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Research article Special Issues

Generalized Reed-Solomon codes over number fields and exact gradient coding

  • Received: 31 December 2023 Revised: 09 February 2024 Accepted: 20 February 2024 Published: 07 March 2024
  • MSC : 11T71, 68P30

  • This paper describes generalized Reed-Solomon (GRS) codes over number fields that are invariant under certain permutations. We call these codes generalized quasi-cyclic (GQC) GRS codes. Moreover, we describe an application of GQC GRS codes over number fields to exact gradient coding.

    Citation: Irwansyah, Intan Muchtadi-Alamsyah, Fajar Yuliawan, Muhammad Irfan Hidayat. Generalized Reed-Solomon codes over number fields and exact gradient coding[J]. AIMS Mathematics, 2024, 9(4): 9508-9518. doi: 10.3934/math.2024464

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  • This paper describes generalized Reed-Solomon (GRS) codes over number fields that are invariant under certain permutations. We call these codes generalized quasi-cyclic (GQC) GRS codes. Moreover, we describe an application of GQC GRS codes over number fields to exact gradient coding.



    Shannon [27] illustrated the classical Shannon of entropy measure of uncertainty. Supported with R, the continuous Shannon entropy function for the random variable (RV) X with the probability density function (PDF) f(x) is provided as follows:

    SN(X)=E(lnf(X))=Rf(x)lnf(x)dx. (1.1)

    Lad et al. [12] presented the idea of an extropy measure as a complementary measure to Shannon's entropy. The extropy of the discrete RV X, which is defined over the set Q={x1,...,xN} and has a probability vector denoted as p=(p1,...,pN), can be formulated in the following manner:

    Ext(X)=Ni=1(1pi)ln(1pi); (1.2)

    see additional details in [10] and the references therein. Additionally, the concept of the continuous RV (C-RV) X's extropy, which is defined over the set of real numbers R, has been presented by Raqab and Qiu [23] and Qiu [21], and it is defined as

    Ext(X)=12Rf2(x)dx. (1.3)

    Denote the non-negative and absolutely C-RV X as the new system life length with time t and cumulative distribution function (CDF) F(.). The residual lifetime of an individual is denoted by X(R)t:=[Xt|Xt] with the PDF f(R)(x;t)=f(x)¯F(t), xt. Moreover, the past lifetime of an item is denoted by X(P)t:=[X|Xt] with the PDF f(P)(x;t)=f(x)F(t), xt, ¯F(t)=1F(t). Qiu and Jia [22] presented the extropy for the residual life time X(R)t as

    RExt(X(R)t)=12t(f(x)1F(t))2dx. (1.4)

    Moreover, Krishnan et al. [11] studied the past extropy as

    PExt(X(P)t)=12t0(f(x)F(t))2dx. (1.5)

    Numerous researchers proposed multiple measures of entropy and their extensions. Among these extensions to account for different forms of uncertainty, Tsallis [29] illustrated the so-called Tsallis entropy. In the context of a C-RV X defined over R, with β1, β>0, the continuous Tsallis entropy is defined as

    Tnβ(X)=1β1(1Rfβ(x)dx), (1.6)

    where limβ1Tnβ(X)=SN(X). In addition, the connection between Tsallis and Renyi entropy can be found in Mariz [18], as we can see that Rnβ(X)=log(1+(1β)Tnβ(X))/(1β), with β1 and β>0, where Rnβ(X) is the Renyi entropy defined in [24]. Moreover, for cumulative Tsallis entropy see Mohamed et al. [17] and the references therein.

    Extropy can be used as an alternate measure to examine uncertainty because it has many matching effects to entropy (Meng et al. [15]; Xie et al. [32]). Under the concept of extropy, numerous dual structures for the entropy have been offered (Zhou and Deng [34]). Jahanshahi et al. [6] suggested a cumulative residual extropy. In addition, a negative cumulative extropy (Tahmasebi and Toomaj [28]) has been presented. Moreover, ordered variables (Noughabi and Jarrahiferiz [20]; Raqab and Qiu [23]; Qiu [21]), lifetime distribution (Kamari and Buono [8]), forecast distribution (Lad et al. [13]) and estimators of RVs (Noughabi and Jarrahiferiz [19]) have been discussed.

    Drawing from the context of a discrete distribution lifetime, Xue and Deng [33] suggested the Tsallis extropy model, which serves as the dual counterpart to the Tsallis entropy, and explored its maximization value. Additionally, Balakrishnan et al. [3] investigated the Tsallis extropy, employing it in the realm of pattern recognition. Using the softmax function, Jawa et al. [7] delved into the residual and past aspects of Renyi and Tsalliss extropy.

    Recently, Mohamed et al. [16] presented the continuous Tsallis extropy of the RV X backed by [a, b], <a<b<, as follows

    Txβ(X)=1β1(ba(1f(x))dxba(1f(x))βdx)=1β1(ba1ba(1f(x))βdx), (1.7)

    where the conditions on β can be given as follows:

    (1) β1, β>0 if f(x)1.

    (2) βZ+{1} if f(x)>1.

    Moreover, regarding the relation to dynamical information measures and the use of survival functions, we can see Contreras-Reyes et al. [4].

    This paper introduces the continuous dynamical version of Tsallis extropy for a continuous distribution lifetime. The residual and past functions for Tsallis extropy and their properties are obtained. Another alternative representation of the Tsallis extropy with additional features is given. The remaining part of the article is therefore structured as follows. In Section 2, the past and residual functions for Tsallis extropy with some bounds, as well as monotone characterization results are introduced. Furthermore, the relation between our models and other measures is obtained. In Section 3, a thorough exploration of multiple properties of the dynamic versions is conducted. Moving on to Section 4, an analysis is presented concerning the Tsallis extropy and its characteristics in terms of both coherent and mixed structures under the conditions of the independent and identically distributed (iid) condition. Additionally, the section provides limits for the Tsallis entropy of system life times. Finally, in Section 4, the Tsallis extropy estimator is presented.

    Inspired by the concepts of Tsallis entropy and extropy functions, this section presents the related measures of residual and past functions for Tsallis extropy as follows.

