No CrossRef data available.
Published online by Cambridge University Press: 01 August 2004
In this paper we derive the necessary and sufficient conditions for the t-ratio to be Student's t distributed. In particular, it is demonstrated for a special case that under conditions of nonnormality characterized by elliptical symmetry, the t-ratio remains Student's t distributed provided that the random vector forming the t-ratio has a diagonal covariance structure. Our results also show that the findings of Magnus (2002, in A. Ullah, A.T.K. Wan, & A. Chaturvedi (eds.), Handbook of Applied Econometrics and Statistical Inference, 277–285) on the sensitivity of the t-ratio remain invariant in the elliptically symmetric distribution setting. Extension to the linear model is considered. Exact results giving finite sample justification for the t-statistic under nonnormal error terms are derived. Furthermore, the distribution of the F-ratio assuming elliptical errors is examined. Our results reject the argument by Zaman (1996, Statistical Foundations for Econometric Techniques) that nonnormality of disturbances has in general no effect on the F-statistic.The authors thank Anurag Banerjee, Judith Clarke, Kazuhiro Ohtani, and Guohua Zou for their helpful suggestions and advice during the course of this work. In particular, we are very grateful to Judith Clarke for bringing to our attention the unpublished work of D.H. Thomas and to Guohua Zou for his careful reading of an earlier version of this paper. Thanks also go to the co-editor Benedikt Pötscher and two anonymous referees for their valuable comments. The second author gratefully acknowledges financial support from the Hong Kong Research Grant Council.
In econometrics the use of the t- and F-ratios is ubiquitous. Let us define the t-ratio as

, where w is a p × 1 random vector with zero mean, a is a p × 1 nonrandom vector, B is a p × p positive semidefinite nonrandom matrix, and r ≥ 1 is the rank of B. It is well recognized that τ will not in general be Student's t distributed for three reasons: (i) w is not normally distributed; (ii) even if w is normally distributed, w′Bw may not follow the chi-square distribution; and (iii) a′w and w′Bw are not distributed independently (Smith, 1992; Magnus, 2002). In the case of τ2, it is well known that if the normality assumption of w is relaxed to one of spherical symmetry, then neither is w′Bw necessarily chi-squared distributed nor are a′w and w′Bw distributed independently, but τ2 remains F distributed under some mild conditions (see, e.g., Ullah and Zinde-Walsh, 1985; Giles, 1991; Qin, Cui, and Li, 1998). Little is known, however, about the (exact) distribution of τ under the nonnormal setting. So far, analytical results on the t-test in the absence of normality have been obtained largely under asymptotic considerations.
1 Note that although τ ∼ tr implies τ2 ∼ F1,r, the converse need not be true.2Consider the variable T1 with density

. It is easy to see that T1 does not follow the t distribution but T12 is F distributed with 1 and v degrees of freedom.
This paper derives the necessary and sufficient conditions for τ to be t distributed for the case of w having a distribution of the elliptically symmetric type. It can be shown that under the aforementioned conditions (i)–(iii), it is still possible for τ to be t distributed. In particular, it is shown that under various conditions of nonnormality the t-ratio remains t distributed in finite samples. That is, for a variety of nonnormal cases the t-test retains finite sample validity. Our results lend support to the general view that the critical values from the t distribution should be used for controlling the t-test's type I error even in the absence of normality. This work also extends results obtained by Magnus (2002), who investigates the effect that dependence between a′w and w′Bw has in respect to the t-ratio. It is shown that the results of Magnus (2002) are in fact independent of the normality of w; provided that w is elliptically symmetric, τ is distributional invariant, and the results obtained by Magnus (2002) on the sensitivity of the t-ratio hold precisely also in the nonnormal cases.
The second part of this paper considers the distribution of the F-ratio for testing linear hypothesis in a regression with nonnormal error terms. Although much has been written on this topic, the type of nonnormal distribution has been limited to that of multivariate t (Ullah and Phillips, 1986) or spherical symmetry (Ullah and Zinde-Walsh, 1985; Giles, 1991; Ohtani and Giles, 1993).3
Linear regression models with elliptically or spherically symmetric errors have been studied from various perspectives. See Breusch, Robertson, and Welsh (1997) for a list of references. Bayesian extensions may be found in Jammalamadaka, Tiwari, and Chib (1987), Chib, Tiwari, and Jammalamadaka (1988), and Osiewalski (1991).
The work of Thomas (1970) is unknown to many, but some of his results are discussed in Fang et al. (1990, pp. 54–55), Giles (1991), and Ohtani and Giles (1993).
The rest of this paper is organized as follows. In Section 2, we consider a general form of the t-ratio and derive the necessary and sufficient conditions for it to be t distributed. The moments of the t-ratio in elliptically distributed variables are also obtained. It is shown that the expressions of the moments are invariant in respect to the distributional setting if the distribution is elliptically symmetric. In Section 3, we extend the analysis to a linear model and consider the distribution of the F-statistic with nonnormal error terms.
Turning first to the t-ratio τ defined earlier, for purposes of analysis we write w = (w1,w2′)′, where w1 is a scalar, w2 is a q × 1 vector, and p = 1 + q. Write, conformably,

as the covariance matrix of w, where γ > 0 is an arbitrary scalar, C is a 1 × q vector, and Σ is a q × q positive definite matrix. Also, let

