Journal of Statistical Theory and Applications

Volume 17, Issue 4, December 2018, Pages 703 - 718

Weighted Entropy Measure: A New Measure of Information with its Properties in Reliability Theory and Stochastic Orders

Authors
M. Ramadan1
1Department of Statistics, Mathematics and Insurance, College of Commerce, Benha University, Egypt.
*

Corresponding author. Email: mramadan@benha-univ.edu.eg

Received 25 April 2017, Accepted 6 May 2018, Available Online 31 December 2018.
DOI
10.2991/jsta.2018.17.4.11How to use a DOI?
Keywords
Shannon information; mean residual life; mean reversed life
Abstract

The weighted entropy measure is a germane dynamic measure of uncertainty in reliability and survival studies. In this paper, the new results of weighted entropies with some characterizations are provided. Furthermore, we have presented some results for weighted entropy residual and weighted past residual of order statistics with some application of some reliability systems such as a series structure and a parallel structure. In addition, we introduced the lower bound for the weighted residual (past) entropy. Moreover, the stochastic orders based on weighted entropy are presented. Finally, we illustrate the usefulness of the proposed non-parametric estimators of weighted entropy by application to real data.

Copyright
© 2018 The Authors. Published by Atlantis Press SARL.
Open Access
This is an open access article under the CC BY-NC license (http://creativecommons.org/licences/by-nc/4.0/).

1. INTRODUCTION

The weighted distributions have been utilized in many applications such as distributions theory, reliability, probability, ecology, bio-statistics and applied.

Consider the distribution function G. for a random variable Y≥0 with density function g.. Suppose

lY=infy∈ℝ1:Gy>0, uY=supy∈ℝ1:Gy<1, SY=lY,uY and w.∈R+ be a weighted function. The weighted random variable YW, having probability density function as:

gw(y)=w(y)g(y)/E[w(y)],−∞≤y≤∞,
where Ewy∈ℝ+. Let Y represents the life length of a “unit” in reliability studies, and life distribution, with survival function G¯Y, hazard rate function φ¯G.=gY./G¯Y., reversed hazard rate φG.=gY./GY., the geometric vitality function ϑY=Eln Y|Y>0 and mean revered residual lifetime as
θ(t)=E[κ−Y|Y≤κ]=∫0κGY(u)duGY(κ),κ∈R+.
As reported by Ebrahimi and Pellery [1] and Asha and Rejeesh [2], the differential entropy HY demonstrate the expected uncertainty of gy. In addition, it measures how the distribution spreads over its domain, where there is an inverse relationship between the value of HY and concentration of the probability mass of Y. HY sometimes called a dynamic measure of uncertainty or Shannon information measure.

The differential entropy of random variable Y can be defined in the continuous case as follows:

HY=E[−ln⁡gY(Y)]=−∫0∞gY(u)ln⁡gY(u)du.
Khinchin (1957) generalized Eq. (3) as
HYϕ=EϕgYy=∫0∞gYuϕgYudu.
Di Crescenzo and Longobardi [4] developed the following convex entropy measure:
HwY=−∫0∞vgYvlngYvdv,
or equivalently:
Hw(Y)=−∫0∞dy∫y∞gY(v)ln⁡gY(v)dv.
The uncertainty of the residual lifetime is discussed in Di Crescenzo and Longobardi [5], with the following measure:
HY,κ=1−Elnφ¯GY|Y>κ=−∫κ∞gYvG¯vlngYvG¯vdv,κ∈ℝ+,
where κ∈A=y∈ℝ+|G¯Yy>0. In addition, the past entropy has been widely researched. We can measure it as follows:
H¯GY,κ=1−ElnφGY|Y<κ=−∫0κgYvGvlngYvGvdv,κ∈ℝ+.
Di Crescenzo and Longobardi [4] defined the convex residual entropy as
HwY,κ=−∫κ∞ygYyG¯κlnygYyG¯κdy,κ∈ℝ+.
Furthermore, let Y1 and Y2 be two random variables with distribution functions G1. and G2., densities functions gY1. and gY2. and survival functions G¯1. and G¯2. respectively. Kullback and Leibler [6] introduced an information distance between two distributions G1 and G2 as follows:
IY1,Y2=∫0∞gY1ulngY1ugY2udu.

In addition, Ebrahimi and Kirmani [7] have demonstrated that the Kullback-Leibler discrimination information of Y1 and Y2 at time κ can be presented as

IRY1,Y2(κ)=∫κ∞gY1(u)G¯1(κ)ln⁡gY1(u)/G¯1(κ)gY(u)/G¯2(κ)du.
We can use Eq. (5) to distinguish between two residual lifetimes those have both survived up to time κ, where IRY1,Y2κ identifies with the relative entropy of Y1−κ|Y1〉κ and Y2−κ|Y2〉κ.

