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On the Use of Second and Third Moments for the Comparison of Linear Gaussian and Simple Bilinear White Noise Processes

Abstract

The linear Gaussian white noise process (LGWNP) is an independent and identically distributed (iid) sequence with zero mean and finite variance with distribution . Some processes, such as the simple bilinear white noise process (SBWNP), have the same covariance structure like the LGWNP. How can these two processes be distinguished and/or compared? If is a realization of the SBWNP. This paper studies in detail the covariance structure of . It is shown from this study that; 1) the covariance structure of is non-normal with distribution equivalent to the linear ARMA(2, 1) model; 2) the covariance structure of is iid; 3) the variance of can be used for comparison of SBWNP and LGWNP.

Share and Cite:

Arimie, C. , Iwueze, I. , Ijomah, M. and Onyemachi, E. (2018) On the Use of Second and Third Moments for the Comparison of Linear Gaussian and Simple Bilinear White Noise Processes. Open Journal of Statistics, 8, 562-583. doi: 10.4236/ojs.2018.83037.

1. Introduction

A stochastic process Xt,tZ , where Z={,1,0,1,} is called a white noise or purely random process, if with finite mean and finite variance, all the autocovariances are zero except at lag zero. In many applications, Xt,tZ is assumed to be normally distributed with mean zero and variance, σ2< , and the series is called a linear Gaussian white noise process with the following properties [1] - [7] .

E(Xt)=μ (1.1)

R(0)=var(Xt)=E(Xtμ)=σ2 (1.2)

R(k)=cov(Xt,Xt+k)=E[(Xtμ)(Xt+kμ)]={σ2,k=00,otherwise (1.3)

ρ(k)=corr(Xt,Xt+k)=R(k)R(0)={1,k=00,otherwise (1.4)

ϕkk=corr(Xt,Xt+k/Xt+1,Xt+2,,Xt+k1)=0k (1.5)

where R(k) is the autocovariance function at lag k, rk is the autocorrelation function at lag k and ϕkk is the partial autocorrelation function at lag k.

In other words, a stochastic process Xt,tZ is called a linear Gaussian white noise if Xt,tZ is a sequence of independent and identically distributed (iid) random variables with finite mean and finite variance. Under the assumption that the sample X1,X2,,Xn is an iid sequence, we compute the sample autocorrelations as

ˆρX(k)=nt=1(XtˉX)(Xt+kˉX)nt=1(XtˉX)2 (1.6)

where

ˉX=1nni=1Xt (1.7)

The iid hypothesis is always tested with the Ljung and Box [8] statistic

QLB(m)=n(n+2)mk=1([ˆρX(k)]2nk) (1.8)

where QLB(m) is asymptotically a chi-squared random variable with m degree of freedom.

Several values of m are often used and simulation studies suggest that the choice of mln(n) provides better power performance [9] .

If the data are iid, the squared data X21,X22,,X2n are also iid [10] . Another portmanteau test formulated by Mcleod and Li [10] is based on the same statistic used for the Ljung and Box [8]

QML(m)=n(n+2)mk=1([ˆρX2(k)]2nk) (1.9)

where the sample autocorrelations of the data are replaced by the sample autocorrelations of the squared data, ˆρX2(k) .

As noted by Iwueze et al. [11] , a stochastic process Xt,tZ may have the covariance structure (1.1) through (1.5) even when it is not the linear Gaussian white noise process. Iwueze et al. [11] provided additional properties of the linear Gaussian white noise process for proper identification and characterization from other processes with similar covariance structure (1.1) through (1.5).

Let Yt=Xdt,d=1,2,3, where Xt,tZ , be the linear Gaussian white noise process, the mean [E(Yt)=E(Xdt)] , the variance [var(Yt)=var(Xdt)] , autocovariances [Ry(k)=cov(YtYtk)=cov(XdtXdtk)] were obtained to be [11]

E(Yt)=E(Xdt)={σ2m(2m1)!!,d=2m,m=1,2,0,d=2m+1,m=0,1,2, (1.10)

Var(Yt)=Var(Xdt)={σ4m[2mk=1(2k1)(mk=1(2k1))2],d=2mσ2(2m+1)2m+1k=1(2k1),d=2m+1 (1.11)

RY(k)=RXdt(l)={σ4m[2mk=1(2k1)(mk=1(2k1))2],d=2m,l=0σ2(2m+1)2m+1k=1(2k1),d=2m+1,l=00,l0 (1.12)

where

(2m1)!!=mk=1(2k1) (1.13)

It is clear from (1.12) that when Xt,tZ are iid, the powers Yt=Xdt,d=1,2,3, of Xt,tZ are also iid. Iwueze et al. [11] also showed the probability density function (pdf) of Yt=X2t to be the pdf of a gamma distribution with parameters

α=12,β=2σ2 . That is, Yt=X2t~G(α,β),α=12,β=2σ2 .

when Xt~N(0,σ2) and [11] concluded that all powers of a linear Gaussian white noise process are iid but not normally distributed.

