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Calculus 3 Chapter 15. Multiple Integrals 15.4. Double Integrals in Polar FormExamples and Proofs of Theorems February 2, 2020 () Calculus 3 February 2, 2020 1 / 12 Table of contents Exercise 15.4.6 1 Exercise 15.4.10 2 Exercise


  1. Calculus 3 Chapter 15. Multiple Integrals 15.4. Double Integrals in Polar Form—Examples and Proofs of Theorems February 2, 2020 () Calculus 3 February 2, 2020 1 / 12

  2. Table of contents Exercise 15.4.6 1 Exercise 15.4.10 2 Exercise 15.4.28 3 Exercise 15.4.38 4 Exercise 15.4.41 5 () Calculus 3 February 2, 2020 2 / 12

  3. Exercise 15.4.6 Exercise 15.4.6 Exercise 15.4.6. Describe the given region in polar coordinates: Solution. Since x = r cos θ then along the vertical line x = 1 we have 1 = r cos θ or r = 1 / cos θ = sec θ . Along the circle we have r = 2. So we can describe the region in terms of r -limits. A typical ray from the origin enters the region where r = sec θ and leaves where r = 2. To find θ -limits, notice the following triangle: () Calculus 3 February 2, 2020 3 / 12

  4. Exercise 15.4.6 Exercise 15.4.6 Exercise 15.4.6. Describe the given region in polar coordinates: Solution. Since x = r cos θ then along the vertical line x = 1 we have 1 = r cos θ or r = 1 / cos θ = sec θ . Along the circle we have r = 2. So we can describe the region in terms of r -limits. A typical ray from the origin enters the region where r = sec θ and leaves where r = 2. To find θ -limits, notice the following triangle: () Calculus 3 February 2, 2020 3 / 12

  5. Exercise 15.4.6 Exercise 15.4.6 Exercise 15.4.6. Describe the given region in polar coordinates: Solution. Since x = r cos θ then along the vertical line x = 1 we have 1 = r cos θ or r = 1 / cos θ = sec θ . Along the circle we have r = 2. So we can describe the region in terms of r -limits. A typical ray from the origin enters the region where r = sec θ and leaves where r = 2. To find θ -limits, notice the following triangle: () Calculus 3 February 2, 2020 3 / 12

  6. Exercise 15.4.6 Exercise 15.4.6 (continued) Solution (continued). We have cos θ = 1 / 2 so that θ = cos − 1 (1 / 2) = π/ 3. So the upper θ -limit is π/ 3 and, by symmetry, the lower θ -limit is − π/ 3. In particular, an integral of f ( r θ ) over the region is of the form � π/ 3 � 2 f ( r , θ ) dr d θ. − π/ 3 sec θ () Calculus 3 February 2, 2020 4 / 12

  7. Exercise 15.4.10 Exercise 15.4.10 Exercise 15.4.10. Change the integral into an equivalent polar integral. Then evaluate the polar integral: � √ � 1 1 − y 2 ( x 2 + y 2 ) dx dy . 0 0 1 − y 2 we have x 2 = 1 − y 2 where x ≥ 0 and � Solution. With x = x 2 + y 2 = 1 x ≥ 0. This is the upper half of the unit circle centered at the origin. With y ranging from 0 to 1 we then have the region: () Calculus 3 February 2, 2020 5 / 12

  8. Exercise 15.4.10 Exercise 15.4.10 Exercise 15.4.10. Change the integral into an equivalent polar integral. Then evaluate the polar integral: � √ � 1 1 − y 2 ( x 2 + y 2 ) dx dy . 0 0 1 − y 2 we have x 2 = 1 − y 2 where x ≥ 0 and � Solution. With x = x 2 + y 2 = 1 x ≥ 0. This is the upper half of the unit circle centered at the origin. With y ranging from 0 to 1 we then have the region: () Calculus 3 February 2, 2020 5 / 12