    Likewise, following the approach presented by Lad et al. [12], we can express the residual and past functions for extropy, respectively, as shown below:

    RExt(X(R)t)=t(1f(x)¯F(t))ln(1f(x)¯F(t))dx, (2.1)

    with f(x)¯F(t)<1, and

    PExt(X(P)t)=0(1f(x)F(t))ln(1f(x)F(t))dx, (2.2)

    with f(x)F(t)<1. There is a significant amount of literature on the use of Eqs (1.4) and (1.5) to discuss extropy. In our research, we will also address Eqs (2.1) and (2.2) as an illustrative representation of extropy. In what follows, we will present the definitions of the residual and past functions for Tsallis extropy.

    Definition 2.1. Let X be a C-RV backed by [a,b], <a<b<, with a PDF f(.). Then, the residual function for the Tsallis extropy of the residual lifetime X(R)t can be provided as

    RTxβ(X;t)=1β1(ba(1f(x))dxbt(1f(x)¯F(t))βdx)=1β1(ba1bt(1f(x)¯F(t))βdx), (2.3)

    where the conditions on β are as follows:

    (1) β1, β>0 if f(x)¯F(t)1.

    (2) βZ+{1} if f(x)¯F(t)>1.

    Definition 2.2. Let X be a C-RV backed by [a,b], <a<b<, with a PDF f(.). Then, the past function for the Tsallis extropy of the past lifetime X(P)t can be provided as

    PTxβ(X;t)=1β1(ba(1f(x))dxta(1f(x)F(t))βdx)=1β1(ba1ta(1f(x)F(t))βdx), (2.4)

    where the conditions on β are as follows:

    (1) β1, β>0 if f(x)F(t)1.

    (2) βZ+{1} if f(x)F(t)>1.

    Proposition 2.1. Suppose that X is a non-negative C-RV backed by [a,b], 0<a<b<. Then, from Eqs (2.1)–(2.4), we have

    limβ1RTxβ(X;t)=RExt(X(R)t), (2.5)

    where β1, β>0 and f(x)¯F(t)1.

    limβ1PTxβ(X;t)=PExt(X(R)t), (2.6)

    where β1, β>0 and f(x)F(t)1.

    Proof. By directly applying L'Hˆopital's rule, the results are obtained.

    Now, to discuss some further properties, it is useful to discuss the sign of our models. The following proposition discusses the conditions that guarantee the non-negativity of the residual and past functions for Tsallis extropy.

    Proposition 2.2. Assume that X is a non-negative C-RV backed by [a,b], 0<a<b<, with a PDF f(.) and CDF F(.). From Eqs (2.3) and (2.4), if β>1 (β<1) and f(x)¯F(t)1, a<t<b<, then the residual function for Tsallis extropy is non-negative (negative). Moreover, if β>1 (β<1) and f(x)F(t)1, a<t<b<, then the past function for Tsallis extropy is non-negative (negative).

    Proof. Since f(x)¯F(t)1, then we have

    0bt(1f(x)¯F(t))βdxbt(1f(x)¯F(t))dx=bt1.

    Therefore, from Eq (2.3), when β>1 (β<1), we obtain

    RTxβ(X;t)=1β1(ba1bt(1f(x)¯F(t))βdx)()1β1(ta)()0.

    Similarly, from Eq (2.4), the result follows.

    Example 2.1. Suppose that the C-RV X has a continuous uniform distribution over [a,b], <a<b<, denoted by U(a,b), with a CDF F(x)=xaba and PDF f(x)=1ba. Then, from (2.3) and (2.4), the residual and past functions for Tsallis extropy are given, respectively, by

    RTxβ(X;t)=1β1(ba1(bt)(11(bt))β),
    PTxβ(X;t)=1β1(ba1(a+t)(11(a+t))β).

    Example 2.2. Suppose that the C-RV X has a power function distribution with a CDF and PDF shown, respectively, by

    F(x)=(xλ)θ,
    f(x)=θx(θ1)λθ,0xλandθ,λ>0.

    Then, from Eqs (2.3) and (2.4), the residual and past functions for Tsallis extropy are given, respectively, by

    RTxβ(X;t)=1β1(λ1λt(1+θx(θ1)(tθλθ))θdx),
    PTxβ(X;t)=1β1(λ1ta(1θtθx(θ1))θdx).

    Using different values of θ and λ, Figure 1 gives the residual and past functions for Tsallis extropy of the power function distribution.

    Figure 1.  Power function distributions for residual function for Tsallis extropy with t=1 (upper panel) and past function for Tsallis extropy with t=3 (lower panel).

    Proposition 2.3. Suppose that X is a non-negative C-RV backed by [a,b], 0<a<b<, with the PDF f(.) and CDF F(.). From Eqs (2.3) and (2.4), we have the following properties.

    i) From Eq (2.3) and under the conditions that 0<f(x)¯F(t)<1, β1 and β>0, we have

    RTxβ(X;t)1β1(ta1+β).

    ii) From Eq (2.4) and under the conditions that 0<f(x)F(t)<1, β1 and β>0, we have

    PTxβ(X;t)1β1(bt1+β).

    Proof. i) Property (i) can be obtained from Eq (2.3) and under the conditions 0<f(x)¯F(t)<1, β1 and β>0. Furthermore, employing Bernoulli's inequality, we have

    RTxβ(X;t)=1β1(ba1bt(1f(x)¯F(t))βdx)1β1(ba1bt(1βf(x)¯F(t))dx)=1β1(ta1+βbtf(x)¯F(t)dx)=1β1(ta1+β).

    Similarly, (ii) can be obtained.

    Definition 2.3. Suppose that X is a C-RV backed by [a,b], <a<b<. Then,

    (1) X is a decreasing (increasing) residual function for Tsallis extropy of order β (DRTEXβ (IRTEXβ)) if RTxβ(X;t) is decreasing (increasing) in terms of t, where β is defined in Eq (2.3).

    (2) X is a decreasing (increasing) past function for Tsallis extropy of order β (DPTEXβ (IPTEXβ)) if PTxβ(X;t) is decreasing (increasing) in terms of t, where β is defined in Eq (2.4).

    Proposition 2.4. Let X be a C-RV backed by [a,b], <a<b<, with a PDF f(.). Therefore, an alternative representation of the residual function for Tsallis extropy with respect to the hazard rate function ψ(x)=f(x)¯F(x) is given by

    RTxβ(X;t)=1β1(ba1+Aβi=0(βi)1iE[(ψ(Xi,t))i1]), (2.7)

    where

    Aβ={β,βZ+{1};,β1,β>0whenf(x)¯F(t)<1,

    and the RV Xi,t has the PDF

    fXi,t(x,t)=if(x)¯F(t)(¯F(x)¯F(t))i1,xt>0.

