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Research article

Daily nonparametric ARCH(1) model estimation using intraday high frequency data

  • Received: 15 October 2020 Accepted: 13 January 2021 Published: 20 January 2021
  • MSC : 62G05, 62G20

  • In this paper, the intraday high-frequency data are used to estimate the volatility function of daily nonparametric ARCH(1) model. A nonparametric volatility proxy model is proposed to achieve this objective. Under regular assumptions, the asymptotic distribution of the proposed estimator is established. The impact of different proxies on the estimation precision is also discussed. Simulation and empirical studies show that using the intraday high frequency data can significantly improve the estimation accuracy of the considered model. The idea of this article can be easily extended to other nonparametric or semiparametric ARCH/GARCH models.

    Citation: Xin Liang, Xingfa Zhang, Yuan Li, Chunliang Deng. Daily nonparametric ARCH(1) model estimation using intraday high frequency data[J]. AIMS Mathematics, 2021, 6(4): 3455-3464. doi: 10.3934/math.2021206

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  • In this paper, the intraday high-frequency data are used to estimate the volatility function of daily nonparametric ARCH(1) model. A nonparametric volatility proxy model is proposed to achieve this objective. Under regular assumptions, the asymptotic distribution of the proposed estimator is established. The impact of different proxies on the estimation precision is also discussed. Simulation and empirical studies show that using the intraday high frequency data can significantly improve the estimation accuracy of the considered model. The idea of this article can be easily extended to other nonparametric or semiparametric ARCH/GARCH models.


    Statistical distributions play a crucial role in modeling and analyzing real data with complex behavior in many fields, such as biology, engineering, and medicine. Traditional distributions sometimes fail to adequately represent the patterns seen in real world data. Thus, researchers have introduced sophisticated alternatives to existing distributions. These new flexible distributions have high performance in modeling complex patterns, and they are in high demand as users seek to achieve accurate modeling and robust analysis.

    In recent years, several approaches have been suggested to achieve highly accurate distributions when fitting different types of data. One popular method for generating more flexible distributions involves raising the cumulative distribution function (cdf) of the base distribution using a shape parameter. This approach was proposed by [1] and is called the exponentiated method. The researchers in [2] extended this approach to more a general class of distributions, calling it the exponentiated generalized (EG) method, by adding another shape parameter to the cdf of the base distribution as follows:

    F(x,a,b,ζ)=[1[1G(x,ζ)]a]b, (1.1)

    with the probability density function (pdf)

    f(x,a,b,ζ)=abg(x,ζ)[1G(x,ζ)]a1[1[1G(x,ζ)]a]b1, (1.2)

    where the shape parameters a,b>1, and ζ is a vector of parameters for the base distribution with the cdf G(x,ζ).

    Since its publication, this approach has been adopted by many researchers working to introduce new flexible distributions. Examples include the exponentiated generalized inverted Gompertz [3], exponentiated generalized exponential geometric [4], exponentiated generalized inverse flexible Weibull [5], exponentiated generalized gull alpha power Rayleigh [6], generalized exponentiated Fréchet–Weibull [7], Burr Ⅲ extended exponentiated Weibull [8], exponentiated generalized Marshall Olkin exponential [9], generalized exponentiated unit Gompertz [10], and type-Ⅰ heavy-tailed exponentiated generalised-log-logistic [11] distributions.

    Another well-known method for attaining more versatile distributions is the transformed-transformer (T-X) method, in which any continuous distribution can be used as a generator. The researchers in [12] proposed the widely known Weibull-G class of distributions with the following cdf and pdf:

    F(x,c,β,ζ)=1e(W(G(x,ζ))β)c, (1.3)
    f(x,c,β,ζ)=cβg(x;ζ)1G(x;ζ)(W(G(x,ζ))β)c1e(W(G(x,ζ))β)c, (1.4)

    where c,β>0 are the shape and scale parameters of the Weibull distribution, and W(G(x,ζ)) is the weight function. This family with different forms of W(G(x,ζ)) has been used extensively by researchers to generate more adaptable distributions capable for the fitting of lifetime data. Some of these distributions include Weibull–Gompertz Makeham [13], generalized Weibull–Lindley [14], extended Weibull Fréchet [15], Weibull Marshall–Olkin power Lomax [16], four-parameter Weibull extended Weibull [17], odd Weibull inverse Gompertz [18], Weibull-inverse Nadarajah Haghighi [19], and type-2 Gumbel Weibull exponential [20].

    In this research, the EG method and Weibull-G approach are combined to introduce a new extension of the Rayleigh distribution with five parameters: the exponentiated generalized Weibull–Rayleigh (EGWR) distribution. The introduction of the EGWR model was motivated by the following objectives:

    ● Deliver a new extension of the Rayleigh distribution with improved efficiency and flexibility.

    ● Enhance the elasticity of the Rayleigh distribution by combining two attractive techniques: the EG approach and the Weibull-G class, both of which have shown great flexibility in a wide range of applications.

    ● Provide an adaptable distribution with great versatility as an alternative to existing distributions in modeling data with different forms as observed from the different shapes of the density function.

    ● Compared to competing distributions, offer a better representation of the variability of real-world data in the field of medicine.

    The remaining sections of this paper are arranged as follows: In Section 2, the EGWR distribution is introduced. In Section 3, important properties of the proposed distribution are presented. In Section 4, we provide the estimators of the distribution parameters using four different methods. To test the efficiency of these methods, related simulation studies were performed, and their results are described in Section 5. In Section 6, different medical datasets are analyzed to compare various estimation methods and illustrate the flexibility of the proposed distribution. Finally, in Section 7, we conclude the paper.

