Page 238 - Schaum's Outline of Theory and Problems of Advanced Calculus
P. 238

Line Integrals, Surface




                       Integrals, and Integral



                                                                      Theorems













                        Construction of mathematical models of physical phenomena requires functional domains of greater
                     complexity than the previously employed line segments and plane regions. This section makes progress
                     in meeting that need by enriching integral theory with the introduction of segments of curves and
                     portions of surfaces as domains.  Thus, single integrals as functions defined on curve segments take
                     on new meaning and are then called line integrals. Stokes’s theorem exhibits a striking relation between
                     the line integral of a function on a closed curve and the double integral of the surface portion that is
                     enclosed. The divergence theorem relates the triple integral of a function on a three-dimensional region
                     of space to its double integral on the bounding surface. The elegant language of vectors best describes
                     these concepts; therefore, it would be useful to reread the introduction to Chapter 7, where the impor-
                     tance of vectors is emphasized.  (The integral theorems also are expressed in coordinate form.)



                     LINE INTEGRALS
                        The objective of this section is to geometrically view the domain of a vector or scalar function as a
                     segment of a curve. Since the curve is defined on an interval of real numbers, it is possible to refer the
                     function to this primitive domain, but to do so would suppress much geometric insight.
                        A curve, C,in three-dimensional space may be represented by parametric equations:
                                             x ¼ f 1 ðtÞ; y ¼ f 2 ðtÞ; z ¼ f 3 ðtÞ;  a @ t @ b       ð1Þ

                     or in vector notation:
                                                           x ¼ rðtÞ                                  ð2Þ
                     where
                                                       rðtÞ¼ xi þ yj þ zk
                     (see Fig. 10-1).
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