    Proposition 2.5. Let X be a C-RV backed by [a,b], <a<b<, with a PDF f(.). Therefore, an alternative representation of the past function for Tsallis extropy with respect to the reversed hazard rate function Ω(x)=f(x)F(x) is given by

    PTxβ(X;t)=1β1(ba1+Bβi=0(βi)1iE[(Ω(Xi,t))i1]), (2.8)

    where

    Bβ={β,βZ+{1};,β1,β>0whenf(x)F(t)<1,

    and the RV Xi,t has the PDF

    gXi,t(x,t)=if(x)F(t)(F(x)F(t))i1,a<t<x<b.

    Lemma 2.1. According to Eqs (2.7) and (2.8), we have

    ddtRTxβ(X;t)=ψ(t)β1(Aβi=0(βi)(ψ(t))i1+Aβi=0(βi)E[(ψ(Xi,t))i1]), (2.9)
    ddtPTxβ(X;t)=Ω(t)β1(Bβi=0(βi)(Ω(t))i1Bβi=0(βi)E[(Ω(Xi,t))i1]) (2.10)

    for all t0.

    Remark 2.1. (1) If X is DRTEXβ (IRTEXβ), then ddtRTxβ(X;t)=0 and we have Aβi=0(βi)E[(ψ(Xi,t))i1]=Aβi=0(βi)(ψ(t))i1.

    (2) If X is DPTEXβ (IPTEXβ), then ddtPTxβ(X;t)=0 and we have Bβi=0(βi)E[(Ω(Xi,t))i1]=Bβi=0(βi)(Ω(t))i1.

    In the upcoming theorem, we examine the connection between IRTEXβ with increasing failure rate (IFR) and DPTEXβ with decreasing reversed failure rate (DRFR).

    Theorem 2.1. Suppose that X is a non-negative C-RV backed by [a,b], 0<a<b<, with a PDF f(.) and CDF F(.).

    (1) From Eqs (2.3) and (2.7), when β>1 and f(x)¯F(t)1, if X is IFR, X is IRTEXβ.

    (2) From Eqs (2.4) and (2.8), when β>1 and f(x)F(t)1, if X is DRFR, X is DPTEXβ.

    Proof. (1) Let X be the IFR; then, ψ(x) is increasing in terms of x. From Eqs (2.3) and (2.7), when β>1 and f(x)¯F(t)1, we have

    Aβi=0(βi)E[(ψ(Xi,t))i1]=Aβi=0(βi)bt(ψ(x))i1fXi,t(x,t)dxAβi=0(βi)(ψ(t))i1

    for t0 and from Eq (2.9) we get the result.

    (2) Let X be the DRFR; then Ω(x) is decreasing in terms of x. From Eqs (2.4) and (2.8), when β>1 and f(x)F(t)1, we have

    Bβi=0(βi)E[(Ω(Xi,t))i1]=Bβi=0(βi)bt(Ω(x))i1gXi,t(x,t)dxBβi=0(βi)(Ω(t))i1

    for t0 and from Eq (2.10) we get the result.

    The plots of the residual and past functions for Tsallis extropy in Figure 2 show that X is not IRTEXβ or DPTEXβ.

    Figure 2.  Power function distribution (β=6,θ=2,λ=5) for the residual function for Tsallis extropy (left panel) and past function for Tsallis extropy (right panel) with respect to t.

    In the next part, we will obtain some interesting residual and past functions for Tsallis extropy when the order β=2 is selected.

    Remark 2.2. According to Definitions 2.1 and 2.2, the residual and past functions for Tsallis extropy of order β=2 is selected; then, they are accurate for both f(x)1 or f(x)>1.

    The following example gives the residual and past functions for Tsallis extropy of order β=2 for the finite range.

    Example 2.3. Suppose that the C-RV X has a continuous finite range with a beta distribution function F(x)=1(1x)θ and PDF f(x)=θ(1x)θ1, x(0,1), θ>1. Then, from Eqs (2.3) and (2.4), the residual and past functions for Tsallis extropy of order β=2 are given, respectively, by

    RTx2(X;t)=1+t+θ2((1+t)(1+2θ)),
    PTx2(X;t)=2t((1+(1t)2θ+t)θ2)((1+(1t)θ)2(1+t)(1+2θ)).

    Proposition 2.6. Suppose that X is a C-RV backed by [a,b], <a<b<. Then, from Eqs (2.3), (2.4), (1.4) and (1.5), we have

    (1) RTx2(X;t)=ta+RTn2(X;t)=ta+1+2RExt(X(R)t),

    (2) PTx2(X;t)=bt+PTn2(X;t)=bt+1+2PExt(X(R)t),

    where RTnβ(X;t)=1β1(1bt(1f(x)¯F(t))βdx) and PTnβ(X;t)=1β1(1ta(1f(x)F(t))βdx) are the residual and past functions for Tsallis entropy of order β, respectively; for more details about those measures, see [1].

    Proof. From Eq (2.3), when β=2, we have

    RTx2(X;t)=121(ba1bt(1f(x)¯F(t))2dx)=ba1(bt2+bt(1f(x)¯F(t))2dx)=ta+RTn2(X;t)=ta+1+2RExt(X(R)t).

    It is similar for PTx2(X;t).

    Theorem 2.2. The residual and past functions for Tsallis entropies of order 2 are uniquely determined by the hazard rate function ψ(t) and reversed hazard rate function Ω(t), t0.

    Proof. From Eq (2.3), when β=2, we have

    ddtRTx2(X;t)=1+2(at1)ψ(t)+ψ2(t)+2ψ(t)RTx2(X;t).

    Therefore, we get

    ddtRTx2(X;t)2ψ(t)RTx2(X;t)=1+2(at1)ψ(t)+ψ2(t). (2.11)

    We can solve the previous first-order linear ordinary differential equation with a varying coefficient ψ(t) by using the integrating factor method (IFM). Thus

    RTx2(X;t)=e2tψ(t1)dt1[t(1+2(at21)ψ(t2)+ψ2(t2))e2t2ψ(t1)dt1dt2+C], (2.12)

    where C is a constant and RTx2(X;t)|t=0=Tx2(X). Similarly, for PTx2(X;t) and from Eq (2.4), when β=2, we have

    ddtPTx2(X;t)=12(tb1)Ω(t)Ω2(t)2Ω(t)PTx2(X;t).