Using the coefficient of symmetry and kurtosis, Iwueze et al. [11] confirmed the non-normality of Yt=Xdt,d=2,3, . Table 1 gives the mean, variance, the coefficient of symmetry ( β1 ) and kurtosis ( β2 ) defined as follows

β1=μ3(d)(μ2(d))3/2 (1.14)

β2=μ4(d)(μ2(d))2 (1.15)

where

μ2(d)=E[(XdtE(Xdt))2]=var(Xdt) (1.16)

d

Y t

E ( Y t )

( μ y )

μ 2 ( d )

( var ( Y t ) )

μ 3 ( d )

μ 4 ( d )

β 1

β 2

1

X t

0

σ 2

0

3 σ 4

0

3.000

2

X t 2

σ 2

2 σ 4

8 σ 6

60 σ 8

2.828

15.000

3

X t 3

0

15 σ 6

0

10395 σ 12

0

46.200

4

X t 4

3 σ 4

96 σ 8

9504 σ 12

1907712 σ 16

10.104

207.00

5

X t 5

0

945 σ 10

0

654729075 σ 20

0

733.159

6

X t 6

15 σ 6

10170 σ 12

33998400 σ 18

3.142 × 10 11 σ 24

33.150

3037.836

  翻译:

Table 1. Mean, Variance, Coefficient of symmetry ( β1 ) and kurtosis ( β2 ) for Yt=Xdt , d=1,2,3,,6 ,when Xt~N(0,σ2) .

Source: Iwueze et al. (2017).

μ3(d)=E[(XdtE(Xdt))3] (1.17)

μ4(d)=E[(XdtE(Xdt))4] (1.18)

Using the standard deviations when σ2=1 and the kurtosis of Yt=Xdt,d=1,2,3, , Iwueze et al. [11] determined the optimal value of d to be three ( d=3 ). Hence, for effective comparison of the linear Gaussian white noise process with any stochastic process with similar covariance structure, Yt=Xdt,d=1,2,3 must be used.

The most commonly used white noise process is the linear Gaussian white noise process. The process is one of the major outcomes of any estimation procedure which is used in checking the adequacy of fitted models. The linear Gaussian white noise process also plays significant role as a basic building block in the construction of linear and non-linear time series models. However, the major problem is that there are many non-linear processes that exhibit the same covariance structure (Equation (1.1) through Equation (1.5)) as the linear Gaussian white noise process. One of such non-linear models is the bilinear models.

The study of bilinear models was introduced by Granger and Andersen [12] and Subba Rao [13] . Granger and Andersen [14] established that all series generated by the simple bilinear model

Xt=βXtketj+et,k>j (1.19)

appear to be second order white noise where β is a constant and et,tZ is an independent identically distributed normal random variable with E(et)=0 , E(e2t)=σ2< . Guegan [15] studied the existence problem of a simple bilinear process Xt,tZ satisfying

Xt=βXt2et1+et (1.20)

Martins [16] obtained the autocorrelation function of the process X2t,tZ for the simple bilinear model defined by (1.19) when et,tZ is iid with a Gaussian distribution. Again, Martins [16] studied the third order moment structure of (1.19) with non-independent shocks. Recently, properties of the simple bilinear model (1.19) were addressed by Malinski and Bielinska [17] , Malinski and Figwer [18] and Malinski [19] . Iwueze [20] studied the more general bilinear white noise model

Xt=(mj=1βjXtqj)etq+et (1.21)

where et,tZ is as defined in (1.19). Iwueze [20] was able to show the following.

1) The series Xt,tZ satisfying (1.21) is strictly stationary, ergodic and unique.

2) The series Xt,tZ satisfying (1.21) is invertible.

3) The series Xt,tZ satisfying (1.21) has the same covariance structure as the linear Gaussian white noise processes.

4) Obtained the covariance structure of (1.21) to be

μ=E(Xt)=0 (1.22)

R(k)={σ21mj=1σ2β2j,k=00,otherwise (1.23)

5) The series satisfying (1.21) is invertible if

2mj=1β2jσ2<1 (1.24)

For the simple bilinear model (1.19), it follows that

R(k)={11σ2β2,σ2β2<10,otherwise (1.25)

and the invertibility condition is

σ2β2<12 (1.26)

It is worthy to note that the stationarity condition

σ2β2<1 (1.27)

is structure (k, n) independent [19] for model (1.19) and our study in this paper will concentrate on model (1.20). The purpose of this paper is to meet the following goals for the simple bilinear model satisfying (1.20).

1) Determine Var(Xdt),d=2,3 for the simple bilinear model (1.20).

2) Determine the covariance structure of Xdt,d=2,3 , when Xt,tZ satisfies (1.20).

3) Determine for what values of β the simple bilinear white noise process will be identified as a Linear Gaussian white noise process.

4) Determine for what values of β the simple bilinear model will be normally distributed.

This paper is further divided into four sections in order to establish and achieve these goals. Section 2 discusses the covariance structure of Yt=Xdt,d=1,2,3 when Xt=βXt2et1+et , et~iidN(0,σ2) , Section 3 presents the methodology, Section 4 is the results and discussion while, Section five is the conclusion.

2. Covariance Structure of Yt=Xdt,d=1,2,3 , When Xt=βXt2et1+et , et~iidN(0,σ2)

Theorem 2.1.

