SUMMARY
The gradient of the scalar field \(u(r,\theta) = r\cos(\theta)\left[1 - \left(\frac{1}{r}\right)^2\right]\) is calculated using the formula for the gradient in spherical coordinates. The resulting gradient in Cartesian coordinates is expressed as \(1 + \frac{2 x^2}{(x^2 + y^2)^2} - \frac{1}{x^2 + y^2}, \frac{2 x y}{(x^2 + y^2)^2}\). To derive this, one must compute the partial derivatives of \(u\) with respect to \(r\) and \(\theta\), and then convert the results into Cartesian coordinates. The discussion emphasizes switching to Cartesian variables for simplification.
PREREQUISITES
- Understanding of spherical coordinates and their gradients
- Familiarity with partial derivatives
- Knowledge of Cartesian coordinate transformations
- Basic calculus concepts related to scalar fields
NEXT STEPS
- Study the derivation of gradients in spherical coordinates
- Learn about converting functions from spherical to Cartesian coordinates
- Explore the application of partial derivatives in vector calculus
- Investigate examples of scalar fields and their gradients in physics
USEFUL FOR
Students and professionals in mathematics, physics, and engineering who are working with scalar fields and vector calculus, particularly those interested in understanding gradients in different coordinate systems.