    Therefore, we get

    ddtPTx2(X;t)+2Ω(t)PTx2(X;t)=12(tb1)Ω(t)Ω2(t). (2.13)

    We can solve the previous first-order linear ordinary differential equation with a varying coefficient Ω(t) by using the IFM. Thus

    PTx2(X;t)=e2tψ(t1)dt1[t(12(tb1)Ω(t)Ω2(t))e2t2ψ(t1)dt1dt2+G], (2.14)

    where G is a constant and PTx2(X;t)|t=0=Tx2(X). This completes the proof.

    Remark 2.3. According to Eqs (2.11) and (2.13), we can state that

    (1) RTx2(X;t) is decreasing (increasing) in terms of t if and only if RTx2(X;t)()ta+11+ψ2(t)2ψ(t);

    (2) PTx2(X;t) is decreasing (increasing) in terms of t if and only if PTx2(X;t)()bt+11+Ω2(t)2Ω(t).

    In what follows, we characterize the distribution of the finite range from the perspective of the residual function for Tsallis extropy.

    Theorem 2.3. Suppose that X is a C-RV with failure rate ψ(.). If RTx2(X;t)=t+12kψ(t), where t0 and the non-negative constant k0; thus, X follows a distribution of finite range if and only if k>14.

    Proof. According to Example 2.3, the necessary condition is obtained. In what follows, we will discuss the sufficient part, assuming that RTx2(X;t)=t+12kψ(t), t0. From (2.11), we can see that

    ψ(t)ψ2(t)=4k12k,t0.

    By resolving the equation provided above, we get that ψ(t)=1qt+s, t0; q=14k2k and s=1ψ(0). Therefore, if k>14, then p>0 and ψ(t) is the failure rate of the distribution of the finite range, which is uniquely determined by its failure rate.

    Residual and past functions for Tsallis extropy of order statistics

    Suppose that X1,X2,...,Xn are n independent random samples from a population with a PDF f(.) and CDF F(.). Then, X1:n,X2:n,...,Xn:n are the order statistics (O.S.) of the random samples, and the ith O.S., 1in, is given by

    fi:n(x)=Fi1(x)¯Fni(x)f(x)B(i,ni+1), (2.15)

    where B(i,ni+1) is the beta function.

    Proposition 2.7. From Eqs (2.3) and (2.4), suppose RTxβ(Xi:n;t) and PTxβ(Xi:n;t) are the residual and past functions for Tsallis extropy of the ith O.S. Xi:n, 1in, respectively. Then, we can conclude the following:

    (1) From Eq (2.3), we have

    RTxβ(Xi:n;t)1β1(ta1+β),

    where 0f(x)¯F(t)1.

    (2) From Eq (2.3), we have

    RTx2(Xi:n;t)=ta+1+2RExt(Xi:n;t)=ta+RTn2(Xi:n;t).

    (3) From Eq (2.4), we have

    PTxβ(Xi:n;t)1β1(bt1+β),

    where 0f(x)F(t)1.

    (4) From Eq (2.4), we have

    PTx2(Xi:n;t)=bt+1+2PExt(Xi:n;t)=bt+PTn2(Xi:n;t).

    Proof. From Eqs (2.3) and (2.4), the residual and past functions for Tsallis extropy of the ith O.S. Xi:n, 1in, respectively, are given by

    RTxβ(Xi:n;t)=1β1(ba1bt(1fi:n(x)¯Fi:n(t))βdx),
    PTxβ(Xi:n;t)=1β1(ba1ta(1fi:n(x)Fi:n(t))βdx),

    where Fi:n(t) is the CDF of the ith O.S. Xi:n, 1in. Then, the results follow.

    Theorem 2.4. For t0, if RTx2(Xi:n;t)=t+12kψ(t), where t0 and the non-negative constant k0, then X follows a distribution of finite range if and only if k>n4.

    From the continuous Tsallis extropy definition presented in Eq (1.7), we can represent the continuous Tsallis extropy of the RV X backed by [a,b], <a<b<, as follows

    Proposition 3.1. Let X be a C-RV backed by [a,b], <a<b<, with a PDF f(.). Therefore, an alternative representation of the Tsallis extropy in terms of the hazard rate function ψ(x)=f(x)¯F(x) is given by

    Txβ(X)=1β1(ba1Tβi=0(βi)ba(f(x))idx)=1β1(ba1+Tβi=0(βi)1iE[(ψ(Xi))i1]), (3.1)

    where

    Tβ={β,βZ+{1};,β1,β>0whenf(x)<1,

    and the RV Xi has the PDF

    fXi(x,t)=i¯Fi1(t)f(x).

    According to Shaked and Shanthikumar [26], we will utilize some stochastic orders known as stochastic order (ST), hazard rate (HR) order and dispersive order (DIS) (the order of variability distribution). Moreover, the previous orders indicate the following:

    1- HRST;

    2- DISST.

    Definition 3.1. Suppose that X1 and X2 are non-negative C-RVs backed by [a,b], 0<a<b<. Then, X1 is smaller than X2 for the case of Tsallis extropy of order β, (X1TxX2) if Txβ(X1)Txβ(X2), where β is defined in Eq (1.7).

    Theorem 3.1. Suppose that X1 and X2 are non-negative C-RVs backed by [a,b], 0<a<b<, with PDFs f1, f2 and CDFs F1, F2, respectively. From (3.1), if X1DISX2 then X1TxX2.

    Proof. From (3.1) with β>1 (<1). If X1DISX2, then

    (β1)Txβ(X2)=ba1Tβi=0(βi)(1)i10fi12(F12(u))du()ba1Tβi=0(βi)(1)i10fi11(F11(u))du=(β1)Txβ(X1).

    Then the result follows for all values of β defined in Eq (1.7).

    The next theorem presents the effect of a transformation on the Tsallis extropy of an RV.

    Theorem 3.2. Suppose that X1 is a non-negative C-RV backed by [a,b], 0<a<b<, with the PDF f1, and that X2=φ(X1) where φ is a continuous function with the derivative φ(x) such that E(X22)<. If |φ(x)|1, x supported with X1, then Txβ(X1)Txβ(X2), β is defined in Eq (1.7).