Let et,tZ be the linear Gaussian white noise process with E(et)=0 and E(e2t)=σ2< . Suppose there exists a stationary and invertible process Xt,tZ satisfying Xt=βXt2et1+et for every tZ for some constant β , then Yt=X2t has the following properties:

E(Yt)=μY=σ21σ2β2;σ2β2<1 (2.1)

RY(k)=cov(Yt,Ytk)={2σ4(1σ2β2)2(13σ4β4),σ2β2<13,k=02σ6β2(1σ2β2)2,σ2β2<1,k=1σ2β2RY(k2),k=2,3, (2.2)

ρY(k)=RY(k)RY(0)={1,k=0σ2β2(13σ4β4),k=1σ2β2ρY(k2),k=2,3, (2.3)

Yt=X2t,tZ has the same covariance structure as the linear ARMA(2, 1) process (2.4)

Xt=λ+ϕ1Xt1+ϕ2Xt2+θ1at1+at,ϕ1=0 (2.4)

where at is the sequence of independent and identically distributed random variable with E(at)=0 and Var(at)=σ21< .

Proof:

Let

Yt=X2t=(βXt2et1+et)2=β2X2t2e2t1+e2t+2βXt2et1et

E(Yt)=E(X2t)=β2E(X2t2)E(e2t1)+E(e2t)+2βE(Xt2)E(et1)E(t)

E(Yt)=E(X2t)=β2E(X2t)E(e2t)+E(e2t)=σ2β2E(X2t)+σ2

(1σ2β2)E(X2t)=σ2

μY=E(X2t)=σ21σ2β2;σ2β2<1 (2.5)

Var(Yt)=Var(X2t)=E(X4t)[E(X2t)]2

X4t=β4X4t2e4t1+4β3X3t2e3t1et+6β2X2t2e2t1e2t+4βXt2et1e3t+e4t

E(X4t)=3σ4β4E(X4t)+6σ4β2E(X2t)+3σ4

(13σ4β4)E(X4t)=6σ6β21σ2β2+3σ4

E(X4t)=3σ4(1+σ2β2)(1σ2β2)(13σ4β4),σ4β4<13 (2.6)

Now,

Var(Yt)=Var(X2t)=E(X4t)[E(X2t)]2=3σ4(1+σ2β2)(1σ2β2)(13σ4β4)(σ21σ2β2)2=3σ4(1+σ2β2)(1σ2β2)σ4(13σ4β4)(1σ2β2)2(13σ4β4) (2.7)

Hence,

RY(0)=Var(Yt)=Var(X2t)=2σ4(1σ2β2)2(13σ4β4),σ2β2<13 (2.8)

RY(k)=E[YtYtl]μ2y=E[X2tX2tl]μ2x,k=0,1,2,

YtYt1=X2tX2t1=β2X2t2X2t1e2t1+2βXt2X2t1et1et+X2t1e2t

E[YtYt1]=β2E[X2t2X2t1e2t1]+σ2E(X2t1)

E[YtYt1]=β2E[X2t1X2te2t]+σ2E(X2t)

X2t1X2te2t=X2t1(β2X2t2e2t1+2βXt2et1et+et)e2t

X2t1X2te2t=β2X2t2X2t1e2t1e2t+2βXt2X2t1et1e3t+X2t1e4t

By the assumption of stationarity,

E[X2t1X2te2t]=σ2β2E[X2t1X2te2t]+3σ4E(X2t)

(1σ2β2)E[X2t1X2te2t]=3σ4(σ21σ2β2)

E[X2t1X2te2t]=3σ6(1σ2β2)2,σ2β2<1 (2.9)

E[YtYt1]=β2[3σ6(1σ2β2)2]+σ2(σ21σ2β2)=σ4(1+2σ2β2)(1σ2β2)2 (2.10)

Hence,

Ry(1)=E(YtYt1)=E2(Yt)=σ4(1+2σ2β2)(1σ2β2)2(σ21σ2β2)2=2σ6β2(1σ2β2)2 (2.11)

YtYt2=X2tX2t2=(β2X2t2e2t1+2βXt2et1et+e2t)X2t2

YtYt2=β2X4t2e2t1+2βX3t2et1et+X2t2e2t

E[YtYt2]=σ2β2E(X4t2)+σ2E(X2t2)

E[YtYt2]=σ2β2E(Y2t2)+σ2E(Yt)

E[YtYt2]=σ2β2E(Y2t)+σ2μy

Ry(2)+μ2y=σ2β2[Ry(0)+μ2y]+σ2μy (2.12)

Ry(2)=σ2β2Ry(0)+σ2β2μ2y+σ2μyμ2y=σ2β2Ry(0)+σ2μyμ2y(1σ2β2)

Note that

μY=E(Yt)=E(X2t)=σ21σ2β2

(1σ2β2)μY=σ2

1σ2β2=σ2μY (2.13)

Hence

RY(2)=σ2β2Ry(0)+σ2μyμ2y(σ2μy)=σ2β2Ry(0)+σ2μyσ2μy=σ2β2Ry(0) (2.14)

We have shown that

σ2β2μ2y+σ2μyμ2y=0 (2.15)

Similarly;

