Polar coordinates are a two-dimensional coordinate system where each point in the plane is determined by a distance from a reference point and an angle from a reference direction. These coordinates are particularly useful in problems involving circular symmetry.
The reference point is called the pole (analogous to the origin in Cartesian coordinates), and the reference direction is typically the positive \(x\)-axis.
In polar coordinates, any point is identified by \(r \) and \(\theta \). The value \(|r| \) is the distance from the pole, and \(\theta \) is the angle from the positive \(x \)-axis.
To convert Cartesian coordinates \( (x, y ) \) to polar coordinates, we use:
- \[ r = \sqrt{x^2 + y^2} \ ]
- \[\theta = \text{arctan} \left(\frac{y}{x}\right) \]
Using polar coordinates simplifies integration over circular regions. When converting the given exercise's square region to polar coordinates, the bounds for \(\theta \) range from \[ \theta = -\frac{\pi}{4} \ to \ \frac{\theta}{4} \], and for \( r \) range from \ 0 \ to \ \frac{a}{\root{2}}\]