
In order to address the problem of information overload, numerous solutions have been proposed, among which recommender systems stand out as one of the most effective. By reviewing and organizing existing literature both domestically and internationally, this paper evaluated personalized recommendations on the Internet across six dimensions: information layout, recommendation way, recommendation strength, recommendation precision, recommendation timeliness, and recommendation interactivity. Simultaneously, it considered the customer's mind-flow experience and perceived trust as mediating variables, and consumer purchasing intention as the dependent variable of the study. Furthermore, based on relevant theories, this paper constructed a corresponding research model to explore how personalized recommendations influence customers' intention to purchase by affecting their mind-flow experience and perceived trust through this model.
Citation: Xin Yun, Myung Hwan Chun. The impact of personalized recommendation on purchase intention under the background of big data[J]. Big Data and Information Analytics, 2024, 8: 80-108. doi: 10.3934/bdia.2024005
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In order to address the problem of information overload, numerous solutions have been proposed, among which recommender systems stand out as one of the most effective. By reviewing and organizing existing literature both domestically and internationally, this paper evaluated personalized recommendations on the Internet across six dimensions: information layout, recommendation way, recommendation strength, recommendation precision, recommendation timeliness, and recommendation interactivity. Simultaneously, it considered the customer's mind-flow experience and perceived trust as mediating variables, and consumer purchasing intention as the dependent variable of the study. Furthermore, based on relevant theories, this paper constructed a corresponding research model to explore how personalized recommendations influence customers' intention to purchase by affecting their mind-flow experience and perceived trust through this model.
Abbreviations | Symbols |
Probability density function | |
cdf | Cumulative distribution function |
NXLD | New X-Lindley distribution |
UNXLD | Unit new X-Lindley distribution |
mrl | Mean residual life |
sf | Survival function |
hrf | Hazard rate function |
LF(x) | Lorenz curve |
BF(x) | Bonferroni curve |
Gi(x) | Gini index |
J(X) | Extropy of X |
Re(δ) | Rényi entropy of X |
Te(λ) | Tsallis entropy of X |
HCe(β) | Havrda and Charvat entropy of X |
ML | Maximum likelihood |
LS | Least-squares |
WLS | Weighted least-squares |
MLE | ML estimate |
LSE | LS estimate |
MSE | Mean square error |
RMSE | Root mean square error |
AIC | Akaike information criterion |
AICc | Akaike information criterion corrected |
CAIC | Consistent Akaike information criterion |
BIC | Bayesian information criterion |
KS | Kolmogorov-Smirnov |
BD | Beta distribution |
TLD | Topp-Leone distribution |
KD | Kumaraswamy distribution |
ETLD | Exponentiated Topp-Leone distribution |
ULD | Unit Lindley distribution |
UBD | Unit Burr-Ⅲ distribution |
Quantile—quantile | |
P-P | Probability—probability |
TTT | Total test time |
The introduction of new distributions allows statisticians and researchers to better model a variety of data types, from symmetric to skewed, and from positive to bi-directional distributions. These distributions provide tools for understanding data variability, estimating parameters, making predictions, and conducting statistical hypothesis testing across diverse fields of study. For instance, percentages, proportions, and other quantities that have limits between 0 and 1 are better represented by bounded distributions. Overall, distributions with bounded support offer practical tools for accurately modeling a wide range of data types and phenomena, supplying information, enabling analysis, and supporting decision-making in a variety of sectors. In the scientific literature, bounded distributions are noticeably scarce compared to unbounded distributions, despite the ubiquity of actual scenarios with bounded data.
The beta distribution, renowned for its versatility and applicability, holds a distinct place in statistical modeling due to its ability to represent data with a range from 0 to 1. The beta distribution was revitalized when Karl Pearson identified it as a member of the Pearson distribution family, specifically as a Pearson Type Ⅰ distribution. While the beta distribution is a valuable tool, it's not a one-size-fits-all solution. As a result, there are more studies on unit modeling in the literature. The transformation of well-known continuous distributions has typically been used to introduce the newly proposed unit distributions. The benefit of these unit distributions is that they increase the basic distribution's flexibility throughout the unit interval without requiring the addition of new parameters. Such as, the Kumaraswamy Kumaraswamy distribution [1], the log-xgamma distribution [2], the one parameter unit-Lindley distribution [3], the unit-Gompertz distribution [4], the unit Weibull distribution [5], the unit Burr-Ⅲ distribution [6], the unit-Rayleigh distribution [7], the unit Burr-XII distribution [8], the unit half normal distribution [9], the exponentiated unit Lindley distribution [10], the unit Teissier distribution [11], the unit two parameters Mirra distribution [12] and the two parameters unit Muth distribution [13], etc.
The NXLD proposed by [14], which is obtained as a special case of the new one-parameter polynomial exponential distribution introduced by [15], is used as the baseline distribution in this article to introduce a new bounded distribution, namely the unit new X-Lindley distribution (UNXLD). Here, it is necessary to mention the NXLD. A continuous random variable (rv) X is said to have the NXLD with parameter θ>0 if its pdf is of the form:
f(x;θ)=θ(1+θx)e−θx2, x>0. | (1.1) |
The cdf of X is given by
F(x;θ)=1−(12θx+1)e−θx, x>0. |
The NXLD is important for its ability to model positive real data, [14] explored the NXLD's applicability in actuarial science by examining its actuarial properties. Due to its qualities, it is a useful tool for statistical analysis, research, and practical applications in a variety of fields. For numerous real-world datasets, the NXLD demonstrated its uniqueness when compared to other models. Moreover, the Lindley distribution has been applied in numerous fields, such as finance, environmental studies, and medical research. Its ability to handle various types of data makes it a valuable tool in statistical modeling. This NXLD offers a unique combination of features from both the Lindley and exponential distributions. These are the motivations for introducing the NXLD on the unit interval.
Numerous probability distributions are created in the literature by combining, expanding, and changing well-known distributions, which makes it possible to describe lifetime data with a more flexible hrf. The bathtub curve is an idealized representation that helps in understanding and modeling the behavior of systems. In the case of real-life datasets that vary over the positive real line, possess bathtub shaped hrf. [16,17,18] etc are examples of the same. In the latter case, it was demonstrated that the unit inverse Gaussian distribution and the logit Slash distribution both produce hrfs with a bathtub shape, as shown in [19] and [20], respectively. Due to the log function's inclusion in their density functions, these two distributions are more complex, and as a result, the cdf is not calculated in closed-form. As a result, modeling studies using these two distributions are quite challenging. Another one is the unit Burr-XII distribution [8], which has two parameters, and the Meijer G-function's presence in the formulation of its moments makes it slightly more difficult to understand the model's flexibility.
The Lambert-uniform distribution with only one-parameter, proposed by [21], faces complications in calculating associated properties due to the presence of the principal branch of the Lambert W function and the logarithm function in its pdf. The unit Muth distribution [13] is another two-parameter distribution. Similarly, the definition of moments comprises the gamma function, which causes complexity. The unit generalized half-normal distribution was recently presented by [22], although it lacks closed-form formulas for the cdf and quantile function. Less parameterized models are typically easier to comprehend and interpret. This facilitates understanding of the underlying relationships and implications of the model by researchers, analysts, and stakeholders.
