and robust alternative for modeling skewed and heavy-tailed lifetime data. 2020 Mathematics Subject Classifications: 60E05, 62E99 Key Words and Phrases: Finite mixture, Gamma distribution, maximum likelihood estimation, survival properties, stochastic ordering 1. Introduction In recent years, research has focused on developing continuous distributions that are more flexible in fitting real lifetime data sets. Some distributions that are finite mixtures of Gamma distributions introduced by Geoffrey et al. (1988) [1], mixture of Exponential and Gamma distributions introduced by Ghitany et al. (2008) [2] and Maiti et al. (2024) [3] used to model lifetime data. Recently, Sen et al. (2016) [4] introduced Xgamma, the Lindley distribution by DV Lindley (1958) [5], Shanker (2015) [6] introduced the Shanker distribution, Gamma-Lindley (Zeghdoudi and Nedjar, (2016) [7]) and several other mix- ture distributions are derived using the literature of Johnson, Kotz and Balakrishnan ∗Corresponding author. DOI: https://doi.org/10.29020/nybg.ejpam.v18i4.6653 Email addresses: khanizhar@iu.edu.sa (M. I. Khan), molayruidas@gmail.com (M. K. Ruidas) https://www.ejpam.com 1 Copyright: © 2025 The Author(s). (CC BY-NC 4.0) M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 2 of 22 (1994) [8] to fit real-life data. However, these distributions are not as sophisticated in modeling datasets more accurately. Various classical distributions are modified and ex- tended to find new distributions like extended Gamma introduced by Bakouch (2012) [9], two-parameter Xgamma Weibull by Yousof et al. (2021) [10], Exponentiated survival func- tion of Beta introduced by Mahmoud et al. (2024)[11], new beta power flexible Weibull (NBPF-Weibull) by Tang et al. (2024)[12], GE Weibull by kamal et al. (2023)[13] and extended Xgamma by Saha et al. (2019)[14], which serve the purpose of flexible data modelling. In this study, we introduce a new one-parameter continuous type of distribu- tion using a similar approach used by Messaadia and Zeghdoudi (2018) [15] but taking a different mixing probability. The rest of the paper is organized as follows. In Section 3, we define the probability density (pdf) and cumulative distribution (cdf) functions of the proposed distribution. Section 4 derives its statistical properties, including raw moments, mean deviation, mo- ment and cumulant generating functions, skewness, and kurtosis. The stochastic ordering that characterizes the structural behavior of the distribution is discussed in Section 5. Reliability properties, such as the hazard function and mean residual life, are presented in Section 7. Section 8 provides results for the order statistics. Parameter estimation meth- ods, including the method of moments and maximum likelihood estimation, are described in Section 9. A Monte Carlo simulation study investigating bias and mean square error of the estimators is given in Section 10. Applications of the proposed distribution to four real-life datasets are discussed in Section 11. Finally, Section 12 concludes the paper with a summary of findings and potential directions for future research. 