The purpose of this study is to develop and add more properties, characterizations, order statistics, some inequalities and stochastic orders of weighted differential entropies measures. In Section 2, definitions, notation, basic properties and characterizations are illustrated. The weighted entropy (residual and past residual) of order statistics with some application of reliability systems such as a series structure and a parallel structure are given in Section 3. In addition, we provided the lower bound for the weighted residual (past) entropy. The stochastic orders based on weighted entropy are developed in Section 4. Lastly, in Section 5, the suggested estimators of weighted entropy are presented. Furthermore, we illustrate the usefulness of the proposed non-parametric estimators of weighted entropy by application to real data.

Throughout this article, the term entropy is used instead of differential entropy and using abbreviation PL for past lifetime, WPE for weighted past residual entropy, WRE for weighted residual entropy, SS for the series system, PS for the parallel system, SE for small than or equal.

2. THE WEIGHTED DIFFERENTIAL ENTROPY

The weighted differential entropy WDE defined by Das [8] for random variable Y with weighted function wx=x as:

ξw(Y)=−ϑw(Y)+∫ℒ​xfY(x)lnfY(x)dx−E[Y]lnE[Y]E[Y],=Hw(Y) E[Y] +ln E[Y] −ϑw(Y) E[Y] ,
where
ϑw(Y)=∫ℒxfY(x)ln⁡xdx=:E(Yln⁡Y).
whenever the integral ∫ℒuθfYu/EYθ1∨|lnuθfYu/EYθ|du<∞.

As a general case, we can be defined the generalized the WDE as the following definition:

Definition 2.1.

Given a function y∈ℒ↦wy≥0, and an RV Y:ℱ→ℒ, with a probability density function gY., survival function G¯. and mean EY. Therefore, the weighted differential entropy with weighted function wy=yθ is defined as

ξwY=E−lngYwY=∫ℒgYwuln1gYwudu,=−∫ℒuθgYuEYθlnuθgYuEYθdu,=−1EYθθ∫ℒuθgYuln udu+∫ℒuθgYulngYudu−EYθlnEYθ.
Now, let Y1,Y2,…,Yn be a sample from the distribution F and n≥3. By using Vasicek [9], express Eq. (6) can be rewritten as
ξw(Y)=∫01ln⁡{∂∂uF−1(u)}du.
In addition, Das [8] have defined the weighted residual entropy as
ξw(Y,κ)=−∫κ∞gYw(v)G¯w(κ)ln gYw(v)G¯w(κ)dv,=−1E[Y|Y>κ]∫κ∞vgY(v)G¯(κ)ln vgY(v)E[Y|Y>κ]G¯(κ)dv, κ∈ℝ+.
If fXx is the actual density function of random variable X and gYx is the density function determined by the researcher. Therefore, the weighted inaccuracy measure can be defined as
Rw(X,Y)=−∫ℒxfX(x)ln⁡gY(x)dx.
Next, we define the relative WDE of two densities.

Definition 2.2.

Let X and Y be two random variables with density function, s∈ℒ↦fXws≥0 and s∈ℒ↦gYs≥0, and mean values EX. and EY., respectively. Therefore, the relative weighted differential entropy of gYx relative to fwx can be defined as

ℝXw∥Y=ElnsfXsEXsgYs,=∫ℒvfXvEXXlnvfXvEXvgYvdv.
By using Eq. (4), we can define an alternative formulas of ℝXw∥Y as follows
ℝXw∥Y=ln1EXX−HwXEXX−∫ℒxfXxEXxln xgYxdx.
Note that when gYx≡fXx, then we have
ℝXw∥X=ln1EXX−HwXEXX−∫ℒxfXxEXxln xfXxdx,=lnexp−ϑwX+2HwXEXX/EXX.

Remark 2.1.

By using Eqs. (8) and (9) we get the following relation

ℝXw∥Yw=lnEYXEXX−HwXEXX+ℝXwX,YEXX.
Furthermore, we can define the divergence between fwx and gYx as follows
K(Xw,Y)=ℝ(Xw∥Y) +ℝw(Y∥X) ,=∫ℒ(fXw(x) −gY(x) ) lnfXw(x) gY(x) dx,
it is a measure of the difficulty of discrimination between them.

Now, let X be RV with beta distribution as follows:

fXs=sα−11−sβ−1/Bα,β,s∈ℒ∈0,1.
By using Eq. (3), we get that HX satisfy the following equation:
HX=ln⁡(B(α,b)exp((α+β−2)Ψ(α+β))exp((α−1)Ψ(α)+(β−1)Ψ(β))),
where B.,. is beta function and Ψ. is psi function.

The following theorem states that this relationship actually characterizes the beta distribution.

Characterization Theorem 2.1:

Any random variable Y with distribution function K, density function fYx, mean EY, mode ΓKY, geometric mean GY, entropy function HY and weighted differential entropy ξwY satisfying the following relationship:

ξwY=HY−α−1ΓKY+EYΓKY+lnEY−lnGY+EY−1/α,
is either degenerate or Y has a beta distribution. Indeed, the degenerate case should be subsumed in the beta distribution with α,β∈R+.

Proof.