    If X is a random variable from the Rayleigh distribution with scale parameter σ>0, then the cdf and pdf are given by the following:

    G(x;σ)=1ex22σ2, (2.1)
    g(x;σ)=xσ2ex22σ2. (2.2)

    By considering weight function W(G(x,ζ))=log(1(G(x,ζ))), using (2.1) in (1.3), the Weibull Rayleigh distribution is obtained with the following cdf:

    F(x,c,β,ζ)=1e(x22σ2β)c. (2.3)

    Substituting (2.3) in (1.1), the EGWR distribution is defined by the following cdf:

    F(x;a,b,c,β,σ)=[1ea(x22σ2β)c]b. (2.4)

    The corresponding pdf is as follows:

    f(x;a,b,c,β,σ)=abc(2σ2β)c2x2c1ea(x22σ2β)c[1ea(x22σ2β)c]b1. (2.5)

    Figures 1 and 2 display different shapes for the pdf and the hazard function (hf) of the EGWR distribution achieved using various parameter values. The pdf takes various forms, such as symmetric, asymmetric, increasing, J-shaped, and reverse J-shaped. In addition, the hf can model data with bathtub and upside-down bathtub shapes. This demonstrates the distribution's capacity to accommodate diverse forms of data, making it a valuable tool for modeling complex phenomena.

    Figure 1.  Plots for the EGWR pdf function with various parameter values.
    Figure 2.  Plots for the EGWR hf with various parameter values.

    The binomial expansion theorem is defined as follows:

    (1x)n1=i=0(1)i(n1i)xi, (2.6)

    where |x|<1 and n>0. Therefore,

    [1ea(x22σ2β)c]b1=i=0(1)i(b1i)eai(x22σ2β)c.

    Thus, the pdf can be re-written as

    f(x;ζ)=i=0(1)i(b1i)2abc(2σ2β)cx2c1ea(i+1)(x22σ2β)c,

    from the following power series:

    ea(i+1)(x22σ2β)c=j=0(1)jj!(a(i+1))j(x22σ2β)cj.

    Hence, the pdf of the EGWR distribution takes the following form:

    f(x;ζ)=i=0j=0(1)i+jj!(b1i)aj+1(i+1)j2bc(2σ2β)c(j+1)x2c(j+1)1.

    Some important statistical properties of the EGWR distribution—moments, incomplete moments, moment generating function, order statistics, and Rényi entropy—are presented in this section.

    For a random variable X from the EGWR distribution, the quantile function can be obtained by inverting (2.4) and presenting the expression in an explicit form as follows:

    xq={2σ2β[1alog(1q1b)]1c}12,0<q<1. (3.1)

    Therefore, the median is given by

    x0.5={2σ2β[1alog(10.51b)]1c}12. (3.2)

    The rth moment [21] of the EGWR distribution is given by

    μr=E(Xr)=0xr2abc(2σ2β)cx2c1ea(x22σ2β)c[1ea(x22σ2β)c]b1dx.

    Using (2.6) for (1ea(x22σ2β)c)b1, we have

    μr=i=0(1)i(b1i)2abc(2σ2β)c0x2c+r1ea(i+1)(x22σ2β)cdx=i=0(1)i(b1i)bar2c(i+1)r2c+1(2σ2β)r2Γ(r2c+1). (3.3)

    The mean and variance of the EGWR distribution can be found from (3.3) as follows:

    Mean=μ1=E(x),Variance=μ2μ21=E(x2)E(x)2.

    Thus, the coefficient of variation (COV), the dispersion index (DI), skewness (SK), and kurtosis (K) can be obtained as follows:

    COV=μ2μ21μ1,DI=μ2μ21μ1,SK=μ33μ2μ1+2μ31(μ2μ21)32,DI=μ44μ3μ1+6μ2μ213μ41(μ2μ21)2.

    These measures can be calculated using any reputable statistical software, such as R.

    Table 1 displays the measures' values for the following cases of parameters:

    I:a=3.4, b=3.0, c=3.6, β=1.3, σ=3.9.II:a=2.3, b=1.1, c=3.7, β=0.6, σ=2.9.III:a=2.5, b=1.0, c=1.5, β=2.3, σ=0.3.IV:a=1.7, b=0.1, c=1.0, β=3.8, σ=1.8.V:a=3.9, b=1.0, c=2.4, β=5.1, σ=1.9.VI:a=1.3, b=2.3, c=0.6, β=2.0, σ=1.5.
    Table 1.  Results (mean, variance, coefficient of variation [COV], dispersion index [CI], skewness [SK], and kurtosis [K]) generated by changes to the parameters.
    Mean Variance COV DI SK K
    5.635465 0.263489 0.091086 0.046755 -0.208116 3.102182
    2.700400 0.165382 0.150597 0.061243 -0.477589 3.253748
    0.423345 0.023673 0.363446 0.055921 0.168102 2.729464
    0.748891 1.661996 1.721458 2.219276 2.481749 9.958432
    4.186111 0.990484 0.237745 0.236612 -0.225393 2.850532
    3.477175 4.145255 0.585529 1.192133 1.18643 5.137207

     | Show Table
    DownLoad: CSV

    As shown in Table 1, the EGWR distribution can be negatively (left) skewed or positively (right) skewed; this illustrates the flexibility of the distribution in fitting various types of asymmetrical data. Moreover, the kurtosis values indicate that the distribution can be leptokurtic or platykurtic. Hence, the distribution is capable for modeling data with sharp peaks and lighter tails or flat peaks with heavier tails. Additionally, the values of the dispersion index shows the flexibility in modeling data with various spreads.

    The sth incomplete moment [22] of the EGWR distribution is defined as

    Is=E(Xs)=z0xs2abc(2σ2β)cx2c1ea(x22σ2β)c[1ea(x22σ2β)c]b1dx,

    where from binomial expansion (2.6), we have

    Is=i=0(1)i(b1i)2abc(2σ2β)cz0x2c+s1ea(i+1)(x22σ2β)cdx=i=0(1)i(b1i)bas2c(i+1)s2c+1(2σ2β)s2γ(s2c+1,uz), (3.4)

    where uz=a(i+1)(z22σ2β)c.