YtYt3=X2tX2t3=(β2X2t2e2t1+2βXt2et1et+e2t)X2t3

YtYt3=β2X2t3X2t2e2t1+2βX2t3Xt2et1et+X2t3e2t

E[YtYt3]=σ2β2E[X2t2X2t1]+σ2E(X2t)=σ2β2E[YtYt1]+σ2E(Yt)

Ry(3)+μ2y=σ2β2[Ry(1)+μ2y]+μ2y=σ2β2Ry(1)+σ2β2μ2y+σ2μyμ2y=σ2β2Ry(1) (2.16)

Generally;

RY(k)=σ2β2RY(k2),k=2,3, (2.17)

Hence,

RY(k)={2σ4(1σ2β2)2(13σ4β4),σ2β2<13,k=02σ6β2(1σ2β2)2,σ2β2<1,k=1σ2β2RY(k2),k=2,3, (2.18)

and

ρY(k)={1,k=0σ2β2(13σ4β4),k=1σ2β2ρY(k2),k=2,3, (2.19)

With this result, it is clear that when Xt,tZ is defined by (1.20), Yt=X2t has the same covariance structure as the linear ARMA(2, 1) process. Its linear equivalence is

Yt=λ+ϕ1Xt1+ϕ2Yt2+θ1at1+at,ϕ1=0 (2.20)

where at is the purely random process with E(at)=0 and Var(at)=σ21< . Table 2 compares Yt=X2t with its linear ARMA(2, 1) equivalence.

Theorem 2.2.:

Let et,tZ be the linear Gaussian white noise process with E(et)=0 and E(e2t)=σ2< . Suppose there exists a stationary and invertible process Xt,tZ satisfying Xt=βXt2et1+et for every tZ and some constant β , then the mean and variance of Yt=X3t,tZ are

E(Yt)=μY=0 (2.21)

Properties

Process

Bilinear

Linear ARMA(2, 1)

Structure

X t = β X t 2 e t 1 + e t , e t ~ N ( 0 , σ 2 ) ,

Y t = X t 2 ~ ARMA ( 2 , 1 ) with ϕ 1 = 0

Y t = λ + ϕ 2 Y t 2 + θ 1 a t 1 + a t , E ( a t ) = 0 , V a r ( a t ) = σ 1 2

Mean

μ Y = E ( Y t ) = E ( X t 2 ) = σ 2 1 σ 2 β 2 ; σ 2 β 2 < 1

μ Y = E ( Y t ) = λ 1 ϕ 2 , [ λ = ( 1 ϕ 2 ) μ X ]

Autocovariance

R Y ( k ) = { 2 σ 4 ( 1 σ 2 β 2 ) 2 ( 1 3 σ 4 β 4 ) , σ 2 β 2 < 1 3 , k = 0 2 σ 6 β 2 ( 1 σ 2 β 2 ) 2 , σ 2 β 2 < 1 , k = 1 σ 2 β 2 R Y ( k 2 ) , k = 2 , 3 ,

R Y ( k ) = { σ 1 2 ( 1 + θ 1 2 ) 1 ϕ 2 2 , | ϕ 2 | < 1 , k = 0 σ 1 2 θ 1 1 ϕ 2 , ϕ 2 1 , k = 1 ϕ 2 R Y ( k 2 ) , k = 2 , 3 ,

Autocorrelation

ρ Y ( k ) = { 1 , k = 0 σ 2 β 2 ( 1 3 σ 4 β 4 ) , k = 1 σ 2 β 2 ρ Y ( k 2 ) , k = 2 , 3 ,

ρ Y ( k ) = { 1 , k = 0 θ 1 ( 1 + ϕ 2 ) 1 + θ 1 2 , k = 1 ϕ 2 ρ Y ( k 2 ) , k = 2 , 3 ,

  翻译:

Table 2. Covariance analysis of Yt=X2t when Xt=βXt2et1+et , et~N(0,σ2) and its linear ARMA(2, 1) equivalence.

RY(k)={15σ6(1+2σ2β2+6σ4β4+3σ6β6)(1σ2β2)(13σ4β4)(115σ6β6),σ2β2<1315,k=00,k0 (2.22)

ρk(k)={1,k=00,k0 (2.23)

The covariance structure of Yt=X3t,tZ is that of the linear white noise process.

Proof:

Let Yt=X3t=(βXt2et1+et)3=β3X3t2e3t1+3β2X2t2e2t1et+3βXt2et1e2t+e3t (2.24)

E(Yt)=E(X3t)=μy=β3E(X3t2e3t1)+3σ2β2E(Xt2et1)=β3E(X3t1e3t)+3σ2β2E(Xt1et)=0 (2.25)

Y2t=X6t=(βXt2et1+et)6=β6X6t2e6t1+6β5X5t2e5t1et+15β4X4t2e4t1e2t+20β3X3t2e3t1e3t+15β2X2t2e2t1e4t+6βXt2et1e5t+e6t (2.26)

E(Y2t)=β6E(X6t2e6t1)+6β5E(X5t2e5t1et)+15β4E(X4t2e4t1e2t)+20β3E(X3t2e3t1e3t)+15β2E(X2t2e2t1e4t)+6βE(Xt2et1e5t)+E(e6t)=β6E(X6t2e6t1)+15σ2β4E(X4t2e4t1)+45σ4β2E(X2t2e2t1)+15σ6=15σ6β6E(X6t)+45σ6β4E(X4t)+45σ6β2E(X2t)+15σ6=15σ6β6E(Y2t)+45σ6β4[3σ4(1+σ2β2)(1σ2β2)(13σ4β4)]+45σ6β2(σ21σ2β2)+15σ6

(115σ6β6)E(Y2t)=45σ6β4[3σ4(1+σ2β2)(1σ2β2)(13σ4β4)]+45σ6β2(σ21σ2β2)+15σ6=1(1σ2β2)(13σ4β4)[45σ6β4[3σ4(1+σ2β2)]+45σ6β2[σ2(13σ4β4)]+15σ6(1σ2β2)(13σ4β4)]

=1(1σ2β2)(13σ4β4)[135σ10β4+135σ12β6+45σ8β2135σ12β6+15σ645σ10β415σ8β2+45σ12β6]=1(1σ2β2)(13σ4β4)[90σ10β4+30σ8β2+15σ6+45σ12β6]=15σ6(1+2σ2β2+6σ4β4+3σ6β6)(1σ2β2)(13σ4β4),σ2β2<1315 (2.27)

E(Y2t)=Ry(0)+μ2y (2.28)

Var(Yt)=Var(X3t)=Ry(0)=E(Y2t)μ2y=15σ6(1+2σ2β2+6σ4β4+3σ6β6)(1σ2β2)(13σ4β4)(115σ6β6),σ2β2<1315 (2.29)

Some Results

E ( X t 1 X t e t ) = σ 2 E ( X t ) = 0

Proof:

X t 1 X t e t = X t 1 [ β X t 2 e t 1 + e t ] e t = β X t 2 X t 1 e t 1 e t + X t 1 e t 2

E ( X t 1 X t e t ) = σ 2 E ( X t 1 ) = σ 2 E ( X t ) = 0

E ( X t 1 X t 2 e t ) = 2 σ 2 β E ( X t 1 X t e t ) = 0

Proof:

X t 1 X t 2 e t = X t 1 [ β 2 X t 2 2 e t 1 2 + 2 β X t 2 e t 1 e t + e t 2 ] e t = β 2 X t 2 2 X t 1 e t 1 2 e t + 2 β X t 2 X t 1 e t 1 e t 2 + e t 3

E ( X t 1 X t 2 e t ) = 2 β σ 2 E ( X t 2 X t 1 e t 1 ) = 2 β σ 2 E ( X t 1 X t e t ) = 0

E ( X t 1 2 X t e t 2 ) = σ 2 β E ( X t 1 X t 2 e t ) = 0

Proof:

X t 1 2 X t e t 2 = X t 1 2 [ β X t 2 e t 1 + e t ] e t 2 = β X t 2 X t 1 2 e t 1 + X t 1 2 e t 3

E ( X t 1 2 X t e t 2 ) = σ 2 β E ( X t 2 X t 1 2 e t 1 ) = σ 2 β E ( X t 1 X t 2 e t ) = 0

E ( X t 1 X t 3 e t ) = 3 σ 2 β 2 E ( X t 1 2 X t e t 2 ) = 0

Proof:

X t 1 X t 3 e t = X t 1 [ β 3 X t 2 3 e t 1 3 + 3 β 2 X t 2 2 e t 1 2 e t + 3 β X t 2 e t 1 e t 2 + e t 3 ] e t = β 3 X t 2 3 X t 1 e t 1 3 e t + 3 β 2 X t 2 2 X t 1 e t 1 2 e t 2 + 3 β X t 2 X t 1 e t 1 e t 3 + X t 1 e t 4

E ( X t 1 X t 3 e t ) = 3 σ 2 β 2 E ( X t 2 2 X t 1 e t 1 2 ) = 3 σ 2 β 2 E ( X t 1 2 X t e t 2 ) = 0

ÞNow

Y t Y t 1 = X t 3 X t 1 3 = [ β 3 X t 2 3 e t 1 3 + 3 β 2 X t 2 2 e t 1 2 e t + 3 β X t 2 e t 1 e t 2 + e t 3 ] X t 1 3 = β 3 X t 2 3 X t 1 3 e t 1 3 + 3 β 2 X t 2 2 X t 1 3 e t 1 2 e t + 3 β X t 2 X t 1 3 e t 1 e t 2 + X t 1 3 e t 3

E ( Y t Y t 1 ) = β 3 E ( X t 2 3 X t 1 3 e t 1 3 ) + 3 σ 2 β E ( X t 2 X t 1 3 e t 1 ) = β 3 E ( X t 1 3 X t 3 e t 3 ) + 3 σ 2 β E ( X t 1 X t 3 e t ) = β 3 E ( X t 1 3 X t 3 e t 3 )

X t 1 3 X t 3 e t 3 = X t 1 3 [ β 3 X t 2 3 e t 1 3 + 3 β 2 X t 2 2 e t 1 2 e t + 3 β X t 2 e t 1 e t 2 + e t 3 ] e t 3 = β 3 X t 2 3 X t 1 3 e t 1 3 e t 3 + 3 β 2 X t 2 2 X t 1 3 e t 1 2 e t 4 + 3 β X t 2 X t 1 3 e t 1 e t 5 + X t 1 3 e t 6

