Loading [MathJax]/jax/element/mml/optable/Latin1Supplement.js
Research article

Geometric inequalities of PR-warped product submanifold in para-Kenmotsu manifold

  • Received: 12 April 2022 Revised: 21 July 2022 Accepted: 31 July 2022 Published: 02 September 2022
  • MSC : 53C12, 53C25, 53B25, 53B30, 53D15

  • The main purpose of this paper is to study the properties of PR-semi-invariant submanifold of para-Kenmotsu manifold. We obtain the integrability conditions for the invariant distribution and anti-invariant distribution. We obtain some existence and non-existence results of PR-semi-invariant warped product submanifolds. We provide some necessary and sufficient conditions for PR-semi-invariant submanifold to be a PR-semi-invariant warped product submanifold in para-Kenmotsu manifold. We also derive some sharp inequalities for PR-semi-invariant warped product submanifold in para-Kenmotsu manifolds.

    Citation: Fatemah Mofarreh, S. K. Srivastava, Anuj Kumar, Akram Ali. Geometric inequalities of PR-warped product submanifold in para-Kenmotsu manifold[J]. AIMS Mathematics, 2022, 7(10): 19481-19509. doi: 10.3934/math.20221069

    Related Papers:

    [1] Jin Gao, Lihua Dai . Weighted pseudo almost periodic solutions of octonion-valued neural networks with mixed time-varying delays and leakage delays. AIMS Mathematics, 2023, 8(6): 14867-14893. doi: 10.3934/math.2023760
    [2] Xiaofang Meng, Yongkun Li . Pseudo almost periodic solutions for quaternion-valued high-order Hopfield neural networks with time-varying delays and leakage delays on time scales. AIMS Mathematics, 2021, 6(9): 10070-10091. doi: 10.3934/math.2021585
    [3] N. Mohamed Thoiyab, Mostafa Fazly, R. Vadivel, Nallappan Gunasekaran . Stability analysis for bidirectional associative memory neural networks: A new global asymptotic approach. AIMS Mathematics, 2025, 10(2): 3910-3929. doi: 10.3934/math.2025182
    [4] Rakkiet Srisuntorn, Wajaree Weera, Thongchai Botmart . Modified function projective synchronization of master-slave neural networks with mixed interval time-varying delays via intermittent feedback control. AIMS Mathematics, 2022, 7(10): 18632-18661. doi: 10.3934/math.20221025
    [5] Nina Huo, Bing Li, Yongkun Li . Global exponential stability and existence of almost periodic solutions in distribution for Clifford-valued stochastic high-order Hopfield neural networks with time-varying delays. AIMS Mathematics, 2022, 7(3): 3653-3679. doi: 10.3934/math.2022202
    [6] R. Sriraman, P. Vignesh, V. C. Amritha, G. Rachakit, Prasanalakshmi Balaji . Direct quaternion method-based stability criteria for quaternion-valued Takagi-Sugeno fuzzy BAM delayed neural networks using quaternion-valued Wirtinger-based integral inequality. AIMS Mathematics, 2023, 8(5): 10486-10512. doi: 10.3934/math.2023532
    [7] Zhifeng Lu, Fei Wang, Yujuan Tian, Yaping Li . Lag synchronization of complex-valued interval neural networks via distributed delayed impulsive control. AIMS Mathematics, 2023, 8(3): 5502-5521. doi: 10.3934/math.2023277
    [8] Ailing Li, Mengting Lv, Yifang Yan . Asymptotic stability for quaternion-valued BAM neural networks via a contradictory method and two Lyapunov functionals. AIMS Mathematics, 2022, 7(5): 8206-8223. doi: 10.3934/math.2022457
    [9] Huahai Qiu, Li Wan, Zhigang Zhou, Qunjiao Zhang, Qinghua Zhou . Global exponential periodicity of nonlinear neural networks with multiple time-varying delays. AIMS Mathematics, 2023, 8(5): 12472-12485. doi: 10.3934/math.2023626
    [10] Yongkun Li, Xiaoli Huang, Xiaohui Wang . Weyl almost periodic solutions for quaternion-valued shunting inhibitory cellular neural networks with time-varying delays. AIMS Mathematics, 2022, 7(4): 4861-4886. doi: 10.3934/math.2022271
  • The main purpose of this paper is to study the properties of PR-semi-invariant submanifold of para-Kenmotsu manifold. We obtain the integrability conditions for the invariant distribution and anti-invariant distribution. We obtain some existence and non-existence results of PR-semi-invariant warped product submanifolds. We provide some necessary and sufficient conditions for PR-semi-invariant submanifold to be a PR-semi-invariant warped product submanifold in para-Kenmotsu manifold. We also derive some sharp inequalities for PR-semi-invariant warped product submanifold in para-Kenmotsu manifolds.



    Because of advancements in manufacturing and technical development, products and devices are becoming increasingly reliable, making typical life tests under normal conditions difficult, if not impossible. For the industrial markets, such tests are too time-consuming and costly to get sufficient information about a product's lifetime distribution or even a prototype. As a result, the accelerated life test (ALT) is becoming more popular as well as important, as it gives information on a highly reliable product's lifetime in a short amount of time, see [1,2]. More failures can be collected quickly by conducting the life test at higher stress levels than normal operating conditions. A suitable stress-response regression model is then used to estimate the lifetime distribution at the usage stress. As a particular class of ALT, the progressive-stress test implements a special stress-loading scheme where the stress increases in time, see [3,4,5,6].

    Censoring often occurs when some lifetimes of products are missing or when some experimental design purposes are being implemented. Type-I and type-II censoring are the most prevalent schemes. These two types of censoring do not have the flexibility to allow the experimenter to withdraw units from a life test at different stages during the experiment. Because of this lack of flexibility, progressive censoring is proposed as a more general censoring technique. This technique enables the experimenter to withdraw units from a life test at different stages, other than the final point, through the test experiment.

    One of various risk factors could cause the units to fail in reliability, engineering, biomedicine, physical studies, and other fields. If the risks are unclear, an issue may occur regarding the factor that caused the unit to fail, and as a result, the lifetime associated with this particular risk cannot be determined. In such cases, the maximum (minimum) lifetime value with all risks can only be observed. This is referred to as a "series (parallel) system" in the literature. These two systems can be joined to form a new system known as a "series-parallel system", see its description in Figure 1. In a series system, components are connected in such a way that the failure of a single component leads to the failure of the system. On the other hand, a system in which failure of all components leads to the failure of the system is called a parallel system. Finally, a series-parallel system is a system in which m subsystems are connected in series and each subsystem consists of k components connected in parallel, see Figure 1. For such a system, failure is observed if a subsystem fails. The technique of compounding of distribution functions may be used to construct the lifetime distribution of the series-parallel system.

    Figure 1.  Diagram for a series-parallel system.

    Abdel-Hamid and Hashem [7] introduced a new distribution for the series-parallel system by compounding two Poisson distributions (truncated at zero) with an exponential distribution. They used six estimation methods to estimate the included parameters. In [8], they obtained a new distribution by compounding two discrete distributions with a mixture of continuous distributions based on a parallel-series system. Nadarajah et al. [9] applied the progressive-stress ALT technique using type-I progressively hybrid censored data with binomial removal to components connected as a parallel-series structure. Hu et al. [10], suggested an ideally distributed series-parallel system, as well as two analytical reliability assessment approaches to analyze the reliability of a distributed power system. Hashem and Alyami [11] introduced a new distribution based on a parallel-series system.

    In this article, we introduce a new distribution that describes the lifetime of a series-parallel system when the lifetimes of the included components are subject to a mixture of exponential and gamma distributions. The distribution will be called Poisson-geometric-Lomax distribution (PGLD) which can be obtained by compounding truncated Poisson, geometric, and Lomax distributions

    The following is how the rest of the article is put together: The distribution of a series-parallel system based on a finite mixture of distributions is constructed in Section 2. In Section 3, the model is described based on progressive-stress ALT and progressive type-II censoring. In Section 4, estimation of the parameters is obtained using the maximum likelihood and Bayes methods. In Section 5, the parameters are estimated numerically using maximum likelihood and Bayes estimation methods. An illustrative example, based on two real data sets, is studied in Section 6. A simulation study is worked done in Section 7. Concluding remarks followed by certain features and motivations of the PGLD as well as future work are presented in Section 8.

    A mixture of distributions is considered a combination of statistical distributions, that occur when sampling from inhomogeneous populations (or mixed populations) with a different probability density function (PDF) in each component.

    Let F(yω) be the cumulative distribution function (CDF) of a continuous random variable (RV) Y, with realization y, that is dependent on a continuous RV Ω, with realization ω, and Π(ω) be the CDF of Ω. The marginal CDF F(y) is given by

    F(y)=ΩF(yω)dΠ(ω), (2.1)

    which is called a mixture (according to Teicher [12]) of the CDFs F(yω) and Π(ω). Fisher [13] called F(y) "compound distribution".

    The corresponding PDF is given by

    f(x)=Ωf(yω)π(ω)dω. (2.2)

    If the RV Ω assumes only a finite number of points {ωj,j=1,,κ}, Π(ω) is then a mass function and assigns positive probabilities to only ωj. The integral in (2.1) is then replaced by a sum to give a { finite mixture} of the form

    F(y)=κj=1F(y;ωj)Π(ωj). (2.3)

    Suppose, in (2.3), Π(ωj)=pj, j=1,,κ, and F(y;ωj)=Fj(y). Then (2.3) takes the form

    F(y)=κj=1pjFj(y). (2.4)

    A corresponding finite mixture of PDFs is given by

    f(y)=κj=1pjfj(y). (2.5)

    In (2.4) and (2.5) the masses pj are called mixing proportions with the conditions:

    0pj1,j=1,,κ,andκj=1pj=1.

    The functions Fj and fj are called jth components in the finite mixture of CDFs (2.4) and PDFs (2.5), respectively. For more details on finite mixture of distributions, see [14,15]. Several distributions may arise due to compound distribution (2.2) and mixture distribution (2.5), see [16], such as

    (i) If in (2.2), f(yω) has exp(yω) distribution and π(ω) has gamma(α,γ) distribution, then we get Lomax(α,γ) distribution (LD) as follows:

    Lomax(α,γ)f(y;α,γ)=0ωeωyγαΓ(α)ωα1eγωdω=αγ(1+yγ)(α+1),y>0,(α,γ>0). (2.6)

    Therefore, the corresponding CDF is given by

    F(y;α,γ)=1(1+yγ)α,x>0,(α,γ>0). (2.7)

    (ii) If in (2.5), κ=2,p1=θθ+1, f1(y) has exp(θ) distribution and f2(y) has gamma(2,θ) distribution, then we get Lindley distribution as follows:

    Lindley(θ)f(y;θ)=θθ+1[θeθy]+1θ+1[θ2yeθy]=θ2θ+1(1+y)eθy,y>0,(θ>0).

    If in (2.2), f(yΩ=ω)=ωf1(y)+(1ω)f2(y) and the RV Ω subjects to a beta distribution, B(a,b), then

    f(y)=10f(yω)π(ω)dω=1B(a,b)10(ωf1(y)+(1ω)f2(y))ωa1(1ω)b1dω=aa+bf1(y)+ba+bf2(y),t>0,(a,b>0). (2.8)

    Several new distributions of the series-parallel system may emerge by choosing different distributions for the number of subsystems as well as those describing the lifetimes of the included components, as explained in [7,8], but in exchange, several questions may arise, for example:

    ● Does the presented distribution have any interesting properties?

    ● Does it arise naturally in some observable process like natural phenomena?

    ● Does it have any motivations?

    There is no need for new distributions if there are no positive answers to the above questions. A response to these questions will be illustrated in Section 8.

    According to [7,8], the following theorem gives the CDF and PDF of the PGLD which represents the failure time distribution of the series-parallel system when the number of series subsystems and the number of their components, that are connected as a parallel structure, are RVs subject to truncated Poisson and geometric distributions, respectively. At the same time, the failure times of the components have a finite mixture of distribution functions each of which may be responsible for a different cause of failure.

