25.06.2013 Views

statistique, théorie et gestion de portefeuille - Docs at ISFA

statistique, théorie et gestion de portefeuille - Docs at ISFA

statistique, théorie et gestion de portefeuille - Docs at ISFA

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

3.2 Typical recurrence time of large losses<br />

L<strong>et</strong> us transl<strong>at</strong>e these formulas in intuitive form. For this, we <strong>de</strong>fine a Value-<strong>at</strong>-Risk VaR ∗ which is such th<strong>at</strong><br />

its typical frequency is 1/T0. T0 is by <strong>de</strong>finition the typical recurrence time of a loss larger than VaR ∗ . In<br />

our present example, we take T0 equals 1 year for example, i.e., VaR ∗ is the typical annual shock or crash.<br />

Expression (49) then allows us to predict the recurrence time T of a loss of amplitu<strong>de</strong> VaR equal to β times<br />

this reference value VaR ∗ :<br />

401<br />

<br />

T<br />

ln (β<br />

T0<br />

c ∗ c VaR<br />

− 1)<br />

+ O(ln β) . (56)<br />

W (0) ˆχ<br />

Figure 2 shows ln T versus β. Observe th<strong>at</strong> T increases all the more slowly with β, the smaller is the<br />

T0<br />

exponent c. This quantifies our expect<strong>at</strong>ion th<strong>at</strong> large losses occur more frequently for the “wil<strong>de</strong>r” subexponential<br />

distributions than for super-exponential ones.<br />

4 Optimal portfolios<br />

In this section, we present our results on the problem of the efficient portfolio alloc<strong>at</strong>ion for ass<strong>et</strong> distributed<br />

according to modified Weibull distributions with the different <strong>de</strong>pen<strong>de</strong>nce structures studied in the previous<br />

sections. We focus on the case when all ass<strong>et</strong> modified Weibull distributions have the same exponent c, as<br />

it provi<strong>de</strong>s the richest and more varied situ<strong>at</strong>ion. When this is not the case and the ass<strong>et</strong>s have different<br />

exponents ci, i = 1, ..., N, the asymptotic tail of the portfolio r<strong>et</strong>urn distribution is domin<strong>at</strong>ed by the ass<strong>et</strong><br />

with the heaviest tail. The largest risks of the portfolio are thus controlled by the single most risky ass<strong>et</strong><br />

characterized by the smallest exponent c. Such extreme risk cannot be diversified away. In such a case, for<br />

a risk-averse investor, the best str<strong>at</strong>egy focused on minimizing the extreme risks consists in holding only the<br />

ass<strong>et</strong> with the thinnest tail, i.e., with the largest exponent c.<br />

4.1 Portfolios with minimum risk<br />

L<strong>et</strong> us consi<strong>de</strong>r first the problem of finding the composition of the portfolio with minimum risks, where<br />

the risks are measured by the Value-<strong>at</strong>-Risk. We consi<strong>de</strong>r th<strong>at</strong> short sales are not allowed, th<strong>at</strong> the risk free<br />

interest r<strong>at</strong>e equals zero and th<strong>at</strong> all the wealth is invested in stocks. This last condition is in<strong>de</strong>ed the only<br />

interesting one since allowing to invest in a risk-free ass<strong>et</strong> would autom<strong>at</strong>ically give the trivial solution in<br />

which the minimum risk portfolio is compl<strong>et</strong>ely invested in the risk-free ass<strong>et</strong>.<br />

The problem to solve reads:<br />

VaR ∗ α = min VaRα = ξ(α) 2/c W (0) · min ˆχ (57)<br />

N<br />

i=1 wi = 1 (58)<br />

wi ≥ 0 ∀i. (59)<br />

In some cases (see table 1), the prefactor ξ(α) <strong>de</strong>fined in (52) also <strong>de</strong>pends on the weight wi’s through λ−<br />

<strong>de</strong>fined in (46). But, its contribution remains subdominant for the large losses. This allows to restrict the<br />

minimiz<strong>at</strong>ion to ˆχ instead of ξ(α) 2/c · ˆχ.<br />

13

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!