  9. Exercise 15.4.10 Exercise 15.4.10 Exercise 15.4.10. Change the integral into an equivalent polar integral. Then evaluate the polar integral: � √ � 1 1 − y 2 ( x 2 + y 2 ) dx dy . 0 0 1 − y 2 we have x 2 = 1 − y 2 where x ≥ 0 and � Solution. With x = x 2 + y 2 = 1 x ≥ 0. This is the upper half of the unit circle centered at the origin. With y ranging from 0 to 1 we then have the region: () Calculus 3 February 2, 2020 5 / 12

  10. Exercise 15.4.10 Exercise 15.4.10 (continued) Solution (continued). We can take the r -limits as 0 to 1 and the θ -limits as 0 to π . Since r 2 = x 2 + y 2 , the integral becomes � √ � 1 � π � 1 � π 1 − y 2 r =1 � 1 ( x 2 + y 2 ) dx dy = r 2 r dr d θ = 4 r 4 � d θ � � 0 0 0 0 0 r =0 � π π � 1 4 d θ = 1 = π � = 4 θ 4 . � � 0 0 () Calculus 3 February 2, 2020 6 / 12

  11. Exercise 15.4.28 Exercise 15.4.28 Exercise 15.4.28. Find the area of the region that lies inside the cardioid r = 1 + cos θ and outside the circle r = 1. Solution. The graphs of the cardioid (which is Exercise #1 on page 652 in Section 11.4) and the circle are: () Calculus 3 February 2, 2020 7 / 12

  12. Exercise 15.4.28 Exercise 15.4.28 Exercise 15.4.28. Find the area of the region that lies inside the cardioid r = 1 + cos θ and outside the circle r = 1. Solution. The graphs of the cardioid (which is Exercise #1 on page 652 in Section 11.4) and the circle are: So the r -limits of the region are 1 and 1 + cos θ and the θ -limits are − π/ 2 and π/ 2. () Calculus 3 February 2, 2020 7 / 12

  13. Exercise 15.4.28 Exercise 15.4.28 Exercise 15.4.28. Find the area of the region that lies inside the cardioid r = 1 + cos θ and outside the circle r = 1. Solution. The graphs of the cardioid (which is Exercise #1 on page 652 in Section 11.4) and the circle are: So the r -limits of the region are 1 and 1 + cos θ and the θ -limits are − π/ 2 and π/ 2. () Calculus 3 February 2, 2020 7 / 12

  14. Exercise 15.4.28 Exercise 15.4.28 (continued) Solution (continued). So the area of the region is � π/ 2 � 1+cos θ � π/ 2 � r =1+cos θ � 1 � �� 2 r 2 � A = r dr d θ = r dr d θ = d θ � � R − π/ 2 1 − π/ 2 r =1 � π/ 2 � π/ 2 � 1 � � � 2(1 + cos θ ) 2 − 1 cos θ + 1 2 cos 2 θ = d θ = d θ 2 − π/ 2 − π/ 2 θ = π/ 2 sin θ + 1 � θ 2 + sin 2 θ � � � 2 + sin 2 x cos 2 x dx = x � = since + C , � 2 4 4 � θ = − π/ 2 by Example 9 in Section 5.5 � � ( π/ 2) �� sin( π/ 2) + 1 + sin 2( π/ 2) = 2 2 4 � � ( − π/ 2) �� sin( − π/ 2) + 1 + sin 2( π/ 2) − 2 2 4 = (1 + (1 / 2)( π/ 4 + 0)) − ( − 1 + (1 / 2)( − π/ 4 + 0)) = 2 + π/ 4 . () Calculus 3 February 2, 2020 8 / 12

  15. Exercise 15.4.38 Exercise 15.4.38 Exercise 15.4.38. Converting to a Polar Integral. Integrate f ( x , y ) = ln( x 2 + y 2 ) over the region 1 ≤ x 2 + y 2 ≤ e 2 . x 2 + y 2 Solution. We have r 2 = x 2 + y 2 so ln( x 2 + y 2 ) = ln r r . The region is an x 2 + y 2 annulus with inner radius 1 and outer radius e 2 : () Calculus 3 February 2, 2020 9 / 12