, the rank of B, satisfy 0 < r ≤ q. Furthermore, it is assumed that w has an elliptically symmetric (or simply elliptical) distribution with mean zero and density function of the form

where ϑ is a normalizing constant and h is some arbitrary function. It is conventional to write

. If

, then the density of w reduces to that of spherical symmetry. Special cases of the elliptical class of distributions include the multivariate normal, multivariate Student's t, multivariate Cauchy, and rotated Laplace distributions.
Elliptical distribution has played an important role in distributional theory and other fields of statistics. Fang, Kotz, and Ng (1990) and Fang and Zhang (1990) provide a thorough discussion of the properties of the elliptical class of distributions and related topics. The results given in these books are in fact central to a generation of efforts devoted to various theoretical developments and applications of symmetric nonnormal distributions, and the following list illustrates some of the interesting examples that have been considered. Läuter (1996) and Läuter, Glimm, and Kropf (1996) use the properties of the spherical matrix distribution (Fang and Zhang, 1990) to obtain statistics that are suitable for the analysis of high-dimensional samples of small size and that result in no test size distortion. Li, Fang, and Zhu (1997) propose probability plots for testing spherical symmetry versus elliptical symmetry based on the invariant property5
This result discussed in Fang et al. (1990) is also of relevance to our paper and is stated as Lemma 2 in the Appendix.
The following theorem gives the necessary and sufficient condition for τ to be t distributed.
THEOREM 1. Under the stated assumptions,

if and only if

.
Proof. See the Appendix.
In the case where a is a p × 1 vector with a single nonzero element, B = diag(0,Σ−1), and Σ is of full rank, Theorem 1 simplifies significantly and reduces to the following corollary.
COROLLARY 1. Let a = (1,0′)′ and B = diag(0,Σ−1); then

if and only if C = 0.
Proof. See the Appendix.
So, under the conditions of nonnormality characterized in Corollary 1, the t-ratio τ remains Student's t distributed provided that the random vector forming the t-ratio has a diagonal covariance structure. To consider an application, suppose that w = (w1,w2′)′ follows the (spherical) multivariate t distribution, i.e.,

where v > 2 and σ2 > 0. Note that cov(w) = (σ2v/(v − 2))Ip and B = diag(0,Iq). Now, by virtue of Corollary 1,

, but w2′w2 is neither chi-squared distributed
6In fact, it can be shown that Φ = w2′w2 has the density

It is also straightforward to show that w1 and w2′w2 are not distributed independently.

with density function

where

. Formula (2.3) characterizes a multivariate t density with a nonspherical covariance structure provided that

. Straightforwardly, by Corollary 1,

Again, the distribution of τ can remain Student's t with q degrees of freedom despite the violation of the aforementioned conditions (i)–(iii).
Under the normal setup, Magnus (2002) derives the even moments of τ. Note that whatever the distribution of w, if it is elliptically symmetric, the odd moments of τ that exist are zero. The following theorem gives the even moments of τ when w follows the elliptically symmetric distribution.
THEOREM 2. Under the stated assumptions, i.e.,

, and a and B are defined as in Section 1, provided that q ≥ r ≥ 2(s + 1), then E(τ2s) exists and has the representation

for s = 1,2,3,…, where

are the nonzero eigenvalues of

, and v1,…,vr are the eigenvectors of B* such that B*vi = λi vi,vi′vi = 1, and vi′vj = 0 for all i ≠ j.
Proof. See the Appendix.
In other words, the moments of τ under the nonnormal elliptical setup are also the same as those under normality. It also follows straightforwardly that

and

These expressions have proved useful for analyzing the sensitivity of τ to the relationship between a′w and w′Bw. Magnus (2002) does so for the special case of w being normally distributed and w′Bw following a chi-square distribution. Magnus's sensitivity analysis is in fact confined to the case where the nonzero eigenvalues of L′BL are all equal, i.e., λ1 = λ2 = ··· = λ. In this case w′Bw must be chi-square distributed except for a constant scalar. This is obvious, as