These problems are improved by our newly defined UNXLD. It presents closed-form expression for cdf, hrf, and all its statistical measures, even when a logarithmic function is present in its pdf. More over, it possesses a monotonically increasing and bathtub-shaped hrf with only one parameter. After all, the supremacy of the suggested model is confirmed by fitting a well-known bathtub-shaped dataset that varies over a unit interval with a few other bounded distributions in the unit interval.
The rest of the paper is presented as follows: In Section 2, moments, incomplete moments, and other properties are explored together with the introduction of the UNXLD. In Section 4, we explore different estimation approaches, such as ML, LS, and WLS. Additionally, a simulation exercise is conducted to assess the effectiveness of model parameter estimates obtained through these methods. Two datasets are used in Section 5 to clarify the recommended distribution. Finally, Section 6 presents the conclusions.
The UNXLD is obtained by the exponential transformation, X=e−Y, of the NXLD. A rv X is said to follow the UNXLD with parameter θ>0, if its pdf is of the following form:
f(x;θ)=θ2xθ−1(1−θlogx), x∈(0,1), θ>0. | (2.1) |
The corresponding cdf is given by
F(x;θ)=xθ−θxθlogx2. | (2.2) |
For any θ>0, limx→0f(x;θ)=0 and limx→1f(x;θ)=θ2. Figure 1 displays the pdf of the UNXLD for various values of the parameter θ.
Furthermore, from Figure 1, it is clear that it serves as an appropriate probability model for modeling right-skewed measurements within the unit interval.
Assume that X is a rv with UNXLD. The kth non-central moment of X for k=1,2,3... is given by
E(Xk)=θ(k+2θ)2(k+θ)2. | (2.3) |
From (2.3), the mean and variance of UNXLD is obtained as
E(X)=θ(2θ+1)2(θ+1)2, | (2.4) |
and
V(X)=7θ4+20θ3+16θ2+4θ4(θ+2)2(θ+1)4. |
Additionally, the skewness and kurtosis of UNXLD are given by
Skewness(X)=4(2+θ)2(−24+θ(−130+θ(−244+θ(−154+3θ(13+θ(22+5θ))))))2θ(3+θ)4(4+θ(16+θ(20+7θ)))3, |
and
Kurtosis(X)=1θ(3+θ)2(4+θ)2(4+θ(16+θ(20+7θ)))23(2+θ)2(384+θ(2880+θ(8864+θ(14704+θ(15272+θ(12100+θ(8324+θ(4099+3θ(362+370))))))))). |
The behavior of the mean, variance, skewness, and kurtosis coefficients for various values of the parameter is graphically depicted in Figures 2 and 3. It is evident that as θ increases, the mean also increases. Additionally, the variance initially increases for certain values of θ, but then it begins to decrease. As for skewness, it increases with θ, indicating a right skew. Additionally, the kurtosis also increases as θ increases.
Proposition 2.1. The kth incomplete moment at x of a rv X with the UNXLD is for any non-negative integer k and for any value of x∈(0,1) is given by
mk(x;θ)=θ2xk+θ[(k+θ)logx−1]2(k+θ)2. |
Proof. According to the definition of the kth incomplete moment, there are
mk(x;θ)=∫x0tkf(t;θ)dt=∫x0tkθ2tθ−1(1−θlogt)dt=θ2xk+θ[(k+θ)logx−1]2(k+θ)2. |
The hrf provides insight into the risk of an event happening at a particular time, considering the history of events up to that time.
Using (2.2), the sf and hrf of X are given by
s(x;θ)=1−xθ+θxθlogx2, |
and
h(x;θ)=θxθ−1(1−θlogx)2(1−xθ+θxθlogx2). | (2.5) |
Additionally, for any θ>0, limx→0h(x;θ)=0 and limx→1h(x;θ)=∞.
The reversed hrf of X is given by
τ(x;θ)=θ(1−θlogx)x(2−θlogx). |
Figure 4 illustrates the hrf for various values of the parameter θ, providing a general understanding of the different forms of the hrf (2.5). It is evident that the UNXLD can exhibit increasing, and bathtub-shaped hrf.
Similarly, mrl provides the average time a system or component can be expected to continue functioning before reaching a specific condition, which is valuable for making informed decisions about maintenance, replacement, and resource allocation.
Proposition 2.2. The mrl of a rv having the UNXLD is given by
r(t;θ)=1s(t;θ)(1−t−1θ+1+tθ+1θ+1−θtθ+1logt2(θ+1)−θ2(θ+1)2+θtθ+12(θ+1)2), 0<t<1, |
where s(x;θ)=1−F(x;θ) is the sf, 0<x<1.
Proof. Let X be a rv with a UNXLD with cdf (2.2). The mrl of X can be stated as follows:
r(t;θ)=E(X−t|X>t)=1s(t;θ)∫1ts(x;θ)dx=1s(t;θ)(1−t−1θ+1+tθ+1θ+1−θtθ+1logt2(θ+1)−θ2(θ+1)2+θtθ+12(θ+1)2). |
Lorenz and Bonferroni curves serve as essential tools for measuring income inequality and have broad applications beyond economics, extending into diverse fields such as reliability analysis, demography, medicine, and insurance. For the UNXLD, we will derive Lorenz and Bonferroni curves in this section.
Proposition 2.3. The Lorenz and Bonferroni curves and Gini index of the UNXLD are given respectively as follows:
(1)
LF(x)=xθ+1(2θ+1−(θ+1)θlogx)2θ+1; |
(2)
BF(x)=x(2θ+1−(θ+1)θlogx)(2θ+1)(1−θlogx2); |
(3)
Gi(x)=1−θ(θ(θ(16θ+21)+8)+1)(2θ+1)4,θ>−12. |
Proof. By using the first incomplete moment m1(x;θ) and the E(X), one can determine the Lorenz and Bonferroni curves.
(1)
LF(x;θ)=m1(x;θ)E(x). | (2.6) |
Now,
m(x;θ)=∫x0tf(t;θ)dt=θxθ+1(2θ+1−(θ+1)θlogx)2(θ+1)2. | (2.7) |
By substituting (2.7), and (2.4) into (2.6), we have
LF(x;θ)=xθ+1(2θ+1−(θ+1)θlogx)2θ+1. |
(2)
BF(x;θ)=m1(x;θ)F(x;θ)E(X). | (2.8) |
By substituting (2.7), (2.4), and (2.2) into (2.8), we have
BF(x)=x(2θ+1−(θ+1)θlogx)(2θ+1)(1−θlogx2). |
(3) The proof is obtained directly by using the cdf in Eq (2.2) and the mean in (2.4) of the UNXLD and is given by
Gi(x)=1−∫10(1−F(x,θ))2dxμ. |
Proposition 2.4. The pdf of the UNXLD has the mode given by
xM=e1(1−θ)θ. |
Proof. To find the mode, take the log of the UNXLD pdf as:
log(f(x;θ))=log(θ/2)+log(x(θ−1))+log(1−θlog(x)). |
Differentiate log(f(x;θ)) with respect to x to obtain:
∂log(f(x;θ))∂x=θ−1x−θx(1−θlog(x)). |
Equating this equation to zero and solving for x, we obtain
xM=e1(1−θ)θ. |
Let X be a non-negative absolutely continuous rv with pdf f(x). In this section, the extropy measure suggested by [23] and three entropy measures, include, the Tsallis entropy proposed by [24], the Rényi entropy introduced by [25], and the Havrda and Charvat entropy suggested by [26] for the UNXLD, are presented.
