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Segmentation of Stochastic Images using ... - Jacobs University

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3.3 Polynomial Chaos Expansions<br />

Theorem 3.3. The Wiener chaos representation <strong>of</strong> any random variable X ∈ L 2 (Ω) converges in the<br />

L 2 (Ω)-sense to X. This means, if X is any functional for which<br />

∫<br />

|X(ω)| 2 dω < ∞ , (3.24)<br />

Ω<br />

then<br />

∫<br />

lim |X(ω) −∑ N N→∞<br />

α=1 a αΨ α (ξ (ω))| 2 dω = 0 . (3.25)<br />

Ω<br />

The Fourier-Hermite coefficient a α is<br />

∫<br />

a α = X(ω)Ψ α (ξ (ω))dω . (3.26)<br />

Ω<br />

The Cameron-Martin theorem ensures that every random variable with finite variance has a representation<br />

in the Wiener chaos, but gives no information about the convergence rate <strong>of</strong> the representation.<br />

The convergence rate is important when the series expansion is cut after a finite number <strong>of</strong> terms.<br />

This is necessary for numerical algorithms dealing with polynomial chaos expansions. In fact, [160]<br />

showed that the convergence rate <strong>of</strong> the Wiener chaos is substantially less the optimal, exponential,<br />

convergence rate. The development <strong>of</strong> other chaos types leads to expansions that have better convergence<br />

properties. This is the topic <strong>of</strong> the next section, which introduces the generalized polynomial<br />

chaos expansion, originally proposed by Xiu and Karniadakis [160].<br />

3.3.3 Generalized Polynomial Chaos<br />

Xiu and Karniadakis [160] generalized the idea <strong>of</strong> the representation <strong>of</strong> random variables in an orthogonal<br />

basis formed by polynomials in random variables with known distribution. They proposed<br />

to use polynomials whose weighting functions correspond to the PDF <strong>of</strong> the underlying random variables.<br />

It turns out that these polynomials are the polynomials from the Askey-scheme [16]. Table 3.2<br />

shows the correspondence between important random variables and the associated polynomials. To<br />

summarize, a random variable with finite variance has a representation in the polynomial chaos by<br />

X(ω) = ∑ ∞ α=1 a αΨ α (ξ ) , (3.27)<br />

where the multi-dimensional polynomials are selected from the Askey-scheme [16]. The multidimensional<br />

polynomials are constructed from one-dimensional polynomials via<br />

ψ α = ∏ n i=1 H α i<br />

(ξ i ) , (3.28)<br />

whereas α is the index corresponding to the multiindex (α 1 ,...,α n ) and H αi , i = 1,...,n are polynomials<br />

in one random variable. Fig. 3.1 shows the first one-dimensional polynomials for the Legendrechaos<br />

and Fig. 3.3 the polynomials for the Hermite-chaos. We rescaled the Legendre- and Hermitepolynomials<br />

to get an orthonormal basis <strong>of</strong> L 2 (Ω) with respect to the weighted scalar product, i.e.<br />

〈Ψ α ,Ψ β 〉 = δ αβ , (3.29)<br />

because the weighting functions for the random variables are 0.5 and 1 √<br />

2π<br />

exp −x2<br />

2 , respectively.<br />

Ernst et al. [50] proved that the polynomial chaos expansion converges in quadratic mean, i.e. in<br />

the L 2 (Ω) sense [73], if and only if the basic random variables have finite moments <strong>of</strong> all orders and<br />

the probability density <strong>of</strong> the basic random variables is continuous. Furthermore, the moment problem<br />

(cf. [50]), i.e. the identification <strong>of</strong> the measure from the moments, has to be uniquely solvable.<br />

Nouy [116] showed that multimodal random variables are hard to approximate in a onedimensional<br />

polynomial chaos expansion. He solved this problem by introducing a special kind<br />

31

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