    Proof. Let X2=φ(X1) since the Jacobian transformation Jφ(X2)=|dφ1(X2)dX2|. Therefore, fX2(x)=fX1(φ1(x))|1φ(φ1(x))|. Then,

    Txβ(X2)=1β1[ba1Tβi=0(βi)(1)ibafiX2(x)dx]=1β1[ba1Tβi=0(βi)(1)ibafiX1(φ1(x))(1φ(φ1(x)))idx]=1β1[ba1Tβi=0(βi)(1)i10fiX1(u)(1φ(u))i1du],

    and the rest of the proof is analogous to Theorem 1 in Ebrahimi et al. [5].

    We consider some aging restrictions of the associated RVs and the order β. The following theorem shows the importance of the stochastic order.

    Proposition 3.2. Suppose that X1 and X2 are non-negative C-RVs backed by [a,b], 0<a<b<, with PDFs f1, f2 and CDFs F1, F2, respectively. If X1STX2, then Txβ(X1)()Txβ(X2) for β>1 (β<1) defined in Eq (1.7).

    Proof. Since X1STX2, ¯F1(x)¯F2(x). From (1.7), the result follows.

    Tsallis extropy of a mixture of coherent systems

    The particular case of a coherent structure is the k-out-of-n system. Moreover, a mixture of coherent schemes is deemed a mixed system; see Samaniego [25]. Under the iid case, the PDF of the mixed system lifetime M is given by

    fM(m)=nj=1qjfj:n(x), (3.2)

    where fj:n(x) is defined in Eq (2.15), 1jn. The system signature is the vector q=(q1,...,qn), and qj=P(M=Xj:n), njqj=1, 1jn. The O.S. Uj:n=F(Xj:n), 1jn, has the PDF

    hj(u)=uj1(1u)njB(j,nj+1).

    Therefore, the PDF of W=F(M) is

    hW(w)=nj=1qjhj(w). (3.3)

    By using the previous transformations, the following formula discusses the Tsallis extropy ofM.

    Theorem 3.3. The Tsallis extropy of the mixed system lifetime M is

    Txβ(M)=11β(Tβi=0(βi)(1)i10hiW(w)fi1(F1(w))dwb+a+1), (3.4)

    where hW(w) is defined in Eq (3.3).

    Proof. From (3.1), and using the transformation w=F(m), we have

    Txβ(M)=11β(Tβi=0(βi)(1)iba(nj=1qjfj:n(m))idmb+a+1)=11β(Tβi=0(βi)(1)i10(nj=1qjwj1(1w)njB(j,nj+1))ifi1(F1(w))dwb+a+1)=11β(Tβi=0(βi)(1)i10hiW(w)fi1(F1(w))dwb+a+1). (3.5)

    Theorem 3.4. Under the same signature, suppose that the lifetime of two mixed systems are MX1 and MX2 with n iid component lifetimes. Then, we have the following:

    (1) If X1DISX2, then MX1TxMX2.

    (2) Suppose that R1={0<w<1f2(F12(w))f1(F11(w))<1} and R2={0<w<1f2(F12(w))f1(F11(w))1}. If X1TxX2, then MX1TxMX2, under the condition that R1=R2=ϕ or infwR1hW(w)supwR2hW(w).

    Proof. (1) Since X1DISX2, from Eq (3.1), we have

    (1β)(Txβ(MX1)Txβ(MX2))=Tβi=0(βi)(1)i10hiW(w)×(fi11(F11(w))fi12(F12(w)))dw0(0),

    where β>1(0<β<1), and the result follows.

    (2) Since X1TxX2, from Eq (3.1) when β>1, we have

    Tβi=0(βi)(1)i10(fi11(F11(w))fi12(F12(w)))dw0. (3.6)

    In the sequel, we get

    (1β)(Txβ(MX1)Txβ(MX2))=Tβi=0(βi)(1)i10hiW(w)×(fi11(F11(w))fi12(F12(w)))dw.

    Thus, using (3.6) and the given infwR1hW(w)supwR2hW(w) for β>1, we obtain

    Tβi=0(βi)(1)iR1hiW(w)(fi11(F11(w))fi12(F12(w)))dw+Tβi=0(βi)(1)iR2hiW(w)(fi11(F11(w))fi12(F12(w)))dwTβi=0(βi)(1)i(infwR1hW(w))iR1(fi11(F11(w))fi12(F12(w)))dw+Tβi=0(βi)(1)i(supwR2hW(w))iR2(fi11(F11(w))fi12(F12(w)))dwTβi=0(βi)(1)i(supwR2hW(w))iR1(fi11(F11(w))fi12(F12(w)))dw+Tβi=0(βi)(1)i(supwR2hW(w))iR2(fi11(F11(w))fi12(F12(w)))dw=Tβi=0(βi)(1)i(supwR2hW(w))i10(fi11(F11(w))fi12(F12(w)))dw0.

    Similarly, the result follows for 0<β<1.

    When the components within the system cannot be quantified, or if the system involves a complex function structure, obtaining the Tsallis extropy often becomes challenging. Consequently, establishing the limits of this measure becomes crucial. The subsequent theorem provides the boundaries for Tsallis extropy of the mixed system.

    Theorem 3.5. Suppose that Txβ(X)<, from Eq (3.4) with β>1 (0<β<1), we have

    Txβ(M)()(supw(0,1)hW(w))β(ba1)b+a+11β+(supw(0,1)hW(w))βTxβ(X).

    Proof. From (3.4), we have

    ba1+(1β)Txβ(M)=Tβi=0(βi)(1)i10hiW(w)(fi1(F1(w)))dwTβi=0(βi)(1)i(supw(0,1)hW(w))i10fi1(F1(w))dw(supw(0,1)hW(w))βTβi=0(βi)(1)i10fi1(F1(w))dw=(supw(0,1)hW(w))β[ba1+(1β)Txβ(X)],

    which proves the theorem.

    In the case of the decreasing failure rate (DFR) of the lifetimes component, the following theorem indicates that the minimum lifetime has a lower or equal Tsallis extropy order in the iid case than for all of the mixed systems.

    Theorem 3.6. Consider the iid case and the lifetime component to be DFR. Then, X1:nTxM, where M is the mixed lifetime system.