Proposition 3.1. If X∼UNXLD, then the extropy of X is defined as:
J(X)=θ2(2(3−5θ)θ−1)8(2θ−1)3. | (3.1) |
Proof. Using the pdf of the UNXLD in Eq (2.1) and the definition of extropy J(X)=−12∫10f2(x)dx, the proof is given by
J(X)=−12∫10f2(x)dx=−12∫1014θ2x2θ−2((θlog(x))2−2θlog(x)+1)dx=−12(∫10θ24x2θ−2dx−∫10θ32x2θ−2log(x)dx+∫10θ44x2θ−2log2(x)dx)=−12(θ42(2θ−1)3+θ32(1−2θ)2+θ24(2θ−1))=θ2(2(3−5θ)θ−1)8(2θ−1)3. |
Proposition 3.2. If X∼UNXLD, then the Rényi entropy of X is defined as:
Re(δ)=11−δlog(θ2δeδ(θ−1)+1θ2δ(δ(θ−1)+1)δ+1Γ(δ+1,δ(θ−1)+1θ)),δ>0,δ≠1. | (3.2) |
Proof. Using the pdf of the UNXLD in Eq (2.1) and the definition of Rényi entropy Re(δ)=11−δlog(∞∫0fδ(x)dx),δ>0,δ≠1, the proof can be obtained.
Proposition 3.3. If X∼UNXLD, then the Tsallis entropy of X is defined as:
Te(λ)=1λ−1(1−θ2λe(θ−1)λ+1θ2λ((θ−1)λ+1)λ+1Γ(λ+1,(θ−1)λ+1θ)),λ>0,λ≠1. | (3.3) |
Proof. Using the pdf of the UNXLD in Eq (2.1) and the definition of Tsallis entropy Re(λ)=1λ−1(1−∫∞0fλ(x)dx),λ>0,λ≠1, the proof can be obtained.
Proposition 3.4. If X∼UNXLD, then for β>0,β≠1 the Havrda and Charvat entropy of X is defined as:
HCe(β)=121−β−1(θ2βeβ(θ−1)+1θ2β(β(θ−1)+1)β+1Γ(β+1,β(θ−1)+1θ)−1). | (3.4) |
Proof. Using the pdf of the UNXLD in Eq (2.1) and the definition of Havrda and Charvat entropy HCe(β)=121−β−1(∞∫0fβ(x)dx−1),β>0,β≠1, the proof can be obtained.
The estimation of the UNXLD parameter is covered in this section. The ML approach is described in Subsection 4.1. The LS and WLS approaches are described in Subsection 4.2. Section 4.3 compares the effectiveness of these techniques using a Monte Carlo simulation analysis.
Let X1,X2,...,Xn be a random sample of size n taken from the UNXLD with parameter θ. x1,x2,...,xn are the observed values. Then the likelihood function is given by
L(x;θ)=n∏i=1f(xi;θ). |
Then the derivative of the log-likelihood function is given by
∂∂θlogL(x;θ)=nθ+n∑i=1logxi−n∑i=1logxi1−θlogxi. | (4.1) |
The MLE of θ is obtained by maximizing the logL(x;θ) with respect to θ. Which is done by solving the equation ∂∂θlogL(x;θ)=0. Due to the difficulty in solving this, we can use the optim function in R to obtain the MLE numerically.
Let X1,X2,...,Xn be a random sample taken from the UNXLD with parameter θ. Let X1:n,X2:n,...,Xn:n be the order statistics and are denoted by x1:n,x2:n,...,xn:n the ordered observed data. Let us set
R(θ)=n∑i=1[F(xi:n;θ)−in+1]2. |
Then, the LSE of θ, say ˆθLS, is acquired by minimizing R(θ) with respect to θ. Practically the LSE is obtained by solving
∂∂θR(θ)=2n∑i=1[F(xi:n;θ)−in+1]D(xi:n,θ)=0, |
where
D(xi:n,θ)=∂∂θF(xi:n;θ)=xθi:nlogxi:n(1−θlogxi:n2). |
Similarly, the WLS estimate (WLSE) of θ, say ˆθWLS, is acquired by minimizing the non-linear function
W(θ)=n∑i=1(n+1)2(n+2)i(n−i+1)[F(xi:n;θ)−in+1]2, |
with respect to θ, that is acquired by solving
∂∂θW(θ)=2n∑i=1(n+1)2(n+2)i(n−i+1)[F(xi:n;θ)−in+1]D(xi:n,θ)=0. |
The LSE and WLSE can be evaluated numerically using the optim function in R.
In the simulation study, the Monte Carlo simulation was carried out to demonstrate the model's efficiency using several estimating techniques, including ML, LS, and WLS. For N=10000 samples of sizes n=50,75,200,300,500, and 1000, the estimates for the true values of the parameters were determined. These random samples from the UNXLD are generated by applying the inverse cdf to uniformly distributed random numbers. The following quantities were computed:
● Mean of the estimates : Mean(η)=1N∑Ni=1ηi;
● Average bias of the estimates, Bias(η)=1N∑Ni=1(ηi−θ);
● Mean square error of the estimates, MSE(η)=1N∑Ni=1(ηi−θ)2;
● Root mean square error of the estimates, RMSE(η)=1N∑Ni=1|ηi−θ|θ,
where η∈(ˆθML,ˆθLS,ˆθWLS), i denotes the number of the sample. The simulation results for the ML, LS, and WLS estimation methods are displayed in Tables 1–3. From these tables, it can be concluded that, for MLEs, there is a noticeable decline in both absolute bias and MSE as the sample size increases. Consequently, the performance of MLE proves to be consistently reliable. Figure 5 shows a graphical comparison of the MSEs derived using the three approaches.
