7.5. Tensor Calculus in Euclidean Spaces - Cartesian coordinates in \(E^3\)#
Using Cartesian coordinates \((q^1, q^2, q^3) = (r, \theta, z)\) and Cartesian base vectors (uniform in space, so that their derivatives are zero), a point in Euclidean vector space \(E^3\) can be represented as
7.5.1. Natural basis, reciprocal basis, metric tensor, and Christoffel symbols#
Cartesian coordinates in Euclidean spaces are a very special coordinate system, with reciprocal basis everywhere coinciding with natural basis, with uniform basis in space (zero second-order derivative of space w.r.t. coordinates, and thus zero first order derivative of base vectors, and thus identically zero Christoffel symbols), and components of the metric tensor equal to the identity matrix
7.5.2. Differential operators#
7.5.2.1. Gradient#
Example 7.8 (Gradient of a scalar field)
Example 7.9 (Gradient of a vector field)
Example 7.10 (Gradient of a \(2^{nd}\)-order tensor field)
7.5.2.2. Directional derivative#
7.5.2.3. Divergence#
Example 7.11 (Divergence of a vector field)
Example 7.12 (Divergence of a \(2^{nd}\)-order tensor field)
7.5.2.4. Laplacian#
Example 7.13 (Laplacian of a scalar field)
Example 7.14 (Laplacian of a vector field)