    Theorem 2.1. Suppose that, for i=1,2,,kj, j=1,2,,m, a mixed system of series-parallel structure type has the lifetime X=minj(maxiYij), where Yij are IID RVs, see Figure 1, with PDF(CDF) fY(y)(FY(y)) of Lomax distribution given by (2.6) ((2.7)). Consider M and Kj are two discrete RVs subject to truncated Poisson and geometric distributions with PMFs P(M=m)=eλλmm!(1eλ),m=1,2,,(λ>0) and P(Kj=kj)=(1θ)θkj1,kj=1,2,,(0<θ<1), respectively. Then the distribution of X has the PGLD with CDF and PDF given, respectively, by

    FX(x)=1eλΩ(x)1eλ, (2.9)
    fX(x)=λΩ2(x)eλΩ(x)fY(x)(1θ)(1eλ)F2Y(x), (2.10)

    where

    Ω(x)=(1θ)FY(x)1θFY(x),x>0. (2.11)

    Proof. The proof is similarly as in [7].

    Remark 2.1. It is worth noting that while γ is a scale parameter for LD with CDF (2.7), it is also a scale parameter for PGLD with CDF (2.9).

    The PDF and hazard rate function (HRF), h(x)=f(x)/(1F(x)), of the PGLD are plotted in Figure 2, in which one can observe that the PDF exhibits decreasing and unimodal shapes while the HRF exhibits a unimodal shape and may be sudden fluctuation at its end. These fluctuations usually imply that the product's performance has degraded over time. Non-stationary data can exhibit this characteristic, and the PGLD can help to represent such data. The non-stationary nature of failure times may help the researcher forecast how some items will behave in the environment.

    Figure 2.  The PDF (left panel) and HRF (right panel) of PGLD for different values of θ, α, γ, and λ.

    The features and motivations of the PGLD with CDF and PDF (2.9) and (2.10) are summarized in the last section.

    In the following section, some important properties of the PGLD are given.

    In this section, some important properties of the PGLD, such as the q-th quantile, mode, r-th moment, mean residual lifetime, Bonferroni and Lorenz curves, Rényi and Shannon's entropies, PDF and CDF of the i-th order statistic, are given.

    Theorem 3.1. The q-th quantile xq of the PGLD with CDF (2.9) can be obtained as

    xq=γ[(1+ln[1q(1eλ)]λλθθln[1q(1eλ)])1α1]. (3.1)

    Proof. By solving the equation FX(xq)=q with respect to xq, the proof can be achieved immediately.

    Remark 3.1. As a particular case, the median of PGLD with CDF (2.9) can be obtained by putting q=1/2 in Eq (3.1).

    Theorem 3.2. Let X be a RV subject to the PGLD with PDF (2.10). Then the mode is given by

    x=γ((D2+D224D1D32D1)1α1), (3.2)

    where

    D1=(α+1)(1θ)2,D2=2θ(1θ)(α+1)+α(λ2θ)(1θ),D3=θ2(1α).

    Proof. The mode can be directly obtained by solving dln[fX(x)]dx=0 with respect to x.

    Theorem 3.3. Let X be a RV subject to PGLD with PDF (2.10). Then, for r=1,2,, the r-th moment of X is given by

    m(r)=Nı=02νı(1yı)2Φ(r)(yı),

    where yı,νı are the zeros and the corresponding Christoffel numbers of the Legendre-Gauss quadrature formula on the interval (-1, 1), see Canuto et al. [17].

    Proof. The r-th moment of X is given by

    m(r)=0xrfX(x)dx=αλγ(1θ)(1eλ)112(1y)2Φ(r)(y)dy,

    where y=1+y1y, and

    Φ(r)(y)=yrΩ2(y)eλΩ(y)(1+yγ)α1(1(1+yγ)α)2. (3.3)

    The last integral can be approximated, by using Legendre-Gauss quadrature formula, as

    m(r)=Nı=02νı(1yı)2Φ(r)(yı), (3.4)

    where

    νı=2(1y2ı)[LN+1(yı)]2andLN+1(yı)=dLN+1(y)dyaty=yı, (3.5)

    and LN(.) is the Legendre polynomial of degree N.

    Theorem 3.4. The mean residual lifetime of the PGLD is given by

    MRL(x0)=2x0eλΩ(x0)eλNı=0νı(1yı)2(eλΩ(2x01yı)eλ),

    where νı is given by (3.5).

    Proof. The mean residual lifetime of the PGLD is given by

    MRL(x0)=E[Xx0X>x0]=1S(x0)x0S(x)dx=1S(x0)112x0(1y)2S(2x01y)dy,

    where S(x)=1F(x) is the survival function.

    The last integral can be approximated, by using Legendre-Gauss quadrature formula, as

    MRL(x0)=2x0eλΩ(x0)eλNı=0νı(1yı)2(eλΩ(2x01yı)eλ),

    where νı is given by (3.5).

    Theorem 3.5. Let X be a RV subject to the PGLD with PDF (2.10). Then, the Bonferroni curve (BC) and Lorenz curve (LC) are given, respectively, by

    BC(η)=AηNı=0νıΦ(1)(pη2(yı+1)),LC(η)=ηAηNı=0νıΦ(1)(pη2(yı+1)), (3.6)

    where νı is given by (3.5), 0<η<1 and

    Aη=αλpη2m(1)ηγ(1θ)(1eλ),
    pη=F1(η)=γ((1+ln[1η(1eλ)]λλθθln[1η(1eλ)])1α1),

    and Φ(1)(.) and m(1) are given, respectively, by (3.3) and (3.4) at r=1.

    Proof. The Bonferroni curve of PGLD is given by

    BC(η)=1ηm(1)pη0xfX(x)dx=Aη11Φ(1)(pη2(y+1))dy=AηNı=0νıΦ(1)(pη2(yı+1)).

    The Lorenz curve of PGLD is given by

    LC(η)=1m(1)pη0xfX(x)dx=ηAηNı=0νıΦ(1)(pη2(yı+1)).

    The Bonferroni and Lorenz curves are plotted in Figure 3.

    Figure 3.  Left (Right) panel: The Bonferroni (Lorenz) Curve of the PGLD.

    Theorem 3.6. Let X be a RV subject to the PGLD with PDF (2.10). Then, the Rényi and Shannon's entropies of X are given, respectively, by

    RE()=11(ln[αλγ(1θ)(1eλ)]+ln[Nı=0νı2(1yı)2W(1+yı1yı)]),SHE=ln[γ(1θ)(1eλ)αλ]+2αλγ(1θ)(1eλ)Nı=02νı(1yı)2W(1+yı1yı)Φ(0)(1+yı1yı), (3.7)

    where νı is given by (3.5) and

    W(y)=Ω2(y)eλΩ(y)(1+yγ)α[1(1+yγ)α]2,
    W(y)=2ln[Ω(y)]+λΩ(y)+(α+1)ln[1+yγ]+2ln[1(1+yγ)α].

    Proof. The Rényi entropy of X is given by

    RE()=11ln[0fX(x)dx],

    where >0 and 1.

    Based on PDF (2.10), we obtain

    0fX(x)dx=[αλγ(1θ)(1eλ)]0W(x)dx=[αλγ(1θ)(1eλ)]Nı=0νı2(1yı)2W(1+yı1yı).

    Then,

    RE()=11(ln[αλγ(1θ)(1eλ)]+ln[Nı=0νı2(1yı)2W(1+yı1yı)]).

    The Shannon's entropy of T is given by

    SHE=E[ln[fX(x)]]=ln[α(1θ)(1eλ)αλ]+E[W(x)]=ln[γ(1θ)(1eλ)αλ]+2αλγ(1θ)(1eλ)Nı=02νı(1yı)2W(1+yı1yı)Φ(0)(1+yı1yı).

    Theorem 3.7. Let X1,,Xn is a random sample from the PGLD with CDF (2.9) and PDF (2.10). Then, the PDF and CDF of the i-th order statistic, say Xi:n, are given, respectively, by

    fj:n(x)=j(nj)αλγ(1θ)Ω2(x)(1+xγ)α1[1(1+xγ)α]2×njr1=0j+r11r2=0(1)r1+r2(njr1)(j+r11r2)eλ(1+r2)Ω(x)(1eλ)r1+j, (3.8)
    Fj:n(x)=nr3=jnr3r4=0r3+r4r5=0(1)r4+r5(nr3)(nr3r4)(r3+r4r5)eλr5Ω(x)(1eλ)r3+r4. (3.9)

    Proof. The PDF fj:n(t) of the j-th order statistic, see [18,19], is given by

    fj:n(x)=j(nj)fX(x)[FX(x)]j1[1FX(x)]nj, (3.10)

    where FX(x) and fX(x) are given by Eqs (2.9) and (2.10), respectively.

    Therefore,

    fj:n(x)=j(nj)njr1=0(1)r1(njr1)fX(x)[FX(x)]j+r11=j(nj)αλγ(1θ)Ω2(x)(1+xγ)α1[1(1+xγ)α]2×njr1=0j+r11r2=0(1)r1+r2(njr1)(j+r11r2)eλ(1+r2)Ω(x)(1eλ)r1+j.

    The CDF Fj:n(x), corresponding to PDF (3.10), is given by

    Fj:n(x)=nr3=j(nr3)[FX(x)]r3[1FX(x)]nr3=nr3=jnr3r4=0r3+r4r5=0(1)r4+r5(nr3)(nr3r4)(r3+r4r5)eλr5Ω(x)(1eλ)r3+r4.

    Based on units connected in a series-parallel structure, we discuss, in this section, the application of a progressive-stress model to units whose lifetime distribution subjects to the PGLD with CDF (2.9). We assume that the units are subject to progressive type-II censoring and that the number of surviving units eliminated follows a binomial distribution.

    It is well-known in the previous literature regarding the progressive-stress model that the stress is considered an increasing linear function of time. Now, in the current article, the stress is supposed to be represented by an increasing nonlinear function of time.

    (1) The lifetime of units under normal conditions is governed by CDF (2.9) of PGLD with scale parameter γ.

    (2) According to the progressive-stress model, it is assumed that the stress s is a function of time t and affects the scale parameter γ of CDF (2.7) which is also a scale parameter of CDF (2.9).

    (3) The parameter γ follows the inverse power law with two parameters c and d. This means that γγ(t)=1c(s(t))d. For the sake of simplicity, we'll assume that the parameter d assigns the value 1 from now on.

    (4) The progressive-stress s(t) assigns an increasing nonlinear function of time, s(t)=sinh(vt), which is also continuous and differentiable for t>0.

    (5) To start the testing procedure, the total N units to be tested are split into (2) groups, each of them consists of ni units under progressive-stress si(t)=sinh(vit),i=1,2,,, such that the stress rates satisfy 0<v1<v2<<v.

    (6) At whatever stress level vi,i=1,2,,, a unit's failure mechanisms are the same.

    (7) The cumulative exposure model holds for the effect of changing stress, see [1].

    According to Steps 1, 3, and 5, and using Assumption 7, we can write

    Φi(x)=x01γ(si(t))dt=cvi(cosh(vix)1),i=1,2,,, (4.1)

    where c is a parameter that should be estimated.

    Therefore, if GiY(.) denotes the CDF for a unit in group i under progressive-stress model, then using Assumption 7, it takes the form

    GiY(x)=FiY(Φi(x))=1[1+cvi(cosh(vix)1)]α=1[Ψi(x)]α, (4.2)

    where FiY(.) is the CDF (2.7) of LD, included in (2.9), under group i, with scale parameter value equal to 1 and

    Ψi(x)=Φi(x)+1, (4.3)

    where Φi(x) is given by (4.1).

    The corresponding PDF of (4.2) is given by

    giY(x)=αcsinh(vix)[Ψi(x)]α1. (4.4)

    Then, by replacing FY(y) and fY(y) with CDF (4.2) and PDF (4.4), respectively, CDF (2.9) under progressive-stress ALT becomes

    FiX(x)=1eλΩi(x)1eλ. (4.5)

    The corresponding PDF of (4.5) is given by

    fiX(x)=λαcΩ2i(x) sinh(vi(x))Ψα1i(x)(1θ)(1eλ)eλΩi(x)(1Ψαi(x))2, (4.6)

    where

    Ωi(x)=(1θ)(1Ψαi(x))1θ(1Ψαi(x)),x>0, (4.7)

    and Ψi(x) is given by (4.3).