By using the following integral formula which is taken from Gradshteyn and Ryzhik ([10], formula 4.253(1), pp. 538):

∫ℒyθ−11−ycλ−1ln ydy=1c2Bθc,λΨθc−Ψθc+λ,
provided that Reθ>0, Reλ>0, c>0. We denote the beta function with the symbol B(·,·) and the digamma function with Ψ(·). Therefore, we have
ϑw(Y)=∫ℒxfX(x)ln xdx,=1B(α,β)[B(α+1,β)(Ψ(α+1)−Ψ(α+β+1))],=E[Y](Ψ(α+1)−Ψ(α+β+1)).
By using Example 2.3 in Di Crescenzo and Longobard ([4], pp.682), Eq. (4) and the recurrence relation of the digamma function, we can rewrite HwY as follows:
Hw(Y)=E[Y][ln⁡B(α,β)+(1−α)(Ψ(α)+1α)+(α+β−2)(Ψ(α+β)+1α+β)+Ψ(β)(1−β)].
We can reduce Eq. (11) as,
Hw(Y)=E[Y] [HY+(1−α) 1α+(α+β−2) (α+β) ] ,=E[Y] [HY−(α−1) [ΓK(Y) +E[Y] ΓK(Y) ] ] .
This is true for fΓK.=max−∞<x<∞fX.. Furthermore by Eqs. (6) and (10) we have
ξwY=HY−α−1ΓKY+EYΓKY+lnEY−Ψα+1−Ψα+β+1,=HY−α−1ΓKY+EYΓKY+lnEY−ln GY+1αEY−1.
In next results we study the closure transformation property of the weighted entropy. We can now proceed analogously to Di Crescenzo and Longobardi [4] and introduce the following theorem.

Theorem 2.2.

Suppose U is RV with density function fU. and ψU is strongly convex, strictly increasing, continuous and differentiable function with derivative dduψu. Then

ξwψU=ξ1wU|ψ−10≤U≤ψ−1∞+Ewln |ddxψx|ψ−10≤U≤ψ−1∞|
where EwU=∫0∞vfUwvdv.

Proof.

From Eq. (6) we have

ξwψU=−∫0∞fUwψ−1u|dduψ−1u|ln fUwψ−1u|dduψ−1u|du.
We will make the following assumptions:
  1. ψu is monotonically increasing in u.

  2. v=ψu,

Therefore, it clear that

ξwψU=−∫ψ−10ψ−1∞fUwvln fUwv|ddvψv|−1dv.=∫ψ−10ψ−1∞fUwvln |ddvψv|dv+ξwU|ψ−10≤U≤ψ−1∞.
Hence the proof is completed.

Proposition 2.3.

Let ϕU=αUβ whereas α,β>0. From this we deduce that

ξwϕU=ln αβ+β−1ϑwUEU+ξwU.

Proof.

From Eq. (6) we have

ξwϕU=∫0∞fwvln |αβvβ−1|dv−∫0∞fwvln fwvdv,=ln αβ+β−1∫0∞fwvln vdv+ξwU.
By using Eq. (7), we get the required results.

From Definitions (2.1), it is easy to obtain the following characterizations:

Example 2.1:

Suppose U be a random variable having Log-Normal with the following density function

fUu=12πσuexp −ln u−ln μ2/2σ2, μ,σ,u>0,
with parameter μ,σ>0. From Eq. (7) we get,
ϑwU=∫0∞v12πσvexp −ln v−ln μ2/2σ2ln vdv.
Set u=ln⁡v−ln⁡μ, then we have
ϑwU=22πσexp 2ln μ∫0∞exp 2u−u22σ2du.
It is follows from Gradshteyn and Ryzhik ([10], formula 3.322(1)) that
∫a∞exp −x24μ−bxdx=πμexp μb21−Φbμ+a2μ, Reμ>0,a≥0.
Therefore,
ϑwU=exp 2ln μ+σ21−Φ−21/2σ.
In addition,
Hw(U) =−∫0∞v12πσvexp(−(ln v−ln μ)2/2σ2)[−ln 2πσ−ln v−(ln v−ln μ)22σ2]dv,=ln 2πσE[U]+ϑw(U)+∫​∞0v12πσvexp (−(ln v−ln μ)2/2σ2)(ln v−ln μ)22σ2dv,
with the same way, set u=ln v−ln μ and by using formula 3.462(1) in Gradshteyn and Ryzhik [10] we have
∫​∞0v12πσvexp (−(ln v−ln μ) 2/2σ2) (ln v−ln μ) 22σ2dv,=(1σ2) (−3/2) +32μ2πexp (σ24) D−3(−σ).
Therefore,
 Hw(X)=ln(2πσ) μexp(σ2/2) +exp(2(ln μ+σ2) ) (1−Φ(−21/2σ) )+(1σ2) (−3/2) +32μ2πexp(σ24) D−3(−σ) ,=ln(2πσ) E[X] +ϑw(X) +σ−32μ2πexp(σ24) D−3(−σ) ,
where Φ. is Error function, ϖμ,σ=μexp σ2/2−1 and Dxy=2x/2exp −y2/4F−x2,12,y22 is Parabolic cylinder function. We denote a confluent hypergeometric function of the first kind with the symbol F.,.,.. Further,
ξwU=ϖμ,σαμ,σ−ln ϖμ,σ−ϖμ,σexp 2ln μ+σ21−Φ−21/2σ,
where αμ,σ=ln 2πσμexp σ2/2+exp 2ln μ+σ21−Φ−21/2σ+1σ2−3/2+32μ2πexp σ24D−3−σ.

