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cwbullivant
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Homework Statement
Taylor, Classical Mechanics Problem 10.11 **
a) Use the result of problem 10.4 (derivation of the general integral for a moment of inertia of a continuous mass distribution in spherical coordinates, using point particles) to find the moment of inertia of a uniform solid sphere for rotation about a diameter.
b) Do likewise for a uniform hollow sphere whose inner and outer radii are a and b. [One slick way to do this is to think of the hollow sphere as a solid sphere of radius b from which you have removed a sphere of the same density but radius a.]
Homework Equations
## I = \int r^2 dm ## - 1
## dm = \rho dV ## - 2
## \rho = \frac{M}{\frac{4\pi R^3}{3}} = \frac{3M}{4\pi R^3} ## - 3
## dV = r^2 sin \theta dr d\theta d\phi ## - 4
The Attempt at a Solution
I'm limiting it to part a for now, since that's where I got stuck. The problem statement is "any diameter", and I'm going to center the sphere on the origin and have it rotate about the z-axis, for convenience. The previous problem it references is a derivation of the general integral in spherical coordinates, so that's the system I'll be using here.
First, combining the equations to make a volume integral:
## I = \frac{3M}{4\pi R^3} \iiint r^4 sin \theta dr d\theta d\phi ##
Where the integration bounds are:
## r: 0 \rightarrow R ##
## \theta: 0 \rightarrow \pi ##
## \phi: 0 \rightarrow 2 \pi ##
First integrating phi:
## I = \frac{3M}{2 R^3} \iint r^4 sin \theta dr d\theta ##
And then theta:
## I = \frac{3M}{R^3} \int r^4 dr ##
And finally r:
## I = \frac{3M}{R^3} \frac{R^5}{5} = \frac{3}{5}MR^2 ##
But I know this is wrong, as the answer I learned in freshman mechanics was
## I = \frac{2}{5} MR^2 ##
And I can't seem to figure out why the answer is incorrect.