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M408M Learning Module Pages

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Chapter 10: Parametric Equations and Polar Coordinates

Chapter 12: Vectors and the Geometry of Space


Chapter 13: Vector Functions


Chapter 14: Partial Derivatives


Chapter 15: Multiple Integrals


Learning module LM 15.1: Multiple integrals

Learning module LM 15.2: Multiple integrals over rectangles:

Learning module LM 15.3: Double integrals over general regions:

Learning module LM 15.4: Double integrals in polar coordinates:

Learning module LM 15.5a: Multiple integrals in physics:

Learning module LM 15.5b: Integrals in probability and statistics:

Learning module LM 15.10: Change of variables:

      Change of variable in 1 dimension
      Mappings in 2 dimensions
      Jacobians
      Examples
      Cylindrical and spherical coordinates

Change of variable in 1 dimension

Change of variable in 1 dimension

Of all the techniques of integration that we have learned, the most powerful, and the simplest, is u-substitution. If u=g(x), then baf(g(x))g(x)dx=g(b)g(a)f(u)du. You probably learned this method in terms of anti-derivatives, as a way to turn the chain rule inside out. That sort of reasoning doesn't generalize very well to multiple dimensions. Instead, let's analyze u-substitution from the definition of an integral.


By definition, baf(g(x))g(x)dx is the limit of a sum Ni=1f(g(xi))g(xi)Δix, where we have broken the interval from a to b into N pieces, xi is a point in the i-th piece, and Δix is the length of the i-th piece. If we let ui=g(xi), then Δiug(xi)Δix, and our sum is approximately Ni=1f(ui)Δiu. The limit of this sum is, by definition, the definite integral of f(u)du from the starting value of u (namely g(a)) to the ending value of u (g(b)). We have converted an integral in x-space into an integral in u-space, but the functions being integrated are not the same. In one case we integrate f(u). In the other case we integrate f(g(x)) times a distortion factor g(x). This factor corrects for Δu being a different size than Δx.


We also learned about inverse u-substitution, especially in the context of trig substitutions. If x=g(u) (rather than the other way around), then baf(x)dx=βαf(g(u))g(u)du, where a=g(α) and b=g(β). That's the same rule we had before, only with the roles of x and u reversed. We say that g is a mapping from u-space to x-space, sending the interval [α,β] to the interval [a,b], and the distortion factor g(u) is called the Jacobian of this mapping. When we write the equation dx=g(u)du, we are saying that the length of a short interval in x-space is g(u) longer than the interval of the corresponding interval in u-space.

Example: Compute 100ex/5dx.
Solution: We let x=g(u)=5u, so ex/5=eu and dx=5du. The map g sends the interval [0,2] in u-space to the interval [0,10] in x-space,
and g(u)=5 tells us that the x-interval is 5 times bigger than the u-interval, so 100ex/5dx=205eudu=5(1e2).