    The moment generating function [23] for the EGWR distribution is obtained as follows:

    MX(t)=E(etx)=0etx2abc(2σ2β)cx2c1ea(x22σ2β)c[1ea(x22σ2β)c]b1dx.

    By applying the binomial expansion (2.6), we obtain

    MX(t)=i=0(1)i(b1i)2abc(2σ2β)c0x2c1etxea(i+1)(x22σ2β)cdx,

    where by using the power series expansion for etx, we have

    MX(t)=i=0r=0(1)i(b1i)trr!2abc(2σ2β)c0x2c+r1ea(i+1)(x22σ2β)cdx=i=0r=0(1)i(b1i)trr!bar2c(i+1)r2c+1(2σ2β)r2Γ(r2c+1). (3.5)

    The Rényi entropy [24] for the EGW-R distribution is defined as

    HR(x)=11Rlog[0(f(x;ζ))Rdx],

    where

    (f(x;ζ))R=(2abc(2σ2β)c)RxR(2c1)eaR(x22σ2β)c[1ea(x22σ2β)c]R(b1).

    Using the binomial expansion (2.6),

    [1ea(x22σ2β)c]R(b1)=i=0(1)i(R(b1)i)eai(x22σ2β)c.

    Thus,

    (f(x;ζ))R=i=0(1)i(R(b1)i)(2abc(2σ2β)c)RxR(2c1)ea(R+i)(x22σ2β)c,

    and therefore,

    0(f(x;ζ))Rdx=i=0(1)i(R(b1)i)(2abc(2σ2β)c)R×0xR(2c1)ea(R+i)(x22σ2β)cdx=i=0(1)i(R(b1)i)(2c)R1bR(1a)1R2c(2σ2β)1R2×[1(R+i)]R(2c1)+12cΓ(R(2c1)+12c). (3.6)

    The Rényi entropy is then given by the following:

    HR(x)=11Rlog[i=0(1)i(R(b1)i)(2c)R1bR(1a)1R2c[1(R+i)]R(2c1)+12c×(2σ2β)1R2Γ(R(2c1)+12c)]=11R{(R1)log(2c)+Rlog(b)+(1R2)log(2σ2β)(1R2c)log(a)+log[i=0(1)i(R(b1)i)[1(R+i)]R(2c1)+12cΓ(R(2c1)+12c)]}. (3.7)

    Let x1,x2,,xn be a sample selected from the EGW-R distribution with order statistics x1:n,x2:n,,xn:n. The ith order statistics then have the following distribution[25]:

    fi:n(x;ζ)=n!(i1)!(ni)![F(x;ζ)]i1[1F(x;ζ)]nif(x;ζ).

    By using the binomial expansion (2.6),

    [1F(x;ζ)]ni=nik=0(1)k(nik)[F(x;ζ)]k,
    fi:n(x;ζ)=nik=0(1)k(nik)n!(i1)!(ni)![F(x;ζ)]k+i1f(x;ζ),

    where

    [F(x;ζ)]k+i1f(x;ζ)=2abc(2σ2β)cx2c1ea(x22σ2β)c[1ea(x22σ2β)c]b(k+i)1.

    By the applying binomial expansion (2.6),

    [1ea(x22σ2β)c]b(k+i)1=j=0(1)j(b(k+i)1j)eaj(x22σ2β)c.

    Thus,

    [F(x;ζ)]k+i1f(x;ζ)=j=0(1)j(b(k+i)1j)2abc(2σ2β)cx2c1ea(j+1)(x22σ2β)c.

    By applying the power series expansion for ea(j+1)(x22σ2β)c, we obtain

    [F(x;ζ)]k+i1f(x;ζ)=j=0m=0(1)j+mm!(b(k+i)1j)am+1(j+1)m×2bc(2σ2β)c(m+1)x2c(m+1)1.

    Therefore, the distribution takes the following form:

    fi:n(x;ζ)=j=0m=0nik=0(1)j+m+km!n!(i1)!(ni)!(b(k+i)1j)(nik)×am+1(j+1)m2bc(12σ2β)c(m+1)x2c(m+1)1. (3.8)

    The maximum likelihood (ML) method is one of the most widely applied methods of estimation in the literature [26,27]. In this method, the values of the parameters are obtained by maximizing the log-likelihood function. Thus, if x1,x2, , xn follows the EGWR distribution with the vector of parameters θ=(a,b,c,β,σ), then the log-likelihood function () is defined by

    = nlog2+nloga+nlogb+nlogcnclog2nclogσ2nclogβ+(2c1)ni=1logxiani=1(x2i2σ2β)c+(b1)ni=1log[1ea(x2i2σ2β)c]. (4.1)

    The aforementioned log-likelihood function is too complicated and difficult to solve analytically. Thus, the derivative of (4.1), with respect to each parameter, is calculated as follows:

    a=nani=1(x2i2σ2β)c+(b1)ni=1[(x2i2σ2β)cea(x2i2σ2β)c1ea(x2i2σ2β)c], (4.2)
    b=nb+ni=1log[1ea(x2i2σ2β)c], (4.3)
    c= ncnlog2nlogσ2nlogβ+2ni=1logxiani=1(x2i2σ2β)clog(x2i2σ2β)+a(b1)ni=1[(x2i2σ2β)clog(x2i2σ2β)e(x2i2σ2β)c1ea(x2i2σ2β)c], (4.4)
    β=ncβ+acβni=1(x2i2σ2β)cac(b1)βni=1[(x2i2σ2β)ce(x2i2σ2β)c1ea(x2i2σ2β)c], (4.5)

    and

    σ=2ncσ+2acσni=1(x2i2σ2β)c2ac(b1)σni=1[(x2i2σ2β)ce(x2i2σ2β)c1ea(x2i2σ2β)c]. (4.6)

    Therefore, the MLEs of the parameter vector θ can be achieved by equating the Eqs (4.2)–(4.6) to zero and solving them in an iterative manner using any numerical method, such as the Newton–Raphson method. Alternatively, the optimization function optim in the statistical software R can be employed to maximize (4.1) directly and obtain the MLEs.