θ=0.6 | θ=1.0 | |||||||
n | MLE | Bias | MSE | RMSE | MLE | Bias | MSE | RMSE |
50 | 0.53725 | 0.06275 | 0.00394 | 0.10458 | 0.92859 | 0.07141 | 0.00510 | 0.07141 |
75 | 0.57799 | 0.02201 | 0.00048 | 0.03668 | 0.96221 | 0.03779 | 0.00143 | 0.03779 |
200 | 0.56584 | 0.03416 | 0.00117 | 0.05693 | 0.95166 | 0.04834 | 0.00234 | 0.04834 |
300 | 0.58957 | 0.01043 | 0.00011 | 0.01739 | 0.98068 | 0.01932 | 0.00037 | 0.01932 |
500 | 0.62133 | 0.02133 | 0.00046 | 0.03556 | 1.04315 | 0.04315 | 0.00186 | 0.04315 |
1000 | 0.60301 | 0.00301 | 0.00001 | 0.00502 | 1.00761 | 0.00761 | 0.00006 | 0.00761 |
θ=1.5 | θ=2.1 | |||||||
n | MLE | Bias | MSE | RMSE | MLE | Bias | MSE | RMSE |
50 | 1.39245 | 0.10755 | 0.01157 | 0.07170 | 1.94940 | 0.15060 | 0.02268 | 0.07171 |
75 | 1.44324 | 0.05676 | 0.00322 | 0.03784 | 2.02057 | 0.07943 | 0.00631 | 0.03782 |
200 | 1.42729 | 0.07271 | 0.00529 | 0.04848 | 1.99820 | 0.10180 | 0.01036 | 0.04848 |
300 | 1.47088 | 0.02912 | 0.00085 | 0.01942 | 2.05923 | 0.04077 | 0.00166 | 0.01941 |
500 | 1.56445 | 0.06445 | 0.00415 | 0.04297 | 2.19025 | 0.09025 | 0.00814 | 0.04297 |
1000 | 1.51125 | 0.01125 | 0.00013 | 0.00750 | 2.11575 | 0.01575 | 0.00025 | 0.00750 |
θ=0.6 | θ=1.0 | |||||||
n | LSE | Bias | MSE | RMSE | LSE | Bias | MSE | RMSE |
50 | 0.58156 | 0.02189 | 0.00034 | 0.03073 | 0.96916 | 0.03695 | 0.00095 | 0.03084 |
75 | 0.56095 | 0.03777 | 0.00153 | 0.06509 | 0.93485 | 0.06326 | 0.00425 | 0.06515 |
200 | 0.55214 | 0.03869 | 0.00229 | 0.07977 | 0.92020 | 0.06476 | 0.00637 | 0.07980 |
300 | 0.58601 | 0.01329 | 0.00020 | 0.02331 | 0.97663 | 0.02252 | 0.00055 | 0.02337 |
500 | 0.62936 | 0.03077 | 0.00086 | 0.04893 | 1.04890 | 0.05116 | 0.00239 | 0.04890 |
1000 | 0.59583 | 0.00176 | 0.00002 | 0.00696 | 0.99300 | 0.00315 | 0.00005 | 0.00700 |
θ=1.5 | θ=2.1 | |||||||
n | LSE | Bias | MSE | RMSE | LSE | Bias | MSE | RMSE |
50 | 1.45373 | 0.05543 | 0.00214 | 0.03084 | 2.03526 | 0.07757 | 0.00419 | 0.03083 |
75 | 1.40227 | 0.09490 | 0.00955 | 0.06515 | 1.96319 | 0.13284 | 0.01872 | 0.06515 |
200 | 1.38028 | 0.09719 | 0.01433 | 0.07981 | 1.93241 | 0.13605 | 0.02809 | 0.07981 |
300 | 1.46495 | 0.03379 | 0.00123 | 0.02337 | 2.05093 | 0.04731 | 0.00241 | 0.02337 |
500 | 1.57335 | 0.07672 | 0.00538 | 0.04890 | 2.20270 | 0.10743 | 0.01055 | 0.04890 |
1000 | 1.48950 | 0.00474 | 0.00011 | 0.00700 | 2.08531 | 0.00662 | 0.00022 | 0.00699 |
θ=0.6 | θ=1.0 | |||||||
n | WLSE | Bias | MSE | RMSE | WLSE | Bias | MSE | RMSE |
50 | 0.57811 | 0.02189 | 0.00048 | 0.03649 | 0.96305 | 0.03695 | 0.00137 | 0.03695 |
75 | 0.56223 | 0.03777 | 0.00143 | 0.06296 | 0.93674 | 0.06326 | 0.00400 | 0.06326 |
200 | 0.56131 | 0.03869 | 0.00150 | 0.06448 | 0.93524 | 0.06476 | 0.00419 | 0.06476 |
300 | 0.58671 | 0.01329 | 0.00018 | 0.02216 | 0.97748 | 0.02252 | 0.00051 | 0.02252 |
500 | 0.63077 | 0.03077 | 0.00095 | 0.05129 | 1.05116 | 0.05116 | 0.00262 | 0.05116 |
1000 | 0.59824 | 0.00176 | 0.00000 | 0.00294 | 0.99685 | 0.00315 | 0.00001 | 0.00315 |
θ=1.5 | θ=2.1 | |||||||
n | WLSE | Bias | MSE | RMSE | WLSE | Bias | MSE | RMSE |
50 | 1.44457 | 0.05543 | 0.00307 | 0.03695 | 2.02243 | 0.07757 | 0.00602 | 0.03694 |
75 | 1.40510 | 0.09490 | 0.00901 | 0.06326 | 1.96716 | 0.13284 | 0.01765 | 0.06326 |
200 | 1.40281 | 0.09719 | 0.00945 | 0.06479 | 1.96395 | 0.13605 | 0.01851 | 0.06478 |
300 | 1.46621 | 0.03379 | 0.00114 | 0.02253 | 2.05269 | 0.04731 | 0.00224 | 0.02253 |
500 | 1.57672 | 0.07672 | 0.00589 | 0.05114 | 2.20743 | 0.10743 | 0.01154 | 0.05115 |
1000 | 1.49526 | 0.00474 | 0.00002 | 0.00316 | 2.09338 | 0.00662 | 0.00004 | 0.00315 |
In this section, two real-life datasets are used to demonstrate the advantages of the UNXLD. After the data were fitted with the UNXLD, the outcomes were compared to those offered by other probability distributions specified in the unit interval based on the AIC, AICc, CAIC, and BIC together with the MLE. In addition, the KS test and the corresponding p−value were used to assess the models' goodness-of-fit, which are listed below
● Akaike information criterion:
AIC=2k−2logl; |
● Akaike information criterion corrected:
AICc=AIC+2k(k+1)n−k−1; |
● Consistent Akaike information criterion:
CAIC=−2logl+k(logn+1); |
● Bayesian information criterion:
BIC=klogn−2logl. |
Here, logl denotes the estimated value of the maximum log-likelihood, k denotes the number of parameters and n denotes the number of observations
For comparison, the following probability distributions were taken into account: BD, TLD proposed by [27], KD suggested by [28], ETLD introduced by [29], and UBD suggested by [6].
The pdf of the compared distributions that are used to compare with the UNXLD on the unit interval (0,1).