    Proof. According to Bagai and Kochar [2], under the condition of the DFR lifetime, we have that X1:nHRM X1:nDISM. From Theorem 3.1, we get that X1:nTxM.

    Theorem 3.7. Suppose that Txβ(Xj:n)<, from Eq (3.4), we have

    Txβ(M)nj=1qjTxβ(Xj:n),

    where Txβ(Xj:n) is the Tsallis extropy of the jth O.S.

    Proof. Recall Eq (3.5), we have

    Txβ(M)=11β(Tβi=0(βi)(1)iba(nj=1qjfj:n(m))idmb+a+1).

    Using Jensen's inequality, we obtain

    (nj=1qjfj:n(m))β()nj=1qjfβj:n(m),

    where fβj:n is concave (convex) when 0<β<1 (β>1) and m>0. Thus,

    bafβM(m)dm=ba(nj=1qjfj:n(m))βdm()nj=1qjbafβj:n(m)dm,Tβi=0(βi)(1)iba(nj=1qjfj:n(m))idm()Tβi=0(βi)(1)inj=1qjbafij:n(m)dm; (3.7)

    multiplying (3.7) by 11β, and noting that 1β>0 (1β<0), it holds that

    Txβ(M)11β[Tβi=0(βi)(1)inj=1qjbafij:n(m)dmb+a+1]=11β[nj=1qjTβi=0(βi)(1)ibafij:n(m)dmnj=1qj(ba1)]=nj=1qj[11β(Tβi=0(βi)(1)ibafij:n(m)dm(ba1))]=nj=1qj[11β(ba(1fj:n(m))βdmba(1fj:n(m))dm)]=nj=1qjTxβ(Xj:n).

    The process of measuring the information of C-RVs has gained the interest of numerous researchers; see Qiu and Jia [22], Qiu [21], Noughabi and Jarrahiferiz [19], Jahanshahi et al. [6], and Contreras-Reyes et al. [4]. In this section, we show a non-parametric approach for estimating the extropy of the Tsallis.

    Using the operator for Vasicek's difference (see Vasicek [30] and Kayal and Balakrishnan [9]), the estimate is produced by utilizing the empirical CDF Fn in place of the CDF F and substituting a difference operator for a differential operator. Then, a function for the the O.S. is applied to estimate the derivative of F1(q). Therefore, from (3.1), the Tsallis extropy estimator can be provided as follows

    Txβ,nm(X)=1β1(ba1Tβi=0(βi)ba(f(x))idx)=1β1(ba1Tβi=0(βi)(1)i10[ddqF1(q)]i+1dq)=1β1(ba1Tβi=0(βi)(1)innj=1[nGjm(Xj+mXjm)]i+1), (4.1)

    where

    Gj={1+j1m,1jm2,m+1jnm1+njm,nm+1jn, (4.2)

    a=X1:nX2:n...Xn:n=b, the window size positive integer m<n2 and Xi=X1 if i<1 and Xi=Xn if i>n.

    The proposed Tsallis extropy estimators are demonstrated to be consistent by the following theorem. Vasicek [30] has stated that its proof is apparent, so it is ignored.

    Theorem 4.1. Suppose that the random sample X1,X2,...,Xn has a CDF F, a PDF f and finite variance. Then,

    Txβ,nm(X)PTxβ(X),

    as n, m and mn.

    We have generated the data from U(a,b) distribution and calculated the Tsallis extropy estimation. Table 1 contains the root mean squared error (RMSE) and standard deviation (SD) of the Tsallis extropy estimates after repetition 1000 times for each sample size. If β=2, then the Tsallis extropies of U(0,1), U(0,2), U(0,3) are 0, 0.5, 23, respectively. If β=3, then the Tsallis extropies of U(0,1), U(0,2), U(0,3) are 0, 38, 59, respectively. Figures 3 and 4 show the behavior of the estimated value to the theoretical value. We can conclude the following from Table 1 and Figures 3 and 4:

