Gradient Vector and Linearization

 

Gradient Vector

The gradient vector is a vector of all partial derivatives of a function. It is defined by the differential operator {\nabla = ( \frac{\partial}{\partial x}, \frac{\partial}{\partial y},...)}. The gradient vector of a function {f} is {\nabla f= (f_x, f_y,...)}.

For a surface given explicitly by {z=f(x,y)}, {\nabla f} is a 2 dimensional vector pointing the direction of steepest increase.

For a surface given implicitly by {f(x,y,z)=0}, {\nabla f} is a 3 dimensional vector that is normal to the surface. We can then compute a tangent plane using point normal form {(\mathbf{r}-\mathbf{r_0})\cdot \mathbf{n} = 0} where {\mathbf{n}=\nabla f(\mathbf{r_0})} (see previous page for example).

Linearisation and Differential Form

In single variable calculus we use a tangent line to linearly approximate a function and compute estimates of function values. In multivariable calculus we use a tangent plane to obtain the linearised change in a function {f(x,y)}. To have a tangent plane at a given point the function must be differentiable at that point.

A function {f(x,y)} is differentiable at {(x_0, y_0)} if {f_x} and {f_y} exist near {(x_0, y_0)} and are continuous at {(x_0, y_0)}.

Thus for the function ({\Delta} means change):

\displaystyle \Delta f(x,y)=f(x,y)-f(x_0,y_0)=f_x(x_0,y_0)\Delta x+f_y(x_0,y_0)\Delta y +\epsilon_1 \Delta x+\epsilon_2 \Delta y

Where {f_x...+f_y...} is the linearised change in {f} and {\epsilon_i} is the error which {\rightarrow 0} as {(x,y)\rightarrow (x_0,y_0)}.

In the limit as {\Delta x, \Delta y \rightarrow 0} the total differential is {df = \frac{\partial f}{\partial x} dx+ \frac{\partial f}{\partial y} dy}, where {df,dx,dz} are infinitesimal differentials.

Note: Also see later section on Taylor series for more on approximations.