● Beta distribution:
f(x;α;β)=Γ(α+β)Γ(α)Γ(β)xα−1(1−x)β−1,x∈(0,1),α>0,β>0. |
● Topp-Leone distribution:
f(x;α)=2α(1−x)xα−1(2−x)α−1, α>0. |
● Kumaraswamy distribution:
f(x;α;β)=αβxα−1(1−xα)β−1, α>0,β>0. |
● Exponentiated Topp-Leone distribution:
f(x;α;β)=2αβ(1−x)(x(2−x))α−1(1−xα(2−x)α)β−1, α>0,β>0. |
● Unit Burr-Ⅱ distribution:
f(x;α;β)=αβx−1(−logx)β−1(1+(−logx)β)−α−1,x∈(0,1), α>0,β>0. |
The first dataset here considered relates to a comparison of the SC 16 and P3 unit capacity factor estimation techniques. [30] and [31] has already been investigated this dataset. The data are displayed in Table 4.
0.853 | 0.759 | 0.866 | 0.809 | 0.717 | 0.544 | 0.492 | 0.403 |
0.344 | 0.213 | 0.116 | 0.116 | 0.092 | 0.070 | 0.059 | 0.048 |
0.036 | 0.029 | 0.021 | 0.014 | 0.011 | 0.008 | 0.006 |
The second set of data comprises the initial 58 observations documenting the time of failure for Kevlar 49/epoxy strands tested at a stress level of 90%. This data was used by [32] and is presented in Table 5. Figures 6–9 show the density plot, QQ plot, PP plot, box plot, estimated pdfs, and TTT plot proposed by [33] may be used for obtaining empirical behavior of the hrf for both datasets considered here.
0.01 | 0.01 | 0.02 | 0.02 | 0.02 | 0.03 | 0.03 | 0.04 | 0.05 |
0.06 | 0.07 | 0.07 | 0.08 | 0.09 | 0.09 | 0.1 | 0.1 | 0.11 |
0.11 | 0.12 | 0.13 | 0.18 | 0.19 | 0.2 | 0.23 | 0.24 | 0.24 |
0.29 | 0.34 | 0.35 | 0.36 | 0.38 | 0.4 | 0.42 | 0.43 | 0.52 |
0.54 | 0.56 | 0.6 | 0.6 | 0.63 | 0.65 | 0.67 | 0.68 | 0.72 |
0.72 | 0.72 | 0.73 | 0.79 | 0.79 | 0.8 | 0.8 | 0.83 | 0.85 |
0.9 | 0.92 | 0.95 | 0.99 | 0.01 |
The results for dataset 1 and dataset 2 are summarized in Tables 6 and 7. These tables specifically provide the log-likelihood value, MLEs, measures AIC, AICc, CAIC, BIC, and the value of the KS statistic together with the corresponding p−value for each fitted model. The UNXLD offers a better fit with the smallest values for the AIC, AICc, CAIC, and BIC criteria, as well as the smallest value for the KS statistic and the largest p−value, as can be observed.
Model | logL | ML estimates | S.Es | AIC | AICc | CAIC | BIC | KS statistic | p−value |
UNXLD | 9.9915 | ˆθ=0.6824 | 0.1244 | -17.9830 | -17.7925 | -15.8475 | -16.8475 | 0.1663 | 0.5483 |
UBD | 5.8728 | ˆα=0.7848 ˆβ=1.5049 |
0.1919 0.2951 |
-7.745593 | -7.145593 | -3.474604 | -5.474604 | 0.2394 | 0.1433 |
ETLD | 9.3913 | ˆα=0.4624 ˆβ=0.6806 |
0.1389 0.1717 |
-14.7827 | -14.1827 | -10.5117 | -12.5117 | 0.1933 | 0.3562 |
TLD | 8.1151 | ˆα=0.5943 | 0.1239 | -14.2303 | -14.0398 | -12.0948 | -13.0948 | 0.1690 | 0.5272 |
BD | 9.6075 | ˆα=0.4869 ˆβ=1.1679 |
0.1208 0.3578 |
-15.2149 | -14.6149 | -10.9439 | -12.9439 | 0.1836 | 0.4203 |
KD | 9.6708 | ˆα=0.5044 ˆβ=1.1862 |
0.1288 0.3265 |
-15.3416 | -14.7416 | -11.0706 | -13.0706 | 0.1790 | 0.4529 |
Model | logL | ML estimates | S.Es | AIC | AICc | CAIC | BIC | KS statistic | p−value |
UNXLD | 5.7959 | ˆθ=0.9861 | 0.1138 | -9.5917 | -9.5203 | -6.5313 | -7.5313 | 0.1013 | 0.5911 |
UBD | 0.4600 | ˆα=1.1262 ˆβ=1.3741 |
0.1581 0.1571 |
3.0799 | 3.2981 | 9.2008 | 7.2008 | 0.1304 | 0.2778 |
ETLD | 5.4371 | ˆα=0.6450 ˆβ=0.5639 |
0.1305 0.0879 |
-6.8742 | -6.6560 | -0.7533 | -2.7533 | 0.1107 | 0.4765 |
BD | 5.6714 | ˆα=0.6777 ˆβ=1.0412 |
0.1107 0.1873 |
-7.3427 | -7.1245 | -1.2218 | -3.2218 | 0.1038 | 0.5592 |
KD | 5.6824 | ˆα=0.6825 ˆβ=1.0472 |
0.1145 0.1794 |
-7.3648 | -7.1467 | -1.2439 | -3.2439 | 0.1036 | 0.5628 |
By using an exponential transformation, we established a bounded form of the NXLD in this study called the UNXLD. Certain important distributional properties, such as the behavior of the pdf and hrf, along with some tractable statistical properties such as moments, incomplete moments, mode, and quantile function, are proposed. Moreover, all the statistical measures are in closed form. The ML approach, LS, and WLS were used to estimate the model parameters, and simulation studies were used to test the estimates. The UNXLD can be thought of as a good contender in distributions in unit interval, when the dominance of the proposed model has been demonstrated using two real datasets. In future work, it would be intriguing to identify the quantile function and extend the research to develop quantile regression models.
M. R. Irshad, S. Aswathy, R. May: Conceptualization, methodology, software, validation, formal analysis, writing-original draft preparation, writing-review and editing, visualization; Amer I. Al-Omari, Ghadah Alomani: Conceptualization, validation, formal analysis, writing-original draft preparation, writing-review and editing, visualization. All authors have read and approved the final version of the manuscript for publication.
Princess Nourah bint Abdulrahman University Researchers Supporting Project number (PNURSP2024R226), Princess Nourah bint Abdulrahman University, Riyadh, Saudi Arabia.
The data supporting the findings of this study are available within the article.
The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.
There is no conflict of interest with the publication of this work.
