M408M Learning Module Pages
Main page Chapter 10: Parametric Equations and Polar CoordinatesChapter 12: Vectors and the Geometry of SpaceChapter 13: Vector FunctionsChapter 14: Partial DerivativesChapter 15: Multiple IntegralsLearning module LM 15.1: Multiple integralsLearning 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 dimensionMappings in 2 dimensions Jacobians Examples Cylindrical and spherical coordinates |
Change of variable in 1 dimensionOf 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 N∑i=1f(g(x∗i))g′(x∗i)Δix, where we have broken the interval from a to b into N pieces, x∗i is a point in the i-th piece, and Δix is the length of the i-th piece. If we let u∗i=g(x∗i), then Δiu≈g′(x∗i)Δix, and our sum is approximately N∑i=1f(u∗i)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.
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