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Mathematical Methods for Physics and Engineering - Matematica.NET

Mathematical Methods for Physics and Engineering - Matematica.NET

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30.5 PROPERTIES OF DISTRIBUTIONSWe note that the notation µ k <strong>and</strong> ν k <strong>for</strong> the moments <strong>and</strong> central momentsrespectively is not universal. Indeed, in some books their meanings are reversed.We can write the kth central moment of a distribution in terms of its kth <strong>and</strong>lower-order moments by exp<strong>and</strong>ing (X − µ) k in powers of X. We have alreadynoted that ν 2 = µ 2 − µ 2 1 , <strong>and</strong> similar expressions may be obtained <strong>for</strong> higher-ordercentral moments. For example,In general, it is straight<strong>for</strong>ward to show thatν 3 = E [ (X − µ 1 ) 3]= E [ X 3 − 3µ 1 X 2 +3µ 2 1X − µ 3 ]1= µ 3 − 3µ 1 µ 2 +3µ 2 1µ 1 − µ 3 1= µ 3 − 3µ 1 µ 2 +2µ 3 1. (30.53)ν k = µ k − k C 1 µ k−1 µ 1 + ···+(−1) r k C r µ k−r µ r 1 + ···+(−1) k−1 ( k C k−1 − 1)µ k 1.(30.54)Once again, direct evaluation of the sum or integral in (30.52) can be rathertedious <strong>for</strong> higher moments, <strong>and</strong> it is usually quicker to use the moment generatingfunction (see subsection 30.7.2), from which the central moments can be easilyevaluated as well.◮The PDF <strong>for</strong> a Gaussian distribution (see subsection 30.9.1) with mean µ <strong>and</strong> varianceσ 2 is given byf(x) = 1 [ ]σ √ 2π exp (x − µ)2− .2σ 2Obtain an expression <strong>for</strong> the kth central moment of this distribution.As an illustration, we will per<strong>for</strong>m this calculation by evaluating the integral in (30.52)directly. Thus, the kth central moment of f(x) isgivenbyν k =∫ ∞−∞= 1σ √ 2π= 1σ √ 2π(x − µ) k f(x) dx∫ ∞−∞∫ ∞−∞](x − µ) k (x − µ)2exp[−2σ 2dx)y k exp(− y2dy, (30.55)2σ 2where in the last line we have made the substitution y = x − µ. It is clear that if k isodd then the integr<strong>and</strong> is an odd function of y <strong>and</strong> hence the integral equals zero. Thus,ν k =0ifk is odd. When k is even, we could calculate ν k by integrating by parts to obtaina reduction <strong>for</strong>mula, but it is more elegant to consider instead the st<strong>and</strong>ard integral (seesubsection 6.4.2)I =∫ ∞−∞exp(−αy 2 ) dy = π 1/2 α −1/2 ,1149

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