The R-code for the empirical study of UNXLD is given below.
library(fitdistrplus)
data < -NULL
n < -length(data)
n
### PDF ###
duxl < - function(x, theta){
((theta/2)*(x^(theta-1))*(1-(theta*log(x))))
}
### CDF ###
puxl < - function(q, theta){
((q^theta)-((theta*(q^theta)*(log(q)))/(2)))
}
prefit(x, "uxl", "mle", list(theta = initial), lower = c(0), upper = c(Inf))
est < - fitdist(x, "uxl", start = list(theta = initial), optim.method="Nelder-Mead")
est
summary(est)
ks.test(x, "puxl", est$ estimate)
logl = est $loglik
AIC = 2*1-2*logl
AIC
BIC = -2*logl+1*(log(length(x)))
BIC
k = number of parameter
CAIC = -2*logl+k*(log(length(x))+1)
CAIC
AICC = AIC+(2*k*(k+1)/(length(x)-k-1))
AICC
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1. | Juan M. Astorga, Yuri A. Iriarte, The Lambert-Topp-Leone distribution: an alternative for modeling proportion and lifetime data, 2025, 11, 2297-4687, 10.3389/fams.2025.1527833 |
θ=0.6 | θ=1.0 | |||||||
n | MLE | Bias | MSE | RMSE | MLE | Bias | MSE | RMSE |
50 | 0.53725 | 0.06275 | 0.00394 | 0.10458 | 0.92859 | 0.07141 | 0.00510 | 0.07141 |
75 | 0.57799 | 0.02201 | 0.00048 | 0.03668 | 0.96221 | 0.03779 | 0.00143 | 0.03779 |
200 | 0.56584 | 0.03416 | 0.00117 | 0.05693 | 0.95166 | 0.04834 | 0.00234 | 0.04834 |
300 | 0.58957 | 0.01043 | 0.00011 | 0.01739 | 0.98068 | 0.01932 | 0.00037 | 0.01932 |
500 | 0.62133 | 0.02133 | 0.00046 | 0.03556 | 1.04315 | 0.04315 | 0.00186 | 0.04315 |
1000 | 0.60301 | 0.00301 | 0.00001 | 0.00502 | 1.00761 | 0.00761 | 0.00006 | 0.00761 |
θ=1.5 | θ=2.1 | |||||||
n | MLE | Bias | MSE | RMSE | MLE | Bias | MSE | RMSE |
50 | 1.39245 | 0.10755 | 0.01157 | 0.07170 | 1.94940 | 0.15060 | 0.02268 | 0.07171 |
75 | 1.44324 | 0.05676 | 0.00322 | 0.03784 | 2.02057 | 0.07943 | 0.00631 | 0.03782 |
200 | 1.42729 | 0.07271 | 0.00529 | 0.04848 | 1.99820 | 0.10180 | 0.01036 | 0.04848 |
300 | 1.47088 | 0.02912 | 0.00085 | 0.01942 | 2.05923 | 0.04077 | 0.00166 | 0.01941 |
500 | 1.56445 | 0.06445 | 0.00415 | 0.04297 | 2.19025 | 0.09025 | 0.00814 | 0.04297 |
1000 | 1.51125 | 0.01125 | 0.00013 | 0.00750 | 2.11575 | 0.01575 | 0.00025 | 0.00750 |
θ=0.6 | θ=1.0 | |||||||
n | LSE | Bias | MSE | RMSE | LSE | Bias | MSE | RMSE |
50 | 0.58156 | 0.02189 | 0.00034 | 0.03073 | 0.96916 | 0.03695 | 0.00095 | 0.03084 |
75 | 0.56095 | 0.03777 | 0.00153 | 0.06509 | 0.93485 | 0.06326 | 0.00425 | 0.06515 |
200 | 0.55214 | 0.03869 | 0.00229 | 0.07977 | 0.92020 | 0.06476 | 0.00637 | 0.07980 |
300 | 0.58601 | 0.01329 | 0.00020 | 0.02331 | 0.97663 | 0.02252 | 0.00055 | 0.02337 |
500 | 0.62936 | 0.03077 | 0.00086 | 0.04893 | 1.04890 | 0.05116 | 0.00239 | 0.04890 |
1000 | 0.59583 | 0.00176 | 0.00002 | 0.00696 | 0.99300 | 0.00315 | 0.00005 | 0.00700 |
θ=1.5 | θ=2.1 | |||||||
n | LSE | Bias | MSE | RMSE | LSE | Bias | MSE | RMSE |
50 | 1.45373 | 0.05543 | 0.00214 | 0.03084 | 2.03526 | 0.07757 | 0.00419 | 0.03083 |
75 | 1.40227 | 0.09490 | 0.00955 | 0.06515 | 1.96319 | 0.13284 | 0.01872 | 0.06515 |
200 | 1.38028 | 0.09719 | 0.01433 | 0.07981 | 1.93241 | 0.13605 | 0.02809 | 0.07981 |
300 | 1.46495 | 0.03379 | 0.00123 | 0.02337 | 2.05093 | 0.04731 | 0.00241 | 0.02337 |
500 | 1.57335 | 0.07672 | 0.00538 | 0.04890 | 2.20270 | 0.10743 | 0.01055 | 0.04890 |
1000 | 1.48950 | 0.00474 | 0.00011 | 0.00700 | 2.08531 | 0.00662 | 0.00022 | 0.00699 |
θ=0.6 | θ=1.0 | |||||||
n | WLSE | Bias | MSE | RMSE | WLSE | Bias | MSE | RMSE |
50 | 0.57811 | 0.02189 | 0.00048 | 0.03649 | 0.96305 | 0.03695 | 0.00137 | 0.03695 |
75 | 0.56223 | 0.03777 | 0.00143 | 0.06296 | 0.93674 | 0.06326 | 0.00400 | 0.06326 |
200 | 0.56131 | 0.03869 | 0.00150 | 0.06448 | 0.93524 | 0.06476 | 0.00419 | 0.06476 |
300 | 0.58671 | 0.01329 | 0.00018 | 0.02216 | 0.97748 | 0.02252 | 0.00051 | 0.02252 |
500 | 0.63077 | 0.03077 | 0.00095 | 0.05129 | 1.05116 | 0.05116 | 0.00262 | 0.05116 |
1000 | 0.59824 | 0.00176 | 0.00000 | 0.00294 | 0.99685 | 0.00315 | 0.00001 | 0.00315 |
θ=1.5 | θ=2.1 | |||||||
n | WLSE | Bias | MSE | RMSE | WLSE | Bias | MSE | RMSE |
