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Scalar Differentiation

Recall the definition of ordinary differentiation. In light of the treatment above, we now recognize that the ``ordinary'' differentiation we learned in the first year of calculus was ordinary because it was scalar differentiation - differentiation of functions that represent scalar quantities. Given a (continuous, differentiable - we will assume this unless stated otherwise for all functions discussed) function $ f(t)$ :

$\displaystyle \ddx{f} = \lim_{\Delta t \to 0} \frac{f(t + \Delta t) - f(t)}{\Delta
t} $

Note my explicit and deliberate use of $ t$ as the independent variable upon which $ f$ depends. This invites us to think of this as a rate of change in physics where $ f$ is some physical quantity as a function of $ t$ the time.

From this one can easily derive all sorts of associated rules, the most important of which are:

We will often express these rules in terms of differentials, not derivatives with respect to specific coordinates. For example:

$\displaystyle df = \ddx{f} dx = \ddt{f} dt $

$\displaystyle d(fg) = g\ df + f\ dg $

Most of these simple scalar rules have counterparts when we consider different kinds of vector differentiation.


next up previous contents
Next: Vector Differentiation Up: Scalar and Vector Calculus Previous: Scalar and Vector Calculus   Contents
Robert G. Brown 2017-07-11