    There are a variety of censored tests available. Progressive type-II censoring is one of the most widely used censored tests. It is implemented under progressive-stress model as follows: Suppose that, in the i-th group, i=1,2,,, ni units are put through a life test and the experimenter specifies beforehand quantity wi, the number of failure units that will be observed. Now, when the first failure occurs, ri1 of the remaining ni1 surviving units are eliminated from the experiment at random. Continuing, when the second failure occurs, ri2 of the remaining niri12 surviving units are eliminated from the experiment at random. Finally, at the time of occurring the wi-th failure, all the remaining riwi=niwiri1ri2riwi1 surviving units are eliminated from the experiment at random. Note that, in this scheme, ri1,ri2,,riwi are all prefixed. However, these numbers may occur at random, in some practical situations. For example, in some reliability experiments, an experimenter may assess that it is unsuitable or too risky to perform the test on some of the tested units even though these units have not failed. In such situations, the pattern of elimination at each failure is random. Such a situation leads to progressive censoring with random removals, see [20,21].

    We discuss, in this section, two estimation methods (maximum likelihood estimation (MLE) and Bayesian estimation (BE)) for the parameters included in CDF (4.5) under progressive type-II censoring with binomial removals.

    For group i, i=1,2,,, suppose xi1,xi2,,xini are ni lifetimes from a population with CDF (4.5) and PDF (4.6), and x=(x(ri1,riwi)i1:wi:ni,x(ri1,riwi)i2:wi:ni, ,x(ri1,riwi)iwi:wi:ni) is a vector of wi progressively type-II ordered lifetimes out of ni with progressive censoring scheme (ri1,riwi). Suppose also wi and rij are all predetermined before the test. From now on, we will write xij instead of x(ri1,riwi)ij:wi:ni, j=1,2,,wi, for simplicity. Then, based on Eqs (4.2)–(4.7), the conditional likelihood function is given by

    L1(α,λ,θ,c;xR=r)i=1wij=1fiX(xij)[1FiX(xij)]rij=(λαc1θ)i=1wi×i=1wij=1Ω2i(xij) sinh(vi(xij))Ψα1i(xij)(1eλ)ri+1eλΩi(xij)(1Ψαi(xij))2(eλΩi(xij)eλ)rij. (5.1)

    The numbers rij may occur at random in some practical scenarios as a result of unanticipated dropout experimental units. Therefore, we assume that Rij(i=1,2,,,j=1,2,,wi1) are RVs, with realizations rij, subject to the following binomial distributions

    Ri1b(niwi,p),

    whereas,

    (Rijri1,ri2,,ri(j1))b(niwij1k=1rik,p),j=2,3,,wi1.

    Then

    L(α,λ,θ,c;x)=L1(α,λ,θ,c;xR=r)P(Ri1=ri1)×wi1k=2P(Rik=rikRi1=ri1,,Ri(k1)=ri(k1)), (5.2)

    where, for fixed i and j, rij is an integer number satisfying 0rijniwi(ri1+ri2+,ri(j1)),i=1,2,,,j=2,3,,wi1, and

    P(Rij=rijRi(j1)=ri(j1),Ri1=ri1)=(niwij1k=1rikrij)prij(1p)niwijkrik.

    Furthermore, suppose that Rij is independent of Xij for i=1,,, j=1,,wi. Then

    P(R=r)=i=1[P(Ri(wi1)=ri(wi1)Ri(wi2)=ri(wi2),,Ri1=ri1)P(Ri1=ri1)]=i=1[(niwi)!(niwiwi1k=1rik)!wi1k=1rik!pwi1k=1rik(1p)(wi1)(niwi)wi1k=1rik(wik)]. (5.3)

    Since P(R=r) does not depend on the parameters (α,λ,θ,c), hence the MLE of them can be derived by maximizing (5.1). Similarly, (5.1) does not involve the binomial parameter p, the MLE of p can be found by maximizing (5.3) directly. Thus

    (lnL)p=0=1pi=1wi1k=1riki=1{(wi1)(niwi)wi1k=1(wik)rik1p}.

    Therefore,

    ˆp=i=1wi1k=1riki=1(wi1)(niwi)i=1wi1k=1(wik1)rik. (5.4)

    The local Fisher information matrix, I, for (ˆα,ˆλ,ˆθ,ˆc) is the 4×4 symmetric matrix of negative second partial derivatives of £ = \text{ln} L_1 with respect to \alpha , \lambda , \theta , and c , see [1]. Let (\varphi_1 = \alpha, \, \varphi_2 = \lambda, \, \varphi_3 = \theta, \, \varphi_4 = c) . Therefore, matrix {\bf{I}} is given by

    \begin{equation*} {\bf{I}} = -\left(\frac{\partial^2\hat{£}}{\partial \varphi_{i} \partial \varphi_{j}} \right)_{4\times4}, i,j = 1,\dots,4, \end{equation*}

    where the caret \hat{} denotes that the derivative is computed at (\hat{\varphi_1} = \hat{\alpha}, \, \hat{\varphi_2} = \hat{\lambda}, \, \hat{\varphi_3} = \hat{\theta}, \, \hat{\varphi_4} = \hat{c}) . It is easy to get the matrix's elements.

    The local estimate {\bf{V}} of the asymptotic variance-covariance matrix of (\hat{\alpha}, \hat{\lambda}, \hat{\theta}, \hat{c}) can be obtained by inverting matrix {\bf{I}} . Therefore,

    \begin{equation} {\bf{V}} = {\bf{I^{-1}}} = \left(\text{cov}\left(\varphi_{i},\varphi_{j}\right) \right)_{4\times4}, i,j = 1,\dots,4. \end{equation} (5.5)

    The sampling distribution of \frac{\hat{\varphi_i}-\varphi_i}{\sqrt{\text{var}(\hat{\varphi_i})}}, \; i = 1, \dots, 4, follows the general asymptotic theory of MLEs and hence it may be approximated by a standard normal distribution which can be used to create confidence intervals (CIs) for unknown parameters.

    Therefore, a two-sided (1-\eta^{\star})100\% asymptotic CIs for the parameters \varphi_i, \; i = 1, \dots, 4 , can then be created as follows:

    \hat{\varphi_i}\mp z_{\eta^{\star}/2}\sqrt{\text{var}(\hat{\varphi_i})}

    where z_{\eta^{\star}/2} is the value of a standard normal RV that leaves an area \eta^{\star}/2 to the right and \sqrt{\text{var}(\hat{\varphi_i})} can be determined from (5.5).

    It's commonly beneficial in practical applications to have a concept of how long a test should last. Because the time it takes to complete the test is proportional to the expense. For i = 1, \dots, \hbar , the expected termination time under progressive type-II censoring scheme with binomial removals is given by, see [22].

    \begin{equation} \begin{split} E[X_{iw_i} \mid {{\bf R}_i} = {{\bf r}_i}] = &C({{\bf r}_i})\sum\limits_{\ell_1 = 0}^{r_{i1}}\dots \sum\limits_{\ell_{w_i} = 0}^{r_{iw_i}}(-1)^{\mathcal{A}_i} \frac{ \left( \begin{array}{c} {r_{i1}}\\ {\ell_1} \\ \end{array} \right) \dots \left( \begin{array}{c} {r_{iw_i}}\\ {\ell_{w_i}} \\ \end{array} \right) }{\prod_{k = 1}^{w_i-1}h(\ell_k)} \int_{0}^{\infty}x f_X(x) F_X^{h(\ell_{w_i})-1}(x)\text{d}x, \end{split} \end{equation} (5.6)

    where {{\bf R}_i} = (R_{i1} = r_{i1}, \dots, R_{i(w_i-1)} = r_{i(w_i-1)}) , ( F_X(x), f_X(x) ) is given by ((4.5), (4.6)), \mathcal{A}_i = \sum_{k = 1}^{w_i}\ell_k , h(\ell_k) = \ell_1+\dots+ \ell_k+k , and C({{\bf r}_i}) = n_i(n_i-r_{i1}-1)(n_i-r_{i1}-r_{i2}-2)\dots(n_i-\sum_{k = 1}^{w_i-1}(r_{ik}+1)) . Therefore,

    \begin{equation*} \begin{split} E[X_{iw_i}] = &E_{{\bf R}}[E(X_{iw_i} \mid {{\bf R}_i})]\\ = & \sum\limits_{r_{i1} = 0}^{q(r_{i1})} \dots \sum\limits_{r_{i(w_i-1)} = 0}^{q(r_{i(w_i-1)})}P({\bf R} = {\bf r})E(X_{iw_i}\mid {\bf R}), \end{split} \end{equation*}

    where q(r_{i1}) = n_i-w_i, \, q(r_{ij}) = n_i-w_i-r_{i1}-r_{i2}-\dots-r_{i(j-1)}, \, i = 1, 2, \dots, \hbar, \, j = 2, 3, \dots, w_i-1, and P({\bf R} = {\bf r}) is given by Eq (5.3). Then compute the ratio of expected experiment time (REET) as follows:

    REET = \frac{E(X_{iw_i})}{E(X_{in_i})}.

    Based on two asymmetric loss functions (general entropy (GE) and linear exponential (LINEX)), we discuss the Bayesian estimation of the parameters of CDF (4.5). Because they offer overestimation or underestimation of the parameters, symmetric loss functions may be unsuitable in many real-life situations. Overestimating the parameters can have worse or worse repercussions than underestimating them or vice versa. As a result, asymmetric loss functions have been the subject of research, see [23,24].

    The LINEX loss function was suggested by Varian [25]. It is given by

    \mathcal{L}(\xi)\propto e^{\nu \xi}- \nu \xi-1, \nu\neq 0,

    where \xi = \tilde{\Theta}-\Theta and \tilde{\Theta} is the LINEX estimator of \Theta .

    The Bayes estimate under LINEX (BEL) loss function of \Theta is given by

    \begin{equation} \begin{split} \tilde{\Theta} = \frac{-1}{\nu}\ln[E({e^{-\nu \Theta}}|{{\bf{x}}})]. \end{split} \end{equation} (5.7)

    The GE loss function was introduced by Calabria and Pulcini [26]. It is given by

    \mathcal{L}(\ddot{\Theta},\Theta)\propto \left(\frac{\ddot{\Theta}}{\Theta}\right)^{\nu}-\nu\ln\left(\frac{\ddot{\Theta}}{\Theta}\right)-1, \nu\neq 0.

    The Bayes estimate under GE (BEG) loss function of \Theta is given by

    \begin{equation} \begin{split} \ddot{\Theta} = \left[E(\Theta^{-\nu})\right]^{\frac{-1}{\nu}}. \end{split} \end{equation} (5.8)

    Assume that the experimenter's prior belief is measured by a function \vartheta(\alpha, \lambda, \theta, c) , with all parameters being independent and having log-normal distributions except \theta , which has a beta distribution. Therefore, if (\varphi_1 = \alpha, \, \varphi_2 = \lambda, \varphi_3 = c, \varphi_4 = \theta) , then the prior function of \varphi_i , i = 1, 2, 3 , is given by

    \begin{equation} \vartheta_i(\varphi_i) = \frac{1}{\sigma_i\varphi_i \sqrt{2 \pi}}\text{exp}\left\{-\frac{1}{2}\left(\frac{\text{ln } \varphi_i-\mu_i}{\sigma_i}\right)^{2}\right\},\; \varphi_i > 0,\; (-\infty < \mu_i < \infty,\, \sigma_i > 0), \end{equation} (5.9)

    and the prior function of \varphi_4 is given by

    \begin{equation} \vartheta_4(\varphi_4) = \frac{1}{B(a_1,a_2)}\varphi_4^{a_1-1}(1-\varphi_4)^{a_2-1},\; 0 < \varphi_4 < 1, \, (a_1,a_2 > 0). \end{equation} (5.10)

    The joint prior density function is then calculated as follows:

    \begin{equation} \vartheta(\alpha,\lambda,\theta,c) = \vartheta_{1}(\alpha)\, \vartheta_{2}(\lambda)\, \vartheta_{3}(c)\, \vartheta_{4}(\theta)\propto \frac{1}{\alpha\lambda c}e^{-\Delta}\theta^{a_1-1}(1-\theta)^{a_2-1}, \end{equation} (5.11)
    \Delta = \frac{1}{2}\left\{\left(\frac{\text{ln } \alpha-\mu_1}{\sigma_1}\right)^{2}+\left(\frac{\text{ln } \lambda-\mu_2}{\sigma_2}\right)^{2}+\left(\frac{\text{ln } c-\mu_3}{\sigma_3}\right)^{2}\right\}.