2. Methodology The new distribution is a finite mixture of two Gamma distributions having differ- ent shape parameters with certain mixing probabilities. The form of the finite mixture distribution is given by g(x) = k∑ i=1 πig(xi). Let g1(x) ∼ Gamma(2, θ) and g2(x) ∼ Gamma(3, θ) and π1 = θ 1 + θ be the mixing probability, then g(x) is our desired probability distribution. Although the Mgamma distribution may be a particular form of one-parameter polynomial Exponential (OPPE) distribution introduced by Bouchahed and Zeghdoudi (2018) [16] taking r = 2 and a0 = 0, a1 = 1, a2 = 1/2, it is easy to use by non-statisticians due to its flexible model. Whereas for OPPE, it is difficult to determine which values of ai yield a good model, i.e., choice of ai’s are very difficult to estimate. Moreover, it is a general form, difficult for non- statisticians to use for modeling. Also, Bouchahed and Zeghdoudi (2018) did not test the bias and MSE, they only provided the formula. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 3 of 22 3. The Mgamma distribution Most of the one-parameter continuous distributions, such as Lindley, Shanker and Xgamma etc., are derived directly from simple transformations or mixtures of Exponential and Gamma with a single mixing scheme, whereas Mgamma is a finite mixture of two Gamma distributions with different shape parameters but a single scale parameter, which makes it different and richer than other classical distributions. A random variable X is said to have the Mgamma distribution with parameter θ if its pdf is defined as f(x) = θ3x ( 1 + x 2 ) e−θx 1 + θ ; x > 0, θ > 0 (1) 0 2 4 6 8 10 0.0 0.2 0.4 0.6 0.8 1.0 Plot of pdf of Mgamma distribution x f(x) θ = 0.5 θ = 0.8 θ = 1 θ = 3 θ = 5 Figure 1: p.d.f. plot of Mgamma distribution for different θ denoted by x ∼ M(θ), its cdf is given by F (x) = 1− [ 1 + θx 1 + θ ( 1 + θ + θx 2 )] e−θx; x > 0, θ > 0 (2) To find the mode of the distribution, we first differentiate equation (1), w. r. t θ d dx f(x; θ) = θ3 1 + θ [1 + x− θx(1 + x/2)] e−θx (3) We observe that for θ < 1 , (1− θ) + √ θ2 + 1 θ is the unique critical point for which f(x) is maximized. And for θ > 1 , f(x) is decreasing. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 4 of 22 0 2 4 6 8 10 0.0 0.2 0.4 0.6 0.8 1.0 Plot of cdf of Mgamma distribution x F(x ) θ = 0.5 θ = 0.8 θ = 1 θ = 3 θ = 5 Figure 2: c.d.f. plot of Mgamma distribution for different θ So, the mode(x) of the new distribution is given by mode(x) = (1− θ) + √ θ2 + 1 θ ; θ < 1 (4) Remark 1. From the above it is seen that mode(x) < median(x) < mean(x) which is same as in the Xgamma and Exponential distribution. We get value of mode for different values of θ 4. Moments and related measures Let x ∼ Mgamma(θ), then the kth raw moment is given by E(Xk) = ∫ ∞ 0 xk θ3x ( 1 + x 2 ) e−θx θ + 1 dx. = θ3 θ + 1 ∫ ∞ 0 xk+1 ( 1 + x 2 ) e−θx dx = θ3 θ + 1 [∫ ∞ 0 xk+1e−θx dx+ 1 2 ∫ ∞ 0 xk+2e−θx dx ] = θ3 θ + 1 [ Γ(k + 2) θk+2 + 1 2 Γ(k + 3) θk+3 ] = θ3 θ + 1 [ (k + 1)! θk+2 + 1 2 (k + 2)(k + 1)! θk+3 ] = θ3(k + 1)! θk+3(θ + 1) [ θ + k+2 2 ] M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 5 of 22 = (k + 1)! θk(θ + 1) ( θ + k + 2 2 ) . (5) Thus, the kth order raw moment is given by E(Xk) = (k + 1)! θk(θ + 1) ( θ + k 2 + 1 ) , θ > 0, k > −2. Therefore putting k = 1, 2, 3 and 4, we get the first, second, third and fourth order moments about the origin as: µ1 ′ = 3 + 2θ θ(1 + θ) = mean(x), µ2 ′ = 6(2 + θ) θ2(1 + θ) , µ3 ′ = 12(5 + 2θ) θ3(1 + θ) and µ4 ′ = 120(3 + θ) θ4(1 + θ) . The variance is given by µ2 = Var(X) = E(X2)− ( E(X) )2 = 6(θ + 2) θ2(θ + 1) − ( 2θ + 3 θ(θ + 1) )2 = 6(θ + 2) θ2(θ + 1) − (2θ + 3)2 θ2(θ + 1)2 = 6(θ + 2)(θ + 1) θ2(θ + 1)2 − (2θ + 3)2 θ2(θ + 1)2 = 6(θ + 2)(θ + 1)− (2θ + 3)2 θ2(θ + 1)2 = 6(θ2 + 3θ + 2)− (4θ2 + 12θ + 9) θ2(θ + 1)2 = 6θ2 + 18θ + 12− 4θ2 − 12θ − 9 θ2(θ + 1)2 = 2θ2 + 6θ + 3 θ2(θ + 1)2 . M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 6 of 22 µ3 = E(X3)− 3E(X)E(X2) + 2(E(X))3 = 12(2θ + 5) θ3(θ + 1) − 3 · 2θ + 3 θ(θ + 1) · 6(θ + 2) θ2(θ + 1) + 2 · (2θ + 3)3 θ3(θ + 1)3 = 12(2θ + 5)(θ + 1)2 − 18(2θ + 3)(θ + 2)(θ + 1) + 2(2θ + 3)3 θ3(θ + 1)3 = 2 ( 2θ3 + 9θ2 + 9θ + 3 ) θ3(θ + 1)3 µ4 = E(X4)− 4E(X3)E(X) + 6(E(X2)E(X))− 3E(X)4 = 24θ4 + 144θ3 + 252θ2 + 180θ + 45 θ4(1 + θ)4 Again, putting the value of (µ2) and (µ4) we get kurtosis (γ2) as, γ2 = µ4 µ2 2 = 24θ4 + 144θ3 + 252θ2 + 180θ + 45 θ4(θ + 1)4 (2θ2 + 6θ + 3)2 θ4(θ + 1)4 = 3(8θ4 + 48θ3 + 84θ2 + 60θ + 15) 4θ4 + 24θ3 + 48θ2 + 36θ + 9 = 24θ4 + 144θ3 + 252θ2 + 180θ + 45 (2θ2 + 6θ + 3)2 Figure 3: The graph of kurtosis for different θ M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 7 of 22 Now, putting the value of (µ2) and (µ3) we get the value of skewness (γ1) as , γ1 = µ3 µ 3/2 2 = 2 ( 2θ3+9θ2+9θ+3 ) θ3(θ+1)3 (2θ2+6θ+3)3/2 θ3(θ+1)3 = 2 ( 2θ3 + 9θ2 + 9θ + 3 ) (2θ2 + 6θ + 3)3/2 . Figure 4: The graph of skewness for different θ M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 8 of 22 From the Fig. 3 and Fig. 4 we can conclude the following observations, • As the numerator and denominator are positive for all θ > 0 in (γ1), so γ1 > 0 i.e. the distribution is right-skewed. • Again, for kurtosis, we found that (γ2 > 3), ∀θ > 0, so the distribution is leptokurtic (heavy-tailed, more peaked than normal). 4.1. Mean Deviation The mean deviation about mean of random variable X, having pdf in equation (1) is obtained as MDx̄ = E(|x− µ|) = ∫ ∞ 0 |x− µ|f(x)dx = ∫ µ 0 |µ− x|f(x)dx+ ∫ ∞ µ |x− µ|f(x)dx = 2µF (µ)− µ+ 2 ∫ ∞ µ xf(x)dx = 2µF (µ)− µ+ 1 θ(1 + θ) ( 2θ(θ2µ2 + 2θµ+ 2) + (θ3µ3 + 3θ2µ2 + 6θµ+ 6) ) e−θµ 4.2. Moment and Cumulant Generating Function It is also possible to express the moment generating function in terms of the moment MX(t) = E(etX) = ∫ ∞ 0 etx θ3x(1 + x 2 )e−θx 1 + θ  dx = θ3 1 + θ ∫ ∞ 0 x ( 1 + x 2 ) e−(θ−t)xdx = θ3 1 + θ (∫ ∞ 0 xe−(θ−t)xdx+ ∫ ∞ 0 x 2 e−(θ−t)x ) dx = θ3 1 + θ ( Γ2 (θ − t)2 + Γ2 2(θ − t)2 ) = θ3(1 + θ − t) (1 + θ)(θ − t)2 The cumulant generating function of the random variable X is given by kX(t) = logMX(t) M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 9 of 22 KX(t) = log ( θ3(1 + θ − t) (1 + θ)(θ − t)2 ) = 3 log θ + log(1 + θ − t)− log(1 + θ)− 2 log(θ − t) 5. Stochastic interpretation of the parameter θ Stochastic orders are important measures for comparing the behavior of random vari- ables shown by Shaked and Santikumar (1995) [17]) Let X and Y are the two random variables with cumulative distribution functions FX(.) and FY (.) respectively. Then X is said to be smaller than Y in the • Stochastic order (X ≺s Y ), ifFX(t) ≥ FY (t), ∀t • Convex order (X ≺cx Y ) if for all convex functions ϕ and provided expectation exist, E[ϕ(X) ≤ E[ϕ(Y )]. • Hazard rate order (X ≺hr Y ), ifhX(t) ≥ hY (t), ∀t. • Likelihood Ratio order (X ≺lr Y ), if fX(t) fY (t) is decreasing in t. Remark 2. Likelihood ratio order ⇒ Hazard rate order ⇒ Stochastic order if E[X] = E[Y] , then Convex order ⇐⇒ Stochastic order. Theorem 1. Let Xi ∼ M(θi), i = 1, 2 be two random variables. If θ1 ≤ θ2, thenX1 ≺lr X2, X1 ≺hr X2, X1 ≺s X2andX1 ≺cx X2 Proof. We have fX1(t) fX2(t) = θ31(1 + θ2) θ32(1 + θ1) e−(θ1−θ2)t differentiating w.r.t t, we get d dt fX1(t) fX2(t) = −(θ1 − θ2)e −(θ1−θ2)t < 0, ∀θ1 ≥ θ2 Hence, we see that fX1 (t) fX2 (t) decreases in t, which holds the above theorem. (proved) 6. Incomplete moments and Inequality curves The rth incomplete moment µr(t) for a random variable X with pdf f(x) and cdf F(x) is given by Sen et al. (2018) [18]) µr(t) = ∫ t 0 xrf(x)dx M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 10 of 22 So, when x ∼ Mgamma(θ), the rth incomplete moment is obtained as µr(t) = ∫ t 0 xr θ3x(1 + x 2 )e−θx 1 + θ  dx = θ3 1 + θ (∫ ∞ 0 xr+1e−θxdx+ ∫ ∞ 0 1 2 xr+2e−θxdx ) = θ3 1 + θ [ γ(r + 2, θt) + 1 2 γ(r + 