    The ordinary least squares (LS) method [28] estimates the distribution parameters by minimizing the square difference between the theoretical cdf and the empirical cdf. Let x(1),x(2), , x(n) follow the EGWR distribution. The LS method minimizes the following sum of squares:

    Q(θ)=ni=1[(1ea(x2(i)2βσ2)c)bin+1]2. (4.7)

    Differentiating (4.7) with respect to the vector of parameters θ results in the following equations:

    Q(θ)a=2b(2βσ2)cni=1x2c(i)ea(x2i2βσ2)c(1ea(x2i2σ2β)c)b1[(1ea(x2i2βσ2)c)bin+1], (4.8)
    Q(θ)b=2ni=1ln(1ea(x2(i)2βσ2)c)(1ea(x2(i)2βσ2)c)b[(1ea(x2(i)2βσ2)c)bin+1], (4.9)
    Q(θ)c=2ab(2βσ2)cni=1x2c(i)ln(x2(i)2βσ2)ea(x2i2βσ2)c(1ea(x2i2σ2β)c)b1[(1ea(x2i2βσ2)c)bin+1], (4.10)
    Q(θ)β=2abcβ(2βσ2)cni=1x2c(i)ea(x2(i)2βσ2)c(1ea(x2(i)2σ2β)c)b1[(1ea(x2(i)2βσ2)c)bin+1], (4.11)
    Q(θ)σ=4abcσ(2βσ2)cni=1x2c(i)ea(x2(i)2βσ2)c(1ea(x2(i)2σ2β)c)b1[(1ea(x2(i)2βσ2)c)bin+1]. (4.12)

    Therefore, minimizing Eq (4.7) or equivalently solving Eqs (4.8)–(4.12) analytically or numerically using R provides the estimates of the vector of parameters θ=(a,b,c,β,σ).

    The maximum product of spacing (MPS) method was produced by [29] as an improvement of the ML method. Let x1,x2, , xn be a sample from an EGWR distribution with a vector of parameters θ=(a,b,c,β,σ) and order statistics x(1),x(2),,x(n). The idea of the MPS is to maximize the following equation:

    M(θ)=1n+1n+1i=1logDi(θ), (4.13)

    where Di(θ)=F[x(i)θ]F[x(i1)θ],i=1,2,,n+1 are the uniform spacings between the consecutive ordered values, F[x(0)θ]=0, and F[x(n+1)θ]=1. The estimates of the vector of parameters θ can be obtained by maximizing (4.13) or equivalently solving the system of Eqs (4.15)–(4.19) using any optimization function in R.

    M(θ)=1n+1n+1i=1log[(1ea(x2(i)2βσ2)c)b(1ea(x2(i1)2βσ2)c)b], (4.14)
    M(θ)a=1n+1b(2βσ2)cn+1i=11Ai[x2c(i)ea(x2(i)2βσ2)c(1ea(x2(i)2βσ2)c)b1x2c(i1)ea(x2(i1)2βσ2)c(1ea(x2(i1)2βσ2)c)b1], (4.15)
    M(θ)b=1n+1n+1i=11Ai[(1ea(x2(i)2βσ2)c)bln(1ea(x2(i)2βσ2)c)(1ea(x2(i1)2βσ2)c)bln(1ea(x2(i1)2βσ2)c)], (4.16)
    M(θ)c=1n+1ab(2βσ2)cn+1i=11Ai[x2c(i)ln(x2(i)2βσ2)ea(x2(i)2βσ2)c(1ea(x2(i)2βσ2)c)b1x2c(i1)ln(x2(i1)2βσ2)ea(x2(i1)2βσ2)c(1ea(x2(i1)2βσ2)c)b1], (4.17)
    M(θ)β=1n+1abcβ(2βσ2)cn+1i=11Ai[x2c(i)ea(x2(i)2βσ2)c(1ea(x2(i)2βσ2)c)b1x2c(i1)ea(x2(i1)2βσ2)c(1ea(x2(i1)2βσ2)c)b1], (4.18)
    M(θ)σ=1n+12abcσ(2βσ2)cn+1i=11Ai[x2c(i)ea(x2(i)2βσ2)c(1ea(x2(i)2βσ2)c)b1x2c(i1)ea(x2(i1)2βσ2)c(1ea(x2(i1)2βσ2)c)b1], (4.19)

    where Ai=[(1ea(x2(i)2βσ2)c)b(1ea(x2(i1)2βσ2)c)b].

