One of the most important concepts in algebra is that of the function. The formal mathematical definition of the term function14 is beyond the scope of this short review, but the summary below should be more than enough to work with.
A function is a mapping between a set of coordinates (which is why we put this section after the section on coordinates) and a single value. Note well that the ``coordinates'' in question do not have to be space and/or time, they can be any set of parameters that are relevant to a problem. In physics, coordinates can be any or all of:
Note well that many of these things can equally well be functions
themselves - a potential energy function, for example, will usually
return the value of the potential energy as a function of some mix
of spatial coordinates, mass, charge, and time. Note that the
coordinates can be continuous (as most of the ones above are
classically) or discrete - charge, for example, comes only
multiples of
and color can only take on three values.
One formally denotes functions in the notation e.g.
where
is the function name represented symbolically and
is
the entire vector of coordinates of all sorts. In physics we often
learn or derive functional forms for important quantities, and may or
may not express them as functions in this form. For example, the
kinetic energy of a particle can be written either of the two following
ways:
| (32) | |||
| (33) |
| (34) |
, and One important property of the mapping required for something to be a true ``function'' is that there must be only a single value of the function for any given set of the coordinates. Two other important definitions are:
Two last ideas that are of great use in solving physics problems algebraically are the notion of composition of functions and the inverse of a function.
Suppose you are given two functions: one for the potential energy of a mass on a spring:
| (35) |
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(36) |
| (37) |
With the composition operation in mind, we can define the inverse. Not all functions have a unique inverse function, as we shall see, but most of them have an inverse function that we can use with some restrictions to solve problems.
Given a function
, if every value in the range of
corresponds to one and only one value in its domain
, then
is also a function, called the inverse of
. When
this condition is satisfied, the range of
is the domain of
and vice versa. In terms of composition:
| (38) |
| (39) |
Many functions do not have a unique inverse, however. For example, the function:
| (40) |
| (41) |
We can get around this problem by restricting the domain to a
region where the inverse mapping is unique. In this particular
case, we can define a function
where the domain of
is only
and the range of
is restricted to
be
. If this is done, then
for all
and
for all
. The
inverse function for many of the functions of interest in physics have
these sorts of restrictions on the range and domain in order to make the
problem well-defined, and in many cases we have some degree of choice in the best definition for any given problem, for example, we
could use any domain of width
that begins or ends on an odd
half-integral multiple of
, say
or
if it suited the needs of our problem to do so
when computing the inverse of
(or similar but different ranges
for
or
) in physics.
In a related vein, if we examine:
| (42) |
| (43) |
| (44) |
The second is that once we have defined the inverse functions for either trig functions or the quadratic function in this way so that they have restricted domains, it is natural to ask: Do these functions have any meaning for the unrestricted domain? In other words, if we have defined:
| (45) |
This leads us naturally enough into our next section (so keep it in mind) but first we have to deal with several important ideas.