3, θt) ] where γ(α, x) = ∫ x 0 uα−1e−u du is lower incomplete Gamma function. When a non-negative continuous random variable X has pdf f (x) and cdf F (x), the Lorenz and Bonferroni curves are defined by l(p) = 1 µ ∫ q 0 xf(x)dx B(p) = 1 pµ ∫ q 0 xf(x)dx respectively, where µ = E(X) and q = F 1(p) for 0 < p < 1. So, when x ∼ Mgamma(θ) the Lorenz and Bonferroni curves are given by l(p) = θ4 3 + θ [ γ(3, θq) + 1 2 γ(4, θq) ] B(p) = θ4 p(3 + θ) [ γ(3, θq) + 1 2 γ(4, θq) ] The Lorenz and Bonferroni curves confirm that Mgamma can capture income/wealth in- equality patterns due to its flexible tail behavior, offering better interpretability compared to simpler one-parameter models 7. Reliability Properties In reliability engineering, a batch of products may contain both weaker items (e.g., Gamma(2, θ)) and stronger items (long-lasting Gamma(3, θ)). Similarly, in the medical field, the patients’ survival times may be a mixture of fast progressors and slow progressors, etc. A mixture allows non-monotone hazard rates, which are often observed in practice but impossible with simple one-parameter models. So Mgamma distribution is very much suitable in this field with single- parameter and mixture distributions. The hazard rate of Mgamma distribution is h(x) = f(x) 1− F (x) M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 11 of 22 = θ3x(1 + x 2 )e−θx[ 1 + θx 1 + θ ( 1 + θ + θx 2 )] e−θx = θ3x ( 1 + x 2 ) [ 1 + θ + θx ( 1 + θ + θx 2 )] From Fig. 5, it is evident that unlike the Exponential and Lindley distributions, the hazard rate of the Mgamma distribution is non-monotone. (i) For small θ, h(x) is increasing. (ii) For moderate θ, h(x) shows a bathtub shape. (iii) For large θ, h(x) is monotone increasing like Lindley. 0 5 10 15 20 0 1 2 3 4 5 Hazard plot of Mgamma distribution x h(x ) θ = 0.8 θ = 1 θ = 3 θ = 0.5 Figure 5: Hazard plot of Mgamma distribution for different values of θ Mean remaining life For a continuous random variable X with pdf f(x) and cdf F (x), the mean residual life (mrl) function is defined as m(x) = E[(X − x)|X > x] M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 12 of 22 = 1 1− F (x) ∫ ∞ x [1− F (t)]dt = ∫∞ x F̄ (t)dt F̄ (x) Where, F̄ (t) = ( 1 + θt 1 + θ (1 + θ + θt 2 ) e−θt and, ∫ ∞ x F̄ (t)dt = 1 1 + θ ( (1 + θ)x+ 2(1 + θ) θ + x+ 1 θ + θx2 2 ) (6) For the Mgamma distribution the mrl function is given by m(x) = (1 + θ)x+ 2(1 + θ) θ + x+ 1 θ + θx2 2 1 + θ + θx(1 + θ + θx/2) Figure 6 shows mrl functions for different choices of θ. 0 2 4 6 8 10 0 1 2 3 4 5 Mean remaining life of Mgamma distribution x mr l(x) θ = 0.8 θ = 1 θ = 3 θ = 5 Figure 6: mrl plot of Mgamma distribution for different values of θ From the plot we found that (i) For x = 0, m(0) = µ = 2θ + 3 θ(1 + θ) which is the mean of Mgamma. (ii) The mrl(x) decreases with both x and θ, indicating that the expected remaining life becomes shorter. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 13 of 22 8. Order Statistics Let Y(1), Y(2), .., Y(n) be the ordered random sample drawn from the Mgamma Distri- bution, then the c.d.f. and p.d.f. of the rth order statistics is given by Gr(y) = n∑ i=r ( n i ) [G(y; θ;λ)]i [1−G(y; θ;λ)]n−i gr(y) = n! (r − 1)!(n− r)! [G(y; θ;λ)]r−1 [1−G(y; θ;λ)]n−r g(y; θ;λ) So, the p.d.f. and c.d.f. of y(1) and y(n) is given by gY1(y) = nθ3x(1 + x/2)e−θx 1 + θ [( 1 + θx 1 + θ (1 + θ + θx 2 ) ) e−θx ]n−1 gYn(y) = nθ3x(1 + x/2)e−θx 1 + θ [ 1− ( 1 + θx 1 + θ (1 + θ + θx 2 ) ) e−θx ]n−1 Gy1(y) = 1− [( 1 + θx 1 + θ (1 + θ + θx 2 ) ) e−θx ]n Gyn(y) = [ 1− ( 1 + θx 1 + θ (1 + θ + θx 2 ) ) e−θx ]n 9. Estimation of the parameters Here we discuss two estimation methods viz. (i) Method of moments and (ii) Methods of maximum likelihood estimation. 