Furthermore,

ℝXw∥X=ln exp −β1μ,σ+2β2μ,σϖμ,σ/ϖμ,σ,
where:
  1. β1μ,σ=exp2ln μ+σ21−Φ−21/2σ;

  2. β2μ,σ=ln2πσEX+ϑwX+1σ2−3/2+32μ2πexpσ24D−3−σ

Example 2.2:

Let X be random variable having Chi distribution with density function

fXx=2π/2π/2γπΓπ/2xπ−1exp−x2π/2γ2,γ,x>0,π is a positive integer, with parameter μ,γ>0. From Eq. (7) we have

ϑwX=2π/2π/2γπΓπ/2∫0∞xπexp−x2π/2γ2ln xdx,
take u=x2π/2γ2, then we get
ϑwX=γ1/2π1/2Γπ/2∫0∞uπ2−0.5exp−ulnu/π/2γ21/2du.
By using Gradshteyn and Ryzhik ([10], 4.352(1)) for evaluate the below formula, we have the following result:
ϑwX=γ1/2π1/2Γπ/2Γπ+12ψπ+12−lnπ/2γ2.
In addition, by Eq. (4) we have
HwX=−∫0∞x2π/2π/2γπΓπ/2xπ−1exp−x2π/2γ2ln2π/2π/2γπΓπ/2+π−1ln x−x2π2γ2dx,
since EX=γ2πΓπ+12Γπ2. With this substitution we obtain
HwX=π2−π1π−1∫0∞vπexp−v2π/2γ2ln vdv+π3∫0∞vπ+2exp−v2π/2γ2dv,
where π1=2π/2π/2/γπΓπ/2, π2=−lnπ1γΓπ+12/Γπ22/π, π3=π/2γ2π1. Direct calculations give
HwX=γπ+1Γπ+122π/21/2Γπ/2−ln2π/2π/2γπΓπ/2γ2πΓπ+12Γπ2−2π/2π/2π−1γπΓπ/2∫0∞xπexp−x2π/2γ2ln xdx.
Again, we the same way and continuing the simplification, we can conclude that
HwX=−γΓπ+12/Γπ/2ln2π/2π/2γπΓπ/22π+2π−14π/2ψπ+12−lnπ/2γ2−π+12π/21/2.
Therefore,
ξwX=−ln2/γπ−2π−14ψπ+12−lnπ/2γ2+π+121−lnπ/2+lnγΓπ+12−ψπ+12+ln π/2γ2.
Continuing the simplification
ξwX=lnπγπ−14−2π−14ψπ+12−lnπ/2γ2+π+121−lnπ/2+lnΓπ+12−ψπ+12.
Moreover,
ℝXw∥X=−πα1ψπ+12−ln π/2γ2+2HwXα1−lnα1,
where α1=γΓπ+12/Γπ22/π. Continuing the simplification
ℝwXw∥X=4π+12lnπ/2γ2+2ln2+ψπ+12π−2−π+1−lnΓπ+12Γπ2.

Example 2.3:

A random variable U has a Laplace α, if it has density function as follows

fUu=12αexp−α|u|,α,∞>u>−∞,
with parameter α>0. From Eq. (7) we obtain,
ϑwU=∫−∞∞v12αexp−α|v|ln vdv=ψ2−ln α/α,
Furthermore, direct calculations give
HwU=−∫0∞xαexp−αxlnα2−αxdx,=2−ln α+ln 2αnats=1+HUαnats.

Since EU=0, we get that ξ1wU and ℝ1wUwU can not be found.

3. CONNECTION TO RELIABILITY THEORY

Suppose U1,U2,…,Un be i.i.d. lifetimes with probability density function g., distribution K., survival function K¯. and reversed hazard rate φK.. Therefore, the probability that any two (or more) observation in random sample take the same magnitude (the same value is equal to zero). Therefore, there exists a unique ordered arrangement of the sample observation according to magnitude. Let 0≤U1≤U2≤…≤Un<∞ be the corresponding order statistics. Therefore, Ur defines the lifetime of an (n−r+1)out of n system. Write gr., Kr., φr. and φ¯r. as the distribution function, the probability density function, the RHR function of Ur and the hazard rate of Ur respectively. Then we have