    The Cramér–von Mises method, also called the minimum distance estimator, was proposed by the researchers in [30] to estimate the values of the parameters by minimizing the following objective function:

    C(θ)=112n+ni=1[(1ea(x2(i)2βσ2)c)b2i12n]2. (4.20)

    Minimizing (4.20) or solving the following system of nonlinear equations (4.21)–(4.25) numerically yields the estimate of the vector of parameters θ:

    C(θ)a=2b(2βσ2)cni=1x2c(i)ea(x2i2βσ2)c(1ea(x2i2σ2β)c)b1[(1ea(x2i2βσ2)c)b2i12n], (4.21)
    C(θ)b=2ni=1ln(1ea(x2(i)2βσ2)c)(1ea(x2(i)2βσ2)c)b[(1ea(x2(i)2βσ2)c)b2i12n], (4.22)
    C(θ)c=2ab(2βσ2)cni=1x2c(i)ln(x2(i)2βσ2)ea(x2i2βσ2)c(1ea(x2i2σ2β)c)b1[(1ea(x2i2βσ2)c)b2i12n], (4.23)
    C(θ)β=2abcβ(2βσ2)cni=1x2c(i)ea(x2(i)2βσ2)c(1ea(x2(i)2σ2β)c)b1[(1ea(x2(i)2βσ2)c)b2i12n], (4.24)
    C(θ)σ=4abcσ(2βσ2)cni=1x2c(i)ea(x2(i)2βσ2)c(1ea(x2(i)2σ2β)c)b1[(1ea(x2(i)2βσ2)c)b2i12n]. (4.25)

    To assess and evaluate the performance of the four methods of estimation in determining the parameters of the EGWR distribution, three cases of simulation studies are presented. A number of iterations equal to nsim=10,000 were applied with different sample sizes (n=50,100,300,and500) for the following three cases of true values of the vector of parameters θtr:

    Case I:a=3.5, b=4.1, c=2.7, β=3.9, σ=3.1,Case II:a=2.1, b=3.7, c=2.5, β=1.1, σ=2,Case III:a=1.6, b=2.8, c=3.1, β=0.6, σ=2.2.

    The root mean square error (RMSE) measure was used to assess the efficiency of estimation methods selected for each estimator ˆθ. The RMSE can be obtained as follows:

    RMSE(ˆθ)=nsimi=1(ˆθiθtr)2nsim. (5.1)

    The estimates obtained by the four methods of estimation together with the RMSE are shown in Tables 24 and Figures 35.

    Table 2.  The estimates and RMSE across sample sizes (N=50,150,300,500) for all methods of estimation (case Ⅰ).
    Sample size Parameter ML LS MPS CVM
    Estimate RMSE Estimate RMSE Estimate RMSE Estimate RMSE
    N = 50 a 3.6995 5.1316 3.6385 3.1513 3.8445 5.9930 3.6248 3.2245
    b 7.7331 14.1917 6.3047 7.0769 7.7140 19.3329 6.4418 7.3492
    c 3.1177 1.6661 3.2465 1.8193 2.9335 1.4354 3.3209 1.8888
    β 3.8604 1.8654 3.9251 1.4071 3.9385 2.1858 3.9085 1.3842
    σ 3.0584 0.7980 3.0365 0.5864 3.0872 0.8721 3.0320 0.5879
    N = 150 a 3.5902 1.9735 3.5586 2.1011 3.6003 2.2346 3.5788 2.1639
    b 5.2776 4.7973 5.5309 4.8928 5.2036 4.8694 5.5530 4.8901
    c 2.8033 0.6916 2.9100 1.0184 2.7373 0.6651 2.9319 1.0278
    β 3.9164 0.9357 3.9108 0.9627 3.9179 0.9034 3.9242 0.9478
    σ 3.0759 0.3867 3.0650 0.4082 3.0881 0.3944 3.0599 0.4122
    N = 300 a 3.5891 1.1388 3.5881 1.6243 3.6112 1.0054 3.5697 1.5720
    b 4.6108 2.3514 5.0208 3.4684 4.5656 2.2800 5.0395 3.4926
    c 2.7453 0.4589 2.7992 0.7028 2.7074 0.4483 2.8098 0.7084
    β 3.9256 0.5161 3.9166 0.7280 3.9496 0.5470 3.9176 0.7181
    σ 3.0916 0.2252 3.0869 0.3065 3.0945 0.2212 3.0801 0.3017
    N = 500 a 3.5909 0.7457 3.5286 1.1656 3.5945 0.7019 3.5446 1.1271
    b 4.3870 1.5444 4.7266 2.6295 4.3670 1.5292 4.7443 2.6457
    c 2.7268 0.3514 2.7568 0.5449 2.7008 0.3456 2.7619 0.5467
    β 3.9320 0.3508 3.8970 0.5732 3.9356 0.3645 3.9042 0.5650
    σ 3.0964 0.1568 3.0938 0.2427 3.1001 0.1417 3.0916 0.2408

     | Show Table
    DownLoad: CSV
    Table 3.  The estimates and RMSE across sample sizes (n=50,150,300,500) for all methods of estimation (case Ⅱ).
    Sample size Parameter ML LS MPS CVM
    Estimate RMSE Estimate RMSE Estimate RMSE Estimate RMSE
    n = 50 a 2.3007 3.6239 2.4348 2.8435 2.6361 5.9388 2.3934 2.8937
    b 6.7193 11.3238 5.8464 7.0627 7.1463 16.7620 5.9316 7.3497
    c 2.8859 1.4829 3.0265 1.7657 2.7074 1.2645 3.0893 1.7993
    β 1.1382 0.6712 1.1378 0.4795 1.1467 0.7854 1.1447 0.4877
    σ 1.9454 0.5375 1.9821 0.4565 1.9902 0.5900 1.9666 0.4616
    n = 150 a 2.1739 1.4165 2.2269 1.6606 2.2102 1.6025 2.2370 1.6667
    b 4.6880 3.9955 4.9683 4.5144 4.6579 5.4461 4.9871 4.4469
    c 2.5963 0.6389 2.6916 0.9416 2.5340 0.6131 2.7117 0.9522
    β 1.1040 0.2837 1.1097 0.3115 1.1025 0.2612 1.1089 0.3091
    σ 1.9890 0.2540 1.9905 0.3235 1.9955 0.2541 1.9909 0.3175
    n = 300 a 2.1724 0.6388 2.1979 1.1787 2.1682 0.6165 2.1942 1.1846
    b 4.1214 1.9782 4.4892 3.0452 4.0889 1.9464 4.5108 3.0684
    c 2.5425 0.4221 2.5894 0.6474 2.5064 0.4120 2.5975 0.6502
    β 1.1058 0.1646 1.1026 0.2326 1.1048 0.1545 1.1045 0.2388
    σ 1.9995 0.1377 2.0031 0.2450 2.0016 0.1321 1.9992 0.2511
    n = 500 a 2.1665 0.4570 2.1914 0.9402 2.1677 0.4323 2.1809 0.9069
    b 3.9390 1.3285 4.2102 2.2266 3.9223 1.3106 4.2180 2.2194
    c 2.5252 0.3230 2.5527 0.4977 2.5004 0.3169 2.5584 0.5009
    β 1.1053 0.1081 1.1013 0.1951 1.1055 0.1051 1.1033 0.1920
    σ 2.0032 0.0934 2.0093 0.1570 2.0048 0.0970 2.0055 0.1958

