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Estimation in Financial Models - RiskLab

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Theorem 6 Depend<strong>in</strong>g on the value of we have the follow<strong>in</strong>g asymptotic<br />

behaviour for the normalized deviation q I n ()(^ n , ):<br />

q<br />

<br />

lim P I<br />

n,!1 n ()(^ n , ) z =<br />

8<br />

><<br />

>:<br />

(z); jj < 1;<br />

H (z); jj =1;<br />

Ch(z); jj > 1;<br />

where (z) is the standard normal distribution, Ch(z) is the Cauchy distribution<br />

and H (z) is the distribution of the random variable<br />

<br />

2 3 2<br />

where W denotes a Wiener process.<br />

W 2 (1) , 1<br />

R 1<br />

0<br />

W 2 (s)ds ;<br />

Hence, <strong>in</strong> the stationary case jj < 1 the normalized deviation q I n ()(^ n ,)<br />

is asymptotically normally distributed, whereas <strong>in</strong> the other cases it has<br />

as limit distribution the Cauchy distribution or the quite unexpected H <br />

distribution. The question arises wether we can reduce the number of limit<br />

distributions by modify<strong>in</strong>g the normaliz<strong>in</strong>g factor q I n (). Indeed, <strong>in</strong>stead of<br />

us<strong>in</strong>g the Fisher <strong>in</strong>formation I n () =EhMi n , choos<strong>in</strong>g the stochastic Fisher<br />

<strong>in</strong>formation hMi n as normaliz<strong>in</strong>g factor we obta<strong>in</strong><br />

Theorem 7<br />

lim<br />

n,!1 P <br />

q<br />

(<br />

(z); jj 6=1;<br />

hMi n (^ n , ) z =<br />

H (z); jj =1:<br />

Summariz<strong>in</strong>g: the MLE ^ n is (strongly) consistent and the normalized deviations<br />

q I n ()(^ n , ) and q hMi n (^ n , ) are asymptotically distributed as<br />

shown <strong>in</strong> both theorems.<br />

3.2.2 ARCH and GARCH models<br />

In the follow<strong>in</strong>g we concentrate on ARCH and GARCH models and especially<br />

on estimation <strong>in</strong> these models. We refer to the fundamental papers by<br />

Engle [22] and Bollerslev [12] and to Bollerslev, Chou and Kroner [13] and<br />

Bollerslev, Engle and Nelson [14].<br />

Conventional econometric time series models assume constantvariance. However,<br />

over a decade ago risk and uncerta<strong>in</strong>ty considerations lead to the development<br />

of new econometric time series models that allow for the model<strong>in</strong>g<br />

45

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