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That term itself isn't zero. But the area under it, taken over the complete cycle 0→2 Pi contributes nothing to the integral that you are about to evaluate. So the author is just looking ahead and seeing that he can save himself a bit of work here, and not bothering to process a term that is going to end up as zero anyway.MissP.25_5 said:Hello.
This is part of a solution but I don't understand the underlined part. Why is it equals to 0?
The "sin rule" is a mathematical rule used to find the values of missing angles in a triangle when the lengths of its sides are known. It states that the ratio of the length of a side to the sine of its opposite angle is equal for all three sides in a triangle.
In trigonometry, the "sin rule" is used to solve problems involving triangles. It allows us to find missing angles or sides in a triangle by using the ratio mentioned above. This rule is particularly useful when dealing with non-right triangles, where the Pythagorean theorem cannot be used.
The "sin rule" and the "cosine rule" are both used to find missing angles and sides in a triangle. However, the "cosine rule" involves the use of cosines, while the "sin rule" involves the use of sines. The "cosine rule" is typically used for finding the length of a side, while the "sin rule" is used for finding the measure of an angle.
To apply the "sin rule" to a triangle, you will need to know the lengths of two sides and the measure of the angle opposite one of those sides. Then, you can use the formula: sine of the angle opposite the known side divided by the length of the known side, is equal to the sine of the angle opposite the unknown side divided by the length of the unknown side. You can then solve for the unknown angle using basic algebra.
The "sin rule" has many real-life applications, particularly in fields such as engineering, architecture, and navigation. For example, it can be used to calculate the height of a building, the slope of a roof, or the distance between two points on a map. It is also used in fields such as astronomy and physics to calculate the angles and distances between celestial objects.