, we have

, where

is an orthogonal matrix such that Q′L′BLQ = λ diag(Ir,0). Magnus (2002) defines

as the dependence parameter in the normal setup. If δ = 0, then a′w and w′Bw are independent; if δ > 0, they are dependent. Magnus (2002) finds that var(τ) decreases linearly from r/(r − 2) to 1 as δ increases from 0 to 1. Hence the more the dependence between a′w and w′Bw, the better the variance of τ is approximated by the standard normal distribution's variance. He also finds that kur(τ) decreases almost linearly from 3(r − 2)/(r − 4) to 3r/(r + 2) and the deviation of the kurtosis from normality decreases as δ increases. So, with dependence the t-ratio τ is better approximated by the standard normal distribution than the Student's t distribution. If w has a (nonnormal) elliptical distribution, then w′Bw may not be chi-square distributed, but Magnus's results are still valid, as τ is distributional invariant for all elliptically symmetric vectors, as is obvious from the proof of Theorem 2. Note that in the elliptical setup, the condition of L′BL having identical nonzero eigenvalues does not imply

for some constant scalar cs, but it does imply

for some random variable cr such that cr ≥ 0 and Pr(cr = 0) = 0. One such example can be constructed from the (nonspherical) multivariate Student's t density given in (2.3) provided that the nonzero eigenvalues of

are all equal. Thus, the results of Magnus (2002) hold also in the more general context of w having an elliptically symmetric distribution; in the case of L′BL having identical nonzero eigenvalues, the higher δ is, the better the t-ratio is approximated by the standard normal distribution.
7In the elliptically symmetric setup, a′w and w′Bw are generally dependent, so δ is better thought of as a representation of the degree of correlation between the two random variables.
In this section we focus our interest on the linear regression model,

where y and ε are n × 1 vectors, X is an n × k fixed matrix of rank k, and β is a k × 1 vector of unknown coefficients. Furthermore, ε ∼ En(0,σ2Ω), and σ2 is an unknown parameter. When Ω = I, the t-statistic for testing the hypothesis that an element of β, say βi, equals a particular value βio is given by

where

is the ith element of the ordinary least squares estimator (X′X)−1X′y,

, and [(X′X)−1]ii is the (i,i)th element of (X′X)−1. Now, under the hypothesis βi = βio, ti can be equivalently expressed as

where

is an (n − k) × n matrix such that

. Now, by the properties of the elliptical distributions, (ϑ1,ϑ2′)′ ∼ En−k+1(0,diag(1,In−k)). Clearly, from Corollary 1, ti ∼ tn−k. The t-statistic therefore remains valid even without normally distributed disturbances.
Now, suppose that Ω ≠ I but Ω is a known positive definite matrix. A test of the hypothesis

where R is an m × k constant matrix of rank m(< k) and c is an m × 1 vector of constants, is carried out by computing the statistic

where

is the generalized least squares estimator of β. Assuming that Ho is true and the distribution of ε reduces to that of normality, the statistic F is well known to follow a central F distribution with m and n − k degrees of freedom. Ullah and Zinde-Walsh (1985) consider the error terms following the class of spherically symmetric disturbances with density function given by

where g is decreasing and twice differentiable on [0,+∞). It is easy to see that the density given in (3.6) is a special case of the (general) spherically symmetric density. Ullah and Zinde-Walsh (1985) show that Fo, which results from replacing Ω with I in (3.5), is distributed as a central F under Ho whatever g is, provided that it is decreasing and twice differentiable. In fact, an earlier unpublished work of Thomas (1970) has shown that F remains central F distributed under Ho when ε follows the class of elliptical distributions, i.e., ε ∼ En(0,σ2Ω). The result of Thomas (1970), however, as discussed in Fang et al. (1990, pp. 54–55), is conditional on the requirement that the distribution's characteristic function is a continuous decreasing function on [0,+∞). In other words, the class of distributions discussed in Thomas (1970) is in fact a subclass of the general class of elliptical distributions with density given in (2.1). Our aim here is to show that whatever the characteristic function, the null distribution of F remains central F under the elliptical distributions of errors.
THEOREM 3. Assume in model (3.1) that ε ∼ En(0,σ2Ω). Under Ho : Rβ = c, the distribution of F is F(m,n−k).
Proof. See the Appendix.
The crucial result for our purpose here is that the distribution of the F-ratio can remain central F even without normally distributed disturbances. Once again, our result relies on the assumption of elliptically symmetric errors. But what if the distribution of ε falls outside that of elliptical symmetry? Zaman (1996, p. 200) argues that the F-test is robust to lack of normality of the errors for a large class of nonnormal densities including all unimodal densities; his argument, however, is incorrect. Let us briefly recall the notation in Zaman's book. He defines the F-ratio as F = ε′Q1ε/ε′Q2ε, where Q1 and Q2 are projection matrices and ε is a vector of independent and identically distributed (i.i.d.) random errors.8
In general, the F-statistic defined in (3.5) cannot be written in the form of F = ε′Q1ε/ε′Q2ε so that Q1 and Q2 are projection matrices. If Ω = σ2I and Rβ = c, then one can write Q1 = X(X′X)−1R′[R(X′X)−1R′]−1R(X′X)−1X′ and Q2 = I − X(X′X)−1X′. In that case F = (ε′Q1ε/ε′Q2ε)(n − k)/m, which is consistent with Zaman's notation except for a constant scalar.
One must interpret the arguments of Zaman (1996) cautiously. His first argument is correct provided that one makes the additional qualification that Pr(θ = 0) = 0, but still this does not lead to the conclusion reached in his second argument. Let

