Mean volume of sphere (normal distributed radius)

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SUMMARY

The discussion centers on the calculation of the mean volume of a sphere with a normally distributed radius, as described in the reference document. The formula used is V = ∫_{-∞}^∞ dr V(r) N(r| r_0,s), which integrates the volume function V=(4/3) π r^3 over the entire real line. The choice of limits from negative to positive infinity allows for a closed-form solution, despite the impracticality of negative radii. The mean volume exceeds the volume calculated using the mean radius due to the cubic relationship in the volume formula, which disproportionately weights larger radii.

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ChrisVer
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I read in http://www-library.desy.de/preparch/books/vstatmp_engl.pdf page 29 (43 for pdf) that the mean volume is:
<V> = \int_{-\infty}^\infty dr V(r) N(r| r_0,s)
I have two questions.
Q1: why do they take the radius to be from -infinity to +infinity and not from 0 to infinity?
Q2: is there an intuitive way to see/describe why the mean volume is larger than the one obtained from the mean radius?

Thanks
 
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It would appear the normal distribution about ## r=r_o ## is an approximation they want you to use even though that allows for a finite probability that ## r<0 ##. The integral from minus infinity to plus infinity can be solved in closed form, but I don't believe you get a closed form if the limits were zero to infinity even though the answer would be nearly identical. The ## V=(4/3) \pi r^3 ## function will add more weight to the larger r's because of the 3rd power dependence, making the mean volume larger than ## V=(4/3) \pi r_o^3 ##, but I don't have a simple intuitive description for that.
 
ChrisVer said:
Q2: is there an intuitive way to see/describe why the mean volume is larger than the one obtained from the mean radius?

You could compare the mean of ##\{1^3, 2^3, 3^3\} ## with ##2^3##.
 
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