    From (5.1) and (5.11), the joint posterior density function is then calculated as follows:

    \begin{equation} \begin{split} \vartheta^{*}(\alpha,\lambda,\theta,c|{{\bf{x}}}, {{\bf{r}}})& = K^{-1}\frac{\alpha^{\sum\limits_{i = 1}^\hbar w_i-1} \lambda^{\sum\limits_{i = 1}^\hbar w_i-1} c^{\sum\limits_{i = 1}^\hbar w_i-1}}{(1-e^{-\lambda})^{\sum\limits_{i = 1}^{\hbar}(w_i+\sum\limits_{j = 1}^{w_i}r_{ij})}} \frac{\theta^{a_1-1}e^ {-\Delta}}{(1-\theta)^{\sum\limits_{i = 1}^{\hbar}w_i-a_2+1}}\\\\& \times \prod\limits_{i = 1}^{\hbar}\prod\limits_{j = 1}^{w_i} \frac{\Omega_{i}^{2}(x_{ij})\text{ sinh}(v_i\,x_{ij})(e^{-\lambda \Omega_i(x_{ij})}-e^{-\lambda})^{r_{ij}}}{[1-(\Psi_{i}(x_{ij}))^{-\alpha}]^2[\Psi_{i}(x_{ij})]^{\alpha+1}e^{\lambda \Omega_i(x_{ij})}}, \end{split} \end{equation} (5.12)

    where

    K = \int_{0}^{\infty}\int_{0}^{1}\int_{0}^{\infty}\int_{0}^{\infty}\vartheta(\alpha,\lambda,\theta,c) L(\alpha,\lambda,\theta,c)\text{ d}\alpha\text{ d}\lambda\text{ d}\theta\text{ d}c.

    It can be noted that K involves quad integral and it is not reducible in a closed form, and hence generating samples directly from the joint posterior density is not possible. The MCMC algorithm, presented in the following subsection, can be implemented in this case in which we need the following conditional posterior distributions of the parameters \alpha , \lambda , \theta and c ,

    \begin{equation} \left. \begin{split} \vartheta^{*}(\alpha\mid \lambda,\theta,c)& \propto \alpha^{\sum\limits_{i = 1}^{\hbar}w_i-1}\text{exp}\left[-\frac{1}{2}\left(\frac{\text{ln }\alpha-\mu_1}{\sigma_1}\right)^{2}\right] \\& \times\prod\limits_{i = 1}^{\hbar}\prod\limits_{j = 1}^{w_i}\frac{\Omega_{i}^{2}(x_{ij})(e^{-\lambda \Omega_i(x_{ij})}-e^{-\lambda})^{r_{ij}}}{[1-(\Psi_{i}(x_{ij}))^{-\alpha}]^2[\Psi_{i}(x_{ij})]^{\alpha+1}e^{\lambda \Omega_i(x_{ij})}}, \\ \vartheta^{*}(\lambda\mid \alpha,\theta,c)& \propto \frac{\lambda^{\sum\limits_{i = 1}^\hbar w_i-1} }{(1-e^{-\lambda})^{\sum\limits_{i = 1}^{\hbar}(w_i+\sum\limits_{j = 1}^{w_i}r_{ij})}} \text{exp}\left[-\frac{1}{2}\left(\frac{\text{ln }\lambda-\mu_2}{\sigma_2}\right)^{2}\right] \\ & \times \prod\limits_{i = 1}^{\hbar}\prod\limits_{j = 1}^{w_i} \frac{(e^{-\lambda \Omega_i(x_{ij})}-e^{-\lambda})^{r_{ij}}}{e^{\lambda \Omega_i(x_{ij})}}, \\ \vartheta^{*}(\theta\mid \alpha,\lambda,c)& \propto \frac{\theta^{a_1-1}}{(1-\theta)^{\sum\limits_{i = 1}^{\hbar}w_i-a_2+1}}\prod\limits_{i = 1}^{\hbar}\prod\limits_{j = 1}^{w_i} \frac{\Omega_{i}^{2}(x_{ij})(e^{-\lambda \Omega_i(x_{ij})}-e^{-\lambda})^{r_{ij}}}{e^{\lambda \Omega_i(x_{ij})}}, \\ \vartheta^{*}(c\mid \alpha,\lambda,\theta)&\propto c^{\sum\limits_{i = 1}^{\hbar}w_i-1}\text{exp}\left[-\frac{1}{2}\left(\frac{\text{ln }c-\mu_3}{\sigma_3}\right)^{2}\right] \\ & \times\prod\limits_{i = 1}^{\hbar}\prod\limits_{j = 1}^{w_i}\frac{\Omega_{i}^{2}(x_{ij})(e^{-\lambda \Omega_i(x_{ij})}-e^{-\lambda})^{r_{ij}}}{[1-(\Psi_{i}(x_{ij}))^{-\alpha}]^2[\Psi_{i}(x_{ij})]^{\alpha+1}e^{\lambda \Omega_i(x_{ij})}}. \end{split}\right\} \end{equation} (5.13)

    The Metropolis-Hasting technique can be used if the conditional posterior distribution isn't one of the known parametric distributions. Then, it can be used to generate samples from conditional posterior distributions using the MCMC algorithm, see [27].

    The following procedure can be used to compute BELs and BEGs of \alpha , \lambda , \theta , and c ,

    (1) Assign some initial values of \alpha , \lambda , \theta and c say \alpha_{0} , \lambda_{0} , \theta_{0} and c_{0} .

    (2) For i = 1 , using Metropolis-Hastings technique, generate \alpha_{i} , \lambda_{i} , \theta_{i} and c_{i} from the conditional posterior distributions presented in (5.13).

    (3) Repeat Step 2, \mathbb{M} times.

    (4) Calculate the BELs of \alpha , \lambda , \theta and c , using Eq (5.7), as

    \begin{equation} \left.\begin{split} \tilde{\alpha}& = \frac{-1}{\nu}\ln\left[ \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}e^{-\nu \alpha_{i}}\right], \tilde{\lambda} = \frac{-1}{\nu}\ln\left[ \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}e^{-\nu \lambda_{i}}\right],\\ \tilde{\theta}& = \frac{-1}{\nu}\ln\left[ \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}e^{-\nu \theta_{i}}\right], \tilde{c} = \frac{-1}{\nu}\ln\left[ \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}e^{-\nu c_{i}}\right], \end{split}\right\} \end{equation} (5.14)

    where \mathbb{W} is the burn-in period.

    (5) Calculate the BEGs of \alpha , \lambda , \theta and c , using Eq (5.8), as follows:

    \begin{equation} \left.\begin{split} \ddot{\alpha}& = \left( \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}\alpha_{i}^{-\nu}\right)^{\frac{-1}{\nu}}, \ddot{\lambda} = \left( \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}\lambda_{i}^{-\nu}\right)^{\frac{-1}{\nu}},\\ \ddot{\theta}& = \left( \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}\theta_{i}^{-\nu}\right)^{\frac{-1}{\nu}}, \ddot{c} = \left( \frac{1}{\mathbb{M}-\mathbb{W}}\sum\limits_{i = \mathbb{W}+1}^{\mathbb{M}}c_{i}^{-\nu}\right)^{\frac{-1}{\nu}}. \end{split}\right\} \end{equation} (5.15)

    (6) The highest posterior density (HPD) credible interval of parameter \alpha can be computed by arranging in an ascending order \alpha_{\mathbb{W}+1} , \dots, \alpha_{\mathbb{M}} as \alpha_{[1]} < \dots < \alpha_{[\mathbb{M}-\mathbb{W}]} , then compute the lower and upper bounds of all (1-\eta^{\star})100\% credible intervals of \alpha as follows:

    \left(\alpha_{[1]},\alpha_{[(\mathbb{M}-\mathbb{W})(1-\eta^{\star})+1]}\right),\dots,\left(\alpha_{[(\mathbb{M}-\mathbb{W})\eta^{\star}]}, \alpha_{[\mathbb{M}-\mathbb{W}]}\right),

    where [x] denotes the largest integer number less than or equal to x . Then the HPD credible interval of \alpha is the one with the shortest length. The HPD credible interval of \lambda , \theta and c can also be computed in the same way.

    (7) The symmetric credible intervals of \alpha can be computed as follows:

    \left(\alpha_{[(\mathbb{M}-\mathbb{W})\frac{\eta^{\star}}{2}]}, \alpha_{[(\mathbb{M}-\mathbb{W})(1-\frac{\eta^{\star}}{2})]}\right).

    The symmetric credible intervals of \lambda , \theta and c can also be computed in the same way.

    Two real data sets are proposed, in this section, for fitting and comparing the PGLD, Poisson-Lomax distribution (PLD) [28], geometric-Lomax distribution (GLD), exponentiated LD (ELD) [29] and LD with CDF (2.7).

    The CDFs of PLD, GLD, and ELD are given, respectively, by

    \begin{equation} \left. \begin{split} F_{PLD}& = \frac{e^{-\lambda \left(1+\frac{x}{\gamma}\right)^{-\alpha} } -e^{-\lambda}} {1-e^{-\lambda}}, \\ F_{GLD}& = \frac{(1-\theta)\left[1-\left(1+\frac{x}{\gamma}\right)^{-\alpha}\right]}{1-\theta\left[1-\left(1+\frac{x}{\gamma}\right)^{-\alpha}\right]},\\ F_{ELD}& = \left[1-\left(1+\frac{x}{\gamma}\right)^{-\alpha}\right]^{\lambda}.\\ \end{split}\right\} \end{equation} (6.1)

    It can be noticed that the GLD is a special case of the PGLD as \lambda\rightarrow 0^+ .

    ● The first data set is taken from [30]. It consists of 72 exceedances for the years from 1958 to 1984, rounded to one decimal place. The data are given as follows:

    1.7, 2.2, 14.4, 1.1, 0.4, 20.6, 5.3, 0.7, 1.9, 13.0, 12.0, 9.3, 1.4, 18.7, 8.5, 25.5, 11.6, 14.1, 22.1, 1.1, 2.5, 14.4, 1.7, 37.6, 0.6, 2.2, 39.0, 0.3, 15.0, 11.0, 7.3, 22.9, 1.7, 0.1, 1.1, 0.6, 9.0, 1.7, 7.0, 20.1, 0.4, 2.8, 14.1, 9.9, 10.4, 10.7, 30.0, 3.6, 5.6, 30.8, 13.3, 4.2, 25.5, 3.4, 11.9, 21.5, 27.6, 36.4, 2.7, 64.0, 1.5, 2.5, 27.4, 1.0, 27.1, 20.2, 16.8, 5.3, 9.7, 27.5, 2.5, 27.0.

    ● The second data set represents the marks of 48 slow space students in Mathematics in the final examination of the Indian Institute of Technology, Kanpur in year 2003, [31]. The data are given as follows:

    29, 25, 50, 15, 13, 27, 15, 18, 7, 7, 8, 19, 12, 18, 5, 21, 15, 86, 21, 15, 14, 39, 15, 14, 70, 44, 6, 23, 58, 19, 50, 23, 11, 6, 34, 18, 28, 34, 12, 37, 4, 60, 20, 23, 40, 65, 19, 31.

