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Exercise 3: Similar to the methods solving sin" (x) cosm instead use tan2(x) + 1 = you can let u = sec2 (x). If m > 2 is even, then you can let u = sec(x). The hard case is n even and m odd. Apply this to the following: (x) dx, we can solve f tan" (x) secm (x) dx. These tan(x), and if n is odd, then 4 (a) tan (x) sec* (x) dx ) / | tan (2) sec*(2) dr (b) | tan (2) sec* (2) da ec*(x) dx (d) (TIard) tan (1) sec (r) «dr 4 tan (x) sec (x) dx

Exercise 3: Similar to the methods solving sin" (x) cosm instead use tan2(x) + 1 = you can let u = sec2 (x). If m > 2 is even, then you can let u = sec(x). The hard case is n even and m odd. Apply this to the following: (x) dx, we can solve f tan" (x) secm (x) dx. These tan(x), and if n is odd, then 4 (a) tan (x) sec* (x) dx ) / | tan (2) sec*(2) dr (b) | tan (2) sec* (2) da ec*(x) dx (d) (TIard) tan (1) sec (r) «dr 4 tan (x) sec (x) dx

Algebra & Trigonometry with Analytic Geometry
Algebra & Trigonometry with Analytic Geometry
13th Edition
ISBN:9781133382119
Author:Swokowski
Publisher:Swokowski
Chapter6: The Trigonometric Functions
Section6.3: Trigonometric Functions Of Real Numbers
Problem 43E
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Exercise 3: Similar to the methods solving sin" (x) cosm instead use tan2(x) + 1 = you can let u = sec2 (x). If m > 2 is even, then you can let u = sec(x). The hard case is n even and m odd. Apply this to the following: (x) dx, we can solve f tan" (x) secm (x) dx. These tan(x), and if n is odd, then 4 (a) tan (x) sec* (x) dx ) / | tan (2) sec*(2) dr (b) | tan (2) sec* (2) da ec*(x) dx (d) (TIard) tan (1) sec (r) «dr 4 tan (x) sec (x) dx
Transcribed Image Text:Exercise 3: Similar to the methods solving sin" (x) cosm instead use tan2(x) + 1 = you can let u = sec2 (x). If m > 2 is even, then you can let u = sec(x). The hard case is n even and m odd. Apply this to the following: (x) dx, we can solve f tan" (x) secm (x) dx. These tan(x), and if n is odd, then 4 (a) tan (x) sec* (x) dx ) / | tan (2) sec*(2) dr (b) | tan (2) sec* (2) da ec*(x) dx (d) (TIard) tan (1) sec (r) «dr 4 tan (x) sec (x) dx
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