g(r)(κ)=Cr[K(κ)]r−1[K¯(κ)]n−rg(κ),κ∈R+,K(r)(κ)=∑i=rn(ni)[K(κ)]i[K¯(κ)]n−i,φ(r)(κ)=CrφK(κ)βr/(∑i=rn(ni)βi),
and
φ¯rκ=grκ/K¯rκ,
where Cr=n!r−1!n−r! and βx=Kκ/K¯κx. The weighted residual entropy of order statistics Ur is given by
ξ1w(U(r) ,κ)=−∫​κ∞g(r) w(u) K¯(r) w(κ) lng(r) w(u) K¯(r) w(κ) du,=−1E[U(r) |U(r) >κ] ∫​κ∞yg(r) (y) K¯(r) (κ) ×lnyg(r) (y) E[U(r) |U(r) >κ] K¯(r) (κ) dy.
Alternatively,
ξ1w(U(r),κ)=−1E[U(r)|U(r)>κ]×∫​κ∞yg(r) (y) K¯(r) (κ) lnyφ¯(r) (y) K¯(r) (y) E[U(r) |U(r) >κ] K¯(r) (κ) dy,=ln[E[U(r) |U(r) >κ] K¯(r) (κ) ]−1E[U(r) |U(r) >κ] ∫​κ∞yg(r) (y) K¯(r) (κ) ln(yφ¯(r) (y) K¯(r) (y) ) dy.
Now, we can proceed analogously to treatment of the weighted entropy of the order statistics of PL as follows
ξ2wUr,κ=−∫0κgrwvKrwκlngrwvKrwκdv,=−1EUr|Ur<κ∫0κvgrvKrκlnvgrvEUr|Ur<κKrwκdv,
which is equivalent to
ξ2wUr,κ=−1EUr|Ur<κ∫0κxgrxKrκlnxφrxK¯rxEUr|Ur<κKrwκdx.
Direct calculations give
ξ2w(U(r),κ)=ln⁡[E[U(r)|U(r)<κ]K(r)(κ)]−1EUr|Ur<κ∫0κvgrvKrwκκlnvφrvKrvdv,
for all κ≥0.

3.1. A Series Structure

It is to be noted that U1 represents an age of the series system. By using Eq. (13), with simple calculation, we have the weighted the residual entropy of U1 as

ξ1w(U(1),κ)=ln[E[U(1)|U(1)>κ]K¯(1)(κ)]−1E[U(1) |U(1) >κ] ∫​κ∞vg(1) (v) K¯(1) (κ) ln(vφ¯(1) (v) K¯(1) (v))dv,=ln[E[U(1) |U(1) >κ] K¯(1) (κ) ]−1E[U(1) |U(1) <κ] ∫​κ∞vn[K¯(v) ] n−1g(v) [K¯(κ) ] nln(vφ¯(1) (v) [K¯(v) ] n) dv. 
It follows from Proposition 1 in Bairamov et al. [11], and definition of mean residual lifetime of n−k+1-out-of-n system in Asadi and Bayramoglu [12] that
EU1|U1>κ=∫κ∞K¯1vdvK¯1κ=M1κsay,
and
K¯κ=M10M1κexp−∫0κM1−1κ1/n,
Then, Eq. (15) can be written in the following form
ξ1wU1,κ=lnM10exp−∫0κM1−1κ+∫κ∞vnK¯vn−1gvK¯κnln vφ¯1vK¯vndvM10exp −∫0κM1−1κ.
Similarly, by Eq. (14), the WPE of U1 follows
ξ2w(U(1) ,κ)=ln[E[U(1) |U(1) <κ] K(1) (κ) ] −1E[U(1) |U(1) <κ] ∫​0κvg(1) (v) K(1) (κ) ln(vφ(1) (v) K(1) (v)) dv,=ln[E[U(1) |U(1) <κ] K(1) (κ) ] −1E[U(1) |U(1) <κ] ∫​0κvn[K¯(v) ] n−1g(v) 1−[K¯(κ) ] nln(vφ(1) (v) [1−K¯n(v) ] ) dv.
Eq. (12) implies that
ξ2w(U(1),κ)=ln⁡(E[U(1)|U(1)<κ](1−K¯n(κ)))+∫0K¯κK¯−1unun−1)ln nK¯−1ugK¯−1uuu−n−11−unduEU1|U1>κ1−K¯nκ.
According to Eqs. (4–5) in Tavangar and Asadi [13], the mean PL of series system can be obtained as follows:
P1(κ)=E[κ−U(1)|U(1)<κ],=∑​​l=1n(n(18) l) ακlSl(κ) ∑​​l=1n(n(19) l) ακl,
where α.=K./K¯. and
Sπκ=∫0κ∑l=1ππlKκ−vKκl1−Kκ−vKκπ−ldv,
Equations (17) and (18) demonstrate that
ξ2wU1,κ=ln κ−P1κ1−K¯nκ+∫0K¯κK¯−1unun−1)ln nK¯−1ugK¯−1uuu−n−11−unduκ−P1κ1−K¯nκ.