    The Kolmogorov-Smirnov (K-S) statistic and its corresponding p-value are used to check the validity of the PGLD, PLD, GLD, ELD, and LD to fit the above two data sets. The results are shown in Table 1. Also, the results of a comparison among these five distributions using some criteria such as the Akaike information criterion (AIC), consistent AIC (CAIC), and Bayesian information criterion (BIC), are shown in Table 1, where

    \text{AIC} = 2\,r-2£(\hat{\beta}), \text{CAIC} = \frac{2\,r\, w}{w-r-1}-2£(\hat{\beta}), \text{BIC} = r\,\ln[w]-2£(\hat{\beta}),
    Table 1.  The MLEs, K-S statistic, p-value, AIC, CAIC, and BIC for the two data sets.
    The first data set
    Model \hat{\alpha} \hat{\gamma} \hat{\theta} \hat{\lambda} K-S p-value AIC CAIC BIC
    PGLD 1.40525 1.34963 0.94075 0.76069 0.109102 0.35816 522.134 522.731 531.241
    PLD 1.12565 5.44626 --- 0.07480 0.178738 0.02010 525.967 526.320 532.797
    GLD 1.00741 2.49201 0.60639 --- 0.111083 0.33669 525.289 525.642 532.119
    ELD 0.66113 1.19104 --- 1.59821 0.165565 0.03861 536.672 537.025 543.502
    LD 1.10933 4.34354 --- --- 0.233859 0.00076 529.953 530.127 534.506
    The second data set
    Model \hat{\alpha} \hat{\gamma} \hat{\theta} \hat{\lambda} K-S p-value AIC CAIC BIC
    PGLD 2.49409 0.63477 0.99986 0.20566 0.05039 0.99971 402.596 403.526 410.08
    PLD 149.855 3788.06 --- 0.72799 0.11165 0.58773 412.330 412.875 417.943
    GLD 1.42011 5.41074 0.84701 --- 0.21077 0.02811 425.597 426.143 431.211
    ELD 0.27741 2.35554 --- 0.79642 0.31822 0.00012 498.599 499.145 504.213
    LD 22.3092 552.211 --- --- 0.19730 0.04765 413.502 413.769 417.244

     | Show Table
    DownLoad: CSV

    where £(\hat{\beta}) stands for the log-likelihood function calculated at the MLE \hat{\beta} of \beta , r and w denote the number of parameters and the sample size, respectively.

    According to the values of K-S statistic and its corresponding p-value, presented in Table 1, it's worth noting that the PGLD has the smallest(largest) K-S (p-)values than those for the PLD, GLD, ELD, and LD. Therefore, the PGLD is a better fit for the data than the other four distributions. Since the PGLD has the smallest values of AIC, CAIC, and BIC, then this is considered another indicator of the superiority of the PGLD. Figure 4 shows the comparison graphically by plotting the empirical CDF against the CDF of PGLD, PLD, GLD, ELD, and LD. In Table 1, we note that the PLD, ELD, and LD (GLD, ELD, and LD) do not fit well the first (second) data set (based on the p-value ( < 0.05 )) but we use them for comparison purposes.

    Figure 4.  Left (Right) panel: Empirical CDF versus CDF of PGLD, PLD, GLD, ELD, and LD for the first (second) data set.

    In this section, a simulation study is performed to evaluate the performance of the estimation methods presented in Section 5. The MLEs, BELs and BEGs of the parameters \alpha , \lambda , \theta and c are computed and compared, through their mean squared errors (MSEs) and relative absolute biases (RABs), via a Monte Carlo simulation. The 95\% CIs, symmetric and HPD credible intervals are also computed and compared through their average interval lengths (AILs). The following algorithm is used to perform a simulation study:

    (1) For i = 1, \dots, \hbar , generate the values of progressive censoring with binomial removals, r_{ij} , such that R_{ij}\sim Binomial (n_{i}-w_{i}-\sum_{k = 1}^{j-1}R_{ik}, p) distribution, where p is the removal probability, j = 1, \dots, w_{i}-1 and R_{i w_{i}} \; = \; n_{i} \; - \; w_{i} \; - \; \sum_{j = 1}^{w_{i}-1} \; R_{ij} .

    (2) For given values of the prior parameters ( \mu_{1} , \mu_{2} , \mu_{3} , \sigma_{1} , \sigma_{2} , \sigma_{3} , a_{1} , a_{2} ), generate values for the parameters ( \alpha , \lambda , \theta, c ).

    (3) For i = 1, \dots, \hbar , generate a progressively type-II censored sample of size w_{i} from PGLD with CDF (2.9), according to the algorithm given in [32].

    (4) The MLEs, BELs and BEGs of the parameters \alpha , \lambda , \theta and c are computed as shown in Section 5. The BELs and BEGs of the parameters \alpha , \lambda , \theta and c are computed based on \mathbb{M}( = 5500) MCMC samples and discard the first 500 values as burn-in period.

    (5) Repeat the above steps \mathbb{N}( = 1,000) times.

    (6) If \hat{\Theta} is an estimate of \Theta , then the average of estimates, MSE and RAB of \hat{\Theta} over \mathbb{N} samples are given, respectively, by

    \begin{split} \overline{\widehat{\Theta}} = \frac{1}{\mathbb{N}}\sum\limits_{i = 1}^{\mathbb{N}}\hat{\Theta}_{i}, \text{MSE}(\hat{\Theta}) = \frac{1}{\mathbb{N}}\sum\limits_{i = 1}^{\mathbb{N}}(\hat{\Theta}_{i}-\Theta)^{2}, \text{RAB}(\hat{\Theta}) = \frac{1}{\mathbb{N}}\sum\limits_{i = 1}^{\mathbb{N}}\frac{|\hat{\Theta}_{i}-\Theta|}{\Theta}. \end{split}

    (7) Calculate the average of estimates of the parameters \alpha , \lambda , \theta and c and their MSEs and RABs as shown in Step 6. Calculate also the average of the MSEs (MMSE) and the average of the RABs (MRAB) over the four parameter estimates.

    (8) Calculate the 95\% CIs (as shown in Subsection 5.1), symmetric and HPD credible intervals (as shown in Subsection 5.3) of the parameters and then calculate the average interval lengths (AILs) of them. Calculate also the average of the AILs (MAIL) over the four parameter estimates.

    Tables 24 provide the computational results, which take into account the prior parameter values: \mu_1 = 0.154 , \mu_2 = 0.8 , \mu_3 = -1.65 , \sigma_1 = 0.8 , \sigma_2 = 0.07 , \sigma_3 = 0.3 , a_{1} = 2.3 and a_{2} = 0.25 to generate population parameter values: \alpha = 1.6 , \lambda = 2.3 , \theta = 0.9 and c = 0.2 . Three distinct removal probabilities p = 0.15, 0.55, and 0.95 are considered.

    Table 2.  MLEs of \alpha, \lambda, \theta and c with their MSEs, RABs, MMSE and MRAB based on 1,000 simulations. Population parameter values are \alpha = 1.6, \lambda = 2.3, \theta = 0.9 and c = 0.2.
    n_{1} w_{1} p=0.15 p=0.55 p=0.95
    . . \overline{\hat{\alpha}} MSE(\hat{\alpha}) RAB(\hat{\alpha}) MMSE \overline{\hat{\alpha}} MSE(\hat{\alpha}) RAB(\hat{\alpha}) MMSE \overline{\hat{\alpha}} MSE(\hat{\alpha}) RAB(\hat{\alpha}) MMSE
    . . \overline{\hat{\lambda}} MSE(\hat{\lambda}) RAB(\hat{\lambda}) MRAB \overline{\hat{\lambda}} MSE(\hat{\lambda}) RAB(\hat{\lambda}) MRAB \overline{\hat{\lambda}} MSE(\hat{\lambda}) RAB(\hat{\lambda}) MRAB
    . . \overline{\hat{\theta}} MSE(\hat{\theta}) RAB(\hat{\theta}) \overline{\hat{\theta}} MSE(\hat{\theta}) RAB(\hat{\theta}) \overline{\hat{\theta}} MSE(\hat{\theta}) RAB(\hat{\theta})
    \hbar N n_{\hbar} w_{\hbar} \overline{\hat{c}} MSE(\hat{c}) RAB(\hat{c}) \overline{\hat{c}} MSE(\hat{c}) RAB(\hat{c}) \overline{\hat{c}} MSE(\hat{c}) RAB(\hat{c})
    2 80 40 20 1.7692 0.4273 0.2736 0.3766 1.7793 0.4334 0.2855 0.4536 1.7900 0.4439 0.2821 0.4166
    40 20 2.2500 1.3743 0.3825 0.3156 2.5275 1.7338 0.4473 0.3599 2.4325 1.5187 0.4291 0.3729
    0.8399 0.0247 0.1060 0.8214 0.0323 0.1297 0.8232 0.0338 0.1322
    0.2503 0.0567 0.8159 0.2491 0.0684 0.9367 0.2703 0.0868 1.0212
    32 1.7112 0.2631 0.2218 0.4094 1.7118 0.2594 0.2231 0.4408 1.7260 0.2935 0.2333 0.4465
    32 2.4709 1.6977 0.4517 0.3352 2.4682 1.8436 0.4612 0.3533 2.4738 1.8411 0.4750 0.3548
    0.8411 0.0218 0.1107 0.8308 0.0274 0.1234 0.8205 0.0298 0.1328
    0.2607 0.0643 0.8917 0.2649 0.0735 0.9590 0.2546 0.0682 0.9331
    140 70 35 1.7235 0.2732 0.2152 0.3939 1.7104 0.2902 0.2283 0.4677 1.6972 0.2575 0.2121 0.4528
    70 35 2.5368 1.6200 0.4369 0.3218 2.5238 1.9496 0.4756 0.3508 2.5618 1.9192 0.4820 0.3414
    0.8555 0.0153 0.0934 0.8402 0.0231 0.1128 0.8418 0.0224 0.1137
    0.2588 0.0612 0.8638 0.2685 0.0756 0.9375 0.2636 0.0650 0.8993
    56 1.7144 0.2323 0.2087 0.4615 1.6803 0.2312 0.2047 0.4594 1.6890 0.2324 0.2054 0.5033
    56 2.5501 1.9964 0.4725 0.3284 2.4981 1.9889 0.4798 0.3312 2.5337 2.1999 0.4905 0.3413
    0.8505 0.0184 0.1038 0.8517 0.0177 0.1013 0.8474 0.0201 0.1077
    0.2606 0.0606 0.8572 0.2670 0.0593 0.8702 0.2702 0.0641 0.9027
    4 80 20 10 1.7224 0.3564 0.2653 0.3963 1.7933 0.4206 0.2728 0.4094 1.7689 0.4255 0.2812 0.4622
    20 10 2.1620 1.5467 0.4146 0.3086 2.4281 1.5124 0.4312 0.3627 2.5324 1.7754 0.4676 0.3609
    20 10 0.8276 0.0223 0.1074 0.8293 0.0285 0.1225 0.8083 0.0379 0.1416
    20 10 0.2309 0.0559 0.7555 0.2638 0.0856 0.9872 0.2405 0.0723 0.9142
    16 1.7504 0.3104 0.2411 0.3767 1.7214 0.2853 0.2379 0.4418 1.6927 0.2635 0.2251 0.4439
    16 2.4045 1.4904 0.4204 0.3243 2.6169 1.8321 0.4668 0.3464 2.4949 1.8477 0.4627 0.3608
    16 0.8357 0.0229 0.1121 0.8406 0.0222 0.1121 0.8407 0.0263 0.1165
    16 0.2460 0.0595 0.8481 0.2565 0.0694 0.9153 0.2862 0.0817 0.9996
    140 35 18 1.6976 0.2483 0.2171 0.3170 1.7063 0.2604 0.2181 0.4347 1.7152 0.2896 0.2212 0.4394
    35 18 2.3230 1.2643 0.3762 0.2965 2.4760 1.8169 0.4667 0.3469 2.5477 1.8211 0.4638 0.3350
    35 18 0.8554 0.0137 0.0869 0.8357 0.0240 0.1178 0.8412 0.0219 0.1093
    35 18 0.2548 0.0588 0.8022 0.2669 0.0723 0.9320 0.2561 0.0645 0.8805
    28 1.6775 0.1812 0.1846 0.4331 1.6684 0.1758 0.1888 0.4781 1.6867 0.1760 0.1864 0.4443
    28 2.5388 1.9152 0.4670 0.3084 2.5493 2.1323 0.4914 0.3330 2.4572 1.9641 0.4774 0.3251
    28 0.8499 0.0179 0.0998 0.8572 0.0176 0.0985 0.8508 0.0179 0.1009
    28 0.2490 0.0510 0.7907 0.2744 0.0648 0.8863 0.2647 0.0633 0.8609