E ( X t 1 3 X t 3 e t 3 ) = 3 β 2 ( 3 σ 4 ) E ( X t 2 2 X t 1 3 e t 1 2 ) = 9 σ 4 β 2 E ( X t 2 2 X t 1 3 e t 1 2 ) = 9 σ 4 β 2 E ( X t 1 2 X t 3 e t 2 )

Hence,

E ( Y t Y t 1 ) = β 3 [ 9 σ 4 β 2 E ( X t 1 2 X t 3 e t 2 ) ] = 9 σ 4 β 5 E ( X t 1 2 X t 3 e t 2 )

Now

X t 1 2 X t 3 e t 2 = X t 1 2 [ β 3 X t 2 3 e t 1 3 + 3 β 2 X t 2 2 e t 1 2 e t + 3 β X t 2 e t 1 e t 2 + e t 3 ] e t 2 = β 3 X t 2 3 X t 1 2 e t 1 3 e t 2 + 3 β 2 X t 2 2 X t 1 2 e t 1 2 e t 3 + 3 β X t 2 X t 1 2 e t 1 e t 4 + X t 1 2 e t 5

E ( X t 1 2 X t 3 e t 2 ) = σ 2 β 3 E ( X t 2 3 X t 1 2 e t 1 3 ) + 3 β ( 3 σ 4 ) E ( X t 2 X t 1 2 e t 1 ) = σ 2 β 3 E ( X t 1 3 X t 2 e t 3 ) + 9 σ 4 β E ( X t 1 X t 2 e t ) = σ 2 β 3 E ( X t 1 3 X t 2 e t 3 )

But,

E ( Y t Y t 1 ) = 9 σ 4 β 5 E ( X t 1 2 X t 3 e t 2 ) = 9 σ 4 β 5 ( σ 2 β 3 E ( X t 1 3 X t 2 e t 3 ) ) = 9 σ 6 β 8 E ( X t 1 3 X t 2 e t 3 )

Now,

X t 1 3 X t 2 e t 3 = X t 1 3 [ β 2 X t 2 2 e t 1 2 + 2 β X t 2 e t 1 e t + e t 2 ] e t 3 = β 2 X t 2 2 X t 1 3 e t 1 2 e t 3 + 2 β X t 2 X t 1 3 e t 1 e t 4 + X t 1 3 e t 5

E ( X t 1 3 X t 2 e t 3 ) = 2 β ( 3 σ 4 ) E ( X t 2 X t 1 3 e t 1 ) = 6 σ 4 β E ( X t 1 X t 3 e t ) = 0

Hence,

E ( Y t Y t 1 ) = 9 σ 6 β 8 [ 6 σ 4 β E ( X t 1 X t 3 e t ) ] = 54 σ 10 β 9 E ( X t 1 X t 3 e t ) = 0

R Y ( 1 ) = 0 , when Y = X t 3 .

Y t Y t 2 = X t 3 X t 2 3 = [ β 3 X t 2 3 e t 1 3 + 3 β 2 X t 2 2 e t 1 2 e t + 3 β X t 2 e t 1 e t 2 + e t 3 ] X t 2 3 = β 3 X t 2 6 e t 1 3 + 3 β 2 X t 2 5 e t 1 2 e t + 3 β X t 2 4 e t 1 e t 2 + X t 2 3 e t 3

E ( Y t Y t 2 ) = 0

R Y ( 2 ) = 0 , when Y = X t 3 .

Generally, R Y ( k ) = 0 k 0 , when Y = X t 3 .

Therefore, given X t = β X t 2 e t 1 + e t , e t ~ N ( 0 , σ 2 ) and Y t = X t 3 , the following are true E ( Y t ) = E ( X t 3 ) = 0 .

R Y ( k ) = { 15 σ 6 ( 1 + 2 σ 2 β 2 + 6 σ 4 β 4 + 3 σ 6 β 6 ) ( 1 σ 2 β 2 ) ( 1 3 σ 4 β 4 ) ( 1 15 σ 6 β 6 ) , σ 2 β 2 < 1 15 3 , k = 0 0 , k 0

ρ k ( k ) = { 1 , k = 0 0 , k 0

The covariance structure of Y t = X t 3 , t Z identifies the process as linear white noise.

3. Methodology

3.1. Normality Checking

The Jarque-Bera (JB) test [21] [22] [23] will be used to determine for which values of β a simple bilinear model (1.20) is normally distributed or not. The JB test statistic is

JB = n ( γ ^ 1 2 6 + ( γ ^ 2 3 ) 2 24 ) (3.1)

where

γ ^ 1 = 1 n t = 1 n ( X t X ¯ ) 3 ( 1 n t = 1 n ( X t X ¯ ) 2 ) 3 / 2 (3.2)

γ ^ 2 = 1 n t = 1 n ( X t X ¯ ) 4 ( 1 n t = 1 n ( X t X ¯ ) 2 ) 2 (3.3)

n is the sample size while, γ ^ 1 and γ ^ 2 are the sample skewness and kurtosis coefficients. The asymptotic null distribution of JB is χ 2 with 2 degrees of freedom.

