Trigonometric IntegralsTrigonometric IntegralsPrerequisite KnowledgeTrigonometric IdentitiesPythagorean IdentityAdditional Pythagorean IdentitiesPythagorean Identity with Tangent and SecantPythagorean Identity with Cotangent and CosecantHalf-angle formulasUse Technology to Recall Half-Angle FormulasDouble-Angle FormulasCheck Your WorkUse Technology to Recall Double-Angle FormulasEvaluation of Trig FunctionsEvaluating Trigonometric RatiosCC BY-NC-SA 4.0
Author: John J Weber III, PhD Corresponding Textbook Sections:
The Pythagorean Identities shown in red will be needed for integrals of trigonometric functions.
One Pythagorean Identity that you should remember from Pre-Calculus (Math 1113):
When integrating trigonometric integrals, you will need two equivalent forms of the above Pythagorean Identity:
Derivation
NOTE: You are not expected to derive the Pythagorean Identity for tangent and secant; however, if you forget the Pythagorean Identity for tangent and secant, then knowing how to derive the identity will be useful.
Divide through by
When integrating trigonometric integrals, you will need the equivalent form of the above Pythagorean Identity:
Derivation
NOTE: You are not expected to derive the Pythagorean Identity for cotangent and cosecant; however, if you forget the Pythagorean Identity for cotangent and cosecant, then knowing how to derive the identity will be useful.
Divide through by
When integrating trigonometric integrals, you will need the equivalent form of the above Pythagorean Identity:
NOTE: You will need to appropriately use the following trigonometric identities. You are not expected to memorize these identities.
Mathematica
NOTE: On all Assessments, Mathematica may be used to appropriately rewrite an even power of sine or cosine without showing any work.
1(* Rewrite sin^2(x) *)2TrigReduce[Sin[x]^2]Warnings:
Be very careful with the syntax. Syntax is the set of rules on how to write computer code. Every software program has its own unique syntax. Some basic Mathematica syntax is located at: https://www.jjw3.com/Common_Mathematica_Code.html.
TrigReduce[ ] has at least one argument:
For help on using the TrigReduce[ ] function:
Remember, correct Mathematica code will be all black except for variables.
To execute code (including comment codes), press and hold the SHIFT key and press the ENTER key.
Mathematica may return a result in a different, but equivalent, form than your answer. In these cases, use FTC-I to check your work.
NOTE: You will need to appropriately use the following trigonometric identities. You are not expected to memorize these identities.
Mathematica
NOTE: On all Assessments, Mathematica may be used to appropriately rewrite an even power of sine or cosine without showing any work.
xxxxxxxxxx21(* Rewrite sin(2x) *)2TrigExpand[Sin[2x]]Warnings:
Be very careful with the syntax. Syntax is the set of rules on how to write computer code. Every software program has its own unique syntax. Some basic Mathematica syntax is located at: https://www.jjw3.com/Common_Mathematica_Code.html.
TrigExpand[ ] has at least one argument:
For help on using the TrigExpand[ ] function:
Remember, correct Mathematica code will be all black except for variables.
To execute code (including comment codes), press and hold the SHIFT key and press the ENTER key.
Mathematica may return a result in a different, but equivalent, form than your answer. In these cases, use FTC-I to check your work.
NOTE: There is NO reason to memorize when to use TrigReduce[ ] and TrigExpand[ ]; one will return the same input and the other will rewrite the input.
There is NO reason to memorize the unit circle. Look at the Table below and consider the patterns of the numbers. Use these patterns to recall your trig ratios1.
| Angles (Degrees) | Angles (Radians) | ||||||
|---|---|---|---|---|---|---|---|
| 0 | |||||||
NOTE: On all Assessments, exact trigonometric values are expected, except where instructed otherwise. There are two options available for evaluating trigonometric ratios, e.g.,
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Created: Monday, 18 January 2021 09:14 EDT Last Modified: Monday, 10 January 2022 - 07:17 (EST)