Series: Calculus Notes

Part 1: Local Motion and Small Errors

Calculus starts with a simple question: what does it mean to know your speed at one exact moment?

Imagine riding a bike down a straight road. Your position at time tt is x(t)x(t), and your speed at time tt is v(t)v(t).

Suppose that at time t=10t = 10 seconds, your speed is 5 meters per second. If that speed stayed constant for a short time, then after hh more seconds you would travel 5h5h meters, so

x(10+h)=x(10)+5h. x(10+h) = x(10) + 5h.

That is the constant-speed picture.

Real motion is usually not that simple. Maybe right after t=10t = 10 you start pedaling harder, so your speed begins to increase. Then the straight-line formula is still a good first guess, but it is no longer exact. A more honest statement is

x(10+h)=x(10)+5h+(extra distance). x(10+h) = x(10) + 5h + \text{(extra distance)}.

Instead of trying to compute that extra distance exactly, we will only track how large it is.

Definition

A notation

A(c)A(c) means some quantity whose absolute value is at most cc.

If you are used to seeing measurements written with a plus/minus, this is the same basic idea. We are keeping track of how large the error can be without needing to know exactly what it is.

For example,

π=3.14+A(0.005) \pi = 3.14 + A(0.005)

means that π\pi differs from 3.14 by at most 0.005. We are not saying exactly what the difference is. We are only saying that it is small.

Now go back to the bike. If hh is small, then your speed does not have much time to change, so the extra distance should be much smaller than the main term 5h5h. If hh is small enough, and the motion is not changing too wildly over that short interval, it is reasonable to write, a bit imprecisely,

x(10+h)=x(10)+5h+A(h2). x(10+h) = x(10) + 5h + A(h^2).

This is not meant to be a fully precise statement yet. It is a good short-time model, and it captures the picture we want.

The term 5h5h is the main change in position, and the A(h2)A(h^2) term is the leftover error. When hh is small, that error is much smaller than the main term. For example, if h=0.01h = 0.01, then h2=0.0001h^2 = 0.0001. So for a first approximation we can ignore the error and get

x(10+h)x(10)+5h, x(10+h) \approx x(10) + 5h,

which is the equation of a line in the variable hh. In other words, if we zoom in to a short enough time scale, the motion starts to look linear.

This suggests a useful way to think about speed. We say, still a bit imprecisely for now, that the speed at time tt is the number v(t)v(t) for which

x(t+h)=x(t)+v(t)h+A(h2) x(t+h) = x(t) + v(t)\,h + A(h^2)

holds when hh is small. So speed is the slope of the best short-time line. In the next note, we will see how this matches the more familiar idea of average speed.

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