3.2. White Noise Test

The modified Ljung-Box test statistic [11] given by

Q * ( m ) = n ( n + 2 ) k = 1 m ( [ ρ ^ X d ( k ) ] 2 n k ) (3.4)

is used to test the iid hypothesis for X t d , d = 1 , 2 , 3 for the simple bilinear model (1.20). It is important to note from Theorem 2.1 that X t 2 has ARMA(2, 1) structure while from Theorem 2.2, X t 3 is iid. This test will look for β values where both X t 2 and X t 3 are jointly iid. That will help determine the values of β for which the simple bilinear model (1.20) is not distinguishable from the linear Gaussian white noise process (LGWNP). Then, the hypothesis of iid data is rejected at level α if the observed Q * ( m ) is larger than the 1 α 2 quartile of the χ 2 ( m ) distribution, where m ln ( n ) [9] .

3.3. Use of Chi-Square Test for Comparison of the Simple Bilinear White Noise Process and the Linear Gaussian White Noise Process

From Theorem 2.3, the third power of the simple bilinear process is iid. A test is needed to confirm that the simple bilinear process (1.20) is not a linear Gaussian white noise process (LGWNP). For the LGWNP X t , t T ; E ( X t ) = μ , var ( X t ) = σ 2 < and var ( X t 3 ) = 15 σ 6 . To show that the simple bilinear process (1.20) is not LGWNP, we need to test the hypothesis;

H 0 : σ X t 3 2 = 15 σ X t 6 (3.5)

against the alternative hypothesis

H 0 : σ X t 3 2 15 σ X t 6 (3.6)

The chi-square test [24] [25] can be used to perform the test. The chi-square test statistic is

χ c a l 2 = ( n 1 ) S X t 3 2 15 σ X t 6 (3.7)

where S X t 3 2 is the sample variance of X t 3 ; X t , t Z that follows (1.20), σ X t 2 is an estimate of the true variance of the simple bilinear process (1.20) and n is the number of observations of the series. The null hypothesis is rejected at level α if the observed value of χ c a l 2 is larger than 1 α 2 quartile of the chi-square distribution with n 1 .degree of freedom. It should be noted that this test works well when the underlying original population X t , t Z is normally distributed.

4. Results and Discussion

One thousand random digits e t , t Z that met the condition e t ~ N ( 0 , 1 ) were simulated using Minitab 16 series software. Only one random digit, shown in Appendix I, was used for demonstration in the study because of want of space. The estimates of the descriptive statistics (mean, variance, skewness ( γ 1 ) and kurtosis ( γ 2 )) and other tests (Jarque Bera (JB) test, modified Ljung Box test (Q*) and chi-square calculated test statistic) for the powers e t d , d = 1 , 2 , 3 of the random digit are shown in Table 3. The results obtained using the JB, Q* and the chi-square test indicated e t , t Z as a LGWNP at 5% level of significance.

The LGWNP were used to simulate the SBWNP X t = B X t 2 e t 1 + e t , e t ~ N ( 0 , 1 ) for 0.60 β 0.60 satisfying the existence of E ( X t 3 ) using Fortran 77 program. The estimates of the descriptive statistic and that for the test statistic (JB, Q* and the chi-square calculated test statistic) are shown in Table 4. The values of the JB statistic show that the SBWNP are normally distributed for 0.56 β 0.60 . Similarly, the values of Q* and the chi-square calculated test statistic ( H 0 ) show that the SBWNP is iid and can be identified as a LGWNP for some β values. The values of β where the SBWNP will be identified as an LGWNP are summarized in Table 5.

5. Conclusion

We have been able to establish the covariance structure for X t d , d = 1 , 2 , 3 ; t Z

Statistic

Mean

Median

Estimated Value

Skewness

Kurtosis

JB

value

Q*

Estimate of Test Statistic

S 2

γ 1

γ 2

( n 1 ) S X t 2 2 2 σ ^ 0 4

( n 1 ) S X t 3 2 15 σ ^ 0 6

X t

0.0000

0.1261

1.0000

−0.28

−0.04

1.87

3.36

-

-

X t 2

0.9931

0.4763

1.9074

1.90

2.79

133.19

0.04

136.38

-

X t 3

−0.2728

0.0020

11.5236

−0.61

6.47

259.67

−0.14

-

109.86

  翻译:

Table 3. Descriptive Statistics and estimate of the test statistic for rejecting the null hypothesis of equality of the variance of higher moment for the simulated series, X t = e t , e t ~ N ( 0 , 1 ) , as linear Gaussian white noise process.

β

Statistic

Estimated Values

Estimate of Test Statistic

Mean

Variance

γ 1

γ 2

JB value

Q*

H 0

−0.60

X t

0.0418

1.9037

0.27

1.20

10.28

8.44

-

X t 2

1.8923

11.3331

3.09

11.85

1072.25

71.39

-

X t 3

0.9233

186.5203

3.78

26.73

4628.20

22.66

257.74

−0.59

X t

0.0410

1.8610

0.24

1.11

8.78

8.16

.

X t 2

1.8490

10.5110

2.99

11.09

952.49

70.34

-

X t 3

0.8100

164.3700

3.61

25.83

4315.90

20.32

243.12

−0.58

X t

0.0390

1.8200

0.21

1.02

7.30

7.89

.