     | Show Table
    DownLoad: CSV
    Table 3.  BELs and BEGs of \alpha, \lambda, \theta and c with their MSEs, RABs, MMSE and MRAB based on 5500 MCMC samples and 1,000 simulations. Population parameter values are \alpha = 1.6, \lambda = 2.3, \theta = 0.9 and c = 0.2.
    n_{1} m_{1} BEL BEG
    . . \nu=-0.5 \nu=0.5 \nu=-0.5 \nu=0.5
    . . \overline{\tilde{\alpha}} MSE(\tilde{\alpha}) RAB(\tilde{\alpha}) MMSE \overline{\tilde{\alpha}} MSE(\tilde{\alpha}) RAB(\tilde{\alpha}) MMSE \overline{\ddot{\alpha}} MSE(\ddot{\alpha}) RAB(\ddot{\alpha}) MMSE \overline{\ddot{\alpha}} MSE(\ddot{\alpha}) RAB(\ddot{\alpha}) MMSE
    . . \overline{\tilde{\lambda}} MSE(\tilde{\lambda}) RAB(\tilde{\lambda}) MRAB \overline{\tilde{\lambda}} MSE(\tilde{\lambda}) RAB(\tilde{\lambda}) MRAB \overline{\ddot{\lambda}} MSE(\ddot{\lambda}) RAB(\ddot{\lambda}) MRAB \overline{\ddot{\lambda}} MSE(\ddot{\lambda}) RAB(\ddot{\lambda}) MRAB
    . . \overline{\tilde{\theta}} MSE(\tilde{\theta}) RAB(\tilde{\theta}) \overline{\tilde{\theta}} MSE(\tilde{\theta}) RAB(\tilde{\theta}) \overline{\ddot{\theta}} MSE(\ddot{\theta}) RAB(\ddot{\theta}) \overline{\ddot{\theta}} MSE(\ddot{\theta}) RAB(\ddot{\theta})
    \hbar N n_{\hbar} m_{\hbar} p \overline{\tilde{c}} MSE(\tilde{c}) RAB(\tilde{c}) \overline{\tilde{c}} MSE(\tilde{c}) RAB(\tilde{c}) \overline{\ddot{c}} MSE(\ddot{c}) RAB(\ddot{c}) \overline{\ddot{c}} MSE(\ddot{c}) RAB(\ddot{c})
    2 80 40 20 0.15 1.6520 0.1912 0.1819 0.0505 1.5559 0.1342 0.1819 0.0369 1.5742 0.1662 0.0161 0.0448 1.5138 0.1567 0.0539 0.0433
    40 20 2.2385 0.0042 0.0268 0.0790 2.2262 0.0058 0.0321 0.0819 2.2296 0.0053 0.0306 0.0356 2.2241 0.0061 0.0330 0.0593
    0.8493 0.0064 0.0675 0.8444 0.0073 0.0723 0.8432 0.0076 0.0631 0.8334 0.0098 0.0740
    0.1990 0.0002 0.0398 0.1970 0.0002 0.0414 0.1935 0.0003 0.0325 0.1847 0.0004 0.0764
    0.55 1.6766 0.1464 0.1786 0.0391 1.5945 0.1086 0.1786 0.0302 1.6098 0.1170 0.0061 0.0323 1.5596 0.1139 0.0253 0.0322
    2.2386 0.0040 0.0267 0.0775 2.2264 0.0057 0.0320 0.0801 2.2297 0.0052 0.0306 0.0317 2.2242 0.0060 0.0329 0.0506
    0.8556 0.0056 0.0634 0.8511 0.0064 0.0676 0.8502 0.0066 0.0554 0.8418 0.0084 0.0647
    0.1986 0.0003 0.0411 0.1966 0.0002 0.0420 0.1930 0.0002 0.0349 0.1841 0.0004 0.0796
    0.95 1.6936 0.2794 0.1926 0.0728 1.5992 0.1265 0.1926 0.0351 1.6212 0.1806 0.0132 0.0486 1.5665 0.1388 0.0210 0.0387
    2.2370 0.0045 0.0274 0.0833 2.2247 0.0062 0.0327 0.0856 2.2281 0.0057 0.0313 0.0315 2.2226 0.0065 0.0337 0.0482
    0.8545 0.0058 0.0638 0.8501 0.0066 0.0680 0.8491 0.0069 0.0566 0.8406 0.0087 0.0660
    0.2009 0.0015 0.0495 0.1987 0.0012 0.0491 0.1950 0.0011 0.0250 0.1856 0.0007 0.0722
    32 0.15 1.6671 0.1794 0.1567 0.0477 1.6099 0.1384 0.1567 0.0379 1.6220 0.1559 0.0137 0.0422 1.5873 0.1452 0.0079 0.0400
    32 2.2369 0.0050 0.0274 0.0744 2.2245 0.0067 0.0328 0.0765 2.2279 0.0062 0.0313 0.0278 2.2224 0.0071 0.0337 0.0395
    0.8637 0.0041 0.0533 0.8607 0.0046 0.0561 0.8601 0.0047 0.0443 0.8549 0.0057 0.0501
    0.2012 0.0022 0.0603 0.1992 0.0021 0.0605 0.1956 0.0020 0.0218 0.1867 0.0019 0.0663
    0.55 1.6684 0.0972 0.1476 0.0265 1.6131 0.0793 0.1476 0.0225 1.6235 0.0837 0.0147 0.0235 1.5901 0.0810 0.0062 0.0233
    2.2386 0.0041 0.0267 0.0697 2.2263 0.0058 0.0321 0.0717 2.2297 0.0053 0.0306 0.0297 2.2241 0.0061 0.0330 0.0409
    0.8654 0.0040 0.0523 0.8623 0.0045 0.0551 0.8617 0.0046 0.0425 0.8562 0.0056 0.0486
    0.1995 0.0006 0.0522 0.1974 0.0004 0.0520 0.1938 0.0004 0.0311 0.1848 0.0004 0.0760
    0.95 1.6736 0.1876 0.1626 0.0493 1.6072 0.1008 0.1626 0.0281 1.6207 0.1193 0.0129 0.0326 1.5849 0.1060 0.0094 0.0297
    2.2375 0.0044 0.0272 0.0756 2.2250 0.0061 0.0326 0.0777 2.2285 0.0056 0.0311 0.0284 2.2229 0.0065 0.0335 0.0409
    0.8645 0.0041 0.0546 0.8614 0.0046 0.0576 0.8608 0.0047 0.0436 0.8553 0.0057 0.0497
    0.2004 0.0009 0.0583 0.1984 0.0008 0.0581 0.1948 0.0008 0.0259 0.1858 0.0006 0.0708
    2 140 70 35 0.15 1.6590 0.1425 0.1527 0.0379 1.5986 0.0848 0.1527 0.0239 1.6106 0.0964 0.0066 0.0267 1.5760 0.0870 0.0150 0.0248
    70 35 2.2388 0.0042 0.0266 0.0732 2.2264 0.0059 0.0320 0.0750 2.2298 0.0054 0.0305 0.0261 2.2242 0.0063 0.0329 0.0411
    0.8654 0.0037 0.0501 0.8627 0.0040 0.0527 0.8622 0.0041 0.0420 0.8575 0.0050 0.0472
    0.2006 0.0011 0.0634 0.1985 0.0010 0.0628 0.1950 0.0010 0.0251 0.1861 0.0009 0.0694
    0.55 1.6450 0.1210 0.1422 0.0325 1.5941 0.0912 0.1422 0.0256 1.6039 0.0985 0.0025 0.0273 1.5735 0.0942 0.0166 0.0266
    2.2374 0.0046 0.0272 0.0697 2.2249 0.0063 0.0326 0.0717 2.2283 0.0058 0.0312 0.0255 2.2228 0.0066 0.0336 0.0420
    0.8664 0.0035 0.0486 0.8637 0.0038 0.0511 0.8632 0.0039 0.0409 0.8586 0.0047 0.0460
    0.2000 0.0012 0.0606 0.1980 0.0010 0.0606 0.1945 0.0010 0.0276 0.1857 0.0010 0.0717
    0.95 1.6732 0.1466 0.1516 0.0392 1.6171 0.1051 0.1516 0.0292 1.6285 0.1147 0.0178 0.0315 1.5960 0.1067 0.0025 0.0298
    2.2373 0.0045 0.0273 0.0743 2.2249 0.0062 0.0327 0.0758 2.2283 0.0057 0.0312 0.0279 2.2227 0.0065 0.0336 0.0381
    0.8660 0.0038 0.0504 0.8631 0.0042 0.0530 0.8626 0.0043 0.0416 0.8577 0.0052 0.0470
    0.2018 0.0018 0.0681 0.1995 0.0013 0.0660 0.1958 0.0012 0.0211 0.1861 0.0007 0.0693
    56 0.15 1.6251 0.0461 0.1064 0.0135 1.5991 0.0443 0.1064 0.0135 1.6038 0.0451 0.0024 0.0136 1.5871 0.0459 0.0081 0.0140
    56 2.2382 0.0047 0.0275 0.0676 2.2258 0.0061 0.0327 0.0693 2.2292 0.0057 0.0308 0.0286 2.2237 0.0064 0.0332 0.0354
    0.8732 0.0026 0.0437 0.8717 0.0027 0.0451 0.8715 0.0028 0.0317 0.8694 0.0031 0.0340
    0.1920 0.0007 0.0926 0.1914 0.0007 0.0929 0.1901 0.0007 0.0497 0.1867 0.0008 0.0665
    0.55 1.6321 0.0503 0.1114 0.0144 1.6059 0.0477 0.1114 0.0143 1.6108 0.0486 0.0067 0.0144 1.5943 0.0486 0.0036 0.0147
    2.2383 0.0041 0.0268 0.0688 2.2261 0.0058 0.0321 0.0707 2.2295 0.0053 0.0307 0.0280 2.2240 0.0061 0.0330 0.0325
    0.8742 0.0027 0.0441 0.8727 0.0028 0.0455 0.8725 0.0029 0.0305 0.8703 0.0032 0.0330
    0.1931 0.0007 0.0930 0.1925 0.0007 0.0937 0.1912 0.0007 0.0439 0.1879 0.0008 0.0603
    0.95 1.6471 0.0524 0.1129 0.0150 1.6211 0.0491 0.1129 0.0146 1.6260 0.0501 0.0163 0.0147 1.6098 0.0497 0.0061 0.0149
    2.2388 0.0041 0.0266 0.0692 2.2266 0.0057 0.0319 0.0708 2.2299 0.0052 0.0305 0.0310 2.2245 0.0060 0.0328 0.0339
    0.8754 0.0026 0.0438 0.8739 0.0028 0.0451 0.8737 0.0028 0.0292 0.8716 0.0031 0.0316
    0.1924 0.0009 0.0935 0.1917 0.0008 0.0934 0.1904 0.0008 0.0481 0.1870 0.0008 0.0652
    4 80 20 10 0.15 1.6816 0.2985 0.2183 0.0779 1.5568 0.1760 0.2183 0.0480 1.5815 0.2294 0.0116 0.0613 1.5056 0.2066 0.0590 0.0566
    20 10 2.2379 0.0047 0.0270 0.0922 2.2255 0.0064 0.0324 0.0951 2.2289 0.0059 0.0309 0.0344 2.2234 0.0067 0.0333 0.0617
    20 10 0.8448 0.0075 0.0751 0.8391 0.0087 0.0808 0.8376 0.0091 0.0693 0.8255 0.0122 0.0827
    20 10 0.2006 0.0010 0.0484 0.1986 0.0009 0.0487 0.1949 0.0009 0.0256 0.1856 0.0008 0.0718
    0.55 1.6668 0.1261 0.1730 0.0340 1.5845 0.1048 0.1730 0.0292 1.5992 0.1108 0.0005 0.0307 1.5476 0.1108 0.0328 0.0314
    2.2381 0.0041 0.0269 0.0753 2.2259 0.0057 0.0322 0.0780 2.2292 0.0053 0.0308 0.0303 2.2237 0.0061 0.0332 0.0523
    0.8549 0.0055 0.0628 0.8505 0.0063 0.0671 0.8495 0.0065 0.0561 0.8411 0.0083 0.0654
    0.1987 0.0001 0.0385 0.1968 0.0001 0.0399 0.1932 0.0001 0.0340 0.1844 0.0003 0.0779
    0.95 1.6906 0.2507 0.1933 0.0656 1.5998 0.1302 0.1933 0.0360 1.6194 0.1676 0.0121 0.0453 1.5667 0.1410 0.0208 0.0393
    2.2378 0.0044 0.0271 0.0835 2.2254 0.0061 0.0324 0.0858 2.2288 0.0056 0.0310 0.0302 2.2233 0.0064 0.0334 0.0471
    0.8568 0.0059 0.0631 0.8524 0.0066 0.0670 0.8515 0.0069 0.0539 0.8431 0.0087 0.0632
    0.2011 0.0016 0.0507 0.1989 0.0013 0.0504 0.1952 0.0012 0.0238 0.1858 0.0009 0.0709
    16 0.15 1.6605 0.1649 0.1614 0.0439 1.5951 0.1106 0.1614 0.0308 1.6083 0.1254 0.0052 0.0344 1.5705 0.1164 0.0185 0.0326
    16 2.2374 0.0048 0.0272 0.0770 2.2249 0.0066 0.0327 0.0790 2.2283 0.0061 0.0312 0.0271 2.2227 0.0069 0.0336 0.0442
    16 0.8620 0.0042 0.0546 0.8587 0.0047 0.0577 0.8581 0.0049 0.0466 0.8523 0.0060 0.0530
    16 0.2007 0.0016 0.0648 0.1986 0.0014 0.0643 0.1949 0.0014 0.0255 0.1856 0.0012 0.0718
    0.55 1.6862 0.2183 0.1632 0.0570 1.6170 0.1042 0.1632 0.0290 1.6330 0.1422 0.0206 0.0384 1.5955 0.1136 0.0028 0.0316
    2.2372 0.0046 0.0273 0.0761 2.2246 0.0063 0.0328 0.0781 2.2280 0.0058 0.0313 0.0315 2.2224 0.0067 0.0337 0.0406
    0.8645 0.0040 0.0524 0.8614 0.0045 0.0552 0.8609 0.0046 0.0435 0.8556 0.0056 0.0493
    0.1997 0.0011 0.0616 0.1975 0.0009 0.0612 0.1939 0.0008 0.0306 0.1847 0.0007 0.0765
    0.95 1.6709 0.1323 0.1523 0.0353 1.6149 0.1007 0.1523 0.0279 1.6261 0.1143 0.0163 0.0312 1.5927 0.1076 0.0046 0.0300
    2.2373 0.0044 0.0273 0.0709 2.2249 0.0061 0.0327 0.0732 2.2283 0.0056 0.0312 0.0314 2.2227 0.0065 0.0336 0.0415
    0.8652 0.0040 0.0512 0.8621 0.0045 0.0540 0.8615 0.0046 0.0427 0.8562 0.0056 0.0486
    0.1985 0.0005 0.0529 0.1965 0.0004 0.0537 0.1929 0.0004 0.0353 0.1841 0.0005 0.0794
    4 140 35 18 0.15 1.6763 0.2148 0.1731 0.0564 1.6019 0.1085 0.1731 0.0303 1.6175 0.1303 0.0109 0.0356 1.5767 0.1137 0.0145 0.0318
    35 18 2.2362 0.0048 0.0278 0.0825 2.2236 0.0067 0.0332 0.0841 2.2270 0.0061 0.0317 0.0269 2.2213 0.0071 0.0342 0.0416
    35 18 0.8644 0.0041 0.0524 0.8615 0.0045 0.0551 0.8609 0.0046 0.0434 0.8559 0.0056 0.0491
    35 18 0.2016 0.0022 0.0768 0.1993 0.0017 0.0750 0.1957 0.0016 0.0216 0.1863 0.0010 0.0685
    0.55 1.6899 0.1523 0.1532 0.0403 1.6366 0.0997 0.1532 0.0277 1.6488 0.1222 0.0305 0.0332 1.6177 0.1049 0.0111 0.0292
    2.2373 0.0047 0.0273 0.0727 2.2248 0.0064 0.0327 0.0745 2.2282 0.0059 0.0312 0.0304 2.2227 0.0068 0.0336 0.0383
    0.8710 0.0032 0.0467 0.8685 0.0035 0.0488 0.8682 0.0035 0.0354 0.8643 0.0042 0.0397
    0.2006 0.0012 0.0638 0.1986 0.0010 0.0634 0.1951 0.0010 0.0246 0.1862 0.0009 0.0688
    0.95 1.6470 0.1052 0.1398 0.0284 1.5957 0.0697 0.1398 0.0200 1.6053 0.0744 0.0033 0.0211 1.5757 0.0717 0.0152 0.0208
    2.2387 0.0041 0.0266 0.0689 2.2262 0.0058 0.0321 0.0707 2.2296 0.0053 0.0306 0.0264 2.2240 0.0061 0.0330 0.0424
    0.8657 0.0036 0.0495 0.8630 0.0040 0.0520 0.8625 0.0041 0.0417 0.8580 0.0048 0.0466
    0.1997 0.0007 0.0596 0.1976 0.0006 0.0589 0.1940 0.0005 0.0301 0.1850 0.0005 0.0749
    28 0.15 1.6453 0.0505 0.1087 0.0144 1.6178 0.0469 0.1087 0.0140 1.6230 0.0480 0.0143 0.0141 1.6058 0.0475 0.0036 0.0143
    28 2.2397 0.0039 0.0262 0.0682 2.2273 0.0056 0.0316 0.0701 2.2307 0.0051 0.0301 0.0312 2.2252 0.0059 0.0325 0.0339
    28 0.8757 0.0024 0.0420 0.8742 0.0026 0.0433 0.8740 0.0026 0.0288 0.8720 0.0029 0.0311
    28 0.1915 0.0008 0.0961 0.1910 0.0008 0.0968 0.1897 0.0008 0.0516 0.1863 0.0009 0.0683
    0.55 1.6337 0.0485 0.1090 0.0139 1.6079 0.0459 0.1090 0.0137 1.6127 0.0468 0.0079 0.0138 1.5964 0.0467 0.0023 0.0141
    2.2386 0.0041 0.0267 0.0676 2.2265 0.0057 0.0320 0.0694 2.2298 0.0052 0.0305 0.0280 2.2244 0.0060 0.0329 0.0319
    0.8756 0.0024 0.0417 0.8741 0.0026 0.0431 0.8739 0.0027 0.0290 0.8717 0.0030 0.0315
    0.1929 0.0007 0.0930 0.1923 0.0007 0.0935 0.1911 0.0007 0.0447 0.1878 0.0008 0.0611
    0.95 1.6310 0.0469 0.1062 0.0135 1.6051 0.0445 0.1062 0.0134 1.6099 0.0453 0.0062 0.0135 1.5935 0.0454 0.0041 0.0138
    2.2386 0.0040 0.0267 0.0675 2.2264 0.0057 0.0320 0.0693 2.2298 0.0052 0.0305 0.0294 2.2243 0.0060 0.0329 0.0342
    0.8733 0.0026 0.0439 0.8718 0.0028 0.0453 0.8715 0.0028 0.0316 0.8693 0.0031 0.0341
    0.1921 0.0007 0.0934 0.1915 0.0007 0.0938 0.1902 0.0007 0.0491 0.1869 0.0008 0.0657