    Table 1.  RMSE and SD results for Tsallis extropy estimator for U(0,1), U(0,2), U(0,3), and β=2,3.
    n m RMSE (SD) with β=2 RMSE (SD) with β=3
    U(0,1) U(0,2) U(0,3) U(0,1) U(0,2) U(0,3)
    5 2 0.7401 (0.7353) 0.4357 (0.4123) 0.4535 (0.3401) 4.21 (3.98) 0.9013 (0.8204) 0.4233 (0.333)
    10 2 0.4975 (0.4821) 0.4552 (0.3015) 0.731 (0.2799) 1.963 (1.796) 0.4461 (0.3418) 0.3868 (0.1735)
    3 0.4367 (0.3326) 0.6363 (0.2466) 0.9241 (0.2646) 1.003 (0.7084) 0.4592 (0.1553) 0.5248 (0.1497)
    4 0.7425 (0.2488) 0.8184 (0.2196) 1.0469 (0.2641) 1.3207 (0.4249) 0.7386 (0.1596) 0.7151 (0.1596)
    20 2 0.2948 (0.2949) 0.584 (0.188) 1.0032 (0.1811) 1.051 (0.8495) 0.3727 (0.1575) 0.4897 (0.1034)
    3 0.3308 (0.2139) 0.7706 (0.1645) 1.2119 (0.1817) 0.4719 (0.196) 0.4192 (0.0833) 0.6055 (0.1066)
    4 0.4375 (0.19701) 0.8469 (0.1648) 1.2742 (0.19102) 0.4934 (0.1147) 0.4861 (0.0872) 0.6637 (0.1117)
    5 0.5387 (0.1786) 0.8936 (0.1623) 1.2949 (0.1976) 0.6106 (0.0992) 0.5563 (0.0874) 0.7081 (0.1131)
    6 0.6698 (0.1687) 0.9495 (0.1646) 1.3186 (0.20614) 0.8034 (0.0892) 0.6525 (0.0894) 0.7663 (0.1163)
    7 0.8267 (0.1477) 1.0087 (0.1539) 1.3352 (0.1986) 1.0962 (0.1396) 0.7793 (0.0947) 0.8368 (0.1137)
    8 1.034 (0.1527) 1.0915 (0.1605) 1.3668 (0.2085) 1.5439 (0.2671) 0.9617 (0.1274) 0.9395 (0.1274)
    9 1.3099 (0.1788) 1.2096 (0.1686) 1.4243 (0.21206) 2.226 (0.4766) 1.228 (0.1902) 1.0915 (0.1525)
    30 2 0.2245 (0.2195) 0.6526 (0.1354) 1.1158 (0.1281) 0.801 (0.5608) 0.3793 (0.1004) 0.5396 (0.0728)
    3 0.32309 (0.1707) 0.8451 (0.1266) 1.3402 (0.1376) 0.4691 (0.2379) 0.442 (0.0677) 0.6586 (0.08)
    4 0.4102 (0.1509) 0.9155 (0.1268) 1.4077 (0.1478) 0.4096 (0.0951) 0.4863 (0.0697) 0.7071 (0.0873)
    5 0.4735 (0.1517) 0.9486 (0.1335) 1.4294 (0.1601) 0.4515 (0.079) 0.5229 (0.0741) 0.7344 (0.0934)
    6 0.5347 (0.1425) 0.97108 (0.134) 1.43307 (0.1649) 0.5066 (0.0454) 0.5592 (0.0754) 0.7554 (0.0954)
    7 0.6008 (0.1368) 0.9926 (0.1354) 1.4334 (0.1707) 0.5929 (0.0413) 0.6023 (0.0756) 0.7785 (0.0971)
    8 0.6714 (0.1279) 1.0129 (0.1308) 1.4294 (0.1677) 0.7097 (0.0477) 0.6532 (0.0726) 0.8038 (0.0942)
    9 0.7569 (0.1253) 1.0389 (0.1318) 1.4275 (0.1707) 0.8596 (0.0625) 0.717 (0.0727) 0.8363 (0.095)
    10 0.8616 (0.1188) 1.0777 (0.1297) 1.4381 (0.1703) 1.0532 (0.0909) 0.8003 (0.0758) 0.8827 (0.0953)
    11 0.9838 (0.1175) 1.1243 (0.1326) 1.4529 (0.1763) 1.3073 (0.1419) 0.9047 (0.0871) 0.9406 (0.1007)
    12 1.1292 (0.1187) 1.1785 (0.1278) 1.4685 (0.16801) 1.6314 (0.2051) 1.034 (0.1006) 1.0111 (0.1016)
    13 1.3103 (0.1326) 1.2578 (0.1373) 1.5091 (0.1789) 2.0697 (0.3103) 1.2073 (0.1329) 1.1114 (0.1175)
    14 1.5193 (0.15704) 1.3459 (0.1485) 1.5501 (0.1877) 2.6384 (0.4579) 1.4218 (0.1805) 1.2317 (0.1405)
    50 2 0.1903 (0.1668) 0.719 (0.0997) 1.2183 (0.0912) 1.1642 (0.9907) 0.4633 (0.2167) 0.5997 (0.0953)
    3 0.3328 (0.1201) 0.9231 (0.0871) 1.4644 (0.0939) 0.4082 (0.1315) 0.4697 (0.0449) 0.7143 (0.0555)
    4 0.4139 (0.1083) 0.9957 (0.08608) 1.5447 (0.0982) 0.3755 (0.0708) 0.5082 (0.0468) 0.7632 (0.0584)
    5 0.4658 (0.1031) 1.0309 (0.0896) 1.57703 (0.1069) 0.3774 (0.0449) 0.5331 (0.0511) 0.7881 (0.0632)
    6 0.5021 (0.1021) 1.0471 (0.0937) 1.5851 (0.1146) 0.3953 (0.0353) 0.5512 (0.0544) 0.8009 (0.0672)
    7 0.5312 (0.0988) 1.0549 (0.09269) 1.5824 (0.1147) 0.4214 (0.0326) 0.566 (0.054) 0.8085 (0.0668)
    8 0.5613 (0.09803) 1.0617 (0.0953) 1.5773 (0.1195) 0.4532 (0.0286) 0.583 (0.0554) 0.8159 (0.069)
    9 0.5913 (0.0988) 1.0667 (0.0978) 1.5694 (0.1238) 0.49201 (0.0276) 0.601 (0.0567) 0.8229 (0.071)
    10 0.6213 (0.0986) 1.0716 (0.0995) 1.5612 (0.1268) 0.53902 (0.0262) 0.6207 (0.0571) 0.8306 (0.0723)
    11 0.6562 (0.0979) 1.0785 (0.10019) 1.5539 (0.1284) 0.5931 (0.02604) 0.6438 (0.057) 0.8404 (0.0727)
    12 0.6933 (0.098) 1.0842 (0.10109) 1.5432 (0.13007) 0.6563 (0.0281) 0.6691 (0.0568) 0.8502 (0.0732)
    13 0.7358 (0.09798) 1.0964 (0.1034) 1.5411 (0.1344) 0.7313 (0.0325) 0.7008 (0.0575) 0.8659 (0.075)
    14 0.782 (0.091301) 1.107 (0.1008) 1.534 (0.1332) 0.8161 (0.0382) 0.7353 (0.0563) 0.8815 (0.0736)
    15 0.8353 (0.09132) 1.1226 (0.10102) 1.5322 (0.1332) 0.9158 (0.0461) 0.7764 (0.0569) 0.9021 (0.0739)
    16 0.8937 (0.09125) 1.1394 (0.1029) 1.5296 (0.1366) 1.0314 (0.0616) 0.823 (0.0593) 0.9252 (0.0758)
    17 0.9607 (0.08766) 1.1631 (0.1026) 1.5344 (0.1378) 1.1669 (0.08305) 0.8787 (0.0627) 0.9552 (0.0771)
    18 1.0361 (0.08854) 1.1906 (0.103) 1.5415 (0.1381) 1.3228 (0.1009) 0.9425 (0.0658) 0.99 (0.0779)
    19 1.118 (0.09106) 1.2202 (0.1063) 1.5485 (0.1429) 1.5074 (0.1331) 1.0155 (0.0749) 1.0293 (0.0827)
    20 1.2109 (0.09113) 1.2561 (0.1034) 1.5609 (0.1387) 1.7206 (0.1677) 1.099 (0.0809) 1.076 (0.0823)
    21 1.3155 (0.1008) 1.2992 (0.1084) 1.5794 (0.1431) 1.9763 (0.2201) 1.199 (0.0991) 1.1323 (0.0913)
    22 1.4295 (0.1075) 1.346 (0.1115) 1.5994 (0.1459) 2.2662 (0.2696) 1.3116 (0.1145) 1.1949 (0.0984)
    23 1.559 (0.11906) 1.4014 (0.1157) 1.6258 (0.14801) 2.6181 (0.3391) 1.4449 (0.1366) 1.27 (0.1087)
    24 1.7022 (0.13414) 1.4636 (0.1228) 1.6571 (0.1533) 3.0253 (0.4178) 1.5971 (0.1629) 1.3559 (0.1224)

     | Show Table
    DownLoad: CSV
    Figure 3.  Tsallis extropy estimator for simulated U(0,1) (upper panel) and U(0,3) (lower panel) when β=2.
    Figure 4.  Tsallis extropy estimator for simulated U(0,1) (upper panel) and U(0,3) (lower panel) when β=3.