X t 2

1.8090

9.7720

2.89

10.39

848.16

69.04

-

X t 3

0.7100

145.5500

3.44

24.98

4028.01

18.02

230.17

−0.57

X t

0.0380

1.7800

0.18

0.94

6.08

7.63

.

X t 2

1.7700

9.1080

2.80

9.75

758.53

67.49

-

X t 3

0.6220

129.4920

3.29

24.13

3753.32

15.84

218.89

−0.56

X t

0.0370

1.7430

0.15

0.87

5.12

7.39

.

X t 2

1.7320

8.5110

2.72

9.16

680.73

65.73

-

X t 3

0.5390

115.7480

3.14

23.25

3479.84

13.84

208.38

−0.55

X t

0.0360

1.7080

0.13

0.80

4.29

7.15

.

X t 2

1.6970

7.9730

2.64

8.61

612.26

63.76

-

X t 3

0.4630

103.9380

2.99

22.32

3203.09

12.04

198.86

−0.54

X t

0.0346

1.6739

0.10

0.74

3.58

6.93

-

X t 2

1.6634

7.4872

2.57

8.09

550.71

61.63

-

X t 3

0.3948

93.7500

2.84

21.33

2921.69

10.48

190.56

−0.53

X t

0.0334

1.6416

0.08

0.69

3.00

6.73

-

X t 2

1.6313

7.0486

2.50

7.59

495.95

59.36

-

X t 3

0.3325

84.9253

2.69

20.27

2637.97

9.18

183.01

−0.52

X t

0.0322

1.6108

0.06

0.64

2.52

6.54

-

X t 2

1.6006

6.6518

2.44

7.12

446.71

56.99

-

X t 3

0.2759

77.2508

2.54

19.16

2356.47

8.12

176.21

−0.51

X t

0.0310

1.5814

0.04

0.59

2.12

6.36

-

X t 2

1.5714

6.2921

2.38

6.66

402.32

54.54

-

X t 3

0.2246

70.5498

2.39

18.01

2082.80

7.31

170.07

  翻译:

Table 4. Descriptive statistics and estimate of the test statistic for simulated bilinear series X t = β X t 2 e t 1 + e t , e t ~ N ( 0 , 1 ) and 0.60 β 0.60 .

α % level

Values of β

Q*

H 0

5

[ 0.23 , 0.44 ]

[ 0.18 , 0.22 ]

10

[ 0.19 , 0.37 ]

[ 0.29 , 0.38 ]

  翻译:

Table 5. Values of β for comparison of SBWNP as a LGWNP at 0.05 and 0.10 α levels.

satisfying (1.20). We have also determined the values of β for which the simple bilinear model (1.20) is normally distributed and in which the process can be determined as a LGWNP or not. We recommend that for proper comparison of SBWNP with LGWNP, the SBWNP should be considered for normality, white noise test and test of equality of variance of its third moment being equivalent to the theoretical values of the LGWNP.

Appendix I

Simulated Random Digits; e t , e t ~ N ( 0 , 1 ) (Read Across).

−0.57532

−0.17491

0.35244

0.30620

−0.76520

−0.10381

−0.78604

0.19891

0.48466

−1.04050

0.25694

2.13936

0.81740

−1.61037

2.38415

0.74182

−1.83436

−0.97443

0.06649

−0.80814

−2.14835

−1.39147

−1.19600

0.16246

1.10204

−0.75625

1.43986

0.41147

0.34040

−0.27339

−0.66471

0.72426

−0.24697

−0.73065

1.22347

1.89188

−0.78388

0.99457

−0.94385

1.99912

0.00884

0.10762

−2.23041

−0.20387

1.20197

−0.12003

1.83635

−0.06882

−2.38069

0.01037

0.55983

−1.86577

0.75661

−0.83977

−0.06520

−0.25303

0.57397

−0.10694

−1.87199

−0.61338

−0.96019

−0.69799

0.41226

−0.13727

0.73620

−0.25448

0.27995

0.82692

1.07422

0.72309

0.44146

0.76731

0.72838

0.39809

0.18794

0.06831

0.45853

−0.79068

−1.97602

−1.55625

0.98349

2.09313

−1.26609

0.50341

−0.98639

0.78335

0.56394

−0.00389

−0.60469

0.68956

0.09199

−0.84437

0.28016

−0.36120

0.16969

−0.32149

−1.97702

−0.98212

−1.26901

0.93133

0.63846

−0.83151

0.68592

0.18103

−0.69071

0.35337

0.67619

0.82779

1.25023

0.50671

1.39091

−0.27367

−0.09697

1.01271

1.21921

0.67856

0.37606

1.16306

−0.11180

−2.39334

1.13787

−0.46900

−1.07178

0.09855

1.96154

−0.45406

−1.57186

0.93940

−0.00755

0.32726

0.57558

0.48859

0.45601

0.14352

−2.13818

0.23375

−1.82588

0.13979

−0.25057

1.17289

0.12739

0.35428

0.12472

−0.92299

  翻译:

Conflicts of Interest

The authors declare no conflicts of interest.

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