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Modelling Dependence with Copulas - IFOR

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6 Elliptical <strong>Copulas</strong><br />

A spherical distribution distribution is an extension of the standard multinormal<br />

distribution N (0, I n ) and an elliptical distribution is an extension of N (µ, Σ). Recall<br />

that N (µ, Σ) can be defined from the standard multivariate normal distribution<br />

N (0, I n )via<br />

X = d µ + AY, (6.0.6)<br />

where X ∼N(µ, Σ), Y ∼N(0, I n )andΣ=AA T . With this in mind it seems<br />

natural to start <strong>with</strong> spherical distributions and then define elliptical distributions<br />

from the spherical in the way indicated by (6.0.6).<br />

Definition 16. An n × 1 random vector X is said to have a spherically symmetric<br />

distribution (or simply spherical distribution) if for every Γ ∈O(n),<br />

where O(n) denotes the set of n × n orthogonal matrices.<br />

ΓX = d X, (6.0.7)<br />

Note that an orthogonal matrix represents a rotation transformation. Hence<br />

spherical distributions are geometrically interpreted as those invariant under rotations.<br />

Theorem 6.1. An n-vector X has a spherical distributions if and only if its characteristic<br />

function Ψ(t) satisfies one of the following equivalent conditions:<br />

1. Ψ(Γ T t)=Ψ(t) for any Γ ∈O(n);<br />

2. There exist a function φ(·) of a scalar variable such that<br />

Ψ(t) =φ(t T t).<br />

For the proof, see Fang, Kotz and Ng (1987) [5].<br />

From the theorem above we see that for spherical distributions the characteristic<br />

function Ψ(t) =E(exp(it T X)) = φ(t T t), and for this reason we will use the notation<br />

X ∼ S n (φ) whenX is spherically distributed. The function φ given above is called<br />

the characteristic generator of the spherical distribution.<br />

Example 6.1. Let X ∼N(0, I n ). Since the components X i ∼N(0, 1),i=1,... ,n<br />

are independent and the characteristic function of X i is exp(−t 2 i /2), the characteristic<br />

function of X is<br />

exp{− 1 2 (t2 1 + ...+ t 2 n)} =exp{− 1 2 tT t}.<br />

From Theorem 6.1 it then follows that X ∼ S n (φ) whereφ(s) =exp(−s/2).<br />

The spherical distributions can be defined in an alternative and equivalent way.<br />

This definition also provides the basis for many random variate generation techniques.<br />

Definition 17. An n × 1 random vector X is said to have a spherically symmetric<br />

distribution (or simply spherical distribution) if it has the stochastic representation<br />

X = d RU (6.0.8)<br />

for some positive random variable R independent of the random vector U uniformly<br />

distributed on the unit hypersphere S n−1 = {z ∈ R n |z T z =1}.<br />

Spherical distributions can thus be interpretated as mixtures of uniform distributions<br />

on hyperspheres <strong>with</strong> different radius.<br />

45

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