    (1) Under a fixed n, the RMSE increases by increasing m.

    (2) Under a large and fixed n, the RMSE increases by increasing the range of a and b in the U(a,b) distribution.

    (3) The SD decreases by increasing n and m.

    In this subsection, we utilized the breast cancer Wisconsin (diagnostic) dataset [31], which comprises 569 diagnoses, focusing on presenting real-valued attributes calculated for individual cell nuclei. These features encompass the following: 1) smoothness (reflecting local variations in radius length); 2) compactness (calculated as perimeter2/area -1); 3) concavity (expressing the degree of concavity in contour segments); 4) concave points (tallying the quantity of concave segments within the contour); 5) symmetry, and 6) fractal dimension (measured via "coastline approximation" -1). Furthermore, the "worst" or most considerable value (mean of the three most significant values) of these attributes was computed for each image. Figures 5 and 6 display the correlation between each variable of the Wisconsin worst breast cancer dataset and their respective histograms. Tables 2 and 3 show the Tsallis extropy estimator results for 569 diagnoses of breast cancer Wisconsin data when β=2,3, neglecting any zero or missing values. Furthermore, Figure 7 shows the Tsallis extropy estimator results for 569 diagnoses of breast cancer Wisconsin data when β=2,3 and m=2,3,...,200. Moreover, we can conclude that the Tsallis extropy estimator increases by increasing m and β.

    Figure 5.  Correlation between each variable for data on the worst breast cancer Wisconsin.
    Figure 6.  Histograms of worst breast cancer Wisconsin functions.
    Table 2.  Tsallis extropy estimator results for the 569 diagnosis breast cancer Wisconsin data, with β=2.
    m Smoothness Compactness Concavity Concave points Symmetry Fractal dimension
    2 -16.072 -1.38291 -0.606017 -5.59625 -5.92697 -26.3413
    5 -12.9753 -0.817777 -0.0124867 -4.23306 -4.77741 -21.4673
    10 -12.1106 -0.634671 0.171713 -3.86458 -4.39443 -19.6003
    30 -11.2559 -0.422343 0.389655 -3.40821 -4.03067 -18.1719
    50 -10.5923 -0.253445 0.51764 -3.10719 -3.70565 -16.9701
    100 -8.49788 0.192588 0.866023 -2.22443 -2.70257 -13.4282
    200 -2.84619 1.22606 1.60576 0.0199367 -0.264414 -4.68175

     | Show Table
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    Table 3.  Tsallis extropy estimator results for the 569 diagnosis breast cancer Wisconsin data, with β=3.
    m Smoothness Compactness Concavity Concave points Symmetry Fractal dimension
    2 228.075 3.39238 2.19059 34.6507 31.7404 659.563
    5 110.648 1.61416 0.794512 14.4676 16.4353 336.679
    10 89.3667 1.30072 0.664333 10.7478 13.0594 252.118
    30 77.0099 1.25187 0.681 7.7352 11.5776 216.794
    50 72.328 1.25625 0.737789 6.93683 10.9402 199.884
    100 60.125 1.25529 0.884281 5.50338 9.03925 157.538
    200 35.7649 1.3679 1.34623 5.8625 4.57925 58.4933

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    Figure 7.  Tsallis extropy estimator results for the 569 diagnosis breast cancer Wisconsin data with β=2,3 and m=2,3,...,200.

    Comparative analysis with extropy

    In this part, using the breast cancer Wisconsin (diagnostic) dataset, we will compare the Tsallis extropy estimator given by Eq (4.1) with the original extropy estimator proposed in [21] as follows

    Exβ,nm(X)=12nnj=1Gjmn(Xj+mXjm), (4.3)

    where Gj is defined in Eq (4.2). Figure 8 shows the extropy estimator, and in comparison with Figure 7, we can conclude that the Tsallis extropy estimator gives negative and positive values, unlike the extropy estimator, which is known for negative values. Thus, a comparison of Figures 7 and 8 shows that the Tsallis extropy, a complementary dual of the Tsallis entropy, as a new measure of uncertainty, takes more versatile values. This opens the door to a more effective analysis of many disciplines whereby knowledge is evaluated by utilizing probabilistic notions.

    Figure 8.  Extropy estimator results for the breast cancer Wisconsin (diagnostic) dataset.

    We have examined further properties of Tsallis extropy and its related measures under the condition of continuity. The residual and past Tsallis extropy functions were presented and the conditions of negativity and non-negativity were discussed for those models. Examples of different distributions applied to our measures were given. Moreover, bounded and monotonically increasing and decreasing measures were obtained. Besides, the characterization results for those measures were studied. Furthermore, the properties of the corresponding O.S. were discussed. On the other hand, an alternative representation of the continuous Tsallis extropy with connection to stochastic orders was revealed. These discoveries prompted our investigation into Tsalli's extropy for mixed systems and coherent structures within the context of the iid scenario. Besides, we formulated certain limitations on the systems' Tsallis extropy and demonstrated the practicality of the provided constraints. Finally, the Tsallis extropy estimator, as determined by using the Vasicek's difference operator, was applied to simulated data and real data for breast cancer in Wisconsin. The estimators exhibited increases and decreases according to the n, m and β values.

    The authors affirm that they did not employ Artificial Intelligence (AI) tools in the development of this article.

    We would like to convey our gratitude to the referees for their invaluable contributions and constructive feedback, which has enhanced the quality of the presentation.

    Princess Nourah bint Abdulrahman University Researchers Supporting Project number (PNURSP2023R368), Princess Nourah bint Abdulrahman University, Riyadh, Saudi Arabia.

    The authors declare no conflict of interest.



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