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Disk integration
From Wikipedia, the free encyclopedia
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Disk integration is a means of calculating the volume of a solid of revolution, when integrating along the axis of revolution. This method models the generated 3 dimensional shape as a "stack" of an infinite number of disks (of varying radius) of infinitesimal thickness.
If the function to be revolved is a function of x, the following integral represents the volume of the solid of revolution:
![\pi \int_{a}^{b} [R(x)]^2 dx](../../../math/f/6/3/f63d1514a5869667288dd9b288a55f15.png)
where R(x) is the distance between the function and the axis of rotation. This works only if the axis of rotation is horizontal (example: y = 3 or some other constant).
If the function to be revolved is a function of y, the following integral will obtain the volume of the solid of revolution:
![\pi \int_{a}^{b} [R(y)]^2 dy](../../../math/7/1/1/711e8b45a8103c62a79e118c5e38b4af.png)
where R(y) is the distance between the function and the axis of rotation. This works only if the axis of rotation is vertical (example: x = 4 or some other constant).
To obtain a "hollow" solid of revolution (sometimes called the "washer method"), the procedure would be to take the volume of the inner solid of revolution and subtract from it the volume of the outer solid of revolution. This can be calculated in a single integral similar to the following:
![\pi \int_{a}^{b} ([R_O(x)]^2 - [R_I(x)]^2 )dx](../../../math/6/0/6/606b3c1a2b3127107f06c8b5dff72a57.png)
Where RO(x) is the function that is farthest from the axis of rotation and RI(x) is the function that is closest to the axis of rotation. One should take caution not to evaluate the square of the difference of the two functions, but to evaluate the difference of the squares of the two functions. ![[R_O(x)]^2 - [R_I(x)]^2 \not\equiv \; [R_O(x) - R_I(x)]^2](../../../math/2/9/2/292397116832d831b596104dfeea3d79.png)
NOTE: the above formula only works for revolutions about the x-axis.
To rotate about any horizontal axis, simply subtract from that axis each formula:
if h is the value of a horizontal axis, then the volume =
![\pi \int_{a}^{b} ([h-R_O(x)]^2 - [h-R_I(x)]^2 )dx](../../../math/7/d/3/7d32945a95ba6eb3dcede9a90db6e4b7.png)
For example, to rotate the region between y = − 2x + x2 and y = x
along the axis y = 4, you would have to integrate as follows:
![\pi \int_{0}^{3} ([4-(-2x+x^2)]^2 - [4-x]^2 )dx](../../../math/d/c/b/dcb0ef1e6f0b98cc65f1395dbac1a17a.png)
Note that when you integrate along an axis other than then the x, the further axis may not be that obvious. In the previous example, even though y = x is further up than y = − 2x + x2, it is the inner axis since it is closer to y = 4
The same idea can be applied to both the y-axis and any other vertical axis. You simply must solve each equation for x before you plug them into the integration formula.