for all i's and θ = (θ1,θ2,…θn)′ be the random vector such that ε = (θ1 z1,θ2 z2,…θn zn)′, i.e.,

. It is easy to see that ε′Q1ε/ε′Q2ε is generally not the same as z′Q1 z/z′Q2 z, except for the special case of θ1 = θ2 = ··· = θn. But the latter situation could not arise at least in the case of continuous θi′s. The following counterexample further clarifies our point. Let ε = (ε1,ε2)′, where ε1 and ε2 are i.i.d. and follow the Cauchy distribution, i.e., fεi(εi) = 1/(π(1 + εi2)), i = 1,2. Also, let Q1 = diag(1,0) and Q2 = diag(0,1). Now, F = ε12/ε22 has the density

which is not the density of an F1,1 variate, although fεi(εi) is unimodal.
Proof of Theorem 1. The proof of Theorem 1 requires the following preliminary results.
LEMMA 1. Let

, where

. Then

if and only if Ω12 = 0.
Proof. See Qin et al. (1998).
LEMMA 2. Let ψ ∼ Ep(0,γI),γ > 0, and l be some arbitrary function. The distribution of a statistic l(ψ) remains invariant provided that

is distributed identically to l(ψ) for all

.
Proof. See Fang et al. (1990, p. 51).
LEMMA 3. Let ψ ∼ Ep(0,γI),γ > 0, a be a p × 1 vector of unit length, and B be a p × p symmetric idempotent matrix of rank r such that 1 ≤ r ≤ q. Then

if and only if a′B = 0.
Proof. Write B = PP′, where P is a p × r matrix such that P′P = Ir. By Lemma 2,

, where

. Let

. Clearly,

, where

. If a′P = 0, then it is obvious that τ ∼ tr, i.e., τ2 ∼ F1,r. Clearly,

. So,

. But by Lemma 1, the latter arises if and only if a′P = 0. It follows that a′P = 0 is also the necessary and sufficient condition for τ ∼ tr. Lemma 3 then follows immediately because a′P = 0 if and only if a′B = 0. █
Now, to prove Theorem 1, note that

, where ψ ∼ Ep(0,γI). So,

. Write

, and then

. Obviously, a′a = 1. Also,

implies that B2 = B. So by virtue of Lemma 3, τ ∼ tr if and only if a′B = 0, i.e.,

. This completes the proof of Theorem 1. █
Proof of Corollary 1. To prove Corollary 1, note that if a = (1,0′)′ and B = diag(0,Σ−1), then

. Clearly,

if and only if C = 0. █
Alternatively, one can prove Corollary 1 independently of Theorem 1 using Lemmas 1 and 2 as follows. Write k1 = 1, k2 = q, Ω11 = γ, Ω12 = γC, and Ω22 = γΣ. Note that if τ ∼ tq, then τ2 ∼ F1,q. So it follows from Lemma 1 that C = 0 is the necessary condition for τ to be t distributed. To prove the sufficiency part of the theorem, let us define

. As

. Clearly,

for all

. Note also that

. Now, because τ ∼ tq for

, by virtue of Lemma 2, the distribution of τ remains invariant for all

.
Proof of Theorem 2. Because

, we have

, where A is a nonnegative random variable such that Pr(A = 0) = 0, U is a uniformly distributed random vector over a p-dimensional hypersphere, and A and U are independent. So,

. Note that

. Hence

, where

. Thus, Theorem 2 is algebraically identical to the corresponding theorem given in Magnus (2002) for the normal case. █
Proof of Theorem 3. Let


and

where P is an (n − k) × n matrix such that P′P = Λ2 and PP′ = In−k. Note that Λ1Λ2′ = 0 and u = (u1′,u2′)′ ∼ En−k+m(0,In−k+m). So, under Ho : Rβ = c,

Theorem 3 then follows directly from Lemma 1. █