  16. Exercise 15.4.38 Exercise 15.4.38 Exercise 15.4.38. Converting to a Polar Integral. Integrate f ( x , y ) = ln( x 2 + y 2 ) over the region 1 ≤ x 2 + y 2 ≤ e 2 . x 2 + y 2 Solution. We have r 2 = x 2 + y 2 so ln( x 2 + y 2 ) = ln r r . The region is an x 2 + y 2 annulus with inner radius 1 and outer radius e 2 : () Calculus 3 February 2, 2020 9 / 12

  17. Exercise 15.4.38 Exercise 15.4.38 Exercise 15.4.38. Converting to a Polar Integral. Integrate f ( x , y ) = ln( x 2 + y 2 ) over the region 1 ≤ x 2 + y 2 ≤ e 2 . x 2 + y 2 Solution. We have r 2 = x 2 + y 2 so ln( x 2 + y 2 ) = ln r r . The region is an x 2 + y 2 annulus with inner radius 1 and outer radius e 2 : () Calculus 3 February 2, 2020 9 / 12

  18. Exercise 15.4.38 Exercise 15.4.38 (continued) Solution. We describe this with r -limits of 1 and e 2 , and θ -limits of 0 and 2 π . Since r 2 = x 2 + y 2 and dx dy = r dr d θ , the integral is then: � 2 π � 2 π � e 2 � e 2 ln( x 2 + y 2 ) �� ln r dx dy = r r dr d θ = ln r dr d θ x 2 + y 2 0 1 0 1 R � 2 π r = e 2 � � � = ( f ln r − r ) d θ since ln x dx = x ln x − x + C � 0 � r =1 by Example 2 in Section 8.1 on page 456 � 2 π � 2 π (( e 2 ln e 2 − e 2 )(1 ln 1 − 1)) d θ = ((2 e 2 − e 2 ) − (0 − 1)) d θ = 0 0 � 2 π 2 π � ( e 2 + 1) d θ = ( e 2 + 1) θ = 2 π ( e 2 + 1) . � = � � 0 0 () Calculus 3 February 2, 2020 10 / 12

  19. Exercise 15.4.38 Exercise 15.4.38 (continued) Solution. We describe this with r -limits of 1 and e 2 , and θ -limits of 0 and 2 π . Since r 2 = x 2 + y 2 and dx dy = r dr d θ , the integral is then: � 2 π � 2 π � e 2 � e 2 ln( x 2 + y 2 ) �� ln r dx dy = r r dr d θ = ln r dr d θ x 2 + y 2 0 1 0 1 R � 2 π r = e 2 � � � = ( f ln r − r ) d θ since ln x dx = x ln x − x + C � 0 � r =1 by Example 2 in Section 8.1 on page 456 � 2 π � 2 π (( e 2 ln e 2 − e 2 )(1 ln 1 − 1)) d θ = ((2 e 2 − e 2 ) − (0 − 1)) d θ = 0 0 � 2 π 2 π � ( e 2 + 1) d θ = ( e 2 + 1) θ = 2 π ( e 2 + 1) . � = � � 0 0 () Calculus 3 February 2, 2020 10 / 12

  20. Exercise 15.4.41 Exercise 15.4.41 Exercise 15.4.41. Converting to Polar Integrals. � ∞ e − x 2 dx is (a) The usual way to evaluate the improper integral I = 0 first to calculate its square: �� ∞ � �� ∞ � ∞ � ∞ � e − x 2 dx e − x 2 dx I 2 = e − ( x 2 + y 2 ) dx dy . = 0 0 0 0 Evaluate the last integral using polar coordinates and solve the resulting equation. for I . Solution. The double integral is over the first quadrant of the Cartesian plane. So in polar coordinated we have the r -limits of 0 and ∞ and the θ -limits of 0 and π/ 2. Since r 2 = x 2 + y 2 and dx dy = r dr d θ then we have: . . . () Calculus 3 February 2, 2020 11 / 12

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