Given a solid shape, if the areas of all slices orthogonal to a direction can be computed, then integrating that area function along the axis gives the volume.
Volume of a solid of rotation can be computed by rotating a line around an axis to create shapes like cylinders or cones.
Solids of Revolution: Disk Method
Given a region D in the plane between two functions f(x) and g(x), the goal is to compute the volume of the solid obtained by rotating D around the y-axis.
Example: A circle centered at (4,3) with radius 1.
Equation of the circle: (x−4)2+(y−3)2=1
Express y in terms of x to find two functions representing the upper and lower halves of the circle. y−3=±1−(x−4)2 y=3±1−(x−4)2
Thus, f(x)=3+1−(x−4)2 (upper half) and g(x)=3−1−(x−4)2 (lower half).
Volume Calculation by Cylindrical Shells
Approximate the area by rectangles.
Riemann sums: ∑[f(x<em>i<em>)−g(x</em>i</em>)]Δx
Consider rotating a single rectangle around the y-axis, forming a cylindrical shell.
Approximate this shell as a rectangular prism.
Dimensions of the Prism
Width (circumference): 2πxi∗
Height: f(x<em>i<em>)−g(x</em>i</em>)
Depth: Δx
Volume of the cylindrical shell: 2πx<em>i∗[f(x</em>i<em>)−g(xi</em>)]Δx
Riemann Sum and the Integral for Volume
Summing the volumes of all cylindrical shells approximates the total volume of the rotational solid.
This sum is a Riemann sum, leading to the integral: V=∫ab2πx[f(x)−g(x)]dx
Example Calculation
Given f(x)=x−1+0.5 and g(x)=x−1 (corrected to be g(x)=(x−1)2+0.5 [Typo in transcript, should read -0.5])
∫(x−1−(x−1)2)2πxdx
Using the substitution u=x−1, the integral can be solved.
Resulting volume: 3029π
General Formula
Region D bounded by x=a and x=b, with a and b positive.
Volume of the solid E obtained by rotating D around the y-axis: V=∫ab2πx[f(x)−g(x)]dx
Thin Rods and Center of Gravity
Mass of a thin rod with density function ρ(x) is computed by integrating the density function: m=∫abρ(x)dx
If density is homogeneous (constant), then mass = density * length.
Center of Gravity Calculation
For evenly distributed mass, the center of mass is at the midpoint.
For non-uniformly distributed mass, the center of gravity is calculated as a weighted average.
Consider the rod as a series of point masses and calculate the balancing point.
Derivation of Center of Gravity Formula
With two masses m<em>a at coordinate a and m</em>b at coordinate b, the center of gravity x<em>B satisfies:
m</em>a(x<em>B−a)=m</em>b(b−xB)
Therefore, x<em>B=m</em>a+mbm</em>aa+m<em>bb
Generalizing for n masses: x<em>B=∑m</em>i</em>∑m</em>i∗x<em>i<em>
Continuous Mass Distribution
Approximate the mass m<em>i<em> in each interval as ρ(x</em>i</em>)Δx