3.2. A Parallel Structure

It is to be noted that Un refers to the lifetime of PS with survival function K¯n.=1−Kn.. Based on Eq. (13), we can define the weighted the residual entropy of Un as

ξ1wUn,κ=lnEUn|Un>κ1−Knκ−1EUn|Un>κ1−Knκ∫κ∞vnKn−1vgvlnvnKn−1vgvdv.
Applying Theorem 2.1, pp. 477 in Asadi and Bayramoglu [14] and Eq. (18), it obtains that,
EUn|Un>κ=Bnκ+κ,
where Bnκ is mean residual lifetime of PS, it can be found as follows
Bnκ=∑l=1n−1nlαlκ∑s=1n−1s−1n−lsβsκ∑l=1n−1nlαlκ,
and βjκ=∫κ∞K¯jvdvK¯jκ. Now, it is evident that
ξ1wUn,κ=ln Bnκ+κ1−Knκ−nBnκ+κ1−Knκ∫κ∞vKn−1vgvln vnKn−1vgvdv.
By using Eq. (4) in Asadi (2006, pp. 1200), we have the mean PL of the components of PS as follows
θnκ=Eκ−Un|Un≤κ=∫0κKnvdvKnκ.
Putting r=n in Eq. (14) and using Eqs. (12 and 14), we get the WPE of Un as follows
ξ2wUn,κ=lnκ−θnκKnκ−1κ−θnκ∫0κvgnvKnwκlnvφnvKnvdv,=lnκ−θnκKnκ−1κ−θnκ∫0κvgnvKnκEUn|Un<κ)lnvnφKvKnvdv,
which is equivalent to,
ξ2wUn,κ=lnκ−θnκKnκ−nκ−θnκKnκκ−θnκ∫0κvKn−1vgvlnvnφKvKnvdv,
for all κ≥0.

3.3. Some Inequalities

Next, we derive the upper bound of WRE of Ur. It is obvious that

ξ1wUr,κ=ln EUr|Ur>κ+ln K¯rκ −1EUr|Ur>κ∫κ∞vgrvK¯rκln vφ¯rvK¯rvdv,
since lnEUr|Ur>κ≥0 and
κ≥0⇒lnK¯rκ≤0,
by using Gupta et al. [16], we can deduce that
ξ1wUr,κ≤lnEUr|Ur>κ.
For r=1, we have
ξ1wU1,κ≤lnM1κ.
In addition, we know that lnBnκ+κ1−Knκ≤0. Hence, we have
ξ1wUn,κ≤lnBnκ+κ1−Knκ.
In next result, we derive the lower bound for WPE of Un.

Proposition 3.1:

Suppose U≥0 be a random variable with distribution function Kv. Then

ξ2wUn,κ≥−n2Eu2K2n−2ugu|U≤κκ−θnκ2Kn−1κ.

Proof.

Using Eq. (2), inequality −ln y≥1−y, for y≥0, and since

∫0κvKn−1vgvdv≤∫0κnv2K2n−2vg2vdv.
The result follows.

4. STOCHASTIC ORDERS BASED ON WEIGHTED ENTROPY

In this section, we explore the possibility of application of stochastic orders.

Definition 4.1.

Assume U1≥0 and U2≥0 be two random variables with density functions g1 and g2, distribution functions GU1 and GU2, reliability functions G¯U1=1−GU1 and G¯U2=1−GU2 , the weighted entropy functions ξg1w. and ξg2w., the convex residual entropy functions Hg1wU1,t and Hg2wU2,t and the weighted inaccuracy measures ℝU1w∥U1 and ℝU2w∥U2, respectively. We say that U1 is SE to U2 in the:

  • weighted entropy ordering (U1≤ξwU2) if ξg1wx≤ξg2wx, for all x≥0.

  • weighted inaccuracy ordering (U1≤ℝwU2) if ℝU1w∥U1≤ℝU2w∥U2.

  • convex residual entropy ordering (U1≤cwU2) if Hg1wU1,t≤Hg2wU2,t.

  • less uncertainty ordering (U1≤UU2) if HU1≤HU2.

Definition 4.2.

Let U1 and U2 be two random variables, then U1 is said to be SE to U2 in the convex order (U1≤cxU2). If

EϕU1≤EϕU2,
This is true for any convex functions ϕ.

Definition 4.3.

The random variable U1 is said to be increasing hazard rate, IHR, if, and only if,

G¯U1u+v/G¯U1u  is decreasing in u≥0, for all v≥0.

Next result discusses the closure under increasing linear transformation of ≤ξw:

Theorem 4.1.

Suppose U1 and U2 are to be two random variables, let we define new functions as

V1=α1U1β1  and V2=α2U2β2, for all α1,α2∈ℝ+ and β1,β2∈ℝ+.

Let (i) U1≤ξwU2, (ii) α1≤α2, (iii) β1≤β2. Then V1≤ξwV2 if U1≤cxU2.

Proof.

Due to fact that φx=xln x is convex function, and when U1≤cxU2 we get that EU1=EU2, if we suppose that ξU1wu is decreasing in u, and let U1≤ξwU2, α1≤α2 and β1≤β2. By apply Eq. (7) and Proposition 2.3, we have V1≤ξwV2.

Corollary 4.1.

Suppose the relationship between two random variables U1 and U2 as follows:

U1 ≤ξwU2.
Define V1=αU1β and V2=αU2β, α,β∈ℝ+. Then U1≤ξwU2 if U1≤cxU2.