9.1. Method of moment Let x1, x2, x3, .., xn be a random sample of size n drawn from the equation (1). We compare the sample mean x̄ = 1 n ∑n i=1 xi with the first order raw moment µ1 ′ to get the mom estimator of θ as θmom = 1 2x̄ ( −x̄+ √ x̄2 + 8x̄+ 4 + 2 ) , x > 0 The method of moment estimator θmom is positively biased, consistent and asymptot- ically normal. For large sample the 100(1-α)% confidence interval of θ is given by θ ± Zα 2 √ 1 nσ2 M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 14 of 22 9.2. Maximum likelihood estimation Let X1, X2, ..., Xn be a random sample of size n drawn independently from the pdf 1. The maximum likelihood estimator (mle) of θ is given by L(θ|x1, x2, .., xn) = n∏ i=1 θ3xi(1 + xi/2)e −θxi 1 + θ The log likelihood equation is as follows L(θ|x) = 3nlog(θ)− nlog(1 + θ) + n∑ i log [xi(1 + xi/2)]− θ n∑ i xi (7) To have the maximum likelihood estimator of θ, we have to solve I(θ|x) = ∂L(θ|x) ∂θ = 0, Hence, we have 3n θ − n 1 + θ − n∑ i=1 xi = 0 Using Newton-Raphson iteration method, we find the θ̂mle for which the log-likelihood equation is maximized. The initial solution for the iteration method is θ0 = 2 x̄ . We continue the iteration process θ(i) = θ(i−1) − I(θ(i−1)|x) I ′(θ(i−1)|x) we stop when θ(i) ≡ θ(i−1). All computations were performed in the updated version of R software [19], following the procedures book [20]. The MLE is consistent and asymptot- ically normal under standard regularity conditions (iid samples, differentiability of likeli- hood). Convergence of Newton–Raphson is generally fast; in our simulation, it stabilized within 4–6 iterations. 10. Simulation Study To generate the random sample from Mgamma distribution, we proceed as follows: Let F (x) = p, where p follows uniform(0, 1). We choose the solution that lies in (0, 1). Here G(x) is the cdf of Mgamma random variable. Then, we follow the approach of generating sample from Mgamma distribution. Hence the algorithm is 1. Generate pi ∼ uniform(0, 1), i = 1, 2, . . . , n. 2. Generate Vi ∼ Gamma(2, θ), i = 1, 2, . . . , n. 3. Generate Wi ∼ Gamma(3, θ), i = 1, 2, . . . , n. 4. If Ui ≤ θ 1+θ , then set Xi = Vi. Otherwise, set Xi = Wi. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 15 of 22 We perform Monte Carlo simulation in R programming considering N=10000 times for different values of n=5, 10, 15 and 20 and θ=0.8, 1, 2 and 3 . The following two measures were computed 1. Average bias of the simulated estimates θ̂i, i = 1, 2, . . . , N : 1 N ∑N i=1(θ̂i − θ) 2. Average Mean Square Error (MSE) of the simulated estimates θ̂i, i = 1, 2, . . . , N : 1 N ∑N i=1(θ̂i − θ)2 Figure 7: mse plot of Mgamma distribution for different value of θ It is observed that both the MSE and bias decrease as the sample size increases and θ decreases. 11. Data Analysis In this section, we have compared our proposed model with the existing one-parameter distributions by fitting some real-life datasets. The first dataset is obtained from Smith and Naylor (1987) [21], which represents the strength of 1.5 cm glass fibres, measured at the National Physical laboratory, England. The second dataset is taken from Bakouch et. al (2021)[22] which concerns the ex- ceedances of flood peaks (in m3/s) of the Wheaton River near Carcross in Yukon Territory, Canada that consist of 72 exceedances for the years 1958–1984 and rounded to one decimal place. The third dataset is about the remission times (in weeks) for 20 leukaemia patients randomly assigned to a certain treatment taken from Al-Babtain et al. (2020) [23]. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 16 of 22 Figure 8: bias plot of Mgamma distribution for different value of θ The last dataset is obtained from Sharma et al. (2017) [24], which consists of the waiting time (in mins) before service for 100 bank customers. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 17 of 22 Fitting to strength of 1.5 cm glass fibres strength (in cms) fr e q u e n c y d e n s it y 0 10 20 30 40 50 60 70 0 .0 0 0 .0 2 0 .0 4 Exponential Xgamma Lindley Mgamma Shanker akash Fitting exceedence of flood peaks of the wheaton river flood peaks (in m^3/s) fr e q u e n c y d e n s it y 0 10 20 30 40 50 60 70 0 .0 0 0 .0 4 0 .0 8 Exponential Xgamma Lindley Mgamma Shanker akash Fitting of Remission times for 20 leukaemia patients times (in weeks) fr e q u e n c y d e n s it y 0 10 20 30 40 50 0 .0 0 0 .0 4 0 .0 8 Exponential Xgamma Lindley Mgamma Shanker akash Fitting waiting time before service of 100 bank customers time(in mins) fr e q u e n c y d e n s it y 0 10 20 30 40 0 .0 0 0 .0 4 0 .0 8 Exponential Xgamma Lindley Mgamma Shanker akash Figure 9: Histogram and Fitted densities for all the four datasets. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 18 of 22 0 200 400 600 100 200 300 400 Theoretical Quantiles (Mgamma) E m p ir ic a l Q u a n ti le s ( D a ta ) QQ Plot for Mgamma Distribution 0 20 40 60 0 10 20 30 Theoretical Quantiles (Mgamma) E m p ir ic a l Q u a n ti le s ( D a ta ) QQ Plot for Mgamma Distribution 0 10 20 30 40 50 10 20 30 40 50 Theoretical Quantiles (Mgamma) E m p ir ic a l Q u a n ti le s ( D a ta ) QQ Plot for Mgamma Distribution 0 10 20 30 40 0 10 20 30 Theoretical Quantiles (Mgamma) E m p ir ic a l Q u a n ti le s ( D a ta ) QQ Plot for Mgamma Distribution Figure 10: Q-Q plot for all the four datasets using Mgamma distribution accordingly. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 19 of 22 Table 1: Model comparison for Dataset I: Strength of 1.5 cm glass fibres Criteria Exponential Lindley Xgamma Shanker Akash Mgamma MLE 0.6636 0.9961 1.3376 0.9562 1.3554 1.8354 AIC 88.83 81.27 85.80 81.14 81.86 58.66 KS Statistic 0.4186 0.3862 0.4196 0.3661 0.3705 0.3361 Cramér–von Mises 3.862 3.332 3.881 3.113 3.192 2.496 Anderson–Darling 18.426 16.425 18.468 15.406 15.736 12.590 Table 2: Model comparison for Dataset II: Exceedances of flood peaks (Wheaton River) Criteria Exponential Lindley Xgamma Shanker Akash Mgamma MLE 0.8194 0.1530 0.2044 0.1646 0.2412 0.2422 AIC 252.120 264.228 266.470 279.790 291.070 251.648 KS Statistic 0.1421 0.2408 0.2562 0.2272 0.3030 0.1325 Cramér–von Mises 0.2319 0.8198 1.0660 0.7775 1.5190 0.1489 Anderson–Darling 1.4680 7.4400 8.8136 6.9887 19.100 1.4231 Table 3: Model comparison for Dataset III: Remission times of 20 leukaemia patients Criteria Exponential Lindley Xgamma Shanker Akash Mgamma MLE 0.0511 0.0977 0.1383 0.1019 0.1522 0.1521 AIC 79.459 78.872 79.398 79.244 81.790 78.746 KS Statistic 0.1143 0.1189 0.1589 0.1095 0.2007 0.0104 Cramér–von Mises 0.0660 0.0344 0.0725 0.0424 0.1366 0.0181 Anderson–Darling 0.410 0.2960 0.5644 0.3351 1.4800 0.2704 Table 4: Model comparison for Dataset IV: Waiting times of 100 bank customers Criteria Exponential Lindley Xgamma Shanker Akash Mgamma MLE 0.1012 0.1865 0.2634 0.1983 0.2952 0.2989 AIC 329.020 319.037 321.020 317.629 320.629 317.062 KS Statistic 0.1730 0.0676 0.0624 0.0881 0.1002 0.0601 Cramér–von Mises 0.7153 0.0581 0.0839 0.1280 0.2170 0.0535 Anderson–Darling 4.2280 0.4863 0.6447 0.9044 1.3797 0.0326 M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 20 of 22 From the table 1 - 4, we find that Mgamma provides the best fit, capturing