50 | 1.44457 | 0.05543 | 0.00307 | 0.03695 | 2.02243 | 0.07757 | 0.00602 | 0.03694 |
75 | 1.40510 | 0.09490 | 0.00901 | 0.06326 | 1.96716 | 0.13284 | 0.01765 | 0.06326 |
200 | 1.40281 | 0.09719 | 0.00945 | 0.06479 | 1.96395 | 0.13605 | 0.01851 | 0.06478 |
300 | 1.46621 | 0.03379 | 0.00114 | 0.02253 | 2.05269 | 0.04731 | 0.00224 | 0.02253 |
500 | 1.57672 | 0.07672 | 0.00589 | 0.05114 | 2.20743 | 0.10743 | 0.01154 | 0.05115 |
1000 | 1.49526 | 0.00474 | 0.00002 | 0.00316 | 2.09338 | 0.00662 | 0.00004 | 0.00315 |
0.853 | 0.759 | 0.866 | 0.809 | 0.717 | 0.544 | 0.492 | 0.403 |
0.344 | 0.213 | 0.116 | 0.116 | 0.092 | 0.070 | 0.059 | 0.048 |
0.036 | 0.029 | 0.021 | 0.014 | 0.011 | 0.008 | 0.006 |
0.01 | 0.01 | 0.02 | 0.02 | 0.02 | 0.03 | 0.03 | 0.04 | 0.05 |
0.06 | 0.07 | 0.07 | 0.08 | 0.09 | 0.09 | 0.1 | 0.1 | 0.11 |
0.11 | 0.12 | 0.13 | 0.18 | 0.19 | 0.2 | 0.23 | 0.24 | 0.24 |
0.29 | 0.34 | 0.35 | 0.36 | 0.38 | 0.4 | 0.42 | 0.43 | 0.52 |
0.54 | 0.56 | 0.6 | 0.6 | 0.63 | 0.65 | 0.67 | 0.68 | 0.72 |
0.72 | 0.72 | 0.73 | 0.79 | 0.79 | 0.8 | 0.8 | 0.83 | 0.85 |
0.9 | 0.92 | 0.95 | 0.99 | 0.01 |
Model | logL | ML estimates | S.Es | AIC | AICc | CAIC | BIC | KS statistic | p−value |
UNXLD | 9.9915 | ˆθ=0.6824 | 0.1244 | -17.9830 | -17.7925 | -15.8475 | -16.8475 | 0.1663 | 0.5483 |
UBD | 5.8728 | ˆα=0.7848 ˆβ=1.5049 |
0.1919 0.2951 |
-7.745593 | -7.145593 | -3.474604 | -5.474604 | 0.2394 | 0.1433 |
ETLD | 9.3913 | ˆα=0.4624 ˆβ=0.6806 |
0.1389 0.1717 |
-14.7827 | -14.1827 | -10.5117 | -12.5117 | 0.1933 | 0.3562 |
TLD | 8.1151 | ˆα=0.5943 | 0.1239 | -14.2303 | -14.0398 | -12.0948 | -13.0948 | 0.1690 | 0.5272 |
BD | 9.6075 | ˆα=0.4869 ˆβ=1.1679 |
0.1208 0.3578 |
-15.2149 | -14.6149 | -10.9439 | -12.9439 | 0.1836 | 0.4203 |
KD | 9.6708 | ˆα=0.5044 ˆβ=1.1862 |
0.1288 0.3265 |
-15.3416 | -14.7416 | -11.0706 | -13.0706 | 0.1790 | 0.4529 |
Model | logL | ML estimates | S.Es | AIC | AICc | CAIC | BIC | KS statistic | p−value |
UNXLD | 5.7959 | ˆθ=0.9861 | 0.1138 | -9.5917 | -9.5203 | -6.5313 | -7.5313 | 0.1013 | 0.5911 |
UBD | 0.4600 | ˆα=1.1262 ˆβ=1.3741 |
0.1581 0.1571 |
3.0799 | 3.2981 | 9.2008 | 7.2008 | 0.1304 | 0.2778 |
ETLD | 5.4371 | ˆα=0.6450 ˆβ=0.5639 |
0.1305 0.0879 |
-6.8742 | -6.6560 | -0.7533 | -2.7533 | 0.1107 | 0.4765 |
BD | 5.6714 | ˆα=0.6777 ˆβ=1.0412 |
0.1107 0.1873 |
-7.3427 | -7.1245 | -1.2218 | -3.2218 | 0.1038 | 0.5592 |
KD | 5.6824 | ˆα=0.6825 ˆβ=1.0472 |
0.1145 0.1794 |
-7.3648 | -7.1467 | -1.2439 | -3.2439 | 0.1036 | 0.5628 |
θ=0.6 | θ=1.0 | |||||||
n | MLE | Bias | MSE | RMSE | MLE | Bias | MSE | RMSE |
50 | 0.53725 | 0.06275 | 0.00394 | 0.10458 | 0.92859 | 0.07141 | 0.00510 | 0.07141 |
75 | 0.57799 | 0.02201 | 0.00048 | 0.03668 | 0.96221 | 0.03779 | 0.00143 | 0.03779 |
200 | 0.56584 | 0.03416 | 0.00117 | 0.05693 | 0.95166 | 0.04834 | 0.00234 | 0.04834 |
300 | 0.58957 | 0.01043 | 0.00011 | 0.01739 | 0.98068 | 0.01932 | 0.00037 | 0.01932 |
500 | 0.62133 | 0.02133 | 0.00046 | 0.03556 | 1.04315 | 0.04315 | 0.00186 | 0.04315 |
1000 | 0.60301 | 0.00301 | 0.00001 | 0.00502 | 1.00761 | 0.00761 | 0.00006 | 0.00761 |
θ=1.5 | θ=2.1 | |||||||
n | MLE | Bias | MSE | RMSE | MLE | Bias | MSE | RMSE |
50 | 1.39245 | 0.10755 | 0.01157 | 0.07170 | 1.94940 | 0.15060 | 0.02268 | 0.07171 |
75 | 1.44324 | 0.05676 | 0.00322 | 0.03784 | 2.02057 | 0.07943 | 0.00631 | 0.03782 |
200 | 1.42729 | 0.07271 | 0.00529 | 0.04848 | 1.99820 | 0.10180 | 0.01036 | 0.04848 |
300 | 1.47088 | 0.02912 | 0.00085 | 0.01942 | 2.05923 | 0.04077 | 0.00166 | 0.01941 |
500 | 1.56445 | 0.06445 | 0.00415 | 0.04297 | 2.19025 | 0.09025 | 0.00814 | 0.04297 |
1000 | 1.51125 | 0.01125 | 0.00013 | 0.00750 | 2.11575 | 0.01575 | 0.00025 | 0.00750 |
θ=0.6 | θ=1.0 | |||||||
n | LSE | Bias | MSE | RMSE | LSE | Bias | MSE | RMSE |
50 | 0.58156 | 0.02189 | 0.00034 | 0.03073 | 0.96916 | 0.03695 | 0.00095 | 0.03084 |
75 | 0.56095 | 0.03777 | 0.00153 | 0.06509 | 0.93485 | 0.06326 | 0.00425 | 0.06515 |
200 | 0.55214 | 0.03869 | 0.00229 | 0.07977 | 0.92020 | 0.06476 | 0.00637 | 0.07980 |