In next theorem, we explain preservation properties and application of ≤ξw, ≤ℝw and ≤U between two exponential RV's if their scale parameters are ordered.

Theorem 4.2.

Let two absolutely continuous random variables U1 and U2 with density function

fix=αiexp−αix, αi,x>0 and i=1,2.

  • If α1≥α2, then U1≤ξwU2.

  • If α1≤α2, then U1≤ℝwU2.

  • If X≤ℝwY then HU2≤UHU1.

Proof.

The result is obtained immediately from Remark 2.1.

Many studies explain the properties of repairable systems such as minimal repair. If the system has the virtual age Un−1 immediately after the n−1th repair, the functioning system obtained has the nth failure-time Yn distributed as

PrYn≤y|Un−1=u=Gy+u−GuG¯u,
where Gy is the failure time distribution of a new system U0=0. Let nth repair cannot remove the damages incurred before the (n−1)th repair and αn be the degree of the nth repair, now the time between n−1th failure and nth failure reduce from Yn to αnYn. If αn=1 for all n≥1 then it agrees with a minimal repair model.

Suppose Vn=∑i=1nYin≧1 with V0=0 which represents the time elapsed since the system was put in operation, or the associated counting process ℕt=supn≧1:Vn−1≦t. Kijima [17] proved that ℕtor Vn0∞ is a non-homogeneous Poisson process when αn=1 for all n≥1. Ebrahimi and Pellerey [1] defined the following definition:

Definition 4.4.

A point process ℕt,t≥0 consisting of interarrival times Y1,Y2,… is increasing (decreasing) in the

  1. convex residual entropy order if

    HwBi,t≤≥HwBj,t,for all t∈R+.

  2. weighted entropy order if

    ξwBi,t≤≥ξwBj,t

and 1≤i≤j≤n, where fk is the conditional probability density function of Yk=Vk−Vk−1 for all k=1,2,…, given Vk−1=vk−1,…,V1=v1, and
Bk=st[Yk|Vk−1=vk−1,…,V1=v1].

From Definition 5.3, we can note that if a point process is increasing (decreasing) means the uncertainty of the distribution is increasing (decreasing), i.e., the process is deterioration (improving).

Lemma 4.1.

Let Bk be as defined in Definition 5.3. Then, for k=1,2,…,

  1. HwBk,t=HwX,t+vk−1;

  2. ξwBk,t=ξwX,t+vk−1.

Proof.

Refer to Ebrahimi and Pellery [1], Theorem 2.5.

Theorem 4.3.

The stochastic point process ℕt=supn≧1:Vn−1≦t consisting of the time of nth failure Vk−1, k=1,2,… generated by a minimal repair policy is increasing (decreasing) in

  1. convex residual entropy order if G. is IHR,

  2. weighted entropy order if ξwU is increasing for all u≥0.

Proof.

Similarly to lemma 5.1, we have HwBk+1,t=HwU,t+vk. In addition, by Theorem 3.1 in Di Crescenzo and Longobardi [4] we conclude that

HwU,t+vk=t+vk1−ln λt+vk+t+vkλt+vkddtHU,t+vk+1G¯t+vkIt+vk,
where
It=∫t∞G¯uHU,udu−∫t∞G¯ulnG¯uG¯tdu,
and by Theorem 2.1 in Ebrahimi and Pellery [1] we have
HwU,t+vk=t+vkHU,t+vk+1G¯t+vkIt+vk.
By Theorem 2.5 in Ebrahimi and Pellery [1] we conclude that HU,t+vn−1≤HU,t+vn. By using Eqs. (20–22), and when a continuous distribution G. is IHR. It is obvious that
G¯t+vk≤G¯t+vk−1,
and
It+vk≥It+vk−1.
Then, we get HwU,t+vk≥HwU,t+vk−1. This complete the proof.

5. ENTROPY ESTIMATION

In this section, we introduce four the non-parametric estimators of Eq. (6) by using the same idea in Vasicek [9], Van Es [18], Ebrahimi et al. [19] and Al-Omari [20].

Let Z1,Z2,…,Zn is a sequence of the random sample with the distribution G and let Z1,Z2,…,Zn be the corresponding order statistics. Besides the sample distribution function Gnz=n−1∑i=1n1Zk≤z,1≤k≤n. Then, the on-parametric estimators can be expressed as:

  1. Weighted Vasicek Entropy (Vξδ,nwZ): We can estimate of Eq. (8) by replacing Gwt by the empirical distribution Gnwt, and using a difference operator in place of the differential operator. Thus, Vξm,nwZ estimator of Eq. (8) can be represented as follows

    Vξδ,nwZ=n−1∑i=1nlnn∑k=1nwZk∑j=1iwZj2δZi+δ−Zi−δ,
    where δ∈ℕ+ know as a window size, δ<n/2, Zs=Z1 if s<1 and Zs=Zn if s>n.