     | Show Table
    DownLoad: CSV
    Table 4.  The estimates and RMSE across sample sizes (n=50,150,300,500) for all methods of estimation (case Ⅲ).
    Sample size Parameter ML LS MPS CVM
    Estimate RMSE Estimate RMSE Estimate RMSE Estimate RMSE
    n = 50 a 1.7729 2.9025 1.9031 2.3260 1.9478 4.2473 1.8835 2.3541
    b 5.0394 11.6821 4.4460 5.3990 5.1186 12.6435 4.4981 5.5023
    c 3.5806 1.8801 3.7252 2.1969 3.3497 1.5768 3.8168 2.3042
    β 0.6295 0.3288 0.6263 0.2435 0.6244 0.3501 0.6306 0.2435
    σ 2.1310 0.5073 2.1771 0.4933 2.1714 0.5138 2.1602 0.4936
    n = 150 a 1.6793 0.9946 1.7432 1.2346 1.7066 0.8836 1.7749 1.4033
    b 3.3994 2.5926 3.6631 3.0490 3.3995 5.2307 3.7503 3.3148
    c 3.2226 0.7839 3.3299 1.1712 3.1400 0.7469 3.3428 1.1677
    β 0.6093 0.1209 0.6112 0.1555 0.6067 0.1216 0.6146 0.1576
    σ 2.1819 0.2386 2.1870 0.3260 2.1930 0.2262 2.1841 0.3395
    n = 300 a 1.6806 0.4577 1.7269 0.9422 1.7020 0.4527 1.7252 0.9100
    b 3.0529 1.2873 3.3295 2.1153 3.0367 1.2752 3.3560 2.1439
    c 3.1548 0.5147 3.2056 0.7994 3.1066 0.5002 3.2138 0.8043
    β 0.6082 0.0653 0.6091 0.1183 0.6096 0.0687 0.6092 0.1147
    σ 2.1946 0.1273 2.1980 0.2464 2.1972 0.1259 2.1959 0.2446
    n = 500 a 1.6776 0.3247 1.6874 0.6620 1.6876 0.3380 1.6951 0.6742
    b 2.9437 0.8820 3.1310 1.5109 2.9391 0.8765 3.1472 1.5431
    c 3.1326 0.3930 3.1627 0.6128 3.0988 0.3845 3.1665 0.6141
    β 0.6080 0.0487 0.6068 0.0907 0.6080 0.0492 0.6069 0.0921
    σ 2.1981 0.0896 2.1998 0.1917 2.1999 0.0870 2.2007 0.1892

     | Show Table
    DownLoad: CSV
    Figure 3.  The values of estimates using the ML, LS, MPS, and CVM methods for parameters: a,b,c,β, andσ, respectively (case Ⅰ).
    Figure 4.  The values of estimates using the ML, LS, MPS, and CVM methods for parameters: a,b,c,β, andσ, respectively (case Ⅱ).
    Figure 5.  The values of estimates using the ML, LS, MPS, and CVM methods for parameters: a,b,c,β, andσ, respectively (case Ⅲ).

    As can be seen from the above tables and figures, all of the examined estimation methods achieved consistency. When the sample size n increased, the RMSE decreased, and the estimate approached its true value. Moreover, For sample size n=50, except for parameter c, the LS method provided the closest estimate to the true value for all parameters. Thus, it was considered the most precise method of estimation, followed by the CVM method, while MPS was considered the worst out of all examined methods. Furthermore, when the sample size increased and reached n=500, the MPS and ML methods outperformed the others. These methods produced the lowest RMSE values, with the MPS method having a slight advantage in most cases.

    In this section, three medical datasets were used to provide insights into which method had the best performance in estimating the parameters of the EGWR distribution.

    Dataset 1

    Provided by a Saudi Ministry of Health hospital, this dataset was reported in [31] and represents the lifetimes (in years) of 40 individuals who were diagnosed with leukemia. The data are listed below: 0.315, 0.496, 0.616, 1.145, 1.208, 1.263, 1.414, 2.025, 2.036, 2.162, 2.211, 2.370, 2.532, 2.693, 2.805, 2.910, 2.912, 3.192, 3.263, 3.348, 3.348, 3.427, 3.499, 3.534, 3.767, 3.751, 3.858, 3.986, 4.049, 4.244, 4.323, 4.381, 4.392, 4.397, 4.647, 4.753, 4.929, 4.973, 5.074, 5.381.

    Dataset 2

    The second dataset was reported by [32] and lists the periods of symptom relief for 36 bladder cancer patients. The durations (in days) were as follows: 0.08, 0.2, 0.4, 0.5, 0.51, 0.81, 0.87, 0.9, 1.05, 1.19, 1.26, 1.35, 1.4, 1.46, 1.76, 2.02, 2.02, 2.07, 2.09, 2.23, 2.26, 2.46, 2.54, 2.62, 2.64, 2.69, 2.69, 2.75, 2.83, 2.87, 3.02, 3.02, 3.25, 3.31, 3.36, 3.36.