300 | 0.58601 | 0.01329 | 0.00020 | 0.02331 | 0.97663 | 0.02252 | 0.00055 | 0.02337 |
500 | 0.62936 | 0.03077 | 0.00086 | 0.04893 | 1.04890 | 0.05116 | 0.00239 | 0.04890 |
1000 | 0.59583 | 0.00176 | 0.00002 | 0.00696 | 0.99300 | 0.00315 | 0.00005 | 0.00700 |
θ=1.5 | θ=2.1 | |||||||
n | LSE | Bias | MSE | RMSE | LSE | Bias | MSE | RMSE |
50 | 1.45373 | 0.05543 | 0.00214 | 0.03084 | 2.03526 | 0.07757 | 0.00419 | 0.03083 |
75 | 1.40227 | 0.09490 | 0.00955 | 0.06515 | 1.96319 | 0.13284 | 0.01872 | 0.06515 |
200 | 1.38028 | 0.09719 | 0.01433 | 0.07981 | 1.93241 | 0.13605 | 0.02809 | 0.07981 |
300 | 1.46495 | 0.03379 | 0.00123 | 0.02337 | 2.05093 | 0.04731 | 0.00241 | 0.02337 |
500 | 1.57335 | 0.07672 | 0.00538 | 0.04890 | 2.20270 | 0.10743 | 0.01055 | 0.04890 |
1000 | 1.48950 | 0.00474 | 0.00011 | 0.00700 | 2.08531 | 0.00662 | 0.00022 | 0.00699 |
θ=0.6 | θ=1.0 | |||||||
n | WLSE | Bias | MSE | RMSE | WLSE | Bias | MSE | RMSE |
50 | 0.57811 | 0.02189 | 0.00048 | 0.03649 | 0.96305 | 0.03695 | 0.00137 | 0.03695 |
75 | 0.56223 | 0.03777 | 0.00143 | 0.06296 | 0.93674 | 0.06326 | 0.00400 | 0.06326 |
200 | 0.56131 | 0.03869 | 0.00150 | 0.06448 | 0.93524 | 0.06476 | 0.00419 | 0.06476 |
300 | 0.58671 | 0.01329 | 0.00018 | 0.02216 | 0.97748 | 0.02252 | 0.00051 | 0.02252 |
500 | 0.63077 | 0.03077 | 0.00095 | 0.05129 | 1.05116 | 0.05116 | 0.00262 | 0.05116 |
1000 | 0.59824 | 0.00176 | 0.00000 | 0.00294 | 0.99685 | 0.00315 | 0.00001 | 0.00315 |
θ=1.5 | θ=2.1 | |||||||
n | WLSE | Bias | MSE | RMSE | WLSE | Bias | MSE | RMSE |
50 | 1.44457 | 0.05543 | 0.00307 | 0.03695 | 2.02243 | 0.07757 | 0.00602 | 0.03694 |
75 | 1.40510 | 0.09490 | 0.00901 | 0.06326 | 1.96716 | 0.13284 | 0.01765 | 0.06326 |
200 | 1.40281 | 0.09719 | 0.00945 | 0.06479 | 1.96395 | 0.13605 | 0.01851 | 0.06478 |
300 | 1.46621 | 0.03379 | 0.00114 | 0.02253 | 2.05269 | 0.04731 | 0.00224 | 0.02253 |
500 | 1.57672 | 0.07672 | 0.00589 | 0.05114 | 2.20743 | 0.10743 | 0.01154 | 0.05115 |
1000 | 1.49526 | 0.00474 | 0.00002 | 0.00316 | 2.09338 | 0.00662 | 0.00004 | 0.00315 |
0.853 | 0.759 | 0.866 | 0.809 | 0.717 | 0.544 | 0.492 | 0.403 |
0.344 | 0.213 | 0.116 | 0.116 | 0.092 | 0.070 | 0.059 | 0.048 |
0.036 | 0.029 | 0.021 | 0.014 | 0.011 | 0.008 | 0.006 |
0.01 | 0.01 | 0.02 | 0.02 | 0.02 | 0.03 | 0.03 | 0.04 | 0.05 |
0.06 | 0.07 | 0.07 | 0.08 | 0.09 | 0.09 | 0.1 | 0.1 | 0.11 |
0.11 | 0.12 | 0.13 | 0.18 | 0.19 | 0.2 | 0.23 | 0.24 | 0.24 |
0.29 | 0.34 | 0.35 | 0.36 | 0.38 | 0.4 | 0.42 | 0.43 | 0.52 |
0.54 | 0.56 | 0.6 | 0.6 | 0.63 | 0.65 | 0.67 | 0.68 | 0.72 |
0.72 | 0.72 | 0.73 | 0.79 | 0.79 | 0.8 | 0.8 | 0.83 | 0.85 |
0.9 | 0.92 | 0.95 | 0.99 | 0.01 |
Model | logL | ML estimates | S.Es | AIC | AICc | CAIC | BIC | KS statistic | p−value |
UNXLD | 9.9915 | ˆθ=0.6824 | 0.1244 | -17.9830 | -17.7925 | -15.8475 | -16.8475 | 0.1663 | 0.5483 |
UBD | 5.8728 | ˆα=0.7848 ˆβ=1.5049 |
0.1919 0.2951 |
-7.745593 | -7.145593 | -3.474604 | -5.474604 | 0.2394 | 0.1433 |
ETLD | 9.3913 | ˆα=0.4624 ˆβ=0.6806 |
0.1389 0.1717 |
-14.7827 | -14.1827 | -10.5117 | -12.5117 | 0.1933 | 0.3562 |
TLD | 8.1151 | ˆα=0.5943 | 0.1239 | -14.2303 | -14.0398 | -12.0948 | -13.0948 | 0.1690 | 0.5272 |
BD | 9.6075 | ˆα=0.4869 ˆβ=1.1679 |
0.1208 0.3578 |
-15.2149 | -14.6149 | -10.9439 | -12.9439 | 0.1836 | 0.4203 |
KD | 9.6708 | ˆα=0.5044 ˆβ=1.1862 |
0.1288 0.3265 |
-15.3416 | -14.7416 | -11.0706 | -13.0706 | 0.1790 | 0.4529 |
Model | logL | ML estimates | S.Es | AIC | AICc | CAIC | BIC | KS statistic | p−value |
UNXLD | 5.7959 | ˆθ=0.9861 | 0.1138 | -9.5917 | -9.5203 | -6.5313 | -7.5313 | 0.1013 | 0.5911 |
UBD | 0.4600 | ˆα=1.1262 ˆβ=1.3741 |
0.1581 0.1571 |
3.0799 | 3.2981 | 9.2008 | 7.2008 | 0.1304 | 0.2778 |
ETLD | 5.4371 | ˆα=0.6450 ˆβ=0.5639 |
0.1305 0.0879 |
-6.8742 | -6.6560 | -0.7533 | -2.7533 | 0.1107 | 0.4765 |
BD | 5.6714 | ˆα=0.6777 ˆβ=1.0412 |
0.1107 0.1873 |
-7.3427 | -7.1245 | -1.2218 | -3.2218 | 0.1038 | 0.5592 |
KD | 5.6824 | ˆα=0.6825 ˆβ=1.0472 |
0.1145 0.1794 |
-7.3648 | -7.1467 | -1.2439 | -3.2439 | 0.1036 | 0.5628 |