     | Show Table
    DownLoad: CSV
    Table 4.  95\% CIs, symmetric credible intervals, HPD credible intervals for \alpha, \lambda, \theta and c with their AILs and MAILs based on 5500 MCMC samples and 1,000 simulations. Population parameter values are \alpha = 1.6, \lambda = 2.3, \theta = 0.9 and c = 0.2.
    n_{1} w_{1} Credible interval
    . . CI Symmetric HPD
    . . AIL(\alpha) MAIL AIL(\alpha) MAIL AIL(\alpha) MAIL
    . . AIL(\lambda) AIL(\lambda) AIL(\lambda)
    . . AIL(\theta) AIL(\theta) AIL(\theta)
    \hbar N n_{\hbar} w_{\hbar} p AIL(c) AIL(c) AIL(c)
    2 80 40 20 0.15 3.4146 3.0673 1.6523 0.7144 1.5547 0.6651
    40 20 9.3383 0.6109 0.5824
    1.0622 0.3577 0.3046
    1.5215 0.2369 0.2186
    0.55 3.2483 3.0103 1.5301 0.6792 1.4479 0.6347
    9.0989 0.6125 0.5825
    1.1630 0.3370 0.2883
    1.5413 0.2372 0.2199
    0.95 3.2459 3.009 1.5365 0.6822 1.4581 0.6387
    9.0252 0.6136 0.5840
    1.1423 0.3394 0.2911
    1.6318 0.2392 0.2214
    32 0.15 2.7872 2.7832 1.2546 0.5955 1.1861 0.5567
    32 8.7304 0.6134 0.5833
    1.0233 0.2796 0.2412
    1.3750 0.2345 0.2164
    0.55 2.8056 2.7834 1.2551 0.5965 1.1847 0.5568
    8.6419 0.6141 0.5831
    1.0474 0.2795 0.2408
    1.4224 0.2372 0.2188
    0.95 2.8068 2.765 1.2616 0.5985 1.1935 0.5598
    8.5702 0.6150 0.5858
    1.0997 0.2818 0.2425
    1.3484 0.2357 0.2174
    140 70 35 0.15 2.8299 2.7787 1.2480 0.5913 1.1732 0.5512
    70 35 8.8112 0.6169 0.5869
    0.9287 0.2635 0.2278
    1.3237 0.2366 0.2171
    0.55 2.6886 2.7106 1.1792 0.5731 1.1093 0.5345
    8.5189 0.6155 0.5842
    0.9782 0.2632 0.2284
    1.3673 0.2346 0.2160
    0.95 2.7318 2.7344 1.2057 0.5815 1.1348 0.5427
    8.6176 0.6126 0.5838
    0.9898 0.2684 0.2324
    1.3326 0.2392 0.2198
    56 0.15 2.4536 2.5300 0.8753 0.4421 0.8257 0.4148
    56 8.1685 0.6119 0.5802
    0.8347 0.1885 0.1668
    1.1931 0.0926 0.0864
    0.55 2.3747 2.5060 0.8788 0.4427 0.8261 0.4143
    8.0651 0.6095 0.5785
    0.8548 0.1898 0.1667
    1.2352 0.0927 0.0858
    0.95 2.3900 2.5214 0.8759 0.4417 0.8271 0.4148
    8.1405 0.6118 0.5818
    0.8549 0.1877 0.1661
    1.2216 0.0913 0.0844
    4 80 20 10 0.15 3.5514 2.9879 1.8141 0.7625 1.7046 0.7083
    20 10 9.0555 0.6117 0.5818
    20 10 0.9926 0.3838 0.3253
    20 10 1.3399 0.2405 0.2214
    0.55 3.3072 3.0253 1.5485 0.6838 1.4686 0.6395
    9.1629 0.6124 0.5826
    1.1114 0.3375 0.2875
    1.5448 0.2368 0.2192
    0.95 3.3013 3.0365 1.5334 0.6802 1.4531 0.6366
    9.2126 0.6123 0.5846
    1.2443 0.3335 0.2853
    1.4244 0.2416 0.2234
    16 0.15 3.0018 2.8487 1.2939 0.6085 1.2209 0.5677
    16 8.8203 0.6151 0.5846
    16 1.0622 0.2872 0.2464
    16 1.3593 0.2380 0.2187
    0.55 2.7877 2.8122 1.2833 0.6045 1.2083 0.5638
    8.8808 0.6181 0.5875
    1.0125 0.2804 0.2416
    1.3797 0.2362 0.2180
    0.95 2.6809 2.7709 1.2539 0.5955 1.1762 0.5541
    8.6718 0.6139 0.5841
    1.0059 0.2782 0.2396
    1.4957 0.2359 0.2165
    140 35 18 0.15 2.9768 2.8485 1.3322 0.6132 1.2466 0.5702
    35 18 8.9141 0.6170 0.5870
    35 18 0.9581 0.2688 0.2318
    35 18 1.3934 0.2349 0.2153
    0.55 2.7722 2.727 1.1958 0.5740 1.1280 0.5365
    8.5091 0.6177 0.5868
    0.9857 0.2487 0.2158
    1.3680 0.2336 0.2155
    0.95 2.7294 2.7466 1.1760 0.5731 1.1088 0.5356
    8.7286 0.6159 0.5867
    0.9769 0.2643 0.2290
    1.2979 0.2362 0.2177
    28 0.15 2.4586 2.5493 0.9017 0.4483 0.8475 0.4203
    28 8.2247 0.6144 0.5847
    28 0.8842 0.1858 0.1640
    28 1.1792 0.0913 0.0849
    0.55 2.3382 2.5347 0.8769 0.4407 0.8265 0.4129
    8.2832 0.6080 0.5768
    0.8100 0.1871 0.1651
    1.2424 0.0907 0.0834
    0.95 2.3738 2.5307 0.8765 0.4429 0.8254 0.4150
    8.1678 0.6098 0.5791
    0.8702 0.1914 0.1689
    1.2415 0.0937 0.0867

     | Show Table
    DownLoad: CSV

    The total number of observations N is divided into two groups, \hbar = 2 , and then into four groups, \hbar = 4 , for comparison among MLEs, BELs, and BEGs.