  2. Weighted δ-spacings Entropy (SEξδ,nwZ): Estimates of weighted entropy based on sample δ-spacings which introduced by Van Es [18], we can provide VEξδ,nwZ estimator of Eq. (6) as

    SEξδ,nwZ=n−1∑i=1n−δlnn∑j=1iZj∑k=1nZkδZi+δ−Zi−ψδ+ln δ+EZ,
    where ψ. is the digamma function and ln δ−ψδ corrected bias entropy estimator.

  3. Weighted Small weights Entropy (WSξδ,nwZ): As assign smaller weights in Vasicek [9], we obtain

    WSξδ,nwZ=n−1∑i=1nlnn∑k=1nZk∑j=1iZjαiδZi+δ−Zi−δ,
    where
    αk={δ+k−1δ,1≤k≤δ2,δ+1≤k≤n−δδ+n−kδ,n−δ+1≤k≤n.

  4. Modified Small weights Entropy (MSξδ,nwZ): As assign smaller weights in Ibrahimi et al. [21] we get

    MSξδ,nwZ=n−1∑i=1nlnn∑k=1nwZk∑j=1iwZjβiδZi+δ−Zi−δ,
    where
    βi={32,1≤i≤δ,2,δ+1≤i≤n−δ,12,n−δ+1≤i≤n..

Example 5.1:

Let Z be random variable having exponential distribution with density function fZx=αexp−αz, α,z>0 with parameter α>0. From Eq. (7) we obtain,

ϑwZ=1αψ2−ln α,
where ψ. is Euler's psi function. By Example (2.1, a) in Di Crescenzo and Longobardi [4] we get,
HwZ=2−ln αα and ξ1wZ=2−ln α−ψ2.
Therefore,
ℝZwZ=−41−ln α−ψ2=−4HZ−ψ2.
Suppose α∈0,100. HwZ, ξwZ and ℝZwZ with weighted function wz=z is evaluated in Table 1.

α H^wZ ξ^wZ ℝ^wZwZ
0.25 13.5452 2.9635 -9.9680
0.5 5.3863 2.2704 −7.1954
1 2 1.5772 −4.4228
5 0.0781 −0.0322 2.0150
10 −0.0303 −0.7254 4.7876
Table 1

Measures of weighted entropies of exponential distribution.

Now, a real data is illustrated to investigate the performance of suggested estimators.

Data Set: The following data set which is taken from Smith and Naylor [22], it represents the strength of 1.5 cm glass fibers measured at the National Physical Laboratory, England.

Data Set: 0.55, 0.93, 1.25, 1.36, 1.49, 1.52, 1.58, 1.61, 1.64, 1.68, 1.73, 1.81, 2.00, 0.74, 1.04, 1.27, 1.39, 1.49, 1.53, 1.59, 1.61, 1.66, 1.68, 1.76, 1.82, 2.01, 0.77, 1.11, 1.28, 1.42, 1.50, 1.54, 1.60, 1.62, 1.66, 1.69, 1.76, 1.84, 2.24, 0.81, 1.13, 1.29, 1.48, 1.50, 1.55, 1.61, 1.62, 1.66, 1.70, 1.77, 1.84, 0.84, 1.24, 1.30, 1.48, 1.51, 1.55, 1.61, 1.63, 1.67, 1.70, 1.78, 1.89

Shanker et al. [23] show the exponential density function (Exp0.663647) provided a better fit for this data. We compute the exact value of the weight entropy measure by the real data and compare this measure with Vξδ,nwZ, SEξδ,nwZ, WSξδ,nwZ and MSξδ,nwZ which shows in Table 2.

δ ξδ,nwZ Vξδ,nwZ SEξδ,nwZ WSξδ,nwZ MSξδ,nwZ
1 1.9872 1.210967749 1.244680937583 1.232972422 1.237538804
2 1.9872 1.200196229 1.231653171583 1.943017269 1.298445816
3 1.9872 1.245455104 1.462350850583 2.308545839 1.323498873
4 1.9872 1.279410563 1.650373401583 2.537544185 1.337842382
5 1.9872 1.282220574 1.820823663583 2.721711858 1.415075846
Table 2

Weighted entropy measure for exponential distribution (0.663647).

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Journal
Journal of Statistical Theory and Applications
Volume-Issue
17 - 4
Pages
703 - 718
Publication Date
2018/12/31
ISSN (Online)
2214-1766
ISSN (Print)
1538-7887
DOI
10.2991/jsta.2018.17.4.11How to use a DOI?
Copyright
© 2018 The Authors. Published by Atlantis Press SARL.
Open Access
This is an open access article under the CC BY-NC license (http://creativecommons.org/licences/by-nc/4.0/).

Cite this article

TY  - JOUR
AU  - M. Ramadan
PY  - 2018
DA  - 2018/12/31
TI  - Weighted Entropy Measure: A New Measure of Information with ts Properties in Reliability Theory and Stochastic Orders
JO  - Journal of Statistical Theory and Applications
SP  - 703
EP  - 718
VL  - 17
IS  - 4
SN  - 2214-1766
UR  - https://doi.org/10.2991/jsta.2018.17.4.11
DO  - 10.2991/jsta.2018.17.4.11
ID  - Ramadan2018
ER  -