    Dataset 3

    The last dataset was reported in [33] and consists of the relief times (in minutes) of 20 patients who received a pain reliever as follows: 1.1, 1.4, 1.3, 1.7, 1.9, 1.8, 1.6, 2.2, 1.7, 2.7, 4.1, 1.8, 1.5, 1.2, 1.4, 3, 1.7, 2.3, 1.6, 2.

    The accuracy of the ML, LS, MPS, and CVM methods in estimating the distribution parameters and fitting the data were compared. Tables 57 offer the estimate and standard error for each parameter along with the Kolmogorov–Smirnov (KS) test statistic and P-value for all the methods of estimation.

    Table 5.  Parameter estimates, standard errors (in parentheses), and KS results for Dataset 1.
    Parameter ML LS MPS CVM
    a 2.5242 (0.0054) 3.4949 (1.3842) 2.7979 (0.0789) 2.9447 (2.3129)
    b 0.1273 (0.0201) 0.1335 (0.0988) 0.1188 (0.0199) 0.1355 (0.1125)
    c 6.3220 (0.0054) 6.0953 (1.3793) 6.1141 (0.0827) 6.2266 (2.3532)
    β 1.6975 (0.0054) 3.2830 (1.3237) 1.6127 (0.3256) 4.0251 (2.2503)
    σ 2.8987 (0.0054) 2.1829 (0.6336) 3.1104 (0.3215) 1.9152 (0.6911)
    KS 0.0659 0.0610 0.0835 0.0557
    P-value 0.9950 0.9983 0.9428 0.9996

     | Show Table
    DownLoad: CSV
    Table 6.  Parameter estimates, standard errors (in parentheses), and KS results for Dataset 2.
    Parameter ML LS MPS CVM
    a 4.0014 (0.0033) 4.6811 (0.4829) 3.2677 (0.0004) 5.1672 (0.1580)
    b 0.1372 (0.0229) 0.1322 (0.0902) 0.0940 (0.0173) 0.1308 (0.0655)
    c 4.8434 (0.0033) 4.7446 (0.4824) 6.6395 (0.0004) 4.9779 (0.1578)
    β 0.4352 (0.0033) 0.5665 (0.2969) 0.9050 (0.0004) 0.7319 (0.1475)
    σ 3.9916 (0.0033) 3.8530 (0.4696) 2.7204 (0.0004) 3.3434 (0.1558)
    KS 0.1193 0.0874 0.1152 0.0848
    P-value 0.6847 0.9460 0.7253 0.9580

     | Show Table
    DownLoad: CSV
    Table 7.  Parameter estimates, standard errors (in parentheses), and KS results for Dataset 3.
    Parameter ML LS MPS CVM
    a 0.0051 (0.0017) 0.0902 (1.2776) 0.0635 (1.2752) 0.0611 (0.6350)
    b 6.4327 (4.6024) 7.3693 (55.6305) 6.4930 (18.9398) 6.5356 (57.7738)
    c 0.7218 (0.1798) 0.7826 (2.2306) 0.5592 (0.6037) 0.9024 (3.0946)
    β 2.3471 (5.7104) 1.4198 (31.5817) 0.0169 (0.0539) 0.0422 (0.2554)
    σ 0.0122 (0.0056) 0.1267 (1.0148) 0.4143 (5.1380) 0.8023 (7.9693)
    KS 0.1595 0.1044 0.1932 0.1101
    P-value 0.6887 0.9812 0.4437 0.9686

     | Show Table
    DownLoad: CSV

    As displayed in Tables 57, from a precision perspective, the ML method provided the smallest values of standard error and would be the most suitable method of estimation for the leukemia dataset. The CVM method would be considered the worst of those examined as it had the highest standard error values. A similar pattern can be seen with the pain relief dataset, except for parameter β. However, for the bladder cancer dataset, MPS slightly outperformed ML although both methods had the lowest standard error, while the worst method for estimation of those examined was the LS method. From a goodness-of-fit perspective, the CVM method produced good fit for the leukemia and the bladder cancer datasets as it provided higher P-values and lower KS statistics among all the examined methods, while LS offered a more suitable fit for the pain relief dataset.

    In this section, the ML method was used to assess the performance of the EGWR distribution in fitting the aforementioned datasets. A comparison was made between the EGWR distribution and some competitors: the exponentiated Weibull Rayleigh (EWR), based on the idea of the researchers in [34]; the Marshall–Olkin Weibull Rayleigh (MOWR), a sub-model from the general class proposed by the researchers in [35]; the Weibull Rayleigh (WR) by [34]; the Kumaraswamy Rayleigh (KumR) presented by the researchers in [36]; the Marshall–Olkin alpha power Rayleigh (MOAPR) by the researchers in [37]; and the generalized Rayleigh (GR) explored by the researchers in [38]. To pick the most suitable of these models, the Akaike information criterion (AIC), Bayesian information criterion (BIC), Hannan–Quinn information criterion (HQIC), and KS statistic with P-value were computed. Tables 810 display the values of the MLEs and goodness-of-fit measures for the EGWR and competing distributions, while the theoretical and empirical cdf and pdf are displayed in Figures 68.