    ● When there are two groups (\hbar = 2) ,

    \begin{split} n_{1}& = n_{2} = N/2 \text{and} w_{1} = w_{2} = 50\% \,\, \text{and} \,\, 80\% \,\,\text{of the sample size},\\ v_{1}& = 0.5 \,\, \text{and}\,\, v_{2} = 1. \end{split}

    ● When there are four groups (\hbar = 4) ,

    \begin{split} n_{1}& = n_{2} = n_{3} = n_{4} = N/4 \; \text{and} \; w_{1} = w_{2} = w_{3} = w_{4} = 50\% \,\, \text{and} \,\, 80\% \,\,\text{of the sample size}\\ v_{1}& = 0.5, v_{2} = 1.0, \, v_{3} = 1.5, \,\, \text{and}\,\, v_{4} = 2.0. \end{split}

    The MLEs (BELs and BEGs) of the parameters \alpha , \lambda , \theta and c with their MSEs, RABs, MMSEs, MRABs are displayed in Table 2 (Table 3). The HPD credible intervals, symmetric credible intervals, and CIs with their AILs and MAILs are presented in Table 4.

    We can observe from Tables 24 that:

    (1) Through the MMSEs and MRABs, the BELs and BEGs outperform the MLEs.

    (2) Through the MAILs, the HPD and symmetric credible intervals are superior to CIs. This confirms that BELs and BEGs are superior to MLEs.

    (3) The HPD is better than symmetric credible intervals via the MAILs.

    (4) For fixed p , \hbar , N , and n_{i} (or w_{i} ), i = 1, \dots, \hbar , by increasing w_{i} (or n_{i} ) the MSEs, RABs, MMSEs, MRABs, AILs and MAILs decrease. This assures that the more data we collect, the more accurate our results will be.

    (5) The BELs and BEGs are better at \nu = 0.5 than those at \nu = -0.5 through comparing the MMSE.

    (6) The BELs are better than BEGs at \nu = 0.5 but the converse is true at \nu = -0.5 through comparing the MMSE.

    (7) The MLEs are better at p = 0.15 than those at p = 0.55, 0.95 through comparing the MMSE.

    (8) Better results have been obtained at \hbar = 2 than those obtained at \hbar = 4 since the number of observations in the subgroups became smaller than those at \hbar = 2 .

    Except in a few rare cases, the above results are satisfactory, which could be related to data fluctuations.

    Furthermore, if the hyperparameters are unknown, we can estimate them using past samples following the empirical Bayes approach, see [33]. Alternatively, the hierarchical Bayes technique, which uses a suitable prior for the hyperparameters, could be utilized, see [34].

    Due to the progress in manufacturing devices in the last decades, physicists and engineers may face a problem in assessing the lifetime distribution of these devices if they are connected in a certain mixed system such as a series-parallel system. To overcome this problem, we have introduced a new distribution called PGLD. The mentioned distribution can describe the lifetime distribution of series-parallel systems when the number of series subsystems, as well as the number of their parallel components, are random variables. The PGLD may arise by compounding two discrete (truncated Poisson and geometric) distributions with a mixture of continuous distributions, LD. Some important properties of the PGLD have been investigated, such as the q -th quantile, mode, r -th moment, mean residual lifetime, Bonferroni and Lorenz curves, Rényi and Shannon's entropies, PDF and CDF of the i -th order statistic. The progressive-stress model has been applied to units connected in a series-parallel structure. The lifetimes of these units under normal stress conditions are assumed to follow LD which is considered a mixture of exponential and gamma distributions. The progressive-stress model was used when the stress is increasing nonlinearly over time, and the inverse power law model had established a relationship between the stress and the proposed distribution's scale parameter. Based on progressively type-II censored data with binomial eliminations, two estimation methods were performed to estimate the unknown parameters. The Bayesian estimation was performed using two asymmetric (LINEX and GE) loss functions. CIs, symmetric, and HPD credible intervals for the unknown parameters were established. The numerical results showed that the Bayes estimates were performed well than the MLEs. An illustrative example, based on two real data sets, demonstrated the superiority of the proposed distribution over some other four distributions.

    Finally, the features and motivations to the PGLD can be summarized as follows:

    (1) The CDF of the PGLD has a closed-form. This feature simplifies its use.

    (2) The four parameters included in the CDF of PGLD give it the ability to fit several data.

    (3) The CDF of PGLD includes the CDF of GLD, PLD, and LD as special cases.

    (4) The PGLD can represent the failure time of a series-parallel system. This is considered a motivation to introduce the PGLD.

    (5) The HRF of PGLD has a unimodal shape. This feature gives it more flexibility to fit and analyze several data arising from increasing and decreasing hazard rates.

    (6) The PGLD can represent the non-stationary data. This feature may be useful for the experimenter to forecast how some products would behave in different environments.

    (7) The PGLD is better to fit the data than some other distributions such as PLD, GLD, ELD, and LD.

    (8) Some other distributions may be emerged from Theorem 2.1 by choosing some other continuous distributions rather than LD.

    Based on the above features and motivations, we hope that the PGLD will attract more attention from physicists and engineers in the near future.

    The following points may be investigated in future work:

    (1) The inference procedure may be implemented based on a general progressive censoring scheme such as hybrid progressive censoring.

    (2) Some other estimation methods such as the moments and probability weighted moments may be discussed.

    (3) Some other types of ALTs such as the step-stress ALT may be considered.

    (4) Prediction of future order statistics based on the PGLD may be investigated.

    The authors would like to thank the Deanship of Scientific Research at Umm Al-Qura University for supporting this work by grant code (19-SCI-1-03-0009). They are also grateful to the editor and reviewers for their valuable comments and suggestions, which improved the paper.

    The authors declare that they have no conflicts of interest regarding the publication of this article.



    [1] R. L. Bishop, B. O'Neill, Manifolds of negative curvature, Trans. Amer. Math. Soc., 145 (1969), 1–49. https://doi.org/10.2307/1995057 doi: 10.2307/1995057
    [2] G. I. Kruchkovich, On motions in semi-reducible Riemann spaces, Usp. Mat. Nauk, 12 (1957), 149–156.
    [3] B. Y. Chen, Geometry of warped product \mathcal{CR}-submanifolds in Kaehler manifolds, Mh. Math., 133 (2001), 177–195. https://doi.org/10.1007/s006050170019 doi: 10.1007/s006050170019
    [4] B. Y. Chen, Geometry of warped product \mathcal{CR}-submanifolds in Kaehler manifolds, II, Mh. Math., 134 (2001), 103–119. https://doi.org/10.1007/s006050170002 doi: 10.1007/s006050170002
    [5] I. Hasegawa, I. Mihai, Contact \mathcal{CR}-warped product submanifolds in Sasakian manifolds, Geom. Dedicata, 102 (2003), 143–150. https://doi.org/10.1023/B:GEOM.0000006582.29685.22 doi: 10.1023/B:GEOM.0000006582.29685.22
    [6] V. A. Khan, K. A. Khan, A note on warped product submanifolds of Kenmotsu manifolds, Math. Slovaca, 61 (2011), 79–92. https://doi.org/10.2478/s12175-010-0061-3 doi: 10.2478/s12175-010-0061-3
    [7] S. Uddin, K. A. Khan, An inequality for contact \mathcal{CR}-warped product submanifolds of nearly cosymplectic manifolds, J. Inequal. Appl., 2012 (2012), 1–7. https://doi.org/10.1186/1029-242X-2012-304 doi: 10.1186/1029-242X-2012-304
    [8] F. R. Al-Solamy, M. A. Khan, Semi-invariant warped product submanifolds of almost contact manifolds, J. Inequal. Appl., 2012 (2012), 1–12. https://doi.org/10.1186/1029-242X-2012-127 doi: 10.1186/1029-242X-2012-127
    [9] I. Mihai, Contact \mathcal{CR}-warped product submanifolds in Sasakian space forms, Geom. Dedicata, 109 (2004), 165–173. https://doi.org/10.1007/s10711-004-5459-z doi: 10.1007/s10711-004-5459-z
    [10] S. Uddin, Geometry of warped product semi-slant submanifolds of Kenmotsu manifolds, Bull. Math. Sci., 8 (2018), 435–451. https://doi.org/10.1007/s13373-017-0106-9 doi: 10.1007/s13373-017-0106-9
    [11] B. Y. Chen, M. I. Munteanu, Geometry of PR-warped products in para-Keahler manifolds, Taiwanese J. Math., 16 (2012), 1293–1327.
    [12] S. K. Srivastava, A. Sharma, Geometry of {\mathcal {P}\mathcal {R}}-semi-invariant warped product submanifolds in paracosymplectic manifold, J. Geom., 108 (2017), 61–74. https://doi.org/10.1007/s00022-016-0325-3 doi: 10.1007/s00022-016-0325-3
    [13] S. K. Srivastava, A. Sharma, Pointwise pseudo-slant warped product submanifolds in a K\ddot{a}hler manifold, Mediterr. J. Math., 14 (2017), 20. https://doi.org/10.1007/s00009-016-0832-3 doi: 10.1007/s00009-016-0832-3
    [14] M. Dhiman, A. Kumar, S. K. Srivastava, \mathcal {PR}-semi slant warped product submanifold of paraKenmotsu manifolds, Results Math., 77 (2022), 1–30. https://doi.org/10.1007/s00025-022-01695-4 doi: 10.1007/s00025-022-01695-4
    [15] S. K. Srivastava, F. Mofarreh, A. Kumar, A. Ali, Characterizations of \mathcal {PR} -pseudo-slant warped product submanifold of para-Kenmotsu manifold with slant base, Symmetry, 14 (2022), 1001. https://doi.org/10.3390/sym14051001 doi: 10.3390/sym14051001
    [16] K. Srivastava, S. K. Srivastava, On a class of \alpha-para Kenmotsu manifolds, Mediterr. J. Math., 13 (2016), 391–399. https://doi.org/10.1007/s00009-014-0496-9 doi: 10.1007/s00009-014-0496-9
    [17] S. Zamkovoy, G. Nakova, The decomposition of almost paracontact metric manifolds in eleven classes revisited, J. Geom., 109 (2018), 1–23. https://doi.org/10.1007/s00022-018-0423-5 doi: 10.1007/s00022-018-0423-5
    [18] J. Nash, The imbedding problem for Riemannian manifolds, Ann. Math., 63 (1956), 20–63. https://doi.org/10.2307/1969989 doi: 10.2307/1969989
    [19] B. Y. Chen, Differential geometry of warped product manifolds and submanifolds, World Scientific, 2017.
    [20] S. Hiepko, Eine innere Kennzeichnung der verzerrten Produkte, Math. Ann., 241 (1979), 209–215. https://doi.org/10.1007/BF01421206 doi: 10.1007/BF01421206
  • This article has been cited by:

    1. Jin Gao, Lihua Dai, Min Xiao, Dynamical analysis of almost periodic solutions for delayed octonion-valued BAM neural networks, 2025, 44, 2238-3603, 10.1007/s40314-025-03112-2
  • Reader Comments
  • © 2022 the Author(s), licensee AIMS Press. This is an open access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0)
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Metrics

Article views(1898) PDF downloads(60) Cited by(1)

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return

Catalog