the skewness and heavy tails of the data. Across all four datasets i.e. spanning engineering, hydrology, medical survival, and queueing contexts the Mgamma distribution consistently outper- formed the classical one-parameter models. The mixture structure of Mgamma allows it to model skewness and heavy-tailed behaviour more effectively. Also the model accommo- dates non-monotone hazard rates (e.g., bathtub-shaped or increasing-decreasing), which are common in practice but not captured by simpler distributions. Even with small sam- ples (as in the remission time data), Mgamma provides superior fit. In every dataset, Mgamma yielded the lowest AIC and other criteria, reinforcing its statistical adequacy. Thus, the Mgamma distribution can be considered a highly competitive and flexible alter- native for real-life data modelling, outperforming several classical and recently proposed lifetime distributions. It is well known that distributions with more parameters usually provide greater flexibility for data modeling. However, the presence of multiple parameters often makes estimation more complex and computationally demanding. In contrast, the proposed Mgamma distribution has the advantage of involving only a single parameter, which is straightforward to estimate, while still offering substantial flexibility. Notably, it provides a superior fit compared to several existing multi-parameter models. 12. Conclusion In this article, we introduced a new one-parameter continuous distribution, the so called Mgamma distribution, by a finite mixture approach of two Gamma distributions with different shape parameters. We studied several of its statistical properties including moments, moment and cumulant generating function, order statistics, mean deviation, incomplete moments and inequality curves. We generated random variables and studied their mean square error and bias and found that both decrease as the sample size increases. The estimation of model parameters is approached by the method of maximum likelihood and method of moments estimation. Two real-life data sets are analyzed using various model selection criteria. It is found that the new distribution provides a consistently better fit than the other probability models available in the literature. For future studies, this new distribution can be modified using a different technique to make it more flexible in data modelling, such as developing its pseudo form, considering the ratio of two random variables, introducing transmuted versions with an additional parameter, or exploring Bayesian estimation approaches. Data availability The data that support the findings of this study are available from the corresponding author upon reasonable request. Conflict of interest There is no conflict of interest. M. I. Khan, M. K. Ruidas / Eur. J. Pure Appl. Math, 18 (4) (2025), 6653 21 of 22 Acknowledgements The authors are grateful to the Deanship of Graduate Studies and Scientific Re- search, Islamic University of Madinah, Saudi Arabia, for the support provided to the Post-Publication Program (4). The authors also thank the unknown referees and editors Eyup Cetin and Baris Kiremitci for their valuable comments and suggestions to improve the quality of the article. References [1] Geoffrey J McLachlan and Kaye E Basford. Mixture models: Inference and applica- tions to clustering, volume 38. M. Dekker New York, 1988. [2] Mohamed E Ghitany, Barbra Atieh, and Saralees Nadarajah. Lindley distribution and its application. Mathematics and computers in simulation, 78(4):493–506, 2008. 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