    Table 8.  The ML estimates and goodness-of-fit measures for all distributions for Dataset 1.
    Model EGWR EWR MOWR WR KumR MOAPR GR
    ˆa=2.5242 ˆa=2.2206 ˆa=5.8178 ˆc=1.2499 ˆa=0.8702 ˆθ=0.9681 ˆa=1.1726
    ˆb=0.1273 ˆc=0.8071 ˆb=1.0348 ˆβ=0.0024 ˆb=0.0714 ˆα=5.8756 ˆσ=2.3002
    MLEs ˆc=6.3220 ˆβ=3.4238 ˆc=0.9117 ˆσ=50.2894 ˆσ=0.6457 ˆσ=2.0199
    ˆβ=1.6975 ˆσ=0.4262 ˆσ=1.5696
    ˆσ=2.8987
    Goodness-of-Fit Measures
    AIC 139.8385 141.5956 143.6428 145.1159 147.3771 143.5203 145.0313
    BIC 148.2829 148.3512 150.3983 150.1826 152.4437 148.5869 148.4091
    HQIC 142.8917 144.0382 146.0854 146.9479 149.2090 145.3522 146.2526
    KS 0.0659 0.1029 0.0913 0.1183 0.1615 0.1029 0.1439
    P-value 0.9950 0.7904 0.8922 0.6301 0.2475 0.7898 0.3786

     | Show Table
    DownLoad: CSV
    Table 9.  The ML estimates and goodness-of-fit measures for all distributions for Dataset 2.
    Model EGWR EWR MOWR WR KumR MOAPR GR
    ˆa=0.4211 ˆa=0.3133 ˆa=0.5504 ˆc=0.8673 ˆa=0.4873 ˆθ=1.6663 ˆa=1.6272
    ˆb=0.1402 ˆc=2.2488 ˆb=0.0659 ˆβ=2.5817 ˆb=0.0905 ˆα=0.7080 ˆσ=0.8335
    MLEs ˆc=4.6449 ˆβ=0.4496 ˆc=1.1090 ˆσ=0.9295 ˆσ=0.4770 ˆσ=1.4234
    ˆβ=1.4346 ˆσ=3.1404 ˆσ=6.8985
    ˆσ=1.7627
    Goodness-of-Fit Measures
    AIC 100.7827 103.1531 113.4518 109.4460 106.3240 107.9504 105.9897
    BIC 108.7003 109.4872 119.7859 114.1966 111.0745 112.7010 109.1567
    HQIC 103.5462 105.3638 115.6626 111.1041 107.9820 109.6085 107.0950
    KS 0.1193 0.1466 0.1928 0.1870 0.1674 0.1369 0.1790
    P-value 0.6847 0.4213 0.1375 0.1611 0.2652 0.5089 0.1986

     | Show Table
    DownLoad: CSV
    Table 10.  The ML estimates and goodness-of-fit measures for all distributions for Dataset 1.
    Model EGWR EWR MOWR WR KumR MOAPR GR
    ˆa=0.0051 ˆa=0.4607 ˆa=0.4710 ˆc=0.3657 ˆa=0.4991 ˆθ=1.2453 ˆa=1.6766
    ˆb=6.4327 ˆc=1.7105 ˆb=0.8595 ˆβ=21.2434 ˆb=0.1073 ˆα=7.6572 ˆσ=0.6289
    MLEs ˆc=0.7218 ˆβ=15.5398 ˆc=1.4638 ˆσ=0.2678 ˆσ=0.4865 ˆσ=1.0740
    ˆβ=2.3471 ˆσ=0.4656 ˆσ=1.8670
    ˆσ=0.0122
    Goodness-of-Fit Measures
    AIC 44.7134 54.7442 48.2518 83.2277 52.9718 46.9752 56.3742
    BIC 49.6920 58.7271 52.2347 86.2149 55.9590 49.9624 58.3657
    HQIC 45.6853 55.5217 49.0293 83.8109 53.5549 47.5584 56.7629
    KS 0.1595 0.2552 0.1764 0.5229 0.2929 0.1624 0.3561
    P-value 0.6887 0.1477 0.5624 <0.001 0.0646 0.6668 0.0125

     | Show Table
    DownLoad: CSV
    Figure 6.  The theoretical and empirical pdf (right) and cdf (left) for all distributions for Dataset 1.
    Figure 7.  The theoretical and empirical pdf (right) and cdf (left) for all distributions for Dataset 2.
    Figure 8.  The theoretical and empirical pdf (right) and cdf (left) for all distributions for Dataset 3.

    The above tables and figures show the potential flexibility of the EGWR distribution in modeling medical data compared to other competing distributions.

    We extended the Rayleigh distribution to obtain a more flexible distribution capable of modeling complex patterns in medical data. The hazard function of the proposed distribution can take on different patterns, which shows great flexibility as required by many lifetime datasets. The statistical characteristics of the new distribution, such as quantile, median, moment-generating function, Rényi entropy, and order statistics, were studied in this research. The distribution's parameters were estimated using ML, LS, MPS, and CVM, and the efficiency of the estimators obtained by the different methods was assessed in the reported Monte Carlo simulation studies. The results revealed that for the three simulated cases, the LS method had better estimation for smaller samples, while the ML and MPS methods performed better for larger samples. The efficiency of the estimation methods was also evaluated using three medical datasets. The results demonstrated the ability of ML and MPS in estimating the model parameters, as they provided lower standard error values compared to other examined methods in most cases. Finally, the EGWR distribution was compared with a selection of competitive distributions to investigate its ability in modeling the provided medical data, and the results clearly demonstrated that the EGWR outperformed other distributions in analyzing the data. Thus, it can provide insights for scientists to better understand and address complex patterns in healthcare data. As future work, more advanced methods of estimation, such as the Bayesian method, could be employed to enhance the estimation of the parameters. Moreover, the development of a discretised version of the EGWR distribution would offer crucial tools for describing, evaluating, and modeling different phenomena with countable and distinct outcomes, which would lead to precise decision-making and offer better understanding of data across a variety of fields.

    The author declares she has not used Artificial Intelligence (AI) tools in the creation of this article.

    For the editor-in-chief and anonymous reviewers, the author extends great gratitude for their insightful comments, which refined the quality of this work.

    The author declares that she has no conflicts of interest.



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